Reliability-based sea-ice parameters for design of offshore structures
BSEE contract number: E13PC00020
Presented by: University of Alaska Anchorage; College of Engineering
Project Team: Hajo Eicken (UAF) Andy Mahoney (UAF) Andrew T. Metzger (UAA) Vincent Valenti (UAA)
December, 2015
Abstract: The intent of this study was to supplement the ISO 19906 Standard: Petroleum and Natural Gas Industries - Arctic Offshore Structures (i.e., the Normative). This supplement provides additional sea-ice information, for US waters in both the Chukchi and Beaufort seas, in a format consistent with the philosophy of the Normative. Currently, implementation of ISO 19906 in US waters is questionable due the lack of sea- ice design criteria. Appendices B.7 (Beaufort Sea) and B.8 (Chukchi Sea) of ISO 19906 are intended to provide this information but the data is not in a format consistent with the philosophy of the Normative – i.e., a reliability (probability)-based format. A full complement of design values for the regions covered in B.7 and B.8 is required to implement the normative provisions and, ultimately, produce a safe and reliable offshore structural design that can successfully survive demands from sea-ice. The work here included an extensive literature review and detailed analysis of sixteen (16) seasons of under-ice measurements from lease sites in the Chukchi and Beaufort seas. The analyses have further characterized ice cover and identified the most acute values for certain ice features. Also included in this study is a means to identify a critical keel depth with a low probability of being exceeded (conversely a high reliability of not being exceeded/failing) in a particular timeframe. The study concluded with an assessment of the suitability of the current ISO 19906 recommendations for estimating global ice actions (forces) on offshore structures. The latter included commentary on possible steps for refining the current standard of practice cited in ISO 19906.
Executive Summary
The project completed the scope set forth under contract E13PC00020 from BSEE; the following objectives were completed: Obtain sea ice data of good quality and sufficient quantity Conduct a literature review Compute statistics for relevant sea ice parameters Determine limit state values for applicable parameters if data was sufficient to do so. In addition to completing the objectives established in the contract the following additional objectives were also completed: Produce ice velocity roses Provide a probabilistic means for calculating critical pressure ridge keel depth Examine how the ISO 19906 computes ridge loading on vertical structures Compare theoretical ridge loads to recorded ridge loads in the Beaufort Sea Investigate the ice strength coefficient, CR Use recorded loadings in the Beaufort Sea to suggest alternative values of CR Overall, this project produced new information that should be able to be easily implemented by industry or regulatory agencies for the Beaufort and Chukchi Seas. Specifically there are reported values and findings that are of particular significance: The ridge keel draft in the Beaufort and Chukchi Seas can be described by a Weibull Distribution, as presented by Eq. 4.2.3.1 with a threshold value, μ, of six meters. o Beaufort Sea: Shape parameter, α = 2.70 o Beaufort Sea: Scale parameter, β = 0.99 o Chukchi Sea: Shape parameter, α = 2.37 o Chukchi Sea: Scale parameter, β = 1.02 There appears to be a majority presence of FY ridges in both seas due to the presence of a modal keel width. Modal ridge keel angles were found: o Beaufort Sea: 33.7° o Chukchi Sea: 32.5° There appears to be no significant relationship between keel depth and speed. From Figure 6.3 and Figure 6.4 it can be seen that, using the probability theory approach, the critical keel depth increases with service life. The annual exceedance probability approach is independent of service life and considers an event on an annual basis as opposed to a service life basis.
In comparison to other studies found this project had a large amount of quality data for analysis, making the results significant. A major component of this study was to verify suggested values for various sea- ice parameters provided in annexes B.7 and B.8 of the ISO 19906. Table ES.1: Beaufort Sea ISO 19906 Sea Ice Conditions; values in bold indicate results from this study (Reproduced from International Organization for Standardization, 2010, Table B.7-4)
Average Range of Parameter Annual Value Annual Values Sea Ice Late September First Ice October to late October Occurrence Early July to Last Ice July mid-August Landfast Ice Thickness 1.8 1.5 to 2.3 Level Ice (m) (FY) Floe Thickness (m) 1.8 1.5 to 2.3 Rafted Ice Rafted Ice Thickness (m) 3 2.5 to 4.5 Sail Height (m) 5 3 to 6 Rubble Fields Length (m) 100 to 1,000 100 to 1,000 3 to 6 Sail Height (m) 5 1 to 7 Ridges 15 to 28 Keel Depth (m) 25 6 to 30 Water Depth Range (m) 20 15 to 30 Stamukhi Sail Height (m) 5 to 10 up to 20 Level Ice (SY Ice Thickness (m) 3 to 6 2 to 11 & MY) Floe Thickness (m) 5 2 to 20 Sail Height (m) Significant Significant Keel Depth (m) 20 10 to 35 Rubble Fields (SY & MY) Average Sail Height (m) 2 to 5 3 to 6 Length Annual Maximum 750 50 to 2,300 (m) Ice Movement Speed in Nearshore (m∙s-1) 0.06 0.04 to 0.2 0.06 to 1.0 Speed in Offshore (m∙s-1) 0.08 0 to 1.5 Icebergs/Ice Islands Size Mass 10 ND Months Present Poorly Known Poorly Known Frequency Number per Year Poorly Known Poorly Known Maximum Number per Rare Rare Month
Table ES.2: Chukchi Sea ISO 19906 Sea Ice Conditions; values in bold indicate results from this study (Reproduced from International Organization for Standardization, 2010, Table B.8-4)
Region Northeastern Parameter Average Range of Annual Annual Values Value Late October to First Ice November Early December Occurrence Mid-June to Late Last Ice July August Level Ice Landfast Ice Thickness (m) 1.5 1.3 to 1.7 (FY) Floe Thickness (m) 0.7 to 1.4 0.7 to 1.8 Rafted Ice Rafted Ice Thickness (m) 1.0 to 2.0 1.0 to 3.0 Sail Height (m) 2 1 to 3 Rubble 300 to Fields Length (m) 300 to 1,000 1,000 1 to 3 Sail Height (m) 2 1 to 6 Ridges (FY) 8 to 15 Keel Depth (m) 10 6 to 26 Water Depth Range (m) None None Stamukhi Sail Height (m) None None Level Ice Floe Thickness (m) 2 to 4 2 to 6 (SY & MY) Ridges (SY Sail Height (m) 1 to 2 1 to 3 & MY) Keel Depth (m) 4 to 8 4 to 10 Ice Speed in Nearshore (m∙s-1) 0.1 to 0.2 0.1 to 0.3 Movement Speed in Offshore (m∙s-1) 0.2 to 0.3 0.2 to 0.3 0 to 1.1
Referencing Table ES.1 and 2, the most significant findings are the ice speed and pressure ridge depth. It should also be noted that this study was confined to information for the offshore environment. The near-shore features shown on the table were not studied. It was not possible to distinguish between first year and multi-year ice from the available data. However, it is likely the Chukchi ice is almost entirely first year ice. The reason for this is a particular mechanism must set up for multi-year ice features to travel from the Canadian Beaufort to the Chukchi Sea. The BSEE studies on freeze-up in the region elaborate on the conditions required for MY ice to travel from the Beaufort. Pressure ridge statistics from the Beaufort Sea data exhibited more dispersion than the Chukchi data. However, data from both seas passed statistical goodness-of-fit tests. It is speculated that MY features, more common in the Beaufort Sea, could be the source of the increased ‘spread’ of the Beaufort data. Based on the results of this study, it is likely that FY pressure ridges will govern the ultimate and possible the abnormal limit states for global ice action on offshore structures in the Chukchi lease areas. For the Beaufort, FY ridges may control the ultimate limit state. Based on experience and information from other studies, MY features may control global ice forces in the Beaufort Sea as the occurrence of these features in more frequent. A means of estimating a critical pressure ridge depth for both seas was derived from the data and is presented in this study. The utility of this information is that it can be used to identify depth at which interference with construction may occur (e.g., well head depth); it can be used to identify a limit-state pressure ridge feature; it can be used to inform decisions regarding burial depth of subsea pipelines. The tables below provide guidance on critical pressure ridge depth on an annual basis as well as a lifetime basis. Service lives are defined in terms of keels passing a given point, a year of service corresponding to the average number of keels in a season for both the Beaufort and Chukchi Sea data used in this study. The “T=100” line represents the critical keel depth based on an annual probability of occurence equal to 0.01 which is independent of service life. Given the availability of the sea-ice data, the study team elected to further study certain aspects of the ISO 19906 document as this was a convenient next step and did not represent any additional cost to the project. In particular, the team explored the suitability of ISO 19906 guidelines for calculating global ice actions (total force from ice on an offshore structure). It was initially found that when estimating pressure ridge loads using the ISO 19906 standard the magnitudes were extremely high, far larger than anything recorded for FY ridges. When this was further investigated by using measured parameters from recorded events and theoretically computing the load, it was still found that the
Figure ES.1: Beaufort Sea Critical Keel Depth as a Function of Service Life
Figure ES.2: Chukchi Sea Critical Keel Depth as a Function of Service Life theoretical action was much greater than the recorded action. While there was not sufficient data to come to a firm conclusion, it appears that the ISO 19906 is conservative
when computing ridge loading but may not be conservative for FY level ice loading. From the literature reviewed for this project it also seems that the ice strength parameter, CR, is not well understood or agreed upon. Furthermore, an investigation into MY ridges and ice was not conducted, which could have an impact on CR. From the results CR values of 1.62 and 3.36 MPa, the weighted average of the CR values, are recommended for FY ridges and FY level ice, respectively. Further research into the computation of ridge loading, particularly with respect to the consolidated layer, would be of great benefit and is advisable. The results of Monte Carlo simulation of global ice forces indicates that while the strength of ice composing a pressure ridge is less than that of level ice, FY pressure ridge features in the Chukchi sea will likely cause governing (in terms of engineering design) global ice forces on offshore structures sited in that sea.
Table of Contents
Page List of Figures ...... xiv
List of Tables ...... xxi
List of Appendices ...... xxiii
Acknowledgments ...... xxv
Chapter 1: Introduction ...... 1
1.1 Background ...... 1
1.2 Objective ...... 2
1.3 Data Collection ...... 3
1.4 Data Processing ...... 3
1.5 Presentation of Results ...... 4
Chapter 2: Literature Review ...... 5
2.1 Beaufort Sea ...... 5
2.2 Chukchi Sea ...... 6
2.3 Measurement of Ice Draft and Keel Depth ...... 8
2.4 Sea Ice Morphology ...... 10
2.4.1 First-Year Ice ...... 10
2.4.2 Multi-Year Ice ...... 11
Page
2.4.3 Pressure Ridges ...... 11
2.4.4 Level Ice ...... 13
2.4.5 Rafted Ice ...... 13
ix 2.4.6 Stamukhi ...... 14
2.4.7 Rubble Ice ...... 15
2.4.8 Icebergs and Ice Islands ...... 15
2.5 Reliability Engineering ...... 16
2.6 ISO 19906 Design Philosophy ...... 17
2.7 Arctic Structure Design ...... 18
2.8 Pressure Ridge Statistics ...... 19
2.8.1 Pressure Ridge Keel Draft Statistics ...... 19
2.8.2 Pressure Ridge Keel Width Statistics ...... 21
2.8.3 Pressure Ridge Keel Angle Statistics ...... 22
2.8.4 Pressure Ridge Keel Spacing Statistics ...... 22
2.8.5 Pressure Ridge Sail Statistics ...... 24
2.9 Ice Velocity ...... 25
2.10 Sea Ice Engineering Properties ...... 25
2.11 Sea Ice Loads on Structures ...... 27
2.12 Changing Ice Conditions ...... 34
Chapter 3: Data ...... 35
3.1 Overview ...... 35
3.2 Data Collection ...... 37
Page
3.3 Pressure Ridge Keel Identification ...... 43
3.4 Level Ice Identification ...... 48
3.5 Other Ice Identification ...... 52
x Chapter 4: Data Analysis ...... 55
4.1 Overview ...... 55
4.2 Probability Density Functions ...... 55
4.2.1 Gamma Distribution ...... 56
4.2.2 Exponential Distribution ...... 57
4.2.3 Weibull Distribution ...... 58
4.2.4 Lognormal Distribution ...... 59
4.3 P-Value Testing of PDFs ...... 59
4.4 Pressure Ridge Keel ...... 61
4.4.1 Keel Identification Starting Threshold Value ...... 61
4.4.2 Pressure Ridge Keel Draft ...... 63
4.4.3 Pressure Ridge Keel Width ...... 71
4.4.4 Pressure Ridge Keel Angle ...... 74
4.4.5 Pressure Ridge Keel Velocity ...... 75
4.4.6 Pressure Ridge Keel Spacing ...... 78
4.5 Ice Velocity ...... 83
4.6 Level Ice ...... 84
4.7 Other Ice ...... 86
Chapter 5: Results...... 89
Page
5.1 Pressure Ridge Keel ...... 89
5.1.1 Pressure Ridge Keel Draft ...... 89
5.1.2 Pressure Ridge Keel Width ...... 90
xi 5.1.3 Pressure Ridge Keel Angle ...... 91
5.1.4 Pressure Ridge Keel Velocity ...... 92
5.1.5 Pressure Ridge Keel Spacing ...... 94
5.2 Ice Velocity ...... 95
5.3 Level Ice ...... 97
5.4 Other Ice ...... 100
Chapter 6: Implementation ...... 101
6.1 ISO 19906 Comparison ...... 101
6.1.1 Beaufort Sea ...... 101
6.1.2 Chukchi Sea ...... 104
6.2 Pressure Ridge Keel Depth Probabilities ...... 106
6.2.1 Pressure Ridge Keel Depth Probability Calculation ...... 110
6.3 Limit State Ice Actions ...... 115
6.3.1 Consolidated Layer Force ...... 115
6.3.2 Keel Force ...... 118
6.3.3 Horizontal FY Ridge Action ...... 121
6.3.4 Monte Carlo Simulation ...... 121
6.3.5 Beaufort Sea Results ...... 122
6.3.6 Chukchi Sea Results ...... 124
Page
6.3.7 Molikpaq Ridge Comparison ...... 125
6.3.8 CR Determination from Molikpaq FY Ridges ...... 129
6.3.9 CR Determination from Molikpaq FY Level Ice...... 135
xii 6.3.10 Impact of CR on Caisson Weight...... 138
6.3.11 Determination of Governing Condition ...... 141
Chapter 7: Recommendations ...... 143
7.1 Pressure Ridge Keels ...... 143
7.1.1 Keel Spacing ...... 143
7.1.2 Keel Age ...... 143
7.2 Level Ice ...... 144
7.3 Other Ice ...... 144
7.4 Ridge Consolidated Layer ...... 144
7.5 Ridge Actions ...... 145
7.5.1 Ice Strength Coefficient CR ...... 145
7.5.2 Keel Action Fk ...... 145
Chapter 8: Conclusions ...... 147
8.1 General ...... 147
8.2 Findings ...... 148
8.3 ISO 19906 Implementation ...... 149
References ...... 151
Appendices ...... 167
xiii List of Figures
Page Figure 2.1: Map of the Beaufort Sea ...... 5 Figure 2.2: Map of the Chukchi Sea ...... 7 Figure 2.3: Ice Thickness ...... 9 Figure 2.4: Pressure Ridge Diagram ...... 12 Figure 2.5: Stamukhi Diagram ...... 15 Figure 2.6: Typical Demand/Capacity Plot ...... 17 Figure 2.7: Offshore Caisson Structure Site Map ...... 28 Figure 2.8: Tarsiut Caisson Profile ...... 30 Figure 2.9: SSDC Beaufort Sea ...... 31 Figure 2.10: CRI Beaufort Sea...... 32 Figure 2.11: Molikpaq Caisson Structure Beaufort Sea ...... 33 Figure 3.1: Site Map ...... 37 Figure 3.2: Typical IPS and ADCP Mooring Diagram...... 39 Figure 3.3: Spatial Conversion Algorithm ...... 41 Figure 3.4: Spatial Ice Profile ...... 42 Figure 3.5: Keel Shadowing Illustration ...... 44 Figure 3.6: Keel Identification Algorithm ...... 46 Figure 3.7: Level Ice Identification Algorithm ...... 50 Figure 3.8: Other Ice Identification Algorithm ...... 52 Figure 4.1: Starting Threshold P-Value Test Summary ...... 62 Figure 4.2: 2005-06 Site A Stacked Keel Shapes ...... 64 Figure 4.3: Keel Draft Histogram ...... 65 Figure 4.4: Shifted Keel Draft Histogram ...... 66 Figure 4.5: Keel Draft Exponential Probability Plot ...... 68 Figure 4.6: Keel Draft Weibull Probability Plot ...... 69 Figure 4.7: Keel Width Exponential Probability Plot ...... 71
xiv Page Figure 4.8: Keel Width Weibull Probability Plot ...... 72 Figure 4.9: Keel Width Lognormal Probability Plot ...... 72 Figure 4.10: Beaufort Keel Width Modal Analysis Plot ...... 74 Figure 4.11: Keel Angle Determination ...... 75 Figure 4.12: Keel Speed Exponential Probability Plot ...... 76 Figure 4.13: Keel Speed Weibull Probability Plot ...... 76 Figure 4.14: Keel Speed Lognormal Probability Plot ...... 77 Figure 4.15: Keel Speed v. Draft ...... 78 Figure 4.16: 2005-06 Site A Keel Spacing ...... 79 Figure 4.17: Keel Spacing Weibull Probability Plot ...... 81 Figure 4.18: Keel Spacing Lognormal Probability Plot ...... 81 Figure 4.19: 2005-06 Site A Ice Velocity Rose ...... 84 Figure 4.20: Level Ice Distribution ...... 85 Figure 4.21: 2005-06 Site A January Level Ice Draft ...... 86 Figure 4.22: 2005-06 Site A Other Ice Histogram ...... 87 Figure 5.1: 2005-06 Site A Keel Totals by Month ...... 89 Figure 5.2: Beaufort Sea Diagrammatic Keel Width/Angle ...... 91 Figure 5.3: Chukchi Sea Diagrammatic Keel Width/Angle ...... 92 Figure 5.4: Beaufort Keel Speed v. Draft ...... 93 Figure 5.5: Chukchi Keel Speed v. Draft ...... 93 Figure 5.6: Keel Spacing...... 94 Figure 5.7: Beaufort Site Ice Velocity Rose ...... 96 Figure 5.8: Chukchi Site Ice Velocity Rose...... 97 Figure 5.9: Monthly Level Ice Growth ...... 99 Figure 5.10: 2005-06 Site A Other Ice Histogram ...... 100 Figure 6.1: Keel Depth Probability v. Depth ...... 107 Figure 6.2: CDF Corresponding to P(D) ...... 109
xv Page Figure 6.3: Beaufort Sea Critical Keel Depth as a Function of Service Life...... 112 Figure 6.4: Chukchi Sea Critical Keel Depth as a Function of Service Life ...... 113 Figure 6.5: Beaufort Limit State Actions ...... 123 Figure 6.6: Chukchi Limit State Actions ...... 125 Figure 6.7: Recorded Molikpaq Ridge Load v. Computed Ridge Load ...... 129
Figure 6.8: CR Estimate from Molikpaq FY Ridges ...... 133
Figure 6.9: Consolidated Layer Load with Variation of CR ...... 134
Figure 6.10: CR Molikpaq Analysis ...... 137 Figure 6.11: FY Level Ice Weight Determination ...... 140 Figure 6.12: FY Ridge Weight Determination ...... 140 Figure A.1: Beaufort Sea Keel Draft Histogram ...... 167 Figure A.2: Chukchi Sea Keel Draft Histogram ...... 168 Figure A.3: Beaufort Sea Keel Draft Exponential Plot ...... 168 Figure A.4: Beaufort Sea Keel Draft Weibull Plot ...... 169 Figure A.5: Chukchi Sea Keel Draft Exponential Plot ...... 169 Figure A.6: Chukchi Sea Keel Draft Weibull Plot ...... 170 Figure A.7: 2005-06 Site A Keel Totals by Month ...... 170 Figure A.8: 2005-06 Site B Keel Totals by Month ...... 171 Figure A.9: 2006-07 Site A Keel Totals by Month ...... 171 Figure A.10: 2006-07 Site B Keel Totals by Month ...... 172 Figure A.11: 2007-08 Site A Keel Totals by Month ...... 172 Figure A.12: 2007-08 Site K Keel Totals by Month ...... 173 Figure A.13: 2007-08 Site V Keel Totals by Month ...... 173 Figure A.14: 2009-10 Site A Keel Totals by Month ...... 174 Figure A.15: 2009-10 Site V Keel Totals by Month ...... 174 Figure A.16: 2009-10 Burger Keel Totals by Month ...... 175 Figure A.17: 2009-10 Crackerjack Keel Totals by Month ...... 175
xvi Page Figure A.18: 2010-11 Site A Keel Totals by Month ...... 176 Figure A.19: 2010-11 Site V Keel Totals by Month ...... 176 Figure A.20: 2010-11 Burger Keel Totals by Month ...... 177 Figure A.21: 2010-11 Crackerjack Keel Totals by Month ...... 177 Figure B.1: Beaufort Sea Diagrammatic Keel Width/Angle 179 Figure B.2: Chukchi Sea Diagrammatic Keel Width/Angle ...... 179 Figure C.1: 2005-06 Site A Ice Velocity Rose 181 Figure C.2: 2005-06 Site B Ice Velocity Rose ...... 182 Figure C.3: 2006-07 Site A Ice Velocity Rose ...... 182 Figure C.4: 2006-07 Site B Ice Velocity Rose ...... 183 Figure C.5: 2006-07 Site K Ice Velocity Rose ...... 183 Figure C.6: 2007-08 Site A Ice Velocity Rose ...... 184 Figure C.7: 2007-08 Site K Ice Velocity Rose ...... 184 Figure C.8: 2007-08 Site V Ice Velocity Rose ...... 185 Figure C.9: 2009-10 Site A Ice Velocity Rose ...... 185 Figure C.10: 2009-10 Site V Ice Velocity Rose ...... 186 Figure C.11: 2009-10 Burger Ice Velocity Rose ...... 186 Figure C.12: 2009-10 Crackerjack Ice Velocity Rose ...... 187 Figure C.13: 2010-11 Site A Ice Velocity Rose ...... 187 Figure C.14: 2010-11 Site V Ice Velocity Rose ...... 188 Figure C.15: 2010-11 Burger Ice Velocity Rose ...... 188 Figure C.16: 2010-11 Crackerjack Ice Velocity Rose ...... 189 Figure D.1: 2005-06 Site A Level Ice Distribution ...... 191 Figure D.2: 2005-06 Site B Level Ice Distribution ...... 192 Figure D.3: 2006-07 Site A Level Ice Distribution ...... 193 Figure D.4: 2006-07 Site B Level Ice Distribution ...... 194 Figure D.5: 2006-07 Site K Level Ice Distribution ...... 195
xvii Page Figure D.6: 2007-08 Site A Level Ice Distribution ...... 196 Figure D.7: 2007-08 Site K Level Ice Distribution ...... 197 Figure D.8: 2007-08 Site V Level Ice Distribution ...... 198 Figure D.9: 2009-10 Site A Level Ice Distribution ...... 199 Figure D.10: 2009-10 Site V Level Ice Distribution ...... 200 Figure D.11: 2009-10 Burger Level Ice Distribution ...... 201 Figure D.12: 2009-10 Crackerjack Level Ice Distribution ...... 202 Figure D.13: 2010-11 Site A Level Ice Distribution ...... 203 Figure D.14: 2010-11 Site V Level Ice Distribution ...... 204 Figure D.15: 2010-11 Burger Level Ice Distribution ...... 205 Figure D.16: 2010-11 Crackerjack Level Ice Distribution ...... 206 Figure E.1: Beaufort Other Ice Draft 207 Figure E.2: Chukchi Other Ice Draft ...... 208 Figure E.3: 2005-06 Site A Other Ice Draft ...... 208 Figure E.4: 2005-06 Site B Other Ice Draft ...... 209 Figure E.5: 2006-07 Site A Other Ice Draft ...... 209 Figure E.6: 2006-07 Site B Other Ice Draft ...... 210 Figure E.7: 2006-07 Site K Other Ice Draft ...... 210 Figure E.8: 2007-08 Site A Other Ice Draft ...... 211 Figure E.9: 2007-08 Site K Other Ice Draft ...... 211 Figure E.10: 2007-08 Site V Other Ice Draft ...... 212 Figure E.11: 2009-10 Site A Other Ice Draft ...... 212 Figure E.12: 2009-10 Site V Other Ice Draft ...... 213 Figure E.13: 2009-10 Burger Other Ice Draft ...... 213 Figure E.14: 2009-10 Crackerjack Other Ice Draft ...... 214 Figure E.15: 2010-11 Site A Other Ice Draft ...... 214 Figure E.16: 2010-11 Site V Other Ice Draft ...... 215
xviii Page Figure E.17: 2010-11 Burger Other Ice Draft ...... 215 Figure E.18: 2010-11 Crackerjack Other Ice Draft ...... 216
xix
List of Tables
Page Table 2.1: Offshore Caisson Site Information ...... 29 Table 3.1: Dataset Details ...... 36 Table 3.2: Keel Identification Summary ...... 47 Table 3.3: Level Ice Identification Summary ...... 51 Table 3.4: Other Ice Identification Summary ...... 53 Table 4.1: Keel Draft PDF Parameters ...... 67 Table 4.2: Keel Draft P-Value Summary ...... 70 Table 4.3: Keel Spacing PDF Parameters ...... 80 Table 4.4: Keel Spacing P-Value Summary ...... 82 Table 5.1: Keel Draft Weibull Parameter Summary ...... 90 Table 5.2: Keel Spacing Lognormal Parameters ...... 95 Table 5.3: Ice Type Percentages ...... 98 Table 6.1: Beaufort Sea ISO 19906 Sea Ice Conditions ...... 102 Table 6.2: Chukchi Sea ISO 19906 Sea Ice Conditions ...... 104 Table 6.3: Ice Properties Summary ...... 120 Table 6.4: Summary of FY Ridge Events on the Molikpaq ...... 126 Table 6.5: Molikpaq Input Parameters ...... 128 Table 6.6: Horizontal Action Variation ...... 130
Table 6.7: CR Molikpaq Ridge Analysis ...... 132
Table 6.8: Molikpaq FY Level Ice CR Analysis ...... 136
xxi
xxii List of Appendices
Page Appendix A: Pressure Ridge Keel Draft ...... 167
Appendix B: Pressure Ridge Keel Width ...... 179
Appendix C: Ice Velocity ...... 181
Appendix D: Level Ice ...... 191
Appendix E: Other Ice ...... 207
xxiii
xxiv Acknowledgments
I am grateful to both Shell Offshore Incorporated (Shell) and ASL Environmental Sciences Inc. (ASL) for sharing sea ice data from lease areas in the Beaufort and Chukchi Seas. I am also appreciative of the instruction and guidance of Dr. Andrew Metzger (University of Alaska Anchorage) and Dr. Hajo Eicken (University of Alaska Fairbanks) throughout the entire process. Furthermore, I am greatly indebted to Dr. Andy Mahoney (University of Alaska Fairbanks), who provided immeasurable help understanding all matters concerning sea ice and Matlab© coding. I would also like to thank the Bureau of Safety and Environmental Enforcement (BSEE), who provided funding and support throughout the project. This work was supported by funding from the Bureau of Safety and Environmental Enforcement, Alaska OSC Region, Anchorage, Alaska, under contract E13PC00020.
xxv
xxvi Chapter 1: Introduction
1.1 Background
The Beaufort and Chukchi Seas are located off the north and north-western coasts of Alaska respectively. Much research and exploration has been conducted by industry in these areas and it seems probable that vast hydrocarbon reservoirs exist in these regions. Due to the highly volatile nature of hydrocarbon prices recently there has been a renewed interest in developing these reservoirs by both the oil companies and the American government (Timco & Frederking, 2009). However, since both seas lie in the Arctic Ocean there are various engineering challenges that must be overcome in order to responsibly develop these resources.
One of the most immediate and pertinent engineering challenges is the presence of sea ice. Sea ice has a major impact on how offshore structures will be designed and constructed in these regions, yet for such an important topic, readily available information on current conditions is sparse (Timco & Johnston, 2002). The majority of literature on this topic is from the 1970’s and 1980’s. Due to the ever-changing nature of the climate and sea ice, having the most recent information is crucial to providing a safe, functional, and cost effective structure.
While industry stakeholders may wish to develop hydrocarbon infrastructure in the Beaufort and Chukchi Seas, it is also important to consider the environmental impact potential accidents may have on these regions. The Beaufort coast provides a critical habitat for several species essential to the subsistence lifestyle of Arctic native populations (Dunton, Weingartner, & Carmack), while the Chukchi Sea is one of the most biologically productive regions in the world ocean due to its nutrient-rich makeup (Grebmeier, Cooper, Feder, & Sirenko, 2006). If a hydrocarbon spill were to occur in these regions it would be disastrous for the entire Arctic ecosystem. An offshore structure improperly designed for the existing sea ice conditions in the region would create a legitimate risk of a spill event occurring. 1 This is a major reason why government agencies have been established to monitor offshore development. Chief among these agencies are the Bureau of Safety and Environmental Enforcement (BSEE) and the Bureau of Ocean Energy Management (BOEM). Among other duties, these agencies are tasked with regulating and monitoring offshore development in the Beaufort and Chukchi Seas. Thus it is critical to have some reference for sea ice conditions in these regions, as they provide the demands on offshore structures (Kovacs A. , 1983). For this reason BSEE is considering the adoption of the ISO 19906 Standard: Petroleum and Natural Gas Industries – Arctic Offshore Structures (i.e., the Normative) as a standard for Arctic offshore structure design.
The ISO 19906 is a design normative that was developed to address design requirements and assessments for all offshore structures used by the petroleum and natural gas industries worldwide (International Organization for Standardization, 2010). The ISO 19906 contains sea ice parameters for both the Beaufort and Chukchi Seas, among many others. However, some of the information in the Normative is inconsistent or has been omitted. Many important design values are not present in the Normative and not all of the given values follow the same mandated reliability based design philosophy. It is important that, before the ISO 19906 is implemented, design values are present and consistent.
1.2 Objective
When designing an offshore structure in either the Beaufort or Chukchi Seas it is critical that the design engineer have access to accurate environmental information to compute structural loads. Due to these seas being part of the Arctic Ocean the most pertinent design load is caused by various sea ice features. The goal of this study was to characterize the physical features of sea ice in these regions using a probability based approach when possible. Furthermore, an examination of the calculation of ice actions was conducted.
2 1.3 Data Collection
The primary data for this project was provided by Shell Offshore Incorporated (Shell). Shell had contracted ASL Environmental Sciences Incorporated (ASL) to collect and preliminarily process both sea ice draft, the distance from the waterline to the bottom of the ice, and velocity data. Beginning in 2005, ASL deployed ice profiling sonar (IPS) and acoustical Doppler current profiler (ADCP) moorings to measure ice draft and velocity at a variety of different sites in both the Beaufort and Chukchi Seas. The IPS measures ice draft by identifying the acoustic echo from the bottom of the ice and computing the distance based on the time it takes the echo to travel (Melling, Johnston, & Riedel, 1995). The ADCP works by determining the motion of an underwater acoustic target by measuring the Doppler shift of the echo returned from it along four separate acoustic beams (Melling, Johnston, & Riedel, 1995). More details about these instruments are provided in the Data section.
Altogether ASL had six sites: four in the Beaufort Sea and two in the Chukchi Sea. In the Beaufort Sea, the moorings at the four sites recorded full datasets for parts of five seasons, 2005-2008 and 2009-2011. In the Chukchi Sea, the moorings at the two sites recorded full datasets for parts of two seasons, 2009-2011. Each dataset consisted of a draft and velocity time series file for an individual site during an independent year long period, or season. This provided a more than adequate amount of information to make a statistical model of different sea ice features.
1.4 Data Processing
The first step in processing the data was performed by ASL before it was delivered to the project team. In order to obtain accurate measurements it is important to incorporate many different factors such as temperature, pressure, and tilt of the IPS (Melling, Johnston, & Riedel, 1995). Furthermore, the change in the density and sound speed profiles within the water column of the IPS must be taken into account (Melling, Johnston, & Riedel, 1995). This preliminary processing of the raw data also included 3 adjusting for erroneous data points, mooring drift over time, and adjusting for errors in the start and end time records (Fissel, et al., 2010). This process is examined further in the Data section.
The next step was to interpolate the draft time series datasets with their respective velocity time series datasets to produce a dataset of evenly spaced draft values. While the ice draft dataset had measurements at regular time intervals, due to the irregular motion of the ice the drafts were unevenly spaced. By incorporating the velocity time series and using a cubic interpolation an evenly spaced spatial was created. The resulting spatially defined dataset contained draft values all separated by one meter (Fissel, et al., 2010). This process is examined further in the Data section.
Now that a consistent series of interpolated datasets had been created, the individual ice features needed to be discerned. For this a suite of interactive software was developed to accurately compile and analyze the data. Utilizing the Matlab© and Mathematica software packages, several programs were written and tested to automate the bulk of the computations. This suite identified different sea ice features such as level ice, pressure ridge keels, and ice that was neither level or ridge ice. Additional statistical analyses were performed on the resulting data. The purpose of the analyses was to enable estimation of critical ice features from information that was available. The specifics of these processes are discussed in the Data Analysis and Results sections.
1.5 Presentation of Results
The results for this project are displayed in a multitude of formats. Emphasis has been placed on trying to present these results in a simple manner that is clear and concise. Results, such as probability density functions, are presented both graphically and numerically. When possible the results are displayed diagrammatically to give the reader a sense of the scale of the results.
4 Chapter 2: Literature Review
2.1 Beaufort Sea
The Beaufort Sea is part of the greater Arctic Ocean and is located along the northern coast of Alaska and the north-western coast of Canada. Between both the American and Canadian regions the Beaufort Sea roughly covers an area from 69° N to 75° N and 125° W to 152° W. The depth of the seafloor in the Beaufort Sea varies greatly, from two meters near shore to several thousand further from shore (see Figure 2.1) (International Organization for Standardization, 2010).
Figure 2.1: Map of the Beaufort Sea (International Organization for Standardization, 2010, Figure B.7-1)
5 Of particular importance to sea ice conditions are the climate and hydrology of the region. The Beaufort Gyre is a major circulatory system of the Arctic Ocean in which the long-term average ice drift forms a clockwise pattern around a persistent region of high pressure known as the Beaufort High. In the southern Beaufort Sea the ice therefore typically drifts westward past the coast of Alaska, driven by prevailing easterly or northeasterly winds. This drift pattern transports ice into U.S. waters from the Canadian high Arctic, where some of the oldest, thickest sea ice in the northern hemisphere is found. These winds can cause large segments of sea ice to converge against the coast leading to deformation and the dynamical creation of thick ice in the form of ridges (Mahoney A. R., 2012).
From an engineering standpoint, sea ice in the Beaufort Sea can differ significantly from that found in the Chukchi Sea. The Beaufort Gyre, as mentioned previously, transports some of the oldest and thickest ice in the Arctic into the Beaufort from the Canadian Archipelago. This, along with other conditions, leads the Beaufort Sea to retain significant perennial ice cover (Mahoney A. R., 2012). Along with this perennial ice cover is landfast ice. Landfast ice is by definition attached to the shoreline and remains stationary for extended periods of time. In the Beaufort Sea landfast ice is not present year round, usually developing in September or October and retreating in June (Mahoney A. , Eicken, Gaylord, & Shapiro, 2007; Mahoney A. R., Eicken, Gaylord, & Gens, 2014). Lastly, the seasonal ice zone occupies the area between the perennial ice zone and landfast ice. This zone is mostly composed of FY ice and its extent varies greatly depending on the time of year (International Organization for Standardization,
2010).
2.2 Chukchi Sea
The Chukchi Sea is part of the greater Arctic Ocean and is located between the north-eastern edge of Asia and the north-western edge of North America. To the west of the Chukchi Sea lies the East Siberian Sea; to the east the Beaufort Sea; to the south the
6 Bering Sea; and to the north the Arctic Basin. The Chukchi Sea covers a large expanse and thus is usually broken into four regions (see Figure 2.2) (International Organization for Standardization, 2010).
Figure 2.2: Map of the Chukchi Sea (International Organization for Standardization, 2010, Figure B.8-1)
Of particular importance to the formation and movement of sea ice in the Chukchi Sea is the climate and hydrography of the region. Strong winds can occur in the Chukchi Sea, from a variety of different directions, which has a direct impact on the movement and deformation of sea ice in the region. Due to the many different currents present in the Chukchi Sea ice conditions can vary greatly between regions. For instance, the warm flow from the Pacific Ocean to the south can quickly melt the sea ice in region three,
7 while the sea ice in region four may melt more slowly due to the colder flow from the Arctic Ocean (International Organization for Standardization, 2010).
Lastly, it is important to describe the ice conditions in the Chukchi Sea. In general, the Chukchi Sea is entirely covered by ice from November or December until May or June. Since the Chukchi Sea is connected to the Pacific Ocean there is a net northward transport of heat which enhances the early loss of ice in the region (Woodgate, Weingartner, & Lindsay, 2010). This, in part, causes the sea ice in the Chukchi Sea to be, in general, newly grown each year. Furthermore, the winds in the Chukchi create sections of open water in leads, which are linear openings in the ice formed either between floes or at the coast (Mahoney A. R., 2012).
In order for landfast ice to extend into the deeper water of the Chukchi Sea the area must be anchored by grounded ridges (Mahoney A. R., Eicken, Gaylord, & Gens, 2014). While the Chukchi Sea is much shallower than the Beaufort Sea on average, within approximately 25 kilometers of the coast the depth of the Chukchi Sea is deeper than the Beaufort (Mahoney A. R., Eicken, Gaylord, & Gens, 2014). Since the seafloor is relatively deep near the coast of the Chukchi there also is not a large presence of grounded pressure ridges.
2.3 Measurement of Ice Draft and Keel Depth
Throughout the history of sea ice research there have been a variety of methods employed to obtain relevant sea ice data. However, before an explanation of this can be done, first one must have a solid grasp on the terms associated with how sea ice thickness is measured. The thickness of a segment of sea ice can effectively be separated into two components: ice draft and ice freeboard. Ice draft consists of the thickness of sea ice below the waterline. This is typically what is measured by underwater methods. Conversely, ice freeboard consists of the thickness of sea ice above the waterline. The overall ice thickness is the total of these two components (see Figure 2.3).
8
Figure 2.3: Ice Thickness
Initial exploration of the Arctic Ocean by the United States began in 1947 with the diesel-battery submarine the U.S.S. Boarfish, which recorded the first successful dive under sea ice in the Chukchi Sea. With the advent of nuclear powered submarines further distances could be traversed, opening the Arctic up for a rapid expanse in exploration. In 1957 the U.S.S. Nautilus, a nuclear powered submarine, cruised 1,300 miles under the sea ice, a first for United States nuclear powered submarines. In order to pilot and record sea ice draft data a series of forward, upward, and downward looking sonars were employed (Lyon, 1961). After the voyage of the U.S.S. Nautilus more sea ice draft data began to be collected in various waters. For example, in 1976 the U.S.S. Gurnard (SSN- 662) collected 1,400 kilometers of data from the Beaufort Sea (Wadhams & Horne, 1980), which was used to look at a number of different ice features. The identification of keel features is similar to that employed today, which is explained in detail in the Data section.
During the late 1970’s and early 1980’s moored self-contained upward looking sonar began to be used to acquire underside topographic measurements of sea ice. Typically, these moorings include an ice profiling sonar (IPS) and acoustic Doppler 9 current profiler (ADCP) (Melling, Johnston, & Riedel, 1995). The workings of these instruments are elaborated on in the Data section of this paper. With the increased cost efficiency and applicability of these instruments in acquiring data they have become a common method for data acquisition in contemporary times (Melling, Johnston, & Riedel, 1995).
2.4 Sea Ice Morphology
The morphology of sea ice in the Beaufort and Chukchi Seas is a wide and complex topic. For this work it is easiest to divide sea ice into three broad categories: pressure ridge, level ice, and other ice. While there certainly are more categories of sea ice, such as ice islands and rafted ice, for the objective of this project only these three broad categories are examined in great detail. Furthermore, it is important to divide sea ice into first-year (FY) and multi-year (MY) ice. While the data used in this study primarily pertains to FY ice, it is important to understand the difference between the two ice types due to their different mechanical engineering properties.
2.4.1 First-Year Ice
FY ice is defined as ice that has not yet existed through one summer. In the Beaufort and Chukchi Seas, FY ice that forms at the beginning of winter typically reaches a thickness of 1.5 to 1.8 meters, though FY ice that begins forming later will be thinner. As sea ice grows, it rejects salt into the ocean beneath, but some salt remains in the ice, encapsulated within liquid brine pockets. Depending on the temperature and growth rate of the ice, this brine volume can represent a bulk salinity of 4 to 12 psu (practical salinity unit) and result in ice porosities of one to ten percent. Due to this, FY ice is typically rather thin and not well developed. Since this ice has only been present for less than one season it is usually relatively porous and has a high salinity. Recently there has been an increase in the number of articles and reports concerning FY ice. This is
10 due to the dramatic shift in climate in the Arctic region, which has drastically changed the ratio of FY ice to MY ice (Wadhams & Toberg, 2012).
2.4.2 Multi-Year Ice
MY ice is defined as ice that has survived one or more summers, though some terminology draws a distinction between MY ice and second year (SY) ice. Due to growth during successive winters, MY ice can grow to greater thicknesses than FY ice. Melt processes in the summer result in a reduction in both salinity and porosity as fresh meltwater flushes brine pockets and refreezes the following winter. Due to its lack of salt, this melt water refreezes more readily and without the porosity of ice formed from saltwater. This combination of low porosity and salinity can greatly increase the strength of MY ice relative to FY ice. MY ice is common in the literature from the 1970’s and 1980’s, however it has become increasingly rare in the Arctic due to the dramatic losses of perennial ice in recent decades (Wadhams & Toberg, 2012).
2.4.3 Pressure Ridges
A pressure ridge is a deformed ice feature composed of blocks of ice piled above and below the waterline. Pressure ridges are formed by convergent deformation of ice cover due to factors such as wind and ocean current. The breaking of existing sea ice cover occurs in some combination of compression and shear, the balance of which has an impact on the characteristics of the ridge. As the existing sea ice cover fractures and deforms, blocks of ice are forced beneath the ice cover. These blocks begin to stack together, forming the keel of the pressure ridge. Simultaneously, blocks also stack above the waterline, forming the sail of the pressure ridge. Ridges formed during winter can consolidate to a certain depth below the waterline over time, due to conduction of heat into the cold atmosphere (see Figure 2.4) (Ekeberg, Høyland, & Hansen, 2014).
11
Figure 2.4: Pressure Ridge Diagram (Reproduced from Strub-Klein & Sudom 2012, Figure 1)
An important aspect of pressure ridges, especially in an engineering context, is whether they are defined as FY or MY ridges. During its first winter an ice ridge is designated as a FY ridge. However, if a ridge manages to survive one or more summer seasons then it is considered a MY ridge (Ekeberg, Høyland, & Hansen, 2014). What separates a FY ridge from a MY ridge is the degree to which it has consolidated. As with brine pockets in MY ice, the voids between ice blocks in a FY pressure ridge can be flushed with fresh meltwater, which refreezes and deepens the consolidated layer. A FY ridge can be thought of as a collection of ice blocks bound together by a weak bond via consolidation (Kovacs, Weeks, Ackley, & Hibler III, 1973). However, a MY ridge can be thought of as an almost solid piece of ice (Kovacs, Weeks, Ackley, & Hibler III, 1973). Since the MY ridge has survived at least a full summer and winter season
12 the blocks have had ample time to freeze together and consolidate into one solid unit. Furthermore, as the ridge consolidates its salinity and porosity decrease,
thereby increasing its strength (Kovacs, Weeks, Ackley, & Hibler III, 1973). This designation between FY and MY ice can have a dramatic impact on the design of offshore structures.
2.4.4 Level Ice
Level ice is a term used to describe sea ice that has not been mechanically thickened through deformation like a pressure ridge. The thickness of level ice is therefore controlled by thermodynamic processes and can be related to the age and growth rate of the ice. In the absence of mechanical deformation, level ice can therefore be identified by the uniformity of its thickness or draft (Melling & Riedel, 1995). The specific thickness of a level ice segment is limited by the number of freezing degree days in a season (International Organization for Standardization, 2010). Overall, there are not a large number of articles that deal with the distribution of level ice in the Arctic. This most likely is due to the fact that level ice is not thought to be the controlling condition for offshore structure design. However, most sources seem to indicate that the majority of an ice floe area consists of level ice (Wadhams & Horne, 1980).
2.4.5 Rafted Ice
There have been two types of rafted ice structures observed: simple rafted and finger rafted. Simple rafting occurs when two ice sheets interact along a straight edge and one sheet overrides the other. Finger rafting occurs when the interacting sheets fracture along lines perpendicular to their interacting edge and form fingers. Alternate fingers are then over-thrust and underthrust, leaving an interlocked structure. Multiple rafting actions may also occur, producing thick sea ice features. While the bonds between the layers are initially weak they can strengthen over time to produce a consolidated ice sheet (Babko, Rothrock, & 13 Maykut, 2002; Bailey, Sammonds, & Feltham, 2012). It has been found that rafted ice often is located near pressure ridges (International Organization for Standardization, 2010).
Due to the absence of a keel or sail, rafted ice can be difficult to distinguish from level ice without in situ observations. However, rafted ice is a design condition that should be taken into consideration when designing offshore structures in the Arctic.
2.4.6 Stamukhi
Stamukhi, a collection of stamukha, is a formation of grounded ice piles and ridges in the seafloor. Stamukha generally occur when an ice pressure ridge moves from a location with a deep seafloor to an area with a shallow seafloor. As the pressure ridge enters the shallow region the keel of the ridge typically does not deform. Instead the ridge creates an indentation in the seabed and forms a large scour as it moves. This scouring can affect undersea utilities such as oil pipelines (see Figure 2.5) (International Organization for Standardization, 2010).
14
Figure 2.5: Stamukhi Diagram (Reproduced from "Stamukha Drawing" by Lusilier - Own work. Licensed under CC BY-SA 3.0 via Wikimedia Commons – http://commons.wikimedia.org/wiki/File:Stamukha_Drawing.svg#/media/File:Stamukha_ Drawing.svg
2.4.7 Rubble Ice
Rubble ice forms mechanically, similarly to pressure ridges. Rubble ice can form from floe deformation or when the ocean swells. For rubble ice the debris does not stack to a large extent and the draft generally remains shallow. Thus the rubble ice is not consistent enough in draft to be classified as level ice, yet generally not deep enough in draft to be classified as a pressure ridge (National Oceanic and Atmospheric Administration, n.d.). Due to its relatively shallow draft rubble ice is not considered a primary design event for offshore structures; however its impact should be considered (International Organization for Standardization, 2010).
2.4.8 Icebergs and Ice Islands
Icebergs and ice islands are important design features to consider for offshore design. An iceberg is a large freshwater ice body that calves off from a 15 glacier. Icebergs can survive for many years in Arctic regions and present a hazard not only to structures but also ships in the region. An ice island is similar to an iceberg, except that it is usually larger and may have been calved from an ice shelf. Besides being created in nature ice islands can also be constructed artificially. Icebergs and ice islands in the Beaufort and Chukchi Seas are rare events that are not well understood (International Organization for Standardization, 2010).
2.5 Reliability Engineering
Due to the large variations of sea ice parameters and the changing conditions in the Arctic it is not realistic to establish deterministic ice features, ice events, or ice actions. However, some values for ice actions (ice forces) must be established to design offshore structures. One way to address a nondeterministic problem is with the likelihood of the occurrence of an event, or its occurrence frequency. The occurrence frequency, a number from zero to one, may be defined as how frequently an event occurs in a large number of trials or experiments. This method requires an appropriately large sample to study the frequency of occurrences of an event (Ross S. , 2002). Reliability shall be defined as:
“The ability of an item to perform a required function, under given
operational conditions, for a stated period of time.” (Høyland & Rausand, 2004)
Reliability engineering is a broad topic that includes not only the determination of design loading but also the reliability of materials and what type of failure mode will occur. There already is an extensive body of knowledge regarding material failure and failure modes (Timco & Weeks, 2010).
Reliability engineering for load determination is essentially trying to make an educated guess using probability on what future loading may be applied based on historical data. Often, this requires the analysis of data related to the load demands on a 16 structure to determine load conditions with a low probability of being exceeded. Such low probability events may be determined by statistical means, sometimes in terms of return periods, or by using probability theory to establish threshold events with a low probability of exceedance in some timeframe (see Figure 2.6).
Figure 2.6: Typical Demand/Capacity Plot
2.6 ISO 19906 Design Philosophy
The ISO 19906 has an inherent design philosophy for offshore structures that follows the reliability based engineering method described above. The ISO 19906 however examines limit states to determine what magnitudes of loads should be considered. The four limit states considered by the ISO 19906 are: ultimate limit state (ULS), service limit state (SLS), fatigue limit state (FLS), and abnormal limit state (ALS) (International Organization for Standardization, 2010).
17 The ULS ensures that over the design life of the structure there is an acceptably low probability of actions that may cause significant structural damage. The ULS considers both local and global actions. The SLS is where the structure loses the capability to perform adequately under normal use. The FLS considers the cyclic or repeated actions due to ice actions, such as compressive and flexural ice failure. Lastly, the ALS considers abnormal ice events. In this case the structure is permitted to suffer some structural damage. However, the structure should have enough reserve strength to keep from losing complete integrity (International Organization for Standardization, 2010).
All of the limit state design values are associated with a specific probability, as stipulated by the ISO 19906. The SLS shall be designed for events with an annual exceedance probability not greater than 10-1, or 10%. The ULS shall be designed for events with an annual exceedance probability not greater than 10-2, or 1%, based on linear elastic methods of structural analysis. The ALS shall be designed for events with an annual exceedance probability not greater than 10-4, or 0.01%, based on non-linear methods of structural analysis (International Organization for Standardization, 2010). For the purposes of this project the FLS shall be omitted.
2.7 Arctic Structure Design
While there are definitely challenges to designing offshore structures in the Arctic environment the general design process is similar to a regular structure. First, a designer must consider the conditions the structure is subjected to, such as location and operating times. Next, they must determine which loading conditions, such as snow or sea ice, should be considered. The designer then selects or computes the loading on the structure, in this case due to sea ice. Upon calculating the forces that will be applied to the structure, the engineer must determine the limit states and begin to design members and connections accordingly.
18 2.8 Pressure Ridge Statistics
Since pressure ridges are commonly considered the design event for offshore structures in ice covered waters there has been much effort expended to develop probabilistic models to predict pressure ridge characteristics (Ekeberg, Høyland, & Hansen, 2014). Since the ISO 19906 uses the draft of the keel as the primary input design value, most of the statistical analysis has been devoted towards that value. However, while less common, there are probabilistic models that examine other keel characteristics such as width, spacing, and angle. There also has been research conducted into determining the properties of the sail of the ridge. While not as critical as the keel, these properties are examined in the literature review since some play a role in the ice action calculations.
2.8.1 Pressure Ridge Keel Draft Statistics
Due to their importance in the design of offshore Arctic structures there is a plethora of literature available on ridge keel draft statistics. Of particular note are the works by Wadhams (2011), Davis (1995) and Fissel (2010), which are all relatively recent.
Wadhams examined 204 kilometers of draft data collected in the Fram Strait and Beaufort Sea during the 2007 season. This included an area of extensive research near this project’s area of interest, at approximately 73° N and 146° W. After determining which ice features were pressure ridges Wadhams applied reliability methods to determine extreme events. Wadhams showed that a negative exponential probability density function (PDF), which represents a stochastic process of ridge production, was an excellent fit for his data. This is consistent with the findings of other researchers and seems to be generally accepted within the scientific community (Ekeberg, Høyland, & Hansen, 2014; Hibler III, Weeks, & Mock, 1972; Obert & Brown, 2011; Wadhams P. , 1983; Wadhams & Davy, 1986; Wadhams P. , 2011). 19 Davis examined 729 ridges that were greater than five meters deep from geographically distinct regions between Greenland and Svalbard during a 1987 study. While Davis was not seeking to determine the extreme design events for pressure ridges, he did fit a PDF to the pressure ridge keel data. Unlike Wadhams, Davis found that a lognormal distribution was a better fit than a negative exponential. While the region of these ridges does not coincide with the regions of this project, it is important to note this work since it is one of the few to suggest this distribution (Davis & Wadhams, 1995).
Lastly, Fissel examined ridges from an extensive dataset. The dataset consisted of multiple seasons at two sites in the Chukchi Sea, which made for a dataset of over 1,800 keels. When looking at keels with a draft greater than 13 meters it was found that a three parameter Weibull distribution produced favorable results (Fissel, et al., 2010).
The three articles above illustrate that there are a variety of methods and PDFs to fit ridge keel data. Some of these authors looked at all keels greater than five meters (Davis & Wadhams, 1995) when analyzing the data while others looked at only those greater than 13 meters (Fissel, et al., 2010). All of these authors found different distributions fit their data relatively well.
Along with the statistical models of sea ice pressure ridge keels the greatest keel draft recorded is also of great interest. From the literature examined for this project it was found that the deepest keel observed was 47 meters. The location of this keel was not present in the literature examined. There also was an extremely large sail observed in the Beaufort Sea and using ratios between the sail and keel a draft of 57 meters was inferred for a FY ridge (Kovacs, Weeks,
Ackley, & Hibler III, 1973).
20 2.8.2 Pressure Ridge Keel Width Statistics
The width of a pressure ridge keel is another important factor in offshore structural design in the Arctic. Most seem to agree that the width of a keel is somewhat dependent on the depth of the keel (Sudom, Timco, Sand, & Fransson, 2011). While some probabilistic models have been fit to keel width data, it is more common to see keel width to depth ratios and average or statistical mode values.
Timco (1997), using a dataset of 112 FY ridges located in the Beaufort and Baltic Seas, reported a ratio of keel width to keel depth of approximately 3.9 for FY ridges (Timco & Burden, 1997). Using a dataset of 64 ridges located in the Beaufort Sea and Queen Elizabeth Island region Timco (1997) reported a ratio of keel width to keel depth of approximately 3.3 for MY ridges (Timco & Burden, 1997). Davis (1995) however did not report his findings in terms of ratios. Davis fit a lognormal distribution to the keel width dataset and found a mean keel width of 72.8 meters and a mode of 65 meters for both FY and MY ridges in geographically distinct regions between Greenland and Svalbard during a 1987 study (Davis & Wadhams, 1995). This value is different than that reported by Sudom (2011). Sudom reported a mean keel width value of 37 meters for FY ridges and a range from 35 to 79 meters for MY ridges. Sudom (2011) examined 262 FY ridges and 85 MY ridges from various locations in the Arctic Ocean (Sudom, Timco, Sand, & Fransson, 2011). Ekeberg (2014) reported in the Fram Strait a mean observed keel width of 28 meters for 30,186 keels, which can be described with a lognormal distribution (Ekeberg, Høyland, & Hansen, 2014).
It can be observed from the examples above that there is considerable variation in the reported keel widths. While a general magnitude of keel width can be determined, it seems that there is no determinant range. The ISO 19906 only gives an angular relationship of 26° from horizontal to determine the keel width
21 based on keel depth, which works out to a 4.1:1 width to depth ratio for isosceles triangular keels (International Organization for Standardization, 2010).
2.8.3 Pressure Ridge Keel Angle Statistics
Due to the variable nature of sea ice finding a consistent angle of repose for ridge keels is difficult. While there have been some studies to examine the angle of repose of a keel, most are limited and only present a mean observed value. Example values are described to develop an understanding of the general range one should expect for a keel angle of repose.
Due to the friction and wear on MY ice ridges, there is usually a distinction made between the angle values for FY and MY ridges. Kovacs (1972) reported FY keel angles between 20 and 55°, with an average of 33° from data gathered in the Bering, Chukchi, and Beaufort Seas (Davis & Wadhams, 1995). Strub-Klein however reported a mean keel angle of 28° for over 300 FY ridges in various seas in the Arctic Ocean, including the Beaufort and Chukchi Seas, between 1971 and 2014 (Strub-Klein & Sudom, 2012). For both FY and MY ridges Davis (1995) reported ridge angle values from 8 to 36°, with a mean of 23.2° and a modal value of 18° for 729 ridges between Greenland and Svalbard. Davis (1995) also found that the data for ridge angles followed a lognormal distribution (Davis & Wadhams, 1995). From the ISO 19906 the prescribed angle for a keel is 26° from horizontal (International Organization for Standardization, 2010).
2.8.4 Pressure Ridge Keel Spacing Statistics
The spacing of pressure ridge keels is another topic that has been extensively studied. Of particular interest are the works by Hibler (1972), Mock (1972) and Wadhams (1986) since they examined data from the Beaufort Sea.
22 These articles studied the distribution of the spacing between ridge keels and looked to apply PDFs to the data.
Hibler examined ridge spacing in the Central Arctic Basin and Beaufort Sea using sonar data from submarine voyages. Looking at numerous datasets, which had a total of 18,906 keels, Hibler came to the conclusion that for the ridge spacing a Poisson distribution was valid, which implies that a negative exponential probability density function is applicable for ridge spacing (Hibler III, Weeks, & Mock, 1972).
Mock examined ridge features in the Beaufort Sea via aerial photographs taken during 1969 and 1971. By analyzing the data using goodness-of-fit tests Mock determined that the keel spacing most closely followed a negative exponential model. However, in his article Mock did note that there were significant deviations from the model, especially for close spacings (Mock, Hartwell, & Hibler III, 1972).
In 1986 Wadhams further investigated the statistics of keel spacing and came to a different conclusion than either Hibler or Mock. Using a 637 kilometer segment from a set of 1976 data in the Beaufort Sea Wadhams analyzed which PDFs would best fit the spacing data. From his research Wadhams concluded that the fit was much improved when using a three-parameter lognormal distribution. To further confirm this model Wadhams also tested it on a variety of different datasets. He found that all fit the distribution well (Wadhams & Davy, 1986).
While the authors used the same general method to come to their conclusions, they got slightly different results. Looking through further literature in this field it seemed that the lognormal distribution was generally accepted. Examples of the lognormal distribution to describe keel spacing can be found in Davis (1995), Sear (1992), and Key (1989).
23 2.8.5 Pressure Ridge Sail Statistics
While most pressure ridge features use a PDF to describe the feature, when analyzing the sail of a pressure ridge the majority of the literature uses simple ratios or equations between the keel depth and sail height. However, depending on the dataset used many of the various researchers found slightly different results. A few of these ratios are examined.
Timco and Burden (1997) reported that for sea ice in the Beaufort Sea they found mean ratios of keel depth to sail height of 4.46 for FY ridges and 3.34 for MY ridges, although it should be noted that there was significant scatter in the results (Timco & Burden, 1997). This is similar to the keel depth to sail height ratios reported by Tucker III (1989). Tucker III found a ratio of 4.5 for FY ridges and 3.2 for MY ridges (Davis & Wadhams, 1995). More recently Sudom (2011) used a dataset from various seas in the Arctic Ocean to determine ratios. Sudom found that the keel depth to sail height ratio was 4.35 for FY ridges and 3.60 for MY ridges (Sudom, Timco, Sand, & Fransson, 2011).
From the examples above it is important to note that while different, the ratios of keel depths to sail heights are relatively close. Even though these researchers used datasets from different seas, during different years, they all found ratios remarkably close. While this project did not directly measure sail height, due to the data collection method, the literature provides valuable information for the ice action calculation component of this project.
Along with the statistical models of sea ice pressure ridge sails the greatest sail height recorded is also of interest. From the literature examined for this project it was found that the highest sail recorded was 12.8 meters in the Beaufort Sea (Kovacs, Weeks, Ackley, & Hibler III, 1973).
24 2.9 Ice Velocity
While there are many different articles that have velocity measurements for different sea ice features, there were none found in this study that attempted to examine ice velocities in the probabilistic sense. In most cases the author simply examined how the velocity of ice features varied at different times of the year (Belliveau, Bugden, Eid, & Calnan, 1989). Another common general analysis of sea ice velocities was to present the average velocity or present a compass-rose plot to show the direction and magnitude of the ice (Fissel, et al., 2010).
2.10 Sea Ice Engineering Properties
When designing an offshore structure in the Arctic it is necessary to not only know the geometric properties of sea ice features but also the material properties. Material properties include compression strength, tensile strength, modulus of elasticity, and many others. The material properties of sea ice allow the design engineer to calculate the magnitude of the loads and forces applied to the structure.
Since sea ice material properties are so vital to design, there has been much effort to research them. The article A review of the engineering properties of sea ice by Timco (2010) presents the most complete findings on material properties for sea ice that was found during this literature review. The article contains findings from many different publications in this field and presents a well-rounded source of information. A few of the sea ice properties that have a particular application to this project are examined further in depth.
One property that is of interest is the angle of internal friction of sea ice. The angle of internal friction is a measure of the ability of a material to resist shear stress. The range of published sea ice rubble internal friction angle varies from 10 to 80°. However, this property is hard to distinguish since it is hard to differentiate between the contributions of the angle of internal friction and the consolidated layer to shear strength.
25 Generally accepted values range from 20 to 40° (International Organization for Standardization, 2010).
Cohesion is another property of interest. Cohesion is a measure of how “together” a material acts. For example, after a keel has impacted a structure and completely broken into separate blocks, it can be said that there is no cohesion between the units. On average the cohesion of a FY ridge keel ranges from 5 to 7 kPa (International Organization for Standardization, 2010).
The porosity of a keel feature is also important when calculating ice forces. The porosity of sea ice is determined as the overall fractional void volume (Leppäranta, Lensu, Kosloff, & Veitch, 1995). Using the equations presented in Timco (2010) the volume of the air and brine can be calculated and used to compute the porosity (Timco & Weeks, 2010). However, the ISO 19906 also gives reported values from collected literature. The Normative states that keel porosity ranges from 10 to 50% and usually increases with depth (International Organization for Standardization, 2010).
The density of sea ice is also needed to compute ice forces. For FY ice, the ice above the waterline has in situ values that range from 0.84 to 0.91 Mg∙m-3. Values ranging from 0.90 to 0.94 Mg∙m-3 have also been reported for ice below the waterline. As described by Timco (2010) a value of 0.92 Mg∙m-3 should serve as a reasonable estimate for ice density of FY ice. Timco (2010) also found that for MY ice the average densities of the complete ice sheet were between 0.910 and 0.915 Mg∙m-3 (Timco & Weeks, 2010).
However, the ISO 19906 prescribes slightly different sea ice density values. The Normative prescribes densities of 0.840 to 0.910 Mg∙m-3 for FY ice above the waterline and 0.720 to 0.910 Mg∙m-3 for MY ice above the waterline. It also has densities ranging from 0.900 to 0.920 Mg∙m-3 for both FY and MY ice below the waterline (International Organization for Standardization, 2010).
26 2.11 Sea Ice Loads on Structures
Sea ice loads on a structure, the forces that the sea ice exerts on the structure, are critical for the design of offshore structures in the Arctic. While there are many different sources to theoretically determine the force a pressure ridge exerts on a structure, there are few studies that have collected in situ data. For this project the works of Dalane (2015) and Timco (2009) are examined to show recorded pressure ridge loads on actual structures.
Dalane (2015) looked to create sea ice loads that modeled actual conditions in a controlled environment. To do this, Dalane produced laboratory ice ridges using a saline solution and set up a “floater” in a 78 meter long, 10 meter wide, and 2.5 meter deep ice tank. A floater, in this case a Sevan FPU-Ice model, is a floating circular structure that is moored to the bottom of a tank, which has a movable false bottom. This floater has various sensors to measure different variables. In order to create the impact between floater and ice ridge, the false bottom moves the floater, attached via mooring, into the ridge. Upon impact the floater measures forces. While the article looked at many different topics, of particular interest to this project were the forces applied. Dalane reported scaled forces that ranged from 50.6 to 156.9 MN corresponding to simulated ice ridges (Dalane, Aksnes, & Løset, 2015).
While the findings from Dalane (2015) were valuable it is important to note that these are scaled values found in a controlled environment. Of greater significance were the findings by Timco (2002, 2004, 2009), which examined the ice loads on caisson structures in the Beaufort Sea. Timco looked at a total of five caisson structures in the Beaufort Sea during the 1980’s. These five structures are: Tarsiut Caisson, Single-Steel Drilling Caisson (SSDC), Caisson-Retained Island (CRI), Molikpaq, and the Glomar Beaufort Sea I (CIDS). While each of these offshore structures provided varying degrees of information, all give some idea of what type of structures may be present in the Arctic (see Figure 2.7 and Table 2.1).
27 28
Figure 2.7: Offshore Caisson Structure Site Map
Table 2.1: Offshore Caisson Site Information
Structure Site Year(s) Map Number Latitude Longitude Tarsiut Tarsiut N-44 1982-83 1 69.8969 -136.1942 Caisson Unviluk P-66 2 70.2633 -132.3120 1982-84 Kogyuk N-67 3 70.1139 -133.3300 SSDC Phoenix 4 70.7169 -150.428 1986-88 Aurora 5 70.1092 -142.785 Kadluk O-07 1983-84 6 69.7800 -136.0205 CRI Amerk O-09 1984-85 7 69.9822 -133.5142 Kaubvik I-43 1986-87 8 69.8761 -135.4225 Tarsiut P-45 1984-85 9 69.9156 -136.4180 Amauligak I-65 1985-87 10 70.0778 -133.8044 Molikpaq Amauligak F-24 1987-89 11 70.0547 -133.6300 Isserk I-15 1989-90 12 69.9122 -134.2992
The Tarsiut Caisson was the first caisson-type structure used in the Arctic. While it did drill wells during the 1981-82 season, during the winter of 1982-83 it was left to study ice interaction at the Tarsiut N-44 site. The Tarsiut Caisson consisted of four individual concrete caissons each ten meters in length. These caissons formed a square pattern, which created an inner core. They were placed on a subsea berm that came within six meters of the water surface, while the inner core was further filled with dredge material. This formed a structure that was approximately 100 meters across at the water line and had a vertical outer surface (see Figure 2.8) (Timco & Johnston, 2002).
29
Figure 2.8: Tarsiut Caisson Profile (Reproduced from Timco & Johnston, 2002, Figure 9)
While the Tarsiut Caisson did experience a number of ice actions, the information was not complete and several assumptions were often made when calculating the loads. The four best events, as defined by Timco (2004), consisted of FY rubble ice loading. The peak load of these was 240 MN (Timco & Johnston, 2004).
The SSDC was a caisson structure owned and operated by Canmar. The SSDC was a heavily modified super tanker 162 meters long, 53 meters wide, and 25 meters high, with all sides vertical. Like the Tarsiut-Caisson the SSDC also rested on a submerged berm. The SSDC was deployed in the Canadian Beaufort from 1982-84 at the Uviluk P-66 and Kogyuk N-67 sites. From 1986-88 the SSDC was deployed in the American Beaufort at the Phoenix and Aurora Sites. The only sites where reliable ice load measurements were taken was in the American Beaufort (see Figure 2.9) (Timco & Johnston, 2002).
30
Figure 2.9: SSDC Beaufort Sea (Timco & Johnston, 2002, Figure 13, reproduced with permission)
From the information gathered at the American Beaufort sites 13 quality load events were determined. It is important to note that the SSDC was surrounded by a rubble field at these sites. From the data gathered the peak load, 74 MN, was generated from a FY 1.65 meter ice feature at the Phoenix site (Timco & Johnston, 2004).
The CRI was a caisson structure deployed in the Canadian Beaufort from 1983- 87. Throughout its use the CRI was stationed at the Kadluk O-07 site from 1983-84, the Amerk O-09 site from 1984-85, and the Kaubvik I-43 site from 1986-1987. The CRI consisted of eight individual caissons in an octagonal pattern. Each individual caisson was 43 meters long, 12.2 meters high, and 13.1 meters wide. Using two pre-stressed bands of steel wire cable to hold the caissons together a central core was constructed. This central core was 92 meters across and filled with sand. Each face of the octagon was approximately 49.2 meters wide, while each flat was approximately 118 meters across. The outside face of the structure was inclined 30° from vertical (see Figure 2.10) (Timco & Johnston, 2002).
31
Figure 2.10: CRI Beaufort Sea (Timco & Johnston, 2002, Figure 27, reproduced with permission)
While there were a number of ice load measurements made the investigators did not use local pressure values to determine a global load on the CRI (Timco & Johnston, 2004). Using the results of the Implementation section with local pressure values would not be useful for this project.
The Molikpaq structure was deployed in the Canadian Beaufort from 1984-89. Throughout its use the Molikpaq was stationed at the Tarsiut P-45 site from 1984-85, the Amauligak I-65 site from 1985-87, the Amauligak F-24 site from 1987-89, and the Isserk I-15 site from 1989-90. The Molikpaq consisted of an octagonal steel annulus on which sat the structure deck. This steel annulus was filled with sand to provide horizontal resistance. The caisson itself had outside dimensions of 111 meters at its base and 86 meters at its deck, with an overall height of 33.5 meters. When deployed at a set down draft of 20 meters the caisson had a waterline diameter of 90 meters. At this deployment draft the Molikpaq had walls 8° off vertical through the waterline and 23° off vertical
32 from 3.5 meters to 15 meters below mean sea level, with a flare out of about 40° thereafter. This caused the consolidated layer of ridges to interact with a near vertical face, while the keel portion primarily interacted with the 23° face (see Figure 2.11) (Wright & Timco, 2001).
Figure 2.11: Molikpaq Caisson Structure Beaufort Sea (Timco & Johnston, 2004, Figure 4, reproduced with permission)
The Molikpaq structure collected a plethora of quality data during its deployment. Most importantly it was able to capture loading from FY ice ridges. The peak recorded ridge load of 89 MN was caused by a ridge with a one meter sail, drifting at 0.1 meters per second, impacting the 105 meter side. This event, along with the 22 other provided ridge interaction events, gave good numbers to compare calculated values to. Furthermore, loads of up to 140 MN were reported for FY level ice interactions with the Molikpaq (Wright & Timco, 2001).
33 Lastly, the CIDS was a structure operated in the American Beaufort Sea. However, in this literature review ice loading values were not discovered for the structure (Timco & Johnston, 2004). This structure did provide any useful information for this project.
2.12 Changing Ice Conditions
Numerous studies about sea ice features in the project domain were carried out in the 1970s, 1980s, and in the most recent several years. However, there was little activity during the interval between these two eras. As of late, there is a consensus that the annual temperature regime has and is changing (i.e. “climate change”). One must take into account the applicability of previous studies in light of recent climatic changes.
For instance, Wang (2009) theorized that there could be an increased September sea ice reduction over the next 25 years. He also stated that there will be a decrease in sea ice thickness, as MY ice becomes rare and is replaced with FY ice. These changes in ice coverage and ice type can have a large impact on offshore structures and shipping in the Arctic (Wang & Overland, 2009).
Another example of changing ice conditions can be found in Wadhams (2011). In this article Wadhams examined an ice draft dataset from the Fram Strait in 2007 and compared it to a similar dataset from 1976. Wadhams found that a decrease in mean draft of 32% occurred over 31 years in this region. This is a drastic change over such a period of time and clearly shows that the Arctic sea ice conditions are constantly evolving and changing (Wadhams, Hughes, & Rodrigues, 2011).
34 Chapter 3: Data
3.1 Overview
In order to analyze sea ice parameters in a reliability based analysis for offshore structure design, data for a statistical sample of ice parameters needed to be obtained. This data needed to have an acceptably large number of entries to be statistically significant. For this project the draft and velocity of sea ice were of particular interest. Field work was not part of the scope of work for the project. The intent of the project was to collect existing samples of sea ice parameters.
Data from recent studies was acquired for Shell by ASL Environmental Sciences Inc. (ASL) and provided by Shell as a collection of annual datasets for different mooring locations in the Beaufort and Chukchi Seas. Each annual dataset consisted of ice draft and velocity time series measured by moored IPSs and ADCPs, respectively. The raw sensor data was processed following methods described by (Melling, Johnston, & Riedel, 1995) and (Fissel, et al., 2010). The physical collection of the data is examined in greater depth in the Data Collection section.
Altogether the data covered seven seasons and six mooring sites, for a total of 16 yearlong datasets of ice draft and velocity. Table 3.1 shows details for each dataset, while Figure 3.1 provides a map of site locations.
35 Table 3.1: Dataset Details. Days included are when both the IPS and ADCP were simultaneously operational and where length does not include periods of open water.
Season Region Site Days Length (km) Site A 328 1,974 2005-06 Beaufort Site B 330 1,989 Site A 248 1,775 2006-07 Beaufort Site B 223 2,131 Site K 250 1,866 Site A 250 2,198 2007-08 Beaufort Site K 256 2,185 Site V 257 2,340 Site A 284 1,303 Beaufort Site V 284 1,955 2009-10 Burger 201 2,096 Chukchi Crackerjack 204 2,194 Site A 228 1,824 Beaufort Site V 168 1,329 2010-11 Burger 214 3,257 Chukchi Crackerjack 215 2,901
36
Figure 3.1: Site Map
3.2 Data Collection
To collect the draft and velocity data two upward looking sonars were deployed. The first was an ice profiling sonar (IPS). This device measured ice draft data to an estimated accuracy of +/- 0.05 meters every one to two seconds using an acoustic beam (Fukamachi, et al., 2006). While the acoustic beam measured the distance to the sea ice above, a pressure sensor on the device determined the depth of the IPS. The IPS used an algorithm to identify the echo of the acoustic beam and then calculated the draft of the ice based on how quickly the sound travelled back through the seawater. It is important to note that an assumed value is used for the speed sound travels through the water. The IPS then recorded when the measurement was taken and the draft of the measurement (Fissel, et al., 2010; Melling, Johnston, & Riedel, 1995; Melling, Johnston, & Riedel, 1995). The IPS also recorded the tilt of the instrument and the surrounding pressure. These parameters were also incorporated to modify the draft readings to increase accuracy (Melling, Johnston, & Riedel, 1995). 37 Along with the IPS is the ADCP, a complex, microprocessor-controlled echo sounder that is used to determine the motion of sea ice (Melling, Johnston, & Riedel, 1995). The ADCP measured velocity by detecting the Doppler shift in acoustic frequency from the transmitted acoustic pulses of the backscattered pulse returns. The ADCP took measurements every 30 minutes for the full deployment. While this project exclusively used the measurements of the sea ice velocity, it is also possible for the ADCP to record water current (Fissel, et al., 2010).
Both the IPS and ADCP were deployed via ship and moored to the sea floor during the summer open water season. They stayed moored on the sea floor for close to a full 12 months at a time, internally collecting and storing data until retrieval. Once they were retrieved by the ship the next summer season, the data was downloaded. It is important to note ASL then made adjustments to this data before it was sent to the project team, such as accounting for erroneous or extraneous data points and correcting for the drift of the instrument’s internal clock (see Figure 3.2).
38
Figure 3.2: Typical IPS and ADCP Mooring Diagram (Reproduced from Fissel, et al., 2010, Figure 2-2)
For the data provided it was necessary to convert from time dependent data to spatially dependent data. This was done by using both the IPS and ADCP datasets. First, the velocity data was linearly interpolated over the IPS draft data, to assign a velocity value to all draft values. Using these interpolated velocity values the distance and direction that the draft measurements moved was calculated. This made the distance between draft measurements known. Lastly, to develop a pseudo-spatial series where each ice draft measurement would be evenly separated by one meter, a cubic spline 39 interpolation was performed between values (Mahoney A. R., et al., 2015). With this new spatial draft dataset all sites, no matter the season, could be compared (see Figure 3.3 and Figure 3.4).
40
Figure 3.3: Spatial Conversion Algorithm
41 2005-06 Site A Spatial Ice Draft Profile 0 10
Draft (m) 20 0 0 5 10 15 20 25 30 35 40 45 50 55 60 65 ) 10 42
Draft (m 20 0 70 75 80 85 90 95 100 105 110 115 120 125 130 ) 10
Draft (m 20 135 140 145 150 155 160 165 170 175 180 185 190 195 Distance Along Profile (km) Figure 3.4: Spatial Ice Profile
3.3 Pressure Ridge Keel Identification
With datasets spatially defined in terms of draft it was possible to develop an algorithm to identify pressure ridge keel features on the underside of the ice. The algorithm used had been extensively vetted in the scientific community and widely employed (Ekeberg, Høyland, & Hansen, 2014; Fissel, et al., 2010; Melling & Riedel, 1996; Wadhams P. , 1992). However, there was variability of the input parameters throughout the literature so a further investigation of these parameters was undertaken.
The first part of the algorithm was to import the spatially defined draft data, set the starting threshold of a keel, ending threshold of a keel, and a value for the Rayleigh Criterion. The spatially defined draft data was what had been computed from the given preprocessed time series data. The starting threshold defines a minimum draft value that an ice feature must exceed to be considered a keel. The ending threshold defines a draft value where a keel is considered to begin and end. The α parameter is the Rayleigh Criterion, a value that looks at slope reversal in a segment identified as a keel, which indicates the ending of a keel that does not go below the end threshold. Essentially, simply using just the start and end thresholds to identify keels could lead to instances of keel shadowing where two keels close together would be counted as a single unit. The purpose of the α value was to eliminate this by looking for a noticeable reversal of keel slope over a keel segment defined by the starting and ending thresholds (see Figure 3.5).
43
Figure 3.5: Keel Shadowing Illustration (Reproduced from Wadhams & Horne, 1980, Figure 9)
It is important to note that while there are many examples in the literature of these parameters being selected, there is much variability in the starting threshold value. Both the α and ending threshold values seemed to be fairly consistent throughout the literature. An α value of 0.5 and ending threshold value of two meters was selected based on previous work (Ekeberg, Høyland, & Hansen, 2014; Fissel, et al., 2010; Wadhams & Davy, 1986). The selection of the starting threshold value however varied from values as low as two meters to as high as 13 meters (Davis & Wadhams, 1995; Fissel, et al., 2010; Wadhams & Davy, 1986).
The keel identification program first processed through the spatially defined draft data and found keels based on the starting and ending thresholds. Next, the maximum keel depth between these points was identified. Then the keel beginning and end points were redefined by finding the beginning and end of the keel based on the maximum depth point and end threshold. After this, the α value was employed to eliminate keel shadowing by separating any shadowed keels. Lastly, a check was done to correct for any keels that slightly overlapped one another. From this an output file was produced that displayed the maximum keel draft, maximum keel location, keel width, separation of keels based on maximum draft point, keel start location, and keel end location. The
44 output file was written in a comma-separated value (.csv) file. This output file was critical for all future analyses (see Figure 3.6 and Table 3.2).
45
Figure 3.6: Keel Identification Algorithm
46 Table 3.2: Keel Identification Summary; where the starting keel threshold is six meters
Keel Identification Summary
Number of Keels Maximum Keel Season Region Site Identified Draft (m)
Site A 5,391 24.36 2005-06 Beaufort Site B 5,614 25.00 Site A 4,198 25.08 2006-07 Beaufort Site B 3,365 23.00 Site K 3,730 25.69 Site A 3,208 25.46 2007-08 Beaufort Site K 2,459 23.56 Site V 4,043 25.60 Site A 3,505 23.55 Beaufort Site V 5,297 29.38 2009-10 Burger 4,121 26.05 Chukchi Crackerjack 4,680 23.98 Site A 2,492 25.39 Beaufort Site V 2,882 22.73 2010-11 Burger 5,766 24.13 Chukchi Crackerjack 4,993 19.50
Beaufort Sea Sites 46,184 29.38 Chukchi Sea Sites 19,560 26.05
47 3.4 Level Ice Identification
While the methodology for the identification of pressure ridge keels was well established in the scientific community, there were a variety of different methods employed to identify level ice. For this project an algorithm using the standard deviation of the sea ice draft values over a predefined minimum length was used to identify segments of level ice. While other methods were examined, particularly looking at the mode of the draft over a predefined minimum length, the results from the standard deviation method best fit the expected distribution of level ice over the entire ice floe.
First, the spatial draft data was imported into the algorithm. It is important to note that the algorithm was established so that datasets could only be run individually. For example, it would be incorrect to combine all 16 datasets and run them through the algorithm. However, it would be correct to run each dataset individually through the program to obtain results. Along with the draft data, the distance between draft measurements was a necessary input. From the spatial draft datasets it was known that all draft values were one meter apart.
Next, three major parameters were established for the algorithm to identify level ice segments. The first of these parameters was the minimum length of a level ice segments. The second was the maximum standard deviation of ice draft over a length. Lastly, the maximum draft value to be considered in the level ice analysis was necessary. For the purposes of this project the minimum length was set to 50 meters, the maximum standard deviation set to 0.1 meters, and the maximum draft considered was 30 meters.
From the literature there was little guidance on how to select the parameter values for the identification of level ice segments. In order to select parameters that would produce results that made logical sense a series of trials were run using varying parameter values. The set of values chosen were those that produced a sensible overall percentage of level ice cover for the dataset.
48 As the algorithm ran it computed both the mean and standard deviation of the draft in segments of sea ice. Thus the running mean and running standard deviation were established for ice segments. The running standard deviation was then compared to the input maximum standard deviation of 0.1 meters. From this the midpoints of the level ice segments were found and consequently used to identify the complete level ice segment. With the entire segment now defined it was possible to find both the beginning and end points of the level ice segment. As an output the program recorded the beginning and end points of the level ice segment, segment mean, segment mode, and segment standard deviation in a .csv file (see Figure 3.7 and Table 3.3).
49
Figure 3.7: Level Ice Identification Algorithm
50 Table 3.3: Level Ice Identification Summary
Level Ice Identification Summary Level Ice Length Level Ice Percentage Season Region Site (km) of Total Ice Site A 428 21.67% 2005-06 Beaufort Site B 604 30.38% Site A 700 39.42% 2006-07 Beaufort Site B 917 43.03% Site K 764 40.93% Site A 1,045 47.56% 2007-08 Beaufort Site K 1,166 53.38% Site V 1,166 49.82% Site A 470 36.04% Beaufort Site V 725 37.07% 2009-10 Burger 938 44.77% Chukchi Crackerjack 1,052 47.94% Site A 693 37.99% Beaufort Site V 486 36.54% 2010-11 Burger 1,437 44.12% Chukchi Crackerjack 1,477 50.90%
Beaufort Sea Sites 9,162 - Chukchi Sea Sites 4,904 -
It is important to note that the algorithm did not differentiate between FY level ice and MY ice that may have been identified as level through the algorithm. While most FY level ice was identified in the literature as ice with a draft up to two meters (Melling & Riedel, 1995), MY level ice is typically much thicker due to its greater time to develop thermodynamically and also exhibits greater spatial variability in thickness due to summer processes. Thus, it was challenging to differentiate between level MY ice and thick FY rubble without additional in situ observations. It is therefore possible that some of the thicker floes identified as level ice were MY ice floes, but it is not certain.
51 3.5 Other Ice Identification
In comparison to the algorithms to determine pressure ridge keels and level ice, the algorithm to identify other ice was relatively simple. Using the total spatial draft dataset for the entire floe, the dataset for pressure ridge keels, and the dataset for the level ice segments, by process of elimination the “other” ice segments were identified. The range of individual keels and range of level ice segments were combined and used to eliminate the ranges in the total draft dataset. From this the remaining ranges were used to establish the other ice draft segments. The other ice segments could be composed of all manner of different ice features such as rubble fields, rafted ice, and MY ice to name a few (see Figure 3.8 and Table 3.4).
Figure 3.8: Other Ice Identification Algorithm
52 Table 3.4: Other Ice Identification Summary
Other Ice Identification Summary Other Ice Length Other Ice Percentage of Season Region Site (km) Total Ice Site A 1,256 64.39% 2005-06 Beaufort Site B 1,107 56.50% Site A 881 50.46% 2006-07 Beaufort Site B 1,059 50.38% Site K 918 49.91% Site A 942 43.52% 2007-08 Beaufort Site K 864 40.10% Site V 970 42.16% Site A 626 48.87% Beaufort Site V 1,001 52.09% 2009-10 Burger 979 47.48% Chukchi Crackerjack 944 43.80% Site A 1,009 55.99% Beaufort Site V 731 55.83% 2010-11 Burger 1,590 49.55% Chukchi Crackerjack 1,244 43.63%
Beaufort Sea Sites 11,363 - Chukchi Sea Sites 4,756 -
53
54 Chapter 4: Data Analysis
4.1 Overview
With all of the data processed and ice features identified as either pressure ridge keel, level ice segment, or other ice segment, analyses were conducted for each feature. Drawing from the categories presented in the ISO 19906 similar parameters were investigated using several different techniques.
4.2 Probability Density Functions
When using a nondeterministic approach the implementation of PDFs was chosen to describe the uncertainty of the data. The general analysis process consisted of producing a histogram of the data being analyzed and then applying various PDFs to the plot, as well as inspecting associated probability plots. From this, candidate PDFs where chosen and a goodness-of-fit analysis was applied to the data to determine the PDF with the best fit. For this project four primary PDFs were utilized and examined. These were the exponential, gamma, Weibull, and lognormal distribution functions. The exponential, gamma, and Weibull are of a particular family of PDFs and thus are closely related (Matlab©).
55 4.2.1 Gamma Distribution
The gamma probability density function is a two parameter function that models sums of exponentially distributed random variables. The gamma distribution, as characterized by Mathematica, can be described by Eq. 4.2.1.1:
0 (Eq. 4.2.1.1)
where:
α – shape parameter β – scale parameter μ – location parameter
The shape and scale parameters were defined using the data; then histograms, probability plots, and goodness-of-fit tests were used to assess the suitability of the PDF for describing the uncertainty in the data. The determination of these parameters was found from internal commands in either the Matlab© or Mathematica software packages (Wolfram).
56 4.2.2 Exponential Distribution
The exponential probability density function is a single parameter function that is a special case the gamma distribution. The exponential distribution is found by setting the α variable in the gamma distribution equal to one. The exponential distribution is special because of its utility in modeling events that occur randomly over time (Matlab©). The exponential distribution, as characterized by Mathematica, can be described by Eq. 4.2.2.1:
0 (Eq. 4.2.2.1)
where:
λ – any real positive number that helps fit the distribution to the data μ – location parameter
The λ parameter was defined using the data; then histograms, probability plots, and goodness-of-fit tests were used to assess the suitability of the PDF for describing the uncertainty in the data. The determination of this parameter was found from internal commands in either the Matlab© or Mathematica software packages (Wolfram).
57 4.2.3 Weibull Distribution
The Weibull probability density function, in the context of this paper, is a three parameter function which is closely related to both the exponential and gamma distributions. The Weibull distribution, as characterized by Mathematica, can be described by Eq. 4.2.3.1:
0 (Eq. 4.2.3.1)
where:
α – shape parameter β – scale parameter μ – location parameter
The shape and scale parameters were defined using the data; then histograms, probability plots, and goodness-of-fit tests were used to assess the suitability of the PDF for describing the uncertainty in the data. The determination of these parameters was found from internal commands in either the Matlab© or Mathematica software packages (Wolfram).
58 4.2.4 Lognormal Distribution
The lognormal distribution, in the context of this paper, is a two parameter function whose logarithm has a normal distribution. The lognormal distribution, as characterized by Matlab©, can be described by Eq. 4.2.4.1: