An Object-Based Approach for Mapping Tundra Ice-Wedge Polygon Troughs from Very High Spatial Resolution Optical Satellite Imagery
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Chapter 7 Seasonal Snow Cover, Ice and Permafrost
I Chapter 7 Seasonal snow cover, ice and permafrost Co-Chairmen: R.B. Street, Canada P.I. Melnikov, USSR Expert contributors: D. Riseborough (Canada); O. Anisimov (USSR); Cheng Guodong (China); V.J. Lunardini (USA); M. Gavrilova (USSR); E.A. Köster (The Netherlands); R.M. Koerner (Canada); M.F. Meier (USA); M. Smith (Canada); H. Baker (Canada); N.A. Grave (USSR); CM. Clapperton (UK); M. Brugman (Canada); S.M. Hodge (USA); L. Menchaca (Mexico); A.S. Judge (Canada); P.G. Quilty (Australia); R.Hansson (Norway); J.A. Heginbottom (Canada); H. Keys (New Zealand); D.A. Etkin (Canada); F.E. Nelson (USA); D.M. Barnett (Canada); B. Fitzharris (New Zealand); I.M. Whillans (USA); A.A. Velichko (USSR); R. Haugen (USA); F. Sayles (USA); Contents 1 Introduction 7-1 2 Environmental impacts 7-2 2.1 Seasonal snow cover 7-2 2.2 Ice sheets and glaciers 7-4 2.3 Permafrost 7-7 2.3.1 Nature, extent and stability of permafrost 7-7 2.3.2 Responses of permafrost to climatic changes 7-10 2.3.2.1 Changes in permafrost distribution 7-12 2.3.2.2 Implications of permafrost degradation 7-14 2.3.3 Gas hydrates and methane 7-15 2.4 Seasonally frozen ground 7-16 3 Socioeconomic consequences 7-16 3.1 Seasonal snow cover 7-16 3.2 Glaciers and ice sheets 7-17 3.3 Permafrost 7-18 3.4 Seasonally frozen ground 7-22 4 Future deliberations 7-22 Tables Table 7.1 Relative extent of terrestrial areas of seasonal snow cover, ice and permafrost (after Washburn, 1980a and Rott, 1983) 7-2 Table 7.2 Characteristics of the Greenland and Antarctic ice sheets (based on Oerlemans and van der Veen, 1984) 7-5 Table 7.3 Effect of terrestrial ice sheets on sea-level, adapted from Workshop on Glaciers, Ice Sheets and Sea Level: Effect of a COylnduced Climatic Change. -
The Periglacial Landscape of Utopia Planitia; Geologic Evidence for Recent Climate Change on Mars
Western University Scholarship@Western Electronic Thesis and Dissertation Repository 1-23-2013 12:00 AM The Periglacial Landscape Of Utopia Planitia; Geologic Evidence For Recent Climate Change On Mars. Mary C. Kerrigan The University of Western Ontario Supervisor Dr. Marco Van De Wiel The University of Western Ontario Joint Supervisor Dr. Gordon R Osinski The University of Western Ontario Graduate Program in Geography A thesis submitted in partial fulfillment of the equirr ements for the degree in Master of Science © Mary C. Kerrigan 2013 Follow this and additional works at: https://ir.lib.uwo.ca/etd Part of the Climate Commons, Geology Commons, Geomorphology Commons, and the Physical and Environmental Geography Commons Recommended Citation Kerrigan, Mary C., "The Periglacial Landscape Of Utopia Planitia; Geologic Evidence For Recent Climate Change On Mars." (2013). Electronic Thesis and Dissertation Repository. 1101. https://ir.lib.uwo.ca/etd/1101 This Dissertation/Thesis is brought to you for free and open access by Scholarship@Western. It has been accepted for inclusion in Electronic Thesis and Dissertation Repository by an authorized administrator of Scholarship@Western. For more information, please contact [email protected]. THE PERIGLACIAL LANDSCAPE OF UTOPIA PLANITIA; GEOLOGIC EVIDENCE FOR RECENT CLIMATE CHANGE ON MARS by Mary C. Kerrigan Graduate Program in Geography A thesis submitted in partial fulfillment of the requirements for the degree of Master of Science The School of Graduate and Postdoctoral Studies The University of Western Ontario London, Ontario, Canada © Mary C. Kerrigan 2013 ii THE UNIVERSITY OF WESTERN ONTARIO School of Graduate and Postdoctoral Studies CERTIFICATE OF EXAMINATION Joint Supervisor Examiners ______________________________ Dr. -
180 in Siberian Syngenetic Ice-Wedge Complexes
14C AND 180 IN SIBERIAN SYNGENETIC ICE-WEDGE COMPLEXES YURIJ K. VASIL'CHUK Department of Cryolithology and Glaciology and Laboratory of Regional Engineering Geology, Moscow State University, Vorob'yovy Gory, 119899 Moscow, Russia and The Theoretical Problems Department, Russian Academy of Sciences, Denezhnyi pereulok, 12, 121002 Moscow, Russia and ALLA C. VASIL'CHUK Institute of Cell Biophysics, The Russian Academy of Sciences, 142292, Pushchino Moscow Region, Russia ABSTRACT. We discuss the possibility of dating ice wedges by the radiocarbon method. We show as an example the Seyaha, Kular and Zelyony Mys ice wedge complexes, and investigated various organic materials from permafrost sediments. We show that the reliability of dating 180 variations from ice wedges can be evaluated by comparison of different organic mate- rials from host sediments in the ice wedge cross sections. INTRODUCTION Permafrost covers 60% of the Russian territory and a large part of North America. During the glacial period, almost all of Europe was also covered by permafrost, with temperatures close to the present ones in the north of western Siberia and Yakutia (Vasil'chuk and Vasil'chuk 1995a). That permafrost melted not more than 10,000 yr ago. This enables radiocarbon dating of paleopermafrost sediments from Europe and North America. Hydrogen and oxygen stable isotopes in syngenetic ice wedges of northern Eurasia and North America permafrost zones yield paleoclimatic parameters, such as paleotemperature. The oxygen isotope composition of a recently formed syngenetic ice wedge together with present winter temper- atures of surface air (Vasil'chuk 1991) made it possible to use stable isotope variations in ancient syngenetic ice wedges as a quantitative paleotemperature indicator (to make sure that the same dependence took place in the past). -
Periglacial Processes, Features & Landscape Development 3.1.4.3/4
Periglacial processes, features & landscape development 3.1.4.3/4 Glacial Systems and landscapes What you need to know Where periglacial landscapes are found and what their key characteristics are The range of processes operating in a periglacial landscape How a range of periglacial landforms develop and what their characteristics are The relationship between process, time, landforms and landscapes in periglacial settings Introduction A periglacial environment used to refer to places which were near to or at the edge of ice sheets and glaciers. However, this has now been changed and refers to areas with permafrost that also experience a seasonal change in temperature, occasionally rising above 0 degrees Celsius. But they are characterised by permanently low temperatures. Location of periglacial areas Due to periglacial environments now referring to places with permafrost as well as edges of glaciers, this can account for one third of the Earth’s surface. Far northern and southern hemisphere regions are classed as containing periglacial areas, particularly in the countries of Canada, USA (Alaska) and Russia. Permafrost is where the soil, rock and moisture content below the surface remains permanently frozen throughout the entire year. It can be subdivided into the following: • Continuous (unbroken stretches of permafrost) • extensive discontinuous (predominantly permafrost with localised melts) • sporadic discontinuous (largely thawed ground with permafrost zones) • isolated (discrete pockets of permafrost) • subsea (permafrost occupying sea bed) Whilst permafrost is not needed in the development of all periglacial landforms, most periglacial regions have permafrost beneath them and it can influence the processes that create the landforms. Many locations within SAMPLEextensive discontinuous and sporadic discontinuous permafrost will thaw in the summer months. -
Growth and Form of the Mound in Gale Crater, Mars: Slope
1 Growth and form of the mound in Gale Crater, Mars: Slope- 2 wind enhanced erosion and transport 3 Edwin S. Kite1, Kevin W. Lewis,2 Michael P. Lamb1 4 1Geological & Planetary Science, California Institute of Technology, MC 150-21, Pasadena CA 5 91125, USA. 2Department of Geosciences, Princeton University, Guyot Hall, Princeton NJ 6 08544, USA. 7 8 Abstract: Ancient sediments provide archives of climate and habitability on Mars (1,2). Gale 9 Crater, the landing site for the Mars Science Laboratory (MSL), hosts a 5 km high sedimentary 10 mound (3-5). Hypotheses for mound formation include evaporitic, lacustrine, fluviodeltaic, and 11 aeolian processes (1-8), but the origin and original extent of Gale’s mound is unknown. Here we 12 show new measurements of sedimentary strata within the mound that indicate ~3° outward dips 13 oriented radially away from the mound center, inconsistent with the first three hypotheses. 14 Moreover, although mounds are widely considered to be erosional remnants of a once crater- 15 filling unit (2,8-9), we find that the Gale mound’s current form is close to its maximal extent. 16 Instead we propose that the mound’s structure, stratigraphy, and current shape can be explained 17 by growth in place near the center of the crater mediated by wind-topography feedbacks. Our 18 model shows how sediment can initially accrete near the crater center far from crater-wall 19 katabatic winds, until the increasing relief of the resulting mound generates mound-flank slope- 20 winds strong enough to erode the mound. Our results indicate mound formation by airfall- 21 dominated deposition with a limited role for lacustrine and fluvial activity, and potentially 22 limited organic carbon preservation. -
A Review of Sample Analysis at Mars-Evolved Gas Analysis Laboratory Analog Work Supporting the Presence of Perchlorates and Chlorates in Gale Crater, Mars
minerals Review A Review of Sample Analysis at Mars-Evolved Gas Analysis Laboratory Analog Work Supporting the Presence of Perchlorates and Chlorates in Gale Crater, Mars Joanna Clark 1,* , Brad Sutter 2, P. Douglas Archer Jr. 2, Douglas Ming 3, Elizabeth Rampe 3, Amy McAdam 4, Rafael Navarro-González 5,† , Jennifer Eigenbrode 4 , Daniel Glavin 4 , Maria-Paz Zorzano 6,7 , Javier Martin-Torres 7,8, Richard Morris 3, Valerie Tu 2, S. J. Ralston 2 and Paul Mahaffy 4 1 GeoControls Systems Inc—Jacobs JETS Contract at NASA Johnson Space Center, Houston, TX 77058, USA 2 Jacobs JETS Contract at NASA Johnson Space Center, Houston, TX 77058, USA; [email protected] (B.S.); [email protected] (P.D.A.J.); [email protected] (V.T.); [email protected] (S.J.R.) 3 NASA Johnson Space Center, Houston, TX 77058, USA; [email protected] (D.M.); [email protected] (E.R.); [email protected] (R.M.) 4 NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA; [email protected] (A.M.); [email protected] (J.E.); [email protected] (D.G.); [email protected] (P.M.) 5 Institito de Ciencias Nucleares, Universidad Nacional Autonoma de Mexico, Mexico City 04510, Mexico; [email protected] 6 Centro de Astrobiología (INTA-CSIC), Torrejon de Ardoz, 28850 Madrid, Spain; [email protected] 7 Department of Planetary Sciences, School of Geosciences, University of Aberdeen, Aberdeen AB24 3FX, UK; [email protected] 8 Instituto Andaluz de Ciencias de la Tierra (CSIC-UGR), Armilla, 18100 Granada, Spain Citation: Clark, J.; Sutter, B.; Archer, * Correspondence: [email protected] P.D., Jr.; Ming, D.; Rampe, E.; † Deceased 28 January 2021. -
Rapid Machine Learning-Based Extraction and Measurement of Ice Wedge Polygons in Airborne Lidar Data Charles J
The Cryosphere Discuss., https://doi.org/10.5194/tc-2018-167 Manuscript under review for journal The Cryosphere Discussion started: 11 September 2018 c Author(s) 2018. CC BY 4.0 License. Brief communication: Rapid machine learning-based extraction and measurement of ice wedge polygons in airborne lidar data Charles J. Abolt1,2, Michael H. Young2, Adam A. Atchley3, Cathy J. Wilson3 1Department of Geological Sciences, The University of Texas at Austin, Austin, TX, USA 5 2Bureau of Economic Geology, The University of Texas at Austin, Austin, TX USA 3Earth and Environmental Sciences Division, Los Alamos National Laboratory, Los Alamos, NM, USA Correspondence to: Charles J. Abolt ([email protected]) Abstract. We present a workflow for rapid delineation and microtopographic characterization of ice wedge polygons within 10 high-resolution digital elevation models. The workflow, which is extensible to other forms of remotely sensed imagery, incorporates a convolutional neural network to detect pixels representing troughs. A watershed transformation is then used to segment imagery into discrete polygons. Regions of non-polygonal terrain are partitioned out using a simple post-processing procedure. Results from training and validation sites at Barrow and Prudhoe Bay, Alaska demonstrate robust performance in diverse tundra landscapes. The methodology permits fast, spatially extensive measurements of polygonal microtopography 15 and trough network geometry. 1 Introduction and Background The objective of this research is to develop and report on a workflow for rapid delineation and microtopographic analysis of ice wedge polygons in airborne lidar data. Ice wedge polygons are the surface expression of ice wedges, a form of ground ice nearly ubiquitous to coastal tundra environments in North America and Eurasia (Leffingwell, 1915; Lachenbruch, 20 1962). -
EVIDENCE from UTOPIA PLANITIA. GE Mcgill, Department Of
Lunar and Planetary Science XXXI 1194.pdf AGE OF THE MARS GLOBAL NORTHERLY SLOPE: EVIDENCE FROM UTOPIA PLANITIA. G. E. McGill, Department of Geosciences, University of Massachusetts, Amherst, MA 01003 ([email protected]). Recent results from the Mars Orbiter about 100, which is Late Hesperian, and Laser Altimeter (MOLA) experiment on thus the tilt must be Late Hesperian or older, Mars Global Surveyor (MGS) indicate that in good agreement with results obtained in most of Mars is characterized by a very Arabia Terra gentle, roughly northerly slope (1,2). The untilted areas of smooth plains Detailed mapping in north-central Arabia occur as a 90-150 km wide bench along the Terra (3) combined with superposition northern margin of the Utopia Planitia relations and crater counts indicate that, in polygonal terrane, north of which the that region at least, this northerly slope must lowland floor resumes its northerly tilt have been formed no later than Late within rough, hummocky terrane. At least Hesperian, with the most likely time of one additional bench may be present within formation being Late Hesperian. Current this hummocky terrane. The bench research in Utopia Planitia intended as a test underlain by smooth plains materials of extant models for the formation of giant maintains a remarkably constant elevation of polygons (4,5) has turned up good evidence about -4700 m, with deviations of less than for a Late Hesperian age for the northerly tilt 100 m over distances of hundreds of km in this region as well, as will be discussed along the northern edge of the polygonal here. -
Durham Research Online
Durham Research Online Deposited in DRO: 27 March 2019 Version of attached le: Published Version Peer-review status of attached le: Peer-reviewed Citation for published item: Orgel, Csilla and Hauber, Ernst and Gasselt, Stephan and Reiss, Dennis and Johnsson, Andreas and Ramsdale, Jason D. and Smith, Isaac and Swirad, Zuzanna M. and S¡ejourn¡e,Antoine and Wilson, Jack T. and Balme, Matthew R. and Conway, Susan J. and Costard, Francois and Eke, Vince R. and Gallagher, Colman and Kereszturi, Akos¡ and L osiak, Anna and Massey, Richard J. and Platz, Thomas and Skinner, James A. and Teodoro, Luis F. A. (2019) 'Grid mapping the Northern Plains of Mars : a new overview of recent water and icerelated landforms in Acidalia Planitia.', Journal of geophysical research : planets., 124 (2). pp. 454-482. Further information on publisher's website: https://doi.org/10.1029/2018JE005664 Publisher's copyright statement: Orgel, Csilla, Hauber, Ernst, Gasselt, Stephan, Reiss, Dennis, Johnsson, Andreas, Ramsdale, Jason D., Smith, Isaac, Swirad, Zuzanna M., S¡ejourn¡e,Antoine, Wilson, Jack T., Balme, Matthew R., Conway, Susan J., Costard, Francois, Eke, Vince R., Gallagher, Colman, Kereszturi, Akos,¡ L osiak, Anna, Massey, Richard J., Platz, Thomas, Skinner, James A. Teodoro, Luis F. A. (2019). Grid Mapping the Northern Plains of Mars: A New Overview of Recent Water and IceRelated Landforms in Acidalia Planitia. Journal of Geophysical Research: Planets 124(2): 454-482. 10.1029/2018JE005664. To view the published open abstract, go to https://doi.org/ and enter the DOI. Additional information: Use policy The full-text may be used and/or reproduced, and given to third parties in any format or medium, without prior permission or charge, for personal research or study, educational, or not-for-prot purposes provided that: • a full bibliographic reference is made to the original source • a link is made to the metadata record in DRO • the full-text is not changed in any way The full-text must not be sold in any format or medium without the formal permission of the copyright holders. -
773593683.Pdf
LAKE AREA CHANGE IN ALASKAN NATIONAL WILDLIFE REFUGES: MAGNITUDE, MECHANISMS, AND HETEROGENEITY A DISSERTATION Presented to the Faculty of the University of Alaska Fairbanks In Partial Fulfillment of the Requirements for the Degree of DOCTOR OF PHILOSOPHY By Jennifer Roach, B.S. Fairbanks, Alaska December 2011 iii Abstract The objective of this dissertation was to estimate the magnitude and mechanisms of lake area change in Alaskan National Wildlife Refuges. An efficient and objective approach to classifying lake area from Landsat imagery was developed, tested, and used to estimate lake area trends at multiple spatial and temporal scales for ~23,000 lakes in ten study areas. Seven study areas had long-term declines in lake area and five study areas had recent declines. The mean rate of change across study areas was -1.07% per year for the long-term records and -0.80% per year for the recent records. The presence of net declines in lake area suggests that, while there was substantial among-lake heterogeneity in trends at scales of 3-22 km a dynamic equilibrium in lake area may not be present. Net declines in lake area are consistent with increases in length of the unfrozen season, evapotranspiration, and vegetation expansion. A field comparison of paired decreasing and non-decreasing lakes identified terrestrialization (i.e., expansion of floating mats into open water with a potential trajectory towards peatland development) as the mechanism for lake area reduction in shallow lakes and thermokarst as the mechanism for non-decreasing lake area in deeper lakes. Consistent with this, study areas with non-decreasing trends tended to be associated with fine-grained soils that tend to be more susceptible to thermokarst due to their higher ice content and a larger percentage of lakes in zones with thermokarst features compared to study areas with decreasing trends. -
Organic Carbon Characteristics in Ice-Rich Permafrost in Alas and Yedoma Deposits, Central Yakutia, Siberia” by Torben Windirsch Et Al
Biogeosciences Discuss., https://doi.org/10.5194/bg-2019-470-RC1, 2020 © Author(s) 2020. This work is distributed under the Creative Commons Attribution 4.0 License. Interactive comment on “Organic Carbon Characteristics in Ice-rich Permafrost in Alas and Yedoma Deposits, Central Yakutia, Siberia” by Torben Windirsch et al. Anonymous Referee #1 Received and published: 27 January 2020 The paper “Organic Carbon Characteristics in Ice-rich Permafrost in Alas and Yedoma Deposits, Central Yakutia, Siberia” by Windirsch et al. reports detailed analyses on carbon and ice contents, stable water isotopes, soil grain size distribution, and age estimates for two long ground profiles in the Central Yakutia, Russia. The presented materials are rare and highly valuable to understand landscape development and con- tents in the permafrost of the Eastern Siberia. Although I expect this paper to be finally published in Biogeosciece, the authors have not fully utilized, described, and discussed the data presented. The importance of this paper is the rareness of the sample core. I encourage the authors to enrich their descriptions about each core unit as a valuable drilling log of a permafrost region. Some portions in Discussion are C1 not logically constructed. For the main datasets of stable water isotopes and carbon parameters, a more in-depth and quantitative discussion is anticipated. Although the authors want to focus on the organic carbon characteristics as indicated in the title, more comprehensive discussion and interpretation must be done using available water geochemistry, cryostratigraphy, grain size distribution, magnetic susceptibility, etc. The usage of references or previous studies is poor and is often not clear or inappropriate. -
Is There Life on Mars?
Life On Mars? Viking Lander Biology Missions and Experiments Kelly Anderson, Sereane Bowstring, Susan Kolibaba, Sara Marvin Rhiannon Rasmussen-Silverstein Is there life on Mars? Are we alone out here? • Humans are instinctively curious about who else is “out there.” • Biology experiments were developed and sent to Mars to try to answer this key question. http://img.dailymail.co.uk/i/pix/2008/01_04/LifeOnMarsBARC_800x496.jpg Oparin-Haldane Hypothesis Scientists Alexander Oparin and John Haldane formed a Hypothesis on the •These first organic compounds Origin of Life on Earth. formed in the atmosphere. They were then transported via •The basic premise was that the Earth’s rain into the rivers, lakes and original atmosphere went through oceans of the world where they synthesis, powered by various energy proceeded to accumulate. sources and became a “prebiotic soup” from which all life forms evolved. Due to the high concentration of molecules, collisions occurred which powered further spontaneous reactions causing molecular or chemical evolution. (Transforming the simple molecules into complex ones.) http://upload.vipulg.com/Biology/600/Part%20II/Chapter%203_files/Chapter%203-5.png 3 Urey-Miller Experiment Experiment designed to test the Oparin-Haldane Hypothesis. •Findings embraced the Hypothesis. Began with Hydrogen, Water, Ammonia and Methane. •End result: organic molecules http://upload.vipulg.com/Zoology/759/Chapter2_files/Chapter2-8.png 4 Atmosphere around the time of Earth’s formation consisted of: •Hydrogen •Water Vapor •Ammonia •Methane Spontaneous reactions occurred, resulting in abiotic synthesis. •Carbon •Hydrogen •Oxygen •Nitrogen •Atoms recombined to form http://karlrichard.files.wordpress.com/2009/07/i11-02-atmocompo.jpg?w=460&h=300 the first organic compounds 5 Mars & Earth Similarities • Planet Rotation on axis: Mars=24.6 hrs Earth=24 hrs • Revolution around sun: Mars=1.88 yrs Earth=1 yr • Tilt of axis: Mars=25.19 o Earth=23.45o • Earth-Water vapor Mars-Ice water • Moons.