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Navigating Troubled Waters a History of Commercial Fishing in Glacier Bay, Alaska
National Park Service U.S. Department of the Interior Glacier Bay National Park and Preserve Navigating Troubled Waters A History of Commercial Fishing in Glacier Bay, Alaska Author: James Mackovjak National Park Service U.S. Department of the Interior Glacier Bay National Park and Preserve “If people want both to preserve the sea and extract the full benefit from it, they must now moderate their demands and structure them. They must put aside ideas of the sea’s immensity and power, and instead take stewardship of the ocean, with all the privileges and responsibilities that implies.” —The Economist, 1998 Navigating Troubled Waters: Part 1: A History of Commercial Fishing in Glacier Bay, Alaska Part 2: Hoonah’s “Million Dollar Fleet” U.S. Department of the Interior National Park Service Glacier Bay National Park and Preserve Gustavus, Alaska Author: James Mackovjak 2010 Front cover: Duke Rothwell’s Dungeness crab vessel Adeline in Bartlett Cove, ca. 1970 (courtesy Charles V. Yanda) Back cover: Detail, Bartlett Cove waters, ca. 1970 (courtesy Charles V. Yanda) Dedication This book is dedicated to Bob Howe, who was superintendent of Glacier Bay National Monument from 1966 until 1975 and a great friend of the author. Bob’s enthusiasm for Glacier Bay and Alaska were an inspiration to all who had the good fortune to know him. Part 1: A History of Commercial Fishing in Glacier Bay, Alaska Table of Contents List of Tables vi Preface vii Foreword ix Author’s Note xi Stylistic Notes and Other Details xii Chapter 1: Early Fishing and Fish Processing in Glacier Bay 1 Physical Setting 1 Native Fishing 1 The Coming of Industrial Fishing: Sockeye Salmon Attract Salters and Cannerymen to Glacier Bay 4 Unnamed Saltery at Bartlett Cove 4 Bartlett Bay Packing Co. -
1 Compiled by Mike Wing New Zealand Antarctic Society (Inc
ANTARCTIC 1 Compiled by Mike Wing US bulldozer, 1: 202, 340, 12: 54, New Zealand Antarctic Society (Inc) ACECRC, see Antarctic Climate & Ecosystems Cooperation Research Centre Volume 1-26: June 2009 Acevedo, Capitan. A.O. 4: 36, Ackerman, Piers, 21: 16, Vessel names are shown viz: “Aconcagua” Ackroyd, Lieut. F: 1: 307, All book reviews are shown under ‘Book Reviews’ Ackroyd-Kelly, J. W., 10: 279, All Universities are shown under ‘Universities’ “Aconcagua”, 1: 261 Aircraft types appear under Aircraft. Acta Palaeontolegica Polonica, 25: 64, Obituaries & Tributes are shown under 'Obituaries', ACZP, see Antarctic Convergence Zone Project see also individual names. Adam, Dieter, 13: 6, 287, Adam, Dr James, 1: 227, 241, 280, Vol 20 page numbers 27-36 are shared by both Adams, Chris, 11: 198, 274, 12: 331, 396, double issues 1&2 and 3&4. Those in double issue Adams, Dieter, 12: 294, 3&4 are marked accordingly. Adams, Ian, 1: 71, 99, 167, 229, 263, 330, 2: 23, Adams, J.B., 26: 22, Adams, Lt. R.D., 2: 127, 159, 208, Adams, Sir Jameson Obituary, 3: 76, A Adams Cape, 1: 248, Adams Glacier, 2: 425, Adams Island, 4: 201, 302, “101 In Sung”, f/v, 21: 36, Adamson, R.G. 3: 474-45, 4: 6, 62, 116, 166, 224, ‘A’ Hut restorations, 12: 175, 220, 25: 16, 277, Aaron, Edwin, 11: 55, Adare, Cape - see Hallett Station Abbiss, Jane, 20: 8, Addison, Vicki, 24: 33, Aboa Station, (Finland) 12: 227, 13: 114, Adelaide Island (Base T), see Bases F.I.D.S. Abbott, Dr N.D. -
The Origin of Ancient Magnetic Activity on Small Planetary Bodies: a Nanopaleomagnetic Study
The Origin of Ancient Magnetic Activity on Small Planetary Bodies: A Nanopaleomagnetic Study James Francis Joseph Bryson Department of Earth Sciences University of Cambridge This dissertation is submitted for the degree of Doctor of Philosophy Selwyn College October 2014 To my family and teachers Declaration I hereby declare that except where specific reference is made to the work of others, the contents of this dissertation are original and have not been submitted in whole or in part for consideration for any other degree or qualification in this, or any other University. This dissertation is the result of my own work and includes nothing which is the outcome of work done in collaboration, except where specifically indicated in the text. This dissertation contains fewer than 225 pages of text, appendices, illustrations, captions and bibliography. James Francis Joseph Bryson October 2014 Acknowledgements First and foremost, I would like to acknowledge my supervisors, Richard Harrison and Simon Redfern. Without Richard’s hard work, dedication, supervision and direction this project would not have been possible, and I feel privileged to have worked with him. Simon should be thanked for his guidance, hours of entertainment and awful jokes. I would like to acknowledge all of my collaborators, in particular Nathan Church, Claire Nichols, Roberts Blukis, Julia Herrero-Albillos, Florian Kronast, Takeshi Kasama and Francis Nimmo. Each has played an invaluable role in acquiring and understanding the data in this thesis and I would not have reached this point without their expertise and help. Martin Walker must be thanked for his assistance and calming influence. I would like to also thank Ioan Lascu for proof-reading this thesis and general advice. -
Evolution of the Lunar Crust Recorded in the Meteoritic
EVOLUTION OF THE LUNAR CRUST RECORDED IN THE METEORITIC FELDSPATHIC REGOLITH BRECCIAS NORTHWEST AFRICA 10291 AND 11182: INSIGHTS INTO THE HETEROGENEITY AND PETROGENESIS OF CRUSTAL LITHOLOGIES USING PETROLOGY AND MINERAL CHEMISTRY By SHANNON BOYLE A thesis submitted to the School of Graduate Studies Rutgers, The State University of New Jersey In partial fulfillment of the requirements For the degree of Master of Science Graduate Program in Earth and Planetary Science Written under the direction of Doctor Juliane Gross And approved by _____________________________________ _____________________________________ _____________________________________ _____________________________________ New Brunswick, New Jersey October 2019 TITLE PAGE ABSTRACT OF THE THESIS Evolution of the lunar crust recorded in the meteoritic feldspathic regolith breccias Northwest Africa 10291 and 11182: Insights into the heterogeneity and petrogenesis of crustal lithologies using petrology and mineral chemistry by SHANNON BOYLE Thesis Director: Doctor Juliane Gross Abstract The geology of the Moon represents nearly a continuous geological record from its formation during the giant impact that resulted in the Earth-Moon system, to its state today. Therefore, it is a prime location for understanding one path of planetary evolution. Lunar meteorites are on average samples of rock and regolith from random areas on the lunar surface. As such, they represent our best available tools to study the crustal evolution of the Moon because they provide data on lunar petrology, geochemistry, and chronology, as well as data on the variety of existing lunar lithologies different from Apollo and Luna mission sample return sites. We investigated two lunar feldspathic regolith breccias found in 2017, Northwest Africa (NWA) 10291 and NWA 11182, to understand their petrogenetic origin and, more broadly, the evolution of lithologies present in unsampled areas of the Moon and place constraints on lunar crustal evolution in these areas. -
University Microfilms, a XEROX Company, Ann Arbor, Michigan
I I 72-4508 GUNNER, John Duncan, 1945- AGE AND ORIGIN OF THE NIMROD GROUP AND OF THE GRANITE HARBOUR INTRUSIVES, BEARDMORE GLACIER REGION, ANTARCTICA. The Ohio State University, Ph.D., 1971 Geology University Microfilms, A XEROX Company, Ann Arbor, Michigan THIS DISSERTATION HAS BEEN MICROFILMED EXACTLY AS RECEIVED AGE AND ORIGIN OP THE NIMROD GROUP AND OF THE GRANITE HARBOUR INTRUSIVES, BEARDMORE GLACIER REGION, ANTARCTICA DISSERTATION Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of The Ohio State University By John Duncan Gunner, 3.A., M.A ****** The Ohio State University 1971 Approved by Adviser Department of Geology PLEASE NOTE: Some Pages have indistinct p rin t. Filmed as received. UNIVERSITY MICROFILMS igure 1: View across the Beardmore Glacier from the Summit of Mount Kyffin. The Rocks in the Foreground are Argillites and Arenites of the 'Goldie Formation, and the Sharp Peak is formed of Hope Granite. The Rounded Mountain on the Left Horizon is The Cloudmaker. ACKNOWLEDGMENTS I am greatly indebted to Dr. Gunter Faure for his enthusiastic ad vice and encouragement throughout this study. I am grateful also to the members of the Institute of Polar Studies expeditions to the Beardmore Glacier region during the 1967-1968 and 1969-1970 field seasons, and especially to David Johnston and to Drs. I. C. Rust and D. H. Elliot for willing assistance and stimulating dis cussions in the field. Logistic field support was provided by Squadron VXE-6 of the U. S. Naval Support Force, Antarctica, without whose help this study would not have been possible. -
Download Version of Record (PDF / 6MB)
Open Research Online The Open University’s repository of research publications and other research outputs An Isotopic Investigation Of Early Planetesimal Differentiation Processes Thesis How to cite: Windmill, Richard Joseph (2021). An Isotopic Investigation Of Early Planetesimal Differentiation Processes. PhD thesis The Open University. For guidance on citations see FAQs. c 2020 Richard Joseph Windmill https://creativecommons.org/licenses/by-nc-nd/4.0/ Version: Version of Record Link(s) to article on publisher’s website: http://dx.doi.org/doi:10.21954/ou.ro.00012472 Copyright and Moral Rights for the articles on this site are retained by the individual authors and/or other copyright owners. For more information on Open Research Online’s data policy on reuse of materials please consult the policies page. oro.open.ac.uk AN ISOTOPIC INVESTIGATION OF EARLY PLANETESIMAL DIFFERENTIATION PROCESSES Richard J. Windmill Supervisors: Dr. I. A. Franchi Professor M. Anand Dr. R. C. Greenwood Submitted to the School of Physical Sciences at The Open University in accordance with the requirements for the degree of Doctor of Philosophy June 2020 School of Physical Sciences Robert Hooke Building The Open University Walton Hall Milton Keynes MK7 6AA United Kingdom Abstract The differentiation and early evolution of planetesimals is relatively poorly understood. The Main- Group pallasites (PMGs) and IIIAB irons are differentiated meteorite groups from deep planetesimal interiors. They provide a window into the early evolution of rocky planets because of the abundance of samples from these groups and because a common planetary provenance has been proposed. Oxygen isotope analyses are crucial in understanding these relationships. -
PSRD: Meteorite Collection in Moscow, Russia
PSRD: Meteorite collection in Moscow, Russia October 31, 2018 Better Know A Meteorite Collection: Fersman Mineralogical Museum in Moscow, Russia Written by Linda M. V. Martel Hawai'i Institute of Geophysics and Planetology PSRD highlights places and people around the world who play central roles in caring for and analyzing meteorites. Join us as we visit the meteorite collection at the Fersman Mineralogical Museum in Moscow and talk with the people who help make history and discoveries come alive. Next to one of Moscow's oldest gardens (the Neskuchny, which aptly translates to "not boring" garden) stands the similarly fascinating Fersman Mineralogical Museum that celebrated its 300th anniversary in 2016. Among the museum's gem and mineral treasures is a collection of meteorites of historical significance, including Pallas' Iron found in 1749 in Siberia, also known as the Krasnojarsk pallasite, pictured above [Data link from the Meteoritical Bulletin]. PSRD had the golden opportunity to visit the Fersman Mineralogical Museum in July 2018, along with other attendees of the 81st Meteoritical Society meeting, in the company of Dr. Mikhail Generalov, Collection Chief Curator, pictured below standing next to a large sample of the Seymchan meteorite [Data link from Meteoritical Bulletin]. In this article we highlight a selection of the extraordinary pieces in this meteorite collection. http://www.psrd.hawaii.edu/Oct18/Meteorites.Moscow.Museum.html PSRD: Meteorite collection in Moscow, Russia Dr. Mikhail Generalov stands next to a large sample of the Seymchan meteorite. http://www.psrd.hawaii.edu/Oct18/Meteorites.Moscow.Museum.html PSRD: Meteorite collection in Moscow, Russia A closer view of the cut, polished, and etched surface of the Seymchan meteorite showing the large schreibersite mineral grains (darker areas) and Widmanstätten pattern in the iron-nickel metal. -
A New Martian Meteorite from Oman: Mineralogy, Petrology, and Shock Metamorphism of Olivine-Phyric Basaltic Shergottite Sayh Al Uhaymir 150
Meteoritics & Planetary Science 40, Nr 8, 1195–1214 (2005) Abstract available online at http://meteoritics.org A new Martian meteorite from Oman: Mineralogy, petrology, and shock metamorphism of olivine-phyric basaltic shergottite Sayh al Uhaymir 150 E. L. WALTON1*, J. G. SPRAY1, and R. BARTOSCHEWITZ2 1Planetary and Space Science Centre, Department of Geology, University of New Brunswick, Bailey Drive, Fredericton, New Brunswick E3B 5A3, Canada 2Meteorite Laboratory, Lehmweg 53, D-38518 Gifhorn, Germany *Corresponding author. E-mail: [email protected] (Received 22 March 2005; revision accepted 17 June 2005) Abstract–The Sayh al Uhaymir (SaU) 150 meteorite was found on a gravel plateau, 43.3 km south of Ghaba, Oman, on October 8, 2002. Oxygen isotope (δ17O 2.78; δ18O 4.74), CRE age (∼1.3 Ma), and noble gas studies confirm its Martian origin. SaU 150 is classified as an olivine-phyric basalt, having a porphyritic texture with olivine macrocrysts set in a finer-grained matrix of pigeonite and interstitial maskelynite, with minor augite, spinel, ilmenite, merrillite, pyrrhotite, pentlandite, and secondary (terrestrial) calcite and iron oxides. The bulk rock composition, in particular mg (68) [molar Mg/(Mg + Fe) × 100], Fe/Mn (37.9), and Na/Al (0.22), are characteristic of Martian meteorites. Based on mineral compositions, cooling rates determined from crystal morphology, and crystal size distribution, it is deduced that the parent magma formed in a steady-state growth regime (magma chamber) that cooled at <2 °C/hr. Subsequent eruption as a thick lava flow or hypabyssal intrusion entrained a small fraction of xenocrystic olivine and gave rise to a magmatic foliation, with slow cooling allowing for near homogenization of igneous minerals. -
Compiled Thesis
SPACE ROCKS: a series of papers on METEORITES AND ASTEROIDS by Nina Louise Hooper A thesis submitted to the Department of Astronomy in partial fulfillment of the requirement for the Bachelor’s Degree with Honors Harvard College 8 April 2016 Of all investments into the future, the conquest of space demands the greatest efforts and the longest-term commitment, but it also offers the greatest reward: none less than a universe. — Daniel Christlein !ii Acknowledgements I finished this senior thesis aided by the profound effort and commitment of my thesis advisor, Martin Elvis. I am extremely grateful for him countless hours of discussions and detailed feedback on all stages of this research. I am also grateful for the remarkable people at Harvard-Smithsonian Center for Astrophysics of whom I asked many questions and who took the time to help me. Special thanks go to Warren Brown for his guidance with spectral reduction processes in IRAF, Francesca DeMeo for her assistance in the spectral classification of our Near Earth Asteroids and Samurdha Jayasinghe and for helping me write my data analysis script in python. I thank Dan Holmqvist for being an incredibly helpful and supportive presence throughout this project. I thank David Charbonneau, Alicia Soderberg and the members of my senior thesis class of astrophysics concentrators for their support, guidance and feedback throughout the past year. This research was funded in part by the Harvard Undergraduate Science Research Program. !iii Abstract The subject of this work is the compositions of asteroids and meteorites. Studies of the composition of small Solar System bodies are fundamental to theories of planet formation. -
Minerals in Meteorites
APPENDIX 1 Minerals in Meteorites Minerals make up the hard parts of our world and the Solar System. They are the building blocks of all rocks and all meteorites. Approximately 4,000 minerals have been identified so far, and of these, ~280 are found in meteorites. In 1802 only three minerals had been identified in meteorites. But beginning in the 1960s when only 40–50 minerals were known in meteorites, the discovery rate greatly increased due to impressive new analytic tools and techniques. In addition, an increasing number of different meteorites with new minerals were being discovered. What is a mineral? The International Mineralogical Association defines a mineral as a chemical element or chemical compound that is normally crystalline and that has been formed as a result of geological process. Earth has an enormously wide range of geologic processes that have allowed nearly all the naturally occurring chemical elements to participate in making minerals. A limited range of processes and some very unearthly processes formed the minerals of meteorites in the earliest history of our solar system. The abundance of chemical elements in the early solar system follows a general pattern: the lighter elements are most abundant, and the heavier elements are least abundant. The miner- als made from these elements follow roughly the same pattern; the most abundant minerals are composed of the lighter elements. Table A.1 shows the 18 most abundant elements in the solar system. It seems amazing that the abundant minerals of meteorites are composed of only eight or so of these elements: oxygen (O), silicon (Si), magnesium (Mg), iron (Fe), aluminum (Al), calcium (Ca), sodium (Na) and potas- sium (K). -
Petrogenesis of Main Group Pallasite Meteorites Based on Relationships
Vrije Universiteit Brussel Petrogenesis of main group pallasite meteorites based on relationships among texture, mineralogy, and geochemistry Mckibbin, Seann; Pittarello, Lidia; Makarona, Christina; Hamman, Christopher; Hecht, Lutz; Chernonozhkin, Stepan; Goderis, Steven; Claeys, Philippe Published in: Meteoritics & Planetary Science DOI: 10.1111/maps.13392 Publication date: 2019 Link to publication Citation for published version (APA): Mckibbin, S., Pittarello, L., Makarona, C., Hamman, C., Hecht, L., Chernonozhkin, S., ... Claeys, P. (2019). Petrogenesis of main group pallasite meteorites based on relationships among texture, mineralogy, and geochemistry. Meteoritics & Planetary Science, 54(11), 2814-2844. https://doi.org/10.1111/maps.13392 General rights Copyright and moral rights for the publications made accessible in the public portal are retained by the authors and/or other copyright owners and it is a condition of accessing publications that users recognise and abide by the legal requirements associated with these rights. • Users may download and print one copy of any publication from the public portal for the purpose of private study or research. • You may not further distribute the material or use it for any profit-making activity or commercial gain • You may freely distribute the URL identifying the publication in the public portal Take down policy If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. Download date: 03. Oct. 2021 Meteoritics & Planetary Science 1–31 (2019) doi: 10.1111/maps.13392 Petrogenesis of main group pallasite meteorites based on relationships among texture, mineralogy, and geochemistry 1,5,6* 1,7 1 Seann J. -
Meteorites of Michigan – Page 1 of 20 Geological Survey ILLUSTRATIONS Bulletin 5 Frontispiece
Sketch of Widmanstatten pattern, see the glossary for more information. Meteorites of Michigan – Page 1 of 20 Geological Survey ILLUSTRATIONS Bulletin 5 Frontispiece. Photograph of September 17, 1966 fireball. ......4 METEORITES OF MICHIGAN Figure 1. Region of observation of December 1965 fireball ....4 Figure 2. Train of December 1965 fireball...............................5 by Figure 3. Train of December 1965 fireball...............................5 VON DEL CHAMBERLAIN Figure 4. Trajectory of December 1965 fireball .......................6 Astronomer Figure 5. Orbit of December 1965 meteorite...........................6 Abrams Planetarium Figure 6. Observations of September 1966 fireball.................6 Michigan State University Figure 7. High velocity projectiles............................................9 Illustrated by James M. Campbell Figure 8. Cross section of stony meteorite............................10 Michigan Department of Conservation Figure 9. Stony-iron meteorite...............................................10 Lansing, 1968 Figure 10. Section of Central Missouri iron meteorite ...........11 Figure 11. Allegan meteorite .................................................14 Figure 12. Grand Rapids meteorite .......................................14 CONTENTS Figure. 13. Iron River meteorite.............................................15 ABSTRACT .....................................................................2 Figure 14. Kalkaska meteorite...............................................15 GLOSSARY.....................................................................2