A Bibliography of Geomorphometry, the Quantitative Representation of Topography Supplement 1.0
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Martian Crater Morphology
ANALYSIS OF THE DEPTH-DIAMETER RELATIONSHIP OF MARTIAN CRATERS A Capstone Experience Thesis Presented by Jared Howenstine Completion Date: May 2006 Approved By: Professor M. Darby Dyar, Astronomy Professor Christopher Condit, Geology Professor Judith Young, Astronomy Abstract Title: Analysis of the Depth-Diameter Relationship of Martian Craters Author: Jared Howenstine, Astronomy Approved By: Judith Young, Astronomy Approved By: M. Darby Dyar, Astronomy Approved By: Christopher Condit, Geology CE Type: Departmental Honors Project Using a gridded version of maritan topography with the computer program Gridview, this project studied the depth-diameter relationship of martian impact craters. The work encompasses 361 profiles of impacts with diameters larger than 15 kilometers and is a continuation of work that was started at the Lunar and Planetary Institute in Houston, Texas under the guidance of Dr. Walter S. Keifer. Using the most ‘pristine,’ or deepest craters in the data a depth-diameter relationship was determined: d = 0.610D 0.327 , where d is the depth of the crater and D is the diameter of the crater, both in kilometers. This relationship can then be used to estimate the theoretical depth of any impact radius, and therefore can be used to estimate the pristine shape of the crater. With a depth-diameter ratio for a particular crater, the measured depth can then be compared to this theoretical value and an estimate of the amount of material within the crater, or fill, can then be calculated. The data includes 140 named impact craters, 3 basins, and 218 other impacts. The named data encompasses all named impact structures of greater than 100 kilometers in diameter. -
GSA ROCKY MOUNTAIN/CORDILLERAN JOINT SECTION MEETING 15–17 May Double Tree by Hilton Hotel and Conference Center, Flagstaff, Arizona, USA
Volume 50, Number 5 GSA ROCKY MOUNTAIN/CORDILLERAN JOINT SECTION MEETING 15–17 May Double Tree by Hilton Hotel and Conference Center, Flagstaff, Arizona, USA www.geosociety.org/rm-mtg Sunset Crater is a cinder cone located north of Flagstaff, Arizona, USA. Program 05-RM-cvr.indd 1 2/27/2018 4:17:06 PM Program Joint Meeting Rocky Mountain Section, 70th Meeting Cordilleran Section, 114th Meeting Flagstaff, Arizona, USA 15–17 May 2018 2018 Meeting Committee General Chair . Paul Umhoefer Rocky Mountain Co-Chair . Dennis Newell Technical Program Co-Chairs . Nancy Riggs, Ryan Crow, David Elliott Field Trip Co-Chairs . Mike Smith, Steven Semken Short Courses, Student Volunteer . Lisa Skinner Exhibits, Sponsorship . Stephen Reynolds GSA Rocky Mountain Section Officers for 2018–2019 Chair . Janet Dewey Vice Chair . Kevin Mahan Past Chair . Amy Ellwein Secretary/Treasurer . Shannon Mahan GSA Cordilleran Section Officers for 2018–2019 Chair . Susan Cashman Vice Chair . Michael Wells Past Chair . Kathleen Surpless Secretary/Treasurer . Calvin Barnes Sponors We thank our sponsors below for their generous support. School of Earth and Space Exploration - Arizona State University College of Engineering, Forestry, and Natural Sciences University of Arizona Geosciences (Arizona LaserChron Laboratory - ALC, Arizona Radiogenic Helium Dating Lab - ARHDL) School of Earth Sciences & Environmental Sustainability - Northern Arizona University Arizona Geological Survey - sponsorship of the banquet Prof . Stephen J Reynolds, author of Exploring Geology, Exploring Earth Science, and Exploring Physical Geography - sponsorship of the banquet NOTICE By registering for this meeting, you have acknowledged that you have read and will comply with the GSA Code of Conduct for Events (full code of conduct listed on page 31) . -
Aquatic Ecomap Team to Develop the Framework, Process Comments, and Develop a Plan Forrevision.These Scientistsare
_i__¸_._. V_!_i Depa_"tment of e_a IC_ .-,4_:..._.A_..:,_,,_gricu 1t u_'e ServiceFo os Framewerku of Aquatim c North Centrai EC@J@g_CaJ U_itS _ N@_th Forest Experiment s [] Station A_er_ca {Nearct_c Z@_e_ General Technical Report NC-17'6 James R. Maxwell, Clayton J. Edwards, Mark E. Jensen, Steven J. Paustian, Harry Parrott, and Donley M. Hitl 8 • _ ...... "'::'":' i:. "S" " : ":','1 _ . / REG I0 NS':_; '"::;:s_:::."_--. .---..:-:!.!:::!:.::_:. ..... •. :.,.:,: .,. -,::.:, .......,.-,.-4S:ifi -.- i::ti/;:.:_: """.::""-:.: .... "':::.:.';.i" . :':" "':":": -. -._ . •....:...{: • . ...:" ZON • .- "." . .. • " . "'...:.:. • .....:....:....:_..-:..:):. -.-. ..... ,:.':::'.':: . .., .... '"_::.--..:.:i i ''_{:;ti}{i_:/.... sub " ,Lri_;gi, • Riverine GroundWater II II _ II I III II I II ],.r ', _ _r',_-- ACFA_OV_rLEDGI_NTS The authors wish to thank the many scientistswho commented on the draftsof thispaper during itspreparation. Their comments dramatically improved the qualiW of the product. These scientistsare listedin Appen- dix F. Specialthanks are offeredto 10 of these scientists,who met with the Aquatic Ecomap team to develop the framework, process comments, and develop a plan forrevision.These scientistsare: Patrick Bourgeron, The Nature Conservancy, Boulder, CO (geoclimatic) James Deacon, Universityof Nevada, Las Vegas, NV (zoogeography) Iris Goodman, Environmental Protection Agency, Las Vegas, NV (ground water) Gordon Grant, Forest Service, Corvallis, OR [riverine) Richard Lillie, Wisconsin Department of Natural Resources, Winona, WI (lacustrine) W.L. Minckley, Arizona State University, Tempe, AZ (zoogeography) Kerry Overton, Forest Service, Boise, [D (riverine) Nick Schmal, Forest Service, Laramie, WY (riverine, lacustrine) Steven Walsh, Fish and Wildlife Service, Gainesville, FL (zoogeography) Mike Wireman, Environmental Protection Agency, Denver, CO (ground water) We wish to especially acknowledge the contributions of Mike Wireman and Iris Goodman of the Environmental Protection Agency. -
22–25 Oct. GSA 2017 Annual Meeting & Exposition
22–25 Oct. GSA 2017 Annual Meeting & Exposition JULY 2017 | VOL. 27, NO. 7 NO. 27, | VOL. 2017 JULY A PUBLICATION OF THE GEOLOGICAL SOCIETY OF AMERICA® JULY 2017 | VOLUME 27, NUMBER 7 SCIENCE 4 Extracting Bulk Rock Properties from Microscale Measurements: Subsampling and Analytical Guidelines M.C. McCanta, M.D. Dyar, and P.A. Dobosh GSA TODAY (ISSN 1052-5173 USPS 0456-530) prints news Cover: Mount Holyoke College astronomy students field-testing a and information for more than 26,000 GSA member readers and subscribing libraries, with 11 monthly issues (March/ Raman BRAVO spectrometer for field mineral identification, examin- April is a combined issue). GSA TODAY is published by The ing pegmatite minerals crosscutting a slightly foliated hornblende Geological Society of America® Inc. (GSA) with offices at quartz monzodiorite and narrow aplite dikes exposed in the spillway 3300 Penrose Place, Boulder, Colorado, USA, and a mail- of the Quabbin Reservoir. All three units are part of the Devonian ing address of P.O. Box 9140, Boulder, CO 80301-9140, USA. GSA provides this and other forums for the presentation Belchertown igneous complex in central Massachusetts, USA. of diverse opinions and positions by scientists worldwide, See related article, p. 4–9. regardless of race, citizenship, gender, sexual orientation, religion, or political viewpoint. Opinions presented in this publication do not reflect official positions of the Society. © 2017 The Geological Society of America Inc. All rights reserved. Copyright not claimed on content prepared GSA 2017 Annual Meeting & Exposition wholly by U.S. government employees within the scope of their employment. Individual scientists are hereby granted 11 Abstracts Deadline permission, without fees or request to GSA, to use a single figure, table, and/or brief paragraph of text in subsequent 12 Education, Careers, and Mentoring work and to make/print unlimited copies of items in GSA TODAY for noncommercial use in classrooms to further 13 Feed Your Brain—Lunchtime Enlightenment education and science. -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
In Pdf Format
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VV D C-A- R 78-03 National Space Science Data Center/ World Data Center a for Rockets and Satellites
VV D C-A- R 78-03 National Space Science Data Center/ World Data Center A For Rockets and Satellites {NASA-TM-79399) LHNAS TRANSI]_INT PHENOMENA N78-301 _7 CATAI_CG (NASA) 109 p HC AO6/MF A01 CSCl 22_ Unc.las G3 5 29842 NSSDC/WDC-A-R&S 78-03 Lunar Transient Phenomena Catalog Winifred Sawtell Cameron July 1978 National Space Science Data Center (NSSDC)/ World Data Center A for Rockets and Satellites (WDC-A-R&S) National Aeronautics and Space Administration Goddard Space Flight Center Greenbelt) Maryland 20771 CONTENTS Page INTRODUCTION ................................................... 1 SOURCES AND REFERENCES ......................................... 7 APPENDIX REFERENCES ............................................ 9 LUNAR TRANSIENT PHENOMENA .. .................................... 21 iii INTRODUCTION This catalog, which has been in preparation for publishing for many years is being offered as a preliminary one. It was intended to be automated and printed out but this form was going to be delayed for a year or more so the catalog part has been typed instead. Lunar transient phenomena have been observed for almost 1 1/2 millenia, both by the naked eye and telescopic aid. The author has been collecting these reports from the literature and personal communications for the past 17 years. It has resulted in a listing of 1468 reports representing only slight searching of the literature and probably only a fraction of the number of anomalies actually seen. The phenomena are unusual instances of temporary changes seen by observers that they reported in journals, books, and other literature. Therefore, although it seems we may be able to suggest possible aberrations as the causes of some or many of the phenomena it is presumptuous of us to think that these observers, long time students of the moon, were not aware of most of them. -
Journal of the Association of Lunar & Planetary Observers
ISSN-0039-2502 Journal of the Association of Lunar & Planetary Observers The Strolling Astronomer Volume 45, Number 1, Winter 2003 Now in Portable Document Format (PDF) for MacIntosh and PC-Compatible Computers Inside...Inside...Inside... More on lunar domes While not the subject of this month’s dome study, we present here a view of lunar dome Mons Gruithuisen Delta (named for Franz von Paul Gruithuisen, a German physician-turned- astronomer) taken from an orbiting Apollo spacecraft. See page 12 for details. • Also . * An ALPO project team to study Saturn’s rings * Isophotes of the Sun * Getting ready for the upcoming Mercury/Venus transits * Getting ready for the Mars apparition * Jupiter and Saturn apparition reports Cover Graphic: John Sanford . plus reports about your ALPO section activities and much, much more. THE ASSOCIATION OF LUNAR AND PLANETARY OBSERVERS (ALPO) P.O. Box 13456, Springfield, Illinois 62791-3456 U.S.A. Thank you for your interest in our organization. The Association of Lunar and Planetary Observers (ALPO) was founded by Walter H. Haas in 1947, and incorporated in 1990, as a medium for advancing and conducting astronomical work by both profes- sional and amateur astronomers who share an interest in Solar System observations. We welcome and provide services for all indi- viduals interested in lunar and planetary astronomy. For the novice observer, the ALPO is a place to learn and to enhance observational techniques. For the advanced amateur astronomer, it is a place where one's work will count. For the professional astronomer, it is a resource where group studies or systematic observing patrols add to the advancement of astronomy. -
Fen-Edebiyat Fakültesi Sosyal Bilimler Dergisi
ISSN: 1302-2423 e-ISSN: 2564-6834 ULUDAĞ ÜNİVERSİTESİ FEN-EDEBİYAT FAKÜLTESİ SOSYAL BİLİMLER DERGİSİ Uludağ University Faculty of Arts and Sciences Journal of Social Sciences YIL / YEAR: 19 CİLT / VOLUME: 18 SAYI / ISSUE: 32 2017/1 ISSN: 1302-2423 e-ISSN: 2564-6834 ULUDAĞ ÜNİVERSİTESİ FEN-EDEBİYAT FAKÜLTESİ SOSYAL BİLİMLER DERGİSİ Uludağ University Faculty of Arts and Sciences Journal of Social Sciences YIL / YEAR: 19 CİLT / VOLUME: 18 SAYI / ISSUE: 32 2017/1 DERGİ HAKKINDA Uludağ Üniversitesi Fen-Edebiyat Fakültesi Sosyal Bilimler Dergisi (UÜFEFSBD); sosyal, beşeri ve idari bilimler temel alanı başta olmak üzere filoloji, eğitim bilimleri ve öğretmen yetiştirme, güzel sanatlar, hukuk ve ilahiyat temel alanlarında yazılmış özgün araştırma makaleleri yayımlamaktadır. Uluslararası hakemli bilimsel bir dergi olup yayın hayatına 1999 yılında başlamıştır. Ocak ve Temmuz aylarında olmak üzere yılda iki kez yayımlanan dergi; EBSCO, MLA (Modern Language Association) International Bibliography, Google Akademik, ULAKBİM TR DİZİN ve Sosyal Bilimler Atıf Dizini (SOBİAD) tarafından taranmaktadır. Derginin Uludağ Üniversitesi Fen-Edebiyat Fakültesi adına sahibi, Fakülte dekanıdır. Derginin yayın kurulu; editör, editör yardımcıları ve Uludağ Üniversitesi Fen-Edebiyat Fakültesinin ilgili sosyal bölümlerinin (Arkeoloji, Coğrafya, Felsefe, Psikoloji, Sanat Tarihi, Sosyoloji, Tarih, Türk Dili ve Edebiyatı) başkanlarından oluşmaktadır. Ocak 2017’den itibaren derginin tüm makale gönderme ve değerlendirme işlemleri çevrimiçi olarak DergiPark Sistemi üzerinden -
Comparison of Different Crater Counting Methods Applicated to Parana Valles
40th Lunar and Planetary Science Conference (2009) 1097.pdf COMPARISON OF DIFFERENT CRATER COUNTING METHODS APPLICATED TO PARANA VALLES. S.Bouley 1,2,3 , R.A. Craddock 2, N.Mangold 3 and V. Ansan 3. 1Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution, Washington D.C. 20560-0315, 2IDES UMR8148, Bat. 509, Université Paris XI, 91405 Orsay Cedex, France ([email protected]), 3LPGNantes UMR6112 CNRS 44322 Université Nantes, France. Introduction: Martian valley networks are good rectangular with a width of ~2 km. We observed that indicators of the past climate. These features are this valley is partially filled by eolian deposits. At an located primarily in heavily cratered terrain of elevation of ~200 m, the main valley in the southern Noachian age (>3.7 Ga) [1] but the exact timing of branch, becomes wider (between 3 and 8 km), exhibits these features is not well understood. Recent global a wide V-shape profile and incises interfluves. We studies using superposed craters along different fluvial suggest that the differences in morphology are the valleys [2, 3] determined that most formed during the result of variation of lithology. Late Noachian to Early Hesperian. However, valley networks are small, linear features that make them difficult to accurately date using traditional crater- counting techniques. In this study, we set out to test the reliability of the counting methods used in [2] and [3] while comparing the results to other methods using fine scale age determination from small diameter craters. We applied these different methods to Parana Valles using a large dataset of high-resolution images from different instruments that allow us to count smaller craters while providing a good sampling of crater populations that is necessary to reduce uncertainties in age determination. -
Geodesy and Geophysics in Canada 1991 Ñ 1995
Geodesy and Geophysics in Canada 1991 Ñ 1995 Quadrennial Report of the Canadian National Committee for the International Union of Geodesy and Geophysics prepared on the occasion of the XXI General Assembly of the IUGG Boulder, Colorado, U.S.A. July 1995 Geodesy and Geophysics in Canada, 1991 Ñ 1995 2 Canadian National Committee for IUGG Chairman: Prof. R. Langley Department of Geodesy and Geomatics Engineering University of New Brunswick P.O. Box 4400 Fredericton, New Brunswick E3B 5A3 Tel: (506) 453-5142 FAX: (506) 453-4943 E-mail: [email protected] Secretary: D.R. McDiarmid Herzberg Institute of Astrophysics National Research Council of Canada Ottawa, Ontario Canada K1A 0R6 Tel: (613) 990-0713 FAX: (613) 952-0974 E-mail: (SPAN) CANOTT::MCDIARMID (Internet) [email protected] IAG: Dr. R. Langley (see above) Prof. M.G. Sideris Dept. of Geomatics Engineering The University of Calgary 2500 University Drive N.W. Calgary, Alberta T2N 1N4 Tel: (403) 220-4985 FAX: (403) 284-1980 E-mail: [email protected] IAGA: Dr. Alan G. Jones Prof. R.E. Horita Geological Survey of Canada Dept. of Physics and Astronomy 1 Observatory Crescent University of Victoria Ottawa, Ontario Victoria, British Columbia K1A 0Y3 V8W 2Y2 Tel: (613) 992-4968 Tel: (604) 721-7731 FAX: (613) 992-8836 FAX: (604) 721-7715 E-mail: [email protected] E-mail: CANOTT::HORITA [email protected] IAMAP: Prof. I. Zawadski Prof. P. A. Taylor Dept. of Atmos. & Oceanic Sciences Dept of Earth & Atmospheric McGill University Sciences 805 Sherbrooke W. York University MontrŽal, QuŽbec 4700 Keele Street H3A 2K6 North York, Ontario Tel: (514) 398-1034 M3J 1P3 FAX: (514) 398-6115 Tel: (416) 736-5245 E-mail: [email protected] FAX: (416) 736-5817 E-mail: [email protected] Geodesy and Geophysics in Canada, 1991 Ñ 1995 3 IAPSO: Dr. -
Annual Report Donors
Sam Houston State University VOLUME 7 • NUMBER 1 • 2013-2014 Annual Reportto Donors Charlie Amato and Gary Dudley A Message from the President early every day, I am reminded of the overwhelming generosity of Sam Houston State NUniversity’s donors. I have heard countless, heartfelt stories from our students who have attributed their ability to attend college and achieve success solely on the scholarships provided by our alumni and friends. I have witnessed the awestruck looks of thousands of visitors as they walk through our beautiful campus with its new and renovated facilities that were built, in part, through donor support. I have had the privilege to speak publicly about the accomplishments of the university and the quality of our academic programs, which would not have been possible without philanthropy. Each of you, who are listed within the pages of this 2013-2014 Annual Report to Donors, has made a meaningful difference for Sam Houston State and its nearly 20,000 students. Your support positively impacts enrollment growth, the quality of academic programs, the strength of athletic teams, and so many other things that enhance the university’s national stature. Simply put, you have invested in changing the lives of tomorrow’s leaders, which will have a profound impact on the future of our region, state, and nation for generations to come. Over the past 300 years, higher education has been the primary source for all significant innovation and change, fueling momentous leaps in scientific and societal advancements. Knowing that Sam Houston has an extraordinary cadre of loyal and dependable support, I am confident this grand old university will continue to honor and uphold longstanding traditions and values, while embracing change and nurturing intellectual inquiry in order to meet the challenges and opportunities of the 21st centur y.