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Planetary Geologic Mappers Annual Meeting
Program Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 Planetary Geologic Mappers Annual Meeting June 12–14, 2018 • Knoxville, Tennessee Institutional Support Lunar and Planetary Institute Universities Space Research Association Convener Devon Burr Earth and Planetary Sciences Department, University of Tennessee Knoxville Science Organizing Committee David Williams, Chair Arizona State University Devon Burr Earth and Planetary Sciences Department, University of Tennessee Knoxville Robert Jacobsen Earth and Planetary Sciences Department, University of Tennessee Knoxville Bradley Thomson Earth and Planetary Sciences Department, University of Tennessee Knoxville Abstracts for this meeting are available via the meeting website at https://www.hou.usra.edu/meetings/pgm2018/ Abstracts can be cited as Author A. B. and Author C. D. (2018) Title of abstract. In Planetary Geologic Mappers Annual Meeting, Abstract #XXXX. LPI Contribution No. 2066, Lunar and Planetary Institute, Houston. Guide to Sessions Tuesday, June 12, 2018 9:00 a.m. Strong Hall Meeting Room Introduction and Mercury and Venus Maps 1:00 p.m. Strong Hall Meeting Room Mars Maps 5:30 p.m. Strong Hall Poster Area Poster Session: 2018 Planetary Geologic Mappers Meeting Wednesday, June 13, 2018 8:30 a.m. Strong Hall Meeting Room GIS and Planetary Mapping Techniques and Lunar Maps 1:15 p.m. Strong Hall Meeting Room Asteroid, Dwarf Planet, and Outer Planet Satellite Maps Thursday, June 14, 2018 8:30 a.m. Strong Hall Optional Field Trip to Appalachian Mountains Program Tuesday, June 12, 2018 INTRODUCTION AND MERCURY AND VENUS MAPS 9:00 a.m. Strong Hall Meeting Room Chairs: David Williams Devon Burr 9:00 a.m. -
The Time Scales of Continental Rifting: Implications for Global Processes
spe500-11 1st pgs page 1 The Geological Society of America 18888 201320 Special Paper 500 2013 CELEBRATING ADVANCES IN GEOSCIENCE The time scales of continental rifting: Implications for global processes Cynthia J. Ebinger* Department of Earth Sciences, University of Rochester, Rochester, New York 14627, USA Jolante van Wijk* Department of Earth and Atmospheric Sciences, University of Houston, Houston, Texas 77204-5007, USA Derek Keir* National Oceanography Centre Southampton, University of Southampton, Southampton, UK ABSTRACT The rifting cycle initiates with stress buildup, release as earthquakes and/or magma intrusions/eruptions, and visco-elastic rebound, multiple episodes of which combine to produce the observed, time-averaged rift zone architecture. The aim of our synthesis of current research initiatives into continental rifting-to-rupture pro- cesses is to quantify the time and length scales of faulting and magmatism that pro- duce the time-averaged rift structures imaged in failed rifts and passive margins worldwide. We compare and contrast seismic and geodetic strain patterns during dis- crete, intense rifting episodes in magmatic and amagmatic sectors of the East African rift zone that span early- to late-stage rifting. We also examine the longer term rifting cycle and its relation to changing far-fi eld extension directions with examples from the Rio Grande rift zone and other cratonic rifts. Over time periods of millions of years, periods of rotating regional stress fi elds are marked by a lull in magmatic activity and a temporary halt to tectonic rift opening. Admittedly, rifting cycle comparisons are biased by the short time scale of global seismic and geodetic measurements, which span a small fraction of the 102–105 year rifting cycle. -
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. -
Seafloor Spreading Event in Western Gulf of Aden During the November
Seafloor spreading event in western Gulf of Aden during the November 2010 -- March 2011 period captured by regional seismic networks: Evidence for diking events and interactions with a nascent transform zone Abdulhakim Ahmed, C´ecileDoubre, Sylvie Leroy, Kassim Mohamed, Derek Keir, Abayazid Ahmadine, Julie Perrot, Laurence Audin, Jerome Vergne, Alexandre Nercessian, et al. To cite this version: Abdulhakim Ahmed, C´ecile Doubre, Sylvie Leroy, Kassim Mohamed, Derek Keir, et al.. Seafloor spreading event in western Gulf of Aden during the November 2010 -- March 2011 period captured by regional seismic networks: Evidence for diking events and interactions with a nascent transform zone. Geophysical Journal International, Oxford University Press (OUP), 2016, 205 (2), pp.1244-1266. <10.1093/gji/ggw068>. <hal-01284416> HAL Id: hal-01284416 https://hal.archives-ouvertes.fr/hal-01284416 Submitted on 7 Mar 2016 HAL is a multi-disciplinary open access L'archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destin´eeau d´ep^otet `ala diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publi´esou non, lished or not. The documents may come from ´emanant des ´etablissements d'enseignement et de teaching and research institutions in France or recherche fran¸caisou ´etrangers,des laboratoires abroad, or from public or private research centers. publics ou priv´es. Title: Seafloor spreading event in western Gulf of Aden during the November 2010 - March 2011 period captured by regional seismic networks: Evidence for diking events and interactions with a nascent transform zone Authors: Ahmed Abdulhakim1,2,3,*, Doubre Cécile4, Leroy Sylvie2,3, Mohamed Kassim5 , Keir Derek6, Ahmadine Abayazid5, Perrot Julie7, Audin Laurence8, Vergne Jérome4, Nercessian Alexandre9, Jacques Eric9, Khanbari Khaled10, Sholan Jamal1, Rolandone Frédérique2,3, Alganad Ismael11 Affiliations: 1Seismological and Volcanological Observatory Center, Dhamar, Yemen. -
Martian Subsurface Properties and Crater Formation Processes Inferred from Fresh Impact Crater Geometries
Martian Subsurface Properties and Crater Formation Processes Inferred From Fresh Impact Crater Geometries The Harvard community has made this article openly available. Please share how this access benefits you. Your story matters Citation Stewart, Sarah T., and Gregory J. Valiant. 2006. Martian subsurface properties and crater formation processes inferred from fresh impact crater geometries. Meteoritics and Planetary Sciences 41: 1509-1537. Published Version http://meteoritics.org/ Citable link http://nrs.harvard.edu/urn-3:HUL.InstRepos:4727301 Terms of Use This article was downloaded from Harvard University’s DASH repository, and is made available under the terms and conditions applicable to Other Posted Material, as set forth at http:// nrs.harvard.edu/urn-3:HUL.InstRepos:dash.current.terms-of- use#LAA Meteoritics & Planetary Science 41, Nr 10, 1509–1537 (2006) Abstract available online at http://meteoritics.org Martian subsurface properties and crater formation processes inferred from fresh impact crater geometries Sarah T. STEWART* and Gregory J. VALIANT Department of Earth and Planetary Sciences, Harvard University, 20 Oxford Street, Cambridge, Massachusetts 02138, USA *Corresponding author. E-mail: [email protected] (Received 22 October 2005; revision accepted 30 June 2006) Abstract–The geometry of simple impact craters reflects the properties of the target materials, and the diverse range of fluidized morphologies observed in Martian ejecta blankets are controlled by the near-surface composition and the climate at the time of impact. Using the Mars Orbiter Laser Altimeter (MOLA) data set, quantitative information about the strength of the upper crust and the dynamics of Martian ejecta blankets may be derived from crater geometry measurements. -
Local Earthquake Magnitude Scale and B-Value for the Danakil Region of Northern Afar by Finnigan Illsley-Kemp, Derek Keir,* Jonathan M
Bulletin of the Seismological Society of America, Vol. 107, No. 2, pp. 521–531, April 2017, doi: 10.1785/0120150253 Ⓔ Local Earthquake Magnitude Scale and b-Value for the Danakil Region of Northern Afar by Finnigan Illsley-Kemp, Derek Keir,* Jonathan M. Bull, Atalay Ayele, James O. S. Hammond, J.-Michael Kendall, Ryan J. Gallacher, Thomas Gernon, and Berhe Goitom Abstract The Danakil region of northern Afar is an area of ongoing seismic and volcanic activity caused by the final stages of continental breakup. To improve the quantification of seismicity, we developed a calibrated local earthquake magnitude scale. The accurate calculation of earthquake magnitudes allows the estimation of b-values and maximum magnitudes, both of which are essential for seismic-hazard analysis. Earthquake data collected between February 2011 and February 2013 on 11 three-component broadband seismometers were analyzed. A total of 4275 earthquakes were recorded over hypocentral distances ranging from 0 to 400 km. A total of 32,904 zero-to-peak amplitude measurements (A) were measured on the seismometer’s horizontal components and were incorporated into a direct linear inversion that M solved for all individual local earthquake magnitudes ( L), 22 station correction fac- C n K M A− tors ( ), and 2 distance-dependent factors ( , ) in the equation L log log A0C. The resultant distance correction term is given by − log A0 1:274336 log r=17 − 0:000273 r − 172. This distance correction term suggests that attenuation in the upper and mid-crust of northern Afar is relatively high, con- sistent with the presence of magmatic intrusions and partial melt. -
Seasonal Melting and the Formation of Sedimentary Rocks on Mars, with Predictions for the Gale Crater Mound
Seasonal melting and the formation of sedimentary rocks on Mars, with predictions for the Gale Crater mound Edwin S. Kite a, Itay Halevy b, Melinda A. Kahre c, Michael J. Wolff d, and Michael Manga e;f aDivision of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California 91125, USA bCenter for Planetary Sciences, Weizmann Institute of Science, P.O. Box 26, Rehovot 76100, Israel cNASA Ames Research Center, Mountain View, California 94035, USA dSpace Science Institute, 4750 Walnut Street, Suite 205, Boulder, Colorado, USA eDepartment of Earth and Planetary Science, University of California Berkeley, Berkeley, California 94720, USA f Center for Integrative Planetary Science, University of California Berkeley, Berkeley, California 94720, USA arXiv:1205.6226v1 [astro-ph.EP] 28 May 2012 1 Number of pages: 60 2 Number of tables: 1 3 Number of figures: 19 Preprint submitted to Icarus 20 September 2018 4 Proposed Running Head: 5 Seasonal melting and sedimentary rocks on Mars 6 Please send Editorial Correspondence to: 7 8 Edwin S. Kite 9 Caltech, MC 150-21 10 Geological and Planetary Sciences 11 1200 E California Boulevard 12 Pasadena, CA 91125, USA. 13 14 Email: [email protected] 15 Phone: (510) 717-5205 16 2 17 ABSTRACT 18 A model for the formation and distribution of sedimentary rocks on Mars 19 is proposed. The rate{limiting step is supply of liquid water from seasonal 2 20 melting of snow or ice. The model is run for a O(10 ) mbar pure CO2 atmo- 21 sphere, dusty snow, and solar luminosity reduced by 23%. -
(Afar) from Insar and Seismicity Alessandro La Rosa, Carolina Pagli, Hua Wang, Cecile Doubre, Sylvie Leroy, Federico Sani, Giacomo Corti, Atalay Ayele, Derek Keir
Plate-Boundary Kinematics of the Afrera Linkage Zone (Afar) From InSAR and Seismicity Alessandro La Rosa, Carolina Pagli, Hua Wang, Cecile Doubre, Sylvie Leroy, Federico Sani, Giacomo Corti, Atalay Ayele, Derek Keir To cite this version: Alessandro La Rosa, Carolina Pagli, Hua Wang, Cecile Doubre, Sylvie Leroy, et al.. Plate-Boundary Kinematics of the Afrera Linkage Zone (Afar) From InSAR and Seismicity. Journal of Geophysical Research : Solid Earth, American Geophysical Union, 2021, 126 (5), 10.1029/2020jb021387. hal- 03266506 HAL Id: hal-03266506 https://hal.sorbonne-universite.fr/hal-03266506 Submitted on 21 Jun 2021 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. RESEARCH ARTICLE Plate-Boundary Kinematics of the Afrera Linkage Zone 10.1029/2020JB021387 (Afar) From InSAR and Seismicity Key Points: Alessandro La Rosa1,2 , Carolina Pagli1 , Hua Wang3 , Cecile Doubre4 , • InSAR time-series and seismicity Sylvie Leroy5 , Federico Sani2 , Giacomo Corti6 , Atalay Ayele7, and Derek Keir2,8 analyses of deformation at the Afrera Plain linkage zone in Northern -
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 -
The Very Forward CASTOR Calorimeter of the CMS Experiment
EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH (CERN) CERN-EP-2020-180 2021/02/11 CMS-PRF-18-002 The very forward CASTOR calorimeter of the CMS experiment The CMS Collaboration* Abstract The physics motivation, detector design, triggers, calibration, alignment, simulation, and overall performance of the very forward CASTOR calorimeter of the CMS exper- iment are reviewed. The CASTOR Cherenkov sampling calorimeter is located very close to the LHC beam line, at a radial distance of about 1 cm from the beam pipe, and at 14.4 m from the CMS interaction point, covering the pseudorapidity range of −6.6 < h < −5.2. It was designed to withstand high ambient radiation and strong magnetic fields. The performance of the detector in measurements of forward energy density, jets, and processes characterized by rapidity gaps, is reviewed using data collected in proton and nuclear collisions at the LHC. ”Published in the Journal of Instrumentation as doi:10.1088/1748-0221/16/02/P02010.” arXiv:2011.01185v2 [physics.ins-det] 10 Feb 2021 © 2021 CERN for the benefit of the CMS Collaboration. CC-BY-4.0 license *See Appendix A for the list of collaboration members Contents 1 Contents 1 Introduction . .1 2 Physics motivation . .3 2.1 Forward physics in proton-proton collisions . .3 2.2 Ultrahigh-energy cosmic ray air showers . .5 2.3 Proton-nucleus and nucleus-nucleus collisions . .5 3 Detector design . .6 4 Triggers and operation . .9 5 Event reconstruction and calibration . 12 5.1 Noise and baseline . 13 5.2 Gain correction factors . 15 5.3 Channel-by-channel intercalibration . -
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Chapter One: Introduction
ADDIS ABABA UNIVERSITY COLLEGE OF NATURAL SCIENCES SCHOOL OF EARTH SCIENCES GRAVITY STUDIES OF THE CRUSTAL STRUCTURES BENEATH THE NORTHERN MAIN ETHIOPIAN RIFT AND THE ADJOINING EASTERN PLATEAU FITHAT HABTEWELD KASSA A thesis submitted to the school of Graduate studies of Addis Ababa University in partial fulfillment of the requirement for the Degree of Masters of Science in Exploration Geophysics Submission date 2014 ADDIS ABABA UNIVERSITY COLLEGE OF NATURAL SCIENCES SCHOOL OF EARTH SCIENCES GEOPHYSICAL STUDIES TO MAP CRUSTAL STRUCTURES BENEATH BOTH THE MAGMATIC SEGMENTS IN THE NORTHERN MAIN ETHIOPIAN RIFT AND THE EASTERN BORDER FAULTS By Fithat Habteweld Kassa Approved by board of examiners: Dr. Seifu Kebede .................................................................................................................................................. (Chairman, Department Signature Graduate Committee) Dr. Tilahun Mammo ……………………………………………………………………………………………… Advisor Signature Dr. Tigstu Haile ……………………………………………………………………………………………… Internal examiner Signature Dr. Tesfaye Kidane ……………………………………………………………………………………………… External examiner Signature Dr. Mulugeta Alene ……………………………………………………………………………………………… Chairman Signature Acknowledgements My profound gratitude goes to my advisor Dr Tilahun Mammo, for the proper supervision, support and guidance he provided me throughout my research. His critical comments, fatherly approach and unreserved effort have given me the opportunity to explore more. Special thanks to Geological Survey of Ethiopia for giving