DOCSLIB.ORG

S01. Open Session

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
S01. Open Session IASPEI Seismological Observation and Session: S01-2 Session title: Open session II Interpretation Type: Oral Date: Monday, July 31, 2017 Time: 10:30 - 12:00 S01. Room: Room 501 Chairs: Thomas Meier (University of Kiel) Open session Aitaro Kato (University of Tokyo) Time Title Program No. 10:30 Calculating the ISC's own S01-2-01 Session: S01-1 magnitudes Session title: Open session I Elizabeth Entwistle, Domenico Di Giacomo, Dmitry Storchak Type: Oral Date: Monday, July 31, 2017 10:45 Policy issues for the European S01-2-02 Time: 08:30 - 10:00 Seismological Services within EPOS Florian Haslinger, EPOS Seismology Room: Room 501 Consortium Chairs: Thomas Meier (University of Kiel) Dmitry Storchak (International Seismological 11:00 The Mexican National Seismological S01-2-03 Centre) Service: An overview Xyoli Perez-Campos, SSN Personnel Time Title Program No. 11:15 Compilation of a Seismic Bulletin for S01-2-04 the European Arctic 08:30 Automatic hypocenter determination S01-1-01 Johannes Schweitzer, Yana for the Seismological Bulletin of Konechnaya, Andrey Fedorov, Steven Japan using Bayesian estimation Gibbons, Berit Paulsen, Myrto Pirli and its applications Koji Tamaribuchi 11:30 The ISC-GEM Global Instrumental S01-2-05 Earthquake Catalogue: Current 08:45 Automated seismic event location S01-1-02 status and efforts to extend the combining waveform stacking and period 1904-1919 relative location techniques Domenico Di Giacomo, Bob Engdahl, Francesco Grigoli, Simone Cesca, Dmitry Storchak, James Harris Frederic Massin, Anne Obermann, Wilfried Strauch, John Clinton, Stefan 11:45 Development of a web-application S01-2-06 Wiemer system for seismic waveform data observed at real-time with the 09:00 Over 20 years of HYPOSAT: Newest S01-1-03 seafloor seismic network, DONET developments Daisuke Sugiyama, Morifumi Takaesu, Johannes Schweitzer Hiroki Horikawa, Kentaro Sueki, 09:15 A tremor location method using S01-1-04 Narumi Takahashi, Seiji Tsuboi products of cross correlations Ka Lok Li, Hamzeh Sadeghisorkhani, Giulia Sgattoni, Olafur Gudmundsson, Roland Roberts Session: S01-3 09:30 Rapid estimation of seismic S01-1-05 Session title: Open session III moment, magnitude and energy for Type: Oral small to large events: improvement Date: Tuesday, August 1, 2017 from Central Italy, 2016 seismic Time: 08:30 - 10:00 sequence Room: Room 501 Antonella Gallo, Giovanni Costa, Chairs: Domenico Di Giacomo (International Seismological Rita De Nardis, Luisa Filippi, Giusy Lavecchia, Elisa Zambonelli Centre) Aitaro Kato (University of Tokyo) 09:45 Towards routine determinations S01-1-06 of earthquake focal mechanisms Time Title Program No. obtained from P-wave first motion polarities 08:30 The Global Seismographic Network S01-3-01 Konstantinos Lentas, Dmitry Storchak (GSN): New VBB Borehole Sensors, Sensor Emplacement Techniques and Data Quality Assessment using MUSTANG Katrin Hafner, Peter Davis, David Wilson, Robert Woodward 08:45 Anatomy of a subduction zone – S01-3-02 seismicity structure of the northern Chilean forearc from >100,000 relocated earthquake hypocenters Bernd Schurr, Christian Sippl 100 09:00 The 30 May 2015 Bonin Deep S01-3-03 11:30 Exhaustive analysis of surface wave S01-4-05 Earthquake and the 660-km propagation in a combined use Discontinuity Around its Source of active and passive surveys for Region detailed site characterization Keiko Kuge Paolo Bergamo, Stefano Marano, Manuel Hobiger, Donat Faeh 09:15 The January 2017 Barrow Strait S01-3-04 Earthquake and Subsequent 11:45 Investigation of deep sedimentary S01-4-06 Seismic Activity in Arctic Canada and crustal structures with passive Allison Bent, Nicholas Ackerley, Michal seismic methods Kolaj, John Adams Dario Chieppa, Manuel Hobiger, Marco Pilz, Donat Faeh 09:30 Long Duration of Ground Motion in S01-3-05 the Paradigmatic Valley of Mexico Victor M. Cruz-Atienza, Josue Tago, Jose David Sanabria-Gomez, Emmanuel Chaljub, Vincent Etienne, Session: S01-P Jean Virieux, Luis Quintanar Type: Poster Date: Tuesday, August 1/ Wednesday, August 2, 2017 09:45 Difference in energy radiation from S01-3-06 Time: 15:30 - 16:30 earthquakes with similar moment magnitude and focal mechanism: Room: Event Hall the broadband body-wave magnitudes of the 2014 Ludian and Title Program No. Jinggu, Yunnan Province, China, Fast hypocenter determination S01-P-01 earthquake with a 3D velocity model and Zhongliang Wu, Changsheng Jiang, its implication for seismicity Xiaoxiao Song monitoring Akio Katsumata Moment tensor inversion of shallow S01-P-02 Session: S01-4 offshore earthquakes in the Nankai Session title: Open session IV subduction zone using a three- dimensional velocity structure Type: Oral model Date: Tuesday, August 1, 2017 Shunsuke Takemura, Takeshi Kimura, Time: 10:30 - 12:00 Katsuhiko Shiomi, Hisahiko Kubo, Room: Room 501 Tatsuhiko Saito Chairs: Domenico Di Giacomo (International Seismological Local Magnitude, ML Scale for S01-P-03 Centre) the Philippines: Investigation of Elizabeth Entwistle (International Seismological Hypocentral Distance Dependence Centre) Johnlery Deximo, Tatsuhiko Hara The Mechanism of Rare Earthquakes S01-P-04 Time Title Program No. in Pidie Jaya, Aceh Derived from 10:30 Recent earthquakes at Disko Island, S01-4-01 Source Parameter and Shear Wave Greenland, with focal mechanisms Splitting Tomography Trine Dahl-Jensen, Peter H Voss, Tine Rexha Verdhora Ry, Andri Dian B Larsen Nugraha, Sri Widiyantoro, Riskiray Ryannugroho, Kadek Hendrawan 10:45 New insights into volcano-tectonic S01-4-02 Palgunadi, Muksin Umar, Zulfakriza seismicity patterns in the Virunga Zulfakriza, Kemal Erbas Volcanic Province, Democratic Republic of the Congo, from a Rupture process of the 1979 S01-P-05 new broadband seismic network Tumaco, Colombia, earthquake (KivuSNet) using teleseismic body waves Adrien Oth, Julien Barriere, Nicolas Masahiro Yoshimoto, Hiroyuki d'Oreye, Francois Kervyn Kumagai, Nelson Pulido 11:00 Monitoring eruption activity using S01-4-03 Stress drop characteristics of the S01-P-06 temporal stress changes at Mount 2008-2016 Storfjorden earthquake Ontake volcano sequence Toshiko Terakawa, Yoshiko Yamanaka, Lars Ottemoller, Norunn Tjaaland, Yuta Maeda, Shinichiro Horikawa, Hasbi Ash Shiddiqi, Won-Young Kim Takashi Okuda Adding manual picks from OBS S01-P-07 11:15 Long-term monitoring of of seismic S01-4-04 stations into the ISC Bulletin: velocity around a source fault of the the example of the 7D Cascadia 1995 Kobe earthquake Initiative Community Experiment Ryoya Ikuta, Koshun Yamaoka, Domenico Di Giacomo, Luke Cottell, Takahiro Kunitomo, Kinya Nishigami, Elizabeth Entwistle, James Harris, Toshiki Watanabe Dmitry Storchak 101 The current status of the ISC S01-P-08 The seismic sequence of the S01-P-19 Bulletin magnitude 5.7 crustal earthquake Elizabeth Entwistle, Rose Hulin, of 2014 of Focsani Basin (Romania) Blessing Shumba, Rebecca Verney, – relevant data regarding the stress Jennifer Weston, Elizabeth Ayres, field in front of the Southeastern James Harris, Dmitry Storchak, Lonn Carpathians bend Brown, Kathrin Lieser, Edith Korger Andreea Craiu, Luminita Angela Ardeleanu, Marius Craiu, Mihail S01-P-09 Automatic classification and onset Diaconescu estimation of seismic P and S wave signals recorded at local seismic Distribution of deep earthquakes in S01-P-20 network using artificial neural the subducting Pacific slab beneath networks Japan Timo Tiira Ayako Tsuchiyama, Junichi Nakajima, Toru Matsuzawa The use of seismic arrays in S01-P-10 geodynamic monitoring of the East The McAdam, New Brunswick S01-P-21 European platform Earthquake Swarms of 2012 and Irina Sanina, Ivan Kitov, Margarita 2015-16: Extremely Shallow, Natural Nesterkina, Natalia Konstantinovskaya, Events Svetlana Kishkina Allison Bent, Stephen Halchuk, Veronika Peci, Karl Butler, Kenneth S01-P-11 Development of JAMSTEC Ocean- Burke, John Adams, Nawa Dahal, bottom Seismology Database Sylvia Hayek (J-SEIS) to download DONET Event Data and Borehole Continuous Data Depth of earthquakes in Greenland S01-P-22 (4) P. H. Voss, T. B. Larsen, T. Dahl- Hiroki Horikawa, Kentaro Sueki, Jensen Kensuke Suzuki, Eiichiro Araki, Akira S01-P-23 Sonoda, Narumi Takahashi, Seiji Mw 5.5 Gyeongju Earthquake of 12 Tsuboi September 2016 in Southeastern Korea: SCR Earthquake Sequence Very wide observation range of S01-P-12 with Moderate Stress Drop the developed borehole stress Won-Young Kim, Yomggyu Ryoo meter and comparison with STS seismometer Hiroshi Ishii, Muneyoshi Furumoto, Yasuhiro Asai High-frequency geophone with S01-P-13 correction scheme for mine explosion monitoring Alina Besedina, Yaroslav Denisenko, S02. Evgeny Vinogradov Anthropogenic RESIF Seismology Distributed S01-P-14 System : Data and Services Catherine Pequegnat, Working seismicity Groupgroup RESIF SI- Data quality Improvement of the S01-P-15 Algerian Digital Seismic Network (ADSN) Session: S02-1 Azouaou Alili, Abdelkarim Yelles- Session title: World overview of anthropogenic seismicity I Chaouche, Mohamed Ouakedi, Hamoud Beldjoudi, Abdelaziz Type: Oral Kherroubi, Izeddine Ameur Date: Monday, July 31, 2017 Time: 08:30 - 10:00 Design and Implementation of S01-P-16 Room: Room 403 the National Seismic Monitoring Network in the Kingdom of Bhutan Chairs: Stanislaw Lasocki (Institute of Geophysics, Polish Shiro Ohmi, Hiroshi Inoue, Jamyang Academy of Sciences) Chophel, Phuntso Pelgay, Dowchu Pankow Kristine (University of Utah) Drukpa New steps towards local seismic S01-P-17 Time Title Program No. hazard assessment of Bucharest 08:30 Insights into faults, crustal S02-1-01
Load more

Recommended publications
  • MSS/1: Single‐Station and Single‐Event Marsquake Inversion
    RESEARCH ARTICLE MSS/1: Single‐Station and Single‐Event 10.1029/2020EA001118 Marsquake Inversion Special Section: Mélanie Drilleau1,2 , Éric Beucler3 , Philippe Lognonné1 , Mark P. Panning4 , InSight at Mars 5 4 6,7 8 Brigitte Knapmeyer‐Endrun , W. Bruce Banerdt , Caroline Beghein , Savas Ceylan , Martin van Driel8 , Rakshit Joshi9 , Taichi Kawamura1, Amir Khan8,10 , Key Points: Sabrina Menina1 , Attilio Rivoldini11 , Henri Samuel1 , Simon Stähler8 , Haotian Xu6 , • In the framework on the InSight 3 8 8 1 12 mission, a synthetic seismogram Mickaël Bonnin , John Clinton , Domenico Giardini , Balthasar Kenda , Vedran Lekic , 3 2 13 4 using a 3‐D crust and a 1‐D velocity Antoine Mocquet , Naomi Murdoch , Martin Schimmel , Suzanne E. Smrekar , model below is proposed Éléonore Stutzmann1 , Benoit Tauzin14,15 , and Saikiran Tharimena4 • This signal is used to present inversion methods, relying on 1Institut de Physique du Globe de Paris, Sorbonne Paris Cité, CNRS F‐7500511, Université Paris Diderot, Paris, France, different parameterizations, to 2ISAE‐SUPAERO, Toulouse University, Toulouse, France, 3Laboratoire de Planétologie et de Géodynamique, Université constrain the 1‐D structure of Mars 4 • The results demonstrate the de Nantes, Université d'Angers, Nantes, France, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, feasibility of the strategy to retrieve CA, USA, 5Bensberg Observatory, University of Cologne, Cologne, Germany, 6Department of Earth, Planetary, and Space 7 8 VS in the crust, and a fairly good Sciences,
    [Show full text]
  • Scientific Rationale and Requirements for a Global Seismic Network on Mars
    SCIENTIFIC RATIONALE AND REQUIREMENTS FOR A GLOBAL SEISMIC NETWORK ON MARS MARS Model AR 90 EARTH 180 (NASA-CR-188806) SCIENTIFIC RATIONALE AND N92-14949 REQUIREMENTS FOR A GLOBAL SEISMIC NETWORK ON MARS (Lunar and Planetary Inst.) 48 p CSCL 03B Unclas G3/91 0040098 LPI Technical Report Number 91-02 LUNAR AND PLANETARY INSTITUTE 3303 NASA ROAD 1 HOUSTON TX 77058-4399 LPI/TR-91-02 SCIENTIFIC RATIONALE AND REQUIREMENTS FOR A GLOBAL SEISMIC NETWORK ON MARS Sean C. Solomon, Don L. Anderson, W. Bruce Banerdt, Rhett G. Butler, Paul M. Davis, Frederick K. Duennebier, Yosio Nakamura, Emile A. Okal, and Roger J. Phillips Report of a Workshop Held at Morro Bay, California May 7-9, 1990 Lunar and Planetary Institute 3303 NASA Road 1 Houston TX 77058 LPI Technical Report Number 91-02 LPI/TR-91-02 Compiled in 1991 by the LUNAR AND PLANETARY INSTITUTE The Institute is operated by Universities Space Research Association under Contract NASW-4574 with the National Aeronautics and Space Administration. Material in this document may be copied without restraint for library, abstract service, educational, or personal research purposes; however, republication of any portion requires the written permission of the authors as well as appropriate acknowledgment of this publication. This report may be cited as: Solomon S. C. et al. (1991) Scientific Rationale and Requirements far a Global Seismic Network on Mars. LPI Tech. Rpt. 91-02, Lunar and Planetary Institute, Houston. 51 pp. This report is distributed by: ORDER DEPARTMENT Lunar and Planetary Institute 3303 NASA Road 1 Houston TX 77058-4399 Mail order requestors will be invoiced for the cost of shipping and handling.
    [Show full text]
  • March 21–25, 2016
    FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk,
    [Show full text]
  • Magnitude Scales for Marsquakes
    Bulletin of the Seismological Society of America, Vol. XX, No. XX, pp. –, – 2018, doi: 10.1785/0120180037 Ⓔ Magnitude Scales for Marsquakes by Maren Böse,* Domenico Giardini, Simon Stähler, Savas Ceylan, John Francis Clinton, Martin van Driel, Amir Khan, Fabian Euchner, Philippe Lognonné, and William Bruce Banerdt Abstract In anticipation of the upcoming 2018 InSight (Interior exploration using Seismic Investigations, Geodesy and Heat Transport) Discovery mission to Mars, we calibrate magnitude scales for marsquakes that incorporate state-of-the-art knowledge on Mars interior structure and the expected ambient and instrumental noise. We re- gress magnitude determinations of 2600 randomly distributed marsquakes, simulated with a spectral element method for 13 published 1D structural models of Mars’ interior. The continuous seismic data from InSight will be returned at 2 samples per second. To account for this limited bandwidth as well as for the expected noise conditions on Mars, we define and calibrate six magnitude scales: (1) local Mars mag- MMa nitude L at a period of 3 s for marsquakes at distances of up to 10°; (2) P-wave mMa mMa magnitude b ; (3) S-wave magnitude bS each defined at a period of 3 s and cali- MMa brated for distances from 5° to 100°; (4) surface-wave magnitude s defined at a MMa MMa period of 20 s, as well as (5) moment magnitudes FB ; and (6) F computed from the low-frequency (10–100 s) plateau of the displacement spectrum for either body waves or body and surface waves, respectively; we calibrate scales (4)–(6) for dis- tances from 5° to 180°.
    [Show full text]
  • Pre-Mission Insights on the Interior of Mars Suzanne E
    Pre-mission InSights on the Interior of Mars Suzanne E. Smrekar, Philippe Lognonné, Tilman Spohn, W. Bruce Banerdt, Doris Breuer, Ulrich Christensen, Véronique Dehant, Mélanie Drilleau, William Folkner, Nobuaki Fuji, et al. To cite this version: Suzanne E. Smrekar, Philippe Lognonné, Tilman Spohn, W. Bruce Banerdt, Doris Breuer, et al.. Pre-mission InSights on the Interior of Mars. Space Science Reviews, Springer Verlag, 2019, 215 (1), pp.1-72. 10.1007/s11214-018-0563-9. hal-01990798 HAL Id: hal-01990798 https://hal.archives-ouvertes.fr/hal-01990798 Submitted on 23 Jan 2019 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. Open Archive Toulouse Archive Ouverte (OATAO ) OATAO is an open access repository that collects the wor of some Toulouse researchers and ma es it freely available over the web where possible. This is an author's version published in: https://oatao.univ-toulouse.fr/21690 Official URL : https://doi.org/10.1007/s11214-018-0563-9 To cite this version : Smrekar, Suzanne E. and Lognonné, Philippe and Spohn, Tilman ,... [et al.]. Pre-mission InSights on the Interior of Mars. (2019) Space Science Reviews, 215 (1).
    [Show full text]
  • Mars Insight Launch Press Kit
    Introduction National Aeronautics and Space Administration Mars InSight Launch Press Kit MAY 2018 www.nasa.gov 1 2 Table of Contents Table of Contents Introduction 4 Media Services 8 Quick Facts: Launch Facts 12 Quick Facts: Mars at a Glance 16 Mission: Overview 18 Mission: Spacecraft 30 Mission: Science 40 Mission: Landing Site 53 Program & Project Management 55 Appendix: Mars Cube One Tech Demo 56 Appendix: Gallery 60 Appendix: Science Objectives, Quantified 62 Appendix: Historical Mars Missions 63 Appendix: NASA’s Discovery Program 65 3 Introduction Mars InSight Launch Press Kit Introduction NASA’s next mission to Mars -- InSight -- will launch from Vandenberg Air Force Base in California as early as May 5, 2018. It is expected to land on the Red Planet on Nov. 26, 2018. InSight is a mission to Mars, but it is more than a Mars mission. It will help scientists understand the formation and early evolution of all rocky planets, including Earth. A technology demonstration called Mars Cube One (MarCO) will share the launch with InSight and fly separately to Mars. Six Ways InSight Is Different NASA has a long and successful track record at Mars. Since 1965, it has flown by, orbited, landed and roved across the surface of the Red Planet. None of that has been easy. Only about 40 percent of the missions ever sent to Mars by any space agency have been successful. The planet’s thin atmosphere makes landing a challenge; its extreme temperature swings make it difficult to operate on the surface. But if a spacecraft survives the trip, there’s a bounty of science to be collected.
    [Show full text]
  • Spacecraft Insight's Mission Is to Find Clues on How Mars First Formed
    Spacecraft InSight's mission is to find clues on how Mars first formed By Washington Post, adapted by Newsela staff on 05.07.18 Word Count 759 Level 840L An illustration of the InSight lander on Mars. Photo by: NASA/JPL-Cal Tech What do you call an earthquake that happens on Mars? Scientists call it a marsquake. This is not a nerdy joke. It's an important part of the mission for NASA's newest spacecraft, InSight. The spacecraft launched early on the morning of Saturday, May 5. It carries tools to take the temperature and measure shakes deep beneath Mars' surface. Even the slightest shake could carry clues about how the planet formed. Scientists will also learn what goes on today beneath the planet's surface. Earth and Mars formed from the same ingredients. That was more than 4.5 billion years ago. InSight aims to help scientists understand why the two planets now look so different. This article is available at 5 reading levels at https://newsela.com. 1 Suzanne Smrekar is a NASA scientist working on the project. She said one reason Earth looks different from Mars is plate tectonics. Plate tectonics means that the outer layer of the Earth is made from separate pieces, or plates. They move very slowly over time. As they move, they reshape the continents, creating volcanoes and causing earthquakes. InSight Will Study Quakes On Mars Plate tectonics also means that Earth's outer layer is made up of different material now than it was billions of years ago. Mars is different too.
    [Show full text]
  • Marsquake Challenge
    MARSQUAKE CHALLENGE Did you know Mars has earthquakes? Or rather… Marsquakes? Scientists theorize that these quakes DESIGN CHALLENGE are similar to what we experience here on Earth, however, it is unclear exactly what goes on beneath Build a model habitat the surface of Mars to cause them. Volcanic activity, that can survive a meteor impacts, and planetary shifting are believed simulated Marsquake. to be the source, yet there is still much to learn. In order to search for an answer, scientists are using data collected from the InSight lander to reveal information about the inner-workings of the Red Planet. InSight will not only help us determine the source of the quakes, but how often CRITERIA and severe they are as well. This information may be helpful to know since NASA is planning to send humans to live on Mars. If the planet experiences You can use any household materials to build, besides extreme quakes, it must be taken into consideration. Habitats must be built and tape. tested against conditions like quakes in order to safely achieve long-term human survival on Mars. To survive, your habitat must remain standing, without your help, during a “mild” HOW IT WORKS Marsquake*. In this activity, learners will attempt to design model habitats that can withstand a quake on Mars. To begin, build a If any element of your habitat collapses or falls off, it did not Marsquake table to simulate the planet’s shaking surface. survive. Then, build a habitat and test it to determine whether it can survive the quakes on Mars.
    [Show full text]
  • Rhyming Dictionary
    Merriam-Webster's Rhyming Dictionary Merriam-Webster, Incorporated Springfield, Massachusetts A GENUINE MERRIAM-WEBSTER The name Webster alone is no guarantee of excellence. It is used by a number of publishers and may serve mainly to mislead an unwary buyer. Merriam-Webster™ is the name you should look for when you consider the purchase of dictionaries or other fine reference books. It carries the reputation of a company that has been publishing since 1831 and is your assurance of quality and authority. Copyright © 2002 by Merriam-Webster, Incorporated Library of Congress Cataloging-in-Publication Data Merriam-Webster's rhyming dictionary, p. cm. ISBN 0-87779-632-7 1. English language-Rhyme-Dictionaries. I. Title: Rhyming dictionary. II. Merriam-Webster, Inc. PE1519 .M47 2002 423'.l-dc21 2001052192 All rights reserved. No part of this book covered by the copyrights hereon may be reproduced or copied in any form or by any means—graphic, electronic, or mechanical, including photocopying, taping, or information storage and retrieval systems—without written permission of the publisher. Printed and bound in the United States of America 234RRD/H05040302 Explanatory Notes MERRIAM-WEBSTER's RHYMING DICTIONARY is a listing of words grouped according to the way they rhyme. The words are drawn from Merriam- Webster's Collegiate Dictionary. Though many uncommon words can be found here, many highly technical or obscure words have been omitted, as have words whose only meanings are vulgar or offensive. Rhyming sound Words in this book are gathered into entries on the basis of their rhyming sound. The rhyming sound is the last part of the word, from the vowel sound in the last stressed syllable to the end of the word.
    [Show full text]
  • Does Mars Still Shake, Rattle and Roll? 13 March 2012, by Paul Scott Anderson
    Does Mars still shake, rattle and roll? 13 March 2012, By Paul Scott Anderson Boulders on the floor of Cerberus Fossae. Credit: NASA/JPL/University of Arizona Closeup of boulders and trails in Cerberus Fossae. Credit: NASA/JPL/University of Arizona Compared to Earth, Mars is a relatively quiet planet, geologically speaking. Actually, very quiet, as in pretty much dead. While it has volcanoes much larger than any here, they have been Scientists in Europe have been examining images inactive for a very long time; the latest studies of a Martian fault system, Cerberus Fossae, taken suggest however that volcanic activity may have by the Mars Reconnaissance Orbiter. They've continued until only a matter of millions of years found a spot where boulders have tumbled down ago. That seems like an eternity to our human cliffs near the fault; what's interesting is that they sense of time, but geologically, it is quite recent. are primarily found in one location, best explained by marsquakes rather than melting ice and There is also the massive canyon system Valles avalanches. This grouping of boulders suggests Marineris, much larger than the Grand Canyon that they were near the epicentre of a marsquake. here on Earth, and evidence for ancient hot The trails behind the rolling boulders are still visible, springs, glaciers, etc. which also show that Mars indicating that they must have fallen relatively was once much more active than it is today. recently, with not enough time yet for winds to erase the trails. Now, there is also evidence that marsquakes (as in earthquakes here) continued to shake the Marsquakes would also be evidence for possible planet until only a few million years ago, and may continued volcanism on the planet, even if only even still happen today.
    [Show full text]
  • Mars Structure Service: Single-Station and Single-Event Marsquake Inversion for Structure Using Synthetic Martian Waveforms
    Geophysical Research Abstracts Vol. 21, EGU2019-7163, 2019 EGU General Assembly 2019 © Author(s) 2019. CC Attribution 4.0 license. Mars Structure Service: Single-station and single-event marsquake inversion for structure using synthetic Martian waveforms Melanie Drilleau (1), Amir Khan (2), Eric Beucler (3), Mark Panning (4), Philippe Lognonne (1), Caroline Beghein (5), Haotian Xu (5), Sabrina Menina (1), Salma Barkaoui (1), Vedran Lekic (6), Simon Stahler (2), Martin van Driel (2), Balthasar Kenda (1), Naomi Murdoch (7), John Clinton (2), Domenico Giardini (2), Suzanne Smrekar (4), Eleonore Stutzmann (1), and Martin Schimmel (8) (1) Institut de Physique du Globe de Paris, Sorbonne Paris Cité, Université Paris Diderot, CNRS F-75005 Paris, France, (2) Institute for Geophysics, ETH Zürich, Zürich, Switzerland , (3) Université de Nantes, Laboratoire de Planétologie et de Géodynamique, UMR-CNRS 6112, Nantes, France, (4) Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA, (5) Department of Earth, Planetary, and Space Sciences, University of California Los Angeles, Los Angeles, CA 90095, USA, (6) Department of Geology, University of Maryland, College Park, MD 20742, USA , (7) ISAE-SUPAERO, Toulouse University, 10 Ave E. Belin, 31400 Toulouse, France, (8) ICTJA-CSIC, Barcelona, Spain The InSight lander successfully delivered geophysical instrument package on the Martian surface on November 26th, 2018, including a broadband and a short-period seismometer (Seismic Experiment for Interior Structure, SEIS). The seismic instrument package is specifically designed to record marsquakes and meteoritic impacts in Martian conditions. Routine operations are split into two services: the Mars Structure Service (MSS) and the Marsquake Service (MQS), which are responsible for defining structure models and seismicity catalogs, respec- tively.
    [Show full text]
  • Building with Martian Regolith Experimental Research on the Efficient and Sustainable Production Process and Construction Method
    BUILDING WITH MARTIAN REGOLITH EXPERIMENTAL RESEARCH ON THE EFFICIENT AND SUSTAINABLE PRODUCTION PROCESS AND CONSTRUCTION METHOD AGATA MINTUS, 4745523 GRADUATION REPORT BUILDING WITH MARTIAN REGOLITH AGATA MINTUS, 4745523 PERSONAL INFORMATION TELEPHONE NUMBER: EMAIL ADDRESS: STUDIO/TOPIC NAME: Sustainable Design Graduation Studio - Material Science & Structural Design THEME: Experimental research on sustainable production and fabrication of novel material MENTORS: Dr.ir. F.A. Veer (first mentor) 2 Dr. O. Copuroglu (second mentor) Dr.D.P. Peck (third mentor) SUPERVISORS: Layla van Ellen Fernando França de Mendonça Filho GRADUATION PROJECT TITLE: Building with Martian regolith TOPIC: Experimental research on the efficient and sustainable production process and construction method KEYWORDS: Mars | building | ISRU fabrication | sustainability | regolith | efficiency Graduation Report | Agata Mintus PREFACE The main reason for choosing this topic is due to my interest in a hands-on approach and structural design. During my studies, I was developing my skills and knowledge in achieving sustainability in structural design optimization and manufacturing methods. Also, my passion for space architecture pushed me in the direction of experimental research which is possible to perform in the Sustainable Graduation Studio. I didn’t expect at the beginning of thesis studies, that I would be able to propose my own topic for the graduation project, that would be unusual and extreme in terms of the context. The fact, that I was able to focus on my passion and interest towards more scientific aspects like material science during this research made the work enjoyable, challenging and exciting. Therefore I would like to express my gratitude to everyone who helped me accomplish this goal and individual growth.
    [Show full text]