A Review of Interferometric Synthetic Aperture RADAR (Insar) Multi-Track Approaches for the Retrieval of Earth’S Surface Displacements
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Mission to Jupiter
This book attempts to convey the creativity, Project A History of the Galileo Jupiter: To Mission The Galileo mission to Jupiter explored leadership, and vision that were necessary for the an exciting new frontier, had a major impact mission’s success. It is a book about dedicated people on planetary science, and provided invaluable and their scientific and engineering achievements. lessons for the design of spacecraft. This The Galileo mission faced many significant problems. mission amassed so many scientific firsts and Some of the most brilliant accomplishments and key discoveries that it can truly be called one of “work-arounds” of the Galileo staff occurred the most impressive feats of exploration of the precisely when these challenges arose. Throughout 20th century. In the words of John Casani, the the mission, engineers and scientists found ways to original project manager of the mission, “Galileo keep the spacecraft operational from a distance of was a way of demonstrating . just what U.S. nearly half a billion miles, enabling one of the most technology was capable of doing.” An engineer impressive voyages of scientific discovery. on the Galileo team expressed more personal * * * * * sentiments when she said, “I had never been a Michael Meltzer is an environmental part of something with such great scope . To scientist who has been writing about science know that the whole world was watching and and technology for nearly 30 years. His books hoping with us that this would work. We were and articles have investigated topics that include doing something for all mankind.” designing solar houses, preventing pollution in When Galileo lifted off from Kennedy electroplating shops, catching salmon with sonar and Space Center on 18 October 1989, it began an radar, and developing a sensor for examining Space interplanetary voyage that took it to Venus, to Michael Meltzer Michael Shuttle engines. -
Geotechnical Reconnaissance of the 2015 Mw8.3 Illapel, Chile Earthquake
GEOTECHNICAL EXTREME EVENTS RECONNAISSANCE (GEER) ASSOCIATION Turning Disaster into Knowledge Geotechnical Reconnaissance of the 2015 Mw8.3 Illapel, Chile Earthquake Editors: Gregory P. De Pascale, Gonzalo Montalva, Gabriel Candia, and Christian Ledezma Lead Authors: Gabriel Candia, Universidad del Desarrollo-CIGIDEN; Gregory P. De Pascale, Universidad de Chile; Christian Ledezma, Pontificia Universidad Católica de Chile; Felipe Leyton, Centro Sismológico Nacional; Gonzalo Montalva, Universidad de Concepción; Esteban Sáez, Pontificia Universidad Católica de Chile; Gabriel Vargas Easton, Universidad de Chile. Contributing Authors: Juan Carlos Báez, Centro Sismológico Nacional; Christian Barrueto, Pontificia Universidad Católica de Chile; Cristián Benítez, Pontificia Universidad Católica de Chile; Jonathan Bray, UC Berkeley; Alondra Chamorro, Pontificia Universidad Católica de Chile; Tania Cisterna, Universidad de Concepción; Fernando Estéfan Thibodeaux Garcia, UC Berkeley; José González, Universidad de Chile; Diego Inzunza, Universidad de Concepción; Rosita Jünemann, Pontificia Universidad Católica de Chile; Benjamín Ledesma, Universidad de Concepción; Álvaro Muñoz, Pontificia Universidad Católica de Chile; Antonio Andrés Muñoz, Universidad de Chile; José Quiroz, Universidad de Concepción; Francesca Sandoval, Universidad de Chile; Pedro Troncoso, Universidad de Concepción; Carlos Videla, Pontificia Universidad Católica de Chile; Angelo Villalobos, Universidad de Chile. GEER Association Report No. GEER-043 Version 1: December 10, 2015 FUNDING -
The Reference Mission of the NASA Mars Exploration Study Team
NASA Special Publication 6107 Human Exploration of Mars: The Reference Mission of the NASA Mars Exploration Study Team Stephen J. Hoffman, Editor David I. Kaplan, Editor Lyndon B. Johnson Space Center Houston, Texas July 1997 NASA Special Publication 6107 Human Exploration of Mars: The Reference Mission of the NASA Mars Exploration Study Team Stephen J. Hoffman, Editor Science Applications International Corporation Houston, Texas David I. Kaplan, Editor Lyndon B. Johnson Space Center Houston, Texas July 1997 This publication is available from the NASA Center for AeroSpace Information, 800 Elkridge Landing Road, Linthicum Heights, MD 21090-2934 (301) 621-0390. Foreword Mars has long beckoned to humankind interest in this fellow traveler of the solar from its travels high in the night sky. The system, adding impetus for exploration. ancients assumed this rust-red wanderer was Over the past several years studies the god of war and christened it with the have been conducted on various approaches name we still use today. to exploring Earth’s sister planet Mars. Much Early explorers armed with newly has been learned, and each study brings us invented telescopes discovered that this closer to realizing the goal of sending humans planet exhibited seasonal changes in color, to conduct science on the Red Planet and was subjected to dust storms that encircled explore its mysteries. The approach described the globe, and may have even had channels in this publication represents a culmination of that crisscrossed its surface. these efforts but should not be considered the final solution. It is our intent that this Recent explorers, using robotic document serve as a reference from which we surrogates to extend their reach, have can continuously compare and contrast other discovered that Mars is even more complex new innovative approaches to achieve our and fascinating—a planet peppered with long-term goal. -
Damage Assessment of the 2015 Mw 8.3 Illapel Earthquake in the North‑Central Chile
Natural Hazards https://doi.org/10.1007/s11069-018-3541-3 ORIGINAL PAPER Damage assessment of the 2015 Mw 8.3 Illapel earthquake in the North‑Central Chile José Fernández1 · César Pastén1 · Sergio Ruiz2 · Felipe Leyton3 Received: 27 May 2018 / Accepted: 19 November 2018 © Springer Nature B.V. 2018 Abstract Destructive megathrust earthquakes, such as the 2015 Mw 8.3 Illapel event, frequently afect Chile. In this study, we assess the damage of the 2015 Illapel Earthquake in the Coquimbo Region (North-Central Chile) using the MSK-64 macroseismic intensity scale, adapted to Chilean civil structures. We complement these observations with the analysis of strong motion records and geophysical data of 29 seismic stations, including average shear wave velocities in the upper 30 m, Vs30, and horizontal-to-vertical spectral ratios. The calculated MSK intensities indicate that the damage was lower than expected for such megathrust earthquake, which can be attributable to the high Vs30 and the low predominant vibration periods of the sites. Nevertheless, few sites have shown systematic high intensi- ties during comparable earthquakes most likely due to local site efects. The intensities of the 2015 Illapel earthquake are lower than the reported for the 1997 Mw 7.1 Punitaqui intraplate intermediate-depth earthquake, despite the larger magnitude of the recent event. Keywords Subduction earthquake · H/V spectral ratio · Earthquake intensity 1 Introduction On September 16, 2015, at 22:54:31 (UTC), the Mw 8.3 Illapel earthquake occurred in the Coquimbo Region, North-Central Chile. The epicenter was located at 71.74°W, 31.64°S and 23.3 km depth and the rupture reached an extent of 200 km × 100 km, with a near trench rupture that caused a local tsunami in the Chilean coast (Heidarzadeh et al. -
Project Xpedition Is the Product of Purdue University‟S Aeronautical and Astronautical Engineering Department Senior Spacecraft Design Class in the Spring of 2009
92 Project Xpedition Purdue University AAE 450 Spacecraft Design Spring 2009 Contents 1 – FOREWORD ........................................................................................................................................... 5 2 – INTRODUCTION ................................................................................................................................... 7 2.1 – BACKGROUND .................................................................................................................................... 7 2.2 – WHAT‟S IN THIS REPORT? .................................................................................................................. 9 2.3 – ACKNOWLEDGEMENTS .....................................................................................................................10 2.4 – ACRONYM LIST .................................................................................................................................12 3 – PROJECT OVERVIEW ....................................................................................................................... 14 3.1 – DESIGN REQUIREMENTS ...................................................................................................................14 3.2 – INTERPRETATION OF DESIGN REQUIREMENTS ...................................................................................18 3.3 – DESIGN PROCESS ..............................................................................................................................19 3.4 – RISK -
The Moon and Eclipses
Lecture 10 The Moon and Eclipses Jiong Qiu, MSU Physics Department Guiding Questions 1. Why does the Moon keep the same face to us? 2. Is the Moon completely covered with craters? What is the difference between highlands and maria? 3. Does the Moon’s interior have a similar structure to the interior of the Earth? 4. Why does the Moon go through phases? At a given phase, when does the Moon rise or set with respect to the Sun? 5. What is the difference between a lunar eclipse and a solar eclipse? During what phases do they occur? 6. How often do lunar eclipses happen? When one is taking place, where do you have to be to see it? 7. How often do solar eclipses happen? Why are they visible only from certain special locations on Earth? 10.1 Introduction The moon looks 14% bigger at perigee than at apogee. The Moon wobbles. 59% of its surface can be seen from the Earth. The Moon can not hold the atmosphere The Moon does NOT have an atmosphere and the Moon does NOT have liquid water. Q: what factors determine the presence of an atmosphere? The Moon probably formed from debris cast into space when a huge planetesimal struck the proto-Earth. 10.2 Exploration of the Moon Unmanned exploration: 1950, Lunas 1-3 -- 1960s, Ranger -- 1966-67, Lunar Orbiters -- 1966-68, Surveyors (first soft landing) -- 1966-76, Lunas 9-24 (soft landing) -- 1989-93, Galileo -- 1994, Clementine -- 1998, Lunar Prospector Achievement: high-resolution lunar surface images; surface composition; evidence of ice patches around the south pole. -
The Chiloé Mw 7.6 Earthquake of 25 December 2016 in Southern Chile and Its Relation to the Mw 9.5 1960 Valdivia Earthquake
2016 Chiloé Earthquake, Southern Chile submitted to Geophysical Journal International The Chiloé Mw 7.6 earthquake of 25 December 2016 in Southern Chile and its relation to the Mw 9.5 1960 Valdivia earthquake 1 2 3 3 Dietrich Lange , Javier Ruiz , Sebastián Carrasco , Paula Manríquez (1) GEOMAR Helmholtz Centre for Ocean Research Kiel, Kiel, Germany (2) Departamento de Geofísica, Facultad de Ciencias Físicas y Matemáticas, Universidad de Chile, Santiago, Chile (3) National Seismological Centre, University of Chile, Santiago, Chile Keywords: 2016 Chiloé earthquake, Subduction Zone, Southern Chile, 1960 Valdivia Earthquake Corresponding author: Dietrich Lange (email: [email protected]) Abstract On 25 December 2016, a Mw 7.6 earthquake broke a portion of the Southern Chilean subduction zone south of Chiloé Island, located in the central part of the Mw 9.5 1960 Valdivia earthquake. This region is characterized by repeated earthquakes in 1960 and historical times with very sparse interseismic activity due to the subduction of a young (~15 Ma), and therefore hot, oceanic plate. We estimate the co-seismic slip distribution based on a kinematic finite fault source model, and through joint inversion of teleseismic body waves and strong motion data. The coseismic slip model yields a total seismic moment of 3.94×1020 Nm that occurred over ~30 s, with the rupture propagating mainly downdip, reaching a peak-slip of ~4.2 m. Regional moment tensor inversion of stronger aftershocks reveals thrust type faulting at depths of the plate interface. The fore- and aftershock seismicity is mostly related to the subduction interface with sparse seismicity in the overriding crust. -
Seismic Performance of Tailings Sand Dams in Chile
16th World Conference on Earthquake, 16WCEE 2017 Santiago Chile, January 9th to 13th 2017 Paper N° 4230 Registration Code: S-V1461865061 Seismic performance of tailings sand dams in Chile J. H. Troncoso (1), R. Verdugo (2), L. Valenzuela (3) (1) Senior Geotechnical Consultant, MWH Chile, (2) Senior geotechnical Consultant, CMGI Consultants (3) Geotechnical Consultant, formerly at Arcadis Abstract An extremely high and frequent seismic activity coincides in Chile with the existence of numerous tailings dams associated to the copper industry. In the country there is a history of tailings dam failures since the early XX century and up to today. Nevertheless since the decade of 1960 there have been a growing number of new large tailings dams that have had a very good performance even when subjected to very strong earthquakes. The paper summarizes the instructive history of failures as well as of successes of the newly designed tailings dams and particularly of the sand tailings dams. Different aspects of the main new sand tailings dams such as the design criteria, tailings sand characteristics under high confining stresses are discussed. These aspects are complemented with information on major earthquakes occurred in Chile in the last years, especially of El Maule Earthquake of Magnitude 8.8 of February 27, 2010 and the location of main tailings dams in the zones impacted by this earthquake. Finally, discussions are included with regard general seismic performance of tailings sand dams, seismic deformations, and seismic instrumentation including dams in operation and dams already inactive. Keywords: Tailings dams, Seismic behavior, Sand dams, Tailings sands, Dynamic properties of sands. -
The Delayed Aftershocks of the Illapel Earthquake Mw 8.3, 2015, Chile
EGU21-6978 https://doi.org/10.5194/egusphere-egu21-6978 EGU General Assembly 2021 © Author(s) 2021. This work is distributed under the Creative Commons Attribution 4.0 License. The delayed aftershocks of the Illapel Earthquake Mw 8.3, 2015, Chile Franco Lema1 and Mahesh Shrivastava1,2 1Departamento de Ciencias Geológicas, Universidad Católica del Norte, Antofagasta, Chile ([email protected]) 2National Research Center for Integrated Natural Disaster Management, Santiago, Chile ([email protected]) The delayed aftershocks 2018 Mw 6.2 on April 10 and Mw 5.8 on Sept 1 and 2019 Mw 6.7 on January 20, Mw 6.4 on June 14, and Mw 6.2 on November 4, associated with the Mw 8.3 2015 Illapel Earthquake occurred in the central Chile. The seismic source of this earthquake has been studied with the GPS, InSAR and tide gauge network. Although there are several studies performed to characterize the robust aftershocks and the variations in the field of deformation induced by the megathrust, but there are still aspects to be elucidated of the relationship between the transfer of stresses from the interface between plates towards delayed aftershocks with the crustal structures with seismogenic potential. Therefore, the principal objective of this study is to understand how the stress transfer induced by the 2015 Illapel earthquake of the heterogeneous rupture mechanism to intermediate-deep or crustal earthquakes. For this, coulomb stress changes from finite fault model of the Illapel earthquake and with the biggest aftershocks in year 2015 are used. These cumulative stress pattern provides substantial evidences for the delayed aftershocks in this region. -
Applications of SAR Interferometry in Earth and Environmental Science Research
Sensors 2009, 9, 1876-1912; doi:10.3390/s90301876 OPEN ACCESS sensors ISSN 1424-8220 www.mdpi.com/journal/sensors Review Applications of SAR Interferometry in Earth and Environmental Science Research Xiaobing Zhou 1,*, Ni-Bin Chang 2 and Shusun Li 3 1 Department of Geophysical Engineering, Montana Tech of The University of Montana, Butte, MT 59701, USA; E-Mail: [email protected] (X.Z.) 2 Department of Civil, Environmental, and Construction Engineering, University of Central Florida, 4000 Central Florida Blvd.; Orlando, FL 32816, USA; E-Mail: [email protected] (N.B.C.) 3 Geophysical Institute, University of Alaska Fairbanks, 903 Koyukuk Drive, P.O. Box 757320, Fairbanks, AK 99775-7320, USA; E-Mail: [email protected] (S.L.) * Author to whom correspondence should be addressed; E-Mail: [email protected] (X.Z.); Tel.: +1-406-496-4350; Fax: +1-406-496-4704 Received: 23 September 2008; in revised version: 10 December 2008 / Accepted: 12 March 2009 / Published: 13 March 2009 Abstract: This paper provides a review of the progress in regard to the InSAR remote sensing technique and its applications in earth and environmental sciences, especially in the past decade. Basic principles, factors, limits, InSAR sensors, available software packages for the generation of InSAR interferograms were summarized to support future applications. Emphasis was placed on the applications of InSAR in seismology, volcanology, land subsidence/uplift, landslide, glaciology, hydrology, and forestry sciences. It ends with a discussion of future research directions. Keywords: InSAR, phase, interferogram, deformation, remote sensing. 1. InSAR Overview of InSAR 1.1. Introduction Interferometric synthetic aperture radar (InSAR) is a rapidly evolving remote sensing technology that directly measures the phase change between two phase measurements of the same ground pixel of Sensors 2009, 9 1877 the Earth’s surface. -
A Comprehensive Analysis of the Illapel 2015 Mw8.3 Earthquake from GPS and Insar Data
A comprehensive analysis of the Illapel 2015 Mw8.3 Earthquake from GPS and InSAR data Emilie Klein, Christophe Vigny, Luce Fleitout, Raphael Grandin, Romain Jolivet, Efrain Rivera, Marianne Métois To cite this version: Emilie Klein, Christophe Vigny, Luce Fleitout, Raphael Grandin, Romain Jolivet, et al.. A comprehen- sive analysis of the Illapel 2015 Mw8.3 Earthquake from GPS and InSAR data. 2017. hal-01502179 HAL Id: hal-01502179 https://hal.archives-ouvertes.fr/hal-01502179 Preprint submitted on 5 Apr 2017 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. Distributed under a Creative Commons Attribution - NonCommercial - ShareAlike| 4.0 International License A comprehensive analysis of the Illapel 2015 Mw 8.3 Earthquake from GPS and InSAR data. (1)(2) (1) (1) (3) (1) (4) (5) Klein, E. , Vigny, C. , Fleitout, L. , Grandin, R. , Jolivet, R. , Rivera, E. , Métois, M. Affiliations : (1) Laboratoire de géologie, Département de Géosciences, ENS, CNRS, UMR8538, PSL research University, Paris, France (2) now at Institut de Physique du Globe de Strasbourg, -
2017 Valparaíso Earthquake Sequence and the Megathrust Patchwork of Central Chile
PUBLICATIONS Geophysical Research Letters RESEARCH LETTER 2017 Valparaíso earthquake sequence and the megathrust 10.1002/2017GL074767 patchwork of central Chile Key Points: Jennifer L. Nealy1 , Matthew W. Herman2 , Ginevra L. Moore1 , Gavin P. Hayes1 , • The 2017 Valparaíso sequence 1 3 4 occurred between the two main Harley M. Benz , Eric A. Bergman , and Sergio E. Barrientos patches of moment release from the 1 2 1985 Valparaíso earthquake National Earthquake Information Center, U.S. Geological Survey, Golden, Colorado, USA, Department of Geosciences, 3 • A large gap in historic ruptures south Pennsylvania State University, University Park, Pennsylvania, USA, Global Seismological Services, Golden, Colorado, USA, of the 2017 sequence, suggests a 4Centro Sismologico Nacional, Universidad de Chile, Santiago, Chile potential for great-sized earthquakes here in the near future • Low resolution in geodetic coupling to Abstract In April 2017, a sequence of earthquakes offshore Valparaíso, Chile, raised concerns of a the south of the 2017 sequence denotes the need for seafloor potential megathrust earthquake in the near future. The largest event in the 2017 sequence was a M6.9 on geodetic monitoring in subduction 24 April, seemingly colocated with the last great-sized earthquake in the region—a M8.0 in March 1985. The zones history of large earthquakes in this region shows significant variation in rupture size and extent, typically highlighted by a juxtaposition of large ruptures interspersed with smaller magnitude sequences. We show Supporting Information: that the 2017 sequence ruptured an area between the two main slip patches during the 1985 earthquake, • Supporting Information S1 rerupturing a patch that had previously slipped during the October 1973 M6.5 earthquake sequence.