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Index Abulfeda crater chain (Moon), 97 Aphrodite Terra (Venus), 142, 143, 144, 145, 146 Acheron Fossae (Mars), 165 Apohele asteroids, 353–354 Achilles asteroids, 351 Apollinaris Patera (Mars), 168 achondrite meteorites, 360 Apollo asteroids, 346, 353, 354, 361, 371 Acidalia Planitia (Mars), 164 Apollo program, 86, 96, 97, 101, 102, 108–109, 110, 361 Adams, John Couch, 298 Apollo 8, 96 Adonis, 371 Apollo 11, 94, 110 Adrastea, 238, 241 Apollo 12, 96, 110 Aegaeon, 263 Apollo 14, 93, 110 Africa, 63, 73, 143 Apollo 15, 100, 103, 104, 110 Akatsuki spacecraft (see Venus Climate Orbiter) Apollo 16, 59, 96, 102, 103, 110 Akna Montes (Venus), 142 Apollo 17, 95, 99, 100, 102, 103, 110 Alabama, 62 Apollodorus crater (Mercury), 127 Alba Patera (Mars), 167 Apollo Lunar Surface Experiments Package (ALSEP), 110 Aldrin, Edwin (Buzz), 94 Apophis, 354, 355 Alexandria, 69 Appalachian mountains (Earth), 74, 270 Alfvén, Hannes, 35 Aqua, 56 Alfvén waves, 35–36, 43, 49 Arabia Terra (Mars), 177, 191, 200 Algeria, 358 arachnoids (see Venus) ALH 84001, 201, 204–205 Archimedes crater (Moon), 93, 106 Allan Hills, 109, 201 Arctic, 62, 67, 84, 186, 229 Allende meteorite, 359, 360 Arden Corona (Miranda), 291 Allen Telescope Array, 409 Arecibo Observatory, 114, 144, 341, 379, 380, 408, 409 Alpha Regio (Venus), 144, 148, 149 Ares Vallis (Mars), 179, 180, 199 Alphonsus crater (Moon), 99, 102 Argentina, 408 Alps (Moon), 93 Argyre Basin (Mars), 161, 162, 163, 166, 186 Amalthea, 236–237, 238, 239, 241 Ariadaeus Rille (Moon), 100, 102 Amazonis Planitia (Mars), 161 COPYRIGHTED -
El Espanol Y El Japones
神戸市外国語大学 学術情報リポジトリ El espanol y el japones タイトル(その他言語 イスパニア語と日本語 ) 著者 福嶌 教隆 journal or Monograph series in Foreign studies publication title number 53 page range 1-188 year 2014-03-01 URL http://id.nii.ac.jp/1085/00001678/ Creative Commons : 表示 - 非営利 - 改変禁止 http://creativecommons.org/licenses/by-nc-nd/3.0/deed.ja 1 NORITAKA FUKUSHIMA EL ESPAÑOL Y EL JAPONÉS Universidad de Estudios Extrranjeros de Kobe Kobe, Japón 2014 1 2 PUBLICACIÓN: marzo de 2014 TÍTULO: El español y el japonés (Tomo LIII de la Serie monográfica en Estudios Extranjeros) AUTOR: Noritaka FUKUSHIMA Publicado por el Instituto de Investigación de la Universidad de Estudios Extranjeros de Kobe. Gakuen-Higashi-machi 9-1, Nishi-ku, Kobe (651-2187), Japón. http://www.kobe-cufs.ac.jp/ ISSN: 1345-8604 2 Índice 3 ÍNDICE Índice ------------------------------------------------------------------------------------------ 3 Prólogo ---------------------------------------------------------------------------------------- 6 Primera parte. El modo y la modalidad ----------------------------------------------- 9 Capítulo 1 La órbita de los estudios contrastivos sobre la modalidad en español y japonés ----------------------------------------------------------------------- 10 1.1. Introducción ------------------------------------------------------------------------ 10 1.2. Estudios del “chinjutsu” y la modalidad del japonés -------------------------- 11 1.3. Estudios sobre la modalidad en español y a nivel universal ----------------- 14 1.4. Estudios contrastivos I. Aproximación directa --------------------------------- -
Bright Peaks, Dark Shadows 20 February 2012, by Jason Major
Bright peaks, dark shadows 20 February 2012, by Jason Major Amaral's "blue" peaks seen in a color-enhanced global image acquired Jan. 14, 2008. Its central peaks also attracted astronomers' MESSENGER image of Mercury's Amaral crater interest, as they were seen to possess a striking blue hue in color-enhanced images that likely indicates rocks with different composition from the surrounding surface. The 68-mile (109-km) -wide Amaral crater on Mercury reveals its brightly-tipped central peaks in Amaral's peaks resemble those of the slightly larger this image, acquired by NASA's MESSENGER crater Eminescu, which is now known to contain spacecraft on Feb. 4, 2012. Long shadows are recently-discovered features called hollows. It's not cast by the crater's peaks and rugged rim (north is yet known if Amaral also contains hollows, but it's to the left.) suspected that they may be present on the tips of the peaks. The image was acquired as a high-resolution targeted observation with MESSENGER's Narrow- The crater is named after Brazilian artist Tarsila do Angle Camera (NAC) on its Mercury Dual Imaging Amaral. She lived from 1886 to 1973 and is System (MDIS). considered to be one of the leading Latin American modernist painters. Amaral's bright peaks were first spotted during MESSENGER's first flyby of Mercury in Jan. 2008. With a smooth floor, visible ejecta and small Source: Universe Today secondary craters, Amaral appeared noticeably younger than the heavily cratered surface around it. 1 / 2 APA citation: Bright peaks, dark shadows (2012, February 20) retrieved 26 September 2021 from https://phys.org/news/2012-02-bright-peaks-dark-shadows.html This document is subject to copyright. -
Evidence for Thermal-Stress-Induced Rockfalls on Mars Impact Crater Slopes
Icarus 342 (2020) 113503 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Evidence for thermal-stress-induced rockfalls on Mars impact crater slopes P.-A. Tesson a,b,*, S.J. Conway b, N. Mangold b, J. Ciazela a, S.R. Lewis c, D. M�ege a a Space Research Centre, Polish Academy of Science, Wrocław, Poland b Laboratoire de Plan�etologie et G�eodynamique UMR 6112, CNRS, Nantes, France c School of Physical Sciences, The Open University, Walton Hall, Milton Keynes MK7 6AA, UK ARTICLE INFO ABSTRACT Keywords: Here we study rocks falling from exposed outcrops of bedrock, which have left tracks on the slope over which Mars, surface they have bounced and/or rolled, in fresh impact craters (1–10 km in diameter) on Mars. The presence of these Thermal stress tracks shows that these rocks have fallen relatively recently because aeolian processes are known to infill Ices topographic lows over time. Mapping of rockfall tracks indicate trends in frequency with orientation, which in Solar radiation � � turn depend on the latitudinal position of the crater. Craters in the equatorial belt (between 15 N and 15 S) Weathering exhibit higher frequencies of rockfall on their north-south oriented slopes compared to their east-west ones. � Craters >15 N/S have notably higher frequencies on their equator-facing slopes as opposed to the other ori entations. We computed solar radiation on the surface of crater slopes to compare insolation patterns with the spatial distribution of rockfalls, and found statistically significant correlations between maximum diurnal inso lation and rockfall frequency. -
Extraordinary Rocks from the Peak Ring of the Chicxulub Impact Crater: P-Wave Velocity, Density, and Porosity Measurements from IODP/ICDP Expedition 364 ∗ G.L
Earth and Planetary Science Letters 495 (2018) 1–11 Contents lists available at ScienceDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl Extraordinary rocks from the peak ring of the Chicxulub impact crater: P-wave velocity, density, and porosity measurements from IODP/ICDP Expedition 364 ∗ G.L. Christeson a, , S.P.S. Gulick a,b, J.V. Morgan c, C. Gebhardt d, D.A. Kring e, E. Le Ber f, J. Lofi g, C. Nixon h, M. Poelchau i, A.S.P. Rae c, M. Rebolledo-Vieyra j, U. Riller k, D.R. Schmitt h,1, A. Wittmann l, T.J. Bralower m, E. Chenot n, P. Claeys o, C.S. Cockell p, M.J.L. Coolen q, L. Ferrière r, S. Green s, K. Goto t, H. Jones m, C.M. Lowery a, C. Mellett u, R. Ocampo-Torres v, L. Perez-Cruz w, A.E. Pickersgill x,y, C. Rasmussen z,2, H. Sato aa,3, J. Smit ab, S.M. Tikoo ac, N. Tomioka ad, J. Urrutia-Fucugauchi w, M.T. Whalen ae, L. Xiao af, K.E. Yamaguchi ag,ah a University of Texas Institute for Geophysics, Jackson School of Geosciences, Austin, USA b Department of Geological Sciences, Jackson School of Geosciences, Austin, USA c Department of Earth Science and Engineering, Imperial College, London, UK d Alfred Wegener Institute Helmholtz Centre of Polar and Marine Research, Bremerhaven, Germany e Lunar and Planetary Institute, Houston, USA f Department of Geology, University of Leicester, UK g Géosciences Montpellier, Université de Montpellier, France h Department of Physics, University of Alberta, Canada i Department of Geology, University of Freiburg, Germany j SM 312, Mza 7, Chipre 5, Resid. -
Shallow Crustal Composition of Mercury As Revealed by Spectral Properties and Geological Units of Two Impact Craters
Planetary and Space Science 119 (2015) 250–263 Contents lists available at ScienceDirect Planetary and Space Science journal homepage: www.elsevier.com/locate/pss Shallow crustal composition of Mercury as revealed by spectral properties and geological units of two impact craters Piero D’Incecco a,n, Jörn Helbert a, Mario D’Amore a, Alessandro Maturilli a, James W. Head b, Rachel L. Klima c, Noam R. Izenberg c, William E. McClintock d, Harald Hiesinger e, Sabrina Ferrari a a Institute of Planetary Research, German Aerospace Center, Rutherfordstrasse 2, D-12489 Berlin, Germany b Department of Geological Sciences, Brown University, Providence, RI 02912, USA c The Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA d Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO 80303, USA e Westfälische Wilhelms-Universität Münster, Institut für Planetologie, Wilhelm-Klemm Str. 10, D-48149 Münster, Germany article info abstract Article history: We have performed a combined geological and spectral analysis of two impact craters on Mercury: the Received 5 March 2015 15 km diameter Waters crater (106°W; 9°S) and the 62.3 km diameter Kuiper crater (30°W; 11°S). Using Received in revised form the Mercury Dual Imaging System (MDIS) Narrow Angle Camera (NAC) dataset we defined and mapped 9 October 2015 several units for each crater and for an external reference area far from any impact related deposits. For Accepted 12 October 2015 each of these units we extracted all spectra from the MESSENGER Atmosphere and Surface Composition Available online 24 October 2015 Spectrometer (MASCS) Visible-InfraRed Spectrograph (VIRS) applying a first order photometric correc- Keywords: tion. -
Democratic Citizenship in the Heart of Empire Dissertation Presented In
POLITICAL ECONOMY OF AMERICAN EDUCATION: Democratic Citizenship in the Heart of Empire Dissertation Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of the Ohio State University Thomas Michael Falk B.A., M.A. Graduate Program in Education The Ohio State University Summer, 2012 Committee Members: Bryan Warnick (Chair), Phil Smith, Ann Allen Copyright by Thomas Michael Falk 2012 ABSTRACT Chief among the goals of American education is the cultivation of democratic citizens. Contrary to State catechism delivered through our schools, America was not born a democracy; rather it emerged as a republic with a distinct bias against democracy. Nonetheless we inherit a great demotic heritage. Abolition, the labor struggle, women’s suffrage, and Civil Rights, for example, struck mighty blows against the established political and economic power of the State. State political economies, whether capitalist, socialist, or communist, each express characteristics of a slave society. All feature oppression, exploitation, starvation, and destitution as constitutive elements. In order to survive in our capitalist society, the average person must sell the contents of her life in exchange for a wage. Fundamentally, I challenge the equation of State schooling with public and/or democratic education. Our schools have not historically belonged to a democratic public. Rather, they have been created, funded, and managed by an elite class wielding local, state, and federal government as its executive arms. Schools are economic institutions, serving a division of labor in the reproduction of the larger economy. Rather than the school, our workplaces are the chief educational institutions of our lives. -
Regional Oral History Off Ice University of California the Bancroft Library Berkeley, California
Regional Oral History Off ice University of California The Bancroft Library Berkeley, California Richard B. Gump COMPOSER, ARTIST, AND PRESIDENT OF GUMP'S, SAN FRANCISCO An Interview Conducted by Suzanne B. Riess in 1987 Copyright @ 1989 by The Regents of the University of California Since 1954 the Regional Oral History Office has been interviewing leading participants in or well-placed witnesses to major events in the development of Northern California, the West,and the Nation. Oral history is a modern research technique involving an interviewee and an informed interviewer in spontaneous conversation. The taped record is transcribed, lightly edited for continuity and clarity, and reviewed by the interviewee. The resulting manuscript is typed in final form, indexed, bound with photographs and illustrative materials, and placed in The Bancroft Library at the University of California, Berkeley, and other research collections for scholarly use. Because it is primary material, oral history is not intended to present the final, verified, or complete narrative of events. It is a spoken account, offered by the interviewee in response to questioning, and as such it is reflective, partisan, deeply involved, and irreplaceable. All uses of this manuscript are covered by a legal agreement between the University of California and Richard B. Gump dated 7 March 1988. The manuscript is thereby made available for research purposes. All literary rights in the manuscript, including the right to publish, are reserved to The Bancroft Library of the University of California, Berkeley. No part of the manuscript may be quoted for publication without the written permission of the Director of The Bancroft Library of the University of California, Berkeley. -
Active Applicant Report Type Status Applicant Name
Active Applicant Report Type Status Applicant Name Gaming PENDING ABAH, TYRONE ABULENCIA, JOHN AGUDELO, ROBERT JR ALAMRI, HASSAN ALFONSO-ZEA, CRISTINA ALLEN, BRIAN ALTMAN, JONATHAN AMBROSE, DEZARAE AMOROSE, CHRISTINE ARROYO, BENJAMIN ASHLEY, BRANDY BAILEY, SHANAKAY BAINBRIDGE, TASHA BAKER, GAUDY BANH, JOHN BARBER, GAVIN BARRETO, JESSE BECKEY, TORI BEHANNA, AMANDA BELL, JILL 10/1/2021 7:00:09 AM Gaming PENDING BENEDICT, FREDRIC BERNSTEIN, KENNETH BIELAK, BETHANY BIRON, WILLIAM BOHANNON, JOSEPH BOLLEN, JUSTIN BORDEWICZ, TIMOTHY BRADDOCK, ALEX BRADLEY, BRANDON BRATETICH, JASON BRATTON, TERENCE BRAUNING, RICK BREEN, MICHELLE BRIGNONI, KARLI BROOKS, KRISTIAN BROWN, LANCE BROZEK, MICHAEL BRUNN, STEVEN BUCHANAN, DARRELL BUCKLEY, FRANCIS BUCKNER, DARLENE BURNHAM, CHAD BUTLER, MALKAI 10/1/2021 7:00:09 AM Gaming PENDING BYRD, AARON CABONILAS, ANGELINA CADE, ROBERT JR CAMPBELL, TAPAENGA CANO, LUIS CARABALLO, EMELISA CARDILLO, THOMAS CARLIN, LUKE CARRILLO OLIVA, GERBERTH CEDENO, ALBERTO CENTAURI, RANDALL CHAPMAN, ERIC CHARLES, PHILIP CHARLTON, MALIK CHOATE, JAMES CHURCH, CHRISTOPHER CLARKE, CLAUDIO CLOWNEY, RAMEAN COLLINS, ARMONI CONKLIN, BARRY CONKLIN, QIANG CONNELL, SHAUN COPELAND, DAVID 10/1/2021 7:00:09 AM Gaming PENDING COPSEY, RAYMOND CORREA, FAUSTINO JR COURSEY, MIAJA COX, ANTHONIE CROMWELL, GRETA CUAJUNO, GABRIEL CULLOM, JOANNA CUTHBERT, JENNIFER CYRIL, TWINKLE DALY, CADEJAH DASILVA, DENNIS DAUBERT, CANDACE DAVIES, JOEL JR DAVILA, KHADIJAH DAVIS, ROBERT DEES, I-QURAN DELPRETE, PAUL DENNIS, BRENDA DEPALMA, ANGELINA DERK, ERIC DEVER, BARBARA -
Producing MIDS NAC Dems from MESSENGER Images
Producing MESSENGER DEMs from MDIS NAC Images MANHEIM1, HENRIKSEN, ROBINSON, AND THE MESSENGER TEAM 1ARIZONA STATE UNIVERSITY, TEMPE AZ—[email protected] Launched: August 2004 MESSENGER Mercury Orbit: March 2011 Completed: April 2015 Mercury Dual Imaging System (MDIS) 2 framing cameras: a monochrome NAC and a multispectral WAC NAC wasn’t a stereo camera, but off-nadir observations enable the creation of DEMs NACs have 5 m pixel scale at closest approach Mercury Laser Altimeter (MLA) Radial accuracy of < 20 m Only available between 90° N and 18° S Highly Elliptical Orbit Periapsis: 200 – 500 km (near North Pole) Apoapsis: 10,000 – 15,000 km Methodology: Overview Site Selection & Image Selection Illumination Conditions Imaging Geometry DEM Production Using the USGS Integrated Software for Imagers and Spectrometers (ISIS) and SOCET SET 5.6 Error analysis Creating data products for PDS release Image Selection Selecting stereo images requires compromise between finding optimal images and building up desired coverage. These parameters will dictate the precision of the final product. Strength of stereo: parallax between the two images / unit height Illumination compatibility: distance between the tips of shadows in two images / unit height *Guidelines adapted from Becker, et al. 2015. Images Selected for Our DEMs n=49 Selecting Images to Build Mosaics Sander Crater mosaic: 21 images Selecting Images to Build Mosaics Sander Crater mosaic: 21 images 36 stereo pairs (areas of overlap producing ‘good’ stereo) Selecting Images to Build Mosaics Sander Crater mosaic: 21 images 36 stereo pairs (areas of overlap producing ‘good’ stereo) Resulting DEMs can be mosaicked together (using ISIS) to create one large-area DEM Processing in SOCET SET: Overview Import into SOCET SET 5.6 Relative Triangulation Registration to MLA tracks DEM Extraction Orthophoto Generation Creating Additional Data Products PDS Release *This process is quite similar to that described for LROC NAC DEMs in Henriksen, et al. -
Packet 12 (1).Pdf
The 2018 Scottie Written and edited by current and former players and coaches including Todd Garrison, Tyler Reid, Olivia Kiser, Anish Patel, Rajeev Nair, Garrison Page, Mason Reid, Parker Bannister, Daniel Dill. Packet Twelve TOSSUPS 1. This mountain has two summits, of which the South summit is approximately 1100 feet higher. The Kahiltna Glacier comes off the southwest side of this mountain, which is named after a Koyukon word meaning ‘high’ or ‘tall’. It was renamed in the lead up to the (*) 1896 presidential election, and retained that name until 2015. For 10 points, name this mountain, which was named Mount McKinley for 119 years before having its original name restored. (OK) ANSWER: Denali [accept Mount McKinley before mention] 2. One work by this non-Ovid poet that was written under the patronage of Maecenas is about the running of a farm and devotes an entire book to bees. Another work by this poet largely consists of pastoral themes, and is sometimes considered to include a reference to Jesus. This author’s most famous work traces the journey of a (*) Trojan warrior to Italy via Carthage. For 10 points, name this Roman poet of the Georgics, the Eclogues, and The Aeneid. (OK) ANSWER: Virgil [ or Publius Vergilius Maro] 3. One event taking place on this holiday is a drawing of lots where one goat is sacrificed and another is sent “to Azazel.” On the day before it, some practitioners swing a chicken over a person’s head in the kapparot ritual. This holiday ends with a long blast of the shofar in the Ne’ila prayer, and during it five (*) prohibitions are observed. -
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,