Attachment C

Total Page:16

File Type:pdf, Size:1020Kb

Attachment C CASSINI FINAL MISSION REPORT 2019 i DISCLAIMER The Cassini Science Bibliographies is not exhaustive and complete. For all other Cassini related references refer to: Attachment B – References & Bibliographies; the sections entitled References contributed by individual Cassini instrument and discipline teams located in Volume 1 Sections 3.1 and 3.2 Science Results; and other resources outside of the Cassini Final Mission Report. CASSINI FINAL MISSION REPORT 2019 iii CONTENTS DISCLAIMER ..................................................................................................................................................................... I REFERENCES ................................................................................................................................................................. 1 FROM 2014 CASSINI SENIOR REVIEW ..................................................................................................................... 116 Cassini Ground-Breaking Science Publications ................................................................................................. 116 Cassini Special Journal Issues and Books ......................................................................................................... 125 Cassini Special Journal Issues .............................................................................................................. 125 Cassini-related Popular Science Print Publications....................................................................... 125 Peer-Reviewed Journals: Special Cassini-related Issues ............................................................. 128 Cassini Books ........................................................................................................................................ 146 Saturn from Cassini-Huygens (M. K. Dougherty, L. W. Esposito, S. K. Krimigis, eds.) ................. 146 Titan from Cassini-Huygens (R. H. Brown, J.-P. Lebreton, J. H. Waite, eds.) .............................. 148 Planetary Rings: A Post-Equinox View (L. W. Esposito) ............................................................... 150 Titan: Interior, Surface, Atmosphere and Space Environment (I. Mueller-Wodarg, C. A. Griffith, E. Lellouch, T. E. Cravens, eds.) ....................................................................................................... 151 Publications from the Cassini Team ................................................................................................................... 153 Publications from Outside the Team .................................................................................................................. 262 Cassini Education and Public Outreach ............................................................................................................. 379 Formal Education .................................................................................................................................. 379 Informal Education ................................................................................................................................ 379 Reaching Underserved Schools ............................................................................................................ 380 Public Outreach: NASA Data Shared with the Public ............................................................................ 380 Other Notable Programs ....................................................................................................................... 381 Products Rated as Outstanding from the NASA Education Review Residing on the NASA Education Portal ..................................................................................................................................... 383 REFERENCES ADDED – JUNE 2018 THROUGH JULY 2019.................................................................................... 384 CASSINI FINAL MISSION REPORT 2019 1 REFERENCES Abbott, A. (2005), Titan team claims just deserts as probe hits moon of creme brulee, Nature, 433. doi: 10.1038/433181a. Achilleos, N., Andr, N., Blanco-Cano, X., Brandt, P. C., Delamere, P. A., and Winglee, R. (2015), 1. Transport of Mass, Momentum and Energy in Planetary Magnetodisc Regions, Space Science Reviews, 187(1-4), 229-299. doi: 10.1007/s11214-014-0086-y. Achilleos, N., Arridge, C. S., Bertucci, C., Guio, P., Romanelli, N., and Sergis, N. (2014), A combined model of pressure variations in Titan's plasma environment, Geophysical Research Letters, 41(24), 8730-8735. doi: 10.1002/2014GL061747. Achterberg R. K., B. J. Conrath, P. J. Gierasch, F. M. Flasar, C. A. Nixon. Titan’s middle- atmospheric temperatures and dynamics observed by the Cassini Composite Infrared Spectrometer. Icarus, vol. 194, pp. 263–277, 2008. Achterberg, R. K., Gierasch, P. J., Conrath, B. J., Fletcher, L. N., Hesman, B. E., Bjoraker, G. L., and Flasar, F. M. (2014), Changes to Saturn's Zonal-mean Tropospheric Thermal Structure after the 2010-2011 Northern Hemisphere Storm, The Astrophysical Journal, 786(2), 92. doi: 10.1088/0004-637X/786/2/92. Adamkovics, M., Wong, M. H., Laver, C., and Pater, I. d. (2007), Widespread morning drizzle on titan, Science, 318. Adams, E. Y. (2006), Titan's thermal structure and the formation of a nitrogen atmosphere, Ph.D. http://adsabs.harvard.edu/abs/2006PhDT........17A. Adriani, A., Moriconi, M. L., D'Aversa, E., Oliva, F., and Filacchione, G. (2015), Faint Luminescent Ring Over Saturn's Polar Hexagon, Astrophysical Journal Letters, 808(1), L16. doi: 10.1088/2041-8205/808/1/l16. Aharonson, O., A. G. Hayes, J. I., Lunine, R. D. Lorenz, M. D. Allison, and C. Elachi. An asymmetric distribution of lakes on Titan as a possible consequence of orbital forcing. Nature Geoscience, vol. 2, pp. 851–854, 2009. Ainslie, M. A., and Leighton, T. G. (2016), Sonar equations for planetary exploration, Journal of the Acoustical Society of America, 140(2), 1400-1419. doi: 10.1121/1.4960786. Ajello, J. M., Aguilar, A., Mangina, R. S., James, G. K., Geissler, P., and Trafton, L. (2008), Middle UV to near-IR spectrum of electron-excited SO2, Journal of Geophysical Research- Planets, 113. http:\\hdl.handle.net\2014/40896. Ajello, J. M., Mangina, R. S., Strickland, D. J., and Dziczek, D. (2011), Laboratory studies of UV emissions from proton impact on N-2: The Lyman-Birge-Hopfield band system for aurora analysis, Journal of Geophysical Research-Space Physics, 116. doi: 10.1029/2010ja016103. Albers, N. (2006), On the Relevance of Particle Adhesion: Applications to Saturn's Rings, Ph.D. http://opus.kobv.de/ubp/volltexte/2006/1084/pdf/albers_diss.pdf. 2 CASSINI FINAL MISSION REPORT 2019 Aleshkina, E. Y. (2009), Synchronous spin-orbital resonance locking of large planetary satellites, Solar System Research, 43. doi: 10.1134/s0038094609010079. Ali, A., Sittler, E. C., Chornay, D., Rowe, B. R., and Puzzarini, C. (2015), Organic chemistry in Titan's upper atmosphere and its astrobiological consequences: I. Views towards Cassini plasma spectrometer (CAPS) and ion neutral mass spectrometer (INMS) experiments in space, Planetary and Space Science, 109, 46-63. doi: 10.1016/j.pss.2015.01.015. Altobelli, N., et al. (2016), Flux and composition of interstellar dust at Saturn from Cassini's Cosmic Dust Analyzer, Science, 352. doi: 10.1126/science.aac6397. Altobelli, N., Lopez-Paz, D., Pilorz, S., Spilker, L. J., Morishima, R., Brooks, S., Leyrat, C., Deau, E., Edgington, S., and Flandes, A. (2014), Two numerical models designed to reproduce Saturn ring temperatures as measured by Cassini-CIRS, Icarus, 238, 205-220. doi: 10.1016/j.icarus.2014.04.031. Altobelli, N., Spilker, L. J., and Edgington, S. G. (2017), Cassini's swan song, Nature Astronomy, 1. doi: 10.1038/s41550-017-0239-5. Anderson, C. M., and Samuelson, R. E. (2011), Titan’s aerosol and stratospheric ice opacities between 18 and 500 _m: Vertical and spectral characteristics from Cassini CIRS, Icarus, 212. doi: 10.1016/j.icarus.2011.01.024. Anderson, C. M., Samuelson, R. E., Achterberg, R. K., Barnes, J. W., and Flasar, F. M. (2014), Subsidence-induced methane clouds in Titan’s winter polar stratosphere and upper troposphere, Icarus, 243, 129-138. doi: 10.1016/j.icarus.2014.09.007. Anderson, C. M., Samuelson, R. E., Yung, Y. L., and McLain, J. L. (2016), Solid-state photochemistry as a formation mechanism for Titan's stratospheric C4N2 ice clouds, Geophysical Research Letters, 43(7), 3088-3094. doi: 10.1002/2016gl067795. Andrews, D. J., A. J. Coates, S. W. H. Cowley, M. K. Dougherty, L. Lamy, G. Provan, and P. Zarka. Magnetospheric period oscillations at Saturn: Comparison of equatorial and high- latitude magnetic field periods with north and south SKR periods. J. Geophys. Res., vol. 115, p. A12252, doi:10.1029/2010JA015666, 2010. Andriopoulou, M., Roussos, E., Krupp, N., Paranicas, C., Thomsen, M., Krimigis, S., Dougherty, M. K., and Glassmeier, K. H. (2014), Spatial and temporal dependence of the convective electric field in Saturn's inner magnetosphere, Icarus, 229, 57-70. doi: 10.1016/j.icarus.2013.10.028. Androes, D. S. (2012), Orbital periodicities reflected in ancient surfaces of our solar system and the implications for a record of early life. Annou, K. (2015), Ion-acoustic solitons in plasma: an application to Saturn's magnetosphere, Astrophysics and Space Science, 357(2), 163. doi: 10.1007/s10509-015-2391-7. Anonymous (1996), JPL receives antenna for Cassini, Aviation Week & Space Technology, 145. Anonymous (2009), Odd tectonics on Enceladus,
Recommended publications
  • 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.
    [Show full text]
  • Lab 7: Gravity and Jupiter's Moons
    Lab 7: Gravity and Jupiter's Moons Image of Galileo Spacecraft Gravity is the force that binds all astronomical structures. Clusters of galaxies are gravitationally bound into the largest structures in the Universe, Galactic Superclusters. The galaxies themselves are held together by gravity, as are all of the star systems within them. Our own Solar System is a collection of bodies gravitationally bound to our star, Sol. Cutting edge science requires the use of Einstein's General Theory of Relativity to explain gravity. But the interactions of the bodies in our Solar System were understood long before Einstein's time. In chapter two of Chaisson McMillan's Astronomy Today, you went over Kepler's Laws. These laws of gravity were made to describe the interactions in our Solar System. P2=a3/M Where 'P' is the orbital period in Earth years, the time for the body to make one full orbit. 'a' is the length of the orbit's semi-major axis, for nearly circular orbits the orbital radius. 'M' is the total mass of the system in units of Solar Masses. Jupiter System Montage picture from NASA ID = PIA01481 Jupiter has over 60 moons at the last count, most of which are asteroids and comets captured from Written by Meagan White and Paul Lewis Page 1 the Asteroid Belt. When Galileo viewed Jupiter through his early telescope, he noticed only four moons: Io, Europa, Ganymede, and Callisto. The Jupiter System can be thought of as a miniature Solar System, with Jupiter in place of the Sun, and the Galilean moons like planets.
    [Show full text]
  • Galileo and the Telescope
    Galileo and the Telescope A Discussion of Galileo Galilei and the Beginning of Modern Observational Astronomy ___________________________ Billy Teets, Ph.D. Acting Director and Outreach Astronomer, Vanderbilt University Dyer Observatory Tuesday, October 20, 2020 Image Credit: Giuseppe Bertini General Outline • Telescopes/Galileo’s Telescopes • Observations of the Moon • Observations of Jupiter • Observations of Other Planets • The Milky Way • Sunspots Brief History of the Telescope – Hans Lippershey • Dutch Spectacle Maker • Invention credited to Hans Lippershey (c. 1608 - refracting telescope) • Late 1608 – Dutch gov’t: “ a device by means of which all things at a very great distance can be seen as if they were nearby” • Is said he observed two children playing with lenses • Patent not awarded Image Source: Wikipedia Galileo and the Telescope • Created his own – 3x magnification. • Similar to what was peddled in Europe. • Learned magnification depended on the ratio of lens focal lengths. • Had to learn to grind his own lenses. Image Source: Britannica.com Image Source: Wikipedia Refracting Telescopes Bend Light Refracting Telescopes Chromatic Aberration Chromatic aberration limits ability to distinguish details Dealing with Chromatic Aberration - Stop Down Aperture Galileo used cardboard rings to limit aperture – Results were dimmer views but less chromatic aberration Galileo and the Telescope • Created his own (3x, 8-9x, 20x, etc.) • Noted by many for its military advantages August 1609 Galileo and the Telescope • First observed the
    [Show full text]
  • Type Tourmalines from Brazil and Mozambique: Implications for Origin and Authenticity Determination
    No.9 May 2009 Chemical Variations in Multicolored “Paraíba”-Type Tourmalines from Brazil and Mozambique: Implications for Origin and Authenticity Determination “Cuprian-Elbaite”-Tourmaline from Mozambique “Paraiba”- Tourmaline from Brazil Manganese Mn Inner core Mn Bi Cu Bi Copper Chemical Variation in “Paraiba”-Tourmaline Chemical Distribution Mapping Editor Message from the Editors Desk: When Dr. A. Peretti, FGG, FGA, EurGeol trace element research matters most GRS Gemresearch Swisslab AG, P.O.Box 4028, 6002 Lucerne, Switzerland When copper bearing tourmalines were found 20 [email protected] years ago in the state of Paraíba in Brazil, they intrigued by their “neon”-blue color and soon became known as “Paraíba” tourmalines in the trade. In the Previous Journal and Movie years before and into the new Millennium, these tourmalines have emerged to become one of the most valuable and demanded gems, comparable to prestigious rubies and sapphires. In the last couple of years an unprecedented tourmaline boom has occurred due to the discovery of new copper-bearing tourmaline deposits. The name “Paraíba” tourmaline was originally associated only with those copper-bearing tourmalines (or “cuprian-elbaites”), which were found in the state of Paraíba (Brazil). New mines were subsequently encountered in Rio Grande do Norte in Brazil, as well as in Nigeria and in Mozambique. The market and the laboratories were split on the issue whether to call the newly discovered neon-blue colored tourmalines “cuprian-elbaites” or “Paraíba tourmaline” regardless of origin. While this controversy initiated the first high-profile law suite in the USA (currently dropped), the debate on Paraíba tourmalines progressed into a new direction.
    [Show full text]
  • Cassini RADAR Images at Hotei Arcus and Western Xanadu, Titan: Evidence for Geologically Recent Cryovolcanic Activity S
    GEOPHYSICAL RESEARCH LETTERS, VOL. 36, L04203, doi:10.1029/2008GL036415, 2009 Click Here for Full Article Cassini RADAR images at Hotei Arcus and western Xanadu, Titan: Evidence for geologically recent cryovolcanic activity S. D. Wall,1 R. M. Lopes,1 E. R. Stofan,2 C. A. Wood,3 J. L. Radebaugh,4 S. M. Ho¨rst,5 B. W. Stiles,1 R. M. Nelson,1 L. W. Kamp,1 M. A. Janssen,1 R. D. Lorenz,6 J. I. Lunine,5 T. G. Farr,1 G. Mitri,1 P. Paillou,7 F. Paganelli,2 and K. L. Mitchell1 Received 21 October 2008; revised 5 January 2009; accepted 8 January 2009; published 24 February 2009. [1] Images obtained by the Cassini Titan Radar Mapper retention age comparable with Earth or Venus (500 Myr) (RADAR) reveal lobate, flowlike features in the Hotei [Lorenz et al., 2007]). Arcus region that embay and cover surrounding terrains and [4] Most putative cryovolcanic features are located at mid channels. We conclude that they are cryovolcanic lava flows to high northern latitudes [Elachi et al., 2005; Lopes et al., younger than surrounding terrain, although we cannot reject 2007]. They are characterized by lobate boundaries and the sedimentary alternative. Their appearance is grossly relatively uniform radar properties, with flow features similar to another region in western Xanadu and unlike most brighter than their surroundings. Cryovolcanic flows are of the other volcanic regions on Titan. Both regions quite limited in area compared to the more extensive dune correspond to those identified by Cassini’s Visual and fields [Radebaugh et al., 2008] or lakes [Hayes et al., Infrared Mapping Spectrometer (VIMS) as having variable 2008].
    [Show full text]
  • Annual Report COOPERATIVE INSTITUTE for RESEARCH in ENVIRONMENTAL SCIENCES
    2015 Annual Report COOPERATIVE INSTITUTE FOR RESEARCH IN ENVIRONMENTAL SCIENCES COOPERATIVE INSTITUTE FOR RESEARCH IN ENVIRONMENTAL SCIENCES 2015 annual report University of Colorado Boulder UCB 216 Boulder, CO 80309-0216 COOPERATIVE INSTITUTE FOR RESEARCH IN ENVIRONMENTAL SCIENCES University of Colorado Boulder 216 UCB Boulder, CO 80309-0216 303-492-1143 [email protected] http://cires.colorado.edu CIRES Director Waleed Abdalati Annual Report Staff Katy Human, Director of Communications, Editor Susan Lynds and Karin Vergoth, Editing Robin L. Strelow, Designer Agreement No. NA12OAR4320137 Cover photo: Mt. Cook in the Southern Alps, West Coast of New Zealand’s South Island Birgit Hassler, CIRES/NOAA table of contents Executive summary & research highlights 2 project reports 82 From the Director 2 Air Quality in a Changing Climate 83 CIRES: Science in Service to Society 3 Climate Forcing, Feedbacks, and Analysis 86 This is CIRES 6 Earth System Dynamics, Variability, and Change 94 Organization 7 Management and Exploitation of Geophysical Data 105 Council of Fellows 8 Regional Sciences and Applications 115 Governance 9 Scientific Outreach and Education 117 Finance 10 Space Weather Understanding and Prediction 120 Active NOAA Awards 11 Stratospheric Processes and Trends 124 Systems and Prediction Models Development 129 People & Programs 14 CIRES Starts with People 14 Appendices 136 Fellows 15 Table of Contents 136 CIRES Centers 50 Publications by the Numbers 136 Center for Limnology 50 Publications 137 Center for Science and Technology
    [Show full text]
  • No. 40. the System of Lunar Craters, Quadrant Ii Alice P
    NO. 40. THE SYSTEM OF LUNAR CRATERS, QUADRANT II by D. W. G. ARTHUR, ALICE P. AGNIERAY, RUTH A. HORVATH ,tl l C.A. WOOD AND C. R. CHAPMAN \_9 (_ /_) March 14, 1964 ABSTRACT The designation, diameter, position, central-peak information, and state of completeness arc listed for each discernible crater in the second lunar quadrant with a diameter exceeding 3.5 km. The catalog contains more than 2,000 items and is illustrated by a map in 11 sections. his Communication is the second part of The However, since we also have suppressed many Greek System of Lunar Craters, which is a catalog in letters used by these authorities, there was need for four parts of all craters recognizable with reasonable some care in the incorporation of new letters to certainty on photographs and having diameters avoid confusion. Accordingly, the Greek letters greater than 3.5 kilometers. Thus it is a continua- added by us are always different from those that tion of Comm. LPL No. 30 of September 1963. The have been suppressed. Observers who wish may use format is the same except for some minor changes the omitted symbols of Blagg and Miiller without to improve clarity and legibility. The information in fear of ambiguity. the text of Comm. LPL No. 30 therefore applies to The photographic coverage of the second quad- this Communication also. rant is by no means uniform in quality, and certain Some of the minor changes mentioned above phases are not well represented. Thus for small cra- have been introduced because of the particular ters in certain longitudes there are no good determi- nature of the second lunar quadrant, most of which nations of the diameters, and our values are little is covered by the dark areas Mare Imbrium and better than rough estimates.
    [Show full text]
  • Book of Abstracts: Studying Old Master Paintings
    BOOK OF ABSTRACTS STUDYING OLD MASTER PAINTINGS ­ TECHNOLOGY AND PRACTICE THE NATIONAL GALLERY TECHNICAL BULLETIN 30TH ANNIVERSARY CONFERENCE 16­18 September 2009, Sainsbury Wing Theatre, National Gallery, London Supported by The Elizabeth Cayzer Charitable Trust STUDYING OLD MASTER PAINTINGS ­ TECHNOLOGY AND PRACTICE THE NATIONAL GALLERY TECHNICAL BULLETIN 30TH ANNIVERSARY CONFERENCE BOOK OF ABSTRACTS 16­18 September 2009 Sainsbury Wing Theatre, National Gallery, London The Proceedings of this Conference will be published by Archetype Publications, London in 2010 Contents Presentations Page Presentations (cont’d) Page The Paliotto by Guido da Siena from the Pinacoteca Nazionale of Siena 3 The rediscovery of sublimated arsenic sulphide pigments in painting 25 Marco Ciatti, Roberto Bellucci, Cecilia Frosinini, Linda Lucarelli, Luciano Sostegni, and polychromy: Applications of Raman microspectroscopy Camilla Fracassi, Carlo Lalli Günter Grundmann, Natalia Ivleva, Mark Richter, Heike Stege, Christoph Haisch Painting on parchment and panels: An exploration of Pacino di 5 The use of blue and green verditer in green colours in seventeenth­century 27 Bonaguida’s technique Netherlandish painting practice Carole Namowicz, Catherine M. Schmidt, Christine Sciacca, Yvonne Szafran, Annelies van Loon, Lidwein Speleers Karen Trentelman, Nancy Turner Alterations in paintings: From non­invasive in­situ assessment to 29 Technical similarities between mural painting and panel painting in 7 laboratory research the works of Giovanni da Milano: The Rinuccini
    [Show full text]
  • General Index
    General Index Italicized page numbers indicate figures and tables. Color plates are in- cussed; full listings of authors’ works as cited in this volume may be dicated as “pl.” Color plates 1– 40 are in part 1 and plates 41–80 are found in the bibliographical index. in part 2. Authors are listed only when their ideas or works are dis- Aa, Pieter van der (1659–1733), 1338 of military cartography, 971 934 –39; Genoa, 864 –65; Low Coun- Aa River, pl.61, 1523 of nautical charts, 1069, 1424 tries, 1257 Aachen, 1241 printing’s impact on, 607–8 of Dutch hamlets, 1264 Abate, Agostino, 857–58, 864 –65 role of sources in, 66 –67 ecclesiastical subdivisions in, 1090, 1091 Abbeys. See also Cartularies; Monasteries of Russian maps, 1873 of forests, 50 maps: property, 50–51; water system, 43 standards of, 7 German maps in context of, 1224, 1225 plans: juridical uses of, pl.61, 1523–24, studies of, 505–8, 1258 n.53 map consciousness in, 636, 661–62 1525; Wildmore Fen (in psalter), 43– 44 of surveys, 505–8, 708, 1435–36 maps in: cadastral (See Cadastral maps); Abbreviations, 1897, 1899 of town models, 489 central Italy, 909–15; characteristics of, Abreu, Lisuarte de, 1019 Acequia Imperial de Aragón, 507 874 –75, 880 –82; coloring of, 1499, Abruzzi River, 547, 570 Acerra, 951 1588; East-Central Europe, 1806, 1808; Absolutism, 831, 833, 835–36 Ackerman, James S., 427 n.2 England, 50 –51, 1595, 1599, 1603, See also Sovereigns and monarchs Aconcio, Jacopo (d. 1566), 1611 1615, 1629, 1720; France, 1497–1500, Abstraction Acosta, José de (1539–1600), 1235 1501; humanism linked to, 909–10; in- in bird’s-eye views, 688 Acquaviva, Andrea Matteo (d.
    [Show full text]
  • Workshop on Lunar Volcanic Glasses: Scientific and Resource Potential
    WORKSHOP ON LUNAR VOLCANIC GLASSES: SCIENTIFIC AND RESOURCE POTENTIAL t)--- LPI Technical Report Number 90~02 .. LUNAR AND PLANETARY INSTITUTE 3303 NASA ROAD 1 HOUSTON, TEXAS 77058-4399 WORKSHOP ON LUNAR VOLCANIC GLASSES: SCIENTIFIC AND RESOlTRCE POTENTIAL Edited by John W. Delano and Grant H. Heiken Held at Lunar and Planetary Institute Houston, Texas October 10 - 11, 1989 Sponsored by Lunar and Planetary Institute Lunar and Planetary Sample Team Lunar and Planetary Institute 3303 NASA Road 1 Houston, Texas 77058-4399 LPI Technical Report Number 90-02 Compiled in 1990 by the LUNAR AND PLANETARY INSTITUTE The Institute is operated by Universities Space Research Association under Contract NASW-4066 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: Delano J. W. and Heiken G. H., eds. (1990) Workshop on Lunar Volcanic Glasses: Scientific alld Resource Potelltial. LPI Tech. Rpt. 90-02. Lunar and Planetary Institute, Houston. 74 pp. Papers in this report may be cited as: Author A. A. (1990) Title of paper. In Workshop Oil Lunar Volcanic Glasses: Scientific alld Resource Potelltial (J. W. Delano and G. H. Heiken, eds.), pp. xx-yy. LPI Tech. Rpt. 90-02. Lunar and Planetary Institute, Houston. This report is distributed by: ORDER DEPARTMENT Lunar and Planetary Institute 3303 NASA Road 1 Houston, TX 77058-4399 Mail order requestors will be ill voiced for the cost ofshippillg and halldling.
    [Show full text]
  • 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.
    [Show full text]
  • CALIFORNIA's NORTH COAST: a Literary Watershed: Charting the Publications of the Region's Small Presses and Regional Authors
    CALIFORNIA'S NORTH COAST: A Literary Watershed: Charting the Publications of the Region's Small Presses and Regional Authors. A Geographically Arranged Bibliography focused on the Regional Small Presses and Local Authors of the North Coast of California. First Edition, 2010. John Sherlock Rare Books and Special Collections Librarian University of California, Davis. 1 Table of Contents I. NORTH COAST PRESSES. pp. 3 - 90 DEL NORTE COUNTY. CITIES: Crescent City. HUMBOLDT COUNTY. CITIES: Arcata, Bayside, Blue Lake, Carlotta, Cutten, Eureka, Fortuna, Garberville Hoopa, Hydesville, Korbel, McKinleyville, Miranda, Myers Flat., Orick, Petrolia, Redway, Trinidad, Whitethorn. TRINITY COUNTY CITIES: Junction City, Weaverville LAKE COUNTY CITIES: Clearlake, Clearlake Park, Cobb, Kelseyville, Lakeport, Lower Lake, Middleton, Upper Lake, Wilbur Springs MENDOCINO COUNTY CITIES: Albion, Boonville, Calpella, Caspar, Comptche, Covelo, Elk, Fort Bragg, Gualala, Little River, Mendocino, Navarro, Philo, Point Arena, Talmage, Ukiah, Westport, Willits SONOMA COUNTY. CITIES: Bodega Bay, Boyes Hot Springs, Cazadero, Cloverdale, Cotati, Forestville Geyserville, Glen Ellen, Graton, Guerneville, Healdsburg, Kenwood, Korbel, Monte Rio, Penngrove, Petaluma, Rohnert Part, Santa Rosa, Sebastopol, Sonoma Vineburg NAPA COUNTY CITIES: Angwin, Calistoga, Deer Park, Rutherford, St. Helena, Yountville MARIN COUNTY. CITIES: Belvedere, Bolinas, Corte Madera, Fairfax, Greenbrae, Inverness, Kentfield, Larkspur, Marin City, Mill Valley, Novato, Point Reyes, Point Reyes Station, Ross, San Anselmo, San Geronimo, San Quentin, San Rafael, Sausalito, Stinson Beach, Tiburon, Tomales, Woodacre II. NORTH COAST AUTHORS. pp. 91 - 120 -- Alphabetically Arranged 2 I. NORTH COAST PRESSES DEL NORTE COUNTY. CRESCENT CITY. ARTS-IN-CORRECTIONS PROGRAM (Crescent City). The Brief Pelican: Anthology of Prison Writing, 1993. 1992 Pelikanesis: Creative Writing Anthology, 1994. 1994 Virtual Pelican: anthology of writing by inmates from Pelican Bay State Prison.
    [Show full text]