P51C:
Geophysical Investigations of Planetary Volatiles II Posters

Friday, 19 December 2014: 8:00 AM-12:20 PM
Primary Convener:  Stephen M Clifford, Lunar and Planetary Institute, Houston, TX, United States
Co-conveners:  Valerie Ciarletti, LATMOS/CNRS, Guyancourt, France, Essam Heggy, NASA Jet Propulsion Laboratory, Pasadena, CA, United States and Igor G. Mitrofanov, Institute for Space Research, Moscow, Russia

Abstracts Submitted to this Session:

 
Exploring Vesta's Surface Roughness and Dielectric Properties Using VIR Spectrometer and Bistatic Radar Observations by the Dawn Mission
Elizabeth M Palmer, University of California Los Angeles, Los Angeles, CA, United States, Essam Heggy, NASA Jet Propulsion Laboratory, Pasadena, CA, United States, Maria Teresa Capria, IAPS-INAF, Rome, Italy, Federico Tosi, INAF, Rome, Italy, Wlodek W Kofman, University Joseph Fourier Grenoble, Grenboble, France and Christopher T Russell, Univ California, Los Angeles, CA, United States
 
A diurnal study of lunar topography to determine regolith temperature contributions to the inference of hydrogen volatiles using epithermal neutrons from the Lunar Exploration Neutron Detector (LEND).
Timothy P McClanahan1, Igor G. Mitrofanov2, William V Boynton3, Gordon Chin4, Larry G. Evans5, Richard D Starr6, Timothy A Livengood7, Maxim L Litvak2, Anton B. Sanin2, Joseph Murray8, Ann M Parsons1, Jao Jiang Su8, Julia Bodnarik3, Karl Harshman3 and Roald Sagdeev8, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)Space Research Institute RAS, Moscow, Russia, (3)Univ Arizona, Tucson, AZ, United States, (4)NASA Goddard Space Flight Center, Code 693, Greenbelt, MD, United States, (5)Computer Sciences Corporation, Stennis Space Center, MS, United States, (6)Catholic University of America, Washington, DC, United States, (7)University of Maryland College Park, College Park, MD, United States, (8)University of Maryland College Park, Physics, College Park, MD, United States
 
MSL DAN Passive Data and Interpretations
Christopher Tate1, Jeffrey Moersch1, Insoo Jun2, Douglas W Ming3, Igor G. Mitrofanov4, Maxim L Litvak4, Alberto Behar2, William V Boynton5, Darrel Drake6, Denis Lisov4, Michael A Mischna2, Craig J Hardgrove7, Ralph Milliken8, Anton B. Sanin4, Richard D Starr9, Javier Martín-Torres10, Maria-Paz Zorzano11, Fedor Fedosov4, Dmitry Golovin4, Karl Harshman5, Alexander Kozyrev4, Alexey Malakhov4, Maxim Mokrousov4, Sergey Nikiforov4 and Aleksey Varenikov4, (1)University of Tennessee, Knoxville, TN, United States, (2)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (3)NASA Johnson Space Center, Houston, TX, United States, (4)Space Research Institute RAS, Moscow, Russia, (5)Univ Arizona, Tucson, AZ, United States, (6)TechSource, Inc, Los Alamos, NM, United States, (7)Arizona State University, Tempe, AZ, United States, (8)Brown University, Providence, RI, United States, (9)Catholic University of America, Washington, DC, United States, (10)Instituto Andaluz de Ciencias de la Tierra, Granada, Spain, (11)INTA-CSIC, Madrid, Spain
 
The Mars Diurnal CO2 Cycle as Observed in the Tharsis Region.
Timothy N Titus and Glen E. Cushing, USGS Astrogeology Science Center, Flagstaff, AZ, United States
 
Joint Analysis of Bulk Water/Chlorine Distribution in the Martian Subsurface along MSL Curiosity Traverse from Comparison between DAN/MSL and other instruments observations onboard Curiosity Rover
Maxim L Litvak1, Igor G. Mitrofanov1, Anton B. Sanin1, Denis Lisov1, Craig J Hardgrove2, William V Boynton3, Insoo Jun4, Ruslan Kuzmin1, Javier Martín-Torres5, Michael A Mischna4, Jeffrey Moersch6, Sergey Nikiforov1, Richard D Starr7, Christopher Tate6 and Maria-Paz Zorzano8, (1)Space Research Institute RAS, Moscow, Russia, (2)Arizona State University, Tempe, AZ, United States, (3)Univ Arizona, Tucson, AZ, United States, (4)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (5)Instituto Andaluz de Ciencias de la Tierra, Granada, Spain, (6)University of Tennessee, Knoxville, TN, United States, (7)Catholic University of America, Washington, DC, United States, (8)INTA-CSIC, Madrid, Spain
 
Performance Modeling of Orbital Gamma-Ray Spectroscopy of Carbonaceous Asteroids: Monte-Carlo Modeling of the HPGe Mars Odyssey GRS
Lucy F Lim1, Richard D Starr2, Larry G. Evans3, Ann M Parsons1, Mike E Zolensky4 and William V Boynton5, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)Catholic University of America, Washington, DC, United States, (3)Computer Sciences Corporation, Stennis Space Center, MS, United States, (4)NASA Johnson Space Center, Houston, TX, United States, (5)Univ Arizona, Tucson, AZ, United States
 
Impact Delivery of Water at the Moon and Mercury
Megan Bruck Syal, Lawrence Livermore National Laboratory, Livermore, CA, United States and Peter H Schultz, Brown University, Providence, RI, United States
 
Estimating Background and Lunar Contribution to Neutrons Detected by the Lunar Reconnaissance Orbiter (LRO) Lunar Exploration Neutron Detector (LEND) Instrument
Timothy A Livengood1, Igor G. Mitrofanov2, Gordon Chin3, William V Boynton4, Larry G. Evans5, Maxim L Litvak2, Timothy P McClanahan6, Roald Sagdeev7, Anton B. Sanin2, Richard D Starr8 and Jao Jiang Su7, (1)University of Maryland College Park, College Park, MD, United States, (2)Space Research Institute RAS, Moscow, Russia, (3)NASA Goddard Space Flight Center, Code 693, Greenbelt, MD, United States, (4)Univ Arizona, Tucson, AZ, United States, (5)Computer Sciences Corporation, Stennis Space Center, MS, United States, (6)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (7)University of Maryland College Park, Physics, College Park, MD, United States, (8)Catholic University of America, Washington, DC, United States
 
3D Synthetic Aperture Radar Imaging of the Interior of the Cometary Nucleus
Yonggyu Gim1, Essam Heggy1, Darmin Arumugam1, Xiaoqing Wu1 and Erik I Asphaug2, (1)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (2)Arizona State University, Tempe, AZ, United States
 
Cross Calibration of Omnidirectional Orbital Neutron Detectors of Lunar Prospector (LP) and Lunar Exploration Neutron Detector (LEND) by Monte Carlo Simulation
Joseph Murray1, Jao Jang SU1, Roald Sagdeev1 and Gordon Chin2, (1)University of Maryland College Park, Physics, College Park, MD, United States, (2)NASA Goddard Space Flight Center, Code 693, Greenbelt, MD, United States
 
Compressive Strength of Cometary Surfaces Derived from Radar Observations
Ahmed ElShafie, University of Arkansas, Fayetteville, AR, United States and Essam Heggy, NASA Jet Propulsion Laboratory, Pasadena, CA, United States
 
Modeling Radar Wave Propagation Through Comet 67P / Churyumov-Gerasimenko
Giovanni Scabbia, California Institute of Technology, Pasadena, CA, United States, Essam Heggy, NASA Jet Propulsion Laboratory, Pasadena, CA, United States, Jeremie Lasue, IRAP, Toulouse, France, Wlodek W Kofman, University Joseph Fourier Grenoble, Grenboble, France and Elizabeth M Palmer, University of California Los Angeles, Los Angeles, CA, United States
 
The Effects of Surface and Subsurface Structural Anomalies on the Detectability of Shallow Aquifers on Europa by Sounding Radar
Essam Heggy, NASA Jet Propulsion Laboratory, Pasadena, CA, United States and Giovanni Scabbia, California Institute of Technology, Pasadena, CA, United States
 
See more of: Planetary Sciences