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Vertical Distribution of Shallow Water in the Distinguishable Regions at Low and High Latitudes of Mars: Neutron Data Deconvolution of HENDHigh Energy Neutron Detector (HEND) is the part of Gamma-Ray Spectrometer suite onboard NASA Mars Odyssey orbiter [1-4]. During 16 months of mapping stage of Odyssey mission HEND has accumulated the set of maps of neutron emission of Mars at more than seven decades of energies range from the Cadmium threshold of 0.4 eV up to 15 MeV. These maps present very large variations of neutrons at different regions of Mars and they also show quite strong changes along Martian seasons.
Document ID
20030066636
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
I G Mitrofanov
(Space Research Institute Moscow, Russia)
M L Litvak
(Space Research Institute Moscow, Russia)
A S Kozyrev
(Space Research Institute Moscow, Russia)
A B Sanin
(Space Research Institute Moscow, Russia)
V Tretakov
(Space Research Institute Moscow, Russia)
W V Boynton
(University of Arizona Tucson, Arizona, United States)
D K Hamara
(University of Arizona Tucson, Arizona, United States)
C Shinohara
(University of Arizona Tucson, Arizona, United States)
R S Saunders
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
D Drake
(Los Alamos National Laboratory Los Alamos, New Mexico, United States)
Date Acquired
August 21, 2013
Publication Date
July 25, 2003
Publication Information
Publication: Sixth International Conference on Mars
Publisher: LPI
Subject Category
Astrophysics
Report/Patent Number
3080
Meeting Information
Meeting: Sixth International Conference on Mars
Location: Pasadena, CA
Country: US
Start Date: July 20, 2003
End Date: July 25, 2003
Sponsors: Lunar and Planetary Institute
Funding Number(s)
CONTRACT_GRANT: NCC5-679
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
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