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Martian Radiation Environment: Model Calculations and Recent Measurements with "MARIE"The Galactic Cosmic Ray spectra in Mars orbit were generated with the recently expanded HZETRN (High Z and Energy Transport) and QMSFRG (Quantum Multiple-Scattering theory of nuclear Fragmentation) model calculations. These model calculations are compared with the first eighteen months of measured data from the MARIE (Martian Radiation Environment Experiment) instrument onboard the 2001 Mars Odyssey spacecraft that is currently in Martian orbit. The dose rates observed by the MARIE instrument are within 10% of the model calculated predictions. Model calculations are compared with the MARIE measurements of dose, dose-equivalent values, along with the available particle flux distribution. Model calculated particle flux includes GCR elemental composition of atomic number, Z = 1-28 and mass number, A = 1-58. Particle flux calculations specific for the current MARIE mapping period are reviewed and presented.
Document ID
20050217203
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Saganti, P. B.
(NASA Johnson Space Center Houston, TX, United States)
Cucinotta, F. A.
(NASA Johnson Space Center Houston, TX, United States)
zeitlin, C. J.
(California Univ., Lawrence Berkeley National Lab. Berkeley, CA, United States)
Cleghorn, T. F.
(NASA Johnson Space Center Houston, TX, United States)
Date Acquired
August 23, 2013
Publication Date
January 1, 2004
Subject Category
Space Radiation
Meeting Information
Meeting: 35th CSOPAR Scientific Assembly
Location: Paris
Country: France
Start Date: July 18, 2004
End Date: July 25, 2004
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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