Published October 2006 | Version v1
Journal article

Helium cosmic ray flux measurements at Mars

  • 1. University of Houston, 4800 Calhoun Rd. Houston, TX 77204 (United States)
  • 2. National Space Biomedical Research Institute, Baylor College of Medicine, Houston, TX (United States)
  • 3. NASA Johnson Space Center, 2101 NASA Road 1, Houston, TX 77058 (United States)
  • 4. Prairie View A and M University, P.O. Box 519, Prairie View, TX 77446-0519 (United States)
  • 5. The Boeing Company, Houston, TX (United States)
  • 6. Advancing National Strategies and Enabling Results (ANSER), Arlington, Virginia (US)

Description

The helium energy spectrum in Martian orbit has been observed by the MARIE charged particle spectrometer aboard the 2001 Mars Odyssey spacecraft. The orbital data were taken from March 13, 2002 to October 28, 2003, at which time a very intense Solar Particle Event caused a loss of communication between the instrument and the spacecraft. The silicon detector stack in MARIE is optimized for the detection of protons and helium in the energy range below 100MeV/n, which typically includes almost all of the flux during SPEs. This also makes MARIE an efficient detector for GCR helium in the energy range of 50-150MeV/n. We will present the first fully normalized flux results from MARIE, using helium ions in this energy range

Additional details

Identifiers

DOI
10.1016/j.radmeas.2006.07.011;
PII
S1350-4487(06)00140-5;

Publishing Information

Journal Title
Radiation Measurements
Journal Volume
41
Journal Issue
9-10
Journal Page Range
p. 1123-1125
ISSN
1350-4487
CODEN
RMEAEP

Optional Information

Copyright
Copyright (c) 2006 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.