Heavy ion observations by MARIE in cruise phase and Mars orbit.
The charged particle spectrum for nuclei from protons to neon, (charge Z=10) was observed during the cruise phase and orbit around Mars by the MARIE charged particle spectrometer on the Odyssey spacecraft. The cruise data were taken between April 23, 2001 and mid-August 2001. The Mars orbit data were taken March 5, 2002 through May 2002 and are scheduled to continue until August 2004. Charge peaks are clearly separated for charges up to Z=10. Especially prominent are the carbon and oxygen peaks, with boron and nitrogen also clearly visible. Although heavy ions are much less abundant than protons in the cosmic ray environment, it is important to determine their abundances because their ionization energy losses (proportional to Z2) are far more dangerous to humans and to instruments. Thus the higher charged nuclei make a significant contribution to dose and dose equivalent received in space. Results of the charged particle spectrum measurements will be reported.
Lee
K T
KT
University of Houston, Houston, TX 77204, USA. ktlee@ems.jsc.nasa.gov
Cleghorn
T
T
Cucinotta
F
F
Pinsky
L
L
Zeitlin
C
C
D002138:Calibration; D003359:Cosmic Radiation; D020450:Heavy Ions; D006371:Helium; D018535:Mars; D009356:Neon; D011522:Protons; D011829:Radiation Dosage; D011834:Radiation Monitoring / Q000295:instrumentation*; D013026:Space Flight / Q000295:instrumentation*; D018531:Spacecraft / Q000295:instrumentation
D011522:Protons; D006371:Helium; D009356:Neon