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Characteristics of trapped proton anisotropy at Space Station Freedom altitudesThe ionizing radiation dose for spacecraft in low-Earth orbit (LEO) is produced mainly by protons trapped in the Earth's magnetic field. Current data bases describing this trapped radiation environment assume the protons to have an isotropic angular distribution, although the fluxes are actually highly anisotropic in LEO. The general nature of this directionality is understood theoretically and has been observed by several satellites. The anisotropy of the trapped proton exposure has not been an important practical consideration for most previous LEO missions because the random spacecraft orientation during passage through the radiation belt 'averages out' the anisotropy. Thus, in spite of the actual exposure anisotropy, cumulative radiation effects over many orbits can be predicted as if the environment were isotropic when the spacecraft orientation is variable during exposure. However, Space Station Freedom will be gravity gradient stabilized to reduce drag, and, due to this fixed orientation, the cumulative incident proton flux will remain anisotropic. The anisotropy could potentially influence several aspects of Space Station design and operation, such as the appropriate location for radiation sensitive components and experiments, location of workstations and sleeping quarters, and the design and placement of radiation monitors. Also, on-board mass could possible be utilized to counteract the anisotropy effects and reduce the dose exposure. Until recently only omnidirectional data bases for the trapped proton environment were available. However, a method to predict orbit-average, angular dependent ('vector') trapped proton flux spectra has been developed from the standard omnidirectional trapped proton data bases. This method was used to characterize the trapped proton anisotropy for the Space Station orbit (28.5 degree inclination, circular) in terms of its dependence on altitude, solar cycle modulation (solar minimum vs. solar maximum), shielding thickness, and radiation effect (silicon rad and rem dose).
Document ID
19910006640
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Armstrong, T. W.
(Science Applications International Corp. Huntsville, AL., United States)
Colborn, B. L.
(Science Applications International Corp. Huntsville, AL., United States)
Watts, J. W.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
September 6, 2013
Publication Date
October 1, 1990
Subject Category
Astrophysics
Report/Patent Number
SAIC-90/1474
NASA-CR-184061
NAS 1.26:184061
Report Number: SAIC-90/1474
Report Number: NASA-CR-184061
Report Number: NAS 1.26:184061
Accession Number
91N15953
Funding Number(s)
CONTRACT_GRANT: NAS8-37916
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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