CRaTER: The Cosmic Ray Telescope for the Effects of Radiation Experiment on the Lunar Reconnaissance Orbiter Mission

CRaTER: телескоп космических лучей для исследования радиационных эффектов в рамках миссии лунного разведывательного орбитального аппарата
H. E. Spence, A. W. Case, M. J. Golightly, Thomas Heine, B. Larsen, J. B. Blake, P. Caranza, William R. Crain, J. George, M.V. Lalić, Albert Y. Lin, M. D. Looper, J. E. Mazur, D. Salvaggio, J. C. Kasper, T. J. Stubbs, M. Doucette, P. G. Ford, Richard F. Foster, R. Goeke, D. D. Gordon, B. W. Klatt, J. R. O'Connor, Matthew W. Smith, T. G. Onsager, C. Zeitlin, Lawrence W. Townsend, Y Charara
2010-01-01

CRaTERgalactic cosmic rayslinear energy transferlunar space radiation environmentsolar energetic protons
The Cosmic Ray Telescope for the Effects of Radiation (CRaTER) on the Lunar Reconnaissance Orbiter (LRO) characterizes the radiation environment to be experienced by humans during future lunar missions. CRaTER measures the effects of ionizing energy loss in matter due to penetrating solar energetic protons (SEP) and galactic cosmic rays (GCR), specifically in silicon solid-state detectors and after interactions with tissue-equivalent plastic (TEP), a synthetic analog of human tissue. The CRaTER investigation quantifies the linear energy transfer (LET) spectrum in these materials through direct measurements with the lunar space radiation environment, particularly the interactions of ions with energies above 10 MeV, which penetrate and are detected by CRaTER. Combined with models of radiation transport through materials, CRaTER LET measurements constrain models of the biological effects of ionizing radiation in the lunar environment as well as provide valuable information on radiation effects on electronic systems in deep space. In addition to these human exploration goals, CRaTER measurements also provide new insights on the spatial and temporal variability of the SEP and GCR populations and their interactions with the lunar surface. We present here an overview of the CRaTER science goals and investigation, including: an instrument description; observation strategies; instrument testing, characterization, and calibration; and data analysis, interpretation, and modeling plans.
1
CRaTER characterizes the lunar radiation environment relevant to human missions by measuring ionizing energy loss from solar energetic protons and galactic cosmic rays.
2
CRaTER measurements, combined with radiation-transport models, constrain predictions of biological radiation effects in the lunar environment.
3
CRaTER observations reveal spatial and temporal variability in solar energetic particle and galactic cosmic-ray populations and their interactions with the lunar surface.
4
The instrument directly measures linear energy transfer spectra in silicon detectors and tissue-equivalent plastic for ions above 10 MeV.
5
The investigation provides information about radiation effects on electronic systems during deep-space missions.

The lunar space radiation environment, including penetrating solar energetic protons and galactic cosmic rays interacting with silicon detectors and tissue-equivalent plastic

Linear energy transfer spectra and the spatial and temporal variability of solar energetic particle and galactic cosmic ray populations, with implications for biological and electronic radiation effects

Publication Details
Publication Date
2010-01-01
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Authors
H. E. Spence
A. W. Case
M. J. Golightly
Thomas Heine
B. Larsen
J. B. Blake
P. Caranza
William R. Crain
J. George
M.V. Lalić
Albert Y. Lin
M. D. Looper
J. E. Mazur
D. Salvaggio
J. C. Kasper
T. J. Stubbs
M. Doucette
P. G. Ford
Richard F. Foster
R. Goeke
D. D. Gordon
B. W. Klatt
J. R. O'Connor
Matthew W. Smith
T. G. Onsager
C. Zeitlin
Lawrence W. Townsend
Y Charara
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