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JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 117, E00H13, doi:10.1029/2011JE003978, 2012
Lunar radiation environment and space weathering
from the Cosmic Ray Telescope for the Effects
of Radiation (CRaTER)
N. A. Schwadron, 1,2 T. Baker,1,2 B. Blake,3 A. W. Case,4 J. F. Cooper,5 M. Golightly,1,2
A. Jordan,1,2 C. Joyce,1 J. Kasper,4 K. Kozarev,4,6 J. Mislinski,1,2 J. Mazur,7 A. Posner,8
O. Rother,9,10 S. Smith,1,2 H. E. Spence,1,2 L. W. Townsend,11 J. Wilson,1,2 and C. Zeitlin12
Received 29 September 2011; revised 27 December 2011; accepted 8 January 2012; published 13 March 2012.
[1] The Cosmic Ray Telescope for the Effects of Radiation (CRaTER) measures linear
energy transfer by Galactic Cosmic Rays (GCRs) and Solar Energetic Particles (SEPs) on
the Lunar Reconnaissance Orbiter (LRO) Mission in a circular, polar lunar orbit. GCR
fluxes remain at the highest levels ever observed during the space age. One of the largest
SEP events observed by CRaTER during the LRO mission occurred on June 7, 2011. We
compare model predictions by the Earth-Moon-Mars Radiation Environment Module
(EMMREM) for both dose rates from GCRs and SEPs during this event with results from
CRaTER. We find agreement between these models and the CRaTER dose rates, which
together demonstrate the accuracy of EMMREM, and its suitability for a real-time space
weather system. We utilize CRaTER to test forecasts made by the Relativistic Electron
Alert System for Exploration (REleASE), which successfully predicts the June 7th event.
At the maximum CRaTER-observed GCR dose rate (11.7 cGy/yr where Gy is a unit
indicating energy deposition per unit mass, 1 Gy = 1 J/kg), GCRs deposit 88 eV/
molecule in water over 4 billion years, causing significant change in molecular
composition and physical structure (e.g., density, color, crystallinity) of water ice, loss of
molecular hydrogen, and production of more complex molecules linking carbon and other
elements in the irradiated ice. This shows
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