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The Evolution of Galactic Cosmic Ray Element Spectra from Solar Minimum to Solar Maximim: ACE Measurements

Davis, A. J. and Mewaldt, R. A. and Binns, W. R. and Christian, E. R. and Cohen, C. M. S. and Cummings, A. C. and George, J. S. and Hink, P. L. and Leske, R. A. and Stone, E. C. and von Rosenvinge, T. T. and Wiedenbeck, M. E. and Yanasak, N. E. (2001) The Evolution of Galactic Cosmic Ray Element Spectra from Solar Minimum to Solar Maximim: ACE Measurements. In: Proceedings of the 27th International Cosmic Ray Conference. Vol.10. Copernicus Systems and Technology GmbH , Berlin, Germany, pp. 3971-3974. http://resolver.caltech.edu/CaltechAUTHORS:20150303-114316464

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Abstract

The spectra of galactic cosmic ray (GCR) elements from Beryllium to Nickel in the energy range 40 - 500 MeV/nucleon at 1 AU are being continuously measured by instruments on-board the Advanced Composition Explorer (ACE). The collecting power of these instruments allows statistically precise spectra to be calculated every few months for most elements. Measurements of temporal variations in GCR spectra over the solar cycle are important for understanding solar modulation processes, and also for refining models of the near-earth radiation environment used to perform shielding and dose calculations for manned and unmanned space missions. We report on ACE observations of the evolution of GCR element spectra from solar minimum in 1997 through Spring 2001. We find significant differences between the ACE measurements and the predictions of available models of the near-Earth radiation environment, suggesting that these models need revision. We describe a cosmic ray interstellar propagation and solar modulation model that provides an improved fit to the ACE measurements compared to radiation environment models currently in use.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://adsabs.harvard.edu/abs/2001ICRC...10.3971DADSArticle
ORCID:
AuthorORCID
Cohen, C. M. S.0000-0002-0978-8127
Additional Information:© Copernicus GmbH. This research was supported by NASA at the California Institute of Technology (under grant NAG5-6912), the Jet Propulsion Laboratory, the Goddard Space Flight Center, and Washington University. We are grateful to Gautam D. Badhwar at NASA Johnson Space Flight Center for providing GCR environment model data, and to the developers of CREME96 for presenting their programs on the Web for public use,
Group:Space Radiation Laboratory
Funders:
Funding AgencyGrant Number
NASANAG5-6912
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Space Radiation Laboratory2001-51
Record Number:CaltechAUTHORS:20150303-114316464
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20150303-114316464
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:55473
Collection:CaltechAUTHORS
Deposited By: Deborah Miles
Deposited On:05 Mar 2015 03:35
Last Modified:12 Sep 2017 23:22

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