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Galactic Cosmic-Ray Energy Spectra and Composition during the 2009-2010 Solar Minimum Period

Lave, K. A. and Wiedenbeck, M. E. and Binns, W. R. and Christian, E. R. and Cummings, A. C. and Davis, A. J. and de Nolfo, G. A. and Israel, M. H. and Leske, R. A. and Mewaldt, R. A. and Stone, E. C. and von Rosenvinge, T. T. (2013) Galactic Cosmic-Ray Energy Spectra and Composition during the 2009-2010 Solar Minimum Period. Astrophysical Journal, 770 (2). Art. No. 117. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20130725-072008737

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Abstract

We report new measurements of the elemental energy spectra and composition of galactic cosmic rays during the 2009-2010 solar minimum period using observations from the Cosmic Ray Isotope Spectrometer (CRIS) onboard the Advanced Composition Explorer. This period of time exhibited record-setting cosmic-ray intensities and very low levels of solar activity. Results are given for particles with nuclear charge 5 ≤ Z ≤ 28 in the energy range ~50-550 MeV nucleon^(–1). Several recent improvements have been made to the earlier CRIS data analysis, and therefore updates of our previous observations for the 1997-1998 solar minimum and 2001-2003 solar maximum are also given here. For most species, the reported intensities changed by less than ~7%, and the relative abundances changed by less than ~4%. Compared with the 1997-1998 solar minimum relative abundances, the 2009-2010 abundances differ by less than 2σ, with a trend of fewer secondary species observed in the more recent time period. The new 2009-2010 data are also compared with results of a simple "leaky-box" galactic transport model combined with a spherically symmetric solar modulation model. We demonstrate that this model is able to give reasonable fits to the energy spectra and the secondary-to-primary ratios B/C and (Sc+Ti+V)/Fe. These results are also shown to be comparable to a GALPROP numerical model that includes the effects of diffusive reacceleration in the interstellar medium.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/770/2/117DOIArticle
http://iopscience.iop.org/0004-637X/770/2/117PublisherArticle
ORCID:
AuthorORCID
Wiedenbeck, M. E.0000-0002-2825-3128
Binns, W. R.0000-0001-6110-3407
Christian, E. R.0000-0003-2134-3937
Cummings, A. C.0000-0002-3840-7696
de Nolfo, G. A.0000-0002-3677-074X
Israel, M. H.0000-0002-8104-208X
Leske, R. A.0000-0002-0156-2414
Mewaldt, R. A.0000-0003-2178-9111
Stone, E. C.0000-0002-2010-5462
Additional Information:© 2013 American Astronomical Society. Received 2013 February 14; accepted 2013 May 11; published 2013 June 3. This work was supported by NASA at the California Institute of Technology (under grants NNX08AI11G and NNX10AE45G), the Goddard Space Flight Center, the Jet Propulsion Laboratory, and Washington University in Saint Louis. We also acknowledge Dr. Nasser Barghouty for his vital help in updating the semi-empirical nuclear production cross sections used in our interstellar transport code.
Group:Space Radiation Laboratory
Funders:
Funding AgencyGrant Number
NASANNX08AI11G
NASANNX10AE45G
Goddard Space Flight CenterUNSPECIFIED
JPLUNSPECIFIED
Washington UniversityUNSPECIFIED
Subject Keywords: cosmic rays; Galaxy: abundances; Sun: activity
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Space Radiation Laboratory2013-17
Issue or Number:2
Record Number:CaltechAUTHORS:20130725-072008737
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20130725-072008737
Official Citation:Galactic Cosmic-Ray Energy Spectra and Composition during the 2009-2010 Solar Minimum Period K. A. Lave, M. E. Wiedenbeck, W. R. Binns, E. R. Christian, A. C. Cummings, A. J. Davis, G. A. de Nolfo, M. H. Israel, R. A. Leske, R. A. Mewaldt, E. C. Stone, and T. T. von Rosenvinge doi:10.1088/0004-637X/770/2/117
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:39571
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:25 Jul 2013 14:46
Last Modified:09 Mar 2020 13:19

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