Observations of Anomalous Cosmic Rays at 1 AU
Leske, R. A. and Mewaldt, R. A. and Christian, E. R. and Cohen, C. M. S. and Cummings, A. C. and Slocum, P. L. and Stone, E. C. and von Rosenvinge, T. T. and Wiedenbeck, M. E.
(2000)
Observations of Anomalous Cosmic Rays at 1 AU.
In:
Acceleration and Transport of Energetic Particles Observed in the Heliosphere.
AIP Conference Proceedings.
No.528.
American Institute of Physics
, Melville, N.Y. , pp. 293-300.
ISBN 1-56396-951-3.
https://resolver.caltech.edu/CaltechAUTHORS:20111208-100352581
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Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20111208-100352581 AbstractAnomalous cosmic rays (ACRs) provide a sensitive probe of the access of energetic particles to the inner heliosphere, varying in intensity by more than two orders of magnitude during the course of the solar cycle. New data which are becoming available from the Advanced Composition Explorer (ACE) can provide a detailed record of ACR intensity and spectral changes on short (~ 1 day) time scales during the approach to solar maximum, which will help address issues of ACR modulation and transport. The elemental and isotopic composition of ACRs provides important information on the source or sources of these particles, while their ionic charge state composition and its energy dependence
serves as a diagnostic of their acceleration time scale. We review measurements of the ACR elemental, isotopic,
and charge state composition and spectra as determined at 1 AU by SAMPEX, ACE, Wind, and other spacecraft. These
results are important input to models of the acceleration, modulation, and transport of ACRs. Item Type: | Book Section |
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Additional Information: | © 2000 American Institute of Physics. Issue Date: 15 September 2000. This research was supported by NASA at the California
Institute of Technology (under grant NAG5-6912), the
Jet Propulsion Laboratory, and the Goddard Space Flight
Center. We thank R. S. Selesnick, N. E. Yanasak, and
B. Klecker for providing data used in some of the figures.
Climax neutron monitor data were obtained from
the web, courtesy of the University of Chicago, National
Science Foundation grant ATM-9613963. |
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Group: | Space Radiation Laboratory |
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Funders: | Funding Agency | Grant Number |
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NASA | NAG5-6912 | JPL | UNSPECIFIED | Goddard Space Flight Center | UNSPECIFIED | NSF | ATM-9613963 |
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Subject Keywords: | primary cosmic rays, interstellar matter, cosmic ray origin, cosmic ray variations, solar activity, cosmic ray composition, element relative abundance, isotope relative abundance, cosmic ray energy spectra, transport processes, acceleration |
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Other Numbering System: | Other Numbering System Name | Other Numbering System ID |
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Space Radiation Laboratory | 2000-25 |
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Series Name: | AIP Conference Proceedings |
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Issue or Number: | 528 |
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Classification Code: | PACS: 98.70.Sa; 96.40.De |
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DOI: | 10.1063/1.1324328 |
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Record Number: | CaltechAUTHORS:20111208-100352581 |
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Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20111208-100352581 |
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Official Citation: | Observations of anomalous cosmic rays at 1 AU
R. A. Leske, R. A. Mewaldt, E. R. Christian, C. M. S. Cohen, A. C. Cummings, P. L. Slocum, E. C. Stone, T. T. von Rosenvinge, and M. E. Wiedenbeck, AIP Conf. Proc. 528, 293 (2000), DOI:10.1063/1.1324328
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Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. |
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ID Code: | 28370 |
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Collection: | CaltechAUTHORS |
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Deposited By: |
Ruth Sustaita
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Deposited On: | 08 Dec 2011 19:46 |
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Last Modified: | 09 Nov 2021 16:56 |
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