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Multiply Charged Anomalous Cosmic Rays Above 15 MeV/nucleon

Selesnick, R. S. and Mewaldt, R. A. and Cummings, J. R. (1997) Multiply Charged Anomalous Cosmic Rays Above 15 MeV/nucleon. In: Proceedings of the 25th International Cosmic Ray Conference. Vol.2. Potchefstroom University, Space Research Unit , Transvaal, South Africa, pp. 269-272. https://resolver.caltech.edu/CaltechAUTHORS:20140703-224910311

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Abstract

Ionic charge states of anomalous cosmic ray nitrogen, oxygen, and neon with kinetic energies above 15 MeV /nucleon have been measured using the geomagnetic field as a rigidity filter. Data from the MAST instrument on the polar-orbiting SAMPEX satellite taken during the period from 1992 to 1996 show that all three elements are predominantly multiply charged at high energies, confirming the earlier result for oxygen alone based on a smaller data set. Energy spectra of the singly charged and multiply charged components of each element are compared with model predictions.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://adslabs.org/adsabs/abs/1997ICRC....2..269S/ADSArticle
ORCID:
AuthorORCID
Mewaldt, R. A.0000-0003-2178-9111
Additional Information:© Space Research Unit. Provided by the NASA Astrophysics Data System. This work was supported by NASA under Cooperative Agreement 26979B with the Aerospace Corporation and grants NAS5-30704 and NAGW-1919 to the California Institute of Technology.
Group:Space Radiation Laboratory
Funders:
Funding AgencyGrant Number
NASA Cooperative Agreement26979B
NASANAS5-30704
NASANAGW-1919
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Space Radiation Laboratory1997-05
Record Number:CaltechAUTHORS:20140703-224910311
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20140703-224910311
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:46855
Collection:CaltechAUTHORS
Deposited By: Deborah Miles
Deposited On:15 Jul 2014 15:52
Last Modified:22 Nov 2019 09:58

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