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The Ionic Charge of Solar Energetic Particles with Energies of 0.3-70 MeV per Nucleon

Oetliker, M. and Klecker, B. and Hovestadt, D. and Mason, G. M. and Mazur, J. E. and Leske, R. A. and Mewaldt, R. A. and Blake, J. B. and Looper, M. D. (1997) The Ionic Charge of Solar Energetic Particles with Energies of 0.3-70 MeV per Nucleon. Astrophysical Journal, 477 (1). pp. 495-501. ISSN 0004-637X. http://resolver.caltech.edu/CaltechAUTHORS:20141202-154908656

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Abstract

With the three particle sensors Low Energy Ion Composition Analyzer (LICA), Heavy Ion Large Area Proportional Counter Telescope (HILT), and Mass Spectrometer Telescope (MAST) on board the polar orbiting Solar, Anomalous, and Magnetospheric Particle Explorer (SAMPEX) satellite, the ionic charge of solar energetic particles (SEP) was measured over a wide energy range from 0.3 to 70 MeV per nucleon. For each sensor, the evaluation was performed separately. The results obtained with LICA (0.3-10 MeV per nucleon) and MAST (15-70 MeV per nucleon) were published earlier by Mason et al. and Leske et al., respectively. In this work we present the results of the HILT sensor (7-50 MeV per nucleon) and discuss the combined results of the three instruments. With HILT, the mean ionic charge of SEP was measured for carbon, nitrogen, oxygen, neon, magnesium, silicon, sulfur, argon, calcium, and iron in the energy range 7È50 MeV per nucleon during two consecutive large SEP events in 1992 OctoberÈNovember. The mean ionic charge was inferred from the rigidity-dependent geomagnetic flux cutoff. The coronal temperatures deduced from the mean ionic charges are well in accordance with the value of ~2x10^6 K except for neon and magnesium, as previously reported. The data measured with the three sensors, LICA, HILT, and MAST, agree well and are in accordance with data previously measured at energies below 3 MeV per nucleon (Luhn et al.), except for iron, where we observed a significant energy dependence of the mean charge over the energy range 0.3-70 MeV per nucleon.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/303679DOIArticle
http://iopscience.iop.org/0004-637X/477/1/495PublisherArticle
ORCID:
AuthorORCID
Mason, G. M.0000-0003-2169-9618
Additional Information:© 1996. American Astronomical Society. Received 1996 March 27, accepted for publication 1996 September 16. We thank the dedicated members of the participating institutes who designed, constructed, and calibrated the HILT, LICA, MAST, and PET instruments. We are particularly grateful to the Small Explorer Project Office and the Orbiting Satellites Branch at Goddard Space Flight Center for the construction, launch, and postlaunch operation of the SAMPEX spacecraft. This work was supported by the Bundesministerium fur Forschung und Technologie, Germany, grant number 50 OC90021 and by NASA, contract, NAS 5-30704, and grant NAG-2963.
Group:Space Radiation Laboratory
Funders:
Funding AgencyGrant Number
NASANAS5-30704
NASANAG-2963
Non-Subject Keywords:Sun: corona; Sun: flares; Sun: particle emission
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Space Radiation Laboratory1997-43
Record Number:CaltechAUTHORS:20141202-154908656
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20141202-154908656
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:52296
Collection:CaltechAUTHORS
Deposited By: Deborah Miles
Deposited On:03 Dec 2014 01:22
Last Modified:14 Sep 2017 22:54

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