CaltechAUTHORS
  A Caltech Library Service

High Energy Ionic Charge State Composition in the October/November 2003 and January 20, 2005 SEP Events

Labrador, A. W. and Leske, R. A. and Mewaldt, R. A. and Stone, E. C. and von Rosenvinge, T. T. (2005) High Energy Ionic Charge State Composition in the October/November 2003 and January 20, 2005 SEP Events. In: Proceedings of the 29th International Cosmic Ray Conference. Vol.1. Tata Institute of Fundamental Research , Pune, India, pp. 99-102. http://resolver.caltech.edu/CaltechAUTHORS:20150406-152216162

[img] PDF - Published Version
See Usage Policy.

1669Kb

Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:20150406-152216162

Abstract

The ionic charge states of solar energetic particles (SEPs) probe source-material temperatures and acceleration and transport conditions. The MAST instrument on SAMPEX measures SEP ionic charge states at energies greater than ~15 MeV/nuc and at iron energies up to ~90 MeV/nuc using the geomagnetic filter technique. Charge state measurements for large gradual SEP events by MAST and by other experiments suggest that event-to-event variations in the mean charge states of abundant elements are correlated with abundance ratios (e.g. Fe/O). We present charge state measurements for the October/November 2003 events that suggest different source material temperatures for those events. We also present charge state measurements for the January 20, 2005 event, which contrasts with the previously demonstrated Q(Fe) vs. Fe/O correlation. In this event solar and SEP data indicate that the first high-energy particles left the sun when the shock was ~1.5 solar radii above the solar surface. At this altitude charge-equilibration calculations and the observed mean charge states of +12 for Fe imply that <90 seconds were available to accelerate and release the particles. These observations therefore present a serious challenge to SEP acceleration models.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://adsabs.harvard.edu/abs/2005ICRC....1...99LADSArticle
Additional Information:Copyright TATA Institute of Fundamental Research We thank Joe Mazur of Aerospace Corp. for making SAMPEX data available for the 20 Jan. 2005 event. This work was supported in part by NASA grant NASGS-8877.
Group:Space Radiation Laboratory
Funders:
Funding AgencyGrant Number
NASANASGS-8877
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Space Radiation Laboratory2005-11
Record Number:CaltechAUTHORS:20150406-152216162
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20150406-152216162
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:56400
Collection:CaltechAUTHORS
Deposited By: Deborah Miles
Deposited On:22 Apr 2015 01:29
Last Modified:22 Apr 2015 01:29

Repository Staff Only: item control page