CaltechAUTHORS
  A Caltech Library Service

Large Proton Anisotropies in the 18 August 2010 Solar Particle Event

Leske, R. A. and Cohen, C. M. S. and Mewaldt, R. A. and Christian, E. R. and Cummings, A. C. and Labrador, A. W. and Stone, E. C. and Wiedenbeck, M. E. and von Rosenvinge, T. T. (2012) Large Proton Anisotropies in the 18 August 2010 Solar Particle Event. Solar Physics, 281 (1). pp. 301-318. ISSN 0038-0938. http://resolver.caltech.edu/CaltechAUTHORS:20121207-133222594

Full text is not posted in this repository. Consult Related URLs below.

Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:20121207-133222594

Abstract

The solar particle event observed at STEREO Ahead on 18 August 2010 displayed a rich variety of behavior in the particle anisotropies. Sectored rates measured by the Low Energy Telescope (LET) on STEREO showed very large bidirectional anisotropies in 4 – 6 MeV protons for the first ∼ 17 hours of the event while inside a magnetic cloud, with intensities along the field direction several hundred to nearly 1000 times greater than those perpendicular to the field. At the trailing end of the cloud, the protons became isotropic and their spectrum hardened slightly, while the He/H abundance ratio plunged by a factor of approximately four for about four hours. Associated with the arrival of a shock on 20 August was a series of brief (< 10 minute duration) intensity increases (commonly called “shock spikes”) with relatively narrow angular distributions (∼ 45∘ FWHM), followed by an abrupt decrease in particle intensities at the shock itself and a reversal of the proton flow to a direction toward the Sun and away from the receding shock. We discuss the STEREO/LET observations of this interesting event in the context of other observations reported in the literature.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1007/s11207-012-0018-5DOIArticle
http://link.springer.com/article/10.1007%2Fs11207-012-0018-5PublisherArticle
ORCID:
AuthorORCID
Cohen, C. M. S.0000-0002-0978-8127
Additional Information:© Springer, Part of Springer Science+Business Media. Received: 3 November 2011; Accepted: 28 April 2012; Published online: 6 June 2012. This work was supported by the National Aeronautics and Space Administration (NASA) at Caltech and JPL under subcontract SA2715-26309 from the University of California at Berkeley under NASA contract NAS5-03131, and by NASA award NNX08AK87G. We thank the PLASTIC (NASA contract NAS5-00132), MAG, and SWEA investigators on STEREO for making their data publicly available. This work benefited greatly from discussions at "The Sun-360 Workshop" held at the Christian-Albrechts-Universität in Kiel, Germany in July 2011. We thank B. Dotson for help in analyzing the data and in preparing the figures.
Group:Space Radiation Laboratory
Funders:
Funding AgencyGrant Number
NASASA2715-26309
NASANNX08AK87G
Subject Keywords:Cosmic rays; solar Energetic particles; propagation Magnetic fields; interplanetary
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Space Radiation Laboratory2012-12
Record Number:CaltechAUTHORS:20121207-133222594
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20121207-133222594
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:35882
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:07 Dec 2012 22:37
Last Modified:10 Sep 2017 04:51

Repository Staff Only: item control page