Observational evidence on the presence of an outer reflecting boundary in solar energetic particle events

43Citations
Citations of this article
18Readers
Mendeley users who have this article in their library.

Abstract

We have focused primarily on the 2001 September 24 solar energetic particle (SEP) event to verify previous indications of the presence of an outer reflecting boundary of SEPs. By using energetic electron and ion data obtained from multi-spacecraft observations, we have identified a collimated particle beam consisting of reflected particles returning from an outer boundary. The peak of reflected particles appears before the arrival of particles at 90° pitch angle. In addition, an onset time analysis is carried out in order to determine parameters characterizing the boundary. Our analysis suggests that the presence of a counter-streaming particle beam with a deep depression at 90° pitch angle during the onset phase is evidence for a nearby reflecting boundary. We have compared this property in the SEP events of 2002 April 21 and August 24. A reflecting boundary that blocks a flux tube is important in space weather forecasting since it can cause the "reservoir" effect that may enhance the intensity and duration of high-energy particles. © 2009 The American Astronomical Society. All rights reserved.

Cite

CITATION STYLE

APA

Tan, L. C., Reames, D. V., Ng, C. K., Saloniemi, O., & Wang, L. (2009). Observational evidence on the presence of an outer reflecting boundary in solar energetic particle events. Astrophysical Journal, 701(2), 1753–1764. https://doi.org/10.1088/0004-637X/701/2/1753

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free