Sustained Energetic Particle Intensity Enhancements at Voyager 1 Beginning in 2002

Details Sustained Energetic Particle Intensity Enhancements at Voyager 1 Beginning in 2002 Sustained Energetic Particle Intensity Enhancements at Voyager 1 Beginning in 2002

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....7.3893h&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

A possible explanation for the large low-energy enhancement of outer heliospheric ion and electron intensities observed at Voyager 1 (V1) during 2002/213 to 2003/035 is an encounter with the solar wind termination shock (TS) [4]. We study the energy spectra of H, He, C, & O ions around this time period and, using the anomalous cosmic ray (ACR) species scaling [2], find the enhancement to be consistent with an ACR population.

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