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Author Klein K-L, Masson S, Bouratzis C, Grechnev V, Hillaris A, Preka-Papadema P,
Title The relativistic solar particle event of 2005 January 20: origin of delayed particle acceleration Type Journal Article
Year (down) 2014 Publication Astronomy & Astrophysics Abbreviated Journal 0004-6361
Volume 572 Issue Pages A4-A4
Keywords
Abstract The highest energies of solar energetic nucleons detected in space or through gamma-ray emission in the solar atmosphere are in the GeV range. Where and how the particles are accelerated is still controversial. We search for observational evidence on the acceleration region(s) by comparing the timing of relativistic protons detected at Earth and radiative signatures in the solar atmosphere during the particularly well observed 2005 Jan 20 event. This investigation focusses on the post-impulsive flare phase, where a second peak was observed in the relativistic proton time profile by neutron monitors. This time profile is compared in detail with UV imaging and radio spectrography over a broad frequency band from the low corona to interplanetary space.It is shown that the late relativistic proton release to interplanetary space was accompanied by a distinct new episode of energy release and electron acceleration in the corona traced by the radio emission and by brightenings of UV kernels. These signatures are interpreted in terms of magnetic restructuring in the corona after the CME passage. We attribute the delayed relativistic proton acceleration to magnetic reconnection and possibly turbulence in large- scale coronal loops. While type II radio emission was observed in the high corona, no evidence of a temporal relationship with the relativistic proton acceleration was found.
Programme 227
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Corporate Author Thesis
Publisher EDP Sciences Place of Publication Editor
Language Summary Language Original Title
Series Editor Series Title Abbreviated Series Title
Series Volume Series Issue Edition
ISSN 0004-6361 ISBN Medium
Area Expedition Conference
Notes Approved yes
Call Number Serial 5829
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