Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/46687
Title: The first SEPServer event catalogue 68-MeV solar proton events observed at 1 AU in 1996-2010
Author: Vainio, Rami
Valtonen, Eino
Heber, Bernd
Malandraki, Olga E.
Papaioannou, Athanasios
Klein, Karl-Ludwig
Afanasiev, Alexander
Agueda Costafreda, Neus
Aurass, Henry
Battarbee, Markus
Braune, Stephan
Dröge, Wolfgang
Ganse, Urs
Hamadache, Clarisse
Heynderickx, Daniel
Huttunen-Heikinmaa, Kalle
Kiener, Jürgen
Kilian, Patrick
Kopp, Andreas
Sanahuja i Parera, Blai
Keywords: Sol
Partícules (Física nuclear)
Radiació solar
Electromagnetisme
Sun
Particles (Nuclear physics)
Solar radiation
Electromagnetism
Issue Date: Feb-2013
Publisher: EDP Sciences
Abstract: SEPServer is a three-year collaborative project funded by the seventh framework programme (FP7-SPACE) of the European Union. The objective of the project is to provide access to state-of-the-art observations and analysis tools for the scientific community on solar energetic particle (SEP) events and related electromagnetic (EM) emissions. The project will eventually lead to better understanding of the particle acceleration and transport processes at the Sun and in the inner heliosphere. These processes lead to SEP events that form one of the key elements of space weather. In this paper we present the first results from the systematic analysis work performed on the following datasets: SOHO/ERNE, SOHO/EPHIN, ACE/EPAM, Wind/WAVES and GOES X-rays. A catalogue of SEP events at 1 AU, with complete coverage over solar cycle 23, based on high-energy (~68-MeV) protons from SOHO/ERNE and electron recordings of the events by SOHO/EPHIN and ACE/EPAM are presented. A total of 115 energetic particle events have been identified and analysed using velocity dispersion analysis (VDA) for protons and time-shifting analysis (TSA) for electrons and protons in order to infer the SEP release times at the Sun. EM observations during the times of the SEP event onset have been gathered and compared to the release time estimates of particles. Data from those events that occurred during the European day-time, i.e., those that also have observations from ground-based observatories included in SEPServer, are listed and a preliminary analysis of their associations is presented. We find that VDA results for protons can be a useful tool for the analysis of proton release times, but if the derived proton path length is out of a range of 1 AU < s[3 AU, the result of the analysis may be compromised, as indicated by the anti-correlation of the derived path length and release time delay from the asso ciated X-ray flare. The average path length derived from VDA is about 1.9 times the nominal length of the spiral magnetic field line. This implies that the path length of first-arriving MeV to deka-MeV protons is affected by interplanetary scattering. TSA of near-relativistic electrons results in a release time that shows significant scatter with respect to the EM emissions but with a trend of being delayed more with increasing distance between the flare and the nominal footpoint of the Earth-connected field line.
Note: Reproducció del document publicat a: http://dx.doi.org/10.1051/swsc/2013030
It is part of: Journal of Space Weather and Space Climate, 2013, vol. 3, num. A12, p. 1-17
Related resource: http://dx.doi.org/10.1051/swsc/2013030
URI: http://hdl.handle.net/2445/46687
ISSN: 2115-7251
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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