Anisotropy analysis by SOHO/ERNE

Details Anisotropy analysis by SOHO/ERNE Anisotropy analysis by SOHO/ERNE

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..201s&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

Solar Cosmic Rays: Anisotropy, Detectors

Scientific paper

High Energy Detector (HED) of SOHO/ERNE detects solar cosmic ray nuclei in the energy range from 12 to 120 MeV/n. It has a wide view cone (120° square), large geometric factor and a good angular resolution of 1°, and thus is a good instrument for the analysis of SCR angular distributions. In this work, a method to analyse the form of SCR directional distributions is presented. It is applied to three solar energetic particle events.

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