The variation of solar proton energy spectra and size distribution with heliolongitude

Details The variation of solar proton energy spectra and size distribution with heliolongitude The variation of solar proton energy spectra and size distribution with heliolongitude

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...41..189v&link_type=abstract

Solar Physics, vol. 41, Mar. 1975, p. 189-223.

Physics

92

Energy Spectra, Particle Size Distribution, Proton Energy, Solar Flares, Solar Protons, Data Reduction, Solar Activity Effects, Solar Corona, Solar Cosmic Rays, Statistical Analysis, Tables (Data)

Scientific paper

A statistical study of the initial phases of a large number of solar particle events provides an approach for an investigation of the variability in the production process and coronal diffusion. A description is given of the procedures which are suitable for identifying the parent flare of an event, taking into account the heliocentric distribution of the flare-associated events. The determination of the proton energy spectrum at the sun is discussed along with the variation of the spectral index with the associated flare heliocentric longitude, questions concerning the source spectra and the acceleration process, and the size distribution of flare associated particle events.

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