Relative Timing of Interacting Solar Flare Particles and Particles Seen in Space and at the Earth

Details Relative Timing of Interacting Solar Flare Particles and Particles Seen in Space and at the Earth Relative Timing of Interacting Solar Flare Particles and Particles Seen in Space and at the Earth

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agufmsh31c..10c&link_type=abstract

American Geophysical Union, Fall Meeting 2001, abstract #SH31C-10

Physics

7519 Flares, 7554 X Rays, Gamma Rays, And Neutrinos

Scientific paper

The observations of meson-decay gamma-rays, relativistic electron bremsstrahlung, and high-energy neutrons by spacecraft instruments and ground-level neutron monitors provide crucial diagnostics for identifying the properties of particle acceleration mechanisms. Using available data and analyses from several missions, we have studied the relative timing between particles accelerated and interacting at the sun and the observation of charged particles in space and at ground level. Radio spectrograph and imaging data are used to determine the time of coronal particle acceleration episodes. We will present results, for several events, on the accuracy of determining the earliest time of acceleration of the interacting particles compared with the time particles are observed. Requirements will be presented for future studies of high energy neutral solar emissions.

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