Beam Width of Solar Electron Bursts Observed Below 1.3 keV

Details Beam Width of Solar Electron Bursts Observed Below 1.3 keV Beam Width of Solar Electron Bursts Observed Below 1.3 keV

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agufmsh21c0438d&link_type=abstract

American Geophysical Union, Fall Meeting 2004, abstract #SH21C-0438

Physics

7807 Charged Particle Motion And Acceleration, 7859 Transport Processes, 2118 Energetic Particles, Solar

Scientific paper

We present a statistical analysis of the beam width of solar electron bursts at energies below 1.3 keV using electron detectors on board the ACE and Genesis spacecraft. Pitch-angle dispersion is typically observed at the beginning of each event, leading to broadening of the pitch-angle distribution as the event progresses. By the time of peak intensity, some bursts have a pitch-angle distribution which is broader than the preceding strahl, although this is not universally true. We discuss the implication of these results for electron injection/acceleration at the Sun and electron propagation in the heliosphere.

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