Physics
Scientific paper
Jun 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..471..613d&link_type=abstract
The solar wind nine conference. AIP Conference Proceedings, Volume 471, pp. 613-616 (1999).
Physics
Solar Wind Plasma, Sources Of Solar Wind
Scientific paper
On the basis of data on flare energetic particle (FEP) generation and propagation in the Heliosphere we calculate the space-time-energy distribution of these particles in the Heliosphere in the periods of great FEP events. On the basis of observation data and investigations of cosmic ray nonlinear processes in the Heliosphere we determine the space-time distribution of solar wind matter. Then we calculate the generation of gamma-rays by decay of neutral pions generated by nuclear interactions of FEP with solar wind matter and determine the expected space-time distribution of gamma-ray emissivity. Then we calculate the expected time variation of the angle distribution and spectra of gamma ray fluxes generated by interaction of FEP with solar wind matter for observations from the Earth or from space-probes on different distances from the Sun.
No associations
LandOfFree
Expected gamma-ray fluxes from solar wind in periods of great flare energetic particle events does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Expected gamma-ray fluxes from solar wind in periods of great flare energetic particle events, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Expected gamma-ray fluxes from solar wind in periods of great flare energetic particle events will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1496418