Physics
Scientific paper
Jun 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992georl..19.1243r&link_type=abstract
Geophysical Research Letters (ISSN 0094-8276), vol. 19, no. 12, June 19, 1992, p. 1243-1246. Research supported by NASA.
Physics
47
Heliosphere, Particle Energy, Solar Electrons, Solar Flares, Ulysses Mission, Electrons, Ions, Magnetic Field Reconnection, Solar Wind, Solar X-Rays
Scientific paper
Ulysses observations at 2.5 AU of 38-315 keV electrons and 61-4752 keV ions during February-April 1991 suggest in several ways that, during periods of sustained high solar activity, the inner heliosphere serves as a 'reservoir' for low-energy solar particles. Particle increases were not associated one-to-one with large X-ray flares because of their poor magnetic connection, yet intensities in March-April remained well above their February levels. The rise phase of the particle event associated with the great flare of 2245UT March 22 lasted most of two days, while throughout the one-week decay phase, the lowest-energy ion fluxes were nearly equal at Ulysses and earth (IMP-8).
Armstrong Thomas P.
Gold Robert E.
Lanzerotti Louis J.
Roelof Edmond C.
Simnett George M.
No associations
LandOfFree
Low-energy solar electrons and ions observed at ULYSSES February-April, 1991 - The inner heliosphere as a particle reservoir 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 Low-energy solar electrons and ions observed at ULYSSES February-April, 1991 - The inner heliosphere as a particle reservoir, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Low-energy solar electrons and ions observed at ULYSSES February-April, 1991 - The inner heliosphere as a particle reservoir will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1205037