Physics
Scientific paper
Jan 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001soph..198..163s&link_type=abstract
Solar Physics, v. 198, Issue 1, p. 163-167 (2001).
Physics
13
Scientific paper
Based on the observed dependence of the mean charge of several elements (C, O, Ne, Mg, Si and Fe) on energy for the gradual event of 6 November 1997 we deduce plasma parameters in the accelerating site. This is done in the framework of a charge-consistent acceleration model which incorporates ionisation and recombination processes during heavy ion energization by a parallel shock wave. To obtain good fits to observations we have to assume for the product of the characteristic acceleration time and number density T^q_acN~ (3-10) ×10^9 s cm^-3 and temperature T=10^6 K of a plasma where all the elements under consideration originated.
Ostryakov Valery M.
Stovpyuk Marianna F.
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