Physics
Scientific paper
Mar 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...269..496l&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 269, no. 1-2, p. 496-502.
Physics
10
Coronal Loops, H Alpha Line, Solar Flares, Solar Limb, Solar Physics, Solar Spectra
Scientific paper
The profiles of H-alpha spectra lines of the loop prominence system on February 18, 1984 at the eastern solar limb are calculated in this paper. The following four 2D fields of physical parameters are obtained: (1) the velocity along the line-of-sight V(parallel); (2) the column number density of the hydrogen atoms at the second level N0,2; (3) the excitation temperature T(exc); and (4) the microturbulence velocity (Vt). The computed results show that the velocities V(parallel) at both the top and the low part of a single loop are smaller than those at the middle. The column number densities at the southern limb are the largest in the loop system. The excitation temperature at the southern limb is higher than elsewhere. The southern position is perhaps the site of the original flare core. In this loop system, V(parallel) goes up to 60 km/s, N0,2 varies from 0.15 to 1.0 x 10 exp 13/sq cm, T(exc): 6000-20,000 K, electron density n(e): 10 exp 11 - 10 exp 12/cu cm, electron pressure P(e): 0.10-10 dyn/sq cm.
Ding Yujie J.
Gu Xiao-Ma
Li Kai-Jun
Li Qi-Sheng
Li Qiu-Yan
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