Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...322..522a&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 322, Nov. 1, 1987, p. 522-543. Research supported by the Ministero della Pu
Astronomy and Astrophysics
Astrophysics
36
Calcium, Coronal Loops, Emission Spectra, Plasma Heating, Solar Flares, Stellar Models, Line Shape, Solar Spectra, Temperature Distribution, Temporal Distribution
Scientific paper
Spectral profiles synthesized from the results of numerical simulations of solar coronal loop plasma are compared with the observed line profiles, and the sensitivity of this comparison to variations in the parameter values is tested. The comparison allows the procedures commonly adopted for obtaining temperatures and velocities directly from the bent crystal spectrometer observations, as well as the interpretation of parameters obtained from hydrodynamical calculations, to be independently validated. The characteristic spectral signatures of different models for the deposition of impulsive thermal energy in the loop are derived assuming two distinct spatial distributions of thermal heating: in one case, the heating function peaks near the apex of the loop, while in the second, energy is deposited directly in the lower atmosphere.
Antonucci Ester
Dodero Maria Adele
Peres Giovanni
Rosner Robert
Serio Salvatore
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