Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...238..343g&link_type=abstract
Astrophysical Journal, Part 1, vol. 238, May 15, 1980, p. 343-348. Research supported by the Smithsonian Institution;
Astronomy and Astrophysics
Astrophysics
112
Atmospheric Heating, Solar Corona, Solar Magnetic Field, Solar Temperature, Solar X-Rays, Electron Density Profiles, Field Strength, Scaling Laws, Solar Electrons, Solar Flux
Scientific paper
General considerations concerning the scaling properties of magnetic-field-related coronal heating mechanisms are used to build a two-parameter model for the heating of closed coronal regions. The model predicts the way in which coronal temperature and electron density are related to photospheric magnetic field strength and the size of the region, using the additional constraint provided by the scaling law of Rosner, Tucker, and Vaiana. The model duplicates the observed scaling of total thermal energy content with total longitudinal flux; it also predicts a relation between the coronal energy density (or pressure) and the longitudinal field strength modified by the region scale size.
Golub Leon
Maxson C.
Rosner Robert
Serio Salvatore
Vaiana Giuseppe S.
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