Some properties of the continuous latitude distributions of the brightness of the K and F coronas as deduced from the LASCO data

Author:

Fainshtein V. G.,Kashapova L. K.,Tsivileva D. M.

Publisher

Pleiades Publishing Ltd

Subject

Space and Planetary Science,Geophysics

Reference3 articles.

1. V. G. Fainshtein, “New Method for Separating K and F Corona Brightness Using the LASCO/SOHO Data,” Soln.-Zemn. Fiz., No. 10, 44–53 (2007a).

2. V. G. Fainshtein, “Some Properties of the Latitude Brightness Distributions in the K and F Coronae According to SOHO/LASCO Data,” Astron. Zh. 84(12), 1135–1145 (2007) [Astron. Rep. 51 (12), 1026–1035 (2007b)].

3. A. P. Hayes, A. Vourlidas, and R. A. Howard, “Deriving the Electron Density of the Solar Corona from the Inversion of Total Brightness Measurements,” Astrophys. J. 548, 1081–1086 (2001).

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