Implications of Liouville's theorem on the apparent brightness temperatures of solar radio bursts

Details Implications of Liouville's theorem on the apparent brightness temperatures of solar radio bursts Implications of Liouville's theorem on the apparent brightness temperatures of solar radio bursts

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..116..141m&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 116, no. 1, 1988, p. 141-156.

Physics

16

Brightness Temperature, Liouville Theorem, Solar Radio Bursts, Astronomical Models, Milne Method, Plasma Radiation

Scientific paper

Liouville's theorem for radiation, of which the generalized étendue is a consequence, implies μ2d2Ωd2A = constant along the ray path, where μ is the refractive index and d2Ω and d2A are the ranges, respectively, of solid angle and of area that define a ray (actually a bundle of rays). Implications of this concept on the propagation of radio waves from the actual to the apparent source in the solar corona (i.e., the scatter image of the true source) are discussed.

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