The solution of the radio transfer equation in a plasma with constant pressure and conductive flux

Details The solution of the radio transfer equation in a plasma with constant pressure and conductive flux The solution of the radio transfer equation in a plasma with constant pressure and conductive flux

May 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....48..359n&link_type=abstract

Astronomy and Astrophysics, vol. 48, no. 3, May 1976, p. 359-365.

Astronomy and Astrophysics

Astrophysics

5

Brightness Temperature, Optical Thickness, Plasma Radiation, Radiative Transfer, Solar Radio Emission, Integral Equations, Pressure Effects, Refractivity, Temperature Effects, Thermal Emission

Scientific paper

The thermal radio emission from a layer of plasma in conductive equilibrium and with constant pressure is studied for propagation perpendicular to the layer. The temperature dependence of the optical depth is given, and the effect of the deviation of the refractive index from unity is discussed. The transfer equation is solved, the dependence of the brightness temperature on frequency, pressure, conductive flux, and highest temperature is discussed, and some approximate formulas are given.

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