Source-Function and Temperature Fluctuations in the Solar Photosphere. I. The Isotropic Approximation.

1964 ◽  
Vol 139 ◽  
pp. 1358 ◽  
Author(s):  
Frank N., Jr. Edmonds
Solar Physics ◽  
1969 ◽  
Vol 9 (2) ◽  
pp. 303-314 ◽  
Author(s):  
P. R. Wilson

Author(s):  
Ю.М. Белоусов ◽  
В.Н. Горелкин ◽  
И.В. Черноусов

AbstractThe quasi-mobility function of charge carriers with a specified energy for describing their dynamics using the kinetic equation is studied in the important case of two-term isotropic approximation. In the stationary case, the quasi-mobility function is independent of the source function of charge carriers and makes it possible to calculate the integral mobility. The correlation between the quasi-mobility and parameters of the system is analyzed. It is proved that this characteristic does not generally describe the contribution of charge carriers with a specified energy to the integral mobility. In the case of almost elastic scattering, the quasi-mobility, as is known, can have a clear physical meaning; however, in the case of the scattering of charge carriers at acoustic phonons in a solid, this quasi-mobility interpretation is found to be incorrect due to the specific features of the collision integral and the form of the quasi-mobility function.


1969 ◽  
Vol 1 (5) ◽  
pp. 195-196
Author(s):  
P. R. Wilson

Recently I have carried out a two-dimensional radiative-transfer analysis of the data given by Edmonds on centrelimb relative rms intensity fluctuations in terms of horizontal temperature fluctuations in the solar photosphere. Edmonds himself attempted an analysis of his data and found a ΔTrms which increased monotonically from about 300°K at unit mean optical depth (i.e. at a given physical depth) to 500°K at optical depth 3.


Solar Physics ◽  
1969 ◽  
Vol 6 (3) ◽  
pp. 364-380 ◽  
Author(s):  
P. R. Wilson

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