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Solar vector magnetic field measurements
Paper "Solar photosphere magnetization".
atom-radiation anisotropic interaction
- density matrix formalism
atom-electron and atom-ion anisotropic interaction
- semi-classical collision theory
In order to solve the problem of non-zero divergence of the magnetic field observed in solar photosphere, thermal escape of solar interior electrons is proposed. They migrate very slowly towards the surface layers. What is measured by Zeeman effect is the solar magnetic field H, which is related to the divergence-free magnetic induction B by the law B=µ0(H+M), where M is the magnetization. To get sufficient magnetization for the problem, the photosphere charged particles density has to be substantially higher than presently very indirectly estimated. The proposal follows.
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