Table 1: Collision frequencies (in Hz) and magnetization ratio of electrons and protons in the photosphere for two altitudes h (in km) and for the magnetic field B₀=10^-2 T.
h $\nu_{\rm in}$ $\nu_{\rm ii}$ $\nu_{\rm en}$ $\nu_{\rm ei}$ $\Omega_{\rm i}/\nu_{\rm it}$ $\Omega_{\rm e}/\nu_{\rm et}$

0 $1.6\times 10^9$ $5\times 10^7$ $1.3\times 10^{10}$ $1.5\times 10^9$ $6\times 10^{-4}$ $1.1\times 10^{-1}$

250 $2.6\times 10^8$ $3.8\times 10^6$ $2.2\times 10^9$ $1.2\times 10^8$ $3.6\times 10^{-3}$ $7.3\times 10^{-1}$

**Table 1:** Collision frequencies (in Hz) and magnetization ratio of electrons and protons in the photosphere for two altitudes h (in km) and for the magnetic field B₀=10^-2 T.
h	$\nu_{\rm in}$	$\nu_{\rm ii}$	$\nu_{\rm en}$	$\nu_{\rm ei}$	$\Omega_{\rm i}/\nu_{\rm it}$	$\Omega_{\rm e}/\nu_{\rm et}$
0	$1.6\times 10^9$	$5\times 10^7$	$1.3\times 10^{10}$	$1.5\times 10^9$	$6\times 10^{-4}$	$1.1\times 10^{-1}$
250	$2.6\times 10^8$	$3.8\times 10^6$	$2.2\times 10^9$	$1.2\times 10^8$	$3.6\times 10^{-3}$	$7.3\times 10^{-1}$

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