Estimate the value of the magnetic field of a star (rotation
period T= 10^6 sec, radius R = 10^12 cm, surface temperature T=10^3
K) that can be determined by observing the Zeeman effect for the
visible range of the hydrogen spectrum.
Estimate the value of the magnetic field of a star (rotation period T= 10^6 sec, radius R = 10^12 cm, surface temperatur
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Estimate the value of the magnetic field of a star (rotation period T= 10^6 sec, radius R = 10^12 cm, surface temperatur
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