Determine the Larmor frequency and the gyration frequency for the following cases: (a) A proton in the solar wind has a temperature of 100,000 K and a magnetic fl ux density of 5 nT. (b) An electron has an energy of 3 keV, a pitch angle of 30 deg, and is in the geomagnetic fi eld with a magnetic fl ux density of 30,000 nT. (c) A He+ ion has a kinetic energy of 1 keV in the photosphere of the sun with a magnetic fl ux density of 0.01 T.
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