Possible evaluation of the magnetic field near pulsars from the beat frequency of atomic transitions

Details Possible evaluation of the magnetic field near pulsars from the beat frequency of atomic transitions Possible evaluation of the magnetic field near pulsars from the beat frequency of atomic transitions

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976sva....19..702r&link_type=abstract

(Astronomicheskii Zhurnal, vol. 52, Nov.-Dec. 1975, p. 1173-1177.) Soviet Astronomy, vol. 19, no. 6, 1976, p. 702-705. Translat

Astronomy and Astrophysics

Astronomy

2

Atomic Energy Levels, Beat Frequencies, Interstellar Magnetic Fields, Pulsars, Zeeman Effect, Atomic Excitations, Crab Nebula, Electron Transitions, Forbidden Transitions, Polarized Light

Scientific paper

For the determination of the magnetic field in astrophysical conditions the use of the 'beats' effect in the atomic transitions is suggested. The frequency of beats under the Zeeman split is proportional to the magnetic field; its Doppler spread is negligible. The synphase excitation of atoms can be accomplished by means of the short pulse of the linear polarized light. The concrete estimations are made for the case of the forbidden lines in the Crab nebula excited by the optic pulse of the pulsar NP 0531.

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