VLF electromagnetic radiation from pulsars in interstellar medium

Details VLF electromagnetic radiation from pulsars in interstellar medium VLF electromagnetic radiation from pulsars in interstellar medium

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976azh....53..527d&link_type=abstract

Astronomicheskii Zhurnal, vol. 53, May-June 1976, p. 527-533. In Russian.

Astronomy and Astrophysics

Astronomy

Pulsars, Radio Astronomy, Stellar Radiation, Very Low Frequencies, Whistlers, Interstellar Space, Magnetic Dipoles, Quadrupoles, Radio Emission

Scientific paper

Whistler mode radiation from pulsars in the interstellar medium is considered. An oblique magnetic rotator is used as a possible source of emission. Formulas are derived for the total power of whistler mode emission from magnetic dipoles and quadrupoles. Special attention is given to the dependence of the radiated power upon frequency. This concept is used for the explanation of the relation, established between the period and its first and second time derivations for Crab pulsar PSRO 532.

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