The pulsar magnetosphere - The unsolved problem

Details The pulsar magnetosphere - The unsolved problem The pulsar magnetosphere - The unsolved problem

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979s%26w....18..348r&link_type=abstract

Sterne und Weltraum, vol. 18, Oct. 1979, p. 348-352. In German.

Astronomy and Astrophysics

Astrophysics

Neutron Stars, Pulsar Magnetospheres, Pulsars, Stellar Atmospheres, Astrophysics, Field Strength, Stellar Magnetic Fields, Stellar Rotation

Scientific paper

An attempt is made to determine the global relationship between a neutron star and its surroundings. A review of the development of neutron star physics is presented, and attention is given to the theory that a pulsar is a rotating neutron star. The application of unipolar induction to determining the existence of a pulsar magnetosphere is discussed in the aligned rotator case. It is determined that a pulsar, identified as a quickly rotating neutron star with a strong magnetic field, is capable of converting its rotational energy into field and kinetic energy of high efficiency.

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