Period Dependence of Radio Emission Altitudes in the Pulsar Magnetosphere

Details Period Dependence of Radio Emission Altitudes in the Pulsar Magnetosphere Period Dependence of Radio Emission Altitudes in the Pulsar Magnetosphere

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...273..563g&link_type=abstract

Astronomy and Astrophysics, Vol.273, NO. 2/JUNII, P. 563, 1993

Astronomy and Astrophysics

Astrophysics

27

Pulsars, Emission Geometry

Scientific paper

It is argued that the altitude of radio emission region depends on pulsar period approximately as . The emission originates near the polar cap in millisecond pulsars and a few hundred km away in longer period pulsars. The magnetic field in the emission region seems to be about 106 G independent of the pulsar period and characteristic age.

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