Geometrical effects on radio pulsar profiles and spectra.

Details Geometrical effects on radio pulsar profiles and spectra. Geometrical effects on radio pulsar profiles and spectra.

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...321..519s&link_type=abstract

Astronomy and Astrophysics, v.321, p.519-522

Astronomy and Astrophysics

Astrophysics

13

Pulsars: General, Radiation Mechanisms: General

Scientific paper

Considering the geometry of the hollow-cone model of radio pulsar emission in detail, one is led to the conclusion that several well-known observed effects may be explained quite easily purely on geometrical terms. It can be shown e.g. that the appearance of out-riders at high frequencies and a steepening of the whole spectrum (cut-off) must be expected for certain geometrical situations as well as variations in component spectra, e.g. a steepening of the central (core) component. These effects appear in addition to the presumably also existing physical variations with frequency.

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