Model for the microstructure emission of pulsars

Details Model for the microstructure emission of pulsars Model for the microstructure emission of pulsars

May 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mnras.179..311b&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 179, May 1977, p. 311-315.

Astronomy and Astrophysics

Astronomy

21

Coherent Radiation, Microstructure, Pulsars, Stellar Models, Stellar Radiation, Dense Plasmas, Filaments, Fine Structure, Plasma Radiation, Radio Spectra, Relativistic Plasmas

Scientific paper

The recent observations of Rickett, Hankins, and Cordes (1975) are used
to construct a qualitative model of the emitting region near pulsars.
Their data can be reconciled with the view that dense regions,
themselves containing many coherent radiating filaments, extend for long
distances along the dipolar field lines.

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