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NASA NTRS ยท 19880031870

A pulsar emission model - Observational tests

Abstract

The usual model for coherent radio emission, curvature radiation from bunches, is applied here to a modified 'hollow cone' model in which only one or a few geometrically fixed flux tubes are radiating into a fan beam. The way that the model handles the basic problems of sufficient radio power output, reasonable spectrum, and narrow pulses as well as the secondary issues of orthogonal mode changing, complex pulse profiles is addressed. Issues that seem more model-dependent, including flux tube scales, nulling, self-absorption, drifting subpulses, and radius-to-frequency mapping, are examined by considering a specific global model.

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BibTeXRIS

Michel, F. Curtis. 1987-11-15. A pulsar emission model - Observational tests. https://ntrs.nasa.gov/citations/19880031870

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