Parameters of the Plasma Affecting the Radiation of Pulsar 1

Details Parameters of the Plasma Affecting the Radiation of Pulsar 1 Parameters of the Plasma Affecting the Radiation of Pulsar 1

May 1968

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1968sci...160..760t&link_type=abstract

Science, Volume 160, Issue 3829, pp. 760

Astronomy and Astrophysics

Astronomy

13

Scientific paper

Analysis of the relation between time delay and frequency for pulses from Pulsar 1 shows that the dispersive region of the ray path must exceed 300 astronomical units and have an average electron number density less than 8000 per cubic centimeter and average magnetic field strength less than 2 × 10-3 gauss. These requirements almost guarantee that the observed dispersion takes place in the interstellar medium.

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