The Effect of Solar Wind by Pulsar Observations

Details The Effect of Solar Wind by Pulsar Observations The Effect of Solar Wind by Pulsar Observations

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aipc.1357..136y&link_type=abstract

RADIO PULSARS: AN ASTROPHYSICAL KEY TO UNLOCK THE SECRETS OF THE UNIVERSE. AIP Conference Proceedings, Volume 1357, pp. 136-137

Astronomy and Astrophysics

Astronomy

Magnetic Fields, Radioastronomy, Rotation Measurement, Radiotelescopes, Gravitational Radiation, Magnetic Fields, And Other Observations, Radio, Microwave, Velocity, Acceleration, And Rotation, Radio Telescopes And Instrumentation, Heterodyne Receivers

Scientific paper

When the line of sight of a pulsar is close to the Sun, the electron
density and magnetic field from the solar wind will strongly affect the
dispersion and rotation measure of the pulsar. Here we present the
effect from pulsar observations and describe our model of the solar
wind.

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