On the structure of pulsar magnetosphere

Details On the structure of pulsar magnetosphere On the structure of pulsar magnetosphere

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011yera.confe..30n&link_type=abstract

The 41st Young European Radio Astronomers Conference, held at University of Manchester/Jodrell Bank Observatory, 18-20 July 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

The angle BETA between rotation and magnetic axes are calculated by two methods for 283 radio pulsars at the wavelength 10 cm, 132 ones at 20 cm and 80 objects at the wavelength near 30 cm. The common average of the angle BETA is 43.5 degrees. Some effects which can give errors in the values of BETA are discussed. There are no correlations between values of BETA and pulsar ages.

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