Characterizing Radio Pulsar Polarizaition Profiles

Details Characterizing Radio Pulsar Polarizaition Profiles Characterizing Radio Pulsar Polarizaition Profiles

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...21110201r&link_type=abstract

American Astronomical Society, AAS Meeting #211, #102.01; Bulletin of the American Astronomical Society, Vol. 39, p.917

Astronomy and Astrophysics

Astrophysics

Scientific paper

Since their discovery, radio pulsars have provided a valuable tool in various areas of astrophysics. Radio pulsars are spinning neutron stars emitting electromagnetic radiation from their magnetic poles. Like a distant lighthouse, they are observed by their periodic bursts of radiation; however much is to be learned about their emission mechanism. We present a new method of characterizing radio pulsar polarization profiles using an objective statistic based on all four Stokes parameters. Various properties of this statistic are analyzed and possible applications are discussed.

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