Tomographic Studies of Pulsar Radio Emission Cones and Searches for Radio Counterparts of Gamma-Ray Pulsars
Radio emission from pulsars is believed to originate from charged particles streaming along the open magnetic field lines, radiating within a narrow cone at each of the two magnetic poles. In each rotation of the star, the emission beam sweeping across the observer’s line of sight, is seen as a puls...
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| Language: | en_US |
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2018
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| Online Access: | http://etd.iisc.ernet.in/2005/3432 http://etd.iisc.ernet.in/abstracts/4299/G25946-Abs.pdf |