Electromagnetic radiation in a helical magnetic field

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3822

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DC Field	Value	Language
dc.contributor.author	Krishan, V	-
dc.date.accessioned	2008-09-23T13:44:40Z	-
dc.date.available	2008-09-23T13:44:40Z	-
dc.date.issued	1984	-
dc.identifier.citation	Astrophysical Letters, Vol. 24, No. 1, pp. 21 - 25	en
dc.identifier.issn	0888-6516	-
dc.identifier.uri	http://hdl.handle.net/2248/3822	-
dc.description.abstract	Electromagnetic radiation spectrum is studied in a helical magnetic field since such magnetic field configurations may be present in cosmic objects. It is shown that, by a proper choice of the spatial period of the magnetic field, one could get large amounts of power over a wide region of the electromagnetic spectrum. The peak in the radiation spectrum shifts toward higher frequencies as the spatial period of the magnetic helix is reduced. As an illustration, this mechanism is applied to the Crab Nebula pulsar NP 0532.	en
dc.language.iso	en	en
dc.relation.uri	http://ads.ari.uni-heidelberg.de/abs/1984ApL....24...21K	en
dc.subject	Astrophysics	en
dc.subject	Electromagnetic Radiation	en
dc.subject	Magnetic Field Configurations	en
dc.subject	Stellar Magnetic Fields	en
dc.subject	Angular Distribution	en
dc.subject	Crab Nebula	en
dc.subject	Helical Inducers	en
dc.subject	Pulsars	en
dc.title	Electromagnetic radiation in a helical magnetic field	en
dc.type	Article	en
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