Radio pulsar emission altitudes

dc.contributor.author	Kapoor, R. C
dc.contributor.author	Shukre, C. S
dc.date.accessioned	2008-07-22T07:44:03Z
dc.date.available	2008-07-22T07:44:03Z
dc.date.issued	2002-09
dc.identifier.citation	BASI, Vol. 30, No. 3, pp. 695 - 696	en
dc.identifier.uri	http://hdl.handle.net/2248/2794
dc.description.abstract	By attributing the often seen longitude offsets between the core and conal component centres of pulsar radio pulses to different emission altitudes, we present a new method for investigating these altitudes. OUf method can explain these offsets and also sheds light on them.	en
dc.format.extent	33677 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Radio Pulsar Emission Altitudes	en
dc.subject	Magnetic Field Line	en
dc.title	Radio pulsar emission altitudes	en
dc.type	Article	en