Pulse fluctuation properties at 35 MHz
| dc.contributor.author | Asgekar, Ashish | |
| dc.contributor.author | Deshpande, A A | |
| dc.date.accessioned | 2007-06-04T08:02:33Z | |
| dc.date.available | 2007-06-04T08:02:33Z | |
| dc.date.issued | 2000 | |
| dc.description | Restricted Access. An open-access version is available at arXiv.org (one of the alternative locations). Pulsar Astronomy - 2000 and Beyond, ASP Conference Series, Vol. 202; Proceedings of the 177th Colloquium of the IAU held in Bonn, Germany, 30 August - 3 September 1999. (San Francisco: ASP). Eds. M. Kramer, N. Wex, and N. Wielebinski, p. 161 | en |
| dc.description.abstract | High time-resolution observations of pulsars were carried out at 35 MHz, using the Gauribidanur Radio Telescope (India), to study the spectra of intrinsic pulse-to-pulse fluctuations. Our sample consists of a few bright pulsars, each of which was observed for $\sim$1000~seconds so as to obtain long sequences of single-pulse data. The results, in terms of fluctuation features apparent at this radio frequency, are presented and compared with similar measurements at higher frequencies. We show that the picture of a circulating system of sub-beams emerges naturally from the behaviour apparent even at these long wavelengths. | en |
| dc.format.extent | 193783 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.identifier.citation | ASP Conference Series, 2000, Vol.202, p161 | en |
| dc.identifier.uri | http://hdl.handle.net/2289/2564 | |
| dc.language.iso | en | en |
| dc.publisher | Astronomical Society of the Pacific | en |
| dc.relation.uri | http://adsabs.harvard.edu/cgi-bin/bib_query?2000ASPC..202..161A | en |
| dc.relation.uri | http://arxiv.org/abs/astro-ph/9911428 | en |
| dc.rights | 2000 Astronomical Society of the Pacific | en |
| dc.title | Pulse fluctuation properties at 35 MHz | en |
| dc.type | Article | en |