Pulse Fluctuation Properties at 35 MHz
| dc.creator | Asgekar, Ashish | |
| dc.creator | Deshpande, A. A. | |
| dc.date | 1999-11-23 | |
| dc.date.accessioned | 2026-07-07T02:34:36Z | |
| dc.date.available | 2026-07-07T02:34:36Z | |
| dc.description | 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. | |
| dc.description | 2 pages, total 4 fig.s (2 color fig.s), to appear in Proceedings of IAU 177 : "Pulsar Astronomy - 2000 & Beyond", Ed. Kramer, Wex, & Wielebinski, ASP Conf. Series. Gzipped PS file also available from http://www.rri.res.in/~ashish/html_files/reprints.html | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9911428 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9911428 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/15310 | |
| dc.subject | Astrophysics | |
| dc.title | Pulse Fluctuation Properties at 35 MHz | |
| dc.type | text |