Heliospheric Origin of Gamma-Ray Bursts
| dc.creator | Li, Ti-Pei | |
| dc.date | 1997-04-28 | |
| dc.date | 1997-05-29 | |
| dc.date.accessioned | 2026-07-07T08:58:26Z | |
| dc.date.available | 2026-07-07T08:58:26Z | |
| dc.description | Systematic variations of average observational characteristics and correlation properties between different parameters of gamma-ray bursts (GRBs) with time from 1991 April to 1994 September are revealed. It is hard to explain the observed long-term variability by variations of experimental conditions. The variability of GRB properties with the time scale of months to years, together with the similarity between GRBs, solar hard X-ray flares and terrestrial gamma-ray flashes, may indicate an origin of GRBs, at least partly, within the heliosphere. Large-voltage and high-temperature pinch plasma columns produced by disruptive electrical discharges in the outer heliosphere can generate hard X-ray and gamma-ray flashes with energy spectra and spectral evolution characters consistent with that observed in GRBs. | |
| dc.description | LaTex, epsfig. 20 pages, 17 figures, replace to correct the definition of Epk and revise Figs 12-15 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9704264 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9704264 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/147324 | |
| dc.subject | Astrophysics | |
| dc.title | Heliospheric Origin of Gamma-Ray Bursts | |
| dc.type | text |