Abstract The PHEBUS observations show that short duration hard X-ray/gamma-ray bursts detected above generally exhibit subsecond time structures. On the contrary, long duration events do not show fast time variations and usually consist in ⋍ one minute duration peaks superposed on a less intense and slowly varying component.
Temporal characteristics of solar hard X-ray/gamma-ray bursts observed by PHEBUS
Advances in Space Research ; 13 , 9 ; 171-174
01.01.1993
4 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
The E p distribution of long-duration γ-ray bursts observed by the PHEBUS experiment
Online Contents | 2006
|PHEBUS: un satellite polyvalent
Tema Archiv | 1977
|Different temporal behaviours in the gamma-ray bursts
Elsevier | 1991
|Gamma ray bursts flares detected and observed by the Swift satellite
Online Contents | 2007
|