Abstract The PHEBUS observations show that short duration hard X-ray/gamma-ray bursts detected above ⋍ 70 keV 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.


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    Title :

    Temporal characteristics of solar hard X-ray/gamma-ray bursts observed by PHEBUS


    Contributors:
    Talon, R. (author) / Barat, C. (author) / Dezalay, J.-P. (author) / Vilmer, N. (author) / Trottet, G. (author) / Sunyaev, R. (author) / Terekhov, O. (author) / Kuznetsov, A. (author)

    Published in:

    Advances in Space Research ; 13 , 9 ; 171-174


    Publication date :

    1993-01-01


    Size :

    4 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English