AbstractBy using radio data from ground-based telescopes (from 270 MHz to 25 MHz), and from the Radio and Plasma Wave experiment (WAVES) on board the WIND spacecraft (1–14 MHz and several kHz-11 MHz), as well as FY -2 satellite data, the origin of coronal and interplanetary shock and particle acceleration of the 14 July 2000 flare/CME event (the Bastille day event) have been studied. Main conclusions are as follows: (1) We investigate the causal relationship between metric type 11 bursts observed by the digital IZMIRAN radio spectrograph and type II radio emissions in the frequency range from 1–14 MHz and several kHz-11 MHz observed by the WAVES/WIND. The analysis indicate that the fast CME is the origin of both coronal and interplanetary shocks. (2)According to the time profiles of Hard X-ray, and energetic particles (include proton, 3He, and 4He) from FY-2 satellite, it is obvious that the Bastille day event is the event, in which both impulsive and gradual phenomena occur. The energetic particles accelerated not only in flare but also in CME.


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    Title :

    Origin of coronal and interplanetary shock and particle acceleration of a flare/CME event


    Contributors:
    Tang, Y.H. (author) / Dai, Y. (author)

    Published in:

    Advances in Space Research ; 32 , 12 ; 2609-2612


    Publication date :

    2003-03-20


    Size :

    4 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English




    Origin of Coronal and Interplanetary Shock and Particle Acceleration of a Flare/CME Event

    Tang, Y. H. / Dai, Y. / International Council of Scientific Unions | British Library Conference Proceedings | 2003




    Solar and interplanetary particle acceleration

    Simnett, G.M. | Elsevier | 2002