The predicted response of the Solar-A Soft X-ray Telescope (SXT) to various solar targets is presented. It is found that the SXT is very sensitive and should be able to observe active regions and flares at its nominal cadence with exposure times ranging from 0.0001 to 1 s. The SXT temperature diagnostic capabilities are presented for various combinations of the X-ray filters.


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    Titel :

    Plasma diagnostic capabilities of the Soft X-ray Telescope on Solar-A


    Beteiligte:
    Strong, K. T. (Autor:in) / Acton, L. W. (Autor:in) / Brown, W. A. (Autor:in) / Claflin, E. S. (Autor:in) / Lemen, J. R. (Autor:in)


    Erscheinungsdatum :

    1991-01-01



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    Plasma diagnostic capabilities of the Soft X-Ray Telescope on Solar-A

    Strong, K.T. / Acton, L.W. / Brown, W.A. et al. | Elsevier | 1991


    Spectral diagnostic capabilities of Solar-B EIS

    Zanna, G.Del | Online Contents | 2005


    Spectral diagnostic capabilities of Solar-B EIS

    Zanna, G. Del / Mason, H.E. | Elsevier | 2005


    Spectral diagnostic capabilities of Solar-B EIS

    Zanna, G. D. / Mason, H. E. / Committee on Space Research | British Library Conference Proceedings | 2005