An improved method has been developed to evaluate element abundances from emission line intensities of thin plasmas, depending on the differential emission measure (DEM) of the source. Observations made by the Solar EUV Rocket Telescope and Spectrograph (SERTS) Rocket EUV Spectrograph are used to perform a detailed analysis of the DEM distribution for temperatures larger than 10(exp 5) K in a solar active region. Comparison of the DEM distributions obtained by means of lines from different elements allows the verification of relative abundances for the most common elements of the solar corona, and gives an abundance estimates for the minor components, such as Na, Al, Ar, Cr, Mn and Zn.


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    Titel :

    Abundance determination in solar active region


    Beteiligte:
    Monsignori Fossi, B. C. (Autor:in) / Landini, M. (Autor:in) / Thomas, R. J. (Autor:in) / Neupert, W. M. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    1994-04-01



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    Abundance determination in solar active region

    Fossi, B.C.Monsignori / Landini, M. / Thomas, R.J. et al. | Elsevier | 1993


    Abundance Determination in Solar Active Region

    Monsignori Fossi, B.C. | Online Contents | 1994


    Abundance Determination in Solar Active Region

    Monsignori Fossi, B. C. / Landini, M. / Thomas, R. J. et al. | British Library Conference Proceedings | 1994


    Abundance variations in solar active regions

    Strong, K. T. / Lemen, J. R. / Linford, G. A. | NTRS | 1991


    Abundance variations in solar active regions

    Strong, K.T. / Lemen, J.R. / Linford, G.A. | Elsevier | 1991