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Diagnostics of solar ions: Ne VI, Mg VI, Si VIII and Mg VIII observed by SERTS

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Abstract

Diagnostics of solar ions Nevi, Mgvi, Siviii, and Mgviii in an active region observed by SERTS have been presented. Density, temperature, and electron pressure in the emitting source have been derived from theoretical line-ratio curves and its EUV spectrum obtained by SERTS. The variation of neon-to-magnesium and silicon-to-magnesium abundances has been discussed in the interpretation of the active region spectrum obtained by SERTS.

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Authors and Affiliations

  1. Department of Applied Physics, Institute of Technology, Banaras Hindu University, 221 005, Varanasi, India

    B. N. Dwivedi & Anita Mohan

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  1. B. N. Dwivedi
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  2. Anita Mohan
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Dwivedi, B.N., Mohan, A. Diagnostics of solar ions: Ne VI, Mg VI, Si VIII and Mg VIII observed by SERTS. Sol Phys 156, 81–94 (1995). https://doi.org/10.1007/BF00669577

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  • DOI: https://doi.org/10.1007/BF00669577

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