Diagnostics of solar ions: NE VI, MG VI, SI VIII and MG VIII observed by SERTS

Details Diagnostics of solar ions: NE VI, MG VI, SI VIII and MG VIII observed by SERTS Diagnostics of solar ions: NE VI, MG VI, SI VIII and MG VIII observed by SERTS

Jan 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995soph..156...81d&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 156, no. 1, p. 81-94

Physics

6

Abundance, Ions, Magnesium, Neon, Ratios, Silicon, Solar Atmosphere, Solar Physics, Electron Density (Concentration), Electron Energy, Electron Pressure, Emissivity, Extreme Ultraviolet Radiation, Line Spectra, Solar Spectra

Scientific paper

Diagnostics of solar ions Ne VI, Mg VI, Si VIII, and Mg VIII in an active region observed by the Solar EUV Rocket Telescope and Spectrograph (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-magnetism and silicon-to-magnetism abundances has been discussed in the interpretation of the active region spectrum obtained by SERTS.

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