Continuum absorption in the solar EUV spectra

Details Continuum absorption in the solar EUV spectra Continuum absorption in the solar EUV spectra

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.119...17n&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Astronomy and Astrophysics

Astrophysics

Absorption Spectra, Continuous Spectra, Extreme Ultraviolet Radiation, Solar Spectra, Ultraviolet Spectra, Optical Thickness, Stellar Spectrophotometry, Temperature Dependence, Transition Points

Scientific paper

The weakening of solar EUV line emission originating in the chromosphere-corona transition region, as it passes through the cool chromospheric material above the EUV-emitting region, has been noted to occur even at the disk center of the quiet sun. Calculations are here presented for the weakening of 11 ions, in order to examine the wavelength dependence of the weakening. The results obtained indicate that weakening increases with increasing wavelength below 912 A; the linearity of the weakening supports the cloud model of Nishikawa (1983).

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