Investigation of HeI 10830 Å `Dark Points' at the Sayan Solar Observatory and the Baikal Astrophysical Observatory

Details Investigation of HeI 10830 Å `Dark Points' at the Sayan Solar Observatory and the Baikal Astrophysical Observatory Investigation of HeI 10830 Å `Dark Points' at the Sayan Solar Observatory and the Baikal Astrophysical Observatory

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001soph..199...37s&link_type=abstract

Solar Physics, v. 199, Issue 1, p. 37-45 (2001).

Physics

Scientific paper

A new two-bandpass birefringent filter has been produced at ISTP, Irkutsk for the investigation of the fine structure of the chromosphere. One filter passband is centered on the Hei 10830 Å line, the second one is centered on Hα. The FWHM of the Hei 10830 Å passband is 0.46 Å and of the Hα passband is 0.3 Å. A large number of filtergrams were obtained with the filter at the Sayan observatory. At the same time, spectral observations with high spatial and spectral resolution were carried out by the large solar vacuum telescope at the Baikal Observatory. We selected 29 `dark point' spectra with sizes from 2'' to 13'', as well as `dark points' on the filtergrams. Comparison of spectrograms and filtergrams has shown a good agreement of their size and intensity in relation with the surrounding chromosphere as well as the absence of primary line-of-sight velocities in both observation types. From spectral observations, the depth of 10830 Å is over 30% for some `dark points', and the FWHM is more than 1 Å. Hei 10830 Å line profiles in `dark points' are more deep and wide than in quiet regions. The optical depth of the chromosphere in `dark points' is estimated. Comparison with the unperturbed chromosphere showed that `dark points' in Hei 10830 Å are more optically thin than the nearby chromosphere.

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