Spectra of several strong lines of sunspots have been obtained with the Echelle spectrograph at the Vacuum Tower Telescope, Sacramento Peak Observatory. With a variety of model atmospheres, Ca II H, K, and 28498 line profiles were calculated using a non-LTE line formation procedure. In the present
On physical conditions in the chromosphere above sunspot umbrae
β Scribed by R. B. Teplitskaja; S. A. Grigoryeva (Efendieva); V. G. Skochilov
- Publisher
- Springer
- Year
- 1978
- Tongue
- English
- Weight
- 467 KB
- Volume
- 56
- Category
- Article
- ISSN
- 0038-0938
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β¦ Synopsis
By means of an inversion of H and K Ca II line profiles the temperature and electron density in the chromosphere above the umbrae of two sunspots have been estimated. The temperature gradient 5 K km -1 exceeds the corresponding values in both quiet regions and plages. At a height of about 1500 km the umbra becomes hotter than the quiet region. At a temperature of about 10 000 K the temperature gradient increases sharply. The electron density at 1500 km is approximately the same as that in the quiet chromosphere at the same height.
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