𝔖 Bobbio Scriptorium
✦   LIBER   ✦

On physical conditions in the chromosphere above sunspot umbrae

✍ 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

No coin nor oath required. For personal study only.

✦ 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.


πŸ“œ SIMILAR VOLUMES


The chromosphere above a sunspot umbra
✍ H. A. Beebe; W. E. Baggett; H. S. Yun πŸ“‚ Article πŸ“… 1982 πŸ› Springer 🌐 English βš– 504 KB

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 the inhomogeneous structure of the ch
✍ J. Staude πŸ“‚ Article πŸ“… 1985 πŸ› John Wiley and Sons 🌐 English βš– 398 KB πŸ‘ 2 views

Zentralinstitut fiir Astrophysik der Akadcmic der Wissenschaftcn der DDR Sonneiiol~servatoriuin Einsteintnrni IVitli 5 f i p r e s (Rcceivctl 1984 Sovembrr 30) Multiple wavelength observations of sunspot umbrae can only be expalined by an inhomogeneous, two-component model for the structure of the u