𝔖 Bobbio Scriptorium
✦   LIBER   ✦

A three-component concept of the chromosphere and transition region

✍ Scribed by Peter Foukal

Publisher
Springer
Year
1974
Tongue
English
Weight
293 KB
Volume
37
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

πŸ“œ SIMILAR VOLUMES

Interpretation of the solar continuum fr
Interpretation of the solar continuum from 1680 to 600 Γ…. Model of the transition region photosphere-chromosphere and of the chromosphere
✍ Yvette Cuny πŸ“‚ Article πŸ“… 1971 πŸ› Springer 🌐 English βš– 867 KB

An interpretation is given of the observations of the continuous solar radiation in the spectral range 600-1700 A. The model allows for deviations from LTE of H, C, Si and S, and is in hydrostatic equilibrium. The predicted intensity from 1680 to 1520/~ has virtually no dependence on the electron te

A three-component model for the formatio
A three-component model for the formation of the chromospheric CaiiK line
✍ P. R. Wilson πŸ“‚ Article πŸ“… 1970 πŸ› Springer 🌐 English βš– 481 KB

A recent two-component model for the formation of the Ca II K line in the solar chromosphere put forward by Beebe and Johnson is discussed. Although this model is a great advance on existing one-component models, it is pointed out that observations require a minimum of three components in order to u

On the inhomogeneous structure of the ch
On the inhomogeneous structure of the chromosphere-corona transition region above sunspot umbrae
✍ 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