THE DETERMINATION OF THE OPTICAL DEPTH OF GRAINS OF CONTINUOUS EMISSION IN SOLAR FACULAE,
Abstract
The weakening of continuous emission in the wings of strong H and K lines of Ca was used for determining the optical depth (in the frequency of the continuous spectrum) of the grains of con tinuous emission. For 7 investigated grains it was found to vary from tau 0 to tau 1.0. It is shown that the rise and fall in the wings of H and K in the grains in comparison to the undisturbed photosphere can be explained by the influence of continuous emission at different depths. (Author)
Document Details
- Document Type
- Technical Report
- Publication Date
- Jan 01, 1963
- Accession Number
- AD0413001
Entities
People
- V.l. Khokhlova