We study the influence of faculae on sunspot heat blockage using a thermal model based on eddy heat diffusion through the convection zone. The facula is represented as a localized area of excess emission surrounding the sunspot, which is represented as a thermal plug. Our computations using a range
β¦ LIBER β¦
The influence of the sunspot model on the Li-abundance
β Scribed by G. Stellmacher; E. Wiehr
- Publisher
- Springer
- Year
- 1971
- Tongue
- English
- Weight
- 197 KB
- Volume
- 21
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
The influence of faculae on sunspot heat
β
Wei-Hwan Chiang; Peter Foukal
π
Article
π
1985
π
Springer
π
English
β 580 KB
A model of the sunspot umbra
β
S. M. Chitre; G. Shaviv
π
Article
π
1967
π
Springer
π
English
β 500 KB
Suggestions of sunspot influence on the
β
Alexander B. MacDowall
π
Article
π
2007
π
John Wiley and Sons
π
English
β 465 KB
The influence of the sunspot cycle on ph
β
C.W. Allen
π
Article
π
1964
π
Elsevier Science
π
English
β 446 KB
The Influence of Reaction Rates on the F
β
W. Rapp; M. Wiescher; H. Schatz; F. KΓ€ppeler
π
Article
π
2005
π
Elsevier Science
π
English
β 106 KB
Mathematical modelling of the sunspot cy
β
F. Meyer
π
Article
π
1981
π
Springer
π
English
β 631 KB
The sunspot record for the time interval 1749-1977 can be represented conveniently by an harmonic model comprising a relatively large number of lines. Solar activity can otherwise be considered as a sequence of partly overlapping events, triggered periodically at intervals of the order of 11 years.