The structure of the solar granulation has been analysed using computer-processed images of two very high resolution (0': 25) white-light pictures obtained at the Pic-du-Midi Observatory. The narrow dispersion in the distribution of granule sizes is not confirmed. On the contrary, it is found that
β¦ LIBER β¦
On the rms intensity fluctuation of solar granulation
β Scribed by J. P. Mehltretter
- Publisher
- Springer
- Year
- 1971
- Tongue
- English
- Weight
- 706 KB
- Volume
- 19
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
Structure of the solar granulation
β
Th. Roudier; R. Muller
π
Article
π
1986
π
Springer
π
English
β 804 KB
Morphological study of the solar granula
β
Nobuyuki Oda
π
Article
π
1984
π
Springer
π
English
β 946 KB
Influence of intensity fluctuation on ex
β
Jie Kang; Gerald T. Mangine; Nicholas A. Ratamess; Avery D. Faigenbaum; Jay R. H
π
Article
π
2007
π
Springer
π
English
β 352 KB
A morphological study of the solar granu
β
O. Namba; W. E. Diemel
π
Article
π
1969
π
Springer
π
English
β 514 KB
Comments on the low-wavenumber power of
β
Claude Aime; Julien Borgnino; FranΓ§ois Martin; Gilbert Ricort
π
Article
π
1977
π
Springer
π
English
β 310 KB
Brightness fluctuations of solar ultravi
β
Giannina Poletto
π
Article
π
1979
π
Springer
π
English
β 789 KB
A simplified method is developed to derive the modifications induced at successive times by the passage of a shock wave in a standard unperturbed transition region atmosphere. Time dependent 'shocked' models allow the evaluation of the effects of the vertically propagating shock wave upon the intens