The velocity of microturbulent motions in the solar photosphere at the level of formation of weak Fraunhofer lines (h-150 km) is found to be 0.1โข kms -~. The observations have been performed with the double-pass spectrometer in Kiev. Apart from thermal motions and damping effects we have taken into
โฆ LIBER โฆ
On determining the microturbulent velocities of solar prominences
โ Scribed by A. G. Nikoghossian; Z. Mouradian
- Publisher
- Springer
- Year
- 2010
- Tongue
- English
- Weight
- 174 KB
- Volume
- 53
- Category
- Article
- ISSN
- 0571-7256
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
On the microturbulence in the solar phot
โ
R. I. Kostik; T. V. Orlova
๐
Article
๐
1979
๐
Springer
๐
English
โ 175 KB
Statistical Investigations of the Solar
โ
M. S. Eigenson
๐
Article
๐
1930
๐
John Wiley and Sons
๐
English
โ 732 KB
The nature of quiescent solar prominence
โ
Max Kuperus; Einar Tandberg-Hanssen
๐
Article
๐
1967
๐
Springer
๐
English
โ 550 KB
Quiescent prominences occur as long-lasting cool sheets of matter in the surrounding hot corona at the base of coronal streamers. Seen on the disk they appear as dark filaments dividing regions of opposite magnetic polarity. In this paper a theoretical model is presented, which describes the genera
The study on fine structures in solar pr
โ
A. Adjabshirizadeh; H. Ebadi
๐
Article
๐
2005
๐
Elsevier Science
๐
English
โ 290 KB
The formation of solar quiescent promine
โ
E. Hildner
๐
Article
๐
1974
๐
Springer
๐
English
โ 760 KB
On the determination of the velocity of
โ
H. G. Bueren; M. Kuperus
๐
Article
๐
1970
๐
Springer
๐
English
โ 177 KB