Segmentation Of Photospheric And Chromospheric Solar Features
β Scribed by F. Berrilli; D. Del Moro; A. Florio; L. Santillo
- Publisher
- Springer
- Year
- 2005
- Tongue
- English
- Weight
- 883 KB
- Volume
- 228
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
Abslract. We have conlpiled the resuhs of our long-term studies of the local magnetic lield and ils activily development, derived from investigating stlnspo[ group evolulion, photoelectrically measured Iongiludinal magnetic and velocity fields, and measurements o[ stmspot proper motions. We estimate
Frazier (1972) has criticized the conclusions of Zirin (1971Zirin ( , 1972)), Veeder and Zirin (1970), and those of Foukal (1971a, b, c) on the relation between He structure and magnetic fields. We wish to reply to these criticisms. Some of the points Frazier mentions refer to statements made by
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