Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-12-01T10:58:22.987Z Has data issue: false hasContentIssue false
  • English
  • Français

Velocity Fields in the Filament Regions: Structure and Evolution

Published online by Cambridge University Press:  12 April 2016

B. Ioshpa  and
E. Kulikova
B. Ioshpa
Affiliation:
Izmiran, 142092, Troitsk, Moscow region, Russia
E. Kulikova
Affiliation:
Radiophysical Institute, Nignij Novgorod, Russia

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The velocity structure in the photosphere under the Hα-filaments is analyzed. The results bring to suggestion that the velocity structure are connected with the stability and the type of the filament.

Type
Session 1. Structure of Active Regions
Information
International Astronomical Union Colloquium , Volume 141: The Magnetic and Velocity Fields of Solar Active Regions , 1993 , pp. 56 - 59
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Ioshpa, B., Kogevatov, I., Kulikova, E., and Mogilevski, E. 1986, Soln. Dannye, 5, 68.Google Scholar
Ioshpa, B., and Kulikuva, E. 1988, in Phizika Solnechnoj Activnosti, Moscow, ed. Nauka p. 168.Google Scholar
Ioshpa, B., and Kulikova, E. 1989, in Trudi 3 Consultativnogo Soveshanija, Novosibirsk, ed. Nauka, p. 167.Google Scholar
Ioshpa, B., Kogevatov, I., and Kulikova, E. 1991, in Proceedings of the Eleventh NSO/ Sac. Peak Workshop on Solar Polarimetry, ed. November, L. J., p. 80.Google Scholar
Martres, M.J., Mein, P., Schmieder, B., Soru-Escaut, I. 1981, Sol. Phys., 69, 301.Google Scholar
Schmieder, B. 1988, in Dynamics and Structure of Quiescent Prominences, ed. Priest, p. 15.Google Scholar
Schmieder, B., Raadu, M.A., Demuulin, P., and Dere, K.P. 1989, A&A, 213, 402.Google Scholar