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Dynamical Fine Structure of Filaments and Prominences

Published online by Cambridge University Press:  12 April 2016

N. Mein ,
P. Mein  and
J.E. Wiik
N. Mein
Affiliation:
Observatoire de Paris, Section de Meudon, F92195Meudon Cedex
P. Mein
Affiliation:
Observatoire de Paris, Section de Meudon, F92195Meudon Cedex
J.E. Wiik
Affiliation:
Observatoire de Paris, Section de Meudon, F92195Meudon Cedex

Extract

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We observed a quiescent prominence on the east limb of the Sun, on June 7, 1988 (Mein P. et al 1990) and a quiescent filament (N 5, W 5) on June 17, 1986 (Schmieder et al 1991). These two observations are made with the Multichannel Subtractive Double Pass spectrograph of the turret dome refractor of the Pic du Midi Observatory, providing simultaneous 2D pictures in 9 channels for Hα.

Type
Session 6. Flares and Transients
Information
International Astronomical Union Colloquium , Volume 141: The Magnetic and Velocity Fields of Solar Active Regions , 1993 , pp. 391 - 393
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Mein, P., Mein, N., 1990, Sol. Phys. 136, 317. Google Scholar
Schinieder, B., Raadu, M. A., Wiik, J.E. 1991, Astron. Astrophys. 252, 353.Google Scholar