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Velocity Fields of a Filament Region Observed with Ground-Based Telescopes and from SOHO

Published online by Cambridge University Press:  12 April 2016

P. Mein
Affiliation:
Observatoire de Paris, Section de Meudon, 5 Place Janssen, F-92195 Meudon, France
B. Schmieder
Affiliation:
Observatoire de Paris, Section de Meudon, 5 Place Janssen, F-92195 Meudon, France
J.-M. Malherbe
Affiliation:
Observatoire de Paris, Section de Meudon, 5 Place Janssen, F-92195 Meudon, France
J.E. Wiik
Affiliation:
Inst. Theoret. Astrophys., University of Oslo, P.O. Box 1029, Blindern, N-0315 Oslo, Norway
O. Engvold
Affiliation:
Inst. Theoret. Astrophys., University of Oslo, P.O. Box 1029, Blindern, N-0315 Oslo, Norway
P. Brekke
Affiliation:
Inst. Theoret. Astrophys., University of Oslo, P.O. Box 1029, Blindern, N-0315 Oslo, Norway
J.B. Zirker
Affiliation:
NSO, NOAO, Sunspot, New Mexico 88349, USA
A.I. Poland
Affiliation:
NASA/Goddard Space Flight Center, Greenbelt, Maryland, USA
J.-P. Delaboudinière
Affiliation:
Inst. d’Astrophysique Spatiale, Université Paris XI, F-91405 Orsay Cedex, France
J. Staiger
Affiliation:
K.I.S., Schöneckstrasse 6, D-79104 Freiburg, Germany

Abstract

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We present preliminary results on solar filaments observed from the ground and from SOHO in September 1996. Motions in the network and close to the filament “barbs” are shown at different levels of the chromosphere and the transition region.

Type
Filaments and Their Environment
Copyright
Copyright © Astronomical Society of the Pacific 1998