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Dynamics and Fine Structures in Quiescent Prominences (MSDP/Pic du Midi, SOHO/SUMER and CDS)

Published online by Cambridge University Press:  12 April 2016

Kejun Li ,
J.-M. Malherbe ,
J.E. Wiik ,
B. Schmieder ,
Th. Roudier ,
T. Kucera  and
A. Poland
Kejun Li
Affiliation:
Yunnan Observatory, Kunming, China
J.-M. Malherbe
Affiliation:
Observatoire de Paris, DASOP, 92195 Meudon, France
J.E. Wiik
Affiliation:
University of Oslo, PO Box 1029, Blindern, 0315 Oslo, Norway Observatoire de Nice, BP 229, 06304 Nice Cedex 4, France
B. Schmieder
Affiliation:
Observatoire de Paris, DASOP, 92195 Meudon, France University of Oslo, PO Box 1029, Blindern, 0315 Oslo, Norway
Th. Roudier
Affiliation:
Observatoire Midi Pyrénées, 65200 Bagnères de Bigorre, France
T. Kucera
Affiliation:
NASA, GSFC, MD 20771, USA
A. Poland
Affiliation:
NASA, GSFC, MD 20771, USA

Abstract

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During the June 1996 campaign using the MSDP spectrograph at Pic du Midi and SUMER/CDS (JOP 12) on board SOHO, quiescent prominences were observed. We present observations and physical quantities of the June 5 prominence. Doppler shifts, temperatures and electron densities of fine structures were deduced from Hα data.

Type
Filaments and Their Environment
Information
International Astronomical Union Colloquium , Volume 167: New Perspectives on Solar Prominences , 1998 , pp. 32 - 35
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

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Li, K. et al. 1994 Solar Phys., 150, 87 CrossRefGoogle Scholar
Wiik, J.E. et al. 1997, JOSO Annual Report, 93 Google Scholar