Physical properties of the quiescent prominence of 5 June 1996, from H alpha observations

Citation
L. Kejun et al., Physical properties of the quiescent prominence of 5 June 1996, from H alpha observations, SOLAR PHYS, 183(2), 1998, pp. 323-338
Citations number
29
Categorie Soggetti
Space Sciences
Journal title
SOLAR PHYSICS
ISSN journal
00380938 → ACNP
Volume
183
Issue
2
Year of publication
1998
Pages
323 - 338
Database
ISI
SICI code
0038-0938(199812)183:2<323:PPOTQP>2.0.ZU;2-Y
Abstract
The Multichannel Subtractive Double Pass spectrograph (MSDP) is designed to observe line profiles in a 2D field of view with a good spatial and tempor al resolution. In order to deal with this unique opportunity, we introduce a new method for fitting the hydrogen H alpha line formed in prominences an d deriving various plasma parameters from line profile observations. A quie scent prominence was observed on 5 June 1996, at the Pic du Midi during an international campaign between 09:30 UT and 11.00 UT with the MSDP spectrog raph operating in H alpha at the Turret Dome. Using the new fitting method, we show that the temperature, column density of hydrogen atoms and microtu rbulent velocity of the prominence are respectively about 8500K, 1.4 x 10(1 2) cm(-2), and 10 to 20 km s(-1). The electron density of the prominence is about 1.8 x 10(10) cm(-3).