Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...153...64s&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 153, no. 1, Dec. 1985, p. 64-70.
Astronomy and Astrophysics
Astrophysics
23
Mass Flow, Photosphere, Solar Activity, Brightness, Carbon, Filaments, Flow Velocity, H Alpha Line, Solar Magnetic Field
Scientific paper
An active region filament near the center of the solar disk was observed on September 29-30, 1980, with the Multichannel Subtractive Double Pass Spectrograph of the Meudon solar tower and the UV Spectrograph and Polarimeter aboard the SMM satellite. H-alpha and C IV measurements are presently used to study brightness and material velocity in the 10,000 and 100,000 K temperature ranges, and photospheric magnetograms are used to investigate the underlying magnetic field. Attention is given to the constraints imposed on possible filament structures by observations, as well as the expected MHD relationships.
Malherbe Jean-Marie
Poland Arthur I.
Schmieder Brigitte
Simon Gabor
No associations
LandOfFree
Dynamics of solar filaments. IV - Structure and mass flow of an active region filament does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Dynamics of solar filaments. IV - Structure and mass flow of an active region filament, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamics of solar filaments. IV - Structure and mass flow of an active region filament will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1159229