Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...119..197m&link_type=abstract
Astronomy and Astrophysics, vol. 119, no. 2, Mar. 1983, p. 197-206.
Astronomy and Astrophysics
Astrophysics
40
H Alpha Line, Plasma Dynamics, Radial Velocity, Solar Atmosphere, Solar Corona, Solar Limb, Solar Prominences, Chromosphere, Doppler Effect, Mass Flow, Radiant Flux Density, Spectroheliographs, Statistical Analysis, Stellar Models, Velocity Distribution
Scientific paper
The authors present the observations of a solar filament obtained at Meudon with the Hα spectroheliograph over a period of 10 d. They show a morphologically stable feature. The authors perform a statistical analysis of the radial velocity field. Assuming long-lived (several days) stationary motions, they compute a 3-dimensional velocity field from center to limb observations of the radial component of velocity in the stable feature. Different pictures of stationary material circulations are suggested and compared with theoretical models of filaments. On the contrary, in the case of short-lived (a few 10 min) flows of material, the authors interpret their data in terms of velocity loops in the magnetic structure supporting the filament, and they compare the results with the MHD model proposed by Ribes and Unno (1980). Possible improvements to this model are pointed out in the conclusion.
Malherbe Jean-Marie
Mein Pierre
Ribes Elizabeth
Schmieder Brigitte
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