Results 221 to 230 of about 498 (257)
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Condensation of solar prominences
Vistas in Astronomy, 1965Abstract Many solar prominences are formed by condensation of coronal gases. Recent progress in our knowledge of the condensation process is surveyed. Some open problems are discussed in the concluding section.
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Kinematics of solar prominences
Solar Physics, 1983Using a 16-mm film recorded by R. B. Dunn at Sacramento Peak Observatory with a 15-inch coronagraph, we have studied motions of three solar prominences from the kinematic point of view. We applied three methods proposed earlier (Billings and Pecker, 1954; Palus, 1972; Makhmudov et al., 1980) to three prominences of the film.
J.L. Ballester, J. Kleczek
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Prominences and Solar Activity
International Astronomical Union Colloquium, 1979The following subjects were discussed:(1)Filament activation(2)Post-flare loops.(3)Surges and sprays.(4)Coronal transients.(5)Disk vs. limb observations.(6)Solar cycle variations of prominence occurrence.(7)Active prominences patrol service.Of all these items, (1) and (2) were discussed in most detail and we also pay most attention to them in this ...
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The Formation of Solar Prominences
1988Recent progress in the understanding of the formation of quiescent solar prominences is summarized in this chapter, from both an observational and theoretical point of view. It is now well known that the mass of a quiescent prominence (seen in emission at the solar limb) or a filament (generally seen in absorption above the disk) is an appreciable part
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The Formation of Solar Prominences
1982The formation of solar prominences is an interesting example of development of cool condensations that are not due to gravitational forces. It is widely believed that the physical processes operating in this case may also be relevant in different astrophysical systems, like the supernova remnants or the nuclei of active galaxies.
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Photography of the solar prominences
1890Thesis (B.S.)--Massachusetts Institute of Technology, Dept. of Physics, 1890. ; by George E. Hale. ; B.S.
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Large-amplitude longitudinal oscillations in solar prominences simulated with different resolutions
Astronomy and Astrophysics, 2021Manuel Luna, Elena Khomenko
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Physics of Solar Prominences: II—Magnetic Structure and Dynamics
Space Science Reviews, 2010Duncan Mackay +2 more
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On the formation of Mg ii h and k lines in solar prominences
Astronomy and Astrophysics, 2014Jean-Claude Vial, U Anzer
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