Results 221 to 230 of about 1,154 (251)

Condensation of solar prominences

Vistas in Astronomy, 1965
Abstract 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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Prominences and Solar Activity

International Astronomical Union Colloquium, 1979
The 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

1982
The 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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The Formation of Solar Prominences

1988
Recent 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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Spatial damping of MHD waves in solar prominences: Effect of background flow

Advances in Space Research, 2021
Ashish Mishra
exaly  

Large-amplitude longitudinal oscillations in solar prominences simulated with different resolutions

Astronomy and Astrophysics, 2021
M Luna, E Khomenko
exaly  

Time‐Latitude Distribution of Prominences for 10 Solar Cycles: A Study Using Kodaikanal, Meudon, and Kanzelhohe Data

Earth and Space Science, 2020
Subhamoy Chatterjee, Manjunath Hegde, Dipankar Banerjee   +2 more
exaly  

Solar prominences: theory and models

Living Reviews in Solar Physics, 2018
Sarah E Gibson, Gibson Sarah E
exaly  

Solar Prominences

1974
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Coronal Mass Ejections and Active Prominences Relationship During Solar Cycle 23

AIP Conference Proceedings, 2007
A Lara
exaly