The Thermal Nonequilibrium of Prominences
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[1] The Dynamic Formation of Prominence Condensations , 1998, astro-ph/9808199.
[2] O. Engvold,et al. Counter-streaming gas flows in solar prominences as evidence for vertical magnetic fields , 1998, Nature.
[3] Sara F. Martin,et al. Conditions for the Formation and Maintenance of Filaments – (Invited Review) , 1998 .
[4] P. Brekke,et al. Time Variability of Active Region Loops Observed with the Coronal Diagnostic Spectrometer (Cds) on Soho , 1998 .
[5] Spiro K. Antiochos,et al. Prominence Formation by Localized Heating , 1998 .
[6] E. Tandberg-Hanssen,et al. The Nature of Solar Prominences , 1995 .
[7] S. Antiochos,et al. The magnetic field of solar prominences , 1994 .
[8] S. Antiochos,et al. A model for the formation of solar prominences , 1991 .
[9] D. Schnack,et al. Prominence formation in a coronal loop , 1990 .
[10] S. Antiochos,et al. Effect of coronal elemental abundances on the radiative loss function , 1989 .
[11] A. Poland,et al. A siphon mechanism for supplying prominence mass , 1986 .
[12] E. Priest,et al. Siphon flows in coronal loops: I. Adiabatic flow , 1980 .
[13] S. Antiochos. A model of active prominences , 1980 .
[14] E. Priest,et al. The structure of coronal arcades and the formation of solar prominences , 1979 .
[15] Spiro K. Antiochos,et al. Numerical modeling of quasi-static coronal loops. I - Uniform energy input , 1979 .
[16] P. Sturrock,et al. Evaporative cooling of flare plasma , 1978 .
[17] R. Rosner,et al. Dynamics of the quiescent solar corona , 1978 .
[18] O. Engvold,et al. On Pikel'ner's theory of prominences , 1977 .
[19] E. C. Bruner,et al. Preliminary results from the Orbiting Solar Observatory 8 - Persistent velocity fields in the chromosphere and transition region , 1976 .
[20] O. Engvold. The fine structure of prominences , 1976 .
[21] S. Pikel’ner. Origin of quiescent prominences , 1971 .