Solar Prominences – An Intriguing Phenomenon
暂无分享,去创建一个
[1] J. Chae. DYNAMICS OF VERTICAL THREADS AND DESCENDING KNOTS IN A HEDGEROW PROMINENCE , 2010 .
[2] Astronomy,et al. Physics of Solar Prominences: I—Spectral Diagnostics and Non-LTE Modelling , 2010, 1001.1620.
[3] B. Schmieder,et al. Physics of Solar Prominences: II—Magnetic Structure and Dynamics , 2010, 1001.1635.
[4] P. Mein,et al. Velocity vectors of a quiescent prominence observed by Hinode/SOT and the MSDP (Meudon) , 2009, 0911.5091.
[5] P. Démoulin,et al. FORMATION OF TORUS-UNSTABLE FLUX ROPES AND ELECTRIC CURRENTS IN ERUPTING SIGMOIDS , 2009 .
[6] T. Kosugi,et al. The Hinode (Solar-B) Mission: An Overview , 2007 .
[7] T. Forbes,et al. CME Theory and Models , 2006 .
[8] India.,et al. Source Regions of Coronal Mass Ejections , 2001, astro-ph/0107138.
[9] E. Tandberg-Hanssen. The History of Solar Prominence Research: Historical Introduction to IAU Colloquium No. 167 “New Perspectives on Solar Prominences” , 1998 .
[10] E. Tandberg-Hanssen,et al. The Nature of Solar Prominences , 1995 .
[11] B. Low. Magnetohydrodynamic processes in the solar corona: Flares, coronal mass ejections, and magnetic helicity* , 1994 .
[12] B. Low,et al. The free energies of partially open coronal magnetic fields , 1993 .
[13] G. Sloan,et al. Spatially Resolved Spectra of the Unidentified Infrared Features around HD 44179 (The Red Rectangle) , 1993 .
[14] E. Tandberg-Hanssen,et al. Dynamics of Quiescent Prominences: IAU Coll.117, 1990 , 1990 .
[15] F. Drago. Radio observations of prominences , 1990 .
[16] J. Zirker,et al. Estimation of the line of sight amplitude of the magnetic field on threads of an active region prominence , 1990 .
[17] E. Priest. Dynamics and Structure of Quiescent Solar Prominences , 1988 .
[18] S. Wu,et al. Application of similitude principle to the numerical simulation of solar atmospheric dynamics , 1988 .
[19] Ronald L. Moore,et al. Evidence that magnetic energy shedding in solar filament eruptions is the drive in accompanying flares and coronal mass ejections , 1988 .
[20] B. Schmieder,et al. Material ejecta in a disturbed solar filament , 1987 .
[21] A. Poland. Coronal and Prominence Plasmas , 1986 .
[22] Z. Svestka,et al. 21 May 1980 flare review , 1985 .
[23] M. Hagyard. Measurements of Solar Vector Magnetic Fields , 1985 .
[24] E. Reichmann,et al. Evidence for systematic flows in the transition region around prominences , 1985 .
[25] C. Fang,et al. Simultaneous monochromatic and spectral observations of two large loop prominence groups , 1985 .
[26] H. Zirin,et al. Magnetic shear. I - Hale region 16918 , 1985 .
[27] A. Hundhausen,et al. Coronal mass ejections observed during the Solar Maximum Mission: Latitude distribution and rate of occurrence , 1984 .
[28] S. Sahal-Bréchot,et al. The magnetic field in the prominences of the polar crown , 1983 .
[29] J. Vial,et al. Preflare heating of filaments , 1982 .
[30] S. Martin. Preflare conditions, changes and events , 1980 .
[31] R. MacQueen,et al. The association of coronal mass ejection transients with other forms of solar activity , 1979 .
[32] J. Vial,et al. Profiles of Hi (La), Mgii (h and k), Caii (H and K) Lines of an active filament at the limb, with the LPSP instrument aboard the OSO-8 Satellite , 1979 .
[33] E. C. Bruner,et al. Preliminary results from the Orbiting Solar Observatory 8 - Persistent velocity fields in the chromosphere and transition region , 1976 .
[34] O. Engvold. The fine structure of prominences , 1976 .
[35] G. Ratier. A polarimeter for monochromatic studies of solar prominences , 1975 .
[36] A. Emslie,et al. The Physics of Solar Flares , 2009 .
[37] S. Martin. The evolution of prominences and their relationship to active centers , 1973 .
[38] A. Bruzek,et al. Physics of solar prominences , 1972 .
[39] U. Anzer,et al. A model for quiescent prominences with helical structure , 1970 .
[40] U. Anzer,et al. The orientation of magnetic fields in quiescent prominences , 1970 .
[41] P. Sweet. Mass Motions in Solar Flares and Related Phenomena , 1969 .
[42] K. O. Kiepenheuer,et al. Structure and Development of Solar Active Regions , 1968 .
[43] J. Harvey,et al. The magnetic field in some prominences measured with the He I, 5876 Å line , 1968 .
[44] J. Malville. Magnetic fields in two active prominences , 1968 .
[45] B. Ioshpa. On the Magnetic-Field Structure Around Filaments , 1968 .
[46] Y. Ohman. Mass Motions in Solar Flares and Related Phenomena , 1968 .
[47] E. Tandberg-Hanssen,et al. The nature of quiescent solar prominences , 1967 .
[48] C. Hyder. Magnetic Fields in the Loop Prominence of March 16, 1964. , 1964 .
[49] E. Tandberg-Hanssen. Physical Conditions in Limb Flares and Active Prominences.VI. Selective Excitation Conditions. , 1963 .
[50] H. Zirin,et al. Measurement of magnetic fields in solar prominences , 1961 .
[51] H. Zirin,et al. Physical Conditions in Limb Flares and Active Prominences.IV. Compersion of Active and Quiescent Prominences. , 1960 .
[52] H. Babcock,et al. The Sun's Magnetic Field, 1952-1954. , 1955 .
[53] J. Greenstein,et al. The Abundance of Beryllium in the Sun. , 1954 .
[54] E. Pettit. Characteristic Features of Solar Prominences , 1932 .