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1. The forms and motions of the solar prominences
by Pettit, Edison
1925, 205-240 p. plates.
Book
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2. Protuberanzen, beobachtet im Jahre 1887 am Haynald-Observatorium
by Fényi, Julius, 1845
1892, Publicationen des Haynald-Observatoriums, Volume 6. Heft, 1892, 78 p., [7] leaves of plates (some folded)
Sun | Sun Prominences
Book
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3. Solar prominences
by Vial, Jean Claude and Engvold, Oddbjorn
2015, Astrophysics and Space Science Library, ISBN 9783319104164, Volume 415
Solar activity | Sun Prominences
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4. Full Text Non-LTE modelling of prominence fine structures using hydrogen Lyman-line profiles
by Schwartz, P and Gunár, S and Curdt, W
Astronomy and Astrophysics, ISSN 0004-6361, 05/2015, Volume 577, p. A92
Aims. We perform a detailed statistical analysis of the spectral Lyman-line observations of the quiescent prominence observed on May 18, 2005. Methods. We used... 
Sun: filaments prominences | Radiative transfer | Methods: statistical | Line: profiles | SUMER | QUIESCENT PROMINENCES | THREADS | radiative transfer | ENERGY-BALANCE | SOHO/SUMER | methods: statistical | Sun: filaments, prominences | line: profiles | ASTRONOMY & ASTROPHYSICS | DYNAMICS | 2-DIMENSIONAL RADIATIVE-TRANSFER | MAGNETIC-FIELD | SOLAR PROMINENCES | SPECTRUM | Fine structure | Lyman spectra | Statistical analysis | Spectra | Two dimensional | Prominences | Line of sight | Astronomy
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5. Protuberanzen Beobachtet in den Jahren 1891, 1892
by Fényi, Julius, 1845
1911, Publicationen des Haynald-Observatoriums, Volume Heft 10, 144 p., [9] folded leaves of plates
Sun | Sun Prominences
Book
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6. Protuberanzen Beobachtet in den Jahren 1888, 1889, 1890 am Haynald-Observatorium
by Fényi, Julius, 1845 and Haynald-Observatorium
1902, Publicationen des Haynald-Observatoriums, Volume Heft 8, 132 p, [10] leaves of plates
Sun | Sun Prominences
Book
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7. Plasma loops in the solar corona
by Bray, R. J
1991, Cambridge astrophysics series, ISBN 0521351073, Volume 18, xx111, 498
This book presents the first comprehensive account of the properties of plasma loops, the fundamental structural elements of the solar corona. Plasma loops... 
Sun Corona | Sun Loop prominences
Book
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8. Full Text FORMATION and PLASMA CIRCULATION of SOLAR PROMINENCES
by Xia, C and Keppens, R
Astrophysical Journal, ISSN 0004-637X, 05/2016, Volume 823, Issue 1, pp. 22 - 22
Solar prominences are long-lived cool and dense plasma curtains in the hot and rarefied outer solar atmosphere or corona. The physical mechanism responsible... 
Sun: filaments, prominences Supporting material: animations | Sun: corona | magnetohydrodynamics (MHD) | CORONAL CAVITY | RAYLEIGH-TAYLOR INSTABILITY | DIPS | SUPPORT | Sun: filaments, prominences | ASTRONOMY & ASTROPHYSICS | DYNAMICS | CONDENSATION | MAGNETIC-FIELD | QUIESCENT PROMINENCE | NUMERICAL SIMULATIONS | MORPHOLOGY | Coronas | Chromosphere | Dynamics | Formations | Solar prominences | Evaporation | Prominences | Circulation | Physics - Solar and Stellar Astrophysics | MAGNETIC FIELDS | MAGNETIC FLUX | PLASMA | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | STAR EVOLUTION | CHROMOSPHERE | MASS | MAGNETOHYDRODYNAMICS | SOLAR PROMINENCES | SOLAR CORONA | COMPUTERIZED SIMULATION
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9. Full Text Properties of the prominence magnetic field and plasma distributions as obtained from 3D whole-prominence fine structure modeling
by Gunár, S and Mackay, D.H
Astronomy and Astrophysics, ISSN 0004-6361, 08/2016, Volume 592, p. A60
Aims. We analyze distributions of the magnetic field strength and prominence plasma (temperature, pressure, plasma beta, and mass) using the 3D... 
Plasmas | Sun: filaments, prominences | Sun: magnetic fields | Methods: numerical | QUIESCENT PROMINENCES | plasmas | THREADS | methods: numerical | RADIATIVE-TRANSFER | EVOLUTION | ASTRONOMY & ASTROPHYSICS | MASS | EQUILIBRIUM | 2-DIMENSIONAL MODELS | SOLAR PROMINENCES | DIAGNOSTICS | LYMAN-LINE-PROFILES | Fine structure | Photosphere | Mathematical models | Magnetic fields | Three dimensional models | Prominences | Strength | Dipping
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10. Full Text Importance of the Hα Visibility and Projection Effects for the Interpretation of Prominence Fine-structure Observations
by Gunár, Stanislav and Dudík, Jaroslav and Aulanier, Guillaume and Schmieder, Brigitte and Heinzel, Petr
Astrophysical Journal, ISSN 0004-637X, 11/2018, Volume 867, Issue 2, p. 115
We construct a new 3D Whole-prominence Fine-structure (WPFS) model based on a prominence magnetic field configuration designed to qualitatively approximate the... 
Sun: filaments, prominences | methods: numerical | magnetic fields | QUIESCENT PROMINENCES | CONFIGURATIONS SUPPORTING PROMINENCES | VERTICAL THREADS | FILAMENT CHANNEL | RADIATIVE-TRANSFER | LATERAL FEET | PERIODIC MOTION | ASTRONOMY & ASTROPHYSICS | MAGNETIC-FIELD | POLAR CROWN | SOLAR PROMINENCES
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11. Dynamics and structure of quiescent solar prominences
by Priest, E. R
1989, ISBN 902772833X, x, 217
Prominences | Congresses
Book
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12. Full Text Magnetic topology of bubbles in quiescent prominences
by Dudík, J and Aulanier, G and Schmieder, B and Zapiór, M and Heinzel, P
Astrophysical Journal, ISSN 0004-637X, 12/2012, Volume 761, Issue 1, pp. 9 - 13
We study a polar-crown prominence with a bubble and its plume observed in several coronal filters by the SDO/AIA and in Ha by the MSDP spectrograph in Bialkow... 
Sun: filaments prominences | Sun: magnetic topology | Sun: UV radiation | Sun: corona | Sun: surface magnetism | QUASI-SEPARATRIX LAYERS | TWISTED FLUX ROPE | FINE-STRUCTURE | CONFIGURATIONS SUPPORTING PROMINENCES | FILAMENT CHANNEL | Sun: filaments, prominences | LATERAL FEET | ASTRONOMY & ASTROPHYSICS | SOLAR-CYCLE 23 | H-ALPHA | ACTIVE-REGION | EUV FILAMENT | Coronas | Bubbles | Brightness | Topology | Separators | Prominences | Plumes | Dipping | MAGNETIC FIELDS | TOPOLOGY | ULTRAVIOLET RADIATION | MAGNETIC RECONNECTION | SUN | SOLAR CORONA | MAGNETISM | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | ASTRONOMY | ASTROPHYSICS | SOLAR PROMINENCES | BRIGHTNESS | SURFACES
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13. Full Text SDO/AIA detection of solar prominence formation within a coronal cavity
by Berger, Thomas E and Liu, Wei and Low, B.C
Astrophysical Journal Letters, ISSN 2041-8205, 10/2012, Volume 758, Issue 2, pp. L37 - 7
We report the first analyses of SDO/AIA observations of the formation of a quiescent polar crown prominence in a coronal cavity. The He II 304 angstrom (log... 
only material: animations, color figures | Sun: chromosphere | Sun: filaments, prominences Online | Sun: coronal mass ejections (CMEs) | HINODE | MAGNETIC RECONNECTION | GROUND-BASED OBSERVATIONS | ERUPTIVE PROMINENCE | Sun: filaments, prominences | ASTRONOMY & ASTROPHYSICS | HYDROMAGNETIC INTERIOR | MASS EJECTION | DYNAMICS | CONDENSATION | QUIESCENT PROMINENCE | FLOWS | Coronas | Clouds | Holes | Formations | Solar prominences | Iron | Prominences | Channels | MAGNETIC FLUX | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | CAVITIES | COOLING | HOT PLASMA | CHROMOSPHERE | CONVECTION | SOLAR PROMINENCES | EMISSION | BRIGHTNESS | SOLAR CORONA
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14. Full Text Dissipative instabilities in a partially ionised prominence plasma slab
by Mather, JF and Ballai, I and Erdelyi, R
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 02/2018, Volume 610
This study deals with the dissipative instability that appears in a compressible partially ionised plasma slab embedded in a uniform magnetic field, modelling... 
Sun: oscillations | waves | QUIESCENT PROMINENCES | plasmas | MAGNETIC-FIELDS | Sun: corona | SURFACE-WAVES | FLUX TUBES | instabilities | NEGATIVE-ENERGY WAVES | Sun: filaments, prominences | STEADY FLOWS | MHD WAVES | ASTRONOMY & ASTROPHYSICS | H-ALPHA | SOLAR PROMINENCE | OSCILLATIONS | Viscosity | Plasma | Solar corona | Magnetohydrodynamics | Stability | Computational fluid dynamics | Fluid flow | Solar prominences | Waves | Equilibrium | Compressibility effects | Numerical analysis | Plasma slabs | Slow waves | Dissipation | Equilibrium flow | Evolution | Instability | Mathematical models | Corona | Magnetic fields | Prominences
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15. Full Text The magnetic field configuration of a solar prominence inferred from spectropolarimetric observations in the He i 10 830 Ã… triplet
by Orozco Suárez, D and Asensio Ramos, A and Trujillo Bueno, J
Astronomy and Astrophysics, ISSN 0004-6361, 2014, Volume 566, pp. A46 - np
Context. Determining the magnetic field vector In quiescent solar prominences Is possible by Interpreting Hanle Manie and Zeeman effects in spectral lines.... 
Sun: filaments, prominences | Sun: chromosphere | Field strength | Mathematical analysis | Chirality | Solar prominences | Vectors (mathematics) | Magnetic fields | Spatial resolution | Prominences
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16. Full Text Physics of solar prominences: II - Magnetic structure and dynamics
by Mackay, D.H and Karpen, J.T and Ballester, J.L and Schmieder, B and Aulanier, G
Space Science Reviews, ISSN 0038-6308, 04/2010, Volume 151, Issue 4, pp. 333 - 399
Observations and models of solar prominences are reviewed. We focus on non-eruptive prominences, and describe recent progress in four areas of prominence... 
Oscillations | Solar prominences | MHD waves | Solar magnetic fields | CORONAL MASS EJECTIONS | QUIESCENT PROMINENCES | CONFIGURATIONS SUPPORTING PROMINENCES | ACTIVE-REGION FILAMENTS | TWISTED FLUX-TUBE | FULL-STOKES SPECTROPOLARIMETRY | FAST MAGNETOHYDRODYNAMIC OSCILLATIONS | ASTRONOMY & ASTROPHYSICS | H-ALPHA | HYDROGEN LYMAN LINES | Plasma physics | Magnetic fields | Analysis | Electric generators | Astrophysics | Research | Sun | Astronomy | Physics - Solar and Stellar Astrophysics
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17. Full Text 3D Whole-prominence fine structure modeling
by Gunár, Stanislav and Mackay, Duncan H
Astrophysical Journal, ISSN 0004-637X, 04/2015, Volume 803, Issue 2, pp. 1 - 12
We present the first 3D whole-prominence fine structure model. The model combines a 3D magnetic field configuration of an entire prominence obtained from... 
Sun: filaments, prominences | Magnetic fields | Radiative transfer | MAGNETIC EQUILIBRIUM | FORCE-FREE | magnetic fields | CONFIGURATIONS SUPPORTING PROMINENCES | HINODE | radiative transfer | MULTILEVEL RADIATIVE-TRANSFER | FILAMENT CHANNEL | EVOLUTION | ASTRONOMY & ASTROPHYSICS | 2-DIMENSIONAL MODELS | SOLAR PROMINENCES | QUIESCENT PROMINENCE | Fine structure | Hydrostatics | Disks | Mathematical models | Three dimensional models | Prominences | Dipping | MAGNETIC FIELDS | RADIANT HEAT TRANSFER | FINE STRUCTURE | MAGNETIC FIELD CONFIGURATIONS | RESOLUTION | COMPARATIVE EVALUATIONS | SUN | COMPUTERIZED SIMULATION | LIMBS | FILAMENTS | PLASMA | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | IMAGES | EQUILIBRIUM
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18. Full Text Formation and evolution of a multi-threaded solar prominence
by Luna, M and Karpen, J.T and Devore, C.R
Astrophysical Journal, ISSN 0004-637X, 02/2012, Volume 746, Issue 1, pp. 30 - 12
We investigate the process of formation and subsequent evolution of prominence plasma in a filament channel and its overlying arcade. We construct a... 
Sun: filaments, prominences | Sun: magnetic topology | Sun: corona | QUIESCENT PROMINENCES | CORONAL LOOPS | MODEL | THERMAL NONEQUILIBRIUM | ALPHA FILTERGRAMS | ASTRONOMY & ASTROPHYSICS | prominences | FILAMENT | DYNAMICS | MAGNETIC-FIELD | ACTIVE-REGION | FLOWS | Sun: filaments | Filaments | Flux | Condensing | Tubes | Magnetic structure | Evolution | Prominences | Arcades | Channels | MAGNETIC FIELDS | PLASMA | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | CHROMOSPHERE | SOLAR SYSTEM EVOLUTION | MASS | ONE-DIMENSIONAL CALCULATIONS | SOLAR PROMINENCES | THREE-DIMENSIONAL CALCULATIONS | TIME DEPENDENCE | SUN
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19. Full Text Dissipative instability in partially ionised prominence plasmas
by Ballai, Istvan and Oliver, Ramon and Alexandrou, Marios
Astronomy and Astrophysics, ISSN 0004-6361, 05/2015, Volume 577, p. A82
Aims. We investigate the nature of dissipative instability at the boundary (seen here as tangential discontinuity) between the viscous corona and the partially... 
Instabilities | Sun: filaments prominences | Sun: magnetic fields | NEGATIVE-ENERGY | ANISOTROPIC VISCOSITY | COMPRESSIBLE PLASMAS | SOLAR ATMOSPHERE | THERMAL-CONDUCTIVITY | instabilities | ALFVEN WAVES | Sun: filaments, prominences | MAGNETOHYDRODYNAMIC WAVES | MHD WAVES | ASTRONOMY & ASTROPHYSICS | QUIESCENT PROMINENCE | OSCILLATIONS | Stability | Dissipation | Instability | Evolution | Solar prominences | Plasmas | Prominences | Plumes | Physics - Solar and Stellar Astrophysics
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