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1. The high energy solar corona
: waves, eruptions, particles
by Klein, L and MacKinnon, A. L
2007, Lecture notes in physics, ISBN 9783540715696, Volume 725., x, 284
Solar energetic particles | Sun | Corona | Atoms and Molecules in Strong Fields, Plasma Physics | Geophysics/Geodesy | Physics | Astronomy, Astrophysics and Cosmology
Book
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2. Full Text Plasma astrophysics
: kinetic processes in solar and stellar coronae
by Benz, A. O and SpringerLink (Online service)
2002, 2nd ed., Astrophysics and space science library, ISBN 1402006950, Volume 279, 328
This textbook is intended as an introduction to the physics of solar and stellar coronae, emphasizing kinetic plasma processes. It is addressed to... 
Particle beams | Plasma astrophysics | Corona | Sun Corona | Stars | Plasma dynamics | Sun | Astrophysics and Astroparticles | Nuclear Physics, Heavy Ions, Hadrons | Planetology | Plasma Physics | Nuclear physics
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3. The solar corona
by Golub, L. (Leon) and Pasachoff, Jay M
1997, ISBN 0521485355, xiv, 374
Sun Corona | Astrophysics
Book
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4. The solar corona
: proceedings. Edited by John W. Evans
by Evans, John Wainwright, 1909 and Air Force Cambridge Research Laboratories (U.S.) and International Astronomical Union. Symposium.16th, Cloudcroft, N.M., 1961
1963, 344
Sun CoronaCongresses
Book
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5. The solar chromosphere and corona
: quiet sun
by Athay, R. Grant
1976, Astrophysics and space science library, ISBN 9027702454, Volume 53, ix, 504
Sun Corona | Solar chromosphere
Book
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6. Physics of the solar corona
: an introduction
by Aschwanden, Markus J
2004, Springer-Praxis books in geophysical sciences, ISBN 3540223215, xxi, 842
Sun Corona
Book
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7. Full Text Alfvén Waves in the Solar Corona
by S. Tomczyk and S. W. McIntosh and S. L. Keil and P. G. Judge and T. Schad and D. H. Seeley and J. Edmondson
Science, ISSN 0036-8075, 8/2007, Volume 317, Issue 5842, pp. 1192 - 1196
Alfvén waves, transverse incompressible magnetic oscillations, have been proposed as a possible mechanism to heat the Sun's corona to millions of degrees by... 
Speed | Solar corona | Wave propagation | Wavelengths | Emission spectra | Linear polarization | Reports | Wave velocity | Magnetic fields | Waves | Pixels | MAGNETOHYDRODYNAMIC WAVES | CHROMOSPHERE | MULTIDISCIPLINARY SCIENCES | TRANSITION-REGION | FREQUENCY | SUN | DYNAMIC FIBRILS | LINES | LOOP OSCILLATIONS | Polarization | Corona | Research | Magnetohydrodynamic waves | Sun | Electromagnetic waves | Astrophysics | Estimates
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8. Physics of the solar corona
: proceedings. Held at Cavouri-Vouliagmeni, Athens, Greece, 6-17 Sept. 1970
by Macris, Constantin J and North Atlantic Treaty Organization. Science Committee and NATO Advanced Study Institute on Physics of the Solar Corona, Athens, 1970 and Athens. Ethnikon Asteroskopeion.Astronomikon Institouton
1971, Astrophysics and space science library, Volume 27, 345
Sun CoronaCongresses
Book
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9. Full Text The Width Distribution of Loops and Strands in the Solar Corona - Are We Hitting Rock Bottom?
by Aschwanden, Markus J and Peter, Hardi
Astrophysical Journal, ISSN 0004-637X, 05/2017, Volume 840, Issue 1, p. 4
In this study, we analyze Atmospheric Imaging Assembly (AIA) and Hi-C. images in order to investigate absolute limits for the finest loop strands. We develop a... 
Sun: corona | Sun: UV emission | ACTIVE-REGION LOOPS | PRINCIPAL COMPONENT ANALYSIS | 3-DIMENSIONAL STEREOSCOPIC ANALYSIS | HIGH-RESOLUTION PHOTOGRAPHY | CROSS-SECTION | SELF-ORGANIZED CRITICALITY | QUIET-SUN | MAGNETOHYDRODYNAMIC WAVES | HI-C | ASTRONOMY & ASTROPHYSICS | MAGNETIC-FIELD | Physics - Solar and Stellar Astrophysics
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10. Full Text High-precision density measurements in the solar corona: I. analysis methods and results for Fe XII and Fe XIII
by Young, P.R and Watanabe, T and Hara, H and Mariska, J.T
Astronomy and Astrophysics, ISSN 0004-6361, 02/2009, Volume 495, Issue 2, pp. 587 - 606
Aims. The EUV Imaging Spectrometer (EIS) instrument on board the Hinode satellite has access to some of the best coronal density diagnostics, and the high... 
Sun: UV radiation | Sun: corona | HINODE | ULTRAVIOLET IMAGING SPECTROMETER | EMISSION-LINES | ELECTRON-IMPACT EXCITATION | PROTON COLLISIONAL EXCITATION | TEMPERATURE | ATOMIC DATABASE | QUIET-SUN | ASTRONOMY & ASTROPHYSICS | EXTREME-ULTRAVIOLET | ACTIVE-REGION | Physics - Cosmology and Nongalactic Astrophysics | Physics - Earth and Planetary Astrophysics | Physics - Instrumentation and Methods for Astrophysics | Physics - High Energy Astrophysical Phenomena | Physics - Solar and Stellar Astrophysics | Physics - Astrophysics of Galaxies
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11. Physics of the solar corona
by Shklovskiĭ, I. S
1965, 2nd ed., Volume 6., x, 475
Corona
Book
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12. Full Text Heating of the Solar Chromosphere and Corona by Alfvén Wave Turbulence
by van Ballegooijen, A. A and Asgari-Targhi, M and Cranmer, S. R and DeLuca, E. E
The Astrophysical Journal, ISSN 0004-637X, 07/2011, Volume 736, Issue 1, p. 3
A three-dimensional magnetohydrodynamic (MHD) model for the propagation and dissipation of Alfven waves in a coronal loop is developed. The model includes the... 
Sun: granulation | turbulence | Sun: corona | magnetohydrodynamics (MHD) | Sun: chromosphere | Sun: surface magnetism | RAY TELESCOPE XRT | RESONANT ABSORPTION | MAGNETIC-FLUX TUBES | LOW-FREQUENCY WAVES | TRANSITION REGION | MAGNETOHYDRODYNAMIC TURBULENCE | REDUCED MAGNETOHYDRODYNAMICS | MHD TURBULENCE | QUIET-SUN | ASTRONOMY & ASTROPHYSICS | ACTIVE-REGION | Physics - Solar and Stellar Astrophysics | SOLAR ATMOSPHERE | HEATING | HYDRODYNAMICS | STELLAR ATMOSPHERES | MAGNETOHYDRODYNAMICS | SIMULATION | THREE-DIMENSIONAL CALCULATIONS | ATMOSPHERES | SOLAR CORONA | MAGNETISM | FLUID MECHANICS | MECHANICS | STELLAR CORONAE | ALFVEN WAVES | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | CHROMOSPHERE | HYDROMAGNETIC WAVES | TURBULENCE
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13. Full Text Alfvénic waves with sufficient energy to power the quiet solar corona and fast solar wind
by McIntosh, Scott W and De Pontieu, Bart and Carlsson, Mats and Hansteen, Viggo and Boerner, Paul and Goossens, Marcel
Nature, ISSN 0028-0836, 07/2011, Volume 475, Issue 7357, pp. 477 - 480
Energy is required to heat the outer solar atmosphere to millions of degrees (refs 1, 2) and to accelerate the solar wind to hundreds of kilometres per second... 
MAGNETOHYDRODYNAMIC TURBULENCE | ACCELERATION | TEMPERATURES | CHROMOSPHERE | MULTIDISCIPLINARY SCIENCES | HOLES | DRIVEN | MODEL | Measurement | Corona | Properties | Observations | Magnetohydrodynamic waves | Sun | Plasma | Solar physics | Coronas | Solar corona | Chromosphere | Amplitudes | Oscillations | Solar atmosphere | Magnetic fields | Solar wind
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14. Full Text Magnetic tornadoes as energy channels into the solar corona
by Wedemeyer-Böhm, Sven and Scullion, Eamon and Steiner, Oskar and Van Der Voort, Luc Rouppe and De La Cruz Rodriguez, Jaime and Fedun, Viktor and Erdélyi, Robert and Institutionen för fysik och astronomi and Teknisk-naturvetenskapliga vetenskapsområdet and Teoretisk astrofysik and Uppsala universitet and Fysiska sektionen
Nature, ISSN 0028-0836, 06/2012, Volume 486, Issue 7404, pp. 505 - 508
Heating the outer layers of the magnetically quiet solar atmosphere to more than one million kelvin and accelerating the solar wind requires an energy flux of... 
DRIVEN VORTEX FLOWS | WIND | ALFVENIC WAVES | CONVECTION | MULTIDISCIPLINARY SCIENCES | PHOTOSPHERE | POWER | GRANULATION | TURBULENCE | SIMULATIONS | QUIET SUN | Thermal properties | Energy transformation | Environmental aspects | Convection (Meteorology) | Corona | Research | Magnetic fields | Solar chromosphere | Sun | Magnetic properties | Studies | Plasma | Photosphere | Coronas | Alternative energy sources | Solar atmosphere | Tornadoes | Atmospherics | Channels | Fysik | Physical Sciences | Naturvetenskap | Natural Sciences
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15. Full Text NASA aims for Sun's corona
by Witze, A
NATURE, ISSN 0028-0836, 07/2018, Volume 559, Issue 7715, pp. 452 - 453
The spacecraft will also visit the birthplace of the solar wind, a flood of energetic particles that streams out into the Solar System at speeds of up to 800... 
MULTIDISCIPLINARY SCIENCES | Physicists | Corona | Emergency preparedness | Solar systems | Sun | Satellite communications
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16. Full Text The Highly Structured Outer Solar Corona
by Deforest, C.E and Howard, R.A and Velli, M and Viall, N and Vourlidas, A
Astrophysical Journal, ISSN 0004-637X, 07/2018, Volume 862, Issue 1, p. 18
We report on the observation of fine-scale structure in the outer corona at solar maximum, using deep-exposure campaign data from the Solar Terrestrial... 
Sun: heliosphere | Sun: corona | techniques: image processing | solar wind | WIND | EARTH | MASS EJECTIONS | MISSION | INTERPLANETARY MAGNETIC-FIELD | IMAGES | ASTRONOMY & ASTROPHYSICS | 30 R | TURBULENCE | HELIOSPHERE | CYCLE
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17. Full Text The Origins of Hot Plasma in the Solar Corona
by B. De Pontieu and S. W. McIntosh and M. Carlsson and V. H. Hansteen and T. D. Tarbell and P. Boerner and J. Martinez-Sykora and C. J. Schrijver and A. M. Title
Science, ISSN 0036-8075, 1/2011, Volume 331, Issue 6013, pp. 55 - 58
The Sun's outer atmosphere, or corona, is heated to millions of degrees, considerably hotter than its surface or photosphere. Explanations for this enigma... 
High temperature plasmas | Solar corona | Chromosphere | Plasma jets | Temperature | Solar temperature | Astrophysics | REPORTS | Coronal holes | Plasma temperature | Solar observatories | SPICULES | MODEL | TRANSITION REGION | MISSION | MULTIDISCIPLINARY SCIENCES | Thermal properties | Composition | Corona | Sun | Natural history | Plasma | Solar physics
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18. Full Text Detection of Waves in the Solar Corona: Kink or Alfvén?
by Van Doorsselaere, T and Nakariakov, V. M and Verwichte, E
The Astrophysical Journal Letters, ISSN 1538-4357, 03/2008, Volume 676, Issue 1, pp. L73 - L75
Recently, the omnipresence of waves has been discovered in the corona using the CoMP instrument. We demonstrate that the observational findings can be... 
Sun: oscillations | MHD | Sun: corona
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19. 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
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