Solar corona / by Evans, John Wainwright, 1909-

Physics of the solar corona / by Macris, Constantin J.

A guide to the solar corona by 209271 Billings, Donald E.

Energy Budget in the Solar Corona by Daniele Telloni, Marco Romoli, Marco Velli, Gary P. Zank, Laxman Adhikari, Lingling Zhao, Cooper Downs, Jasper S. Halekas, Jaye L. Verniero, Michael D. McManus, Chen Shi, Aleksandr Burtovoi, Roberto Susino, Daniele Spadaro, Alessandro Liberatore, Ester Antonucci, Yara De Leo, Lucia Abbo, Federica Frassati, Giovanna Jerse, Federico Landini, Gianalfredo Nicolini, Maurizio Pancrazzi, Giuliana Russano, Clementina Sasso, Vincenzo Andretta, Vania Da Deppo, Silvano Fineschi, Catia Grimani, Petr Heinzel, John D. Moses, Giampiero Naletto, Marco Stangalini, Luca Teriaca, Michela Uslenghi, Stuart D. Bale, Justin C. Kasper

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Current understanding of the heating of the solar corona by Jordan, C

Kinetic Physics of the Solar Corona and Solar Wind by Marsch Eckart

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Resolved magnetohydrodynamic wave lensing in the solar corona by Xinping Zhou, Yuandeng Shen, Ding Yuan, Rony Keppens, Xiaozhou Zhao, Libo Fu, Zehao Tang, Jiaoyang Wang, Chengrui Zhou

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How Transverse Waves Drive Turbulence in the Solar Corona by Thomas Howson

“…Oscillatory power is pervasive throughout the solar corona, and magnetohydrodynamic (MHD) waves may carry a significant energy flux throughout the Sun’s atmosphere. …”
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A Near-half-century Simulation of the Solar Corona by Valentin Aslanyan, Karen A. Meyer, Roger B. Scott, Anthony R. Yeates

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Oscillatory Reconnection as a Plasma Diagnostic in the Solar Corona by Konstantinos Karampelas, James A. McLaughlin, Gert J. J. Botha, Stéphane Régnier

“…This gives us a quantified relation for oscillatory reconnection, to be used as a plasma diagnostic in the solar corona, opening up the possibility of using oscillatory reconnection for coronal seismology.…”
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How Nonlinearity Changes Different Parameters in the Solar Corona by S. Sabri, S. Poedts, H. Ebadi

“…We consider different velocity amplitudes of incident waves to study nonlinearity effects on the plasma parameters around a magnetic null point in the solar corona. This could query the seismological methods used to observe and interpret damping profiles of oscillations of magnetic structures, based on linear theory. …”
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Tracking of an electron beam through the solar corona with LOFAR by Mann, G, Breitling, F, Vocks, C, Aurass, H, Steinmetz, M, Strassmeier, K, Bisi, M, Fallows, R, Gallagher, P, Kerdraon, A, Mackinnon, A, Magdalenic, J, Rucker, H, Anderson, J, Asgekar, A, Avruch, I, Bell, M, Bentum, M, Bernardi, G, Best, P, Birzan, L, Bonafede, A, Broderick, J, Brueggen, M, Butcher, H, Ciardi, B, Corstanje, A, de Gasperin, F, de Geus, E, Deller, A, Duscha, S, Eisloeffel, J, Engels, D, Falcke, H, Fender, R, Ferrari, C, Frieswijk, W, Garrett, M, Griessmeier, J, Gunst, A, van Haarlem, M, Hassall, T, Heald, G, Hessels, J, Hoeft, M, Horandel, J, Horneffer, A, Juette, E, Karastergiou, A, Klijn, W, Kondratiev, V, Kramer, M, Kuniyoshi, M, Kuper, G, Maat, P, Markoff, S, McFadden, R, McKay-Bukowski, D, McKean, J, Mulcahy, D, Munk, H, Nelles, A, Norden, M, Orru, E, Paas, H, Pandey-Pommier, M, Pandey, V, Pizzo, R, Polatidis, A, Rafferty, D, Reich, W, Rottgering, H, Scaife, A, Schwarz, D, Serylak, M, Sluman, J, Smirnov, O, Stappers, B, Tagger, M, Tang, Y, Tasse, C, ter Veen, S, Thoudam, S, Toribio, M, Vermeulen, R, van Weeren, R, Wise, M, Wucknitz, O, Yatawatta, S, Zarka, P, Zensus, J

On the shape of force–free field lines in the solar corona by Prior, C, Berger, M

Ion Kinetics of Plasma Interchange Reconnection in the Lower Solar Corona by Vladimir Krasnoselskikh, Arnaud Zaslavsky, Anton Artemyev, Clara Froment, Thierry Dudok de Wit, Nour E. Raouafi, Oleksiy V. Agapitov, Stuart D. Bale, Jaye L. Verniero

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Periodic Variations of Solar Corona Index during 1939–2020 by Rui Tang, Yu Fei, Chun Li, Wen Liu, Xinan Tian, Zhongjie Wan

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Ion Heating by a Fast Magnetosonic Turbulence in the Solar Corona by S. A. Markovskii, Bernard J. Vasquez

“…We carry out three-dimensional kinetic simulations with particle ions and fluid electrons to evaluate the proton and alpha-particle heating produced by the damping of the fast waves in the solar corona. Realistic parameters at 5 solar radii, including the fluctuation amplitude, are used. …”
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Extended MHD modeling of the steady solar corona and the solar wind by Tamas I. Gombosi, Bart van der Holst, Ward B. Manchester, Igor V. Sokolov

“…Abstract The history and present state of large-scale magnetohydrodynamic modeling of the solar corona and the solar wind with steady or quasi-steady coronal physics is reviewed. …”
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Suprathermal Electron Transport and Electron Beam Formation in the Solar Corona by Bofeng Tang, Haihong Che, Gary P. Zank, Vladimir I. Kolobov

Subjects: “…Solar corona…”
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Research Paper: Solar Corona Flares and Its Effect on the Earth’s Atmosphere by Sima Zeighami, Ehsan Tavabi, Hedye Rostaii

“…Solar winds result from the eruption of plasma streams from the solar corona. This plasma, which consists of proton particles, electrons, X-rays, and radio waves, penetrates the heliosphere and accelerates from the interplanetary space toward the Earth with high kinetic energy and thermal energy. …”
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Nonequilibrium Ionization Effects on Synthetic Spectra in the AWSoM Solar Corona by J. Szente, E. Landi, B. van der Holst

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