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Cyclotron Heating of the Solar Corona
Astrophysics and Space Science, 1998A physical model of the solar transition region and corona is presented, in which plasma flows in rapidly-diverging coronal funnels and holes are described within the framework of a two-fluid model including wave-particle interactions. The ions are heated by wave dissipation and accelerated by the pressure gradient of high-frequency Alfven waves, which
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Parker Solar Probe Enters the Magnetically Dominated Solar Corona
Physical Review Letters, 2021Davin Larson +2 more
exaly
Waves and Turbulence in the Solar Corona
2004In the solar corona (and solar wind) waves and turbulence occur at all scales ranging from the particles’ gyroradii to the size of a solar radius (or even to an astronomical unit). A concise review of some new observations and theories of waves in the sun’s atmosphere and corona is given, with the focus being on coronal waves that are magnetically ...
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Magnetohydrodynamic modeling of the global solar corona
Physics of Plasmas, 1999Roberto Lionello +2 more
exaly