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Solar coronal heating and weak fast shocks
2002It is suggested that protons and minor ions in the solar corona can be heated and accelerated by fast shocks.
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Coronal heating and solar wind acceleration by turbulence
2006Observations such as Spartan and SOHO UVCS have challenged ideas for the acceleration of the solar wind by constraining models to produce >1.5 Million K protons, several hundred km~s-1 radial outflows, and >700 km~s-1 terminal speeds in the wind emanating from polar coronal holes, with coronal electrons remaining cooler than protons.
VERDINI, ANDREA +2 more
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HEATING CORONAL HOLES AND ACCELERATING THE SOLAR WIND
1992The special energy requirements of a coronal hole combined with current knowledge of the limited dissipation of Alfven and fast mode MHD waves in the solar corona suggest a unique source of heat for the coronal hole. The near coronal hole requires approximately 3 - 4 x 10 exp 5 ergs/sq cm s, which can come only from the fluid jets, fast particles, and ...
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Understanding coronal heating and solar wind acceleration: Case for in situ near-Sun measurements
Reviews of Geophysics, 2007D J Mccomas +2 more
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Solar flares, microflares, nanoflares, and coronal heating
Solar Physics, 1991Hugh S Hudson, Hudson H S
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On the relationship between coronal heating, magnetic flux, and the density of the solar wind
Journal of Geophysical Research, 2010Pete Riley +2 more
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Effect of time-dependent coronal heating on the solar wind
Journal of Geophysical Research, 2002ØYSTEIN Lie-Svendsen +2 more
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Highly structured slow solar wind emerging from an equatorial coronal hole
Nature, 2019S D Bale, J W Bonnell, Trevor A Bowen
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