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Showing 2011 · physics.space-phShow all
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physics.space-ph2011★ 47 cited
Apparent temperature anisotropies due to wave activity in the solar wind
Daniel Verscharen, Eckart Marsch
The fast solar wind is a collisionless plasma permeated by plasma waves on many different scales. A plasma wave represents the natural interplay between the periodic changes of the…
physics.space-ph2011★ 118 cited
Intermittent heating in the solar corona employing a 3D MHD model
Sven Bingert, Hardi Peter
We investigate the spatial and temporal evolution of the heating of the corona of a cool star such as our Sun in a three-dimensional magneto-hydrodynamic (3D MHD) model. We solve t…