activity
19932026
most citedA turbulence-driven model for heating and acceleration of the fast wind in coronal holes

234 citations · 6.4k across the 170 of their papers we have counts for

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Showing 2010Show all

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astro-ph.SR2010

Ultraviolet Coronagraph Spectroscopy: A Key Capability for Understanding the Physics of Solar Wind Acceleration

S. R. Cranmer, J. L. Kohl, D. Alexander +21

Understanding the physical processes responsible for accelerating the solar wind requires detailed measurements of the collisionless plasma in the extended solar corona. Some key c…

physics.flu-dyn2010★ 20 cited

Large scale behavior and statistical equilibria in rotating flows

P. D. Mininni, P. Dmitruk, W. H. Matthaeus +1

We examine long-time properties of the ideal dynamics of three--dimensional flows, in the presence or not of an imposed solid-body rotation and with or without helicity (velocity-v…