81 citations · 317 across the 14 of their papers we have counts for
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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…
astro-ph.SR2010★ 81 cited
A Kinetic Alfven wave cascade subject to collisionless damping cannot reach electron scales in the solar wind at 1 AU
J. J. Podesta, J. E. Borovsky, S. P. Gary
(Abridged) Turbulence in the solar wind is believed to generate an energy cascade that is supported primarily by Alfvén waves or Alfvénic fluctuations at MHD scales and by kinetic…