Radial evolution of cross helicity in high-latitude solar wind

Details Radial evolution of cross helicity in high-latitude solar wind Radial evolution of cross helicity in high-latitude solar wind

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005georl..3206103b&link_type=abstract

Geophysical Research Letters, Volume 32, Issue 6, CiteID L06103

Physics

Plasma Physics

20

Interplanetary Physics: Interplanetary Magnetic Fields, Interplanetary Physics: Mhd Waves And Turbulence (2752, 6050, 7836), Interplanetary Physics: Solar Wind Plasma, Space Plasma Physics: Mhd Waves And Instabilities (2149, 2752, 6050), Space Plasma Physics: Turbulence (4490)

Scientific paper

We employ a turbulence transport theory to explain the high-latitude
radial evolution of cross helicity, or Alfvénicity, observed by
the Ulysses spacecraft. Evolution is slower than at low latitudes due to
weakened shear driving.

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