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Radial evolution of cross helicity in high-latitude solar wind
Radial evolution of cross helicity in high-latitude solar wind
Abstract
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.
Type
Journal Article
Type of thesis
Series
Citation
Breech, B., Matthaeus, W. H., Minnie, J., Oughton, S., Oarhi, S., Bieber, J. W., & Bavassano, B. (2005). Radial evolution of cross helicity in high-latitude solar wind. Geophysical Research Letters, 32(6), L06103.
Date
2005
Publisher
American Geophysical Union
Degree
Supervisors
Rights
© 2005 the American Geophysical Union