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Detailed Reference Information |
Breech, B., Matthaeus, W.H., Minnie, J., Oughton, S., Parhi, S., Bieber, J.W. and Bavassano, B. (2005). Radial evolution of cross helicity in high-latitude solar wind. Geophysical Research Letters 32: doi: 10.1029/2004GL022321. issn: 0094-8276. |
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We employ a turbulence transport theory to explain the high-latitude radial evolution of cross helicity, or Alfv¿nicity, observed by the Ulysses spacecraft. Evolution is slower than at low latitudes due to weakened shear driving. |
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BACKGROUND DATA FILES |
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Abstract |
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Keywords
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 |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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