Physics – Plasma Physics
Scientific paper
May 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996jgr...10111149m&link_type=abstract
Journal of Geophysical Research, Volume 101, Issue A5, p. 11149-11152
Physics
Plasma Physics
10
Solar Physics, Astrophysics, And Astronomy: Coronal Holes, Interplanetary Physics: Mhd Waves And Turbulence, Space Plasma Physics: Turbulence
Scientific paper
The spatial evolution of the spectral exponent of magnetic field fluctuations in the solar wind is investigated by a comparison of spectra and length functions obtained from Helios for in-ecliptic and from Ulysses for high-latitude observations. A similar radial evolution trend is found in both data sets for the Bz component of the magnetic field, which is least affected by compressive interactions. Yet the fluctuations seem to evolve more slowly in the polar flows as compared with the Alfvénic fluctuations found by the Helios experiments in coronal-hole-related flows near the Sun in the ecliptic plane.
Marsch Eckart
Tu Chia-Ying
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