Physics
Scientific paper
Jun 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sowi.conf...62k&link_type=abstract
Nagoya Univ., International Solar Wind 8 Conference, p. 62
Physics
Solar Wind, Scintillation, Solar Wind Velocity, Interplanetary Space, Coronal Holes, Solar Corona, Bias, Line Of Sight, Electron Scattering, Wave Scattering, Magnetohydrodynamic Waves
Scientific paper
The radial distance dependence of solar wind speeds, which were measured by interplanetary scintillation method, has been studied especially for a high-speed solar wind, and large increase of the IPS speeds (300 km/s) was observed at the distance range of 0.1 - 0.3 AU. When the streams are mapped back onto the source surface, they distribute in polar coronal holes or their boundaries. Since the IPS measurement can be biased by several effects such as of line-of-sight integration, strong scattering and random velocities, we examined these biasing effects and have found difficulty to explain the large IPS speed increase with the biasing effects.
Kojima Masamichi
Misawa Hiroaki
Watanabe Hiroko
Yamauchi Yoshiaki
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