Low-Speed Solar Winds Observed at Distances of 20-60 RS and Coronal Structure of their Source Regions

Details Low-Speed Solar Winds Observed at Distances of 20-60 RS and Coronal Structure of their Source Regions Low-Speed Solar Winds Observed at Distances of 20-60 RS and Coronal Structure of their Source Regions

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994kofu.symp..105k&link_type=abstract

In: Proceedings of Kofu Symposium, Kofu, Japan, Sept. 6-10, 1993, p.105-108.

Physics

Scientific paper

The interplanetary scintillation (IPS) can probe the solar wind at distance and latitude range where in situ measurements have been impossible. Using the IPS method very low-speed (< 200 km/s) solar winds were observed at coronal active regions. Low-speed (~300 km/s) winds can be observed even around a polar coronal hole, and this winds is observed with a speed of 600 km/s at R > 60Rs.

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