Interplanetary scintillation measurements of high-speed flow in the low-latitude solar wind

Details Interplanetary scintillation measurements of high-speed flow in the low-latitude solar wind Interplanetary scintillation measurements of high-speed flow in the low-latitude solar wind

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..471..317b&link_type=abstract

The solar wind nine conference. AIP Conference Proceedings, Volume 471, pp. 317-320 (1999).

Physics

Solar Wind Plasma, Sources Of Solar Wind, Radio, Microwave

Scientific paper

Observations of interplanetary scintillation (IPS) made using the EISCAT
facility provide accurate measurements of solar wind velocity between 15
and 120 solar radii (R). In this paper we present observations of the
solar wind at low latitudes made between 1991 and 1998, with particular
emphasis on flow from trans-equatorial coronal holes.

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