Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000angeo..18.1003m&link_type=abstract
Annales Geophysicae, Volume 18, Issue 9, p.1003
Astronomy and Astrophysics
Astrophysics
3
Interplanetary Physics (Solar Wind Plasma, Sources Of The Solar Wind) - Solar Physics, Astrophysics And Astronomy (Instruments And Techniques)
Scientific paper
Observations of interplanetary scintillation (IPS) allow accurate solar wind velocity measurements to be made at all heliographic latitudes and at a range of distances from the Sun. The data may be obtained with either single, double or multiple antennas, each requiring a different method of analysis. IPS data taken during the 1998 whole sun month (30th July-31st August 1998) by EISCAT, the ORT (Ooty Radio Telescope), India, and the Nagoya IPS system, Japan, allow the results of individual methods of analysis to be compared. Good agreement is found between the velocity measurements using each method, and when combined an improved understanding of the structure of the solar wind can be obtained.
Ananthakrishnan S.
Balasubramanian Vijay
Breen Andrew Robert
Canals Agusti
Fallows Richard Andrew
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