933 MHz IPS velocity measurements at EISCAT

Details 933 MHz IPS velocity measurements at EISCAT 933 MHz IPS velocity measurements at EISCAT

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..382..180k&link_type=abstract

Proceedings of the eigth international solar wind conference: Solar wind eight. AIP Conference Proceedings, Volume 382, pp. 180

Physics

1

Particle Emission, Solar Wind, Solar Instruments

Scientific paper

Two-antenna scintillation observations (IPS), made at the EISCAT observatory in northern Scandinavia, provide unusually accurate measurements of the solar wind speed near the Sun. Here we show how the long inter-antenna baselines at EISCAT allow us to separate the contributions of fast and slow wind to a single IPS observation. We show as examples, an IPS observation of a quasi-static structure and one of a transient event.

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