Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995soph..156..377m&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 156, no. 2, p. 377-393
Astronomy and Astrophysics
Astronomy
36
Interplanetary Medium, Scintillation, Solar Physics, Solar Wind Velocity, Sun, Indexes (Ratios), International Cooperation, Radio Telescopes, Shock Wave Propagation, Sky Surveys (Astronomy), Solar Activity
Scientific paper
The recently refurbished Ooty Radio Telescope in southern India was used in a two-month campaign of interplanetary scintillation (IPS) observations in collaboration with the Cambridge IPS array in England during Apr.-May 1992. The unique feature of this campaign was that, for the first time, scintillation enhancements were predicted in real time by observing solar events on 7-8 May, 1992 and then detected at both Ooty and Cambridge. Also, for the first time, high spatial resolution (approximately 100 sources/sr) solar wind all-sky velocity maps were obtained at Ooty. Good consistency is found between the IPS observations from both observatories and in-situ shocks detected at Earth by IMP-8. Yohkoh soft X-ray images were used to infer the generation of a coronal mas ejection on 7 May 1992.
Ananthakrishnan S.
Detman T. R.
Dryer Murray
Kahn Jeff
Kojima Masamichi
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