Interplanetary scintillation observations with the Cocoa Cross radio telescope

Details Interplanetary scintillation observations with the Cocoa Cross radio telescope Interplanetary scintillation observations with the Cocoa Cross radio telescope

Feb 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976jgr....81..695c&link_type=abstract

Journal of Geophysical Research, vol. 81, Feb. 1, 1976, p. 695-697.

Astronomy and Astrophysics

Astronomy

1

Interplanetary Medium, Radio Sources (Astronomy), Radio Telescopes, Scintillation, Block Diagrams, Channels (Data Transmission), Solar Wind

Scientific paper

Physical and electrical parameters for the 34.3-MHz Cocoa Cross radio telescope are given. The telescope is dedicated to the determination of solar-wind characteristics in and out of the ecliptic plane through measurement of electron-density irregularity structure as determined from IPS (interplanetary scintillation) of natural radio sources. The collecting area (72,000 sq m), angular resolution (0.4 deg EW by 0.6 deg NS), and spatial extent (1.3 km EW by 0.8 km NS) make the telescope well suited for measurements of IPS index and frequency scale for hundreds of weak radio sources without serious confusion effects.

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