Some characteristics of the local radio sources from the observations of the solar eclipse on the 7th of March 1970 in Cuba

Journal Article · Sat Jan 01 00:00:00 EST 1972 · Izv. Krym. Astrofiz. Observ., v. 46, pp. 136-143

OSTI ID:4362702

Yurovskii, Yu F; Yurovskaya, L I

The analysis of the observational data received during solar eclipse on the 7th of March 1970 has shown that the sources of S-component at the wavelength 10 cm correspond to all sunspots. The maximum radio emlssion above unipolar sunspots do not show apparent displacement relative to the radius passing through the center of these sunspots. In complex groups the brightest part of radio source is displaced from the preceding sunspot to following smaller ones which are of the opposite polarity. Two sources of noise storm were found at wavelengih 1.37 m. The noise bursts regions didn't coincide on the disk of Sun with the regions of continuum but were located just beside them. (auth)

• Research Organization: Originating Research Org. not identified
• NSA Number: NSA-29-016580
• OSTI ID: 4362702
• Journal Information: Izv. Krym. Astrofiz. Observ., v. 46, pp. 136-143, Other Information: Orig. Receipt Date: 30-JUN-74
• Country of Publication: Country unknown/Code not available
• Language: Russian

Related Subjects

N56400* -Physics (Astrophysics & Cosmology)-Solar Phenomena
*SUNSPOTS- RADIOWAVE RADIATION
BRIGHTNESS
ECLIPSE
SUN