OBSERVATIONS OF SOLAR RADIATION CONDUCTED DURING SOLAR ECLIPSE ON JUNE 30TH, 1954, IN BYURAKAN,
FOREIGN TECHNOLOGY DIV WRIGHT-PATTERSON AFB OHIO
Pagination or Media Count:
A solar eclipse, which was visible over the European part of the Soviet Union in June 1954, was observed at wavelengths of 4.2, 1.5, 0.5 m. The observational procedures are described and the resultant data are discussed. It is confirmed that the long wavelength emissions originate primarily in the corona, while the short wavelengths emanate almost entirely from the lower layers of the corona.