During a period of intense decametric continuum arising near the center of the sun, there occurred additional very strong emission closely associated with the flare beginning at 1522 UT on August 28, 1966. Owing to strong ionospheric absorption from about 1527 UT on, which eliminated telecommunicati
The Sagamore Hill Solar Radio Observatory and the event of August 28, 1966
β Scribed by J. P. Castelli; G. A. Michael
- Publisher
- Springer
- Year
- 1967
- Tongue
- English
- Weight
- 226 KB
- Volume
- 1
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
The slowly varying solar radio and X-ray emissions are considered theoretically and statistically concerning their significance as potential indicators of energy storage processes in active regions leading to large flare-burst events. A correlation analysis has been carried out in order to test diff
An energetic solar proton and electron evcnt was observed by particle detcctors aboard Explorer 33 (AIMP-I) and OGO-3 during the period July . [16][17][18][19] 1966. Optical and radio observations of the sun suggest that these particles were produced by a Ilare which may have occurred on July 16 nea
The results are given of observation of solar radio emission of the S-component at 8.15 ram-2 and 2.25 ram-2 made with the 22 m radio telescope of the Crimean Astrophysical Observatory. Solar radio images are obtained at both wavelengths. The data are presented of radio emission intensity and bright