Radio emission of the NGC 1499 nebula at decametric wavelengths
โ Scribed by V. V. Krymkin
- Publisher
- Springer Netherlands
- Year
- 1978
- Tongue
- English
- Weight
- 332 KB
- Volume
- 58
- Category
- Article
- ISSN
- 0004-640X
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
We have observed the slowly varying component of solar radio emission at a frequency of 34.5 MHz with half power beam widths of 26'/40' in the east-west and north-south directions, respectively. It is found that the observed brightness temperatures vary within the limits of 0.3x 106 K to 1.5 x 106 K
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