๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Observations and analysis of lunar radio emission at 3.09 mm wavelength

โœ Scribed by Bobby L. Ulich; John R. Cogdell; John H. Davis; Ted A. Calvert


Publisher
Springer Netherlands
Year
1974
Tongue
English
Weight
556 KB
Volume
10
Category
Article
ISSN
1573-0794

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


Observation of solar radio emission by t
โœ V. A. Efanov; A. G. Kislyakov; I. G. Moiseev; A. I. Naumov ๐Ÿ“‚ Article ๐Ÿ“… 1969 ๐Ÿ› Springer ๐ŸŒ English โš– 463 KB

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

Observations and interpretation of the s
โœ Ch. V. Sastry; K. S. Dwarkanath; R. K. Shevgaonkar; V. Krishan ๐Ÿ“‚ Article ๐Ÿ“… 1981 ๐Ÿ› Springer ๐ŸŒ English โš– 517 KB

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

Radio interferometric observations of so
โœ M. R. Kundu; P. E. Angerhofer ๐Ÿ“‚ Article ๐Ÿ“… 1979 ๐Ÿ› Springer ๐ŸŒ English โš– 219 KB

Several solar active regions were observed during the 1976 vernal equinox with the 3-element interferometer of the National Radio Astronomy Observatory. The element spacings for these observations were 600, 2100, and 2700 m, resulting in maximum angular resolutions of about 3 arc sec at 3.7 cm and 8