In recent years radiation has been observed from planets, Sun and stars that is best explained by the cyclotron maser instability; in fact, all celestial bodies that might feasibly emit and be detected by their cyclotron maser radiation have been detected. Here we review those observations, the dev
โฆ LIBER โฆ
Maser emission of SiO isotopes from stars and the pumping mechanism
โ Scribed by Zhou Zhen-pu; N. Kaifu
- Publisher
- Elsevier Science
- Year
- 1989
- Tongue
- English
- Weight
- 370 KB
- Volume
- 13
- Category
- Article
- ISSN
- 0275-1062
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
Evidence for cyclotron maser emission fr
โ
G. A. Dulk; R. M. Winglee
๐
Article
๐
1987
๐
Springer
๐
English
โ 366 KB
Electron-cyclotron maser emission from t
โ
R. M. Winglee; G. A. Dulk
๐
Article
๐
1986
๐
Springer
๐
English
โ 235 KB
Very bright and highly circularly polarized radio bursts from the Sun, the planets, flare stars, and close binary stars are attributed to the electron-cyclotron maser instability. The mode and frequency of the dominant radiation from the maser instability is shown to be dependent on the plasma tempe
MERLIN polarimetry of the OH maser emiss
โ
M. Szymczak; R. J. Cohen; A. M. S. Richards
๐
Article
๐
1999
๐
John Wiley and Sons
๐
English
โ 295 KB
Delayed neutron emission from the decay
โ
E. Roeckl; P.F. Dittner; R. Klapisch; C. Thibault; C. Rigaud; R. Prieels
๐
Article
๐
1974
๐
Elsevier Science
๐
English
โ 559 KB
The A โ X emission spectra of PbS and Pb
โ
Richard A. Teichman III; Eugene R. Nixon
๐
Article
๐
1975
๐
Elsevier Science
๐
English
โ 549 KB
Physical conditions in emission regions
โ
V. P. Grinin
๐
Article
๐
1980
๐
Springer
๐
English
โ 991 KB