The profiles of the Fe XlV, 25303, and Fe x, 26374, emission lines of the solar corona have been observed at different positions using a photoelectric scanning Fabry-Perot interferometer. These profiles were obtained during the eclipse of 7th March 1970, in Mexico and at the Pic-du-Midi coronagraph
โฆ LIBER โฆ
Emission lines from the solar corona
โ Scribed by Helen E Mason
- Book ID
- 111100771
- Publisher
- John Wiley and Sons
- Year
- 2008
- Tongue
- English
- Weight
- 425 KB
- Volume
- 49
- Category
- Article
- ISSN
- 1366-8781
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
An interferometric investigation of emis
โ
P. M. Marshall; G. Henderson
๐
Article
๐
1973
๐
Springer
๐
English
โ 861 KB
Variation in OviiX-ray line-emission fro
โ
H. R. Rugge; A. B. C. Walker
๐
Article
๐
1970
๐
Springer
๐
English
โ 352 KB
The Yellow Emission Line of the Solar Co
โ
LAYZER, DAVID
๐
Article
๐
1955
๐
Nature Publishing Group
๐
English
โ 205 KB
Emission Lines in the Spectrum of the So
โ
ZESSEWITSCH, W.; NIKONOW, W.
๐
Article
๐
1929
๐
Nature Publishing Group
๐
English
โ 230 KB
Pulsating radio emissions from the solar
โ
A. Abrami
๐
Article
๐
1970
๐
Springer
๐
English
โ 554 KB
Three solar outbursts which show pulsating radio emissions at metric waves (239 MHz) are examined. The behaviour of the single frequency, high-time resolution records and the spectral diagrams seem to indicate that such phenomena are peculiar phases of type IV radiation, perhaps connected with absor
Solar abundance determination from ultra
โ
Andrea K. Dupree; Leo Goldberg
๐
Article
๐
1967
๐
Springer
๐
English
โ 623 KB