Equivalent widths of weak and moderately strong Fraunhofer lines observed in an area roughly 3500 โข 10000 km in extent are found to show small variations of the order of 1 mA, on a time scale of minutes. The dependence of amplitude on line strength and excitation closely fits that predicted for a co
Five minute microwave solar oscillations
โ Scribed by F. M. Strauss; P. Kaufmann; R. Opher
- Publisher
- Springer
- Year
- 1980
- Tongue
- English
- Weight
- 264 KB
- Volume
- 67
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
Oscillations with a period of 5.6 min were observed on 10 July, 1978 while tracking at 22 GHz the active region McMath 15403. The oscillations were strong, clearly defined, had no damping, and lasted for about two hours. The rarity of the phenomenon is indicated by the fact that it occurred only once in more than 250 hr of solar observations. The possibility that these oscillations are due to a standing Alfv6n wave driven by the photospheric velocity field is discussed.
๐ SIMILAR VOLUMES
The acoustic overstability in a polytropic plane-parallel atmosphere with superadiabatic temperature gradient and radiative dissipation is demonstrated for optically thick disturbances. The periods of oscillation are found to be in the range 250-480 s and the associated wavelength of the order of 40
The 5-min oscillations in the photospheric velocity fields have been studied in detail from measurements on 14 absorption lines from three time sequences of spectrograms of high quality. The lines cover a range of heights in the solar atmosphere from log z = + 0.2 to --1.2. Regions oscillating coher