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
Infrared continuum observations of five-minute oscillations
โ Scribed by C. A. Lindsey
- Book ID
- 104642973
- Publisher
- Springer
- Year
- 1977
- Tongue
- English
- Weight
- 920 KB
- Volume
- 52
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
โฆ Synopsis
Infrared continuum observations of the Sun at wavelengths between 10p, and 30p, show a nonisothermal response of the upper photosphere to compression waves associated with the fiveminute oscillations. Observations were made with four broad-band filters with effective transmission wavelengths between 10p, and 26ix and with a 10" aperture. Further observations at submillimeter wavelengths with a 2' aperture did not resolve oscillatory fluctuations of five-minute period.
Comparisons with velocity field data of Howard (1976) suggest that the relaxation time of the photosphere exceeds (300/2w) seconds at the height of formation of the 26p, continuum (~soooA-10-2). The photosphere reponds to 3 mHz oscillatory motion with considerably less cgmpression than expected for simple acoustic modes in an adiabatically responsive atmosphere, confirming the evanescent character of the five-minute oscillations.
๐ SIMILAR VOLUMES
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