It is suggested that longitudinal compression waves are propagating parallel to the solar surface from the umbra towards the photosphere. It is shown that the line-absorption coefficient is asymmetrical, when integrated over a wavelength of the compression wave. The effect of the waves on the line p
The umbral flash as a magneto-acoustic wave phenomenon
โ Scribed by Ove Havnes
- Book ID
- 104645273
- Publisher
- Springer
- Year
- 1970
- Tongue
- English
- Weight
- 388 KB
- Volume
- 13
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
The suggestion that an 'umbra flash' may be caused by a magneto-acoustic wave phenomenon is examined. It is suggested that the flash in Call lines is formed during the compressional stage in a magneto-acoustic wave. The compression which is assumed to be adiabatic will produce a rise in temperature and a corresponding increase in number of CaiI atoms. The variations in line emission (absorption) coefficient of the Cali K-line are calculated on this assumption and are found to be in general agreement with the observed variations. Other observed quantities as proper motion, magnitude of line shift etc., also agree with the wave hypothesis. Further observations which may serve as tests on the wave hypothesis are suggested.
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