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Observational study of the five-minute oscillations in the solar atmosphere

✍ Scribed by K. R. Sivaraman


Publisher
Springer
Year
1973
Tongue
English
Weight
323 KB
Volume
33
Category
Article
ISSN
0038-0938

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πŸ“œ SIMILAR VOLUMES


Observational study of the five-minute o
✍ K. R. Sivaraman πŸ“‚ Article πŸ“… 1973 πŸ› Springer 🌐 English βš– 658 KB

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

The five-minute oscillations in the sola
✍ S. M. Chitre; M. H. Gokhale πŸ“‚ Article πŸ“… 1975 πŸ› Springer 🌐 English βš– 370 KB

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

Wave propagation in a non-isothermal atm
✍ C. Chiuderi; C. Giovanardi πŸ“‚ Article πŸ“… 1979 πŸ› Springer 🌐 English βš– 776 KB

This paper presents a detailed discussion of the properties of linear, periodic acoustic waves that propagate vertically in a non-isothermal atmosphere. In order to retain the basic feature of the solar atmosphere we have chosen a temperature profile presenting a minimum. An analytical solution of t

Solar seeing and the spatial properties
✍ John H. Thomas πŸ“‚ Article πŸ“… 1972 πŸ› Springer 🌐 English βš– 625 KB

A numerical simulation of observations of the spatial properties of the five-minute oscillations is carried out, assuming the oscillations are internal gravity waves excited by granular convection according to the theory of Thomas et al. (1971). The simulation includes the effects of seeing and fini