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Stellar Turbulence : Proceedings of Colloquium 51 of the International Astronomical Union, Held at the University of Western Ontario, London, Ontario, Canada, August 27-30, 1979

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目次 Stellar convection theory
Instabilities in a polytropic atmosphere
On the dynamics of the solar convection zone
Thermal and continuum driven convection in B-stars
The height dependence of granular motion
Numerical simulation of the solar granulation
Differential rotation in stars with convection zones
Generation of oscillatory motions in the stellar atmosphere
The evolution of an average solar granule
Observed solar spectral line asymmetries and wavelength shifts due to convection
Differential line shifts in late type stars
Temporal and spatial fluctuations in widths of solar EUV lines
Formation of the profiles of absorption lines in the inhomogeneous medium
The determination of stellar turbulence by low resolution techniques
Analysis of high resolution stellar line profiles
Examples of non-thermal motions as seen on the sun
Diagnostic use of FE II H & K wing emission lines
Turbulence in main sequence stars
Observational aspects of macroturbulence in early type stars
Photospheric Macroturbulence in late-type stars
Depth-dependence of turbulence in stellar atmospheres
Turbulence in the atmospheres of eclipsing binary stars
Differential line-shifts
Time dependence of Balmer progression in the spectrum of HD 92207
Microturbulence : Age dependences
High luminosity F-K stars motions and H? emissions
Turbulence in the atmosphere of B-type starsmissions
Mesoturbulence
Stochastic approach
The application of mesoturbulence to stellar atmospheres
Effects of acoustic waves on spectral line profiles
Some effects of strong acoustic waves on strong spectral lines
Numerical simulation of granular convection: Effects on photospheric spectral line profiles
Mechanical energy transport
Stellar chromospheres
Observations of the outer atmospheric regions of ? Orionis
Stellar-winds and coronas in cool stars
Relationship between envelope structure and energy source of non-thermal motions
An analysis of microturbulence in the atmosphere of the F-type supergiant gamma cygni
The solar chromospheric microturbulence and the emission observed at eclipse
Excitation dependent gf-values and depth dependent microturbulences
On the structural and stochastic motions in the solar and stellar atmospheres
I U E observations of circumstellar lines and mass loss from B-star
On the establishment of internally consistent abundance-oscillator strength scales
Differential rotation and magnetic activity of the lower main sequence stars
Changes of photospheric line asymmetries with effective temperature
Small-scale versus large scale motions in the solar atmosphere derived from a non-LTE calculation of multiplet 38 of Ti I
Effects of flux tubes on conventional chromospheric diagnostics
Summary.
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登録日 2020.06.27
更新日 2020.06.28