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
সংরক্ষণ করুন:
| প্রধান লেখক: | |
|---|---|
| সংস্থা লেখক: | |
| অন্যান্য লেখক: | |
| বিন্যাস: | Livre numérique |
| ভাষা: | Anglais |
| প্রকাশিত: |
Berlin [etc.] :
Springer
[20..].
Cham : Springer Nature |
| মালা: | Lecture notes in physics
114 |
| বিষয়গুলি: | |
| অনলাইন ব্যবহার করুন: | Accès sur la plateforme de l'éditeur Accès sur la plateforme Istex Accès Université d'Orléans Accès INSA CVL |
| টীকা: |
Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| Autres localisations: | Voir dans le Sudoc |
| Edition sous un autre format: | • 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, edited by D. F. Gray and J. L. Linsky, 1980, Berlin, Springer-Verlag, 1 vol. (VII-308 p.), Lecture notes in physics, 3-540-09737-6 • Stellar Turbulence, Texte imprimé, 9783662214046 |
সূচিপত্রের সারণি:
- 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.