Stellar Turbulence [electronic resource] : Proceedings of Colloquium 51 of the International Astronomical Union Held at the Universtiy of Western Ontario London, Ontario, Canada August 27–30, 1979 /
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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Format: | Texto biblioteca |
Language: | eng |
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Berlin, Heidelberg : Springer Berlin Heidelberg,
1980
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Subjects: | Physics., Observations, Astronomical., Astronomy, Astrophysics., Astronomy, Observations and Techniques., Astrophysics and Astroparticles., |
Online Access: | http://dx.doi.org/10.1007/3-540-09737-6 |
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KOHA-OAI-TEST:2084212018-07-30T23:39:23ZStellar Turbulence [electronic resource] : Proceedings of Colloquium 51 of the International Astronomical Union Held at the Universtiy of Western Ontario London, Ontario, Canada August 27–30, 1979 / Gray, David F. editor. Linsky, Jeffery L. editor. SpringerLink (Online service) textBerlin, Heidelberg : Springer Berlin Heidelberg,1980.engStellar 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.Physics.Observations, Astronomical.AstronomyAstrophysics.Physics.Astronomy, Observations and Techniques.Astrophysics and Astroparticles.Springer eBookshttp://dx.doi.org/10.1007/3-540-09737-6URN:ISBN:9783540385547 |
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Physics. Observations, Astronomical. Astronomy Astrophysics. Physics. Astronomy, Observations and Techniques. Astrophysics and Astroparticles. Physics. Observations, Astronomical. Astronomy Astrophysics. Physics. Astronomy, Observations and Techniques. Astrophysics and Astroparticles. |
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Physics. Observations, Astronomical. Astronomy Astrophysics. Physics. Astronomy, Observations and Techniques. Astrophysics and Astroparticles. Physics. Observations, Astronomical. Astronomy Astrophysics. Physics. Astronomy, Observations and Techniques. Astrophysics and Astroparticles. Gray, David F. editor. Linsky, Jeffery L. editor. SpringerLink (Online service) Stellar Turbulence [electronic resource] : Proceedings of Colloquium 51 of the International Astronomical Union Held at the Universtiy of Western Ontario London, Ontario, Canada August 27–30, 1979 / |
description |
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. |
format |
Texto |
topic_facet |
Physics. Observations, Astronomical. Astronomy Astrophysics. Physics. Astronomy, Observations and Techniques. Astrophysics and Astroparticles. |
author |
Gray, David F. editor. Linsky, Jeffery L. editor. SpringerLink (Online service) |
author_facet |
Gray, David F. editor. Linsky, Jeffery L. editor. SpringerLink (Online service) |
author_sort |
Gray, David F. editor. |
title |
Stellar Turbulence [electronic resource] : Proceedings of Colloquium 51 of the International Astronomical Union Held at the Universtiy of Western Ontario London, Ontario, Canada August 27–30, 1979 / |
title_short |
Stellar Turbulence [electronic resource] : Proceedings of Colloquium 51 of the International Astronomical Union Held at the Universtiy of Western Ontario London, Ontario, Canada August 27–30, 1979 / |
title_full |
Stellar Turbulence [electronic resource] : Proceedings of Colloquium 51 of the International Astronomical Union Held at the Universtiy of Western Ontario London, Ontario, Canada August 27–30, 1979 / |
title_fullStr |
Stellar Turbulence [electronic resource] : Proceedings of Colloquium 51 of the International Astronomical Union Held at the Universtiy of Western Ontario London, Ontario, Canada August 27–30, 1979 / |
title_full_unstemmed |
Stellar Turbulence [electronic resource] : Proceedings of Colloquium 51 of the International Astronomical Union Held at the Universtiy of Western Ontario London, Ontario, Canada August 27–30, 1979 / |
title_sort |
stellar turbulence [electronic resource] : proceedings of colloquium 51 of the international astronomical union held at the universtiy of western ontario london, ontario, canada august 27–30, 1979 / |
publisher |
Berlin, Heidelberg : Springer Berlin Heidelberg, |
publishDate |
1980 |
url |
http://dx.doi.org/10.1007/3-540-09737-6 |
work_keys_str_mv |
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