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_a10.1007/3-540-09737-6 _2doi |
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_aStellar Turbulence _h[electronic resource] : _bProceedings of Colloquium 51 of the International Astronomical Union Held at the Universtiy of Western Ontario London, Ontario, Canada August 27–30, 1979 / _cedited by David F. Gray, Jeffery L. Linsky. |
| 264 | 1 |
_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg, _c1980. |
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| 300 | _bonline resource. | ||
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_atext _btxt _2rdacontent |
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_acomputer _bc _2rdamedia |
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_aonline resource _bcr _2rdacarrier |
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_aLecture Notes in Physics, _x0075-8450 ; _v114 |
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| 505 | 0 | _aStellar 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. | |
| 650 | 1 | 4 |
_aAstronomy, Observations and Techniques. _0http://scigraph.springernature.com/things/product-market-codes/P22014 |
| 650 | 2 | 4 |
_aAstrophysics and Astroparticles. _0http://scigraph.springernature.com/things/product-market-codes/P22022 |
| 700 | 1 |
_aGray, David F. _eeditor. _4edt _4http://id.loc.gov/vocabulary/relators/edt |
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| 700 | 1 |
_aLinsky, Jeffery L. _eeditor. _4edt _4http://id.loc.gov/vocabulary/relators/edt |
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| 710 | 2 | _aSpringerLink (Online service) | |
| 773 | 0 | _tSpringer eBooks | |
| 776 | 0 | 8 |
_iPrinted edition: _z9783540097372 |
| 776 | 0 | 8 |
_iPrinted edition: _z9783662214046 |
| 830 | 0 |
_aLecture Notes in Physics, _x0075-8450 ; _v114 |
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| 856 | 4 | 0 | _uhttps://doi.org/10.1007/3-540-09737-6 |
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