Simulations of stellar convection with CO5BOLD
暂无分享,去创建一个
W. Schaffenberger | B. Freytag | M. Steffen | H.-G. Ludwig | S. Wedemeyer-Böhm | O. Steiner | O. Steiner | H. Ludwig | B. Freytag | W. Schaffenberger | M. Steffen | S. Wedemeyer-Böhm | Bernd Freytag | Matthias Steffen | Sven Wedemeyer-Böhm | Werner Schaffenberger | Oskar Steiner
[1] Kenneth G. Powell,et al. Axisymmetric modeling of cometary mass loading on an adaptively refined grid: MHD results , 1994 .
[2] H. Spruit,et al. Is stellar granulation turbulence , 1997 .
[3] A. Vögler,et al. Three-dimensional simulations of magneto-convection in the solar photosphere , 2004 .
[4] E. Spiegel,et al. Stellar convection theory. I. The anelastic Modal equations , 1976 .
[5] H. Gail,et al. Dust Formation in Stellar Winds , 1985 .
[6] Bernd Freytag,et al. Three-dimensional simulations of the atmosphere of an AGB star , 2008 .
[7] R. Blomme,et al. Line formation in solar granulation VI. [Cl], Cl, CH and C2 lines and the photospheric C abundance , 2004, astro-ph/0410681.
[8] M. Asplund,et al. Testing 3D solar models against observations - center-to-limb variations of oxygen lines, spatially-resolved line formation and probing for departures from LTE , 2008 .
[9] M. Schüssler,et al. Models of Magnetic Flux Sheets , 1989 .
[10] U. Jørgensen,et al. Dynamic model atmospheres of AGB stars. I. Atmospheric structure and dynamics , 1998 .
[11] B. Pagel,et al. Stellar atmospheres , 1978, Nature.
[12] Observation of a short-lived pattern in the solar chromosphere , 2006, astro-ph/0609382.
[13] R. Rezaei,et al. The Horizontal Internetwork Magnetic Field: Numerical Simulations in Comparison to Observations with Hinode , 2008, 0801.4915.
[14] A. Brandenburg,et al. Magnetoconvection and dynamo coefficients: Dependence of the alpha-effect on rotation and magnetic field , 2001, astro-ph/0108274.
[15] Y. Suematsu,et al. EXCITATION OF SLOW MODES IN NETWORK MAGNETIC ELEMENTS THROUGH MAGNETIC PUMPING , 2011, 1102.5164.
[16] G. Tóth. The ∇·B=0 Constraint in Shock-Capturing Magnetohydrodynamics Codes , 2000 .
[17] Thierry Emonet,et al. On the Interaction between Convection and Magnetic Fields , 2003 .
[18] M. Roth,et al. Magneto‐acoustic wave propagation and mode conversion in a magnetic solar atmosphere: Comparing results from the CO5BOLD code with ray theory , 2010, 1009.5586.
[19] L. Auer,et al. Short characteristic integration of radiative transfer problems: Formal solution in two-dimensional slabs , 1988 .
[20] Å. Nordlund,et al. Bulk Heating and Slender Magnetic Loops in the Solar Corona , 2002 .
[21] E. Caffau,et al. 3D hydrodynamical CO5BOLD model atmospheres of late-type giants: chemical abundances from molecular lines , 2010, 1010.1722.
[22] Bram van Leer,et al. On the Relation Between the Upwind-Differencing Schemes of Godunov, Engquist–Osher and Roe , 1984 .
[23] A. Vögler. Effects of non-grey radiative transfer on 3D simulations of solar magneto-convection , 2004 .
[24] V. Krishan,et al. Alfvén-like mode in partially ionized solar atmosphere , 2010 .
[25] Paul Glaister,et al. An approximate linearised Riemann solver for the Euler equations for real gases , 1988 .
[26] D. Balsara,et al. A Staggered Mesh Algorithm Using High Order Godunov Fluxes to Ensure Solenoidal Magnetic Fields in Magnetohydrodynamic Simulations , 1999 .
[27] Robert F. Stein,et al. Solar Small-Scale Magnetoconvection , 2006 .
[28] P. Bonifacio,et al. The photospheric solar oxygen project. I. Abundance analysis of atomic lines and influence of atmosp , 2008, 0805.4398.
[29] G. Fisher,et al. Improving Large-scale Convection Zone-to-Corona Models , 2010, 1005.0641.
[30] R. Kurucz. Atlas: a Computer Program for Calculating Model Stellar Atmospheres , 1970 .
[31] James A. Klimchuk,et al. On Solving the Coronal Heating Problem , 2006 .
[32] M. Schüssler,et al. CONVECTIVE INTENSIFICATION OF SOLAR SURFACE MAGNETIC FIELDS : RESULTS OF NUMERICAL EXPERIMENTS , 1998 .
[33] P. Bonifacio,et al. Lithium in the Globular Cluster NGC 6397: Evidence for dependence on evolutionary status , 2009, 0909.0983.
[34] M. Asplund,et al. The chemical composition of the Sun , 2009, 0909.0948.
[35] I. Baraffe,et al. Towards a new generation of multi-dimensional stellar evolution models: development of an implicit hydrodynamic code , 2011, 1103.1524.
[36] A. Tritschler,et al. The solar chromosphere at high resolution with IBIS. IV. Dual-line evidence of heating in chromospheric network , 2009, 0906.2083.
[37] J. Hawley,et al. Simulation of magnetohydrodynamic flows: A Constrained transport method , 1988 .
[38] James M. Stone,et al. Magnetohydrodynamical non‐radiative accretion flows in two dimensions , 2001 .
[39] A. Malagoli,et al. Turbulent supersonic convection in three dimensions , 1990 .
[40] S. M. Chitre,et al. The Current State of Solar Modeling , 1996, Science.
[41] M. Asplund,et al. New light on stellar abundance analyses: Departures from LTE and homogeneity. , 2005 .
[42] Dinshaw S. Balsara,et al. Maintaining Pressure Positivity in Magnetohydrodynamic Simulations , 1999 .
[43] Chi-Wang Shu,et al. Total variation diminishing Runge-Kutta schemes , 1998, Math. Comput..
[44] Bernd Freytag,et al. Spots on the surface of Betelgeuse -- Results from new 3D stellar convection models , 2002 .
[45] U. Jørgensen,et al. Dynamic model atmospheres of AGB stars - III. Effects of frequency-dependent radiative transfer , 2003 .
[46] M. Schuessler,et al. A solar surface dynamo , 2007, astro-ph/0702681.
[47] First local helioseismic experiments with CO5BOLD , 2007, astro-ph/0701029.
[48] J. Toomre,et al. Two Dimensional Compressible Convection Extending Over Multiple Scale Heights , 1984 .
[49] P ? ? ? ? ? ? ? % ? ? ? ? , 1991 .
[50] H. Ludwig,et al. Solution to the problem of the surface gravity distribution of cool DA white dwarfs from improved 3D model atmospheres , 2011, 1106.6007.
[51] F. Allard,et al. Numerical simulations of surface convection in a late M-dwarf , 2002, astro-ph/0208584.
[52] E. Parker. The Origin of Magnetic Fields , 1970 .
[53] C. Cannon. Line transfer in two dimensions , 1970 .
[54] L. Lindegren,et al. Solar granulation - Influence of convection on spectral line asymmetries and wavelength shifts , 1981 .
[55] R. Stein,et al. Excitation of Chromospheric Wave Transients by Collapsing Granules , 2000 .
[56] E. Spiegel,et al. The Eddington Approximation in the Radiative Heat Equation , 1966 .
[57] M. Schüssler,et al. Model calculations of magnetic flux tubes. II: Stationary results for solar magnetic elements , 1984 .
[58] N. Weiss,et al. Convection and magnetic fields in stars , 1981 .
[59] B. Jurcevich,et al. The Solar Optical Telescope for the Hinode Mission: An Overview , 2007, 0711.1715.
[60] Å. Nordlund,et al. Accurate Radiation Hydrodynamics and MHD Modeling of 3‐D Stellar Atmospheres , 2009 .
[61] R. Rezaei,et al. Hinode observations reveal boundary layers of magnetic elements in the solar photosphere , 2007, 0711.0408.
[62] W. Rossow. Cloud microphysics: Analysis of the clouds of Earth, Venus, Mars and Jupiter , 1978 .
[63] C. Schrijver. Catastrophic cooling and high-speed downflow in quiescent solar coronal loops observed with TRACE , 2001 .
[64] P. Murdin,et al. Encyclopedia of Astronomy and Astrophysics , 2002 .
[65] Hydrodynamical non-radiative accretion flows in two dimensions , 1999, astro-ph/9908185.
[66] S. Sofia,et al. Compressible magnetic convection : formulation and two-dimensional models , 1991 .
[67] Cambridge,et al. MHD Simulations of Penumbra Fine Structure , 2006, astro-ph/0612648.
[68] P. Roe,et al. On Godunov-type methods near low densities , 1991 .
[69] A. Malagoli,et al. Turbulent compressible convection , 1991 .
[70] W. Abbett,et al. The Magnetic Connection between the Convection Zone and Corona in the Quiet Sun , 2007 .
[71] Kenneth G. Powell,et al. AN APPROXIMATE RIEMANN SOLVER FOR MAGNETOHYDRODYNAMICS (That Works in More than One Dimension) , 1994 .
[72] R. Stothers,et al. Luminosities, masses and periodicities of massive red supergiants , 1971 .
[73] R. Stein,et al. Supergranulation Scale Convection Simulations , 2009 .
[74] K. Powell,et al. Axisymmetric Modeling of Cometary Mass Loading on an Adaptively Refined Grid: Hydrodynamic Results , 2013 .
[75] P. Roe. CHARACTERISTIC-BASED SCHEMES FOR THE EULER EQUATIONS , 1986 .
[76] M. Schuessler,et al. Strong horizontal photospheric magnetic field in a surface dynamo simulation , 2008, 0801.1250.
[77] Allan Sacha Brun,et al. Global-Scale Turbulent Convection and Magnetic Dynamo Action in the Solar Envelope , 2004 .
[78] F. Millour,et al. VLTI/AMBER spectro-interferometric imaging of VX Sagittarii's inhomogenous outer atmosphere , 2009, 0911.4422.
[79] T. Beers,et al. First stars XI. Chemical composition of the extremely metal-poor dwarfs in the binary CS 22876-032 , 2007, 0712.2949.
[80] Robert L. Kurucz,et al. ATLAS12, SYNTHE, ATLAS9, WIDTH9, et cetera , 2005 .
[81] G. D. Nelson. A two-dimensional solar model , 1978 .
[82] S. Poedts,et al. Analysis of the effect of neutral flow on the waves in the solar photosphere , 2007 .
[83] M. Carlsson,et al. Dynamic Hydrogen Ionization , 2002, astro-ph/0202313.
[84] Irene A. Stegun,et al. Handbook of Mathematical Functions. , 1966 .
[85] R. Rutten,et al. Magnetic Coupling between the Interior and Atmosphere of the Sun , 2010 .
[86] M. Schüssler,et al. UNIVERSALITY OF THE SMALL-SCALE DYNAMO MECHANISM , 2011, 1105.0546.
[87] F. Kneer,et al. Acoustic waves in the solar atmosphere at high spatial resolution , 2009 .
[88] M. Norman,et al. ZEUS-2D: A radiation magnetohydrodynamics code for astrophysical flows in two space dimensions. I - The hydrodynamic algorithms and tests. II - The magnetohydrodynamic algorithms and tests , 1992 .
[89] E. Böhm-Vitense,et al. Über die Wasserstoffkonvektionszone in Sternen verschiedener Effektivtemperaturen und Leuchtkräfte. Mit 5 Textabbildungen , 1958 .
[90] P. Bonifacio,et al. Sulphur abundances in halo stars from multiplet 3 at 1045 nm , 2010, 1003.4914.
[91] G. G. Stokes. "J." , 1890, The New Yale Book of Quotations.
[92] E. Toro. Riemann Solvers and Numerical Methods for Fluid Dynamics , 1997 .
[93] H. Ludwig,et al. 3D simulations of M star atmosphere velocities and their influence on molecular FeH lines , 2009, 0910.3493.
[94] Dust formation in winds of long-period variables V. The influence of micro-physical dust properties in carbon stars , 2002, astro-ph/0210282.
[95] Luigi Vigevano,et al. An Evaluation of Roe's Scheme Generalizations for Equilibrium Real Gas Flows , 1997 .
[96] K. Chan,et al. ADI on staggered mesh—A method for the calculation of compressible convection , 1982 .
[97] E. Avrett,et al. Radiative transfer in two-component stellar atmospheres , 1971 .
[98] D. Mihalas,et al. Two-dimensional radiative transfer. I - Planar geometry , 1978 .
[99] Scott W. McIntosh,et al. Waves in the Magnetized Solar Atmosphere. II. Waves from Localized Sources in Magnetic Flux Concentrations , 2003 .
[100] P. Lax,et al. On Upstream Differencing and Godunov-Type Schemes for Hyperbolic Conservation Laws , 1983 .
[101] M. Steffen. A simple method for monotonic interpolation in one dimension. , 1990 .
[102] T. Beers,et al. The metal–poor end of the Spite plateau , 2009, Proceedings of the International Astronomical Union.
[103] P. Bonifacio,et al. Convection and 6Li in the atmospheres of metal-poor halo stars , 2009, Proceedings of the International Astronomical Union.
[105] Martin Schwarzschild,et al. On the scale of photospheric convection in red giants and supergiants. , 1975 .
[106] Peter H. Hauschildt,et al. Parallel Implementation of the PHOENIX Generalized Stellar Atmosphere Program. II. Wavelength Parallelization , 1996, astro-ph/9709238.
[107] P. Matthews,et al. Photospheric convection in strong magnetic fields , 1996 .
[108] Peter H. Hauschildt,et al. Model atmospheres for M (sub)dwarf stars. 1: The base model grid , 1995, astro-ph/9601150.
[109] S. Solanki,et al. QUIET-SUN INTENSITY CONTRASTS IN THE NEAR-ULTRAVIOLET AS MEASURED FROM Sunrise , 2010, 1009.1050.
[110] Excitation of solar-like oscillations across the HR diagram , 2006, astro-ph/0611762.
[111] B. Gudiksen,et al. An Ab Initio Approach to Solar Coronal Loops , 2004, astro-ph/0407267.
[112] D. Psaltis. Two-Dimensional Radiative Transfer , 2001 .
[113] F. Allard,et al. The role of convection, overshoot, and gravity waves for the transport of dust in M dwarf and brown dwarf atmospheres , 2010, 1002.3437.
[114] U. Ziegler,et al. Self-gravitational adaptive mesh magnetohydrodynamics with the NIRVANA code , 2005 .
[115] Edward A. Spiegel,et al. The Smoothing of Temperature Fluctuations by Radiative Transfer . , 1957 .
[116] W. Dobler,et al. Magnetic Field Generation in Fully Convective Rotating Spheres , 2006 .
[117] M. Axer,et al. Balmer lines in cool dwarf stars. I: Basic influence of atmospheric models , 1993 .
[118] M. Carlsson,et al. Radiation shock dynamics in the solar chromosphere - results of numerical simulations , 1994 .
[119] M. Schüssler,et al. Penumbral Structure and Outflows in Simulated Sunspots , 2009, Science.
[120] M. Asplund. Line formation in solar granulation , 2000 .
[121] J. Toomre,et al. Three-dimensional compressible convection at low prandtl numbers , 1990 .
[122] C. Helling,et al. Dust in brown dwarfs. II. The coupled problem of dust formation and sedimentation , 2003 .
[123] Robert F. Stein,et al. Does a nonmagnetic solar chromosphere exist , 1995 .
[124] H. Gail,et al. Dust formation in stellar winds. IV: Heteromolecular carbon grain formation and growth , 1988 .
[125] A. Vecchio,et al. The solar chromosphere at high resolution with IBIS - I. New insights from the Ca II 854.2 nm line , 2007, 0709.2417.
[126] P. Woodward,et al. The Piecewise Parabolic Method (PPM) for Gas Dynamical Simulations , 1984 .
[127] M. Carlsson,et al. Non-equilibrium hydrogen ionization in 2D simulations of the solar atmosphere , 2007, 0709.3751.
[128] N. Weiss,et al. Convection-driven Emergence of Small-Scale Magnetic Fields and their Role in Coronal Heating and Solar Wind Acceleration , 2008 .
[129] T. Berger,et al. The Horizontal Magnetic Flux of the Quiet-Sun Internetwork as Observed with the Hinode Spectro-Polarimeter , 2008 .
[130] E. Caffau,et al. Chemical abundances in metal-poor giants: limitations imposed by the use of classical 1D stellar atmosphere models , 2010, 1010.2507.
[131] M. Steffen,et al. Line Formation in Convective Stellar Atmospheres , 1999 .
[132] Fausto Cattaneo,et al. On the Origin of Magnetic Fields in the Quiet Photosphere , 1999 .
[133] E. Caffau,et al. Can we trust elemental abundances derived in late-type giants with the classical 1D stellar atmosphere models? , 2009, Proceedings of the International Astronomical Union.
[134] A. Lagg,et al. Coupling from the Photosphere to the Chromosphere and the Corona , 2008, 0809.0987.
[135] Oskar Steiner,et al. Dynamic Interaction of Convection with Magnetic Flux Sheets: First Results of a New MHD Code , 1994 .
[136] K. L. Chan,et al. Radiative hydrodynamics models of stellar convection , 2007 .
[137] S. Wedemeyer-Bohm,et al. On the continuum intensity distribution of the solar photosphere , 2009, 0905.0705.
[138] D. Buscher,et al. Detection of a bright feature on the surface of Betelgeuse. , 1990 .
[139] MAGNETOHYDRODYNAMIC SIMULATION FROM THE CONVECTION ZONE TO THE CHROMOSPHERE , 2005 .
[140] J. Zahn. Stellar convection theory , 1980 .
[141] P. Bonifacio,et al. Cu i resonance lines in turn-off stars of NGC 6752 and NGC 6397 Effects of granulation from CO5BOLD models , 2010, 1009.1848.
[142] Åke Nordlund,et al. Numerical Simulations of the Solar Granulation , 1980 .
[143] P. Bonifacio,et al. The CIFIST 3D model atmosphere grid , 2009, 0908.4496.
[144] Time-dependent hydrogen ionisation in 3D simulations of the solar chromosphere. Methods and first results , 2006, astro-ph/0608620.
[145] D. E. Kerr. Physics of Fully Ionized Gases. , 1956 .
[146] I. Kamp,et al. Carbon monoxide in the solar atmosphere I. Numerical method and two-dimensional models , 2005, astro-ph/0503496.
[147] Robert F. Stein,et al. Simulations of Solar Granulation. I. General Properties , 1998 .
[148] G. D. Byrne,et al. VODE: a variable-coefficient ODE solver , 1989 .
[149] W. Thi,et al. Dust in brown dwarfs and extra-solar planets - I. Chemical composition and spectral appearance of quasi-static cloud layers , 2008, 0803.4315.
[150] M. Norman,et al. ZEUS-2D : a radiation magnetohydrodynamics code for astrophysical flows in two space dimensions. II : The magnetohydrodynamic algorithms and tests , 1992 .
[151] Bernd Freytag,et al. Solar Chemical Abundances Determined with a CO5BOLD 3D Model Atmosphere , 2010, 1003.1190.
[152] M. Carlsson,et al. Twisted Flux Tube Emergence From the Convection Zone to the Corona , 2007, 0906.5464.
[153] K. Eriksson,et al. Grid of model atmospheres for metal-deficient giant stars. I , 1975 .
[154] V. Sheminova,et al. Numerical simulation of the interaction between solar granules and small-scale magnetic fields , 1996, 1011.1778.
[155] O. Steiner,et al. Dynamical Interaction of Solar Magnetic Elements and Granular Convection: Results of a Numerical Simulation , 1998 .
[156] L. H. Thomas. THE RADIATION FIELD IN A FLUID IN MOTION , 1930 .
[157] J. Toomre,et al. Stellar convection theory. III - Dynamical coupling of the two convection zones in A-type stars by penetrative motions , 1981 .
[158] M. Knoelker,et al. RADIATIVE MAGNETOHYDRODYNAMIC SIMULATION OF SUNSPOT STRUCTURE , 2008, 0808.3294.
[159] Vasilis Archontis,et al. The Three-dimensional Interaction between Emerging Magnetic Flux and a Large-Scale Coronal Field: Reconnection, Current Sheets, and Jets , 2005 .
[160] Holistic MHD-Simulation from the Convection Zone to the Chromosphere , 2006 .
[161] R. LeVeque. Numerical methods for conservation laws , 1990 .
[162] S. B. F. Dorch,et al. Waves in the Magnetized Solar Atmosphere. I. Basic Processes and Internetwork Oscillations , 2002 .
[163] Juri Toomre,et al. Magnetic fields interacting with nonlinear compressible convection , 1988 .
[164] Gary A. Glatzmaier,et al. Numerical Simulations of Stellar Convective Dynamos , 1984 .
[165] David R. Alexander,et al. THE LIMITING EFFECTS OF DUST IN BROWN DWARF MODEL ATMOSPHERES , 2001 .
[166] P. Bonifacio,et al. Impact of granulation effects on the use of Balmer lines as temperature indicators , 2009, 0906.4697.
[167] G. Mellema,et al. Hydrodynamical models of aspherical planetary nebulae , 1991 .
[168] R. Klein,et al. Dust in brown dwarfs - I. Dust formation under turbulent conditions on microscopic scales , 2001 .
[169] M. Cheung,et al. Moving magnetic tubes: fragmentation, vortex streets and the limit of the approximation of thin flux tubes , 2006 .
[170] P. Cally. What to look for in the seismology of solar active regions , 2007 .
[171] A. Wray,et al. Realistic Numerical Simulations of Solar Convection and Oscillations in Magnetic Regions , 2008 .
[172] A. M. Title,et al. SIMULATION OF THE FORMATION OF A SOLAR ACTIVE REGION , 2010, 1006.4117.
[173] S. Wedemeyer,et al. Numerical simulation of the three-dimensional structure and dynamics of the non-magnetic solar chromosphere , 2003, astro-ph/0311273.
[174] G. Newkirk. Carbon Monoxide in the Solar Atmosphere. , 1957 .
[175] Stuart M. Jefferies,et al. The Energy Flux of Internal Gravity Waves in the Lower Solar Atmosphere , 2008 .
[176] John N. Bahcall,et al. Solar Models: Current Epoch and Time Dependences, Neutrinos, and Helioseismological Properties , 2001 .
[177] P. Petitjean,et al. Line shift, line asymmetry, and the 6Li/7Li isotopic ratio determination , 2007, 0708.3819.
[178] M. Proctor,et al. Oscillatory convection in sunspot umbrae , 1990, Monthly Notices of the Royal Astronomical Society.
[179] J. R. Elliott,et al. Computational aspects of a code to study rotating turbulent convection in spherical shells , 1999, Parallel Comput..
[180] M. Carlsson,et al. The stellar atmosphere simulation code Bifrost , 2011, 1105.6306.
[181] A. Skumanich,et al. The formation of resonance lines in multidimensional media. II. Radiation operators and their numerical representation , 1973 .
[182] John B. Shoven,et al. I , Edinburgh Medical and Surgical Journal.
[183] Gary A. Glatzmaier,et al. Numerical Simulations of Stellar Convective Dynamos. I. The Model and Method , 1984 .
[184] P. Janhunen,et al. A Positive Conservative Method for Magnetohydrodynamics Based on HLL and Roe Methods , 2000 .
[185] M. Rieutord,et al. MHD simulations of the solar photosphere , 2012, 1206.6630.
[186] Kjell Eriksson,et al. A grid of MARCS model atmospheres for late-type stars. I. Methods and general properties , 2008, 0805.0554.
[187] J. Quirk. A Contribution to the Great Riemann Solver Debate , 1994 .
[188] G. Strang. On the Construction and Comparison of Difference Schemes , 1968 .
[189] Åke Nordlund,et al. Numerical simulations of the solar granulation. I - Basic equations and methods , 1982 .
[190] T. Clune,et al. Pumping of Magnetic Fields by Turbulent Penetrative Convection , 1998 .
[191] B. Plez,et al. Radiative hydrodynamics simulations of red supergiant stars - IV. Gray versus non-gray opacities , 2011, 1109.3619.
[192] J. Smagorinsky,et al. GENERAL CIRCULATION EXPERIMENTS WITH THE PRIMITIVE EQUATIONS , 1963 .
[193] Robert F. Stein,et al. Solar Surface Convection , 2009, Living reviews in solar physics.
[194] J. Brackbill,et al. The Effect of Nonzero ∇ · B on the numerical solution of the magnetohydrodynamic equations☆ , 1980 .
[195] P. Lenz,et al. ANTARES – A Numerical Tool for Astrophysical RESearch with applications to solar granulation , 2009, 0905.0177.
[196] O. Steiner. Magnetic Coupling in the Quiet Solar Atmosphere , 2009, 0904.2026.
[197] The metal-poor end of the Spite plateau - I. Stellar parameters, metallicities, and lithium abundances , 2010, 1003.4510.
[198] M. Roth,et al. Modification of wave propagation and wave travel-time by the presence of magnetic fields in the solar network atmosphere , 2012 .
[199] H. Ludwig,et al. HYDRODYNAMICAL MODELS OF STELLAR CONVECTION : THE ROLE OF OVERSHOOT IN DA WHITE DWARFS, A-TYPE STARS, AND THE SUN , 1996 .
[200] USA,et al. Numerical 3D constraints on convective eddy time-correlations: Consequences for stochastic excitation of solar p modes , 2003, astro-ph/0304457.
[201] P. Bonifacio,et al. Galactic evolution of oxygen - OH lines in 3D hydrodynamical model atmospheres , 2010, 1005.3754.
[202] Juri Toomre,et al. Stellar convection theory. II - Single-mode study of the second convection zone in an A-type star , 1976 .
[203] M. Carlsson,et al. 3d Numerical Models of the Chromosphere, Transition Region, and Corona , 2007, 0704.1511.
[204] B. Plez,et al. Radiative hydrodynamics simulations of red supergiant stars - I. interpretation of interferometric observations , 2009, 0907.1860.
[205] Hirohisa Hara,et al. ON REDSHIFTS AND BLUESHIFTS IN THE TRANSITION REGION AND CORONA , 2010, 1001.4769.
[206] T. Greif,et al. The First Stars , 2003, astro-ph/0311019.
[207] P. Bonifacio,et al. Three carbon-enhanced metal-poor dwarf stars from the SDSS - Chemical abundances from CO5BOLD 3D hydrodynamical model atmospheres , 2010, 1002.1670.
[208] M. Figueroa,et al. Energy for Transport , 2014 .
[209] Forrest J. Rogers,et al. Spin-Orbit Interaction Effects on the Rosseland Mean Opacity , 1992 .
[210] Carolus J. Schrijver,et al. Solar surface magnetism , 1994 .