- Sound Speed Variations Near the Photosphere due to Entropy Perturbations in 3D Numerical
- WHAT CAUSES p-MODE ASYMMETRY REVERSAL? Dali Georgobiani and Robert F. Stein
- ON THE ORIGIN OF THE BASAL EMISSION FROM STELLAR ATMOSPHERES: ANALYSIS OF SOLAR C ii LINES
- ASP Conference Series, Vol. **VOLUME***, **YEAR OF PUBLICATION** **NAMES OF EDITORS**
- THE NEW CHROMOSPHERE MATS CARLSSON
- J. Fluid Mech. (1995), vol. 000, pp. 000--000 Copyright c
- Multi-Wavelength Investigations of Solar Activity Proceedings IAU Symposium No. 223, 2004
- J. Astrophys. Astr. (0000) 00, 000{000 Magnetoconvection and the Solar Dynamo
- SOLAR SURFACE MAGNETOCONVECTION AND DYNAMO ACTION Robert F. Stein 1 and Ake Nordlund 2
- THE ASTROPHYSICAL JOURNAL, 546:585603, 2001 January 1 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
- ASP Conference Series, Vol. **VOLUME***, **YEAR OF PUBLICATION** **NAMES OF EDITORS**
- Solar MagnetoConvection David J. Bercik
- MagnetoConvection R. F. Stein, D. Georgobiani and D. J. Bercik
- ASP Conference Series, Vol. **VOLUME***, **YEAR OF PUBLICATION** **NAMES OF EDITORS**
- Mon. Not. R. Astron. Soc. 000, 000--000 (0000) Printed 20 March 2000 (MN L A T E X style file v1.4) The response of a turbulent accretion disc to an imposed
- WAVES IN THE MAGNETIZED SOLAR ATMOSPHERE. II. WAVES FROM LOCALIZED SOURCES IN MAGNETIC FLUX CONCENTRATIONS
- ASYMMETRY REVERSAL IN SOLAR ACOUSTIC MODES Dali Georgobiani 1 , Robert F. Stein 1 , and #
- Institute of Theoretical Astrophysics University of Oslo
- Stellar evolution with a variable mixinglength parameter Regner Trampedach and Robert F. Stein
- Simulations of Solar Granulation: I. General Properties R. F. Stein
- IL NUOVO CIMENTO Vol. ?, N. ? ? Solar Convection and MagnetoConvection Simulations
- arXiv:astro-ph/0110208v19Oct2001 IL NUOVO CIMENTO Vol. ?, N. ? ?
- DYNAMIC BEHAVIOR OF THE SOLAR ATMOSPHERE ROBERT F. STEIN AND MATS CARLSSON
- Modelling of Stellar Atmospheres IAU Symposium, Vol. xxx, xxxx
- Realistic Solar Convection Simulations Robert F. Stein
- Nordlund, A. and Stein, R. F.: 1990, ``3D Simulations of Solar and Stellar Convection and Magnetoconvection'', Computer Phys. Communications 59, 119
- A&A 463, 297308 (2007) DOI: 10.1051/0004-6361:20041953
- Figure 5. The total energy flux and the fluxes that contribute to it (enthalpy, radiative, kinetic energy and viscous) are shown for a toy so
- A&A manuscript no. (will be inserted by hand later)
- NEARSURFACE CONSTRAINTS ON THE STRUCTURE OF STELLAR CONVECTION ZONES
- RADIATION SHOCK DYNAMICS IN THE SOLAR CHROMOSPHERE --RESULTS OF NUMERICAL SIMULATIONS
- A&A 403, 303312 (2003) DOI: 10.1051/0004-6361:20030356
- Chromospheric Dynamics ---What Can Be Learnt from Numerical Simulations
- FORMATION OF CALCIUM H AND K GRAINS Mats Carlsson
- Dynamic Hydrogen Ionization Mats Carlsson
- EXCITATION AND DAMPING OF PMODES AKE NORDLUND
- A&A manuscript no. (will be inserted by hand later)
- THE ASTROPHYSICAL JOURNAL, 546:576584, 2001 January 1 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
- Living Rev. Solar Phys., 6, (2009), 2 http://www.livingreviews.org/lrsp-2009-2 in solar physics
- Local helioseismology and correlation tracking analysis of surface structures in realistic simulations of solar convection
- VELOCITIES MEASURED IN SMALL-SCALE SOLAR MAGNETIC ELEMENTS ystein Langangen, Mats Carlsson,1
- Surface Convection Robert F. Stein*, David Benson''', Dali Georgobiani*, Ake Nordlund** and
- SIMULATION OF QUIET-SUN WAVES IN THE Ca ii INFRARED TRIPLET A. Pietarila,1
- Astron. Nachr. / AN 326, No. 8, 681692 (2005) / DOI 10.1002/asna.200510411 Effect of the radiative background flux in convection
- J. Astrophys. Astr. (2005) 26, 171184 Excitation of Solar-like Oscillations: From PMS to MS Stellar Models
- OSCILLATION POWER SPECTRA OF THE SUN AND OF CEN A: OBSERVATIONS VERSUS MODELS Reza Samadi1
- The Astrophysical Journal, 610:L137L140, 2004 August 1 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A.
- A&A 404, 11291137 (2003) DOI: 10.1051/0004-6361:20030504
- A&A 377, L14L17 (2001) DOI: 10.1051/0004-6361:20011160
- Astron. Astrophys. 359, 729742 (2000) ASTROPHYSICS
- Exploring magnetohydrodynamic turbulence on the computer
- THE NONMAGNETIC SOLAR CHROMOSPHERE MATS CARLSSON
- THE ASTROPHYSICAL JOURNAL, 564:508524, 2002 January 1 ( 2002. The American Astronomical Society. All rights reserved. Printed in U.S.A.
- SOLAR SMALL-SCALE MAGNETOCONVECTION R. F. Stein
- UNDERSTANDING THE CONVECTIVE SUN Regner Trampedach 1 , Dali Georgobiani 1 , Robert F. Stein 1 , and Ake Nordlund 2
- Realistic Solar Surface Convection Simulations Robert F. Stein
- A&A 419, 747756 (2004) DOI: 10.1051/0004-6361:20034159
- The Excitation of Solar Oscillations \Gamma\GammaObservations and Simulations
- MHD Simulations on Parallel Computers R.F. Stein \Lambda Klaus Galsgaard y Ake Nordlund y
- IAU Colloquium 176 THE IMPACT OF LARGESCALE SURVEYS ON PULSATING STAR RESEARCH ASP Conference Series, Vol. 3 \Theta 10 8
- EXCITATION OF CHROMOSPHERIC WAVE TRANSIENTS BY COLLAPSING GRANULES R. Skartlien #
- Astron. Nachr./AN 32X (200X) X, XXX--XXX Waves in magnetic flux concentrations: The critical role of mode
- Numerical Simulations of Oscillation Modes of the Solar Convection Zone
- CALCIUM II PHASE RELATIONS AND CHROMOSPHERIC DYNAMICS
- HIGH DEGREE SOLAR OSCILLATIONS IN 3D NUMERICAL SIMULATIONS Dali Georgobiani1
- EXCITATION OF RADIAL P-MODES IN THE SUN AND STARS ROBERT STEIN1, DALI GEORGOBIANI1, REGNER TRAMPEDACH1,
- CONVECTION AND PMODES R. F. Stein 1 and A. Nordlund 2
- A&A manuscript no. (will be inserted by hand later)
- Convection Simulations A. Nordlund
- VALIDATION OF TIME-DISTANCE HELIOSEISMOLOGY BY USE OF REALISTIC SIMULATIONS OF SOLAR CONVECTION
- Stellar background power spectra from hydrodynamical simulations of stellar atmospheres
