- Astron. Nachr. / AN 999, No. 88, 789 792 (2006) / DOI please set DOI! Dynamo Action in The Presence of an Imposed Magnetic Field
- THE ASTROPHYSICAL JOURNAL, 525:10321041, 1999 November 10 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
- TURBULENT CONVECTION UNDER THE INFLUENCE OF ROTATION: SUSTAINING A STRONG DIFFERENTIAL ROTATION
- The Astrophysical Journal, 648: L157L160, 2006 September 10 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.
- SENSITIVITY OF p AND gMODES ON SPECIFIED PHYSICAL PROCESSES OF SOLAR MODELING
- Ecole Doctorale d'Astronomie d'Ile de France ESE de DOCTORAT
- The Astrophysical Journal, 555:L69--L73, 2001 The American Astronomical Society. reserved. Printed
- Astron. Nachr. / AN 000, No. 00, 1 4 (0000) / DOI please set DOI! Rapid Rotation, Active Nests of Convection and Global-scale Flows in
- MEAN FLOWS IN ROTATING TURBULENT CONVECTIVE SHELLS Allan Sacha Brun & Juri Toomre
- THE SOLAR TACHOCLINE: WHERE DO WE STAND? Allan Sacha Brun
- STELLAR CONVECTION : Theory and Models by Dr. A.S. Brun and M.S. Miesch
- Highlights of Astronomy, Vol 12 ASP Conference Series, in press, 2001
- Astronomische Nachrichten Astronomical Notes
- LiBeB, Cosmic Rays and GammaRay Line Astronomy ASP Conference Series, Vol. 171, 1999
- Influence of the Tachocline on Solar Evolution A. S. Brun 1 and J.P. Zahn
- Astronomy & Astrophysics manuscript no. (will be inserted by hand later)
- A&A 474, 145154 (2007) DOI: 10.1051/0004-6361:20077653
- Astronomy & Astrophysics manuscript no. dynamobenchmark3 c ESO 2008 February 15, 2008
- Astron. Nachr. / AN 328, No. 10, 1137 1141 (2007) / DOI 10.1002/asna.200710846 Nonlinear simulations of magnetic instabilities in stellar radiation
- A&A 474, 239250 (2007) DOI: 10.1051/0004-6361:20077070
- Astronomy & Astrophysics manuscript no. BrunZahn.v6 c ESO 2006 March 20, 2006
- ON THE INTERACTION BETWEEN DIFFERENTIAL ROTATION AND MAGNETIC FIELDS IN THE SUN
- SIMULATIONS OF CORE CONVECTION IN ROTATING A-TYPE STARS: DIFFERENTIAL ROTATION AND OVERSHOOTING
- 3-D MHD SIMULATIONS OF THE SOLAR CONVECTION ZONE AND TACHOCLINE Allan Sacha Brun
- DIFFERENTIAL ROTATION WHEN THE SUN SPUN FASTER Benjamin P. Brown, Matthew K. Browning, Allan Sacha Brun, and Juri Toomre
- Astron. Nachr. / AN 328, No. 10, 1100 1103 (2007) / DOI 10.1002/asna.200710849 Dynamo action in simulations of penetrative solar convection with an
- F. Combes, D. Barret, T. Contini, F. Meynadier and L. Pagani (eds) TURBULENT CONVECTION AND DYNAMO ACTION IN
- Astron. Nachr. / AN 328, No. 3/4, 329 338 (2007) / DOI 10.1002/asna.200610739 Towards using modern data assimilation and weather forecasting
- MACROSCOPIC PROCESSES IN THE SOLAR INTERIOR A.S. Brun 1;2 , S. TurckChi`eze 1 , J.P. Zahn 2
- LowDegree LowOrder Solar P Modes As Seen By GOLF Onboard SoHO.
- SENSITIVITY OF THE SOUND SPEED TO THE PHYSICAL PROCESSES INCLUDED IN THE STANDARD SOLAR MODEL
- THE ASTROPHYSICAL JOURNAL, 506 : 913925, 1998 October 20 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.
- FIRST VIEW OF THE SOLAR CORE FROM GOLF ACOUSTIC MODES
- Mixing Below the Solar Convective Zone A. S. Brun 1,2 and S. TurckChieze
- Draft version October 10, 2005 Preprint typeset using LATEX style emulateapj v. 10/10/03
- STRUCTURE AND EVOLUTION OF GIANT CELLS IN GLOBAL MODELS OF SOLAR CONVECTION Mark S. Miesch
- SIMULATIONS OF TURBULENT CONVECTION IN ROTATING YOUNG SOLARLIKE STARS: DIFFERENTIAL ROTATION AND MERIDIONAL CIRCULATION
