Aulanier, Guillaume - Observatoire de Paris

• Solar Phys (2008) 248: 2950 DOI 10.1007/s11207-008-9155-2
• THE ASTROPHYSICAL JOURNAL, 543:447456, 2000 November 1 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
• THE ASTROPHYSICAL JOURNAL, 540:11261142, 2000 September 10 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
• The 2011/02/15 X2 flare, ribbons, coronal wave, and mass ejection: interpreting the 3-d views from SDO and STEREO guided by MHD flux-rope
• The Astrophysical Journal, 701:19111921, 2009 August 20 doi:10.1088/0004-637X/701/2/1911 C 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
• The Astrophysical Journal, 567:L97L101, 2002 March 1 2002. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• Solar Physics (2006) 238: 347376 DOI: 10.1007/s11207-006-0230-2 C Springer 2006
• COEXISTING FLUX ROPE AND DIPPED ARCADE SECTIONS ALONG ONE SOLAR This article has been downloaded from IOPscience. Please scroll down to see the full text article.
• THE MAGNETIC HELICITY INJECTED BY SHEARING MOTIONS P. DMOULIN1, C. H. MANDRINI2,, L VAN DRIEL-GESZTELYI1,3,4,5,
• The Astrophysical Journal, 724:10831098, 2010 December 1 doi:10.1088/0004-637X/724/2/1083 C 2010. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
• SOLAR PROMINENCE MERGING Guillaume Aulanier
• A&A 444, 961976 (2005) DOI: 10.1051/0004-6361:20053600
• RESISTIVE EMERGENCE OF UNDULATORY FLUX TUBES E. Pariat, G. Aulanier, and B. Schmieder1
• Solar Phys (2009) 258: 5367 DOI 10.1007/s11207-009-9392-z
• The Astrophysical Journal, 693:L27L30, 2009 March 1 doi:10.1088/0004-637X/693/1/L27 c 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
• Astron. Astrophys. 325, 12131225 (1997) ASTROPHYSICS
• SOLAR PROMINENCE INTERACTIONS C. Richard DeVore1
• A&A 465, 603612 (2007) DOI: 10.1051/0004-6361:20065845
• THE ASTROPHYSICAL JOURNAL, 534:482489, 2000 May 1 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
• MAGNETOHYDROSTATIC MODEL OF A BALD-PATCH FLARE G. AULANIER1, P. DMOULIN1, B. SCHMIEDER1, C. FANG2 and Y. H. TANG2
• Solar Phys (2009) 259: 3147 DOI 10.1007/s11207-009-9427-5
• A&A 386, 11061122 (2002) DOI: 10.1051/0004-6361:20020179
• Astron. Astrophys. 335, 309322 (1998) ASTROPHYSICS
• Solar Physics (2006) 237: 85100 DOI: 10.1007/s11207-006-0173-7 C Springer 2006
• The Astrophysical Journal, 708:314333, 2010 January 1 doi:10.1088/0004-637X/708/1/314 C 2010. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
• NONLINEAR FORCE-FREE FIELD MODELING OF A SOLAR ACTIVE REGION AROUND THE TIME OF A MAJOR FLARE AND CORONAL MASS EJECTION
• The Astrophysical Journal, 700:559578, 2009 July 20 doi:10.1088/0004-637X/700/1/559 C 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
• Astron. Astrophys. 342, 867880 (1999) ASTROPHYSICS
• A&A 463, 727736 (2007) DOI: 10.1051/0004-6361:20065673
• A&A 490, 353356 (2008) DOI: 10.1051/0004-6361:200810386
• A&A 508, 433443 (2009) DOI: 10.1051/0004-6361/200912664
• Solar Physics (2006) 236: 7595 DOI: 10.1007/s11207-006-0089-2 C Springer 2006
• Solar Phys (2008) 247: 123150 DOI 10.1007/s11207-007-9085-4
• A&A 526, A137 (2011) DOI: 10.1051/0004-6361/201015231
• Journal of Atmospheric and Solar-Terrestrial Physics 62 (2000) 14371448 www.elsevier.nl/locate/jastp
• A&A 381, 290299 (2002) DOI: 10.1051/0004-6361:20011495
• The Astrophysical Journal, 728:65 (6pp), 2011 February 10 doi:10.1088/0004-637X/728/1/65 C 2011. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
• The Astrophysical Journal, 718:13881399, 2010 August 1 doi:10.1088/0004-637X/718/2/1388 C 2010. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
• The Astrophysical Journal, 704:485495, 2009 October 10 doi:10.1088/0004-637X/704/1/485 C 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
• Mon. Not. R. Astron. Soc. 398, 189200 (2009) doi:10.1111/j.1365-2966.2009.14881.x Surface magnetic fields on two accreting T Tauri stars: CV Cha
• Solar Physics (2006) 238: 245259 DOI: 10.1007/s11207-006-0252-9 C Springer 2006
• A&A 456, 725735 (2006) DOI: 10.1051/0004-6361:20064923
• A&A 430, 10671087 (2005) DOI: 10.1051/0004-6361:20041519
• A&A 423, 11191131 (2004) DOI: 10.1051/0004-6361:20040259
• A&A 402, 769780 (2003) DOI: 10.1051/0004-6361:20030227
• A&A 405, 313323 (2003) DOI: 10.1051/0004-6361:20030359
• CME ASSOCIATED WITH TRANSEQUATORIAL LOOPS AND A BALD PATCH FLARE
• FILAMENT CHANNEL STRUCTURES IN A Si IV LINE RELATED TO A 3D MAGNETIC MODEL
• Astron. Astrophys. 329, 11251137 (1998) ASTROPHYSICS
• G. Aulanier, HDR, Simulation MHD des phnomnes actifs de l'atmosphre solaire Universit Paris Diderot
• A reconnection-driven rarefaction wave model for coronal outflows S. J. Bradshaw
• The Astrophysical Journal, 738:167 (23pp), 2011 September 10 doi:10.1088/0004-637X/738/2/167 C 2011. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
• Solar Phys (2012) 276:451477 DOI 10.1007/s11207-011-9882-7
• Solar Phys (2012) 276:199217 DOI 10.1007/s11207-011-9886-3
• Sigmoidal Active Region on the Sun: Comparison of a Magnetohydrodynamical Simulation and a Non-Linear Force-Free Field Model