Thomas Wiegelmann
Thomas Wiegelmann
MPI for Solar System Research
Bestätigte E-Mail-Adresse bei - Startseite
Zitiert von
Zitiert von
Structure, stability, and evolution of magnetic flux ropes from the perspective of magnetic twist
R Liu, B Kliem, VS Titov, J Chen, Y Wang, H Wang, C Liu, Y Xu, ...
The Astrophysical Journal 818 (2), 148, 2016
Computing nonlinear force-free coronal magnetic fields in spherical geometry
T Wiegelmann
Solar Physics 240, 227-239, 2007
Changes of magnetic structure in three dimensions associated with the X3. 4 flare of 2006 December 13
J Jing, T Wiegelmann, Y Suematsu, M Kubo, H Wang
The Astrophysical Journal 676 (1), L81, 2008
Broad Hα wings from the optically thin stellar wind of the hot components in symbiotic binaries
A Skopal
Astronomy & Astrophysics 457 (3), 1003-1010, 2006
Quasi-static three-dimensional magnetic field evolution in solar active region noaa 11166 associated with an x1. 5 flare
P Vemareddy, T Wiegelmann
The Astrophysical Journal 792 (1), 40, 2014
Source region of the 18 November 2003 coronal mass ejection that led to the strongest magnetic storm of cycle 23
N Srivastava, SK Mathew, RE Louis, T Wiegelmann
Journal of Geophysical Research: Space Physics 114 (A3), 2009
A comparison of preprocessing methods for solar force-free magnetic field extrapolation
M Fuhrmann, N Seehafer, G Valori, T Wiegelmann
Astronomy & Astrophysics 526, A70, 2011
Magneto-static modeling of the mixed plasma beta solar atmosphere based on Sunrise/IMaX data
T Wiegelmann, T Neukirch, DH Nickeler, SK Solanki, VM Pillet, ...
The Astrophysical Journal 815 (1), 10, 2015
Comparison between the eruptive X2. 2 flare on 2011 February 15 and confined X3. 1 flare on 2014 October 24
J Jing, Y Xu, J Lee, NV Nitta, C Liu, SH Park, T Wiegelmann, H Wang
Research in Astronomy and Astrophysics 15 (9), 1537, 2015
in Proceedings: Modern Solar Facilities—Advanced Solar Science
C Denker, DE Gary, TR Rimmele
Eds. F. Kneer, KG Puschmann & D. Wittmann 31, 2007
Reconstruction of 3D coronal magnetic structures from THEMIS/MTR and Hinode/SOT vector maps
B Schmieder, Y Guo, G Aulanier, P Démoulin, T Török, V Bommier, ...
Hinode-3: The 3rd Hinode Science Meeting 454, 363, 2012
A comparision of nonlinear force-free extrapolations based on SDO/HMI and SOLIS/VSM data
JK Thalmann, A Pietarila, X Sun, T Wiegelmann
Nonlinear Force-Free Extrapolation of Vector Magnetograms into the Corona
JK Thalmann, T Wiegelmann, X Sun, JT Hoeksema, Y Liu, T Tadesse
AGU Fall Meeting Abstracts 2011, SH33C-05, 2011
Evolution of Magnetic Field in the Flaring Active Region 11158 Observed by SDO/HMI
X Sun, T Hoeksema, Y Liu, T Wiegelmann, K Hayashi
AAS/Solar Physics Division Abstracts# 42 42, 21.01, 2011
Nonpotentiality of Chromospheric Fibrils in the Active Regions NOAA 9661 and NOAA 11092
J Jing, Y Yuan, K Reardon, T Wiegelmann, N Deng, Y Xu, H Wang
AAS/Solar Physics Division Abstracts# 42 42, 17.38, 2011
First Result of Field Extrapolation Based on HMI Vector Magnetic Data
X Sun, JT Hoeksema, T Wiegelmann, K Hayashi, Y Liu
AGU Fall Meeting Abstracts 2010, SH11A-1607, 2010
An Attempt in Incorporating Local and Global Coronal Magnetic Field Modeling
X Sun, JT Hoeksema, X Zhao, T Wiegelmann
American Astronomical Society Meeting Abstracts# 216 216, 402.15, 2010
The Formation of Magnetic Channel by Emergence of Current-carrying Magnetic Field
EK Lim, J chul Chae, J Jing, H Wang, T Wiegelmann
한국천문학회보 34 (2), 26-26, 2009
A First Step Towards a Nonlinear and Self-consistent Modelling of the Interface Region Between Photosphere, Chromosphere and Corona
T Wiegelmann, T Neukirch
AGU Fall Meeting Abstracts 2008, SH51C-02, 2008
Nonlinear force-free field models
T Wiegelmann, J Thalmann, B Inhester
37th COSPAR Scientific Assembly 37, 3462, 2008
Das System kann den Vorgang jetzt nicht ausführen. Versuchen Sie es später erneut.
Artikel 1–20