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Zeitschriftenartikel (138)
121.
Zeitschriftenartikel
453, S. 737 - 741 (2006)
Testing non-linear force-free coronal magnetic field extrapolations with the Titov-Démoulin equilibrium. Astronomy and Astrophysics 122.
Zeitschriftenartikel
233, S. 215 - 232 (2006)
Preprocessing of vector magnetograph data for a nonlinear force-free magnetic field reconstruction. Solar Physics 123.
Zeitschriftenartikel
457, S. 1053 - 1058 (2006)
An optimization principle for the computation of MHD equilibria in the solar corona. Astronomy and Astrophysics 124.
Zeitschriftenartikel
228, S. 67 - 78 (2005)
How to use magnetic field information for coronal loop identification. Solar Physics 125.
Zeitschriftenartikel
433, S. 701 - 705 (2005)
Comparing magnetic field extrapolations with measurements of magnetic loops. Astronomy and Astrophysics 126.
Zeitschriftenartikel
432, S. L1 - L4 (2005)
Links between magnetic fields and plasma flows in a coronal hole. Astronomy and Astrophysics 127.
Zeitschriftenartikel
428, S. 629 - 645 (2004)
Coronal plasma flows and magnetic fields in solar active regions Combined observations from SOHO and NSO/Kitt Peak. Astronomy and Astrophysics 128.
Zeitschriftenartikel
219, S. 87 - 108 (2004)
Optimization code with weighting function for the reconstruction of coronal magnetic fields. Solar Physics 129.
Zeitschriftenartikel
225, S. 227 - 247 (2004)
Similarities and differences between coronal holes and the quiet sun: are loop statistics the key? Solar Physics 130.
Zeitschriftenartikel
218, S. 29 - 40 (2003)
A quantitative method to optimise magnetic field line fitting of observed coronal loops. Solar Physics 131.
Zeitschriftenartikel
214, S. 287 - 312 (2003)
Magnetic modelling and tomography: First steps towards a consistent reconstruction of the solar corona. Solar Physics 132.
Zeitschriftenartikel
10, S. 313 - 322 (2003)
Computing nonlinear force free coronal magnetic fields. Nonlinear Processes in Geophysics 133.
Zeitschriftenartikel
9 (2), S. 139 - 147 (2002)
Evolution of magnetic helicity under kinetic magnetic reconnection 2. B ≠ 0 reconnection. Nonlinear Processes in Geophysics 134.
Zeitschriftenartikel
208, S. 233 - 251 (2002)
Including stereoscopic information in the reconstruction of coronal magnetic fields. Solar Physics 135.
Zeitschriftenartikel
8 (3), S. 127 - 140 (2001)
Evolution of magnetic helicity in the course of kinetic magnetic reconnection 1. B=0 reconnection. Nonlinear Processes in Geophysics 136.
Zeitschriftenartikel
7, S. 141 - 150 (2000)
Kinetic simultations of the coupling between current instabilities and reconnection in thin current sheets. Nonlinear Processes in Geophysics 137.
Zeitschriftenartikel
191 (2), S. 391 - 407 (2000)
Helmet Streamers with Triple Structures: Simulations of resistive dynamics. Solar Physics 138.
Zeitschriftenartikel
T74, S. 77 - 81 (1998)
Solar magnetic fields: Triple arcade structures. Physica Scripta Buchkapitel (1)
139.
Buchkapitel
Büchner, J.; Dum, C.; Scholer, M.). Copernicus Gesellschaft 2001 (2001)
Particle code simulation - Tests and limits of Vlasov code simulations and its application to null-helicity and co-helicity reconnection. In: Space Plasma Simulation, S. 58 - 61 (Hg. Konferenzbeitrag (10)
140.
Konferenzbeitrag
Internetwork Horizontal Magnetic Fields in the Quiet Sun Chromoshpere: Results from a Joint Hinode/VTT Study. In: The Second Hinode Science Meeting: Beyond Discovery - Torward Understanding, 327 (Hg. B., L.; M., C.; T., M.; J., M.; K., R.). (2009)