papers
Publications (19)
astro-ph.SR2013
Kelvin-Helmholtz instability of a coronal streamer
Li Feng, Bernd Inhester, Weiqun Gan
astro-ph2006
Testing non-linear force-free coronal magnetic field extrapolations with the Titov-Demoulin equilibrium
Thomas Wiegelmann, Bernd Inhester, Bernhard Kliem +2
astro-ph.SR2017
Nonlinear force-free coronal magnetic stereoscopy
Iulia Chifu, Thomas Wiegelmann, Bernd Inhester
astro-ph2006
Stereoscopy basics for the STEREO mission
Bernd Inhester
astro-ph.SR2016
Analysis of UV and EUV emission from impacts on the Sun after 2011 June 7 eruptive flare
Davina Innes, Philipp Heinrich, Bernd Inhester +1
astro-ph.SR2009
A Critical Assessment of Nonlinear Force-Free Field Modeling of the Solar Corona for Active Region 10953
Marc L. DeRosa, Carolus J. Schrijver, Graham Barnes +16
astro-ph.IM2018
On the error analyses of polarization measurements of the white-light coronagraph aboard ASO-S
Li Feng, Hui Li, Bernd Inhester +4
astro-ph.SR2011
2D and 3D Polar Plume Analysis from the Three Vantage Positions of STEREO/EUVI A, B, and SOHO/EIT
Judith de Patoul, Bernd Inhester, Li Feng +1
astro-ph2006
Magnetic Stereoscopy
Thomas Wiegelmann, Bernd Inhester
astro-ph.SR2016
Comparison of CME/shock propagation models with heliospheric imaging and in situ observations
Xinhua Zhao, Ying D. Liu, Bernd Inhester +3
astro-ph.SR2010
The solar magnetic field
Sami K. Solanki, Bernd Inhester, Manfred Schüssler
astro-ph.SR2013
Polar plumes' orientation and the Sun's global magnetic field
Judith de Patoul, Bernd Inhester, Robert Cameron
astro-ph2006
Inversion of coronal Zeeman and Hanle Observations to reconstruct the coronal magnetic field
Maxim Kramar, Bernd Inhester
astro-ph.SR2016
Thomson Scattering in the Solar Corona
Bernd Inhester
astro-ph.SR2015
Radial Flow Pattern of a Slow CME
Li Feng, Bernd Inhester, Weiqun Gan
astro-ph2006
Preprocessing of vector magnetograph data for a non-linear force-free magnetic field reconstruction
Thomas Wiegelmann, Bernd Inhester, Takashi Sakurai
astro-ph.SR2016
Measure the Propagation of a halo CME and Its Driven Shock with the Observations from a Single Perspective at Earth
Lei Lu, Bernd Inhester, Li Feng +2
astro-ph.SR2012
Comparisons of CME morphological characteristics derived from five 3D reconstruction methods
Li Feng, Bernd Inhester, Mierla Marilena
astro-ph.SR2015
Why does the apparent mass of a coronal mass ejection increase?
Li Feng, Yuming Wang, Fang Shen +4