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Rapid Changes of Photospheric Magnetic Field after Tether-Cutting Reconnection and Magnetic Implosion
Chang Liu, Na Deng, Rui Liu +6
The rapid, irreversible change of the photospheric magnetic field has been recognized as an important element of the solar flare process. This Letter reports such a rapid change of…
Particle kinetic analysis of a polar jet from SECCHI COR data
L. Feng, B. Inhester, J. de Patoul +2
Aims. We analyze coronagraph observations of a polar jet observed by the Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI) instrument suite onboard the Solar TEr…
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
Polar plumes are seen as elongated objects starting at the solar polar regions. Here, we analyze these objects from a sequence of images taken simultaneously by the three spacecraf…
LEMUR: Large European Module for solar Ultraviolet Research. European contribution to JAXA's Solar-C mission
Luca Teriaca, Vincenzo Andretta, Frédéric Auchère +39
Understanding the solar outer atmosphere requires concerted, simultaneous solar observations from the visible to the vacuum ultraviolet (VUV) and soft X-rays, at high spatial resol…
Coronal Magnetic Field Structure and Evolution for Flaring AR 11117 and its Surroundings
Tilaye Tadesse, T. Wiegelmann, B. Inhester +1
In this study, photospheric vector magnetograms obtained with the Synoptic Optical Long-term Investigations of the Sun survey (SOLIS), are used as boundary conditions to model the…
Magnetic Connectivity between Active Regions 10987, 10988, and 10989 by Means of Nonlinear Force-Free Field Extrapolation
T. Tadesse, T. Wiegelmann, B. Inhester +1
Extrapolation codes for modelling the magnetic field in the corona in cartesian geometry do not take the curvature of the Sun's surface into account and can only be applied to rela…