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The Interaction of Successive Coronal Mass Ejections: A Review
Noé Lugaz, Manuela Temmer, Yuming Wang +1
We present a review of the different aspects associated with the interaction of successive CMEs in the corona and inner heliosphere, focusing on the initiation of series of CMEs, t…
Verification of high-speed solar wind stream forecasts using operational solar wind models
Martin A. Reiss, Manuela Temmer, Astrid M. Veronig +4
High-speed solar wind streams emanating from coronal holes are frequently impinging on the Earth's magnetosphere causing recurrent, medium-level geomagnetic storm activity. Modelin…
Projection effects in coronal dimmings and associated EUV wave event
Karin Dissauer, Manuela Temmer, Astrid M. Veronig +2
We investigate the high-speed ( 1000 km s) extreme-ultraviolet (EUV) wave associated with an X1.2 flare and coronal mass ejection (CME) from NOAA active region 11283 on…
The Exceptional Aspects of the Confined X-class Flares of Solar Active Region 2192
Julia K. Thalmann, Yang Su, Manuela Temmer +1
During late October 2014, active region NOAA 2192 caused an unusual high level of solar activity, within an otherwise weak solar cycle. While crossing the solar disk, during a peri…
Kinematical properties of coronal mass ejections
Manuela Temmer
Coronal mass ejections (CMEs) are the most dynamic phenomena in our solar system. They abruptly disrupt the continuous outflow of solar wind by expelling huge clouds of magnetized…
Chromospheric evaporation flows and density changes deduced from Hinode/EIS during an M1.6 flare
P. Gömöry, A. M. Veronig, Y. Su +2
We analyzed high-cadence sit-and-stare observations acquired with the Hinode/EIS spectrometer and HXR measurements acquired with RHESSI during an M-class flare. During the flare im…