Manuela Temmer

TL;DR: An overview of solar flares and associated phenomena, drawing upon a wide range of observational data primarily from the RHESSI era, is presented in this paper, where the focus is on different areas of flare phenomena (footpoints and ribbons, coronal sources, relationship to coronal mass ejections) and their interconnections.

TL;DR: An overview of solar flares and associated phenomena, drawing upon a wide range of observational data primarily from the RHESSI era, is presented in this article, with the emphasis on the observations from multiple points of view, while bearing in mind the models that link them to each other and to theory.

TL;DR: In this article, the authors present the "Drag-Based Model" (DBM) of heliospheric propagation of interplanetary coronal mass ejections (ICMEs) based on the hypothesis that the driving Lorentz force, which launches a CME, ceases in the upper corona and that beyond a certain distance the dynamics becomes governed by the interaction of the ICME and the ambient solar wind.

TL;DR: In this article, the authors presented extreme ultraviolet and X-ray observations of a solar flare showing magnetic reconnection with a level of clarity not previously achieved, including inflowing cool loops and newly formed outflowing hot loops.

TL;DR: In this article, a statistical analysis of almost 50,000 soft X-ray (SXR) flares observed by GOES during the period 1976-2000 is presented, and the results of the analysis with respect to statistical flare models, the idea of coronal heating by nanoflares, and elaborate on implications of the obtained results on the Neupert effect in solar flares.