Signatures of magnetic reconnection in solar eruptive flares: A multi-wavelength perspective
arXiv:1211.2914 · doi:10.1007/978-3-642-30442-2_4
Abstract
In this article, we review some key aspects of a multi-wavelength flare which have essentially contributed to form a standard flare model based on the magnetic reconnection. The emphasis is given on the recent observations taken by the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) on the X-ray emission originating from different regions of the coronal loops. We also briefly summarize those observations which do not seem to accommodate within the canonical flare picture and discuss the challenges for future investigations.
13 pages; Book chapter published in "Multi-scale Dynamical Processes in Space and Astrophysical Plasmas", Springer-Verlag Berlin Heidelberg
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Cited by in corpus (7)
- Formation and eruption of a flux rope from the sigmoid active region NOAA 11719 and associated M6.5 flare: A multi-wavelength study
- Blowout Jets and Impulsive Eruptive Flare in a Bald-Patch Topology
- HXR emission from an activated flux rope and subsequent evolution of an eruptive long duration solar flare
- Eruptive-Impulsive Homologous M-class Flares Associated with Double-Decker Flux Rope Configuration in Mini-Sigmoid of NOAA 12673
- A Study of a long duration B9 flare-CME event and associated piston-driven shock
- Investigation of two coronal mass ejections from circular ribbon source region: Origin, Sun-Earth propagation and Geo-effectiveness
- Two-stage evolution of an extended C-class eruptive flaring activity from sigmoid active region NOAA 12734: SDO and Udaipur-CALLISTO observations