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Multi-wavelength observations of the 2014 June 11 M3.9 flare: temporal and spatial characteristics

Research in Astronomy and Astrophysics 2019年第7期19卷 123-132页

作者： Damian J.Christian David Kuridze David B.Jess Menoa Yousefi Mihalis Mathioudakis Department of Physics and Astronomy California State University NorthridgeNorthridgeCA 91330USA Institute of Mathematics Physics and Computer ScienceAberystwyth UniversityCeredigionCymruSY23 3UK Astrophysics Research Center School of Mathematics and PhysicsQueen's University BelfastBelfast BT7 INNUK

We present multi-wavelength observations of an M-class flare(M3.9) that occurred on 2014 June *** observations were conducted with the Dunn Solar Telescope(DST),employing adaptive optics,the multi-camera system Rapid Oscillations in Solar Atmosphere(ROSA),the new Hydrogen-Alpha Rapid Dynamics camera(HARDcam) in various wavelengths,such as Ca II K,Mg I b2(at 5172.7 A),and Hα narrow band and G-band continuum *** were re-constructed using the Kiepenheuer-Institut Speckle Interferometry Package(KISIP) code,to improve our image *** observed intensity increases of ≈120%–150% in the Mg,Ca K and Hα narrow band filters during the *** increases for the flare observed in the SDO EUV channels were several times larger,and the X-rays,as recorded by GOES,increased over a factor of 30 for the harder *** a modest delay was found between the onset of flare ribbons of a nearby sympathetic flare and the main flare ribbons observed in these narrow band *** peak flare emission occurred within a few seconds for the Ca K,Mg and Hα *** techniques indicate propagation velocities of ≈60 km s^-1 for the main flare ribbon and as high as300 km s^-1 for smaller regions,which we attribute to filament *** result and delays and velocities observed with SDO(≈100 km s^-1) for different coronal heights agree well with the simple model of energy propagation versus height,although a more detailed model for the flaring solar atmosphere is ***,we detected marginal quasi-periodic pulsations(QPPs) in the 40–60 s range for the Ca K,Mg and Hα bands,and such measurements are important for disentangling the detailed flare-physics.

关键词： magnetic reconnection-sun flares-sun atmosphere

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