2021/01/31 by Yuhu Miao, Dong Li, Ding Yuan +4
Earth and Planetary Sciences · Physics and Astronomy · #Core (optical fiber) #Coronal mass ejection #Earthquake Detection and Analysis #Excited state #Extrapolation #Flare #Ionosphere and magnetosphere dynamics #Magnetic field #Magnetogram #Magnetohydrodynamic drive #Solar and Space Plasma Dynamics #Solar flare #astro-ph.SR
paper · pdf · doi:10.3847/2041-8213/abdfce
ApJL,10 pages,5 figures
openalex publication_date 2021/02/01 · arxiv created 2021/02/07 · openalex created_date 2021/02/15 · arxiv updated 2021/03/03 · openalex updated_date 2026/08/06
Abstract Quasi-periodic fast propagating (QFP) waves are often excited by solar flares, and could be trapped in the coronal structure with low Alfvén speed, so they could be used as a tool for diagnosing both the flaring core and magnetic waveguide. As the periodicity of a QFP wave could originate from a periodic source or be dispersively waveguided, it is a key parameter for diagnosing the flaring core and waveguide. In this paper, we study two QFP waves excited by a Geostationary Operational Environmental Satellite-class C1.3 solar flare occurring at active region NOAA 12734 on 2019 March 8. Two QFP waves were guided by two oppositely oriented coronal funnels. The periods of two QFP waves were identical and were roughly equal to the period of the oscillatory signal in the X-ray and 17 GHz radio emission released by the flaring core. It is very likely that the two QFP waves could be periodically excited by the flaring core. Many features of this QFP wave event are consistent with the magnetic tuning fork model. We also investigated the seismological application with QFP waves, and found that the magnetic field inferred with magnetohydrodynamic seismology was consistent with that obtained in the magnetic extrapolation model. Our study suggests that the QFP wave is a good tool for diagnosing both the flaring core and the magnetic waveguide.