Eruptions from coronal bright points: A spectroscopic view by IRIS of a mini-filament eruption, QSL reconnection, and reconnection-driven outflows
arXiv:2202.00370 · doi:10.1051/0004-6361/202142439
Abstract
The present study investigates a mini-filament eruption associated with cancelling magnetic fluxes. The eruption originates from a small-scale loop complex commonly known as a Coronal Bright Point (CBP). The event is uniquely recorded in both the imaging and spectroscopic data taken with IRIS. We analyse IRIS spectroscopic and slit-jaw imaging observations as well as images taken in the extreme-ultraviolet channels of AIA, and line-of-sight magnetic-field data from HMI onboard the SDO. We also employ an NLFFF relaxation approach based on the HMI magnetogram time series. We identify a strong small-scale brightening as a micro-flare in a CBP. The mini-eruption manifests with the ejection of hot (CBP loops) and cool (mini-filament) plasma recorded in both the imaging and spectroscopic data. The micro-flare is preceded by the appearance of an elongated bright feature in the IRIS slit-jaw 1400 A images located above the polarity inversion line. The micro-flare starts with an IRIS pixel size brightening and propagates bi-directionally along the elongated feature. We detect in both the spectral and imaging IRIS data and AIA data, strong flows along and at the edges of the elongated feature which we believe represent reconnection outflows. Both edges of the elongated feature that wrap around the edges of the erupting MF evolve into a J-type shape creating a sigmoid appearance. A quasi-separatrix layer (QSL) is identified in the vicinity of the polarity inversion line by computing the squashing factor Q in different horizontal planes of the NLFFF model. The QSL reconnection site has the same spectral appearance as the so-called explosive events identified by strong blue- and red-shifted emission, thus answering a long outstanding question about the true nature of this spectral phenomenon.
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References in corpus (12)
- Torus instability
- Generalized Squashing Factors for Covariant Description of Magnetic Connectivity in the Solar Corona
- Photospheric flux cancellation and associated flux rope formation and eruption
- Formation of current sheets and sigmoidal structure by the kink instability of a magnetic loop
- Observational Evidence for Gentle Chromospheric Evaporation During the Impulsive Phase of a Solar Flare
- Flux Rope Formation Preceding Coronal Mass Ejection Onset
- Quiet Sun mini-CMEs activated by supergranular flows
- Modeling the Dispersal of an Active Region: Quantifying Energy Input into the Corona
- Explosive events on sub-arcsecond scale in IRIS observations: a case study
- Formation and eruption of a flux rope from the sigmoid active region NOAA 11719 and associated M6.5 flare: A multi-wavelength study
- Eruptions from Quiet Sun Coronal Bright Points. II. Non-Potential Modeling
- A coronal wave and an asymmetric eruptive filament in SUMER, CDS, EIT, and TRACE co-observations
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- Explosive Events in the Quiet Sun Near and Beyond the Solar Limb Observed with the Interface Region Imaging Spectrograph (IRIS)
- Thermodynamic properties of small flares in the quiet Sun observed by H and EUV: plasma motion of the chromosphere and time evolution of temperature/emission measure
- Spectral Characteristics of a Rotating Solar Prominence in Multiple Wavelengths