Solar jet-coronal hole collision and a related coronal mass ejection
arXiv:1602.06493 · doi:10.3847/2041-8205/819/2/L18
Abstract
Jets are defined as impulsive, well-collimated upflows, occurring in different layers of the solar atmosphere with different scales. Their relationship with coronal mass ejections (CMEs), another type of solar impulsive events, remains elusive. Using the high-quality imaging data of AIA/SDO, here we show a well-observed coronal jet event, in which part of the jets, with the embedding coronal loops, runs into a nearby coronal hole (CH) and gets bounced towards the opposite direction. This is evidenced by the flat-shape of the jet front during its interaction with the CH and the V-shaped feature in the time-slice plot of the interaction region. About a half-hour later, a CME initially with a narrow and jet-like front is observed by the LASCO C2 coronagraph, propagating along the direction of the post-collision jet. We also observe some 304 A dark material flowing from the jet-CH interaction region towards the CME. We thus suggest that the jet and the CME are physically connected, with the jet-CH collision and the large- scale magnetic topology of the CH being important to define the eventual propagating direction of this particular jet-CME eruption.
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Cited by in corpus (10)
- Observation and Modeling of Solar Jets
- On a solar blowout jet: driven mechanism and the formation of cool and hot components
- A New Tool for CME Arrival Time Prediction Using Machine Learning Algorithms: CAT-PUMA
- On the Magnetic and Energy Characteristics of Recurrent Homologous Jets from An Emerging Flux
- A Quasi-periodic propagating wave and EUV waves excited simultaneously in a solar eruption event
- The Birth of a Jet-driven Twin CME and Its Deflection from Remote Magnetic Fields
- Interaction of two filaments in a long filament channel associated with twin coronal mass ejections
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