From fundamental theory to realistic modeling of the birth of solar eruptions
C Jiang - Science China Earth Sciences, 2024 - Springer
Solar eruptions, primarily manifested as solar flares, filament eruptions and coronal mass
ejections, represent explosive releases of magnetic energy stored in the solar corona, with …
ejections, represent explosive releases of magnetic energy stored in the solar corona, with …
Developments of a fundamental mechanism for initiation of solar eruptions
Solar eruptions are outbursts of magnetized plasma in the atmosphere of the Sun,
encompassing phenomena like solar flares, ejective prominences and coronal mass …
encompassing phenomena like solar flares, ejective prominences and coronal mass …
Fast Downflows Observed during a Polar Crown Filament Eruption
Solar filaments can undergo eruptions that result in the formation of coronal mass ejections,
which can significantly impact planetary space environments. Observations of eruptions …
which can significantly impact planetary space environments. Observations of eruptions …
Imaging and spectroscopic observations of a confined solar filament eruption with two-stage evolution
Z Xu, X Yan, L Yang, Z Xue, J Wang… - Monthly Notices of the …, 2024 - academic.oup.com
Solar filament eruptions are often characterized by stepwise evolution due to the
involvement of multiple mechanisms, such as magnetohydrodynamic instabilities and …
involvement of multiple mechanisms, such as magnetohydrodynamic instabilities and …
A model of solar magnetic flux rope eruption initiated primarily by magnetic reconnection
Q Liu, C Jiang, X Bian, X Feng, P Zuo… - Monthly Notices of the …, 2024 - academic.oup.com
There is a heated debate regarding the specific roles played by ideal magnetohydrodynamic
(MHD) instability and magnetic reconnection in triggering solar eruptions. In the context of a …
(MHD) instability and magnetic reconnection in triggering solar eruptions. In the context of a …
Data-driven Modeling of a Coronal Magnetic Flux Rope: from Birth to Death
Magnetic flux ropes are a bundle of twisted magnetic field lines produced by internal electric
currents, which are responsible for solar eruptions and are the major drivers of geomagnetic …
currents, which are responsible for solar eruptions and are the major drivers of geomagnetic …
Failure of a solar filament eruption caused by magnetic reconnection with overlying coronal loops
The failure of a filament eruption caused by magnetic reconnection between the erupting
filament and the overlying magnetic field has been previously proposed in numerical …
filament and the overlying magnetic field has been previously proposed in numerical …
Stealth Non-standard-model Confined Flare Eruptions: Sudden Reconnection Events in Ostensibly Inert Magnetic Arches from Sunspots
We report seven examples of a long-ignored type of confined solar flare eruption that does
not fit the standard model for confined flare eruptions. Because they are confined eruptions …
not fit the standard model for confined flare eruptions. Because they are confined eruptions …
Association Between a Failed Prominence Eruption and the Drainage of Mass from Another Prominence
J Xue, L Feng, H Li, P Zhang, J Chen, G Shi, K Ji, Y Qiu… - Solar Physics, 2024 - Springer
Sympathetic eruptions of solar prominences have been studied for decades, however, it is
usually difficult to identify their causal links. Here, we present two failed prominence …
usually difficult to identify their causal links. Here, we present two failed prominence …
Why Could a Newborn Active Region Produce Coronal Mass Ejections?
H Yang, L Liu - The Astrophysical Journal, 2024 - iopscience.iop.org
Solar active regions (ARs) are the main sources of flares and coronal mass ejections
(CMEs). NOAA AR 12089, which emerged on 2014 June 10, produced two C-class flares …
(CMEs). NOAA AR 12089, which emerged on 2014 June 10, produced two C-class flares …