Solar eruptions are explosive disruption of coronal magnetic fields, and often launch coronal
mass ejections into the interplanetary space. Intriguingly, many solar eruptions fail to escape …

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 …

Solar eruptions are outbursts of magnetized plasma in the atmosphere of the Sun,
encompassing phenomena like solar flares, ejective prominences and coronal mass …

Context. Coronal mass ejections (CMEs) stand as intense eruptions of magnetized plasma
from the Sun, and they play a pivotal role in driving significant changes of the heliospheric …

Transient and time-harmonic waves are analysed for a new class of elongated chiral multi-
structures subjected to gravity. The governing equations of motion incorporate a gyroscopic …

Prominences are important features in the solar atmosphere. Their activities often develop
into solar eruptions, such as flares and/or coronal mass ejections. We report here on …

Geomagnetic storms (GSs) are major disturbances in the terrestrial atmosphere caused by
the reconnection process between the incoming plasma ejecta in the solar wind and the …

Through independent research by the Chinese scientists or their international
collaborations, great achievements have been made in interplanetary physics research in …

Solar eruptions often show the rotation of filaments, which is a manifestation of the rotation of
erupting magnetic flux rope (MFR). Such a rotation of MFR can be induced by either the …