Coronal mass ejections (CMEs) play an important role in space weather. The propagation
characteristics of CMEs in the Corona and interplanetary space determine whether, when …

Using in situ measurements from the Parker Solar Probe and Wind spacecraft, we
investigate the small-scale magnetic flux ropes (SFRs) and their properties inside stream …

The origination and generation mechanisms of small magnetic flux ropes (SMFRs), which
are important structures in solar wind, are not clearly known. In the present study, 1993 …

In this study, we probe the turbulence characteristic within the small-scale magnetic flux
ropes (SSMFRs) close to the Sun using Parker Solar Probe (PSP) magnetic field data. The …

The small-scale interplanetary magnetic flux ropes (SIMFRs) are common magnetic
structures in the interplanetary space, yet their origination is still an open question. In this …

During solar eruptions, many closed magnetic flux ropes are ejected into interplanetary
space, which contribute to the heliospheric magnetic field and have important space …

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

The solar wind is a plasma constantly blowing out from the Sun with a large-scale magnetic
field having significant local complexity at small scales. Small-scale magnetic flux ropes …

Interplanetary coronal mass ejections (ICMEs) are massive magnetized plasma clouds
originating from the Sun. They are the interplanetary counterparts of coronal mass ejections …