activity
20172022
most citedThe First 3D Coronal Loop Model Heated by MHD Waves against Radiative Losses

44 citations · 110 across the 8 of their papers we have counts for

collaborators

11 papers

astro-ph.SR20228 cited

Three-Dimensional Propagation of Kink Wave Trains in Solar Coronal Slabs

Bo Li, Mingzhe Guo, Hui Yu +2

Impulsively excited wave trains are of considerable interest in solar coronal seismology. To our knowledge, however, it remains to examine the three-dimensional (3D) dispersive pro…

astro-ph.SR20225 cited

Oblique Quasi-Kink Modes in Solar Coronal Slabs Embedded in an Asymmetric Magnetic Environment: Resonant Damping, Phase and Group Diagrams

Shao-Xia Chen, Bo Li, Mingzhe Guo +2

There has been considerable interest in magnetoacoustic waves in static, straight, field-aligned, one-dimensional equilibria where the exteriors of a magnetic slab are different be…

astro-ph.SR20224 cited

Influence of fine structures on gyrosynchrotron emission of flare loops modulated by sausage modes

Mijie Shi, Bo Li, Mingzhe Guo

Sausage modes are one leading mechanism for interpreting short period quasi-periodic pulsations (QPPs) of solar flares. Forward modeling their radio emission is crucial for identif…

physics.space-ph2021

Observations of an Electron-cold Ion Component Reconnection at the Edge of an Ion-scale Antiparallel Reconnection at the Dayside Magnetopause

S. Q. Zhao, H. Zhang, Terry Z. Liu +11

Solar wind parameters play a dominant role in reconnection rate, which controls the solar wind-magnetosphere coupling efficiency at Earth's magnetopause. Besides, low-energy ions f…

astro-ph.SR202144 cited

The First 3D Coronal Loop Model Heated by MHD Waves against Radiative Losses

Mijie Shi, Tom Van Doorsselaere, Mingzhe Guo +3

In the quest to solve the long-standing coronal heating problem, it has been suggested half a century ago that coronal loops could be heated by waves. Despite the accumulating obse…

astro-ph.SR201910 cited

Transition region loops in the very late phase of flux-emergence in IRIS sit-and-stare observations

Zhenghua Huang, Bo Li, Lidong Xia +3

Loops are one of the fundamental structures that trace the geometry of the magnetic field in the solar atmosphere. Their evolution and dynamics provide a crucial proxy for studying…