Kelvin–Helmholtz Waves on the Magnetopause at the Lunar Distances under Southward IMF: ARTEMIS Observations
The Kelvin–Helmholtz (KH) instability, a common phenomenon widely observed at the magnetopause, plays an important role in plasma transport while reconnection at low latitude is less efficient during the northward interplanetary magnetic field (IMF). In this study, we analyze the magnetic field and...
Main Authors: | Lu, J. (Author), Wang, M. (Author), Zhou, Y. (Author) |
---|---|
Format: | Article |
Language: | English |
Published: |
MDPI
2022
|
Subjects: | |
Online Access: | View Fulltext in Publisher |
Similar Items
-
Compiling Magnetosheath Statistical Data Sets Under Specific Solar Wind Conditions: Lessons Learnt From the Dayside Kinetic Southward IMF GEM Challenge
by: A. P. Dimmock, et al.
Published: (2020-06-01) -
TEC Variations Over Korean Peninsula During Magnetic Storm
by: E.-Y. Ji, et al.
Published: (2008-03-01) -
The financial benefits of the IMF
by: Age F. P. Bakker, et al.
Published: (2000-09-01) -
The Kelvin-Helmholtz instability on the Kronian magnetopause
by: Cutler, Jack
Published: (2014) -
IMF İSTİKRAR PROGRAMLARININ TEMEL ESASLARI ve REFORM GEREKSİNİMİ
by: M. Okan TAŞAR
Published: (2009-12-01)