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A flapping wave was observed by THEMIS-B (P1) and THEMIS-C (P2) probes on the dawn side of the magnetotail, while the solar wind was generally stable. The magnetic activity was quite weak, suggesting that this flapping wave was generated by an internal instability, which normally occurs during magnetic quiet times. Our analysis shows that the flapping wave was propagating downward with a tail-aligned...
The motion and deceleration processes of plasma sheet high-speed flows have great significance to magnetospheric particle acceleration, magnetic field perturbation, magnetic flux transport, triggering of substorm, and the current system formation in the magnetotail. From February to April 2009, two satellites of the Time History of Events and Macroscale Interactions during Substorms mission, THA and...
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