Observations of a Quickly Flapping Interplanetary Magnetic Reconnection Exhaust
On the basis of the Petschek reconnection model and the characteristics of reconnection, hundreds of reconnection exhausts were reported in the solar wind. Many multi-spacecraft observations also indicated that interplanetary magnetic reconnection is a quasi–steady-state plasma process and the recon...
Main Authors: | Jiemin Wang, Yan Zhao |
---|---|
Format: | Article |
Language: | English |
Published: |
Frontiers Media S.A.
2021-09-01
|
Series: | Frontiers in Physics |
Subjects: | |
Online Access: | https://www.frontiersin.org/articles/10.3389/fphy.2021.736319/full |
Similar Items
-
Observations of a Quickly Flapping Interplanetary Magnetic Reconnection Exhaust
by: Wang, J., et al.
Published: (2021) -
Statistical Study of Small-Scale Interplanetary Magnetic Flux Ropes in the Vicinity of the Heliospheric Current Sheet
by: Liu, Q., et al.
Published: (2021) -
Observations of Magnetic Flux Ropes Opened or Disconnected From the Sun by Magnetic Reconnection in Interplanetary Space
by: Hengqiang Feng, et al.
Published: (2021-05-01) -
Coalescence of Magnetic Flux Ropes Within Interplanetary Coronal Mass Ejections: Multi-cases Studies
by: Yan Zhao, et al.
Published: (2019-10-01) -
Onset of Fast Magnetic Reconnection via Subcritical Bifurcation
by: ZHIBIN eGUO
Published: (2015-04-01)