scholarly journals Observations of whistler mode waves with nonlinear parallel electric fields near the dayside magnetic reconnection separatrix by the Magnetospheric Multiscale mission

2016 ◽  
Vol 43 (12) ◽  
pp. 5909-5917 ◽  
Author(s):  
F. D. Wilder ◽  
R. E. Ergun ◽  
K. A. Goodrich ◽  
M. V. Goldman ◽  
D. L. Newman ◽  
...  
2004 ◽  
Vol 21 (7) ◽  
pp. 1306-1309 ◽  
Author(s):  
Guo Jun ◽  
Lu Quan-Ming ◽  
Wang Shui ◽  
Wang Yu-Ming ◽  
Dou Xian-Kang

2019 ◽  
Vol 46 (17-18) ◽  
pp. 10295-10302 ◽  
Author(s):  
W. M. Macek ◽  
M. V. D. Silveira ◽  
D. G. Sibeck ◽  
B. L. Giles ◽  
J. L. Burch

2018 ◽  
Vol 45 (17) ◽  
pp. 8783-8792 ◽  
Author(s):  
J. E. Stawarz ◽  
J. P. Eastwood ◽  
K. J. Genestreti ◽  
R. Nakamura ◽  
R. E. Ergun ◽  
...  

2013 ◽  
Vol 52 (1) ◽  
pp. 205-210 ◽  
Author(s):  
X.H. Wei ◽  
J.B. Cao ◽  
G.C. Zhou ◽  
H.S. Fu ◽  
O. Santolík ◽  
...  

2021 ◽  
Vol 922 (2) ◽  
pp. 96
Author(s):  
S. Y. Tang ◽  
Y. C. Zhang ◽  
L. Dai ◽  
T. Chen ◽  
C. Wang

Abstract In this paper, we investigate the structure of out-of-plane magnetic field in the reconnection event observed by Magnetospheric Multiscale Mission at the magnetopause of the Earth magnetosphere on 2015 October 21. We find that the perturbation of out-of-plane magnetic field in this event is different from previous observations of the quadrupolar Hall magnetic field. The distinct out-of-plane magnetic field is interpreted as a part of the hexapolar Hall magnetic field obtained in a recent simulation of asymmetric reconnection with the guide field. This is significant evidence of hexapolar Hall magnetic field in collisionless magnetic reconnection from the observations in the magnetosphere. High-resolution measurements of particle and field are used to provide a comprehensive description of the features of the hexapolar Hall magnetic field. The results from this study offer an insight into the Hall effect in collisionless magnetic reconnection.


2021 ◽  
Vol 922 (1) ◽  
pp. 56
Author(s):  
K. Jiang ◽  
S. Y. Huang ◽  
H. S. Fu ◽  
Z. G. Yuan ◽  
X. H. Deng ◽  
...  

Abstract Electron heating/acceleration in the foreshock, by which electrons may be energized beyond thermal energies prior to encountering the bow shock, is very important for the bow shock dynamics. And then these electrons would be more easily injected into a process like diffusive shock acceleration. Many mechanisms have been proposed to explain electrons heating/acceleration in the foreshock. Magnetic reconnection is one possible candidate. Taking advantage of the Magnetospheric Multiscale mission, we present two magnetic reconnection events in the dawnside and duskside ion foreshock region, respectively. Super-Alfvénic electron outflow, demagnetization of the electrons and the ions, and crescent electron distributions in the plane perpendicular to the magnetic field are observed in the sub-ion-scale current sheets. Moreover, strong energy conversion from the fields to the plasmas and significant electron temperature enhancement are observed. Our observations provide direct evidence that magnetic reconnection could occur in the foreshock region and heat/accelerate the electrons therein.


Sign in / Sign up

Export Citation Format

Share Document