scholarly journals Characteristics of Minor Ions and Electrons in Flux Transfer Events Observed by the Magnetospheric Multiscale Mission

Author(s):  
S. M. Petrinec ◽  
J. L. Burch ◽  
M. Chandler ◽  
C. J. Farrugia ◽  
S. A. Fuselier ◽  
...  
2020 ◽  
Author(s):  
Steven Petrinec ◽  
James Burch ◽  
Michael Chandler ◽  
Charlie Farrugia ◽  
Stephen Fuselier ◽  
...  

<p>Several dayside magnetosheath flux transfer events (FTEs) have been observed at high temporal resolution by the four-spacecraft MMS mission. In this study, we examine ion energy spectrograms, ion moments, and ion distribution functions for several long duration magnetosheath FTEs observed by MMS. For these cases, the spacecraft were positioned at similar locations (i.e., south of the equatorial plane, post-noon local time sector). The ion observations are placed in context with electron energy spectrograms parallel and anti-parallel to the observed magnetic field and the location of MMS relative to the predicted reconnection line location as determined from convected solar wind conditions. This combined set of observations provide important information on the formation, topologies, and evolution of FTEs.</p>


2021 ◽  
Author(s):  
Wei-Jie Sun ◽  
James Slavin ◽  
Rumi Nakamura ◽  
Daniel Heyner ◽  
Johannes Mieth

<p>BepiColombo is a joint mission of the European Space Agency (ESA) and the Japan Aerospace Exploration Agency (JAXA) to the planet Mercury. The BepiColombo mission consists of two spacecraft, which are the Mercury Planetary Orbiter (MPO) and Mercury Magnetospheric Orbiter (Mio). The mission made its first planetary flyby, which is the only Earth flyby, on 10 April 2020, during which several instruments collected measurements. In this study, we analyze MPO magnetometer (MAG) observations of Flux Transfer Events (FTEs) in the magnetosheath and the structure of the subsolar magnetopause near the  flow stagnation point. The magnetosheath plasma beta was high with a value of ~ 8 and the interplanetary magnetic field (IMF) was southward with a clock angle that decreased from ~ 100 degrees to ~ 150 degrees.  As the draped IMF became increasingly southward several of the flux transfer event (FTE)-type flux ropes were observed. These FTEs traveled southward indicating that the magnetopause X-line was located northward of the spacecraft, which is consistent with a dawnward tilt of the IMF. Most of the FTE-type flux ropes were in ion-scale, <10 s duration, suggesting that they were newly formed. Only one large-scale FTE-type flux rope, ~ 20 s, was observed. It was made up of two successive bipolar signatures in the normal magnetic field component, which is evidence of coalescence at a secondary reconnection site. Further analysis demonstrated that the dimensionless reconnection rate of the re-reconnection associated with the coalescence site was ~ 0.14. While this investigation was limited to the MPO MAG observations, it strongly supports a key feature of dayside reconnection discovered in the Magnetospheric Multiscale mission, the growth of FTE-type flux ropes through coalescence at secondary reconnection sites.</p>


2020 ◽  
Vol 125 (10) ◽  
Author(s):  
M. V. D. Silveira ◽  
D. G. Sibeck ◽  
S. H. Lee ◽  
D. Koga ◽  
V. M. Souza ◽  
...  

2016 ◽  
Vol 43 (12) ◽  
pp. 6070-6077 ◽  
Author(s):  
C. J. Farrugia ◽  
B. Lavraud ◽  
R. B. Torbert ◽  
M. Argall ◽  
I. Kacem ◽  
...  

2019 ◽  
Vol 46 (8) ◽  
pp. 4106-4113 ◽  
Author(s):  
C. Chen ◽  
T. R. Sun ◽  
C. Wang ◽  
Z. H. Huang ◽  
B. B. Tang ◽  
...  

1984 ◽  
Vol 11 (2) ◽  
pp. 131-134 ◽  
Author(s):  
M. A. Saunders ◽  
C. T. Russell ◽  
N. Sckopke

1985 ◽  
Vol 90 (A5) ◽  
pp. 4069 ◽  
Author(s):  
C. K. Goertz ◽  
E. Nielsen ◽  
A. Korth ◽  
K. H. Glassmeier ◽  
C. Haldoupis ◽  
...  

2017 ◽  
Vol 44 (21) ◽  
Author(s):  
Roger P. Leyser ◽  
Suzanne M. Imber ◽  
Stephen E. Milan ◽  
James A. Slavin

1982 ◽  
Vol 87 (A4) ◽  
pp. 2159 ◽  
Author(s):  
G. Paschmann ◽  
G. Haerendel ◽  
I. Papamastorakis ◽  
N. Sckopke ◽  
S. J. Bame ◽  
...  

2017 ◽  
Vol 44 (12) ◽  
pp. 5951-5959 ◽  
Author(s):  
X.-C. Dong ◽  
M. W. Dunlop ◽  
K. J. Trattner ◽  
T. D. Phan ◽  
H.-S. Fu ◽  
...  

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