scholarly journals Magnetospheric Multiscale Observations of the Off-equatorial Dipolarization Front Dynamics in the Terrestrial Magnetotail

2020 ◽  
Vol 899 (2) ◽  
pp. 125
Author(s):  
Huimin Li ◽  
Congkuan Zhu ◽  
Lixin Guo ◽  
Qi Cheng ◽  
O. Le Contel
2019 ◽  
Vol 124 (9) ◽  
pp. 7533-7542 ◽  
Author(s):  
Dong Lin ◽  
Wayne A. Scales ◽  
Gurudas Ganguli ◽  
Xiangrong Fu ◽  
Chris Crabtree ◽  
...  

2020 ◽  
Author(s):  
Rumi Nakamura ◽  
Wolfgang Baumjohann ◽  
Joachim Birn ◽  
Jim Burch ◽  
Chris Carr ◽  
...  

<p>We report the evolution of the current sheet associated with a localized flow burst in the near-Earth magnetotail on Sep. 8, 2018 around 14 UT when MMS (Magnetospheric Multiscale) and Cluster at about X=17 RE, separated mainly in the dawn-dusk direction at a distance of about 4 RE, encountered at duskside and dawnside part of a dipolarization front, respectively.  We analyzed the mesoscale current sheet disturbances based on multi-point data analysis between Cluster and MMS. It is shown that the current sheet thickens associated with the passage of the dipolarization front confirming results from previous statistical studies. The thickness of the current sheet, however, decreased subsequently, before recovering toward the original configuration. MMS observed enhanced field aligned currents exclusively during this thinning of the current sheet at the off-equatorial region. Multiple layers of small-scale, intense field-aligned currents accompanied by enhanced Hall-currents were detected at this region.  Based on these mesoscale and microscale multipoint observations, we infer the current structures around the localized flow and discuss the role of these mesoscale flow processes in the larger-scale magnetotail dynamics.</p><p> </p><p> </p>


2012 ◽  
Vol 694 ◽  
pp. 399-407 ◽  
Author(s):  
Yulii D. Shikhmurzaev ◽  
James E. Sprittles

AbstractA new approach to the modelling of wetting fronts in porous media on the Darcy scale is developed, based on considering the types (modes) of motion the menisci go through on the pore scale. This approach is illustrated using a simple model case of imbibition of a viscous incompressible liquid into an isotropic porous matrix with two modes of motion for the menisci, the wetting mode and the threshold mode. The latter makes it necessary to introduce an essentially new technique of conjugate problems that allows one to link threshold phenomena on the pore scale with the motion on the Darcy scale. The developed approach (a) makes room for incorporating the actual physics of wetting on the pore scale, (b) brings in the physics associated with pore-scale thresholds, which determine when sections of the wetting front will be brought to a halt (pinned), and, importantly, (c) provides a regular framework for constructing models of increasing complexity.


2002 ◽  
Vol 65 (2) ◽  
Author(s):  
A. Antonov ◽  
M. Gaidarov ◽  
M. Ivanov ◽  
D. Kadrev ◽  
G. Krumova ◽  
...  

2004 ◽  
Vol 70 (5) ◽  
Author(s):  
Bradley Marts ◽  
Karl Martinez ◽  
Anna L. Lin

2011 ◽  
Vol 116 (A5) ◽  
Author(s):  
K. Sakaguchi ◽  
K. Shiokawa ◽  
E. Donovan ◽  
A. Nakajima ◽  
Y. Hiraki ◽  
...  
Keyword(s):  

2019 ◽  
Author(s):  
Hiroshi Hasegawa ◽  
Takuma Nakamura ◽  
Daniel J Gershman ◽  
Yasuhiro Nariyuki ◽  
Viñas Adolfo ◽  
...  

2021 ◽  
Author(s):  
Soboh Alqeeq ◽  
Olivier Le Contel ◽  
Patrick Canu ◽  
Alessandro Retino ◽  
Thomas Chust ◽  
...  

<p>In the present work, we consider four dipolarization front (DF) events detected by MMS spacecraft in the Earth’s magnetotail during a substorm on 23rd of July 2017 between 16:05 and 17:19 UT. From their ion scale properties, we show that these four DF events embedded in fast Earthward plasma flows have classical signatures with increases of Bz, velocity and temperature and a decrease of density across the DF. We compute and compare current densities obtained from magnetic and particle measurements and analyse the Ohm’s law. Then we describe the wave activity related to these DFs. We investigate energy conversion processes via J.E calculations and estimate the importance of the electromagnetic energy flow by computing the divergence of the Poynting vector. Finally we discuss the electromagnetic energy conservation in the context of these DFs.</p>


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