Characteristics of Electron Pitch-angle Distribution in the Flapping Magnetotail

The configuration, local motions, and related physics processes of the terrestrial magnetotail have been well studied, playing a key role in magnetotail dynamics. But characteristics of electron pitch-angle distribution (PAD), and the formation mechanisms, at different regions in the flapping magnetotail were not pointed out. Here, we study a current sheet crossing event detected by the Magnetospheric Multiscale Mission inside a magnetotail, and investigate the electron PAD of the event in detail. When the spacecraft are out of the current sheet, low-energy and high-energy electrons present field-aligned PAD and cigar-type PAD, respectively. This difference shows different motions of electrons. We proposed two possible explanation mechanisms: crossing a newly dipolarized magnetotail, or crossing the exhaust region of the reconnection region, and we discussed them in the paper adequately. Based on the dipolarized mechanism, for the first time, we point out that bouncing electrons could be the indicator of a newly dipolarized magnetotail. In addition, four other current sheet crossing cases with similar signatures are observed. Our study improves the understanding of current sheet dynamics and magnetotail configuration physics.

[1]  Z. Wang,et al.  Electron Thermalization and Electrostatic Turbulence Caused by Flow Reversal in Dipolarizing Flux Tubes , 2022, The Astrophysical Journal.

[2]  J. Cao,et al.  Formation of Rolling‐Pin Distribution of Suprathermal Electrons Behind Dipolarization Fronts , 2022, Journal of Geophysical Research: Space Physics.

[3]  C. Norgren,et al.  Electron‐Scale Measurements of Antidipolarization Front , 2021, Geophysical Research Letters.

[4]  C. Russell,et al.  Magnetotail reconnection onset caused by electron kinetics with a strong external driver , 2020, Nature Communications.

[5]  Z. Wang,et al.  A New Theory for Energetic Electron Generation Behind Dipolarization Front , 2020, Geophysical Research Letters.

[6]  V. Angelopoulos,et al.  Near-Earth Magnetotail Reconnection Powers Space Storms , 2019, Nature physics.

[7]  E. Grigorenko,et al.  Magnetotail dipolarization fronts and particle acceleration: A review , 2019, Science China Earth Sciences.

[8]  Y. Liu,et al.  Parallel Electron Heating by Tangential Discontinuity in the Turbulent Magnetosheath , 2019, The Astrophysical Journal.

[9]  A. Vaivads,et al.  Super-efficient Electron Acceleration by an Isolated Magnetic Reconnection , 2019, The Astrophysical Journal.

[10]  J P Eastwood,et al.  Electron-scale dynamics of the diffusion region during symmetric magnetic reconnection in space , 2018, Science.

[11]  C. Norgren,et al.  Formation of dipolarization fronts after current sheet thinning , 2018, Physics of Plasmas.

[12]  D. Delcourt,et al.  On the response of quasi-adiabatic particles to magnetotail reconfigurations , 2017 .

[13]  U. Gliese,et al.  Fast Plasma Investigation for Magnetospheric Multiscale , 2016 .

[14]  Thomas E. Moore,et al.  Magnetospheric Multiscale Overview and Science Objectives , 2016 .

[15]  Wolfgang Baumjohann,et al.  The Magnetospheric Multiscale Magnetometers , 2016 .

[16]  Wolfgang Baumjohann,et al.  The FIELDS Instrument Suite on MMS: Scientific Objectives, Measurements, and Data Products , 2016 .

[17]  P. Pritchett,et al.  The kinetic ballooning/interchange instability as a source of dipolarization fronts and auroral streamers , 2014 .

[18]  V. Angelopoulos,et al.  Electromagnetic Energy Conversion at Reconnection Fronts , 2013, Science.

[19]  A. Vaivads,et al.  Energetic electron acceleration by unsteady magnetic reconnection , 2013, Nature Physics.

[20]  V. Angelopoulos,et al.  On the current sheets surrounding dipolarizing flux bundles in the magnetotail: The case for wedgelets , 2013 .

[21]  A. Vaivads,et al.  Pitch angle distribution of suprathermal electrons behind dipolarization fronts: A statistical overview , 2012 .

[22]  A. Vaivads,et al.  Electron acceleration in the reconnection diffusion region: Cluster observations , 2012 .

[23]  A. Vaivads,et al.  Fermi and betatron acceleration of suprathermal electrons behind dipolarization fronts , 2011 .

[24]  C. Russell,et al.  Flux transport, dipolarization, and current sheet evolution during a double-onset substorm , 2011 .

[25]  M. W. Dunlop,et al.  Geomagnetic signatures of current wedge produced by fast flows in a plasma sheet , 2010 .

[26]  V. Angelopoulos,et al.  Accelerated ions ahead of earthward propagating dipolarization fronts , 2010 .

[27]  Wolfgang Baumjohann,et al.  Evolution of dipolarization in the near-Earth current sheet induced by Earthward rapid flux transport , 2009 .

[28]  I. J. Rae,et al.  Tail Reconnection Triggering Substorm Onset , 2008, Science.

[29]  R. Nakamura,et al.  Joint observations by Cluster satellites of bursty bulk flows in the magnetotail , 2006 .

[30]  J. Huba Hall magnetic reconnection: Guide field dependence , 2005 .

[31]  J. Birn,et al.  Thin current sheets and loss of equilibrium: Three‐dimensional theory and simulations , 2004 .

[32]  K. Glassmeier,et al.  Motion of the dipolarization front during a flow burst event observed by Cluster , 2002 .

[33]  P. Pritchett,et al.  does ion tearing exist , 1991 .

[34]  J. Eastwood Consistency of fields and particle motion in the ‘Speiser’ model of the current sheet , 1972 .

[35]  Robert L. McPherron,et al.  SUBSTORM RELATED CHANGES IN THE GEOMAGNETIC TAIL: THE GROWTH PHASE. , 1972 .