On the electron agyrotropy during rapid asymmetric magnetic island coalescence in presence of a guide field

We present an analysis of the properties of the electron velocity distribution during island coalescence in asymmetric reconnection with and without guide field. In a previous study, three main domains were identified, in the case without guide field, as X, D, and M regions featuring different reconnection evolutions. These regions are also identified here in the case with guide field. We study the departure from isotropic and gyrotropic behavior by means of different robust detection algorithms proposed in the literature. While in the case without guide field these metrics show an overall agreement, when the guide field is present, a discrepancy in the agyrotropy within some relevant regions is observed, such as at the separatrices and inside magnetic islands. Moreover, in light of the new observations from the Multiscale MagnetoSpheric mission, an analysis of the electron velocity phase-space in these domains is presented.

[1]  S. Markidis,et al.  Separatrices: The crux of reconnection , 2014, Journal of Plasma Physics.

[2]  P. Pritchett Kinetic properties of magnetic merging in the coalescence process , 2007 .

[3]  J. Birn,et al.  On the electron diffusion region in asymmetric reconnection with a guide magnetic field , 2016 .

[4]  P. Cassak,et al.  Asymmetric Magnetic Reconnection: General Theory and Collisional Simulations , 2007 .

[5]  Michael Hesse,et al.  Electron nongyrotropy in the context of collisionless magnetic reconnection , 2013 .

[6]  Stefano Markidis,et al.  Progress towards physics-based space weather forecasting with exascale computing , 2017, Adv. Eng. Softw..

[7]  William Daughton,et al.  ''Illuminating'' electron diffusion regions of collisionless magnetic reconnection using electron agyrotropy , 2008 .

[8]  M. Shay,et al.  Electron acceleration from contracting magnetic islands during reconnection , 2006, Nature.

[9]  F. Mozer,et al.  Asymmetric magnetic reconnection in the presence of a guide field , 2009 .

[10]  M. Shay,et al.  Diamagnetic suppression of component magnetic reconnection at the magnetopause , 2003, physics/0305021.

[11]  F. Coroniti,et al.  Tearing at the dayside magnetopause , 1981 .

[12]  Stefano Markidis,et al.  Scales of guide field reconnection at the hydrogen mass ratio , 2010 .

[13]  S. Markidis,et al.  On the electron dynamics during island coalescence in asymmetric magnetic reconnection , 2015, 1511.05693.

[14]  G. Lapenta,et al.  What Can We Learn about Magnetotail Reconnection from 2D PIC Harris-Sheet Simulations? , 2016 .

[15]  M. Fujimoto,et al.  ELECTRON ACCELERATION BY MULTI-ISLAND COALESCENCE , 2010, 1004.1154.

[16]  P. Cassak,et al.  Reconnection at Earth’s Dayside Magnetopause , 2016 .

[17]  M. Hesse,et al.  Electron energization and structure of the diffusion region during asymmetric reconnection , 2016 .

[18]  M. Swisdak,et al.  Quantifying gyrotropy in magnetic reconnection , 2015, 1509.00787.

[19]  P. Pritchett Collisionless magnetic reconnection in an asymmetric current sheet , 2008 .

[20]  G. Lapenta,et al.  Reconnection Separatrix: Simulations and Spacecraft Measurements , 2016 .

[21]  Stefano Markidis,et al.  Multi-scale simulations of plasma with iPIC3D , 2010, Math. Comput. Simul..

[22]  J. B. Blake,et al.  Electron-scale measurements of magnetic reconnection in space , 2016, Science.

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