Mozer F S, Bale S D, Phan T D
Space Sciences Laboratory, University of California, Berkeley, California 94720, USA.
Phys Rev Lett. 2002 Jul 1;89(1):015002. doi: 10.1103/PhysRevLett.89.015002. Epub 2002 Jun 12.
On 1 April 2001, the Polar satellite crossed a subsolar magnetopause associated with antiparallel magnetic fields. Over a width approximately 6 magnetosheath ion skin depths (approximately 3 magnetospheric ion skin depths), perpendicular ion flows different from E x B/B(2) as well as Hall magnetic and electric field signatures were observed. At a smaller scale, the electron flow decoupled from the magnetic field near a deep minimum in the magnetic field strength. Separatrices were identified as boundaries of low frequency electric field turbulence associated with density minima and parallel electric fields. The reconnection rate was less than 2% of the asymptotic Alfvén speed.
2001年4月1日,极地卫星穿过了与反平行磁场相关的次太阳磁层顶。在大约6个磁鞘离子趋肤深度(约3个磁层离子趋肤深度)的宽度范围内,观测到了不同于E×B/B²的垂直离子流以及霍尔磁场和电场特征。在较小尺度上,电子流在磁场强度的一个深度最小值附近与磁场解耦。分界面被确定为与密度最小值和平行电场相关的低频电场湍流的边界。重联率小于渐近阿尔文速度的2%。