Panov Evgeny V, Lu San, Pritchett Philip L
Space Research Institute Austrian Academy of Sciences Graz Austria.
Institute of Physics University of Graz Graz Austria.
Geophys Res Lett. 2022 Feb 16;49(3):e2021GL096796. doi: 10.1029/2021GL096796. Epub 2022 Feb 8.
By combining three-probe THEMIS observations and 3-D Particle-in-Cell simulations, we identify key structures on the ion gyroradius scale that occur in connection with ballooning-interchange instability heads in the Earth's magnetotail. The mesoscale structures occur at sites of strong ion velocity shear and vorticity where the thermal ion Larmor radius is about half of the width of the head. Finer structures occur at the smaller scales characterizing the wavelength of the electromagnetic ion cyclotron waves generated at the heads. These two processes act to erode and thin the current sheet, thereby forming a local magnetotail configuration that is favorable for reconnection.
通过结合三探针THEMIS观测数据和三维粒子模拟,我们识别出了与地球磁尾中气球交换不稳定性头部相关的离子回旋半径尺度上的关键结构。这些中尺度结构出现在强离子速度剪切和涡度区域,此处热离子拉莫尔半径约为头部宽度的一半。更精细的结构出现在更小尺度上,这些尺度表征了在头部产生的电磁离子回旋波的波长。这两个过程会侵蚀并使电流片变薄,从而形成有利于重联的局部磁尾构型。