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Radial Propagation Velocity Of Energetic Particle Injectionsaccording To Measurements Onboardrnthe Cluster Satellites

机译:高能粒子注入的径向传播速度根据星团卫星的测量

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Injections of energetic electrons with a dispersion over energies were observed during the February 23, 2004 (at about 03:20 UT) substorm onboard the Cluster satellites in the vicinity of perigee near the midnight meridian. The delays in the particle observation caused by the energy dependence of the magnetic drift velocities made it possible to determine the position and time of the beginning of the drift, tracing the trajectories of the leading center of particles back in time in the magnetospheric model. The comparisons of the measurements of four satellites allowed us to determine the radial propagation of the injection front with a velocity of 100-150 km/s at a distance of 7-9 R_E. The comparison with a few previous measurements shows a substantial slowing down of injections as they approached the Earth, and this confirms the prospects of this method for more detailed study of propagation of plasma injection into the inner magnetosphere.
机译:在2004年2月23日(约UT 03:20 UT)亚暴期间,在午夜子午线附近近地点附近的星团卫星上观察到注入了能量分散的高能电子。由磁漂移速度的能量依赖性引起的粒子观测中的延迟使得确定漂移开始的位置和时间成为可能,从而在磁层模型中追溯粒子的前导中心的轨迹。通过对四颗卫星的测量结果进行比较,我们可以确定以7-9 R_E的距离以100-150 km / s的速度注入前锋的径向传播。与之前的一些测量结果的比较表明,随着注入接近地球,注入的速度大大降低,这证实了该方法用于更详细研究等离子体注入内部磁层的传播的前景。

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