极光千米辐射通过等离子体边界的低密度通道传输

Pub Date : 2024-03-26 DOI:10.12737/stp-101202403
V. Kolpak, Michael Mogilevsky, D. Chugunin, Aleksandr Chernyshov, I. Moiseenko
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引用次数: 0

摘要

我们介绍了对ERG(Arase)卫星质点附近极光千米辐射(AKR)的测量结果。卫星轨道的远地点位于黄道面附近,纬度为±30°。根据普遍接受的观点,在这一区域不可能观测到 AKR,因为它受到质球的屏蔽。通过同时测量 AKR 和当地等离子体密度,可以确定近赤道地区的 AKR 发生在等离子体通道中--沿磁场线拉长的密度不均匀性。来自极光磁层的 AKR 通过这些通道转移到赤道地区。这项研究分析了 AKR 在低等离子体密度通道中捕获和传播的条件。在几何光学近似条件下,我们模拟了辐射捕获和传播的条件。计算结果表明,所提出的将 AKR 捕获到等离子体通道的方案可以解释测量结果--从极光区到近赤道区的辐射传输。
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Transfer of auroral kilometric radiation through low-density channels at the boundary of plasmasphere
We present the results of Auroral Kilometric Radiation (AKR) measurements near the plasmapause on the ERG (Arase) satellite. The apogee of the satellite's orbit is located near the ecliptic plane, at latitudes ±30°. According to the generally accepted point of view, AKR observation is impossible in this region since it is shielded by the plasmasphere. Simultaneous measurements of AKR and local plasma density made it possible to determine that AKR in near-equatorial regions occur in plasma channels — density inhomogeneities elongated along magnetic field lines. AKR from sources located in the auroral magnetosphere is transferred by these channels to the equatorial region. This work analyzes the conditions for the capture and propagation of AKR in low plasma density channels. In the geometrical optics approximation, we have simulated the conditions for the radiation capture and propagation. The calculation results show that the proposed scheme for AKR capture into plasma channels can explain the measurement results — the radiation transfer from the auroral region to the near-equatorial region.
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