Magnetosheath Jet-Triggered ULF Waves: Energy Deposition in the Ionosphere

IF 2.6 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
E. Krämer, M. Hamrin, H. Gunell, L. Baddeley, N. Partamies, S. Raptis, K. Herlingshaw, A. Schillings
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Abstract

Magnetosheath jets, transient plasma structures of enhanced dynamic pressure, have been observed to trigger ultra-low frequency (ULF) waves in the magnetosphere. These ULF waves contribute to energy transport in the magnetosphere-ionosphere system. Therefore, there is a need to estimate the energy input into the ionosphere due to jet-triggered ULF waves. In this study, we combine measurements from Magnetospheric Multiscale, ground-based magnetometers, the EISCAT radar on Svalbard, and SuperDARN to estimate the Joule heating in the ionosphere resulting from jet impacts at the magnetopause. Focusing on three jets observed on 2016-01-07 we were able to calculate the Joule heating for two jets. We found an average Joule heating rate of 0.38 $0.38$ mW/m2 which is on par with other processes such as field line resonances. However, due to the short duration and spatial confinement of the jet-induced ULF waves, the average energy input was only 9 1 0 10 $9\cdot 1{0}^{10}$ J. This suggests that the energy deposition of jet-triggered ULF waves is small compared to other magnetospheric processes, and thus does not significantly impact the average energy budget of the magnetosphere.

Abstract Image

磁鞘射流触发的超高频波:电离层中的能量沉积
磁鞘射流是一种动态压力增强的瞬态等离子体结构,已被观察到在磁层中触发超低频(ULF)波。这些极低频波有助于磁层-电离层系统中的能量传输。因此,有必要估计由于喷射触发的超高频波而输入电离层的能量。在这项研究中,我们结合了来自磁层多尺度、地面磁力计、斯瓦尔巴群岛上的EISCAT雷达和SuperDARN的测量结果,估计了磁层顶射流撞击引起的电离层焦耳加热。以2016年1月7日观测到的三个射流为重点,我们能够计算出两个射流的焦耳热。我们发现平均焦耳加热速率为0.38$ 0.38$ mW/m2,与其他过程(如场线共振)相当。然而,由于射流诱导的超低频波持续时间短且空间受限,平均能量输入仅为9⋅1 10 $9\cdot 1{0}^{10}$ J.这表明与其他磁层过程相比,射流触发的极低频波的能量沉积较小。因此不会显著影响磁层的平均能量收支。
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来源期刊
Journal of Geophysical Research: Space Physics
Journal of Geophysical Research: Space Physics Earth and Planetary Sciences-Geophysics
CiteScore
5.30
自引率
35.70%
发文量
570
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