2022年7月11日由射流相关的受限耀斑引起的日冕环横向振荡

IF 2.4 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Musheng Lin, Ya Wang, Liheng Yang, Jie Chen, Wenwei Pan, Shuyue Li, Qingmin Zhang
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引用次数: 0

摘要

在这篇文章中,我们报告了2022年7月11日在NOAA 13056活跃区由射流相关的受限耀斑引起的两个环状链横向振荡的多波长和多视角观测。射流起源于靠近环的右足点,并向东北方向传播。射流的平均上升时间约为11分钟,平均下降时间约为13.5分钟,射流的寿命约为24.5分钟。射流的上升运动分为两个阶段,平均速度为≈164和≈546 km s−1。射流的下落运动是相干的,平均速度约为124 km s−1。环的横向振荡,持续3 - 5个周期,是基本的常设扭结模式。两股的最大初始振幅分别为≈5.8和≈4.9 Mm,平均周期分别为≈405 s和≈407 s。在振荡过程中,两条链都经历缓慢的膨胀。loop_1和loop_2的扭结速度下限分别为\(895_{-17}^{+21}\) km s−1和\(891_{-35}^{+29}\) km s−1。相应的alfv速度下限估计为\(664_{-13}^{+16}\) km s−1和\(661_{-26}^{+22}\) km s−1。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Transverse Oscillations of Coronal Loops Induced by a Jet-Related Confined Flare on 11 July 2022

In this article, we report the multiwavelength and multiview observations of transverse oscillations of two loop strands induced by a jet-related, confined flare in active region NOAA 13056 on 11 July 2022. The jet originates close to the right footpoint of the loops and propagates in the northeast direction. The average rise time and fall time of the jet are ≈ 11 and ≈ 13.5 minutes, so that the lifetime of the jet reaches ≈ 24.5 minutes. The rising motion of the jet is divided into two phases with average velocities of ≈ 164 and ≈ 546 km s−1. The falling motion of the jet is coherent with an average velocity of ≈ 124 km s−1. The transverse oscillations of the loops, lasting for 3 – 5 cycles, are of fundamental standing kink mode. The maximal initial amplitudes of the two strands are ≈ 5.8 and ≈ 4.9 Mm. The average periods are ≈ 405 s and ≈ 407 s. Both of the strands experience slow expansions during oscillations. The lower limits of the kink speed are \(895_{-17}^{+21}\) km s−1 for loop_1 and \(891_{-35}^{+29}\) km s−1 for loop_2, respectively. The corresponding lower limits of the Alfvén speed are estimated to be \(664_{-13}^{+16}\) km s−1 and \(661_{-26}^{+22}\) km s−1.

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来源期刊
Solar Physics
Solar Physics 地学天文-天文与天体物理
CiteScore
5.10
自引率
17.90%
发文量
146
审稿时长
1 months
期刊介绍: Solar Physics was founded in 1967 and is the principal journal for the publication of the results of fundamental research on the Sun. The journal treats all aspects of solar physics, ranging from the internal structure of the Sun and its evolution to the outer corona and solar wind in interplanetary space. Papers on solar-terrestrial physics and on stellar research are also published when their results have a direct bearing on our understanding of the Sun.
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