Plasma structuring within an expanded polar cap and cusp studied with the SS-520-3 sounding rocket.

IF 2.5 3区 地球科学
Earth, Planets and Space Pub Date : 2025-01-01 Epub Date: 2025-05-26 DOI:10.1186/s40623-025-02189-7
L M Buschmann, K Asamura, L B N Clausen, Y Jin, H Kojima, A Kumamoto, S Kurita, Y Ogawa, K Oksavik, Y Saito, A Spicher, S Yokota, W J Miloch
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引用次数: 0

Abstract

Abstract: The SS-520-3 sounding rocket was launched on November 4th, 2021 as part of the Grand Challenge Initiative - Cusp from Ny-Ålesund, Svalbard. The rocket was launched into the cusp ionosphere during the main phase of a geomagnetic storm. In this study we utilize two low energy particle analyzers as well as a multi-needle Langmuir probe and an impedance probe as part of the rocket payload. This study aims to provide an overview of the flight conditions from a range of ground-based instruments and scintillation receivers. We were able to confirm that the rocket entered the cusp through the poleward edge at around 74 of northern geographic latitude. Additionally, the rocket encountered polar cap patches (PCP), as well as a patch within the cusp (CP) and a newly-formed tongue of ionisation (TOI). Analysis of the density variations within different scale sizes show enhancements within meter-size and kilometer-size scales on the edges of PCP, within the CP and TOI. Overall, the enhancements within the variations on all sizes, as well as enhancements of the electron density were significantly higher within the CP and TOI in comparison to the PCP, though all structures were encountered at similar altitudes. The strongest enhancements were found on the poleward edge of the TOI, corresponding to strong fluctuations within the electron density. The TOI also had the largest enhancements within gradients of kilometer-size in comparison to meter-sizes. As the TOI is convecting with respect to the background plasma, the edges are susceptible to instabilities like the Kelvin-Helmholtz instability (KHI) and Gradient-Drift instability (GDI), giving rise to plasma density structures on several scale sizes.

Graphical abstract:

用SS-520-3探空火箭研究了扩展极帽和尖端内的等离子体结构。
摘要:SS-520-3探空火箭于2021年11月4日在斯瓦尔巴群岛Ny-Ålesund发射,作为“大挑战计划”的一部分。这枚火箭是在地磁风暴的主要阶段发射到电离层尖端的。在这项研究中,我们利用两个低能粒子分析仪以及一个多针朗缪尔探针和一个阻抗探针作为火箭有效载荷的一部分。本研究旨在从一系列地面仪器和闪烁接收器提供飞行条件的概述。我们能够确认,火箭是从北纬74度左右的极缘进入尖端的。此外,火箭还遇到了极帽斑块(PCP),以及尖端(CP)内的斑块和新形成的电离舌(TOI)。不同尺度的密度变化分析表明,在PCP边缘、CP和TOI范围内,米尺度和公里尺度的密度变化都有所增强。总体而言,尽管所有结构都在相似的高度上遇到,但与PCP相比,所有尺寸变化中的增强以及CP和TOI中的电子密度增强都明显更高。在TOI的极向边缘发现了最强的增强,对应于电子密度的强烈波动。与米级相比,印度时报在公里级梯度内也有最大的增强。由于TOI相对于背景等离子体是对流的,边缘容易受到像开尔文-亥姆霍兹不稳定性(KHI)和梯度漂移不稳定性(GDI)这样的不稳定性的影响,从而产生了几个尺度上的等离子体密度结构。图形化的简介:
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Earth, Planets and Space
Earth, Planets and Space 地学天文-地球科学综合
CiteScore
5.80
自引率
16.70%
发文量
167
期刊介绍: Earth, Planets and Space (EPS) covers scientific articles in Earth and Planetary Sciences, particularly geomagnetism, aeronomy, space science, seismology, volcanology, geodesy, and planetary science. EPS also welcomes articles in new and interdisciplinary subjects, including instrumentations. Only new and original contents will be accepted for publication.
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