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Temperature anisotropy, instabilities, and thermal processes in low-β plasma

Shaikh, Zubair I; Verscharen, Daniel; Vasko, Ivan Y; Maruca, Bennett A; (2025) Temperature anisotropy, instabilities, and thermal processes in low-β plasma. Astronomy & Astrophysics 10.1051/0004-6361/202555506. (In press). Green open access

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Abstract

Interplanetary coronal mass ejections (ICMEs) are large-scale magnetic structures that influence heliospheric dynamics and space weather. While wave activity has been observed within their low-β (≪ 1) magnetic obstacles, the role of temperature anisotropy and instability remains underexplored. This study examines proton temperature anisotropies, heating, cooling, turbulence, and collisional effects within ICME magnetic obstacles, which are low-β plasmas. Using Wind spacecraft data from 382 ICME magnetic obstacles at 1 au (spanning 1995–2021), we observe that proton temperature and proton β_p follow log-normal distributions. The anisotropy within these regions is primarily constrained to the stable parameter regime below the thresholds for the mirror-mode and oblique firehose instabilities. Additionally, plasmas unstable to proton cyclotron and firehose instabilities exhibit temperatures that are significantly higher -- 50 to 100 times higher than those of stable plasma. Notably, enhanced magnetic fluctuations and low collisional age are observed near instability thresholds, regardless of beta. Although a clear relationship exists between temperature and collisional age, the correlation between turbulent amplitude and collisional age is weak, differing from trends observed in the solar wind. Our results suggest a causal chain whereby high turbulence amplitudes are associated with enhanced heating, linked to reduced collisions, causing increased temperature anisotropy, and ultimately favouring the development of instabilities within ICME magnetic obstacles.

Type: Article
Title: Temperature anisotropy, instabilities, and thermal processes in low-β plasma
Open access status: An open access version is available from UCL Discovery
DOI: 10.1051/0004-6361/202555506
Publisher version: https://doi.org/10.1051/0004-6361/202555506
Language: English
Additional information: This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions.
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery.ucl.ac.uk/id/eprint/10218429
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