Advanced methods for analyzing in-situ observations of magnetic reconnection
H. Hasegawa, M. R. Argall, N. Aunai, R. Bandyopadhyay, N. Bessho, I., J. Cohen, R. E. Denton, J. C. Dorelli, J. Egedal, S. A. Fuselier, P. Garnier,, V. Genot, D. B. Graham, K. J. Hwang, Y. V. Khotyaintsev, D. B. Korovinskiy,, B. Lavraud, Q. Lenouvel, T. C. Li, Y.-H. Liu

TL;DR
This paper reviews advanced techniques for analyzing in-situ spacecraft data to better understand magnetic reconnection, emphasizing recent multi-spacecraft methods enabled by the Magnetospheric Multiscale mission.
Contribution
It provides an overview of innovative data analysis methods for magnetic reconnection, highlighting recent advances with multi-spacecraft measurements at electron scales.
Findings
Enhanced detection of diffusion regions in reconnection
Improved visualization of plasma and field interactions
Identification of electron-scale reconnection processes
Abstract
There is ample evidence for magnetic reconnection in the solar system, but it is a nontrivial task to visualize, to determine the proper approaches and frames to study, and in turn to elucidate the physical processes at work in reconnection regions from in-situ measurements of plasma particles and electromagnetic fields. Here an overview is given of a variety of single- and multi-spacecraft data analysis techniques that are key to revealing the context of in-situ observations of magnetic reconnection in space and for detecting and analyzing the diffusion regions where ions and/or electrons are demagnetized. We focus on recent advances in the era of the Magnetospheric Multiscale mission, which has made electron-scale, multi-point measurements of magnetic reconnection in and around Earth's magnetosphere.
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Taxonomy
TopicsGeomagnetism and Paleomagnetism Studies · Ionosphere and magnetosphere dynamics · Solar and Space Plasma Dynamics
