Oscillatory Reconnection as a Plasma Diagnostic in the Solar Corona

Karampelas, Konstantinos, McLaughlin, James, Botha, Gert and Regnier, Stephane (2023) Oscillatory Reconnection as a Plasma Diagnostic in the Solar Corona. The Astrophysical Journal, 943 (2). p. 131. ISSN 0004-637X

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Official URL: https://doi.org/10.3847/1538-4357/acac90


Oscillatory reconnection is a relaxation process in magnetized plasma, with an inherent periodicity that is exclusively dependent on the properties of the background plasma. This study focuses on the seismological prospects of oscillatory reconnection in the solar corona. We perform three sets of parameter studies (for characteristic coronal values of the background magnetic field, density, and temperature) using the PLUTO code to solve the fully compressive, resistive MHD equations for a 2D magnetic X-point. From each parameter study, we derive the period of the oscillatory reconnection. We find that this period is inversely proportional to the characteristic strength of the background magnetic field and the square root of the initial plasma temperature, while following a square root dependency upon the equilibrium plasma density. These results reveal an inverse proportionality between the magnitude of the Alfvén speed and the period, as well as the background speed of sound and the period. Furthermore, we note that the addition of anisotropic thermal conduction only leads to a small increase in the mean value for the period. Finally, we establish an empirical formula that gives the value for the period in relation to the background magnetic field, density, and temperature. This gives us a quantified relation for oscillatory reconnection, to be used as a plasma diagnostic in the solar corona, opening up the possibility of using oscillatory reconnection for coronal seismology.

Item Type: Article
Additional Information: Funding information: All authors acknowledge the UK Science and Technology Facilities Council (STFC) for support from grant No. ST/T000384/1. K.K. also acknowledges the support of an FWO (Fonds voor Wetenschappelijk Onderzoek - Vlaanderen) postdoctoral fellowship (1273221N). This work used the Oswald High Performance Computing facility operated by Northumbria University (UK).
Uncontrolled Keywords: The Sun and the Heliosphere
Subjects: F300 Physics
Department: Faculties > Engineering and Environment > Mathematics, Physics and Electrical Engineering
Depositing User: Rachel Branson
Date Deposited: 03 Feb 2023 15:20
Last Modified: 07 Mar 2023 10:55
URI: https://nrl.northumbria.ac.uk/id/eprint/51314

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