Electron Dissipation and Electromagnetic Work

dc.contributor.authorYang, Yan
dc.contributor.authorAdhikari, Subash
dc.contributor.authorMatthaeus, William H.
dc.date.accessioned2025-01-07T20:42:08Z
dc.date.available2025-01-07T20:42:08Z
dc.date.issued2024-10-14
dc.descriptionThis article was originally published in JGR: Space Physics. The version of record is available at: https://doi.org/10.1029/2024JA033105. © 2024. American Geophysical Union. All Rights Reserved. This article will be embargoed until 04/14/2025.
dc.description.abstractWith the increase in technical capabilities of computer simulation in recent years, it has become feasible to quantify the degradation of fluid scale plasma and electromagnetic energies in favor of increases of internal energies. While it is understood that electromagnetic energy can be exchanged with fluid scale velocities, it is the pressure strain interaction that exchanges energy between fluid motions and internal energy. Here using simulations of both turbulence and reconnection we show that for electrons, the pressure strain and electromagnetic work are closely related and are frequently comparable when appropriate time and spatial averaging is applied. Otherwise, the instantaneous spatial averaged pressure strain and electromagnetic work are nearly equal for slowly evolving systems, like the reconnection case, while they differ significantly in rapidly evolving systems, like the turbulence case. This clarifies the relationship between these two quantities, which are each frequently used as measures of dissipation. Key Points - Time integrated volume averaged electromagnetic work does not formally or generally correspond to dissipation - Due to small electron mass, time integrated volume averaged pressure strain and electromagnetic work are nearly equal for electrons - Differences between instantaneous electromagnetic work and pressure strain can be considerable, but for electrons, these average to zero Plain Language Summary The electromagnetic field changes the fluid velocity of each type of plasma particle. Meanwhile, the pressure of each plasma species, interacts with nonuniform fluid velocities to produce heat. The intermediate steps are in general, complicated, but because electrons are so light, a special simplifying approximation holds, equating properly averaged electromagnetic work on electrons to the rate of increase of electron internal energy. This result may help clarify differences in how the reconnection and turbulence communities quantify “dissipation”.
dc.description.sponsorshipThis research is partially supported by the MMS Theory, Modeling and Data Analysis team under NASA Grant 80NSSC19K0565, by the NASA LWS program under grants 80NSSC20K0198 and 80NSSC22K1020, and a subcontract from the New Mexico consortium 655–001, a NASA Heliophysics MMS-GI grant through a Princeton subcontract SUB0000517, and by the National Science Foundation Solar Terrestrial Program grant AGS-2108834. This research was also supported by the International Space Science Institute (ISSI) in Bern, through ISSI International Team projects #556 (Cross-scale energy transfer in space plasmas) and #23-588 (“Unveiling energy conversion and dissipation in non-equilibrium space plasmas”). We would like to acknowledge high-performance computing support from Cheyenne (doi:10.5065/D6RX99HX) and Derecho (https://doi.org/10.5065/qx9a-pg09) provided by NCAR's Computational and Information Systems Laboratory, sponsored by the National Science Foundation. We are particularly grateful to Sylvie Yang Jin (金浠言) for cooperation and assisting the lead author in completing this research.
dc.identifier.citationYang, Y., Adhikari, S., & Matthaeus, W. H. (2024). Electron dissipation and electromagnetic work. Journal of Geophysical Research: Space Physics, 129, e2024JA033105. https://doi.org/10.1029/2024JA033105
dc.identifier.issn2169-9402
dc.identifier.urihttps://udspace.udel.edu/handle/19716/35699
dc.language.isoen_US
dc.publisherJGR: Space Physics
dc.subjectenergy dissipation
dc.subjectelectromagnetic work
dc.subjectpressure strain interaction
dc.subjectplasma turbulence
dc.subjectmagnetic reconnection
dc.titleElectron Dissipation and Electromagnetic Work
dc.typeArticle

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