Reduced fluid-kinetic equations for low-frequency dynamics, magnetic reconnection, and electron heating in low-beta plasmas
A minimal model for magnetic reconnection and, generally, low-frequency dynamics in low-beta plasmas is proposed. The model combines analytical and computational simplicity with physical realizability: it is a rigorous limit of gyrokinetics for plasma beta of order the electron-ion mass ratio. The m...
| Main Authors: | , |
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| Format: | Journal article |
| Sprog: | English |
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2011
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| _version_ | 1826274973778444288 |
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| author | Zocco, A Schekochihin, A |
| author_facet | Zocco, A Schekochihin, A |
| author_sort | Zocco, A |
| collection | OXFORD |
| description | A minimal model for magnetic reconnection and, generally, low-frequency dynamics in low-beta plasmas is proposed. The model combines analytical and computational simplicity with physical realizability: it is a rigorous limit of gyrokinetics for plasma beta of order the electron-ion mass ratio. The model contains collisions and can be used both in the collisional and collisionless reconnection regimes. It includes gyrokinetic ions (not assumed cold) and allows for the topological rearrangement of the magnetic field lines by either resistivity or electron inertia, whichever predominates. The two-fluid dynamics are coupled to electron kinetics-electrons are not assumed isothermal and are described by a reduced drift-kinetic equation. The model, therefore allows for irreversibility and conversion of magnetic energy into electron heat via parallel phase mixing in velocity space. An analysis of the exchanges between various forms of free energy and its conversion into electron heat is provided. It is shown how all relevant linear waves and regimes of the tearing instability (collisionless, semicollisional, and fully resistive) are recovered in various limits of our model. An efficient way to simulate our equations numerically is proposed, via the Hermite representation of the velocity space. It is shown that small scales in velocity space will form, giving rise to a shallow Hermite-space spectrum, whence it is inferred that, for steady-state or sufficiently slow dynamics, the electron heating rate will remain finite in the limit of vanishing collisionality. © 2011 American Institute of Physics. |
| first_indexed | 2024-03-06T22:51:38Z |
| format | Journal article |
| id | oxford-uuid:5efbc0ee-b83b-458c-bb37-a9e9e72d0acd |
| institution | University of Oxford |
| language | English |
| last_indexed | 2024-03-06T22:51:38Z |
| publishDate | 2011 |
| record_format | dspace |
| spelling | oxford-uuid:5efbc0ee-b83b-458c-bb37-a9e9e72d0acd2022-03-26T17:44:04ZReduced fluid-kinetic equations for low-frequency dynamics, magnetic reconnection, and electron heating in low-beta plasmasJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:5efbc0ee-b83b-458c-bb37-a9e9e72d0acdEnglishSymplectic Elements at Oxford2011Zocco, ASchekochihin, AA minimal model for magnetic reconnection and, generally, low-frequency dynamics in low-beta plasmas is proposed. The model combines analytical and computational simplicity with physical realizability: it is a rigorous limit of gyrokinetics for plasma beta of order the electron-ion mass ratio. The model contains collisions and can be used both in the collisional and collisionless reconnection regimes. It includes gyrokinetic ions (not assumed cold) and allows for the topological rearrangement of the magnetic field lines by either resistivity or electron inertia, whichever predominates. The two-fluid dynamics are coupled to electron kinetics-electrons are not assumed isothermal and are described by a reduced drift-kinetic equation. The model, therefore allows for irreversibility and conversion of magnetic energy into electron heat via parallel phase mixing in velocity space. An analysis of the exchanges between various forms of free energy and its conversion into electron heat is provided. It is shown how all relevant linear waves and regimes of the tearing instability (collisionless, semicollisional, and fully resistive) are recovered in various limits of our model. An efficient way to simulate our equations numerically is proposed, via the Hermite representation of the velocity space. It is shown that small scales in velocity space will form, giving rise to a shallow Hermite-space spectrum, whence it is inferred that, for steady-state or sufficiently slow dynamics, the electron heating rate will remain finite in the limit of vanishing collisionality. © 2011 American Institute of Physics. |
| spellingShingle | Zocco, A Schekochihin, A Reduced fluid-kinetic equations for low-frequency dynamics, magnetic reconnection, and electron heating in low-beta plasmas |
| title | Reduced fluid-kinetic equations for low-frequency dynamics, magnetic reconnection, and electron heating in low-beta plasmas |
| title_full | Reduced fluid-kinetic equations for low-frequency dynamics, magnetic reconnection, and electron heating in low-beta plasmas |
| title_fullStr | Reduced fluid-kinetic equations for low-frequency dynamics, magnetic reconnection, and electron heating in low-beta plasmas |
| title_full_unstemmed | Reduced fluid-kinetic equations for low-frequency dynamics, magnetic reconnection, and electron heating in low-beta plasmas |
| title_short | Reduced fluid-kinetic equations for low-frequency dynamics, magnetic reconnection, and electron heating in low-beta plasmas |
| title_sort | reduced fluid kinetic equations for low frequency dynamics magnetic reconnection and electron heating in low beta plasmas |
| work_keys_str_mv | AT zoccoa reducedfluidkineticequationsforlowfrequencydynamicsmagneticreconnectionandelectronheatinginlowbetaplasmas AT schekochihina reducedfluidkineticequationsforlowfrequencydynamicsmagneticreconnectionandelectronheatinginlowbetaplasmas |