Please use this identifier to cite or link to this item: https://dspace.iiti.ac.in/handle/123456789/15409
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dc.contributor.authorPaul, Arghyadeepen_US
dc.contributor.authorNandy, Sirshaen_US
dc.contributor.authorVaidya, Bhargav Pradeepen_US
dc.date.accessioned2025-01-15T07:10:31Z-
dc.date.available2025-01-15T07:10:31Z-
dc.date.issued2020-
dc.identifier.citationPaul, A., Nandy, S., & Vaidya, B. (2020). Plasmoid Dominated Magnetic Reconnection and Particle Acceleration. Proceedings of the International Astronomical Union, 16(S362), 410–416. https://doi.org/10.1017/S1743921322001272en_US
dc.identifier.issn1743-9213-
dc.identifier.otherEID(2-s2.0-85146967591)-
dc.identifier.urihttps://doi.org/10.1017/S1743921322001272-
dc.identifier.urihttps://dspace.iiti.ac.in/handle/123456789/15409-
dc.description.abstractThe effect of a parallel velocity shear on the explosive phase of magnetic reconnection in a double tearing mode is investigated within the 2D resistive magneto-hydrodynamic framework. All the systems follow a three phase evolution pattern with the phases delayed in time for an increasing shear speed. We find that the theoretical dependence of the reconnection rate with shear remains true in more general scenarios such as that of a plasmoid dominated double current sheet system. We also find that the power-law distribution of plasmoid sizes become steeper with an increasing sub-Alfvénic shear. We further demonstrate the effect of a velocity shear on acceleration of test particles pertaining to the modification in the energy spectrum. © The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union.en_US
dc.language.isoenen_US
dc.publisherCambridge University Pressen_US
dc.sourceProceedings of the International Astronomical Unionen_US
dc.subjectDouble Tearing Modeen_US
dc.subjectExplosive reconnectionen_US
dc.subjectParticle accelerationen_US
dc.subjectPlasmoidsen_US
dc.titlePlasmoid Dominated Magnetic Reconnection and Particle Accelerationen_US
dc.typeConference Paperen_US
Appears in Collections:Department of Astronomy, Astrophysics and Space Engineering

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