Observational and Theoretical Study of Lower Hybrid Drift Waves

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dc.contributor.author Arya, Neetasha
dc.contributor.author Kakad, Amar
dc.date.accessioned 2024-04-23T05:56:42Z
dc.date.available 2024-04-23T05:56:42Z
dc.date.issued 2024
dc.identifier.citation EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-7061, https://doi.org/10.5194/egusphere-egu24-7061, 2024. en_US
dc.identifier.uri http://library.iigm.res.in:8080/xmlui/handle/123456789/2008
dc.description.abstract One of the most important diamagnetic current driven instability transverse to the magnetic field is lower hybrid drift instability (LHDI) which excites lower hybrid drift waves (LHDW). LHDI gives rise to anomalous resistivity which further leads to onset of magnetic reconnection. Because of its high anomalous collision frequency, LHDI enhances the rate of transverse diffusion. The lower hybrid frequency (LHF) ranges between electron and ion cyclotron frequency which is a natural resonance. LHDW is generally observed in transition layer regions and magnetic reconnection sites, where the gradient in density occurs. We are presenting electromagnetic kinetic model including gradients in density and magnetic field, finite parallel wavenumber and non-thermal particle distribution function or kappa velocity distribution function. The effect of the aforementioned factors on the growth rate of LHDI in different plasma beta circumstances has been thoroughly investigated and will be discussed. Space observation of drift driven wave using MMS spacecraft will also be discussed. en_US
dc.language.iso other en_US
dc.subject Lower Hybrid Drift Waves en_US
dc.subject Observational studies en_US
dc.subject Theoretical studies en_US
dc.title Observational and Theoretical Study of Lower Hybrid Drift Waves en_US
dc.type Presentation en_US


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