Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/1241
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dc.contributor.authorZeković, Vladimiren_US
dc.date.accessioned2022-09-29T16:43:38Z-
dc.date.available2022-09-29T16:43:38Z-
dc.date.issued2019-03-01-
dc.identifier.issn1070664Xen
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/1241-
dc.description.abstractA case of two interpenetrating, cold and quasi-neutral ion-electron plasmas is investigated with the multi-fluid approach. We consider that one plasma flows quasi-parallel to the lines of a background magnetic field embedded in another static plasma. If the flow turns super-Alfvénic, we show that parallel R/L-modes and perpendicular X/O-modes become unstable and grow in amplitude. Within the linear theory, we find that the growth rate curve of an unstable mode has a maximum at some wavenumber specific to each mode. If we consider a shock-like plasma configuration, we find that the fastest growing mode is the resonant one (with k ∼ r gi - 1) which strongly interacts with ions. In Particle-In-Cell (PIC) simulations, we observe that a resonant wave with the same properties is excited during the early phases of shock formation. Once the wave becomes non-linear, it efficiently scatters ions and triggers the initial shock formation. This implies that the typical compression ratio of ∼4 could naturally arise as a consequence of a highly resonant micro-physical process. We model the interaction of ions reflected from the reforming shock barrier in a weak-beam case, and we show that the upstream wave now matches the instability we expect from the equations. By using PIC simulations, we explain how the strong-beam resonant instability triggers shock formation in the non-linear stage, and how the weak-beam instability reforms and transmits the shock afterwards. The micro-instabilities that we study here could largely contribute to shock triggering as well as to the reformation and transmission of the shock itself.en
dc.relation.ispartofPhysics of Plasmasen
dc.titleResonant micro-instabilities at quasi-parallel collisionless shocks: Cause or consequence of shock (re)formationen_US
dc.typeArticleen_US
dc.identifier.doi10.1063/1.5050909-
dc.identifier.scopus2-s2.0-85062837343-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/85062837343-
dc.contributor.affiliationAstronomyen_US
dc.relation.volume26en
dc.relation.issue3en
item.fulltextNo Fulltext-
item.openairetypeArticle-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0002-4985-3253-
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