Abstract:Generation and propagation of lower hybrid drift wave (LHDW) near the electron diffusion region (EDR) during guide field reconnection at the magnetopause is studied with data from the Magnetospheric Multiscale mission and a theoretical model. Inside the current sheet, the electron beta (β e) determines which type of LHDW is excited. Inside the EDR, where the electron beta is high (β e ∼ 5), the long-wavelength electromagnetic LHDW is observed propagating obliquely to the local magnetic field. In contrast, the … Show more
“…To further corroborate our results, we make sure that the fluctuations that we have identified as the EF waves are not the electromagnetic lower hybrid mode, which has been reported in several studies investigating magnetic reconnection in the Earth's magnetotail and at the magnetopause (Chen et al., 2020; Cozzani et al., 2021; Wang et al., 2022; Yoo et al., 2020). This further check is motivated by the fact that the observations are complex and characterized by significant uncertainties.…”
Kinetic plasma instabilities driven by temperature anisotropies are known to play an essential role in collisionless plasma dynamics, scattering the particles and affecting particle heating and energy conversion between the electromagnetic fields and particles (e.g., Gary, 1993). Among these anisotropy-driven instabilities, the whistler anisotropy instability is excited by electron temperature anisotropy T e,‖ /T e,⊥ < 1 while the electron firehose instability (EFI) develops if T e,‖ /T e,⊥ > 1, where T e,‖ and T e,⊥ are the electron temperatures respectively parallel and perpendicular with respect to the background magnetic field. The EFI is believed to constrain the electron temperature anisotropy by inducing heating (cooling) in the perpendicular (parallel) direction with respect to the background magnetic field, thus leading to isotropization.The EFI was described for the first time by Hollweg and Völk (1970) and W. Pilipp and Völk (1971). Then, Gary and Madland (1985) provided the parametric dependencies of the growth rate of the EF modes with the assumption of parallel propagation, that is, the wave vector k is directed parallel to the background magnetic field. One-dimensional Particle-In-Cell (PIC) simulations further investigated the properties of the parallel propagating EF mode (
“…To further corroborate our results, we make sure that the fluctuations that we have identified as the EF waves are not the electromagnetic lower hybrid mode, which has been reported in several studies investigating magnetic reconnection in the Earth's magnetotail and at the magnetopause (Chen et al., 2020; Cozzani et al., 2021; Wang et al., 2022; Yoo et al., 2020). This further check is motivated by the fact that the observations are complex and characterized by significant uncertainties.…”
Kinetic plasma instabilities driven by temperature anisotropies are known to play an essential role in collisionless plasma dynamics, scattering the particles and affecting particle heating and energy conversion between the electromagnetic fields and particles (e.g., Gary, 1993). Among these anisotropy-driven instabilities, the whistler anisotropy instability is excited by electron temperature anisotropy T e,‖ /T e,⊥ < 1 while the electron firehose instability (EFI) develops if T e,‖ /T e,⊥ > 1, where T e,‖ and T e,⊥ are the electron temperatures respectively parallel and perpendicular with respect to the background magnetic field. The EFI is believed to constrain the electron temperature anisotropy by inducing heating (cooling) in the perpendicular (parallel) direction with respect to the background magnetic field, thus leading to isotropization.The EFI was described for the first time by Hollweg and Völk (1970) and W. Pilipp and Völk (1971). Then, Gary and Madland (1985) provided the parametric dependencies of the growth rate of the EF modes with the assumption of parallel propagation, that is, the wave vector k is directed parallel to the background magnetic field. One-dimensional Particle-In-Cell (PIC) simulations further investigated the properties of the parallel propagating EF mode (
“…In these two regions, LHW are commonly observed in the vicinity of magnetic reconnection sites where strong density gradients do form. Their role on the onset (or relaxation) of magnetic reconnection has been addressed in the past and still represents a key point in the context of reconnection research (Daughton 2003;Lapenta et al 2003Lapenta et al , 2018Yoo et al 2020).…”
Context. Density inhomogeneities are ubiquitous in space and astrophysical plasmas, particularly at contact boundaries between different media. They often correspond to regions that exhibit strong dynamics across a wide range of spatial and temporal scales. Indeed, density inhomogeneities are a source of free energy that can drive various instabilities such as the lower-hybrid-drift instability, which, in turn, transfers energy to the particles through wave-particle interactions and eventually heats the plasma.
Aims. Our study is aimed at quantifying the efficiency of the lower-hybrid-drift instability to accelerate or heat electrons parallel to the ambient magnetic field.
Methods. We combine two complementary methods: full-kinetic and quasilinear models.
Results. We report self-consistent evidence of electron acceleration driven by the development of the lower-hybrid-drift instability using 3D-3V full-kinetic numerical simulations. The efficiency of the observed acceleration cannot be explained by standard quasilinear theory. For this reason, we have developed an extended quasilinear model that is able to quantitatively predict the interaction between lower-hybrid fluctuations and electrons on long time scales, which is now in agreement with full-kinetic simulations results. Finally, we apply this new, extended quasilinear model to a specific inhomogeneous space plasma boundary, namely, the magnetopause of Mercury. Furthermore, we discuss our quantitative predictions of electron acceleration to support future BepiColombo observations.
“…The guide field can also reduce the reconnection rate, the electron nongyrotropic effects, and the thickness of the electron diffusion region (EDR; Yamada et al 2010). In addition, both asymmetries and the guide field have influence on the distributions and properties of plasma waves that play crucial roles in reconnection (Graham et al 2016(Graham et al , 2017Le et al 2018;Wilder et al 2019;Yoo et al 2020), such as whistler waves and lowerhybrid drift waves (LHDWs).…”
Section: Introductionmentioning
confidence: 99%
“…Besides, the LHDWs can be also induced by the modified two-stream instability (Graham et al 2017(Graham et al , 2019. The short-wavelength mode with k ⊥ ρ e ∼ 1 often develops at the current sheet boundary, while the longwavelength mode with k ⊥ (ρ i ρ e ) 0.5 ∼ 1 develops in the current sheet center (Norgren et al 2012;Yoo et al 2020;Wang et al 2022).…”
Utilizing high-resolution data from the Magnetospheric Multiscale mission, we present new observations of lower-hybrid drift waves (LHDWs) in terrestrial magnetotail reconnection with guide field levels of ∼70% and asymmetric plasma density (N
high/N
low ∼ 2.5). The LHDWs, driven by lower-hybrid drift instability, were observed in correlation with magnetic field and density gradients at separatrices on both sides of the reconnection current sheet. The properties of the LHDWs at both sides of the separatrices are different: (1) At high-density side separatrices, the LHDWs with wavelength kρ
e ∼ 0.41 propagated away from the X-line mainly in the L–M plane; (2) at the low-density side separatrices, the LHDWs with wavelengths kρ
e ∼ 0.76 and kρ
e ∼ 0.35 propagated mainly along the outflow direction and current sheet normal. It is also found that the perpendicular magnetic field fluctuations were comparable to the parallel component. Wave potential of the LHDWs was 20% ∼ 35% of the electron temperature. The LHDWs contributed to electron demagnetization and energy dissipation. Our study can promote understanding of properties of LHDWs during magnetic reconnection.
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