REVIEW 4 major objections 6 minor 96 references
Electron scale magnetic holes generation driven by Whistler-to-Bernstein mode conversion in fully kinetic plasma turbulence
T0 review · 4 major / 6 minor · reviewed 2026-08-10 · deepseek-v4-flash
Pith's one-line read A turbulence-born chain of waves and vortices can create electron-scale magnetic holes.
desk verdict A plausible new turbulence-driven pathway to electron-scale magnetic holes, but the asserted whistler-to-Bernstein conversion needs a frequency-wavenumber check before the central claim is granted. read the letter →
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
The reading
What carries the argument
The load-bearing object is the whistler-to-Bernstein-like mode conversion: as the whistler propagates into regions where the background field tilts out of the plane, its propagation becomes quasi-perpendicular and a longitudinal electrostatic component with harmonic structure at multiples of kde = 0.81 appears. The authors interpret this through a nonlinear forced-wave expansion of the kinetic equations, in which the whistler acts as an antenna that drives higher harmonics whose character changes as the background plasma varies. The resulting Bernstein-like electrostatic field, combined with the ambient magnetic field through the E×B drift, sets up the space-alternating current filaments that merge into the vortex sustaining the magnetic hole.
What would settle it
Compute the dispersion relation of the longitudinal electrostatic fluctuations seen at t = 225–275 Ωe⁻¹ and check whether the frequency–wavenumber pairs, with k⊥ resolved, lie on the Bernstein dispersion branches at multiples of the electron cyclotron frequency. If the measured harmonics do not fall on a Bernstein branch, or if a control run with a uniform background field (no tilt past 45 degrees) still produces the same harmonic chain and current filaments, then the observed 'conversion' would be a nonlinear property of the whistler itself rather than a true change of mode identity.
Extended reading notes
Core claim
The central claim is that turbulence alone, without any electron-scale initial perturbation, can produce electron-scale magnetic holes. In the simulation the holes emerge from a chain beginning with turbulent velocity shear, which through the pressure tensor raises Te⊥/Te∥ locally; the resulting oblique whistler-cyclotron instability radiates waves at kde ~ 0.81; as those waves travel through the inhomogeneous field, the angle between propagation and B rises past roughly 45 degrees, longitudinal electric field fluctuations appear with harmonics at kde = 0.81, 1.62, 2.43, and near-linear polarization; these are identified as quasi-electrostatic Bernstein-like modes; the longitudinal electric field creates alternating E×B drift current filaments; two filaments merge into a larger electron ring-current vortex; and the vortex's diamagnetic current lowers |B| by about 30 percent over about 5de. The resulting structure hosts trapped high-pitch-angle electrons, higher Te⊥/Te∥, increased density, and a 'mushroom' electron velocity distribution, matching reported features of sub-ion-scale magnetic holes.
Load-bearing premise
The chain's pivotal step is the claim that the whistler actually converts into a Bernstein-like mode; the evidence is harmonic peaks in the longitudinal electric field and linear polarization, but the paper does not quantitatively rule out that the same harmonics could arise from nonlinear steepening of the whistler or from wave-particle effects, so the mode-conversion reading is the premise on which the title's causal chain rests.
Editorial extensions
If this is right
- Electron-scale magnetic holes in turbulent magnetosheath-like plasmas can be produced by the cascade itself, so their presence does not require pre-existing electron-scale seeds.
- The holes form as the final product of whistler waves, meaning wave-driven hole formation can complement the previously proposed electron Kelvin-Helmholtz route; the two mechanisms produce holes at different scales (about 5de versus about di).
- The same mechanism generates short-lived magnetic hump vortices that are later destroyed by turbulence, offering a possible counterpart to electron-scale magnetic peaks in observations.
- The mushroom-shaped electron velocity distribution inside the hole is a kinetic signature that could be sought in spacecraft particle data to identify turbulence-born holes.
- Because the simulation starts from large-scale fluctuations only, the mechanism demonstrates a concrete energy path from MHD scales to electron scales through wave conversion and vortex merging.
Reading between the lines
- If the conversion interpretation holds, the mechanism implies that the rate of electron-scale magnetic hole production in the magnetosheath should track the local whistler activity and the presence of large-scale velocity shears; a statistical test with spacecraft data correlating hole counts with whistler wave power and shear amplitude could verify this.
- The 2D geometry may exaggerate the vortex-merging stage; in 3D, out-of-plane wave propagation could change the mode conversion and the stability of the merged vortex, so the specific size scaling (about twice the driving wavelength) is a prediction that should be tested in 3D simulations.
- The same chain might operate in other turbulent space environments with similar electron beta and anisotropy conditions, such as the solar wind; the simulation's parameters are magnetosheath-like, so the solar-wind case is an open extrapolation.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper uses a 2D fully kinetic PIC simulation of freely decaying plasma turbulence (ECsim, 64 d_i box, magnetosheath-like parameters) to document one electron-scale magnetic hole at t = 500 Ω_e^{-1}. It proposes a five-step causal chain: large-scale turbulent velocity shears locally enhance electron temperature anisotropy; the plasma becomes unstable to the oblique whistler-cyclotron instability; the resulting whistlers convert into quasi-electrostatic Bernstein-like modes as they propagate through the inhomogeneous background; the electrostatic fluctuations drive filamentary E×B currents; and merging of the resulting electron vortices forms the magnetic hole. The fully developed hole is characterized through magnetic-field, density, temperature, current, pitch-angle, and electron velocity-distribution diagnostics, and the whistler step is checked against the DIS-K linear solver using parameters measured from the simulation.
Significance. If the proposed chain is correct, the paper provides a new, self-consistent turbulence-driven pathway for forming electron-scale magnetic holes, a process whose origin is currently debated, and it explicitly links whistler-to-Bernstein mode conversion to coherent-structure formation. Strengths include the use of a fully kinetic simulation with injection scales far above electron scales, an external linear-stability check with DIS-K using measured plasma parameters, step-by-step time tracing of the structure, and quantitative current-correlation statistics. The central weakness is that the key mode-conversion step rests on qualitative signatures; this is the main load-bearing point that needs to be hardened.
major comments (4)
- [3.3, Figure 6] The evidence for whistler-to-Bernstein mode conversion is not yet sufficient. The longitudinal electric field shows spatial harmonics at integer multiples of k d_e = 0.81, 1.62, 2.43, and the hodograms show near-linear polarization, but these signatures are also produced by nonlinear steepening of a whistler or by wave-particle trapping without any change of wave identity. The paper invokes the nonlinear expansion of Yu et al. (2021b) in the text but does not perform that expansion or any equivalent quantitative test, and it does not measure the frequencies of the harmonics. A direct frequency-wavenumber analysis (for example, temporal FFT along the same cuts) comparing the harmonic dispersion with the whistler and Bernstein branches would distinguish true mode conversion from harmonic generation; without this, the central claim in the title and abstract is not established.
- [3.4, Figure 8] The correlation between the observed normal electron current and the E×B drift current is moderate rather than strong: Pearson coefficients are 0.81, 0.58, and 0.70 at t = 225, 250, and 275 Ω_e^{-1}, with fitted slopes 1.37, 1.24, and 1.23, meaning that the drift explains at most R^2 ≈ 0.66 of the variance and underestimates the current amplitude by 23–37%. Moreover, the authors state that the correlation is absent in the merged-vortex region. Because the vortex chain is attributed to these drift currents, the paper should quantify the remaining current contributions (pressure-gradient drift, polarization current, inertial effects) and demonstrate that the mechanism still operates where vortex merging actually occurs.
- [3.2, Table 1] The DIS-K check is a useful external consistency test, but the linear-solver inputs are single-time, single-cut spatial averages taken in a strongly inhomogeneous turbulent background. The observed wavenumber and propagation angle could be selected by the background gradients rather than by the local linear instability. A sensitivity analysis varying A_e, β_∥e, and ω_pe/Ω_e within the measured ranges, together with a comparison of the predicted fastest-growing mode with the observed peak, would make the whistler-generation claim more robust.
- [3.1 and Conclusions] The full causal chain is demonstrated for a single magnetic hole in a single 2D simulation. The authors acknowledge the 2D limitation, but the broader claim that turbulence generates electron-scale MHs through this mechanism would be substantially strengthened by showing that the same sequence occurs for at least one additional independent structure in the same run, or by providing event statistics. As it stands, the paper is a detailed case study rather than a statistical demonstration of the mechanism.
minor comments (6)
- [Throughout] The notation for the local coordinate system alternates between 'LNz' and 'LNZ'; please use a single convention consistently.
- [1, Introduction] The phrase 'Kelvin-Helhomtz' should be corrected to 'Kelvin-Helmholtz'.
- [3.3, Figure 6 caption] The caption describes the white lines as 'harmonics of the frequency i.e. kde = 0.81, 1.62, 2.43', but these are wavenumbers rather than frequencies; please clarify the distinction.
- [2, Simulation Setup] The Gaussian-filter scale of 0.75 d_i is stated but not tested. Because all high-pass/low-pass quantities depend on this scale, a short robustness check (for instance, 0.5 or 1.0 d_i) would help show that the identified wave and vortex features are not filter artifacts.
- [3.3] The term 'quasi-electrostatic' is used without a quantitative definition. Reporting, for example, the ratio of longitudinal electric to magnetic fluctuation energy or δE·B/|δE||B| would make the electrostatic character of the Bernstein-like mode testable.
- [References] There appear to be duplicate or inconsistent entries for Arrò et al. 2024; please verify the reference list and unify the citation format.
Circularity Check
No significant circularity: the paper's causal chain is assembled from independent diagnostics and external linear-theory checks, not from fitting or self-defined quantities.
full rationale
The paper's five-step mechanism is supported by separate diagnostics, none of which is defined in terms of the conclusion. The whistler-wave identification uses the DIS-K linear solver (cited as López et al. 2021) with plasma parameters averaged from the simulation (Ae = 2.1, β∥e = 0.3, etc.), not fitted to the observed wave frequency, growth rate, or polarization; the predicted quantities are compared with simulation output as an external consistency check. The wavenumber kde = 0.81 is measured from the simulation's FFT, not imposed by the solver. The Bernstein-like stage is identified by harmonics at integer multiples of that measured wavenumber and by nearly linear polarization; although this identification is qualitative and alternative explanations (nonlinear steepening, wave-particle effects) are not quantitatively excluded, that is an evidentiary weakness rather than circularity. The vortex-formation step compares the simulated δJeN with the E×B drift current computed from the same measured fields; this is a diagnostic decomposition, not a fitted prediction. Self-citations (Arrò et al. 2023 for the simulation run; López et al. 2021 for DIS-K) are used as data and software provenance and do not carry the load-bearing argument; no uniqueness theorem or ansatz is imported from the authors' prior work. The paper explicitly acknowledges the 2D-geometry limitation and states it does not claim this is the only possible generation mechanism. No circular step can be exhibited from the text.
Assumptions & free parameters
free parameters (1)
- Gaussian filter scale =
0.75 d_i
assumptions (4)
- domain assumption Vlasov-Maxwell system solved by ECsim is a faithful model of collisionless magnetosheath plasma dynamics
- domain assumption The initial conditions (beta_i=8, beta_e=2, delta B/B0=0.9, delta u/cA=3.6) are representative of typical magnetosheath conditions
- domain assumption The nonlinear interaction described by Yu et al. (2021b) applies to the inhomogeneous turbulent background in the simulation
- ad hoc to paper The Gaussian filter scale 0.75 d_i separates large-scale turbulence from electron-scale fluctuations without distorting the wave dynamics
Cite this review
Pith. "Pith review of Electron scale magnetic holes generation driven by Whistler-to-Bernstein mode conversion in fully kinetic plasma turbulence." pith.science (2026). https://pith.science/paper/O6XEQX7J
@misc{pith2026250109651,
author = {Pith},
title = {Pith review of: Electron scale magnetic holes generation driven by Whistler-to-Bernstein mode conversion in fully kinetic plasma turbulence},
year = {2026},
howpublished = {\url{https://pith.science/paper/O6XEQX7J}},
note = {Machine review of arXiv:2501.09651}
}
read the original abstract
Magnetic holes (MHs) are coherent structures characterized by a strong and localized magnetic field amplitude dip, commonly observed in the solar wind and planetary magnetosheaths. These structures come in different sizes, from magnetohydrodynamic to kinetic scales. Magnetospheric Multiscale (MMS) observations have revealed electron scale MHs to be ubiquitous in the turbulent Earth's magnetosheath, potentially playing an important role in the energy cascade and dissipation. Despite abundant observations, the origin of electron scale MHs is still unclear and debated. In this work, we use fully kinetic simulations to investigate the role of plasma turbulence in generating electron scale MHs. We perform a fully kinetic simulation of freely decaying plasma turbulence, initialized with typical Earth's magnetosheath parameters. We find that electron scale MHs can be generated by turbulence via the following mechanism: first, large-scale turbulent velocity shears produce regions with high electron temperature anisotropy; these localized regions become unstable, generating oblique electron scale whistler waves; as they propagate over the inhomogeneous turbulent background, whistler fluctuations develop an electrostatic component, turning into Bernstein-like modes; the strong electrostatic fluctuations produce current filaments that merge into an electron scale current vortex; the resulting electron vortex locally reduces the magnetic field amplitude, finally evolving into an electron scale MH. We show that MHs generated by this mechanism have properties consistent with MMS observations and nontrivial kinetic features. We provide numerical evidence of a new electron scale MH generation mechanism, driven by turbulence. Our results have potential implications for understanding the formation and occurrence of electron scale MHs in turbulent environments, such as the Earth's magnetosheath.
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Works this paper leans on
-
[1]
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-
[2]
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-
[3]
2017, Physics of Plasmas, 24, 122121
Ahmadi, N., Germaschewski, K., & Raeder, J. 2017, Physics of Plasmas, 24, 122121
2017
-
[4]
D., Ergun, R
Ahmadi, N., Wilder, F. D., Ergun, R. E., et al. 2018, Journal of Geophysical Research: Space Physics, 123, 6383
2018
-
[5]
Arr \`o , G., Li, H., & Matthaeus, W. H. 2024, arXiv preprint arXiv:2411.19927
work page Pith review arXiv 2024
-
[6]
2024, The Astrophysical Journal Letters, 970, L6
Arrò, G., Califano, F., Pucci, F., Karlsson, T., & Li, H. 2024, The Astrophysical Journal Letters, 970, L6
2024
-
[7]
E., & Lapenta, G
Arrò, G., Pucci, F., Califano, F., Innocenti, M. E., & Lapenta, G. 2023, The Astrophysical Journal, 958, 11
2023
-
[8]
, Califano, F
Arró, G. , Califano, F. , & Lapenta, G. 2022, A&A, 668, A33
2022
Show all 96 references
-
[9]
2020, Phys
Bandyopadhyay, R., Sorriso-Valvo, L., Chasapis, A., et al. 2020, Phys. Rev. Lett., 124, 225101
2020
-
[10]
& Coppi, B
Basu, B. & Coppi, B. 1982, Phys. Rev. Lett., 48, 799
1982
-
[11]
2003, Geophysical Research Letters, 30
Baumgärtel, K., Sauer, K., & Dubinin, E. 2003, Geophysical Research Letters, 30
2003
-
[12]
L., Moore, T
Burch, J. L., Moore, T. E., Torbert, R. B., & Giles, B. L. 2015, Space Science Reviews, 199, 5–21
2015
-
[13]
2008, Journal of Geophysical Research: Space Physics, 113
Califano, F., Hellinger, P., Kuznetsov, E., et al. 2008, Journal of Geophysical Research: Space Physics, 113
2008
-
[14]
& Williamson, C
Cerreteli, C. & Williamson, C. H. K. 2003, Journal of Fluid Mechanics, 475, 41–77
2003
-
[15]
2022, Frontiers in Astronomy and Space Sciences, 9
Chen, Y., Wu, M., Xiao, S., et al. 2022, Frontiers in Astronomy and Space Sciences, 9
2022
-
[16]
T., & Janaki, M
Dasgupta, B., Tsurutani, B. T., & Janaki, M. S. 2003, Geophysical Research Letters, 30
2003
-
[17]
& Pegoraro, F
Del Sarto, D. & Pegoraro, F. 2017, Monthly Notices of the Royal Astronomical Society, 475, 181
2017
-
[18]
2016, Phys
Del Sarto, D., Pegoraro, F., & Califano, F. 2016, Phys. Rev. E, 93, 053203
2016
-
[19]
& Kostadinova, E
Dharodi, V. & Kostadinova, E. 2024, Physics of Plasmas, 31, 053702
2024
-
[20]
& Moya, P
Gallo-Méndez, I. & Moya, P. S. 2023, The Astrophysical Journal, 952, 30
2023
-
[21]
Gary, S. P. 1993, Theory of Space Plasma Microinstabilities, Cambridge Atmospheric and Space Science Series (Cambridge University Press)
1993
-
[22]
Gary, S. P. & Karimabadi, H. 2006, Journal of Geophysical Research: Space Physics, 111
2006
-
[23]
P., Lavraud, B., Thomsen, M
Gary, S. P., Lavraud, B., Thomsen, M. F., Lefebvre, B., & Schwartz, S. J. 2005, Geophysical Research Letters, 32
2005
-
[24]
Gary, S. P. & Wang, J. 1996, Journal of Geophysical Research: Space Physics, 101, 10749
1996
-
[25]
B., Burch, J
Giagkiozis, S., Wilson, L. B., Burch, J. L., et al. 2018, Journal of Geophysical Research: Space Physics, 123, 5435
2018
-
[26]
A., Bonnell, J
Goodrich, K. A., Bonnell, J. W., Curry, S., et al. 2021, Geophysical Research Letters, 48, e2020GL090329, e2020GL090329 2020GL090329
2021
-
[27]
T., Burgess, D., Camporeale, E., & Sundberg, T
Haynes, C. T., Burgess, D., Camporeale, E., & Sundberg, T. 2015, Physics of Plasmas, 22, 012309
2015
-
[28]
& Stverák, S
Hellinger, P. & Stverák, S. 2018, Journal of Plasma Physics, 84, 905840402
2018
-
[29]
Y., Du, J
Huang, S. Y., Du, J. W., Sahraoui, F., et al. 2017 a , Journal of Geophysical Research: Space Physics, 122, 8577
2017
-
[30]
Y., Sahraoui, F., Deng, X
Huang, S. Y., Sahraoui, F., Deng, X. H., et al. 2014, The Astrophysical Journal Letters, 789, L28
2014
-
[31]
Y., Sahraoui, F., Yuan, Z
Huang, S. Y., Sahraoui, F., Yuan, Z. G., et al. 2018, The Astrophysical Journal, 861, 29
2018
-
[32]
Y., Sahraoui, F., Yuan, Z
Huang, S. Y., Sahraoui, F., Yuan, Z. G., et al. 2017 b , The Astrophysical Journal Letters, 836, L27
2017
-
[33]
2014, Journal of Geophysical Research: Space Physics, 119, 4281
Ji, X.-F., Wang, X.-G., Sun, W.-J., et al. 2014, Journal of Geophysical Research: Space Physics, 119, 4281
2014
-
[34]
Johnson, J. R. & Cheng, C. Z. 1997, Journal of Geophysical Research: Space Physics, 102, 7179
1997
-
[35]
2013, Physics of Plasmas, 20
Karimabadi, H., Roytershteyn, V., Wan, M., et al. 2013, Physics of Plasmas, 20
2013
-
[36]
2021, Journal of Geophysical Research: Space Physics, 126, e2020JA028961, e2020JA028961 2020JA028961
Karlsson, T., Heyner, D., Volwerk, M., et al. 2021, Journal of Geophysical Research: Space Physics, 126, e2020JA028961, e2020JA028961 2020JA028961
2021
-
[37]
Kivelson, M. G. & Southwood, D. J. 1996, Journal of Geophysical Research: Space Physics, 101, 17365
1996
-
[38]
Krall, N. A. & Trivelpiece, A. W. 1986, Principles of plasma physics (San Francisco Press)
1986
-
[39]
A., Passot, T., & Sulem, P
Kuznetsov, E. A., Passot, T., & Sulem, P. L. 2007, Phys. Rev. Lett., 98, 235003
2007
-
[40]
2017, Journal of Computational Physics, 334, 349
Lapenta, G. 2017, Journal of Computational Physics, 334, 349
2017
-
[41]
2023, Physics, 5, 72
Lapenta, G. 2023, Physics, 5, 72
2023
-
[42]
2018, Journal of Geophysical Research: Space Physics, 123, 3277
Lee, S.-Y., Lee, E., Seough, J., et al. 2018, Journal of Geophysical Research: Space Physics, 123, 3277
2018
-
[43]
Leweke, T., Le Dizès, S., & Williamson, C. H. 2016, Annual Review of Fluid Mechanics, 48, 507
2016
-
[44]
2020, Nature Communications, 11
Li, J.-H., Yang, F., Zhou, X.-Z., et al. 2020, Nature Communications, 11
2020
-
[45]
& Zhang, M
Li, Z. & Zhang, M. 2023, Monthly Notices of the Royal Astronomical Society, 522, 2075
2023
-
[46]
2016, Journal of Geophysical Research: Space Physics, 121, 4180
Li, Z.-Y., Sun, W.-J., Wang, X.-G., et al. 2016, Journal of Geophysical Research: Space Physics, 121, 4180
2016
-
[47]
2016, The Astrophysical Journal, 824, 47
Lion, S., Alexandrova, O., & Zaslavsky, A. 2016, The Astrophysical Journal, 824, 47
2016
-
[48]
M., Fu, H
Liu, C. M., Fu, H. S., Liu, Y. Y., & Xu, Y. 2021, Geophysical Research Letters, 48, e2021GL093174, e2021GL093174 2021GL093174
2021
-
[49]
2019, Nature Communications, 10
Liu, H., Zong, Q.-G., Zhang, H., et al. 2019, Nature Communications, 10
2019
-
[50]
A., Moya, P
L \'o pez, R. A., Moya, P. S., Shaaban, S. M., et al. 2021, Advanced Numerical Tools for Studying Waves and Instabilities in Kappa Distributed Plasmas, ed. M. Lazar & H. Fichtner (Cham: Springer International Publishing), 163--184
2021
-
[51]
2013, Phys
Lyutikov, M. 2013, Phys. Rev. E, 88, 053103
2013
-
[52]
2021, Journal of Plasma Physics, 87, 905870310
López, R., Shaaban, S., & Lazar, M. 2021, Journal of Plasma Physics, 87, 905870310
2021
-
[53]
A., Nezlina, Y
Marchenko, V. A., Nezlina, Y. M., & Pokhotelov, O. A. 1988, Plasma Physics and Controlled Fusion, 30, 957
1988
-
[54]
& Lapenta, G
Markidis, S. & Lapenta, G. 2011, Journal of Computational Physics, 230, 7037
2011
-
[55]
V., Zabusky, N
Melander, M. V., Zabusky, N. J., & Mcwilliams, J. C. 1988, Journal of Fluid Mechanics, 195, 303–340
1988
-
[56]
2005, Comptes Rendus Physique, 6, 431, aircraft trailing vortices
Meunier, P., Le Dizès , S., & Leweke, T. 2005, Comptes Rendus Physique, 6, 431, aircraft trailing vortices
2005
-
[57]
1997, Physics of Plasmas, 4, 2871
Miura, A. 1997, Physics of Plasmas, 4, 2871
1997
-
[58]
2016, The Astrophysical Journal Letters, 827, L8
Narita, Y., Nakamura, R., Baumjohann, W., et al. 2016, The Astrophysical Journal Letters, 827, L8
2016
-
[59]
2016, The Astrophysical Journal, 826, 196
Perrone, D., Alexandrova, O., Mangeney, A., et al. 2016, The Astrophysical Journal, 826, 196
2016
-
[60]
D., Eastwood, J
Phan, T. D., Eastwood, J. P., Shay, M. A., et al. 2018, Nature, 557, 202–206
2018
-
[61]
A., Onishchenko, O
Pokhotelov, O. A., Onishchenko, O. G., & Stenflo, L. 2013, Physica Scripta, 87, 065303
2013
-
[62]
2021, The Astrophysical Journal Letters, 922, L18
Pucci, F., Viviani, M., Valentini, F., et al. 2021, The Astrophysical Journal Letters, 922, L18
2021
-
[63]
2021, Frontiers in Astronomy and Space Sciences, 7
Rakhmanova, L., Riazantseva, M., & Zastenker, G. 2021, Frontiers in Astronomy and Space Sciences, 7
2021
-
[64]
2015, Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, 373, 20140151
Roytershteyn, V., Karimabadi, H., & Roberts, A. 2015, Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, 373, 20140151
2015
-
[65]
T., Riedler, W., Schwingenschuh, K., & Yeroshenko, Y
Russell, C. T., Riedler, W., Schwingenschuh, K., & Yeroshenko, Y. 1987, Geophysical Research Letters, 14, 644
1987
-
[66]
2020, Reviews of Modern Plasma Physics, 4
Sahraoui, F., Hadid, L., & Huang, S. 2020, Reviews of Modern Plasma Physics, 4
2020
-
[67]
2012, Physical review letters, 108, 045001
Servidio, S., Valentini, F., Califano, F., & Veltri, P. 2012, Physical review letters, 108, 045001
2012
-
[68]
F., Artemyev, A
Shahid, M., Bashir, M. F., Artemyev, A. V., et al. 2024, Physics of Plasmas, 31, 072103
2024
-
[69]
2024, Science China Earth Sciences, 67, 2739–2771
Shi, Q., Yao, S., Hamrin, M., & Liu, J. 2024, Science China Earth Sciences, 67, 2739–2771
2024
-
[70]
Q., Pu, Z
Shi, Q. Q., Pu, Z. Y., Soucek, J., et al. 2009, Journal of Geophysical Research: Space Physics, 114
2009
-
[71]
2012, Journal of Geophysical Research: Space Physics, 117
Shoji, M., Omura, Y., & Lee, L.-C. 2012, Journal of Geophysical Research: Space Physics, 117
2012
-
[72]
2008, Journal of Geophysical Research: Space Physics, 113
Soucek, J., Lucek, E., & Dandouras, I. 2008, Journal of Geophysical Research: Space Physics, 113
2008
-
[73]
M., Baumg\"artel, K., & Ness, N
Sperveslage, K., Neubauer, F. M., Baumg\"artel, K., & Ness, N. F. 2000, Nonlinear Processes in Geophysics, 7, 191
2000
-
[74]
E., Eastwood, J
Stawarz, J. E., Eastwood, J. P., Phan, T. D., et al. 2019, The Astrophysical Journal Letters, 877, L37
2019
-
[75]
Stevens, M. L. & Kasper, J. C. 2007, Journal of Geophysical Research: Space Physics, 112
2007
-
[76]
V., & André, M
Svenningsson, I., Yordanova, E., Cozzani, G., Khotyaintsev, Y. V., & André, M. 2022, Geophysical Research Letters, 49, e2022GL099065, e2022GL099065 2022GL099065
2022
-
[77]
V., et al
Svenningsson, I., Yordanova, E., Khotyaintsev, Y. V., et al. 2024, Journal of Geophysical Research: Space Physics, 129, e2024JA032661, e2024JA032661 2024JA032661
2024
-
[78]
2010, Plasma Physics and Controlled Fusion, 53, 015003
Tenerani, A., Faganello, M., Califano, F., & Pegoraro, F. 2010, Plasma Physics and Controlled Fusion, 53, 015003
2010
-
[79]
T., Dasgupta, B., Galvan, C., et al
Tsurutani, B. T., Dasgupta, B., Galvan, C., et al. 2002, Geophysical Research Letters, 29, 86
2002
-
[80]
T., Lakhina, G
Tsurutani, B. T., Lakhina, G. S., Pickett, J. S., et al. 2005, Nonlinear Processes in Geophysics, 12, 321
2005
-
[81]
& Yanovsky, V
Tur, A. & Yanovsky, V. 2017, Coherent vortex structures in fluids and plasmas (Springer)
2017
-
[82]
M., Burlaga, L
Turner, J. M., Burlaga, L. F., Ness, N. F., & Lemaire, J. F. 1977, Journal of Geophysical Research (1896-1977), 82, 1921
1977
-
[83]
L., Delva, M., et al
Volwerk, M., Zhang, T. L., Delva, M., et al. 2008, Journal of Geophysical Research: Planets, 113
2008
-
[84]
2024 a , Earth and Planetary Physics, 8, 326
Wang, G., Xiao, S., Wu, M., Chen, Y., & Zhang, T. 2024 a , Earth and Planetary Physics, 8, 326
2024
-
[85]
Q., Volwerk, M., Wu, M
Wang, G. Q., Volwerk, M., Wu, M. Y., et al. 2021, The Astronomical Journal, 161, 110
2021
-
[86]
2024 b , Geophysical Research Letters, 51, e2023GL107968, e2023GL107968 2023GL107968
Wang, S., Wang, R., Lu, Q., Lu, S., & Huang, K. 2024 b , Geophysical Research Letters, 51, e2023GL107968, e2023GL107968 2023GL107968
2024
-
[87]
J., Neugebauer, M., Goldstein, B
Winterhalter, D., Smith, E. J., Neugebauer, M., Goldstein, B. E., & Tsurutani, B. T. 2000, Geophysical Research Letters, 27, 1615
2000
-
[88]
B., Huang, S
Xu, S. B., Huang, S. Y., Yuan, Z., et al. 2024, Journal of Geophysical Research: Space Physics, 129
2024
-
[89]
2023, Chinese Journal of Geophysics (in Chinese), 66, 871
YangJun, C., MingYu, W., SuDong, X., et al. 2023, Chinese Journal of Geophysics (in Chinese), 66, 871
2023
-
[90]
2021, Earth and Planetary Physics, 5, 63
Yao, S., Yue, Z., Shi, Q., et al. 2021, Earth and Planetary Physics, 5, 63
2021
-
[91]
T., Li, J
Yao, S. T., Li, J. H., Zhou, X.-Z., et al. 2023, Journal of Geophysical Research: Space Physics, 128, e2023JA031749, e2023JA031749 2023JA031749
2023
-
[92]
T., Shi, Q
Yao, S. T., Shi, Q. Q., Yao, Z. H., et al. 2019, Geophysical Research Letters, 46, 523
2019
-
[93]
T., Wang, X
Yao, S. T., Wang, X. G., Shi, Q. Q., et al. 2017, Journal of Geophysical Research: Space Physics, 122, 1990
2017
-
[94]
Y., Yuan, Z
Yu, L., Huang, S. Y., Yuan, Z. G., et al. 2021, The Astrophysical Journal, 908, 56
2021
-
[95]
L., Russell, C
Zhang, T. L., Russell, C. T., Baumjohann, W., et al. 2008, Geophysical Research Letters, 35
2008
-
[96]
H., Zhou, M., Huang, S
Zhong, Z. H., Zhou, M., Huang, S. Y., et al. 2019, Geophysical Research Letters, 46, 6248
2019
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