Publications

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Below, by year, are the publications listed in the HAL open archive.

2018

Electron Jet Detected by MMS at Dipolarization Front
- Liu C. M.
- Fu H.S.
- Vaivads A.
- Khotyaintsev Y. V.
- Gershman D. J.
- Hwang K.-J.
- Chen Z. Z.
- Cao D.
- Xu Y.
- Yang J.
- Peng F. Z.
- Huang S. Y.
- Burch J. L.
- Giles B. L.
- Ergun R. E.
- Russell C. T.
- Lindqvist P.-A.
- Le Contel Olivier
Geophysical Research Letters, American Geophysical Union, 2018, 45 (2), pp.556-564. Using MMS high-resolution measurements, we present the first observation of fast electron jet (<fi>V</fi><fi>e</fi> 2,000 km/s) at a dipolarization front (DF) in the magnetotail plasma sheet. This jet, with scale comparable to the DF thickness ( 0.9 <fi>d</fi><fi>i</fi>), is primarily in the tangential plane to the DF current sheet and mainly undergoes the E × B drift motion; it contributes significantly to the current system at the DF, including a localized ring-current that can modify the DF topology. Associated with this fast jet, we observed a persistent normal electric field, strong lower hybrid drift waves, and strong energy conversion at the DF. Such strong energy conversion is primarily attributed to the electron-jet-driven current (E s j<fi>e</fi> ≈ 2 E s j<fi>i</fi>), rather than the ion current suggested in previous studies. (10.1002/2017GL076509)
DOI : 10.1002/2017GL076509
A rotational Raman study under non-thermal conditions in a pulsed CO2 glow discharge
- Klarenaar Bart
- Grovulović Marija
- Morillo-Candas Ana-Sofia
- Bekerom D C M van Den
- Damen Mark
- Sanden Richard van De
- Guaitella Olivier
- Engeln Richard
Plasma Sources Science and Technology, IOP Publishing, 2018, 27 (4), pp.045009. The implementation of in situ rotational Raman spectroscopy is realized for a pulsed glow discharge in CO2 in the mbar range and is used to study the rotational temperature and molecular number densities of CO2, CO, and O2. The polarizability anisotropy of these molecules is required for extracting number densities from the recorded spectra and is determined for incident photons of 532 nm. The spatiotemporally-resolved measurements are performed in the same reactor and at equal discharge conditions (510 ms onoff cycle, 50 mA plasma current, 6.7 mbar pressure) as in recently published work employing in situ Fourier transform infrared (FTIR) spectroscopy. The rotational temperature ranges from 394 to 809 K from start to end of the discharge pulse and is constant over the length of the reactor. The discharge is demonstrated to be spatially uniform in gas composition, with a CO2 conversion factor of 0.15 ± 0.02. Rotational temperatures and molecular composition agree well with the FTIR results, while the spatial uniformity confirms the assumption made for the FTIR analysis of a homogeneous medium over the line-of-sight of absorption. Furthermore, the rotational Raman spectra of CO2 are related to vibrational temperatures through the vibrationally averaged nuclear spin degeneracy, which is expressed in the intensity ratio between even and odd numbered Raman peaks. The elevation of the odd averaged degeneracy above thermal conditions agrees well with the elevation of vibrational temperatures of CO2, acquired in the FTIR study. (10.1088/1361-6595/aabab6)
DOI : 10.1088/1361-6595/aabab6
Living on mars: how to produce oxygen and fuel to get home
- Guerra V.
- Silva Tiago
- Guaitella Olivier
Europhysics News, EDP Sciences, 2018, 49 (3), pp.15-18. Sending a manned mission to Mars is one of the next major steps in space exploration. Creating a breathable environment, however, is a substantial challenge. A sustainable oxygen supply on the red planet can be achieved by converting carbon dioxide directly from the Martian atmosphere. A new solution to do so is on the way: plasma technology. (10.1051/epn/2018302)
DOI : 10.1051/epn/2018302
Observations of Whistler Waves Correlated with Electron-scale Coherent Structures in the Magnetosheath Turbulent Plasma
- Huang S. Y.
- Sahraoui Fouad
- Yuan Z. G.
- Le Contel Olivier
- Breuillard Hugo
- He J. S.
- Zhao J. S.
- Fu H.S.
- Zhou M.
- Deng X. H.
- Wang X. Y.
- Du J. W.
- Yu X. D.
- Wang D. D.
- Pollock C. J.
- Torbert R. B.
- Burch J. L.
The Astrophysical Journal, American Astronomical Society, 2018, 861. A new type of electron-scale coherent structure, referred to as electron vortex magnetic holes, was identified recently in the Earth's magnetosheath turbulent plasma. These electron-scale magnetic holes are characterized by magnetic field strength depression, electron density enhancement, temperature and temperature anisotropy increase (a significant increase in perpendicular temperature and a decrease in parallel temperature), and an electron vortex formed by the trapped electrons. The strong increase of electron temperature indicates that these magnetic holes have a strong connection with the energization of electrons. Here, using high time resolution in situ measurements from the MMS mission, it is further shown that electron-scale whistler waves coexist with electron-scale magnetic holes. These whistler waves were found not propagating from remote regions, but generated locally due to electron temperature anisotropy (T e⊥/T e||) inside the magnetic holes. This study provides new insights into the electron-scale plasma dynamics in turbulent plasmas. (10.3847/1538-4357/aac831)
DOI : 10.3847/1538-4357/aac831
Higher-Order Turbulence Statistics in the Earth's Magnetosheath and the Solar Wind Using Magnetospheric Multiscale Observations
- Chhiber R.
- Chasapis A.
- Bandyopadhyay R.
- Parashar T. N.
- Matthaeus W. H.
- Maruca B. A.
- Moore T. E.
- Burch J. L.
- Torbert R. B.
- Russell C. T.
- Le Contel Olivier
- Argall M. R.
- Fischer D.
- Mirioni Laurent
- Strangeway R. J.
- Pollock C. J.
- Giles B. L.
- Gershman D. J.
Journal of Geophysical Research Space Physics, American Geophysical Union/Wiley, 2018, 123 (12), pp.9941-9954. High-resolution multispacecraft magnetic field measurements from the Magnetospheric Multiscale mission's flux-gate magnetometer are employed to examine statistical properties of plasma turbulence in the terrestrial magnetosheath and in the solar wind. Quantities examined include wave number spectra; structure functions of order two, four, and six; probability density functions of increments; and scale-dependent kurtoses of the magnetic field. We evaluate the Taylor frozen-in approximation by comparing single-spacecraft time series analysis with direct multispacecraft measurements, including evidence based on comparison of probability distribution functions. The statistics studied span spatial scales from the inertial range down to proton and electron scales. We find agreement of spectral estimates using three different methods, and evidence of intermittent turbulence in both magnetosheath and solar wind; however, evidence for subproton-scale coherent structures, seen in the magnetosheath, is not found in the solar wind. (10.1029/2018JA025768)
DOI : 10.1029/2018JA025768
Optical actinometry of O-atoms in pulsed nanosecond capillary discharge: peculiarities of kinetics at high specific deposited energy
- Zhu Yifei
- Lepikhin N D
- Orel Inna
- Salmon A.
- Klochko A.V.
- Starikovskaia Svetlana
Plasma Sources Science and Technology, IOP Publishing, 2018. Density of O-atoms was studied in capillary nanosecond discharge in air with 5.3% additions of Ar at 28.5 mbar. Time-resolved electrical current, longitudinal electric fifield, optical emission of O(3p3P), Ar(2p1) and their ratio, and emission of N2(C)were measured. A kinetic scheme describing consistent behavior of the set of the experimental data was developed. The main processes responsible for population and decay of the species of interest were selected on the basis of sensitivity and rate analysis. The electric fifield was taken as input data; all other experimentally obtained signals were modeled; experimental data and results of calculations are in good agreement. The role of the reactions between excited, charged species and electrons in early afterglow for pulsed discharges at high reduced electric fifields and high specifific deposited energy was discussed. Density of O atoms in the ground state was calculated. It was concluded that Ar-based traditional actinometry demands an advanced kinetic modeling in the case of the nanosecond discharge with a high specifific energy deposition. (10.1088/1361-6595/aac95f)
DOI : 10.1088/1361-6595/aac95f
Imaging axial and radial electric field components in dielectric targets under plasma exposure
- Slikboer Elmar
- Sobota Ana
- Guaitella Olivier
- Garcia-Caurel Enric
Journal of Physics D: Applied Physics, IOP Publishing, 2018, 51 (11), pp.115203. Mueller polarimetry is used to investigate the behavior of an electro optic target (BSO crystal) under exposure of guided ionization waves produced by an atmospheric pressure plasma jet. For the first time, this optical technique is time resolved to obtain the complete Mueller matrix of the sample right before and after the impact of the discharges. By analyzing the induced birefringence, the spatial profiles and local values are obtained of both the electric field and temperature in the sample. Electric fields are generated due to deposited surface charges and a temperature profile is present, due to the heat transferred by the plasma jet. The study of electric field dynamics and local temperature increase at the target, due to the plasma jet is important for biomedical applications, as well as surface functionalization. This work shows how Mueller polarimetry can be used as a novel diagnostic to simultaneously acquire the spatial distribution and local values of both the electric field and temperature, by coupling the external source of anisotropy to the measured induced birefringence via the symmetry point group of the examined material. (10.1088/1361-6463/aaad99)
DOI : 10.1088/1361-6463/aaad99
Electron Energization at a Reconnecting Magnetosheath Current Sheet
- Eriksson Elin
- Vaivads Andris
- Graham Daniel B.
- Divin Andrey
- Khotyaintsev Yu. V.
- Yordanova Emiliya
- André Mats
- Giles Barbara L.
- Pollock Craig J.
- Russell Christopher T.
- Le Contel O.
- Torbert Roy B.
- Ergun Robert E.
- Lindqvist Per-Arne
- Burch James L.
Geophysical Research Letters, American Geophysical Union, 2018, 45, pp.8081-8090. We present observations of electron energization within a sub-ion-scale magnetosheath current sheet (CS). A number of signatures indicate ongoing reconnection, including the thickness of the CS (&tilde;0.7 ion inertial length), nonzero normal magnetic field, Hall magnetic fields with electrons carrying the Hall currents, and electron heating. We observe localized electron acceleration and heating parallel to the magnetic field at the edges of the CS. Electrostatic waves observed in these regions have low phase velocity and small wave potentials and thus cannot provide the observed acceleration and heating. Instead, we find that the electrons are accelerated by a parallel potential within the separatrix regions. Similar acceleration has been reported based on magnetopause and magnetotail observations. Thus, despite the different plasma conditions in magnetosheath, magnetopause, and magnetotail, the acceleration mechanism and corresponding heating of electrons is similar. (10.1029/2018GL078660)
DOI : 10.1029/2018GL078660
Study of Ionospheric Variability Using GNSS Observations
- Taoufiq Jouan
- Mourad Bouziani
- Rachid Azzouzi
- Amory-Mazaudier Christine
Positioning, SCIRP, 2018, 09 (04), pp.79-96. <div>With the increasing number of applications of Global navigation satellite system, the modeling of the ionosphere is a crucial element for precise positioning. Indeed, the ionosphere delays the electromagnetic waves which pass through it and induces a delay of propagation related to the electronic density (TEC) Total Electronic Content and to the frequency of the wave. The impact of this ionospheric error often results in a poor determination of the station's position, particularly in strong solar activity. The first part of this paper focuses on a bibliographic study oriented first of all on the study of the ionosphere in relation to solar activity and secondly on the determination of the total electron content using GNSS measurements from the IGS network reference stations. Measurements were made on two permanent stations "RABT", "TETN". We selected years of GNSS measurements to evaluate the geomagnetic impact on the ionosphere, 2001, 2009 and 2013. A description of the ionospheric disturbances and geomagnetic storms was analyzed by determination of TEC, especially in high solar activity. The results show a strong dependence of the ionospheric activity with the geomagnetic activity.</div> (10.4236/pos.2018.94006)
DOI : 10.4236/pos.2018.94006
Kinetics of highly vibrationally excited O2 (X) molecules in inductively-coupled oxygen plasmas
- Annusova Adriana
- Marinov Daniil
- Booth Jean-Paul
- Sirse Nishant
- Silva Mrio Lino Da
- Lopez B.
- Guerra V.
Plasma Sources Science and Technology, IOP Publishing, 2018, 27 (4), pp.045006. The high degree of vibrational excitation of O 2 ground state molecules recently observed in inductively coupled plasma discharges is investigated experimentally in more detail and interpreted using a detailed self-consistent 0D global kinetic model for oxygen plasmas. Additional experimental results are presented and used to validate the model. The vibrational kinetics considers vibrational levels up to v = 41 and accounts for electron impact excitation and de-excitation (e-V), vibration-to-translation relaxation (V-T) in collisions with O 2 molecules and O atoms, vibration-to-vibration energy exchanges (V-V), excitation of electronically excited states, dissociative electron attachment, and electron impact dissociation. Measurements were performed at pressures of 10?80 mTorr (1.33 and 10.67 Pa) and radio frequency (13.56 MHz) powers up to 500 W. The simulation results are compared with the absolute densities in each O 2 vibrational level obtained by high sensitivity absorption spectroscopy measurements of the Schumann?Runge bands for O 2 ( X , v = 4?18), O( 3 P ) atom density measurements by two-photon absorption laser induced fluorescence (TALIF) calibrated against Xe, and laser photodetachment measurements of the O ? negative ions. The highly excited O 2 ( X , v ) distribution exhibits a shape similar to a Treanor-Gordiets distribution, but its origin lies in electron impact e-V collisions and not in V-V up-pumping, in contrast to what happens in all other molecular gases known to date. The relaxation of vibrational quanta is mainly due to V-T energy-transfer collisions with O atoms and to electron impact dissociation of vibrationally excited molecules, e O 2 ( X , v )?O( 3 P) O( 3 P). (10.1088/1361-6595/aab47d)
DOI : 10.1088/1361-6595/aab47d
Recent advances in the modeling and computer simulations of non-equilibrium plasma discharges
- Raja Laxminarayan L
- Bourdon Anne
- Ventzek Peter L G
Journal of Physics D: Applied Physics, IOP Publishing, 2018, 51 (15), pp.150202. The mathematical modeling and computer simulation of low-temperature plasmas is gradually such a level of maturity that these simulation tools can be used not just for improving scientific understanding but also as computer-aided engineering design tools in an industrial setting. These models necessarily involve the description of multiple physical phenomena occurring over a range of times and lengths, thereby complicating their numerical implementation and solution. This special issue presents 12 invited contributions that present recent developments in the field of modeling and simulation of low-temperature plasma discharges. This editorial introduces these papers by providing an overview of the context in which these papers are presented. (10.1088/1361-6463/aab1b9)
DOI : 10.1088/1361-6463/aab1b9
Investigation of a plasma--target interaction through electric field characterization examining surface and volume charge contributions: modeling and experiment
- Viegas Pedro
- Slikboer Elmar
- Obrusník Adam
- Bonaventura Zdenek
- Sobota Ana
- Garcia-Caurel Enric
- Guaitella Olivier
- Bourdon Anne
Plasma Sources Science and Technology, IOP Publishing, 2018, 27. Numerical simulations and experiments are performed to better understand the interaction between a pulsed helium plasma jet and a dielectric target. The focus of this work lies on the volume and surface charge influence on the electric field distribution. Experimentally, the electric field due to surface charges is measured inside an electro-optic target under exposure of a plasma jet, using the optical technique called Mueller polarimetry. For the first time, the time-resolved spatial distributions of both the axial and radial components of electric field inside the target are obtained simultaneously. A 2D fluid model is used in a complementary way to the experiments in order to study separately the contribution of volume charges and surface charges to the spatio-temporal evolutions of the electric field during the plasma--surface interaction. The experimental investigation shows that the average axial and radial components of electric field inside the dielectric target, only due to surface charges, are lower than generally reported for electric field values in the plasma plume. Thanks to the phenomenological comparison with experiments, simulations show that during the plasma--surface interaction two effects sequentially determine the electric field inside the target: firstly, a relatively high electric field is observed due to the proximity of the ionization front; afterwards, in longer timescales, lower electric fields are induced due to the contribution of both leftover volume charges close to the target and surface charges deposited on its surface. The experimental technique provides a unique way to examine this second phase of the plasma--surface interaction. (10.1088/1361-6595/aadcc0)
DOI : 10.1088/1361-6595/aadcc0
Drift-wave observation in a toroidal magnetized plasma and comparison with a modified Hasegawa-Wakatani model
- Donnel Peter
- Morel Pierre
- Honoré Cyrille
- Gürcan Özgür D.
- Pisarev V.
- Metzger C.
- Hennequin Pascale
Physics of Plasmas, American Institute of Physics, 2018, 25 (6), pp.062127. This paper presents the results of fluctuation measurements in a toroidal magnetized plasma, using Langmuir probes, and comparisons between the observed frequency modes and a Hasegawa-Wakatani model including curvature, adapted to the specifics of the toroidal device. More precisely, two kinds of signals are detected in the presence of an additional vertical magnetic field in the region of significant density and potential gradients. A high frequency, propagating component, corresponding to dissipative drift-waves in the curved magnetic field, is observed and the frequency and typical wavelengths are found to be in good agreement with the linear Hasegawa-Wakatani model including curvature effects. A second, low frequency component is observed at lower frequencies and is shown to correspond to large scale vertical electrostatic field structures. A significantly high level of cross correlation is observed between these two signals, with an identifiable time delay, which suggests an analogy to the time delayed quasi-periodic dynamics in predator-prey systems, and a similar phenomenon is observed between zonal flows and microturbulence in tokamaks and other magnetised plasma systems. (10.1063/1.5025141)
DOI : 10.1063/1.5025141
Observations of core ion cyclotron emission on ASDEX Upgrade tokamak
- Ochoukov R.
- Bobkov V.
- Chapman B.
- Dendy R.
- Dunne M.
- Faugel H.
- García Muñoz M.
- Geiger B.
- Hennequin Pascale
- Mcclements K. G.
- Moseev D.
- Nielsen S.
- Rasmussen J.
- Schneider P.
- Weiland M.
- Noterdaeme J.-M.
Review of Scientific Instruments, American Institute of Physics, 2018, 89 (10), pp.10J101. The B-dot probe diagnostic suite on the ASDEX Upgrade tokamak has recently been upgraded with a new 125 MHz, 14 bit resolution digitizer to study ion cyclotron emission (ICE). While classic edge emission from the low field side plasma is often observed, we also measure waves originating from the core with fast fusion protons or beam injected deuterons being a possible emission driver. Comparing the measured frequency values with ion cyclotron harmonics present in the plasma places the origin of this emission on the magnetic axis, with the fundamental hydrogen/second deuterium cyclotron harmonic matching the observed values. The actual values range from ∼27 MHz at the on-axis toroidal field BT = -1.79 T to ∼40 MHz at BT = -2.62 T. When the magnetic axis position evolves during this emission, the measured frequency values track the changes in the estimated on-axis cyclotron frequency values. Core ICE is usually a transient event lasting ∼100 ms during the neutral beam startup phase. However, in some cases, core emission occurs in steady-state plasmas and lasts for longer than 1 s. These observations suggest an attractive possibility of using a non-perturbing ICE-based diagnostic to passively monitor fusion alpha particles at the location of their birth in the plasma core, in deuterium-tritium burning devices such as ITER and DEMO. (10.1063/1.5035180)
DOI : 10.1063/1.5035180
Logarithmically discretized model of bounce averaged gyrokinetics and its implications on tokamak turbulence
- Xu S.
- Morel Pierre
- Gürcan Özgür D.
Physics of Plasmas, American Institute of Physics, 2018, 25 (10), pp.102306. A logarithmically discretized model, which consists of writing the system in log polar coordinates in wave-number domain and reducing the nonlinear interactions to a sum over neighboring scales that satisfy the triad conditions, is proposed for bounce averaged gyrokinetics, where the energy dependence is kept over a semi-regular grid that allows quadrature calculations in order to guarantee quasi-neutrality. The resulting model is a cheaper implementation of nonlinear multi-scale physics involving trapped electron modes, trapped ion modes, and zonal flows, which can handle anisotropy. The resulting wave-number spectrum is anisotropic at large scales, where the energy injection is clearly anisotropic, but is isotropised rapidly, leading generally towards an isotropic k−4 spectrum for spectral potential energy density for fully kinetic system and a k−5 spectrum for the system with one adiabatic species. Zonal flow damping, which is necessary for reaching a steady state in this model, plays an important role along with electron adiabaticity. Interesting dynamics akin to predator-prey evolution is observed among zonal flows and similarly large scale but radially elongated structures. (10.1063/1.5049681)
DOI : 10.1063/1.5049681
Self-organized patterns by a DC pin liquid anode discharge in ambient air: Effect of liquid types on formation
- Zhang Shiqiang
- Dufour Thierry
Physics of Plasmas, American Institute of Physics, 2018, 25 (7), pp.073502. A pin liquid anode DC discharge is generated in open air without any additional gas feeding to form self-organized patterns (SOPs) on various liquid interfaces. Axially resolved emission spectra of the whole discharge reveal that the self-organized patterns are formed below a dark region and are visible mainly due to the N2 (C 3 -B 3 ) transitions. The high energy N2 (C) level is mainly excited by the impact of electrons heated by the local increased electric field at the interface. For the first time, the effect of the liquid type on the SOP formation is presented. With almost the same other discharge conditions, the formed SOPs are significantly different from HCl and H2SO4 liquid anodes. The SOP difference is repeated when the discharge current and gap distance change for both liquid anodes. The variations of SOP size and discretization as a function of discharge current and gap distance are discussed and confirm that different SOPs are formed by the HCl liquid anode from tap water or the H2SO4 liquid anode. A possible explanation is brought up to explain the dependence of SOPs on the liquid type. (10.1063/1.5030099)
DOI : 10.1063/1.5030099
Reply to Comment on `The case for in situ resource utilisation for oxygen production on Mars by non-equilibrium plasmas
- Guerra Vasco
- Silva Tiago
- Ogloblina Polina
- Grofulovic Marija
- Terraz Loann
- Lino da Silva Mário
- Pintassilgo Carlos D.
- Alves Luís L.
- Guaitella Olivier
Plasma Sources Science and Technology, IOP Publishing, 2018, 27. Not Available (10.1088/1361-6595/aaa570)
DOI : 10.1088/1361-6595/aaa570
Numerical study of the influence of surface reaction probabilities on reactive species in an rf atmospheric pressure plasma containing humidity
- Schröter Sandra
- Gibson Andrew R.
- Kushner Mark J.
- Gans Timo
- O'Connell Deborah
Plasma Physics and Controlled Fusion, IOP Publishing, 2018, 60. The quantification and control of reactive species (RS) in atmospheric pressure plasmas (APPs) is of great interest for their technological applications, in particular in biomedicine. Of key importance in simulating the densities of these species are fundamental data on their production and destruction. In particular, data concerning particle-surface reaction probabilities in APPs are scarce, with most of these probabilities measured in low-pressure systems. In this work, the role of surface reaction probabilities, gamma, of reactive neutral species (H, O and OH) on neutral particle densities in a He-H2O radio-frequency micro APP jet (COST-mu APPJ) are investigated using a global model. It is found that the choice of gamma, particularly for low-mass species having large diffusivities, such as H, can change computed species densities significantly. The importance of gamma even at elevated pressures offers potential for tailoring the RS composition of atmospheric pressure microplasmas by choosing different wall materials or plasma geometries. (10.1088/1361-6587/aa8fe9)
DOI : 10.1088/1361-6587/aa8fe9
Fast gas heating of nanosecond pulsed surface dielectric barrier discharge: spatial distribution and fractional contribution from kinetics
- Zhu Yifei
- Starikovskaia Svetlana
Plasma Sources Science and Technology, IOP Publishing, 2018, 27. The effect of heat release in reactions with charged and electronically excited species, or so-called fast gas heating (FGH), in nanosecond surface dielectric barrier discharge (nSDBD) in atmospheric pressure air is studied. Two-dimensional numerical simulations based on the PArallel Streamer Solver with KinEtics code are conducted. The code is based on the direct coupling of a self-consistent fluid model with detailed kinetics, an efficient photoionization model, and Euler equations. The choice of local field approximation for nSDBD modeling with simplified kinetics is discussed. The reduced electric field and the electron density are examined at both polarities for identical high-voltage pulses 24 kV in amplitude on a high-voltage electrode and 20 ns full width at half maximum. The distribution of the FGH energy and the resulting gas temperature field are studied and compared with findings in the literature. The input of different reactions to the appearance of hydrodynamic perturbations is analyzed. (10.1088/1361-6595/aaf40d)
DOI : 10.1088/1361-6595/aaf40d
Magnetic depression and electron transport in an ion-scale flux rope associated with Kelvin–Helmholtz waves
- Tang Binbin
- Li Wenya
- Wang Chi
- Dai Lei
- Khotyaintsev Yuri
- Lindqvist Per-Arne
- Ergun Robert
- Le Contel Olivier
- Pollock Craig
- Russell Christopher
- Burch James
Annales Geophysicae, European Geosciences Union, 2018, 36 (3), pp.879-889. We report an ion-scale magnetic flux rope (the size of the flux rope is ∼ 8.5 ion inertial lengths) at the trailing edge of Kelvin–Helmholtz (KH) waves observed by the Magnetospheric Multiscale (MMS) mission on 27 Septem-ber 2016, which is likely generated by multiple X-line re-connection. The currents of this flux rope are highly filamen-tary: in the central flux rope, the current flows are mainly parallel to the magnetic field, supporting a local magnetic field increase at about 7 nT, while at the edges the current filaments are predominantly along the antiparallel direction, which induce an opposing field that causes a significant magnetic depression along the axis direction (> 20 nT), meaning the overall magnetic field of this flux rope is depressed compared to the ambient magnetic field. Thus, this flux rope, accompanied by the plasma thermal pressure enhancement in the center, is referred to as a crater type. Intense lower hybrid drift waves (LHDWs) are found at the magnetospheric edge of the flux rope, and the wave potential is estimated to be ∼ 17 % of the electron temperature. Though LHDWs may be stabilized by the mechanism of electron resonance broadening , these waves could still effectively enable diffusive electron transports in the cross-field direction, corresponding to a local density dip. This indicates LHDWs could play important roles in the evolution of crater flux ropes. (10.5194/angeo-36-879-2018)
DOI : 10.5194/angeo-36-879-2018
Analyzing the Magnetopause Internal Structure: New Possibilities Offered by MMS Tested in a Case Study
- Rezeau Laurence
- Belmont Gérard
- Manuzzo Roberto
- Aunai Nicolas
- Dargent Jérémy
Journal of Geophysical Research Space Physics, American Geophysical Union/Wiley, 2018, 123 (1), pp.227-241. We explore the structure of the magnetopause using a crossing observed by the Magnetospheric Multiscale (MMS) spacecraft on 16 October 2015. Several methods (minimum variance analysis, BV method, and constant velocity analysis) are first applied to compute the normal to the magnetopause considered as a whole. The different results obtained are not identical, and we show that the whole boundary is not stationary and not planar, so that basic assumptions of these methods are not well satisfied. We then analyze more finely the internal structure for investigating the departures from planarity. Using the basic mathematical definition of what is a one‐dimensional physical problem, we introduce a new single spacecraft method, called LNA (local normal analysis) for determining the varying normal, and we compare the results so obtained with those coming from the multispacecraft minimum directional derivative (MDD) tool developed by Shi et al. (2005). This last method gives the dimensionality of the magnetic variations from multipoint measurements and also allows estimating the direction of the local normal when the variations are locally 1‐D. This study shows that the magnetopause does include approximate one‐dimensional substructures but also two‐ and three‐dimensional structures. It also shows that the dimensionality of the magnetic variations can differ from the variations of other fields so that, at some places, the magnetic field can have a 1‐D structure although all the plasma variations do not verify the properties of a global one‐dimensional problem. A generalization of the MDD tool is proposed. (10.1002/2017JA024526)
DOI : 10.1002/2017JA024526
Plasma-activation of tap water using DBD for agronomy applications: Identification and quantification of long lifetime chemical species and production/consumption mechanisms
- Judée Florian
- Simon Stéphane
- Bailly Christophe
- Dufour Thierry
Water Research, IWA Publishing/Elsevier, 2018, 133, pp.47-59. Cold atmospheric plasmas are weakly ionized gases that can be generated in ambient air. They produce energetic species (e.g. electrons, metastables) as well as reactive oxygen species, reactive nitrogen species, UV radiations and local electric field. Their interaction with a liquid such as tap water can hence change its chemical composition. The resulting " plasma-activated liquid " can meet many applications, including medicine and agriculture. Consequently, a complete experimental set of analytical techniques dedicated to the characterization of long lifetime chemical species has been implemented to characterize tap water treated using cold atmospheric plasma process and intended to agronomy applications. For that purpose, colorimetry and acid titrations are performed, considering acid-base equilibria, pH and temperature variations induced during plasma activation. 16 species are quantified and monitored: hydroxide and hydronium ions, ammonia and ammonium ions, orthophosphates, carbonate ions, nitrite and nitrate ions and hydrogen peroxide. The related consumption/production mechanisms are discussed. In parallel, a chemical model of electrical conductivity based on Kohlrausch's law has been developed to simulate the electrical conductivity of the plasma-activated tap water (PATW). Comparing its predictions with experimental measurements leads to a narrow fitting, hence supporting the self-sufficiency of the experimental set, i.e. the fact that all long lifetime radicals of interest present in PATW are characterized. Finally, to evaluate the potential of cold atmospheric plasmas for agriculture applications, tap water has been daily plasma-treated to irrigate lentils seeds. Then, seedlings lengths have been measured and compared with untreated tap water, showing an increase as high as 34.0% and 128.4% after 3 days and 6 days of activation respectively. The interaction mechanisms between plasma and tap water are discussed as well as their positive synergy on agronomic results. (10.1016/j.watres.2017.12.035)
DOI : 10.1016/j.watres.2017.12.035
A turbulent cascade model of bounce averaged gyrokinetics
- Xu S.
- Morel Pierre
- Gürcan Özgür D.
Physics of Plasmas, American Institute of Physics, 2018, 25 (2), pp.022304. A shell model is derived for the description of nonlinear bounce averaged gyrokinetics, which is one of the simplest kinetic descriptions in magnetized plasmas. In order to validate the numerical implementation, detailed linear evolution of the system is compared with a linear benchmark based on solving the linear dispersion relation numerically. The resulting wave number spectrum, which extends over 34 decades, is shown to have a robust general structure to model parameters, such as dissipation or the ratio of linear energy injection to nonlinear transfer. In a range of wave numbers where the nonlinear transfer term is dominant, a power law spectrum, roughly of the form k−4 , is observed for the spectral electrostatic potential energy density. The model, being fully kinetic, can be used to obtain the free energy spectra for ion and electron distribution functions as functions of E. This model constitutes the first numerical implementation of a kinetic shell model. (10.1063/1.5020145)
DOI : 10.1063/1.5020145
Electron Power-Law Spectra in Solar and Space Plasmas
- Oka Mitsuo
- Birn J.
- Battaglia Marina
- Chaston C. C.
- Hatch S. M.
- Livadiotis G.
- Imada S.
- Miyoshi Y.
- Kuhar M.
- Effenberger F.
- Eriksson E.
- Khotyaintsev Yu. V.
- Retinò Alessandro
Space Science Reviews, Springer Verlag, 2018, 214. Particles are accelerated to very high, non-thermal energies in solar and space plasma environments. While energy spectra of accelerated electrons often exhibit a power law, it remains unclear how electrons are accelerated to high energies and what processes determine the power-law index delta . Here, we review previous observations of the power-law index delta in a variety of different plasma environments with a particular focus on sub-relativistic electrons. It appears that in regions more closely related to magnetic reconnection (such as the `above-the-looptop' solar hard X-ray source and the plasma sheet in Earth's magnetotail), the spectra are typically soft (delta &gsim;4). This is in contrast to the typically hard spectra (delta &lsim;4) that are observed in coincidence with shocks. The difference implies that shocks are more efficient in producing a larger non-thermal fraction of electron energies when compared to magnetic reconnection. A caveat is that during active times in Earth's magnetotail, delta values seem spatially uniform in the plasma sheet, while power-law distributions still exist even in quiet times. The role of magnetotail reconnection in the electron power-law formation could therefore be confounded with these background conditions. Because different regions have been studied with different instrumentations and methodologies, we point out a need for more systematic and coordinated studies of power-law distributions for a better understanding of possible scaling laws in particle acceleration as well as their universality. (10.1007/s11214-018-0515-4)
DOI : 10.1007/s11214-018-0515-4
Wave Phenomena and Beam-Plasma Interactions at the Magnetopause Reconnection Region
- Burch J. L.
- Webster J. M.
- Genestreti K. J.
- Torbert R. B.
- Giles B. L.
- Fuselier S. A.
- Dorelli J. C.
- Rager A. C.
- Phan T. D.
- Allen R. C.
- Chen L.-J.
- Wang S.
- Le Contel Olivier
- Russell C. T.
- Strangeway R. J.
- Ergun R. E.
- Jaynes A. N.
- Lindqvist P.-A.
- Graham D. B.
- Wilder F. D.
- Hwang K.-J.
- Goldstein J.
Journal of Geophysical Research Space Physics, American Geophysical Union/Wiley, 2018, 123 (2), pp.1118-1133. This paper reports on Magnetospheric Multiscale observations of whistler mode chorus and higher-frequency electrostatic waves near and within a reconnection diffusion region on 23 November 2016. The diffusion region is bounded by crescent-shaped electron distributions and associated dissipation just upstream of the X-line and by magnetic field-aligned currents and electric fields leading to dissipation near the electron stagnation point. Measurements were made southward of the X-line as determined by southward directed ion and electron jets. We show that electrostatic wave generation is due to magnetosheath electron beams formed by the electron jets as they interact with a cold background plasma and more energetic population of magnetospheric electrons. On the magnetosphere side of the X-line the electron beams are accompanied by a strong perpendicular electron temperature anisotropy, which is shown to be the source of an observed rising-tone whistler mode chorus event. We show that the apex of the chorus event and the onset of electrostatic waves coincide with the opening of magnetic field lines at the electron stagnation point. (10.1002/2017JA024789)
DOI : 10.1002/2017JA024789

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