Publications

2013

• Asymmetric distribution of reconnection jet fronts in the Jovian nightside magnetosphere
  
  • Kasahara S.
  • Kronberg E. A.
  • Kimura T.
  • Tao C.
  • Badman S. V.
  • Masters A.
  • Retinò Alessandro
  • Krupp N.
  • Fujimoto M.
  Journal of Geophysical Research Space Physics, American Geophysical Union/Wiley, 2013, 118, pp.375-384. Magnetic reconnection plays important roles in mass transport and energy conversion in planetary magnetospheres. It is considered that transient reconnection causes localized auroral arcs or spots in the Jovian magnetosphere, by analogy to the case in the Earth's magnetosphere. However, the local structures of transient reconnection events (i.e., magnetospheric plasma parameters) and their spatial distribution have not been extensively investigated for the Jovian magnetosphere. Here we examine plasma velocity and density during strong north-south magnetic field events in the Jovian nightside magnetosphere, which may be associated with tail reconnection. We find prominent reconnection jet fronts predominantly on the dawnside of the nightside magnetosphere, which would be a signature unique to rotation-dominant planetary magnetospheres. The observed plasma structures are consistent with significant field-aligned currents which would generate localized aurora. (10.1029/2012JA018130)
  DOI : 10.1029/2012JA018130
• Comparison between hybrid and fully kinetic models of asymmetric magnetic reconnection: Coplanar and guide field configurations
  
  • Aunai Nicolas
  • Hesse Michael
  • Zenitani Seiji
  • Kuznetsova M. M.
  • Black Carrie
  • Evans Rebekah
  • Smets Roch
  Physics of Plasmas, American Institute of Physics, 2013, 20, pp.022902. Magnetic reconnection occurring in collisionless environments is a multi-scale process involving both ion and electron kinetic processes. Because of their small mass, the electron scales are difficult to resolve in numerical and satellite data, it is therefore critical to know whether the overall evolution of the reconnection process is influenced by the kinetic nature of the electrons, or is unchanged when assuming a simpler, fluid, electron model. This paper investigates this issue in the general context of an asymmetric current sheet, where both the magnetic field amplitude and the density vary through the discontinuity. A comparison is made between fully kinetic and hybrid kinetic simulations of magnetic reconnection in coplanar and guide field systems. The models share the initial condition but differ in their electron modeling. It is found that the overall evolution of the system, including the reconnection rate, is very similar between both models. The best agreement is found in the guide field system, which confines particle better than the coplanar one, where the locality of the moments is violated by the electron bounce motion. It is also shown that, contrary to the common understanding, reconnection is much faster in the guide field system than in the coplanar one. Both models show this tendency, indicating that the phenomenon is driven by ion kinetic effects and not electron ones. (10.1063/1.4792250)
  DOI : 10.1063/1.4792250
• Nonturbulent stabilization of ion fluxes by the fan instability
  
  • Krafft C.
  • Volokitin A.
  Physics Letters A, Elsevier, 2013, 377 (16-17), pp.1189-1198. Resonant interactions between energetic ion fluxes and wave packets they excite through fan instability are studied using self-consistent 3D simulations to explain the nonlinear wave-particle mechanisms at work and to estimate the energy lost by the flux and its sharing between wave emission and particle heating. The saturation of waves and the relaxation of particles are studied over long time periods. The ions are not only diffusing in the waves but are also trapped simultaneously by several potential wells of large amplitude overlapping waves. Estimates of the ion heating energy and rate are given and compared with space observations. (10.1016/j.physleta.2013.03.011)
  DOI : 10.1016/j.physleta.2013.03.011
• Ozone kinetics in low-pressure discharges: vibrationally excited ozone and molecule formation on surfaces
  
  • Marinov Daniil
  • Guerra V.
  • Guaitella Olivier
  • Booth Jean-Paul
  • Rousseau Antoine
  Plasma Sources Science and Technology, IOP Publishing, 2013, 22, pp.055018. A combined experimental and modeling investigation of the ozone kinetics in the afterglow of pulsed direct current discharges in oxygen is carried out. The discharge is generated in a cylindrical silica tube of radius 1 cm, with short pulse durations between 0.5 and 2 ms, pressures in the range 15 Torr and discharge currents ∼40120 mA. Time-resolved absolute concentrations of ground-state atoms and ozone molecules were measured simultaneously in situ, by two-photon absorption laser-induced fluorescence and ultraviolet absorption, respectively. The experiments were complemented by a self-consistent model developed to interpret the results and, in particular, to evaluate the roles of vibrationally excited ozone and of ozone formation on surfaces. It is found that vibrationally excited ozone, O∗ 3, plays an important role in the ozone kinetics, leading to a decrease in the ozone concentration and an increase in its formation time. In turn, the kinetics of O∗ 3 is strongly coupled with those of atomic oxygen and O2(a 1g) metastables. Ozone formation at the wall does not contribute significantly to the total ozone production under the present conditions. Upper limits for the effective heterogeneous recombination probability of O atoms into ozone are established. (10.1088/0963-0252/22/5/055018)
  DOI : 10.1088/0963-0252/22/5/055018
• Redistribution of high energy alpha particles due to sawteeth with partial reconnection
  
  • Farengo R.
  • Ferrari H.E.
  • García-Martínez P.L.
  • Firpo Marie-Christine
  • Ettoumi Wahb
  • Lifschitz A.F.
  Nuclear Fusion, IOP Publishing, 2013, 53, pp.043012. The redistribution of high energy alpha particles due to internal kink modes is studied in plasmas with ITER-like parameters. The exact particle trajectories in the total fields, equilibrium plus perturbation, are calculated. The equilibrium magnetic field is obtained by analytically solving the GradShafranov equation and the perturbed electric and magnetic fields are reconstructed using ideal MHD and the experimental information about the displacement eigenfunction. The (1, 1), (2, 2) and (2, 1) modes are included and the effect of changing their amplitude and frequency is determined. The results show that if the conditions are similar to those reported in Igochine et al (2007 Nucl. Fusion 47 23), the peak density of counter-passing particles decreases between 25% and 40% (depending on the energy); the peak of the trapped particles density shifts outwards by approximately 10% of the minor radius and the total on axis density decreases by more than 25%. This redistribution occurs inside the q = 1 surface. The addition of a (2, 1) mode, which can produce the stochastization of the magnetic field, significantly increases particle redistribution and allows particles to spread beyond the q = 1 surface. Different groups of particles (co-passing, counter-passing, trapped) respond differently to the perturbations. (10.1088/0029-5515/53/4/043012)
  DOI : 10.1088/0029-5515/53/4/043012
• Direction for the future - Successive acceleration of positive and negative ions applied to space propulsion
  
  • Aanesland Ane
  • Bredin Jérôme
  • Popelier Lara
  • Chabert Pascal
  , 2013 (CERN-2013-007).
• Multi-dipolar microwave plasmas and their application to negative ion production
  
  • Béchu Stéphane
  • Soum-Glaude A.
  • Bès A.
  • Lacoste A.
  • Svarnas P.
  • Aleiferis S.
  • Ivanov Jr. A.A.
  • Bacal M.
  Physics of Plasmas, American Institute of Physics, 2013, 20, pp.101601. (10.1063/1.4823466)
  DOI : 10.1063/1.4823466
• Collisionless Plasmas in Astrophysics
  
  • Belmont Gérard
  • Grappin Roland
  • Mottez Fabrice
  • Pantellini F.
  • Pelletier Guy
  , 2013 (ISBN: 978-3-527-41074-3).
• Enhanced Magnetic Compressibility and Isotropic Scale Invariance at Sub-ion Larmor Scales in Solar Wind Turbulence
  
  • Kiyani K. H.
  • Chapman S. C.
  • Sahraoui Fouad
  • Hnat B.
  • Fauvarque O.
  • Khotyaintsev Y. V.
  The Astrophysical Journal, American Astronomical Society, 2013, 763 (1), pp.10. The anisotropic nature of solar wind magnetic turbulence fluctuations is investigated scale by scale using high cadence in situ magnetic field measurements from the Cluster and ACE spacecraft missions. The data span five decades in scales from the inertial range to the electron Larmor radius. In contrast to the inertial range, there is a successive increase toward isotropy between parallel and transverse power at scales below the ion Larmor radius, with isotropy being achieved at the electron Larmor radius. In the context of wave-mediated theories of turbulence, we show that this enhancement in magnetic fluctuations parallel to the local mean background field is qualitatively consistent with the magnetic compressibility signature of kinetic Alfvén wave solutions of the linearized Vlasov equation. More generally, we discuss how these results may arise naturally due to the prominent role of the Hall term at sub-ion Larmor scales. Furthermore, computing higher-order statistics, we show that the full statistical signature of the fluctuations at scales below the ion Larmor radius is that of a single isotropic globally scale-invariant process distinct from the anisotropic statistics of the inertial range. (10.1088/0004-637X/763/1/10)
  DOI : 10.1088/0004-637X/763/1/10
• First demonstration of an asymmetric kinetic equilibrium for a thin current sheet
  
  • Aunai Nicolas
  • Belmont Gérard
  • Smets Roch
  Physics of Plasmas, American Institute of Physics, 2013, 20 (11), pp.110702. The modeling of steady state collisionless asymmetric tangential current layers is a challenging and poorly understood problem. For decades now, this difficulty has been limiting numerical models to approximate equilibria built with locally Maxwellian current layers and theoretical analyses to the very restricted Harris equilibrium. We show how the use of any distribution functions depending only on local macroscopic quantities results in a strong alteration of the current layer internal structure, which converges toward an unpredictable quasi-steady state with emission of ion scale perturbations. This transient can be explained in terms of ion kinetic and electron fluid physics. We demonstrate, for the first time, the validity of an asymmetric kinetic equilibrium model as well as its usability as an initial condition of hybrid kinetic simulations. This offers broad perspectives for the current sheet modeling, for which the early phase of instabilities can be studied within the kinetic formalism. (10.1063/1.4833679)
  DOI : 10.1063/1.4833679
• Sahraoui et al. Reply:
  
  • Sahraoui Fouad
  • Robert Patrick
  • Goldstein M. L.
  • Khotyaintsev Y. V.
  Physical Review Letters, American Physical Society, 2013, 111, pp.149002. A Reply to the Comment by O. Alexandrova, S. D. Bale, and C. Lacombe.
• Electron acceleration to relativistic energies at a strong quasi-parallel shock wave
  
  • Masters A.
  • Stawarz L.
  • Fujimoto M.
  • Schwartz S. J.
  • Sergis N.
  • Thomsen M. F.
  • Retinò Alessandro
  • Hasegawa H.
  • Zieger B.
  • Lewis G. R.
  • Coates A. J.
  • Canu Patrick
  • Dougherty M. K.
  Nature Physics, Nature Publishing Group [2005-....], 2013, 9, pp.164-167. Electrons can be accelerated to ultrarelativistic energies at strong (high Mach number) collisionless shock waves that form when stellar debris rapidly expands after a supernova. Collisionless shock waves also form in the flow of particles from the Sun (the solar wind), and extensive spacecraft observations have established that electron acceleration at these shocks is effectively absent whenever the upstream magnetic field is roughly parallel to the shock-surface normal (quasi-parallel conditions). However, it is unclear whether this magnetic dependence of electron acceleration also applies to the far stronger shocks around young supernova remnants, where local magnetic conditions are poorly understood. Here we present Cassini spacecraft observations of an unusually strong solar system shock wave (Saturn's bow shock) where significant local electron acceleration has been confirmed under quasi-parallel magnetic conditions for the first time, contradicting the established magnetic dependence of electron acceleration at solar system shocks. Furthermore, the acceleration led to electrons at relativistic energies (about megaelectronvolt), comparable to the highest energies ever attributed to shock acceleration in the solar wind. These observations suggest that at high Mach numbers, such as those of young supernova remnant shocks, quasi-parallel shocks become considerably more effective electron accelerators. (10.1038/nphys2541)
  DOI : 10.1038/nphys2541
• Magnetic field and dynamic pressure ULF fluctuations in coronal-mass-ejection-driven sheath regions
  
  • Kilpua E. K. J.
  • Hietala H.
  • Koskinen H. E. J.
  • Fontaine Dominique
  • Turc Lucile
  Annales Geophysicae, European Geosciences Union, 2013, 31, pp.1559-1567. Compressed sheath regions form ahead of interplanetary coronal mass ejections (ICMEs) that are sufficiently faster than the preceding solar wind. The turbulent sheath regions are important drivers of magnetospheric activity, but due to their complex internal structure, relatively little is known on the distribution of the magnetic field and plasma variations in them. In this paper we investigate ultra low frequency (ULF) fluctuations in the interplanetary magnetic field (IMF) and in dynamic pressure (P<SUB>dyn</SUB>) using a superposed epoch analysis of 41 sheath regions observed during solar cycle 23. We find strongest fluctuation power near the shock and in the vicinity of the ICME leading edge. The IMF and P<SUB>dyn</SUB> ULF power have different profiles within the sheath; the former is enhanced in the leading part of the sheath, while the latter is increased in the trailing part of the sheath. We also find that the ICME properties affect the level and distribution of the ULF power in sheath regions. For example, sheath regions associated with strong or fast ICMEs, or those that are crossed at intermediate distances from the center, have strongest ULF power and large variation in the power throughout the sheath region. The weaker or slower ICMEs, or those that are crossed centrally, have in general considerably weaker ULF power with relatively smooth profiles. The strong and abrupt decrease of the IMF ULF power at the ICME leading edge could be used to distinguish the ICME from the preceding sheath plasma. (10.5194/angeo-31-1559-2013)
  DOI : 10.5194/angeo-31-1559-2013
• Modes of underwater discharge propagation in a series of nanosecond successive pulses
  
  • Marinov Ilya
  • Guaitella Olivier
  • Rousseau Antoine
  • Starikovskaia Svetlana
  Journal of Physics D: Applied Physics, IOP Publishing, 2013, 46, pp.464013. Initiation and development of nanosecond electric discharges in deionized water was studied by time-resolved shadowgraphy and emission imaging. Pulses of 410 kV in amplitude, 5 ns rise time and 30 ns duration were applied to a high-voltage (HV) pin-like electrode with the diameter of the pin tip about 2&#956;m. Two distinct bush-like and tree-like modes of the discharge propagation were observed in the same conditions already at the rising slope of HV pulse. Both the modes are supersonic. The probability of finding one of them depends on applied voltage. Bush-mode propagates at 4 kms&#8722;1 at the initial stage; the deposited energy is less than 0.05 mJ. For the tree-like mode, propagation velocity, number of branches and deposited energy show well-prononced dependence on applied voltage. It is suggested that the bush-like discharge ignites in the gaseous cavity, whereas the tree-like discharge propagates in bulk liquid. The role of electrostriciton in the initiation and propagation of two modes is discussed, and comparison with microsecond discharges is given. Transition from bush-like discharge to tree-like mode may occur in successive positive pulse coming 500 ns after initial pulse. (10.1088/0022-3727/46/46/464013)
  DOI : 10.1088/0022-3727/46/46/464013
• Investigation of NO and NO<SUB>2</SUB> adsorption mechanisms on TiO<SUB>2</SUB> at room temperature
  
  • Sivachandiran Loganathan
  • Thévenet Frédéric
  • Gravelat Paul
  • Rousseau Antoine
  Applied Catalysis B: Environmental, Elsevier, 2013, 142-143, pp.196-204. In this study, NO and NO2 adsorption mechanisms on TiO2 at room temperature have been investigated separately. Atmospheric pressure gas phase Fourier Transform Infrared Spectroscopy (FTIR) coupled to adsorption and temperature programmed desorption (TPD) experiments have been used to characterize gas phase and adsorbed phase species. TiO2 coated glass beads packed-bed reactor has been designed and used for NO and NO2 adsorption and storage capacity under dark and gas-flowing conditions at room temperature. For NO adsorption, experimental data suggests that, at room temperature, NO shows no significant adsorption on TiO2. On the other hand NO2 adsorbs in a reactive way by evolving NO in the gas phase. We quantitatively evidenced that, the ratio between consumed NO2, desorbed NO2 by TPD after adsorption and produced NO during NO2 adsorption is 3:2:1, by a qualitative and quantitative analysis performed downstream the reactor. Based on the quantitative analysis, a new NO2 adsorption mechanism on TiO2 at room temperature has been proposed, and validated for various NO2 inlet concentrations. The proposed mechanism is valid on the investigated NO2 inlet concentration range. In addition, it was found that, NO formation time, during NO2 adsorption, is rather controlled by TiO2 surface coverage than NO2 inlet concentration; similarly, adsorption time i.e. surface coverage, significantly modifies the nature of adsorbed species on TiO2 surface. (10.1016/j.apcatb.2013.04.073)
  DOI : 10.1016/j.apcatb.2013.04.073
• Radio frequency current-voltage probe for impedance and power measurements in multi-frequency unmatched loads
  
  • Lafleur Trevor
  • Delattre Pierre-Alexandre
  • Johnson E.V.
  • Booth Jean-Paul
  • Diné Sébastien
  Review of Scientific Instruments, American Institute of Physics, 2013, 84, pp.015001. A broad-band, inline current-voltage probe, with a characteristic impedance of 50 &#937;, is presented for the measurement of voltage and current waveforms, impedance, and power in rf systems. The probe, which uses capacitive and inductive sensors to determine the voltage and current, respectively, can be used for the measurement of single or multi-frequency signals into both matched and unmatched loads, over a frequency range of about 1100 MHz. The probe calibration and impedance/power measurement technique are described in detail, and the calibrated probe results are compared with those obtained from a vector network analyzer and other commercial power meters. Use of the probe is demonstrated with the measurement of power into an unmatched capacitively coupled plasma excited by multi-frequency tailored voltage waveforms. (10.1063/1.4773540)
  DOI : 10.1063/1.4773540
• Frequency dependence of the electrical asymmetry effect in dual-frequency capacitively coupled discharges
  
  • Booth Jean-Paul
  • Lafleur Trevor
  Applied Physics Letters, American Institute of Physics, 2013, 102, pp.154104. Using experimental measurements complemented with particle-in-cell (PIC) simulations, we demonstrate a reduction in the electrical asymmetry effect in capacitively coupled discharges for low excitation frequencies (0.8&#8201;MHz&#8201;<&#8201;f<10&#8201;MHz). These results confirm PIC simulation predictions made by [I. Korolov, Z. Donkó, U. Czarnetzki, and J. Schulze, J. Phys. D: Appl. Phys. 45, 465205 (2012)], where this effect was investigated for dual-frequency discharges in which the driving frequencies are phase-shifted harmonics. Because the reduction in electrical asymmetry is a sensitive function of the secondary electron emission coefficient, we are able to non-invasively estimate this coefficient as 0.035 for argon ions incident on aluminium electrodes. (10.1063/1.4802241)
  DOI : 10.1063/1.4802241
• Non thermal Pasma regeneration of Acetone adsorbed TiO<SUB>2</SUB> Surface
  
  • Sivachandiran Loganathan
  • Thévenet Frédéric
  • Rousseau Antoine
  Plasma Chemistry and Plasma Processing, Springer Verlag, 2013. Improvement of indoor air quality regarding volatile organic compounds (VOCs) requires the development of innovative oxidation processes. This paper investigates the coupling of a metal oxide sorbent with non-thermal plasma (NTP) in an especially designed reactor. TiO2 was selected as model sorbent and acetone was used as model VOC. The analyses of gas phase species at the reactor downstream have been performed using FTIR spectroscopy. In a first step, acetone adsorption on TiO2 surface under dry air was characterized in terms of total amount adsorbed, as well as reversibly and irreversibly adsorbed fractions. Obtained results were compared and discussed with literature in terms of acetone reactive adsorption on TiO2 surface. Mesityloxide was proposed as the major compound in the irreversibly adsorbed fraction. In a second time, acetone saturated TiO2 surface was exposed to NTP surface discharge. Irrespectively of the injected power, <30 % of the initially adsorbed acetone has been recovered as CO, CO2 and desorbed acetone. Finally, thermal desorptions have been performed. They evidenced that (1) NTP treatment modifies the nature of the adsorbed organic species, (2) mineralization rate is considerably improved. Based on desorbed species temporal profile analysis, carboxylates and more especially formates are suggested as major adsorbed species after NTP treatment (Pinj > 0.2 W). This hypothesis has been evaluated and confirmed. This paper finally evidenced that NTP can be used as an efficient pretreatment technique to promote the mineralization of adsorbed acetone for further thermal treatment (10.1007/s11090-013-9463-7)
  DOI : 10.1007/s11090-013-9463-7
• Cluster Observations of Ion-Scale Magnetic Structures and their Coupling with Whistler Waves During the August 17th 2003 Substorm Event
  
  • Tenerani Anna
  • Le Contel Olivier
  • Califano F.
  • Robert Patrick
  • Fontaine Dominique
  • Cornilleau-Wehrlin Nicole
  • Sauvaud J.-A.
  Journal of Geophysical Research Space Physics, American Geophysical Union/Wiley, 2013, 118, pp.6072-6089. We provide evidence of the simultaneous occurrence of large-amplitude, quasi-parallel whistler mode waves and ion-scale magnetic structures, which have been observed by the Cluster spacecraft in the plasma sheet at 17 Earth radii, during a substorm event. It is shown that the magnetic structures are characterized by both a magnetic field strength minimum and a density hump and that they propagate in a direction quasi-perpendicular to the average magnetic field. The observed whistler mode waves are efficiently ducted by the inhomogeneity associated with such ion-scale magnetic structures. The large amplitude of the confined whistler waves suggests that electron precipitations could be enhanced locally via strong pitch angle scattering. Furthermore, electron distribution functions indicate that a strong parallel heating of electrons occurs within these ion-scale structures. This study provides new insights on the possible multiscale coupling of plasma dynamics during the substorm expansion, on the basis of the whistler mode wave trapping by coherent ion-scale structures. (10.1002/jgra.50562)
  DOI : 10.1002/jgra.50562
• First Realistic validation of Plasma Air treatment with QCL-OFCEAS detection of formaldehyde below ppb range
  
  • Guaitella Olivier
  • Barakat Christelle
  • Fasci Eugenio
  • Rousseau Antoine
  • Gorrotxategi Carbajo P.
  • Ventrillard I.
  • Carras M.
  • Maisons G.
  • Romanini D.
  , 2013.