Jan Karsten Trulsen

• Fredriksen, Åshild; Pecseli, Hans & Trulsen, Jan Karsten (2018). A solvable model for the basic properties of a simple magnetized plasma torus. Plasma Physics and Controlled Fusion.  ISSN 0741-3335.  60:085021(8) . doi: 10.1088/1361-6587/aacd2a Full text in Research Archive.
• Omang, Marianne Gjestvold & Trulsen, Jan Karsten (2017). Shock Ignition of Reactive Particles, In Gabi Ben-Dor; Oren Sadot & Ozer Igra (ed.),  30th International Symposium on Shock Waves 1.  Springer.  ISBN 978-3-319-46211-0.  Chapter.  s 771 - 775
• Pecseli, Hans & Trulsen, Jan Karsten (2016). Plankton’s perception of signals in a turbulent environment. Advances in Physics: X.  ISSN 2374-6149.  1(1), s 20- 34 . doi: 10.1080/23746149.2015.1136567
• Bergsaker, Anne Schad; Fredriksen, Åshild; Pecseli, Hans & Trulsen, Jan Karsten (2015). Models for the probability densities of the turbulent plasma flux in magnetized plasmas. Physica Scripta.  ISSN 0031-8949.  90(10) . doi: 10.1088/0031-8949/90/10/108005
• Garcia, Odd Erik; Leer, Egil; Pecseli, Hans & Trulsen, Jan Karsten (2015). Magnetic field-aligned plasma currents in gravitational fields. Annales Geophysicae.  ISSN 0992-7689.  33(3), s 257- 266 . doi: 10.5194/angeo-33-257-2015 Full text in Research Archive.
• Bergsaker, Anne Schad; Fredriksen, Åshild; Pecseli, Hans & Trulsen, Jan Karsten (2014). Analytical models for skewness-kurtosis relations in turbulent transport, In  41st EPS Conference on Plasma Physics.  European Physical Society.  ISBN 2-914771-90-8.  P2.143.
• Børve, Steinar; Sato, Hiroatsu; Pecseli, Hans & Trulsen, Jan Karsten (2014). Low frequency oscillations of the magnetosphere, In  2014 XXXIst URSI General Assembly and Scientific Symposium (URSI GASS 2014).  Curran Associates, Inc..  ISBN 978-14673-5224-6.  Kapittel.  s 3299 - 3301
• Omang, Marianne Gjestvold & Trulsen, Jan Karsten (2014). Multi-phase shock simulations with smoothed particle hydrodynamics (SPH). Shock Waves.  ISSN 0938-1287.  24(5), s 521- 536 . doi: 10.1007/s00193-014-0506-7
• Pecseli, Hans; Trulsen, Jan Karsten & Fiksen, Øyvind (2014). Predator-prey encounter and capture rates in turbulent environments. Limnology and Oceanography.  ISSN 0024-3590.  4, s 85- 105 . doi: 10.1215/21573689-2768717
• Miloch, Wojciech Jacek; Pecseli, Hans & Trulsen, Jan Karsten (2013). Unstable ring-shaped ion distribution functions induced by charge–exchange collisions. Plasma Physics and Controlled Fusion.  ISSN 0741-3335.  55(12) . doi: 10.1088/0741-3335/55/12/124006
• Rekaa, Vegard Lundby; Pecseli, Hans & Trulsen, Jan Karsten (2013). Self-similar space-time evolution of an initial density discontinuity. Physics of Plasmas.  ISSN 1070-664X.  20(7) . doi: 10.1063/1.4816953 Full text in Research Archive.
• Fattorini, L.; Fredriksen, Åshild; Pecseli, Hans; Riccardi, C. & Trulsen, Jan Karsten (2012). Turbulent transport in a toroidal magnetized plasma. Plasma Physics and Controlled Fusion.  ISSN 0741-3335.  54(8) . doi: 10.1088/0741-3335/54/8/085017
• Miloch, Wojciech Jacek; Yaroshenko, V.; Vladimirov, Sergei V.; Pecseli, Hans & Trulsen, Jan Karsten (2012). Spacecraft charging in flowing plasmas; numerical simulations. Journal of Physics: Conference Series.  ISSN 1742-6588.  370 . doi: 10.1088/1742-6596/370/1/012004
• Pecseli, Hans; Trulsen, Jan Karsten & Fiksen, Øyvind (2012). Predator-prey encounter and capture rates for plankton in turbulent environments. Progress in Oceanography.  ISSN 0079-6611.  101(1), s 14- 32 . doi: 10.1016/j.pocean.2011.12.001
• Rekaa, Vegard Lundby; Pecseli, Hans & Trulsen, Jan Karsten (2012). Numerical studies of a plasma diode with external forcing. Physics of Plasmas.  ISSN 1070-664X.  19(8) . doi: 10.1063/1.4747620 Full text in Research Archive.
• Sato, Hiroatsu; Pecseli, Hans & Trulsen, Jan Karsten (2012). Fluctuations in the direction of propagation of intermittent low-frequency ionospheric waves. Journal of Geophysical Research (JGR): Space Physics.  ISSN 2169-9380.  117 . doi: 10.1029/2011JA017242
• Børve, Steinar; Sato, Hiroatsu; Pecseli, Hans & Trulsen, Jan Karsten (2011). Minute-scale period oscillations of the magnetosphere. Annales Geophysicae.  ISSN 0992-7689.  29(4), s 663- 671 . doi: 10.5194/angeo-29-663-2011 Full text in Research Archive.
• Daldorff, Lars Kristen Selberg; Pecseli, Hans; Trulsen, Jan Karsten; Ulriksen, Margit Iren; Eliasson, B. & Stenflo, Lennart (2011). Nonlinear beam generated plasma waves as a source for enhanced plasma and ion acoustic lines. Physics of Plasmas.  ISSN 1070-664X.  18(5) . doi: 10.1063/1.3582084
• Pecseli, Hans & Trulsen, Jan Karsten (2011). Encounter rates and transit time distributions for surfaces moving in turbulent flows. Journal of Physics: Conference Series.  ISSN 1742-6588.  318 . doi: 10.1088/1742-6596/318/5/052034
• Sato, Hiroatsu; Pecseli, Hans & Trulsen, Jan Karsten (2011). Fluctuations in the Direction of Propagation of Low Frequency Ionospheric Waves, In L Ouwehand (ed.),  Proceedings of the 20th ESA Symposium on European Rocket and Balloon Programmes and Related Research.  ESA Communications.  ISBN 978-92-9092-264-3.  Space Weather and Ionosphere.  s 625 - 628
• Krane, Bård; Pecseli, Hans; Sato, Hiroatsu; Trulsen, Jan Karsten & Wernik, A. W. (2010). Low-frequency electrostatic waves in the ionospheric E region. Plasma sources science & technology (Print).  ISSN 0963-0252.  19(3) . doi: 10.1088/0963-0252/19/3/034007
• Miloch, Wojciech Jacek; Rekaa, Vegard Lundby; Pecseli, Hans & Trulsen, Jan Karsten (2010). Ion acoustic double layers forming behind irradiated solid objects in streaming plasmas. Journal of Plasma Physics.  ISSN 0022-3778.  76, s 429- 439 . doi: 10.1017/S002237780999064X
• Pecseli, Hans & Trulsen, Jan Karsten (2010). Transit times in turbulent flows. Physical Review E. Statistical, Nonlinear, and Soft Matter Physics.  ISSN 1539-3755.  81(4) . doi: 10.1103/PhysRevE.81.046310
• Pecseli, Hans; Trulsen, Jan Karsten & Fiksen, Øyvind (2010). Predator-prey encounter rates in turbulent water: Analytical models and numerical tests. Progress in Oceanography.  ISSN 0079-6611.  85(3-4), s 171- 179 . doi: 10.1016/j.pocean.2010.01.002
• Børve, Steinar; Speith, Roland & Trulsen, Jan Karsten (2009). Numerical dissipation in RSPH simulations of astrophysical flows with applications to protoplanetary disks. Astrophysical Journal.  ISSN 0004-637X.  701(2), s 1269- 1282 . doi: 10.1088/0004-637X/701/2/1269
• Miloch, Wojciech Jacek; Vladimirov, Sergei V.; Pecseli, Hans & Trulsen, Jan Karsten (2009). Charging of Dust in the Presence of a Directed Photon Flux: Numerical Simulations. Journal of Plasma and Fusion Research Series.  ISSN 1883-9630.  8, s 265- 268
• Miloch, Wojciech Jacek; Vladimirov, Sergei V.; Pecseli, Hans & Trulsen, Jan Karsten (2009). Charging of insulating and conducting dust grains by flowing plasma and photoemission. New Journal of Physics.  ISSN 1367-2630.  11 . doi: 10.1088/1367-2630/11/4/043005
• Miloch, Wojciech Jacek; Vladimirov, Sergei V.; Pecseli, Hans & Trulsen, Jan Karsten (2009). Interaction of two elongated dust grains in flowing plasmas studied by numerical simulations. Physics of Plasmas.  ISSN 1070-664X.  16(2) . doi: 10.1063/1.3077667
• Omang, Marianne Gjestvold; Christensen, S. O.; Børve, Steinar & Trulsen, Jan Karsten (2009). Height of burst explosions: a comparative study of numerical and experimental results. Shock Waves.  ISSN 0938-1287.  19(2), s 135- 143 . doi: 10.1007/s00193-009-0196-8
• Pecseli, Hans & Trulsen, Jan Karsten (2009). Predator-prey Encounter Rates in Turbulent Environments: Consequences of Inertia Effects and Finite Sizes. AIP Conference Proceedings.  ISSN 0094-243X.  1177, s 85- 95 . doi: 10.1063/1.3253968
• Dyrud, Lars; Krane, B.; Oppenheim, Meers; Pecseli, Hans; Trulsen, Jan Karsten & Wernik, Andrzej (2008). Structure functions and intermittency in ionospheric plasma turbulence. Nonlinear processes in geophysics.  ISSN 1023-5809.  15(6), s 847- 862
• Dyrud, Lars; Wilson, Derek; Børve, Steinar; Trulsen, Jan Karsten; Pecseli, Hans; Close, Sigrid; Chen, Chen & Lee, Yoonjae (2008). Plasma and Electromagnetic Simulations of Meteor Head Echo Radar Reflections. Earth, moon, and planets.  ISSN 0167-9295.  102 . doi: 10.1007/s11038-007-9189-8 Show summary

  Recently, meteor head echo detections from high powered large aperture radars (HPLA) have brought new measurements to bear on the study of sporadic interplanetary meteors. These same observations have demonstrated an ability to observe smaller meteoroids without some of the geometrical restrictions of specular radar techniques. Yet incorporating data from various radar reflection types and from different radars into a single consistent model has proven challenging. We believe this arises due to poorly understood radio scattering characteristics of the meteor plasma, especially in light of recent work showing that plasma turbulence and instability greatly influences meteor trail properties at every stage of evolution. In order to overcome some of the unknown relationships between meteoroid characteristics (such as mass and velocity) and the resulting head echo radar cross-sections (RCS), we present our results on meteor plasma simulations of head echo plasmas using particle in cell (PIC) ions, which show that electric fields strongly influence early stage meteor plasma evolution, by accelerating ions away from the meteoroid body at speeds as large as several kilometers per second. We also present the results of finite difference time domain electromagnetic simulations (FDTD), which can calculate the radar cross-section of the simulated meteor plasma electron distributions. These simulations have shown that the radar cross-section depends in a complex manner on a number of parameters. In this paper we demonstrate that for a given head echo plasma the RCS as a function of radar frequency peaks at sqrt (2*peak plasma frequency) and then decays linearly on a dB scale with increasing radar frequency. We also demonstrate that for a fixed radar frequency, the RCS increases linearly on a dB scale with increasing head echo plasma frequency. These simulations and resulting characterization of the head echo radar cross-section will both help relate HPLA radar observations to meteoroid properties and aid in determining a particular radar facility’s ability to observe various meteoroid populations.

• Dyrud, Lars; Wilson, Derek; Børve, Steinar; Trulsen, Jan Karsten; Pecseli, Hans; Close, Sigrid; Chen, Chen & Lee, Yoonjae (2008). Plasma and electromagnetic wave simulations of meteors. Advances in Space Research.  ISSN 0273-1177.  42, s 136- 142 . doi: 10.1016/j.asr.2007.03.048 Show summary

  Every day billions of meteoroids impact and disintegrate in the Earth’s atmosphere. Current estimates for this global meteor flux vary from 2000-200,000 tons per year, and estimates for the average velocity range between 10 km/s to 70 km/s. The basic properties of this global meteor flux, such as the average mass, velocity, and chemical composition remain poorly constrained. We believe much of the mystery surrounding the basic parameters of the interplanetary meteor flux exists for the following reason, the unknown sampling characteristics of different radar meteor observation techniques, which are used to derive or constrain most models. We believe this arises due to poorly understood radio scattering characteristics of the meteor plasma, especially in light of recent work showing that plasma turbulence and instability greatly influences meteor trail properties at every stage of evolution. We present our results on meteor plasmas simulations of head echoes using particle in cell (PIC) ions, which show that electric fields strongly influence early stage meteor plasma evolution, by accelerating ions away from the meteoroid body. We also present the results of finite difference time domain electromagnetic simulations (FDTD), which can calculate the radar cross section of the simulated meteor plasmas. These simulations have shown that the radar cross section depends in a complex manner on a number of parameters. These include the angle between radar and meteor entry, a large dependence on radar frequency, which shows that for a given meteor plasma size and density, the reflectivity as a function of probing radar frequency varies, but typically peaks below 100 MHz.

• Fredriksen, Åshild; Fredriksen, A.A.; Pecseli, Hans L. & Trulsen, Jan (2008). Crash and recovery of the potential in a toroidal plasma column, as observed by generalized conditional sampling. New Journal of Physics.  ISSN 1367-2630.  10(033030) . doi: 10.1088/1367-2630/10/3/033030 Full text in Research Archive.
• Guio, Patrick; Miloch, Wojciech Jacek; Pecseli, Hans & Trulsen, Jan Karsten (2008). Patterns of sound radiation behind pointlike charged obstacles in plasma flows. Physical Review E. Statistical, Nonlinear, and Soft Matter Physics.  ISSN 1539-3755.  78 . doi: 0.1103/PhysRevE.78.016401
• Guio, Patrick; Miloch, Wojciech Jacek; Pecseli, Hans & Trulsen, Jan Karsten (2008). Sound Radiation from Moving Point-Like Charged Particles in Plasmas. AIP Conference Proceedings.  ISSN 0094-243X.  1061, s 142- 151 . doi: 10.1063/1.3013762
• Miloch, Wojciech Jacek; Pecseli, Hans; Trulsen, Jan Karsten & Vladimirov, Sergei V. (2008). Ion focusing and interaction potential for spherical and rodlike obstacles in a supersonic plasma flow: numerical simulations. AIP Conference Proceedings.  ISSN 0094-243X.  1041, s 287- 288 . doi: 10.1063/1.2997133
• Miloch, Wojciech Jacek; Trulsen, Jan Karsten & Pecseli, Hans (2008). Numerical studies of ion focusing behind macroscopic obstacles in a supersonic plasma flow. Physical Review E. Statistical, Nonlinear, and Soft Matter Physics.  ISSN 1539-3755.  77
• Miloch, Wojciech Jacek; Vladimirov, Sergei V.; Pecseli, Hans & Trulsen, Jan Karsten (2008). Numerical simulations of potential distribution for elongated insulating dust being charged by drifting plasmas. Physical Review E. Statistical, Nonlinear, and Soft Matter Physics.  ISSN 1539-3755.  78 . doi: 10.1103/PhysRevE.78.036411
• Miloch, Wojciech Jacek; Vladimirov, SV; Pecseli, Hans & Trulsen, Jan Karsten (2008). Wake behind dust grains in flowing plasmas with a directed photon flux. Physical Review E. Statistical, Nonlinear, and Soft Matter Physics.  ISSN 1539-3755.  77 . doi: 10.1103/PhysRevE.77.065401
• Børve, Steinar; Speith, Roland; Omang, Marianne Gjestvold & Trulsen, Jan Karsten (2007). Challenges related to particle regularization in SPH, In Alejandro J.C. Crespo; Moncho Gómez-Gesteira; Antonio Souto-Iglesias; Louis Delorme & José María Grassa (ed.),  SPHERIC – Smoothed Particle Hydrodynamics European Research Interest Community: SECOND INTERNATIONAL WORKSHOP.  Aica Ediciones.  ISBN 978-84-690-6159-6.  Kapittel.  s 67 - 70
• Daldorff, Lars K Selberg; Pecseli, Hans & Trulsen, Jan Karsten (2007). Nonlinearly generated plasma waves as a model for enhanced ion acoustic lines in the ionosphere. Geophysical Research Letters.  ISSN 0094-8276.  34 . doi: 10.1029/2007/2007GL031513
• Miloch, Wojciech Jacek; Pecseli, Hans & Trulsen, Jan Karsten (2007). Numerical simulations of the charging of dust particles by contact with hot plasmas. Nonlinear processes in geophysics.  ISSN 1023-5809.  14, s 575- 586
• Omang, Marianne Gjestvold; Børve, Steinar; Christensen, S. O. & Trulsen, Jan Karsten (2007). Symmetry assumptions in SPH, In Alejandro J.C. Crespo; Moncho Gómez-Gesteira; Antonio Souto-Iglesias; Louis Delorme & José María Grassa (ed.),  SPHERIC – Smoothed Particle Hydrodynamics European Research Interest Community: SECOND INTERNATIONAL WORKSHOP.  Aica Ediciones.  ISBN 978-84-690-6159-6.  Kapittel.  s 103 - 106
• Omang, Marianne Gjestvold; Børve, Steinar & Trulsen, Jan Karsten (2007). Shock collisions in 3D using an axi-symmetric regularized smoothed particle hydrodynamics code. Shock Waves.  ISSN 0938-1287.  16, s 467- 475 . doi: 10.1007/s00193-007-0083-0
• Pecseli, Hans & Trulsen, Jan Karsten (2007). Numerical studies of viscous effects for particle fluxes to perfectly absorbing spherical surfaces in turbulent environments: biological applications, In B. J. Geurts; H Clercx & W Uijttewaal (ed.),  Particle-Laden Flows. From Geophysical to Kolmogorov Scales.  Springer.  ISBN 978-1-4020-6217-9.  19.  s 229 - 241
• Pecseli, Hans & Trulsen, Jan Karsten (2007). Turbulent particle fluxes to perfectly absorbing surfaces: a numerical study. Journal of turbulence.  ISSN 1468-5248.  8(42) . doi: 10.1080/14685240701615986
• Børve, Steinar; Omang, Marianne Gjestvold & Trulsen, Jan Karsten (2006). Multidimensional MHD Shock Tests of Regularized Smoothed Particle Hydrodynamics. Astrophysical Journal.  ISSN 0004-637X.  652, s 1306- 1317
• Mann, Jakob; Ott, Søren; Pecseli, Hans & Trulsen, Jan Karsten (2006). Predator-prey encounters studied as relative particle diffusion, In Marcel Ausloos & Michel Dirickx (ed.),  The Logistic map and the Route to Chaos.  Springer.  ISBN 3-540-28366-8.  Kapittel.  s 131 - 146

View all works in Cristin

• Pecseli, Hans & Trulsen, Jan Karsten (2015). Excess statistics with applications to turbulence in marine environments.
• Bergsaker, Anne Schad; Fredriksen, Åshild; Pecseli, Hans & Trulsen, Jan Karsten (2014). Analytical models for skewness-kurtosis relations in turbulent transport.
• Børve, Steinar; Sato, Hiroatsu; Pecseli, Hans & Trulsen, Jan Karsten (2014). LOW FREQUENCY OSCILLATIONS OF THE MAGNETOSPHERE.
• Miloch, Wojciech Jacek; Pecseli, Hans & Trulsen, Jan Karsten (2013). Kinetic plasma instabilities due to charge exchange collisions.
• Miloch, Wojciech Jacek; Pecseli, Hans & Trulsen, Jan Karsten (2013). Numerical simulations of kinetic plasma instabilities induced by charge exchange collisions.
• Pecseli, Hans; Miloch, Wojciech Jacek & Trulsen, Jan Karsten (2013). Kinetically unstable velocity distributions formed by charge exchange collisions with drifting ions.
• Pecseli, Hans; Trulsen, Jan Karsten & Fiksen, Øyvind (2013). Predator-prey encounter and capture rates in turbulent environments.
• Miloch, Wojciech Jacek; Pecseli, Hans & Trulsen, Jan Karsten (2012). Numerical simulations of collisional partially ionized plasmas. Show summary

  The stability of plasma can be related to the shape of its velocity distributions [1]. For instance, for ionospheric plasmas it is argued that ion velocity distributions can deviate from Maxwellian giving rise to plasma instabilities [2, 3]. In order to study the possibility for losscone instabilities in collisional plasmas with Hall currents, we have modified our particle-in-cell code to include collisional effects in a magentized plasma. We have the option of adding a DCelectric field in the direction perpendicular to the magnetic field. We present the results from the self-consistent three dimensional simulations of the plasma velocity distributions under such conditions. In this study we investigate the role of collisions with the neutral component for the evolution and stability of the velocity distributions. In the most general case, we include elastic electron-neutral collisions, as well as charge exchange and elastic ion-neutral collisions. The results will be important for a detailed understanding of low frequency ionospheric plasmas, for instance in the E-region. References [1] O. Penrose, Phys. Fluids 3, 258 (1960). [2] J.-P. St.-Maurice, E. Winkler, and A. M. Hamza, J. Geophys. Res. 99, 19527 (1994) [3] J.-P. St.-Maurice and R. W. Schunk, Planet. Space Sci. 25, 243 (1977

• Rekaa, Vegard Lundby; Pecseli, Hans & Trulsen, Jan Karsten (2012). Numerical studies of a plasma diode with external forcings. Show summary

  With reference to laboratory studies we analyze the dynamics of a plasma diode under external forcing. Assuming a strong axial magnetic field, the problem is analyzed in one spatial dimension by a Particle in Cell code. The cathode is assumed to be operated in electron rich conditions, supplying an abundance of electrons. We compare different forcing schemes with the results obtained by solving the van der Pol equation. In one method of forcing we apply an oscillation in addition to the DC end plate bias, and consider both amplitude and frequency variations. An alternative method of perturbation consists of modelling an absorbing grid at some internal position. Also in this case we can have a constant frequency with varying amplitude, or alternatively an oscillation with chirped frequency but constant amplitude. We find that the overall features of the forced van der Pol equation are recovered, but the details in the plasma response require more attention to the harmonic responses, requiring extensions of the model equation. The analysis is extended by introducing collisional effects, where we emphasize charge exchange collisions of ions, since these processes usually have the largest cross sections. Charge exchange collisions give significant modifications of the diode performance when the effects are compared with the influence of elastic electron-neutral and ion-neutral collisions with the same collisional mean free paths.

• Sato, Hiroatsu; Børve, Steinar; Pécseli, Hans & Trulsen, Jan Karsten (2012). Minute-scale period oscillations of the magnetosphere. Show summary

  Oscillations with periods on the order of 5–10 min have been observed by instrumented spacecrafts in the Earth’s magnetosphere. These oscillations often follow sudden impacts related to coronal mass ejections. It is demonstrated that a simple model is capable of explaining the basic properties of these oscillations and give scaling laws for their basic characteristics in terms of the basic parameters of the problem. The period of the oscillations and their anharmonic nature, in particular, are accounted for. The model has no free adjustable numerical parameters. We use measurable quantities as inputs (such as Solar wind momentum density), and our results can be seen as an effort to predict some dynamic properties of magnetospheres on the basis of measurable steady state characteristics. A simple test of the model is found by comparing its prediction of the Earth-Magnetopause distance with observed values. The general results agree with observations. The analysis is supported by numerical simulations solving the Magneto-Hydro-Dynamic (MHD) equations in two spatial dimensions, where we let a solar wind interact with a magnetic dipole representing a magnetized Earth. Two tilt-angles of the magnetic dipole axis were considered. We observed the formation of a magnetosheath, with the magnetopause at a distance corresponding well to the analytical results. Sudden pulses in the model solar wind sets the model magnetosphere into damped oscillatory motions and quantitatively good agreement with the analytical results is found. The models seem to be robust, and give good qualitative agreement with the numerical simulations for a range of parameters.

• Sato, Hiroatsu; Pecseli, Hans; Børve, Steinar & Trulsen, Jan Karsten (2012). Dynamic models for magnetospheric oscillations on the minute scale.
• Trulsen, Jan Karsten & Omang, Marianne Gjestvold (2012). Shock propagation through bounded dust clouds.
• Miloch, Wojciech Jacek; Yaroshenko, V.; Vladimirov, Sergei V.; Pecseli, Hans & Trulsen, Jan Karsten (2011). Spacecraft charging in space and ionospheric plasma; numerical simulations.
• Omang, Marianne Gjestvold; Christensen, Svein Olav; Hauge, Knut Ove & Trulsen, Jan Karsten (2011). A numerical and experimental study on charge geometries.
• Pecseli, Hans & Trulsen, Jan Karsten (2011). Encounter rates and transit time distributions for surfacesmoving in turbulent flows. Show summary

  Reaction rates as relevant for many chemical processes as well as a number of biological applications depend on encounter rates of reacting elements and the probability of a reaction occurring given an encounter. Turbulent mixing can enhance the encounter rate, but it can also have adverse effects by reducing the reaction probability. We model the probability for a reaction by letting it depend on the time available, i.e. the time spent by of reacting particles within some given interaction volume. We study the problems by numerical simulations where we analyze the statistics of the motion of passively convected point particles in turbulent flows. The database used is obtained by direct numerical solution of the Navier-Stokes equation. We estimate the encounter rates and also the probability distribution of the transit times of particles through reference volumes with given forms and sizes. A selected position within the reference volume is moving self consistently with the local flow velocity, thus determining the motion of the entire surface. The transit time is defined as the interval between entrance and exit times of surrounding particles convected through the volume by the turbulent motions. Scale sizes in the inertial as well as in the viscous subranges of the turbulence are considered. Simple, and seemingly universal, scaling laws are obtained for the encounter rate as well as the probability density of the transit times in terms of the basic properties of the turbulent flow and the geometry. In the present formulation, the results of the analysis are relevant for chemical reactions, but also for understanding details of the feeding rate of micro-organisms in turbulent waters, for instance.

• Rekaa, Vegard Lundby; Pecseli, Hans & Trulsen, Jan Karsten (2011). Numerical simulations of anomalous resistivity in the ion acoustic and Buneman regime.
• Omang, Marianne Gjestvold; Christensen, S. O.; Børve, Steinar & Trulsen, Jan Karsten (2010). Blast wave generation and propagation.
• Miloch, Wojciech Jacek; Pecseli, Hans & Trulsen, Jan Karsten (2009). Interactions of two objects in flowing plasmas studied by numerical simulations.
• Miloch, Wojciech Jacek; Pecseli, Hans & Trulsen, Jan Karsten (2009). Ion focusing behind finite size objects in flowing plasmas; numerical studies in two and three dimensions.
• Miloch, Wojciech Jacek; Pecseli, Hans & Trulsen, Jan Karsten (2009). Numerical studies of ion focusing in streaming plasmas; two and three dimensions.
• Pecseli, Hans; Trulsen, Jan Karsten & Fiksen, Øyvind (2009). Predators in turbulent waters: an analytical model and a numerical test.
• Børve, Steinar; Omang, Marianne; Trulsen, Jan Karsten & Bjerke, Audun (2008). A Comparative Study of ANSYS AUTODYN and RSPH Simulations of Blast Waves.
• Dyrud, Lars; Krane, Bård; Oppenheim, Mers; Pecseli, Hans; Trulsen, Jan Karsten & Wernik, A. W. (2008). Structure functions and intermittency in ionospheric plasma turbulence.
• Fredriksen, Åshild; Pecseli, Hans & Trulsen, Jan Karsten (2008). Crash and recovery of the potential in a toroidal plasma column, as observed by generalized conditional sampling.
• Guio, Patrick; Miloch, Wojciech Jacek; Pecseli, Hans & Trulsen, Jan Karsten (2008). Ion-sound from charged obstacles in a plasma flow.
• Guio, Patrick; Miloch, Wojciech Jacek; Pecseli, Hans & Trulsen, Jan Karsten (2008). Sound radiation from moving point-like charged particles in plasmas.
• Miloch, Wojciech Jacek; Pecseli, Hans & Trulsen, Jan Karsten (2008). Wake formation behind elongated insulating object in drifting plasmas: numerical simulations.
• Miloch, Wojciech Jacek; Pecseli, Hans; Trulsen, Jan Karsten & Vladimirov, Sergei V. (2008). Ion focusing and interaction potential for sphericaland rodlike obstacles in a supersonic plasma flow: numerical simulations.
• Miloch, Wojciech Jacek; Pecseli, Hans; Trulsen, Jan Karsten & Vladimirov, Sergei V. (2008). Numerical simulations of interactions between solid surfaces (dust grains) and plasmas.
• Miloch, Wojciech Jacek; Vladimirov, Sergei V.; Pecseli, Hans & Trulsen, Jan Karsten (2008). Charge and potential distributions on and around elongated dust grains in flowing plasmas: numerical simulations.
• Miloch, Wojciech Jacek; Vladimirov, Sergei V.; Pecseli, Hans & Trulsen, Jan Karsten (2008). Charging and wake of dust grains in supersonic plasma flows: numerical simulations.
• Miloch, Wojciech Jacek; Vladimirov, Sergei V.; Pecseli, Hans & Trulsen, Jan Karsten (2008). Charging of dust grains in flowing plasmas with a directed photon flux: numerical simulations.
• Miloch, Wojciech Jacek; Vladimirov, Sergei V.; Pecseli, Hans & Trulsen, Jan Karsten (2008). Charging of dust in the presence of a directed photon flux: numerical simulations.
• Miloch, Wojciech Jacek; Vladimirov, Sergei V.; Pecseli, Hans & Trulsen, Jan Karsten (2008). Charging of insulating grains in flowing plasmas with a directed photon flux.
• Miloch, Wojciech Jacek; Vladimirov, Sergei V.; Pecseli, Hans & Trulsen, Jan Karsten (2008). Interaction potential between two elongated dust grains in flowing plasmas: numerical simulations.
• Miloch, Wojciech Jacek; Vladimirov, Sergei V.; Pecseli, Hans & Trulsen, Jan Karsten (2008). Numerical simulations of the charging and wake of dust grains in flowing plasmas.
• Miloch, Wojciech Jacek; Vladimirov, Sergei V.; Pecseli, Hans & Trulsen, Jan Karsten (2008). The charging of dust grains and the wake formation studied by numerical simulations.
• Miloch, Wojciech Jacek; Vladimirov, Sergei V.; Pecseli, Hans & Trulsen, Jan Karsten (2008). Wake formation behind elongated insulating dust grains in drifting plasmas: numerical simulations.
• Omang, Marianne; Børve, Steinar & Trulsen, Jan Karsten (2008). Numerical Simulations of Blast Wave Propagation in Underground Facilities.
• Omang, Marianne; Christensen, S. O.; Børve, Steinar & Trulsen, Jan Karsten (2008). Numerical Simulations of Blast Waves from Spherical and Cylindrical Charges.
• Pecseli, Hans & Trulsen, Jan Karsten (2008). Planktonic contact and capture rates in turbulent environments. Show summary

  The motion of plankton in turbulent environments is studied by numerical simulations, where point particles are moving in a flow described by Navier-Stokes equation. Parts of the results are supported also by observations from a controlled laboratory experiment, where approximately homogeneous and isotropic turbulence can be generated by two moving grids. We find that the contact rates of passively moving prey and predators with a spherical capture volume follow seemingly universal scaling laws in terms of the specific turbulent dissipation rate and the radius in the capture volume. For radii smaller than or comparable to the Kolmogorov-scale, also the viscosity enters the scaling laws. The models are extended to cover also non-spherical capture volumes. The average capture rate of prey is modelled by a product of the encounter rate and a capture probability, where the basic parameter for the capture is identified as the time duration of the encounter. Also the transit time of passively moving prey through the volume of interception is measured, and universal scaling laws for its probability density are estimated. Parameterizing the capture probability for given transit times, we obtain an estimate of the average capture rate of prey, indicating that small or moderate levels of turbulence are advantageous for the capture by increasing the contact rate, while strong turbulence is a disadvantage by reducing the capture probability due to the short transit times. We demonstrate how self induced cruising motions of predators can be included in the models, and obtain a parameterized expression for the average capture rate that includes also this effect.

• Miloch, Wojciech Jacek; Pecseli, Hans & Trulsen, Jan Karsten (2007). Numerical simulations of interactions of warm plasmas and a dust-grain. Show summary

  Results from numerical simulations of the interaction between a warm plasma and individual dust particles are reported. The analysis is carried out in two spatial dimensions, using a particle-in-cell (PIC) numerical code, considering conducting as well as insulating materials for the dust. For macroscopic dust particles in streaming plasmas, we observe the development of an electric dipole moment associated with the particles. The strength of this dipole moment is very different for conducting and insulating materials, and its direction is opposite for the two cases. For supersonic flows we note the formation of a Mach-cone, with properties in agreement with analytical results, in particular also concerning the effects of Landau damping.

• Miloch, Wojciech Jacek; Pecseli, Hans & Trulsen, Jan Karsten (2007). Numerical simulations of the charging of dust particles by contact with warm plasmas.
• Miloch, Wojciech Jacek; Pecseli, Hans & Trulsen, Jan Karsten (2007). PIC simulations of dusty plasmas.
• Miloch, Wojciech Jacek; Trulsen, Jan Karsten & Pecseli, Hans (2007). Interactions between warm, drifting plasmas and dust grains, studied by numerical simulations.
• Pecseli, Hans; Dyrud, Lars; Oppenheim, Meers; Wernik, Andrzej & Trulsen, Jan Karsten (2007). Low-frequency electrostatic waves in the ionospheric E region: a comparison of rocket observations and numerical simulations. Show summary

  Low frequency electrostatic waves in the lower parts of the ionosphere are studied by a comparison of observations by instrumented rockets and of results from numerical simulations [1,2]. Particular attention is given to the spectral properties of the waves [1]. On the basis of a good agreement between the observations and the simulations, it can be argued that the most important nonlinear dynamics can be accounted for in a two-dimensional numerical model, referring to a plane perpendicular to a locally homogeneous magnetic field. It does not seem necessary to take into account turbulent fluctuations or motions in the neutral gas component. The numerical simulations explain the observed strongly intermittent nature of the fluctuations: secondary instabilities develop on the large scale gradients of the largest amplitude waves, and the small scale dynamics is strongly influenced by these secondary instabilities. We compare potential variations obtained at a single position in the numerical simulations with two point potential-difference signals, where the latter is the adequate representation for the data obtained by instrumented rockets. We can demonstrate a significant reduction in the amount of information concerning the plasma turbulence when the latter signal is used for analysis [2]. In particular we show that the bicoherence estimate is strongly affected. The conclusions have implications for studies of low frequency ionospheric fluctuations in the E and F regions by instrumented rockets, and also for other methods relying on difference measurements, using two probes with large separation. The analysis also resolves a long standing controversy concerning the supersonic phase velocities of these cross-field instabilities being observed in laboratory experiments. In a general context we might argue that our results illustrate the necessity of being particularly careful when comparing analytical and experimental results when the latter are obtained by instrumented space-crafts. [1] B. Krane, H.L. Pécseli, J. Trulsen and F. Primdahl, Spectral properties of low-frequency electrostatic waves in the ionospheric E-region. J. Geophys. Res. 105, 10,585-10,602, 2000 [2] L. Dyrud, B. Krane, M. Oppenheim, H.L. Pécseli, K. Schlegel, J. Trulsen and A.W. Wernik, Low-frequency electrostatic waves in the ionospheric E region: a comparison of rocket observations and numerical simulations. Ann. Geophysicae, 24, 2959-2979, 2006

• Pecseli, Hans & Trulsen, Jan Karsten (2007). Numerical simulations of predator-prey encounters in turbulent environments: effects of viscosity and fields of view.
• Pecseli, Hans & Trulsen, Jan Karsten (2007). Numerical simulations of predator-prey encounters in turbulent environments: effects of viscosity and fields of view. Show summary

  The motion of aquatic micro-organisms is modeled by a numerical simulation with realistic Reynolds numbers. Particular attention is given to the effect of viscosity for the case where the capture range of a micro-organism is comparable to or smaller than the Kolmogorov length-scale. It is demonstrated that the viscous sub-range is particularly important for realistic values of capture ranges and turbulence parameters in nature. We obtain an empirical expression for the prey flux to a predator with spherical surface of interception, and demonstrate its applicability for a wide range of radii and two values of turbulence Reynolds numbers. The range of validity of this result covers the viscous as well as the universal sub-ranges. It is demonstrated that for realistic conditions the result remains valid also for conical contact volumes, apart from a scaling factor which depends on the opening angle of the cone. In spite of significant differences in the velocity structure functions for universal and viscous sub-ranges, we find a surprisingly small change in the scaling law for the average prey flux to small predators as the capture range changes from the universal to the viscous sub-range.

• Diomede, P.; Børve, Steinar; Longo, Savino; Miloch, Wojciech; Pecseli, Hans & Trulsen, Jan Karsten (2006). Kinetic simulation of plasma injection in neutral gas.
• Dyrud, Lars; Lee, Yoonjae; Børve, Steinar; Trulsen, Jan Karsten & Pecseli, Hans (2006). Plasma and electromagnetic wave simulations of meteors. Show summary

  Every day billions of meteoroids impact and disintegrate in the Earth’s atmosphere. Current estimates for this global meteor flux vary from 2000-200,000 tons per year, and estimates for the average velocity range between 10 km/s to 70 km/s. The basic properties of this global meteor flux, such as the average mass, velocity, and chemical composition remain poorly constrained. We believe much of the mystery surrounding the basic parameters of the interplanetary meteor flux exists for the following reasons, the unknown sampling characteristics of different radar meteor observation techniques, which are used to derive or constrain most models. We believe this arises due to poorly understood radio scattering characteristics of the meteor plasma, especially in light of recent work showing that plasma turbulence and instability greatly influences meteor trail properties at every stage of evolution. We present our results on meteor plasmas simulations of head echoes using PIC ions, which show that electric fields strongly influence early stage meteor plasma evolution, by accelerating ions away from the meteoroid body. We also present the results of time domain electromagnetic simulations (FDTD) which can calculate the radar cross section of the simulated meteor plasmas. These simulations have shown that the radar cross section depends in a complex manner on a number of parameters. These include the angle between radar and meteor entry, a large dependence on radar frequency, which shows that for a given meteor plasma size and density, the peak reflectivity for the meteor varies but is usually less then 100 Mhz. The simulations also show that the majority of the reflection occurs at the very central high density portion of the meteor, a region that is often much smaller then the radar wavelength.

• Miloch, Wojciech Jacek; Pecseli, Hans & Trulsen, Jan Karsten (2006). Numerical simulations of interactions between warm plasmas and a dust-grain.

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