426 Alfven PPTs View free & download

Nonlinear Alfven waves in dusty astrophysical plasmas PowerPoint PPT Presentation

Nonlinear Alfven waves in dusty astrophysical plasmas - Plasma Kinetics around a Dust Grain in an Ion Flow N F Cramer and S V Vladimirov, School of Physics, University of Sydney, S A Maiorov, General Physics Institute ...

Plasma Kinetics around a Dust Grain in an Ion Flow N F Cramer and S V Vladimirov, School of Physics, University of Sydney, S A Maiorov, General Physics Institute ...

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Kinetic Alfven waves in space plasmas by Yuriy Voitenko PowerPoint PPT Presentation

Kinetic Alfven waves in space plasmas by Yuriy Voitenko - Kinetic Alfv n turbulence driven by MHD turbulent cascade Yuriy Voitenko & Space Physics team Belgian Institute for Space Aeronomy, Brussels, Belgium

Kinetic Alfv n turbulence driven by MHD turbulent cascade Yuriy Voitenko & Space Physics team Belgian Institute for Space Aeronomy, Brussels, Belgium

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Nonlinear effects on torsional Alfven waves PowerPoint PPT Presentation

Nonlinear effects on torsional Alfven waves - Nonlinear effects on torsional Alfven waves S. Vasheghani Farahani, V.M. Nakariakov, T. Van Doorsselaere, E. Verwichte Why isn't the plane wave model sufficient to ...

Nonlinear effects on torsional Alfven waves S. Vasheghani Farahani, V.M. Nakariakov, T. Van Doorsselaere, E. Verwichte Why isn't the plane wave model sufficient to ...

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Turbulent Heating in Goldreich-Sridhar Shear Alfven Cascade - Turbulent Heating in GoldreichSridhar Shear Alfven Cascade

Turbulent Heating in GoldreichSridhar Shear Alfven Cascade

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SOLAR MICROWAVE DRIFTING SPIKES AND SOLITARY KINETIC ALFVEN WAVES - SOLAR MICROWAVE DRIFTING SPIKES AND SOLITARY KINETIC ALFVEN WAVES

SOLAR MICROWAVE DRIFTING SPIKES AND SOLITARY KINETIC ALFVEN WAVES

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Phase Dynamics of Alfven Intermittent Turbulence in the Heliosphere PowerPoint PPT Presentation

Phase Dynamics of Alfven Intermittent Turbulence in the Heliosphere - Spatiotemporal chaos can be described in terms of UPOs. Christiansen et al., Nonlinearity 1997 ... Spatiotemporal phase dynamics of Alfven waves. Chian et al. ...

Spatiotemporal chaos can be described in terms of UPOs. Christiansen et al., Nonlinearity 1997 ... Spatiotemporal phase dynamics of Alfven waves. Chian et al. ...

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Plasmas in Laboratory and Astrophysics Alfven Wave Turbulence and Heating. PowerPoint PPT Presentation

Plasmas in Laboratory and Astrophysics Alfven Wave Turbulence and Heating. - Plasmas in Laboratory and Astrophysics. Alfven Wave Turbulence and Heating. ... fine scale mixing - jagged f. Less collisions more jagged f. Entropy production ...

Plasmas in Laboratory and Astrophysics. Alfven Wave Turbulence and Heating. ... fine scale mixing - jagged f. Less collisions more jagged f. Entropy production ...

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UHECR Acceleration via Alfven Wave Induced Plasma Wakefield PowerPoint PPT Presentation

UHECR Acceleration via Alfven Wave Induced Plasma Wakefield - Alfven Mach Number = 2.3. Magnetic Field Evolution. Magnetic Field Evolution ... The Alfven Mach number is the ratio V/Va. In other words the piston is ...

Alfven Mach Number = 2.3. Magnetic Field Evolution. Magnetic Field Evolution ... The Alfven Mach number is the ratio V/Va. In other words the piston is ...

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Ion Heating by Alfven Waves and Reconnection in NSTX PowerPoint PPT Presentation

Ion Heating by Alfven Waves and Reconnection in NSTX - Second example we have clear evidence of heating and at ... dB2 1/2modes/B dn2 1/2modes/n 1-1.5 % Difficult to push ion heating power to significant level. ...

Second example we have clear evidence of heating and at ... dB2 1/2modes/B dn2 1/2modes/n 1-1.5 % Difficult to push ion heating power to significant level. ...

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Polarization intermittency in Alfvenic turbulence. PowerPoint PPT Presentation

Polarization intermittency in Alfvenic turbulence. - Therefore there is a dynamic alignment of otherwise independent elsasser vectors ... Alignment have an intermittent nature, being stronger in regions with large wave ...

Therefore there is a dynamic alignment of otherwise independent elsasser vectors ... Alignment have an intermittent nature, being stronger in regions with large wave ...

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AT Target Plasma Studies: Alfven Wave Cascades and RS Discharge with ICRH and Ip Ramp PowerPoint PPT Presentation

AT Target Plasma Studies: Alfven Wave Cascades and RS Discharge with ICRH and Ip Ramp - ... similar to the JT-60U and JET results which have been interpreted in terms of ... requires installation of additional magnetic loop(s) during the next major break ...

... similar to the JT-60U and JET results which have been interpreted in terms of ... requires installation of additional magnetic loop(s) during the next major break ...

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Initial 3D MHD Simulation of CHI Plasma Xianzhu Tang Plasma Theory Group, Theoretical Division LANL xtang@lanl.gov PowerPoint PPT Presentation

Initial 3D MHD Simulation of CHI Plasma Xianzhu Tang Plasma Theory Group, Theoretical Division LANL xtang@lanl.gov - Nonlinearly implicit time stepping scheme attractive for long time simulation of ... 2. 2D run of 500 Alfven time, followed by 3D run of 1800 Alfven time. 12/7 ...

Nonlinearly implicit time stepping scheme attractive for long time simulation of ... 2. 2D run of 500 Alfven time, followed by 3D run of 1800 Alfven time. 12/7 ...

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Pr - Alfven waves (Alfven-Ion-Cyclotron waves, AIC) are widely observed downstream of ... Dynamic spectrogram (Wavelet transforms of Bn) (II) : Field aligned current tubes ...

Alfven waves (Alfven-Ion-Cyclotron waves, AIC) are widely observed downstream of ... Dynamic spectrogram (Wavelet transforms of Bn) (II) : Field aligned current tubes ...

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POLAR Scientists Discover the Energy Source Powering the Aurora PowerPoint PPT Presentation

POLAR Scientists Discover the Energy Source Powering the Aurora - Measurements from POLAR in the geomagnetic tail show that energy is transmitted towards the Earth along magnetic ... solar wind. Alfven waves have been ...

Measurements from POLAR in the geomagnetic tail show that energy is transmitted towards the Earth along magnetic ... solar wind. Alfven waves have been ...

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Turbulent Reconnection in a Partially Ionized Gas PowerPoint PPT Presentation

Turbulent Reconnection in a Partially Ionized Gas - Ambipolar Drift - this has a modest effect on reconnection. ... like the Alfven speed of the reconnecting field component - set by the energy ...

Ambipolar Drift - this has a modest effect on reconnection. ... like the Alfven speed of the reconnecting field component - set by the energy ...

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Auroral energy flow budget as a function of altitude: How does energy arrive from the magnetosphere? PowerPoint PPT Presentation

Auroral energy flow budget as a function of altitude: How does energy arrive from the magnetosphere? - Comprehensive statistical study using 5 years of Polar data (EFI MFE) ... A. Olsson, J. Hanasz, C.T. Russell, H. Laakso and J.C. Samson, Different Alfven ...

Comprehensive statistical study using 5 years of Polar data (EFI MFE) ... A. Olsson, J. Hanasz, C.T. Russell, H. Laakso and J.C. Samson, Different Alfven ...

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Simulations of Energetic Particle Modes PowerPoint PPT Presentation

Simulations of Energetic Particle Modes - Need to study possible new features of beam-driven Alfven modes ... In this work we investigate stability and nonlinear dynamics ... burst at the same time. ...

Need to study possible new features of beam-driven Alfven modes ... In this work we investigate stability and nonlinear dynamics ... burst at the same time. ...

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Global Control of Merging by the IMF: Cluster Observations of Dawnside Flank Magnetopause Reconnection PowerPoint PPT Presentation

Global Control of Merging by the IMF: Cluster Observations of Dawnside Flank Magnetopause Reconnection - Global Control of Merging by the IMF: Cluster Observations of Dawnside Flank ... Note that the average Mach numbers during the jet intervals are super-Alfvenic. ...

Global Control of Merging by the IMF: Cluster Observations of Dawnside Flank ... Note that the average Mach numbers during the jet intervals are super-Alfvenic. ...

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NSTX research and the connection to community needs PowerPoint PPT Presentation

NSTX research and the connection to community needs - ... for and how to manage the control development effort (Gates, Mueller, Bell) ... ions with large orbits; Alfven eigenmodes and turbulence with Vfast/VA 1 ...

... for and how to manage the control development effort (Gates, Mueller, Bell) ... ions with large orbits; Alfven eigenmodes and turbulence with Vfast/VA 1 ...

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Plasma Electrodynamics PowerPoint PPT Presentation

Plasma Electrodynamics - Fluid velocity : not the same with the velocity of guiding centers. For ... 'Whistler' wave, becoming shear Alfven R-wave. at low frequency, vp -- vA as -- 0. ...

Fluid velocity : not the same with the velocity of guiding centers. For ... 'Whistler' wave, becoming shear Alfven R-wave. at low frequency, vp -- vA as -- 0. ...

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Long Term Simulations of Astrophysical Jets Energy Structure and QuasiPeriodic Ejection PowerPoint PPT Presentation

Long Term Simulations of Astrophysical Jets Energy Structure and QuasiPeriodic Ejection - ... the cubic interpolated propagation (CIP) method (Yabe &Aoki ... 1-Torsional Alfven wave is generated at the disk surface and propagates up into the corona ...

... the cubic interpolated propagation (CIP) method (Yabe &Aoki ... 1-Torsional Alfven wave is generated at the disk surface and propagates up into the corona ...

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ICS9 Session 2: SUBSTORMS : ONSET, PROPAGATION PowerPoint PPT Presentation

ICS9 Session 2: SUBSTORMS : ONSET, PROPAGATION - Breakup always corresponds (in space&time) to tailward Alfvenic outflows (XNL reconnection? ... deceleration of incoming electrons crossing the separatrix. ...

Breakup always corresponds (in space&time) to tailward Alfvenic outflows (XNL reconnection? ... deceleration of incoming electrons crossing the separatrix. ...

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Recent Progress in Astroparticle Physics PowerPoint PPT Presentation

Recent Progress in Astroparticle Physics - Some shocks are very efficient accelerators 50% Magnetic amplification mG- mG ... Most CRs decompress until. expansion sub-Alfvenic. Pulsars, stars more complex! ...

Some shocks are very efficient accelerators 50% Magnetic amplification mG- mG ... Most CRs decompress until. expansion sub-Alfvenic. Pulsars, stars more complex! ...

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Current Sheet Formation Along Magnetic Separators in 3d PowerPoint PPT Presentation

Current Sheet Formation Along Magnetic Separators in 3d - Boundary motion drives field singular. equilibrium via repeated Alfven wave ... Vorticity. sheet @ sep'x. S Merging height: No motion across sep'x S ...

Boundary motion drives field singular. equilibrium via repeated Alfven wave ... Vorticity. sheet @ sep'x. S Merging height: No motion across sep'x S ...

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Young Stars I,II PowerPoint PPT Presentation

Young Stars I,II - Essentially ALL protostellar cloud magnetic flux must be lost during star ... collimation. Alfven surface. Accretion leads to ejection. dM/dt (wind) = 0.1 dM/dt (acc) ...

Essentially ALL protostellar cloud magnetic flux must be lost during star ... collimation. Alfven surface. Accretion leads to ejection. dM/dt (wind) = 0.1 dM/dt (acc) ...

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High R asymmetry seen in 24 atm D3He shots PowerPoint PPT Presentation

High R asymmetry seen in 24 atm D3He shots - D. Casey (G) N. Sinenian (G) LLNL. P. Amendt. O. Landen. J. Rygg. R. Town. GA. C. Back. J. Kilkenny ... 1/2 ~ 5 ns (Sweet-Parker) Where: Alfven ~ L/ vA ~ 1 ns ...

D. Casey (G) N. Sinenian (G) LLNL. P. Amendt. O. Landen. J. Rygg. R. Town. GA. C. Back. J. Kilkenny ... 1/2 ~ 5 ns (Sweet-Parker) Where: Alfven ~ L/ vA ~ 1 ns ...

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Auroral energy flow budget as a function of altitude: How does energy arrive from the magnetosphere? - Auroral energy flow budget as a function of altitude: ... Harri Laakso, ESA/ESTEC. Nikolai Tsyganenko, NASA/GSFC. Lars Blomberg, KTH/Stockholm ...

Auroral energy flow budget as a function of altitude: ... Harri Laakso, ESA/ESTEC. Nikolai Tsyganenko, NASA/GSFC. Lars Blomberg, KTH/Stockholm ...

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Nonresonant pitch angle scattering of electrons and breakdown of adiabatic invariance: Modeling PowerPoint PPT Presentation

Nonresonant pitch angle scattering of electrons and breakdown of adiabatic invariance: Modeling - Nonresonant pitch angle scattering of electrons and breakdown of adiabatic invariance: Modeling Surja Sharma, Alexey Karavaev, Erin Lynch, Nail Gumerov, Xi Shao ...

Nonresonant pitch angle scattering of electrons and breakdown of adiabatic invariance: Modeling Surja Sharma, Alexey Karavaev, Erin Lynch, Nail Gumerov, Xi Shao ...

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Integrated Simulations of Energetic Particle-driven PowerPoint PPT Presentation

Integrated Simulations of Energetic Particle-driven - Effects of energetic particles on thermal plasmas: needs a lot of work (integrated simulations) ... Integration of different time scale. Integration of physics: ...

Effects of energetic particles on thermal plasmas: needs a lot of work (integrated simulations) ... Integration of different time scale. Integration of physics: ...

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Heating the Corona and Driving the Solar Wind PowerPoint PPT Presentation

Heating the Corona and Driving the Solar Wind - Feb. 2006. HMI/AIA Science Team Mtg. 1. Heating the Corona and Driving the Solar Wind ... Feb. 2006. HMI/AIA Science Team Mtg. 2. Coronal Heating. The corona ...

Feb. 2006. HMI/AIA Science Team Mtg. 1. Heating the Corona and Driving the Solar Wind ... Feb. 2006. HMI/AIA Science Team Mtg. 2. Coronal Heating. The corona ...

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Orion Workshop, SLAC, Feb. 18-20, 2003 PowerPoint PPT Presentation

Orion Workshop, SLAC, Feb. 18-20, 2003 - Steeping dispersiodissipation (eg. wave-particle trap) ... Wave-particle trapping time (dissipation) Ttr ~ (w / kII Vperp) [sinq (Bw/Bo)]-1/2 ...

Steeping dispersiodissipation (eg. wave-particle trap) ... Wave-particle trapping time (dissipation) Ttr ~ (w / kII Vperp) [sinq (Bw/Bo)]-1/2 ...

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Abstract - The magnetic field has a component perpendicular to the computational plane, ... Numerical Softwares), which is an integrated code to simulate astrophysical ...

The magnetic field has a component perpendicular to the computational plane, ... Numerical Softwares), which is an integrated code to simulate astrophysical ...

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Wave and Plasma Simulations: Resonant Effects PowerPoint PPT Presentation

Wave and Plasma Simulations: Resonant Effects - Happens Naturally for wave travel along and across magnetic field. This wave is an Arc-Wave. ... Arc-Wave could travel without changing form. But the slightest ...

Happens Naturally for wave travel along and across magnetic field. This wave is an Arc-Wave. ... Arc-Wave could travel without changing form. But the slightest ...

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PLASMA WAKEFIELD ACCELERATION FOR UHECR IN RELATIVISTIC JETS - PLASMA WAKEFIELD ACCELERATION FOR UHECR IN RELATIVISTIC JETS

PLASMA WAKEFIELD ACCELERATION FOR UHECR IN RELATIVISTIC JETS

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Lecture Series in Energetic Particle Physics of Fusion Plasmas PowerPoint PPT Presentation

Lecture Series in Energetic Particle Physics of Fusion Plasmas - F. Zonca, F. Romanelli, G. Vlad and C. Kar 1995, Phys. Rev. Lett. 74, 698 ... Particle/MHD hybrid model. Use M3D code ... M3D XMHD Model ...

F. Zonca, F. Romanelli, G. Vlad and C. Kar 1995, Phys. Rev. Lett. 74, 698 ... Particle/MHD hybrid model. Use M3D code ... M3D XMHD Model ...

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Magnetoseismology: Pi 2 Travel Time Peter Chi (IGPP/UCLA) PowerPoint PPT Presentation

Magnetoseismology: Pi 2 Travel Time Peter Chi (IGPP/UCLA) - ... Tamao s Model of Impulse Propagation via ... Nsh[cm-3] Ls Pi 2 Source distance ... AU AL(nT) Pi2-inferred start time t Current Disruption Near ...

... Tamao s Model of Impulse Propagation via ... Nsh[cm-3] Ls Pi 2 Source distance ... AU AL(nT) Pi2-inferred start time t Current Disruption Near ...

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Thin Electron Current Sheets and Auroral Arcs PowerPoint PPT Presentation

Thin Electron Current Sheets and Auroral Arcs - (Sergeev et al.) twisted or sheared magnetic field field-aligned current flow Macro-scale ... and auroral arcs Earthward moving bubble Current layers Large ...

(Sergeev et al.) twisted or sheared magnetic field field-aligned current flow Macro-scale ... and auroral arcs Earthward moving bubble Current layers Large ...

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Acceleration%20of%20Coronal%20Mass%20Ejection%20In%20Long%20Rising%20Solar%20Flares PowerPoint PPT Presentation

Acceleration%20of%20Coronal%20Mass%20Ejection%20In%20Long%20Rising%20Solar%20Flares - Ideal MHD, MHD Waves and ... Coronal heating process has three basic elements Generation of mechanical energy Transport of mechanical energy Dissipation of the ...

Ideal MHD, MHD Waves and ... Coronal heating process has three basic elements Generation of mechanical energy Transport of mechanical energy Dissipation of the ...

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Contents - ... MHD 1 2 ... A., and T. Sato, Generation of field aligned ...

... MHD 1 2 ... A., and T. Sato, Generation of field aligned ...

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HIGH-QUALITY FAST QPOs FROM MAGNETARS: AN ELECTRIC CIRCUIT MODEL PowerPoint PPT Presentation

HIGH-QUALITY FAST QPOs FROM MAGNETARS: AN ELECTRIC CIRCUIT MODEL - HIGH-QUALITY FAST QPOs FROM MAGNETARS: AN ELECTRIC CIRCUIT MODEL A.Stepanov (Pulkovo Observatory, St.Petersburg) V.Zaitsev (Institute of Applied Physics, N.Novgorod)

HIGH-QUALITY FAST QPOs FROM MAGNETARS: AN ELECTRIC CIRCUIT MODEL A.Stepanov (Pulkovo Observatory, St.Petersburg) V.Zaitsev (Institute of Applied Physics, N.Novgorod)

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Energetic Particle Physics in Burning Plasmas: from ITER to DEMO PowerPoint PPT Presentation

Energetic Particle Physics in Burning Plasmas: from ITER to DEMO - on behalf of Energetic Particle SFG. FESAC Strategic Planning Meeting, ... ARIES-ST. DEMO_EU. Multiple high-n TAEs are expected be excited in ITER from NOVA-K ...

on behalf of Energetic Particle SFG. FESAC Strategic Planning Meeting, ... ARIES-ST. DEMO_EU. Multiple high-n TAEs are expected be excited in ITER from NOVA-K ...

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Poynting%20Flux%20Dominated%20Jets%20in%20Decreasing%20Density%20Atmospheres.%20I.%20The%20Non-relativistic%20Current-driven%20Kink%20Instability%20and%20the%20Formation%20of%20 - Poynting Flux Dominated Jets in Decreasing Density Atmospheres. ... the physical connection between this central region and the sub-parsec region? ...

Poynting Flux Dominated Jets in Decreasing Density Atmospheres. ... the physical connection between this central region and the sub-parsec region? ...

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Lecture Series in Energetic Particle Physics of Fusion Plasmas - F. Zonca, F. Romanelli, G. Vlad and C. Kar 1995, Phys. Rev. Lett. 74, 698 ... Particle/MHD hybrid model. Use M3D code ... XMHD Model. Experimental observation ...

F. Zonca, F. Romanelli, G. Vlad and C. Kar 1995, Phys. Rev. Lett. 74, 698 ... Particle/MHD hybrid model. Use M3D code ... XMHD Model. Experimental observation ...

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The energy balance in the solar wind formation region PowerPoint PPT Presentation

The energy balance in the solar wind formation region - ... carry out the analysis of energetic balanse of solar wind in formation region on ... Dependence of electron density, nonthermal velocity and temperature from ...

... carry out the analysis of energetic balanse of solar wind in formation region on ... Dependence of electron density, nonthermal velocity and temperature from ...

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Dynamical Systems Approach to Space Environment Research PowerPoint PPT Presentation

Dynamical Systems Approach to Space Environment Research - Nonlinear plasma waves and intermittent turbulence play a fundamental role in ... (b) an enlargement of the middle branch of attractor A3. ...

Nonlinear plasma waves and intermittent turbulence play a fundamental role in ... (b) an enlargement of the middle branch of attractor A3. ...

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INTRODUCTION OF WAVEPARTICLE RESONANCE IN TOKAMAKS PowerPoint PPT Presentation

INTRODUCTION OF WAVEPARTICLE RESONANCE IN TOKAMAKS - Landau damping. Due to velocity space gradient ... Phase mixing and resonant absorption has exact analogy with Landau damping for Vlasov plasma. ...

Landau damping. Due to velocity space gradient ... Phase mixing and resonant absorption has exact analogy with Landau damping for Vlasov plasma. ...

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Discrete effects in Wave Turbulence PowerPoint PPT Presentation

Discrete effects in Wave Turbulence - Discrete effects in Wave Turbulence Sergey Nazarenko (Warwick) Collaborators: Yeontaek Choi, Colm Connaughton, Petr Denissenko, Uriel Frisch, Sergei Lukaschuk, Yuri ...

Discrete effects in Wave Turbulence Sergey Nazarenko (Warwick) Collaborators: Yeontaek Choi, Colm Connaughton, Petr Denissenko, Uriel Frisch, Sergei Lukaschuk, Yuri ...

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Particle Acceleration At Astrophysical Shocks PowerPoint PPT Presentation

Particle Acceleration At Astrophysical Shocks - Title: Slide 1 Last modified by: SCIPP Document presentation format: Custom Other titles: Times New Roman Tahoma Arial Wingdings Avant Garde Gothic Comic Sans MS ...

Title: Slide 1 Last modified by: SCIPP Document presentation format: Custom Other titles: Times New Roman Tahoma Arial Wingdings Avant Garde Gothic Comic Sans MS ...

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Hybrid Simulations of Energetic Particledriven PowerPoint PPT Presentation

Hybrid Simulations of Energetic Particledriven - Mode Structure: Ideal Kink v.s. Fishbone. ITER: alpha particle ... stabilize n=1 internal kink mode. Fast Ion-driven TAE in a Quasi-symmetric stellarator ...

Mode Structure: Ideal Kink v.s. Fishbone. ITER: alpha particle ... stabilize n=1 internal kink mode. Fast Ion-driven TAE in a Quasi-symmetric stellarator ...

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POLAR Scientists Discover the Energy Source Powering the Aurora - It is known that the aurora is created by intense electron beams ... three-axis electric field detector flown in the magnetosphere, resolves without ...

It is known that the aurora is created by intense electron beams ... three-axis electric field detector flown in the magnetosphere, resolves without ...

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What - What's New With The R-modes? Gregory Mendell. LIGO Hanford ... Have really intense magnetic fields (1012 Gauss) ... Wu, Matzner, and Arras, astro-ph/0006123 ...

What's New With The R-modes? Gregory Mendell. LIGO Hanford ... Have really intense magnetic fields (1012 Gauss) ... Wu, Matzner, and Arras, astro-ph/0006123 ...

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Multiscale issues in modeling magnetic reconnection PowerPoint PPT Presentation

Multiscale issues in modeling magnetic reconnection - Multiscale issues in modeling magnetic reconnection J. F. Drake University of Maryland IPAM Meeting on Multiscale Problems in Fusion Plasmas

Multiscale issues in modeling magnetic reconnection J. F. Drake University of Maryland IPAM Meeting on Multiscale Problems in Fusion Plasmas

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Chromospheric Anemone Jets Outside of Sunspots in Active Regions PowerPoint PPT Presentation

Chromospheric Anemone Jets Outside of Sunspots in Active Regions - Hinode discovered ubiquitous Ca jets (anemone jets) in the solar chromosphere ... Chromoshperic anemone jet seems to be accelerated by slow mode shock generated ...

Hinode discovered ubiquitous Ca jets (anemone jets) in the solar chromosphere ... Chromoshperic anemone jet seems to be accelerated by slow mode shock generated ...

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The Story of Star Birth PowerPoint PPT Presentation

The Story of Star Birth - 1950's Chandrasekhar, Fermi use polarization data to estimate interstellar B ... Magnetic Fields and Polarimetry. Courtesy A. Goodman ...

1950's Chandrasekhar, Fermi use polarization data to estimate interstellar B ... Magnetic Fields and Polarimetry. Courtesy A. Goodman ...

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A Joint Australian Fusion Energy Initiative PowerPoint PPT Presentation

A Joint Australian Fusion Energy Initiative - A Joint Australian Fusion Energy Initiative Strategic plan for Fusion Science ITER forum Capability, infrastructure, Flagship Diagnostic? Initial ISL projects ...

A Joint Australian Fusion Energy Initiative Strategic plan for Fusion Science ITER forum Capability, infrastructure, Flagship Diagnostic? Initial ISL projects ...

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Solar Wind Iron Ions with STEREO/PLASTIC: PowerPoint PPT Presentation

Solar Wind Iron Ions with STEREO/PLASTIC: - Alpha/proton magnetosonic instability in the solar wind ... Heavy species are always faster than protons ... heavy species compared to protons. At least in the ...

Alpha/proton magnetosonic instability in the solar wind ... Heavy species are always faster than protons ... heavy species compared to protons. At least in the ...

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Alfven PowerPoint PPT Presentations