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Alfv PowerPoint PPT Presentation
Alfv - Carbon coats DIII-D mirrors when escaping fast ions ablate the graphite wall1 ... result must be a powerful aggregate reflexion, even though the effect of an ...
Carbon coats DIII-D mirrors when escaping fast ions ablate the graphite wall1 ... result must be a powerful aggregate reflexion, even though the effect of an ...
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Dissipation of Alfv PowerPoint PPT Presentation
Dissipation of Alfv - 'broken' flux tube The magnetic surface separates into various sheets At break ... Magnetic field topology: sites of magnetic lines exponential separation ...
'broken' flux tube The magnetic surface separates into various sheets At break ... Magnetic field topology: sites of magnetic lines exponential separation ...
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Excitation of Alfv PowerPoint PPT Presentation
Excitation of Alfv - Excitation of Alfvn eigenmodes with subAlfvnic neutral beam ions in JET and DIIID plasmas
Excitation of Alfvn eigenmodes with subAlfvnic neutral beam ions in JET and DIIID plasmas
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Results from Visible Light Imaging of Alfv PowerPoint PPT Presentation
Results from Visible Light Imaging of Alfv - Results from Visible Light Imaging of Alfv n Fluctuations in the H-1NF Heliac J. Read, J. Howard, B. Blackwell, David Oliver, & David Pretty Acknowledgements: Greg ...
Results from Visible Light Imaging of Alfv n Fluctuations in the H-1NF Heliac J. Read, J. Howard, B. Blackwell, David Oliver, & David Pretty Acknowledgements: Greg ...
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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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SOLAR MICROWAVE DRIFTING SPIKES AND SOLITARY KINETIC ALFVEN WAVES PowerPoint PPT Presentation
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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Alfvn Waves in the Solar Corona PowerPoint PPT Presentation
Alfvn Waves in the Solar Corona - T. Schad, D. Seeley, J. Edmondson. Science, Vol. 317, Sep., 2007. October 31, 2007. What's new? ... Coronal Multi-channel Polarimeter (CoMP) ...
T. Schad, D. Seeley, J. Edmondson. Science, Vol. 317, Sep., 2007. October 31, 2007. What's new? ... Coronal Multi-channel Polarimeter (CoMP) ...
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Beam Voltage Threshold for Excitation of Compressional Alfv PowerPoint PPT Presentation
Beam Voltage Threshold for Excitation of Compressional Alfv - Amplitude, number of modes, strong function of voltage above threshold. ... Only fast ions, above 50 keV, drive waves. ... TRANSP calculation, recalibrated Thomson Te. ...
Amplitude, number of modes, strong function of voltage above threshold. ... Only fast ions, above 50 keV, drive waves. ... TRANSP calculation, recalibrated Thomson Te. ...
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Cluster observation of electron acceleration by ULF Alfv PowerPoint PPT Presentation
Cluster observation of electron acceleration by ULF Alfv - Vortex structure. CLUSTER-II 2002-04-15 summary. B-field. E-field. dB. Poynting Flux. S ... Several hundreds km of perpendicular wave length. Vortex structure. ...
Vortex structure. CLUSTER-II 2002-04-15 summary. B-field. E-field. dB. Poynting Flux. S ... Several hundreds km of perpendicular wave length. Vortex structure. ...
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Jovian Sbursts generation by Alfvn waves PowerPoint PPT Presentation
Jovian Sbursts generation by Alfvn waves - Torus period = Jupiter's Period = 9 hours 55.5 min. } Io is moving relative to the plasma. Io's obital period = 42 hours 27.5 minutes. Electric field generation: E ...
Torus period = Jupiter's Period = 9 hours 55.5 min. } Io is moving relative to the plasma. Io's obital period = 42 hours 27.5 minutes. Electric field generation: E ...
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Winds of cool supergiant stars driven by Alfv PowerPoint PPT Presentation
Winds of cool supergiant stars driven by Alfv - A simplified coronal holes geometry ... A simplified coronal holes geometry. Heating due to Alfv n waves. Radiative cooling. ... Self consistent coronal holes geometry ...
A simplified coronal holes geometry ... A simplified coronal holes geometry. Heating due to Alfv n waves. Radiative cooling. ... Self consistent coronal holes geometry ...
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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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Active MHD Spectroscopy of Alfvn Eigenmodes PowerPoint PPT Presentation
Active MHD Spectroscopy of Alfvn Eigenmodes - MIT Plasma Science and Fusion Center. Cambridge, MA USA ... C-Mod Active MHD antennas ... tiles, 5 turns/antenna, 4 antennas on the outboard wall at 2 poloidal and ...
MIT Plasma Science and Fusion Center. Cambridge, MA USA ... C-Mod Active MHD antennas ... tiles, 5 turns/antenna, 4 antennas on the outboard wall at 2 poloidal and ...
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The Role of Damping in Stable and Unstable Alfv PowerPoint PPT Presentation
The Role of Damping in Stable and Unstable Alfv - The Role of Damping in Stable and Unstable Alfv n Eigenmodes ... [Hasegawa & Chen Phys. Fluids 19 1924 (1976)] [Mett and Mahajan, Phys. Fluids B 4 2885 (1992) ...
The Role of Damping in Stable and Unstable Alfv n Eigenmodes ... [Hasegawa & Chen Phys. Fluids 19 1924 (1976)] [Mett and Mahajan, Phys. Fluids B 4 2885 (1992) ...
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Alfvn waves propagation in homogeneous and dusty astrophysical plasmas PowerPoint PPT Presentation
Alfvn waves propagation in homogeneous and dusty astrophysical plasmas - A low temperature plasma containing disperse particles of solid material, ... If dust particles are charged, they interact with the waves, and give rise ...
A low temperature plasma containing disperse particles of solid material, ... If dust particles are charged, they interact with the waves, and give rise ...
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Mass loss and Alfvn waves in cool supergiant stars PowerPoint PPT Presentation
Mass loss and Alfvn waves in cool supergiant stars - Coronal holes: origin of fast solar wind u 600 km s-1. Cranmer & Ballegooijen (2005) ... A simplified coronal holes geometry ...
Coronal holes: origin of fast solar wind u 600 km s-1. Cranmer & Ballegooijen (2005) ... A simplified coronal holes geometry ...
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Evidence for Alfvn waves propagating in a coronal loop PowerPoint PPT Presentation
Evidence for Alfvn waves propagating in a coronal loop - The method of coronal seismology (Uchida 1970; Roberts et al 1984) based on ... We used the observed properties of the waves for coronal seismology. ...
The method of coronal seismology (Uchida 1970; Roberts et al 1984) based on ... We used the observed properties of the waves for coronal seismology. ...
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Mirrorinduced Alfvn Eigenmodes MAE in a Periodic Magnetic Mirror Geometry PowerPoint PPT Presentation
Mirrorinduced Alfvn Eigenmodes MAE in a Periodic Magnetic Mirror Geometry - Bragg reflection condition 2k// =km or ? = 2 ?m predicts a propagation gap at. fB=vA///2 ?m ... Reflection Effect? Mirror Caused Periodicity Changes Wave ...
Bragg reflection condition 2k// =km or ? = 2 ?m predicts a propagation gap at. fB=vA///2 ?m ... Reflection Effect? Mirror Caused Periodicity Changes Wave ...
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Flows in coronal loops driven by Alfvn waves: 1D simulations PowerPoint PPT Presentation
Flows in coronal loops driven by Alfvn waves: 1D simulations - PHYSICAL PROBLEM: how transverse motions (Alfv n waves) drive parallel motion ... large injection of compressive waves, large reflexion at boundary ...
PHYSICAL PROBLEM: how transverse motions (Alfv n waves) drive parallel motion ... large injection of compressive waves, large reflexion at boundary ...
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Solar coronal heating on current sheets where kinetic Alfvn waves are generated PowerPoint PPT Presentation
Solar coronal heating on current sheets where kinetic Alfvn waves are generated - A null and the associated separatrix. Continuous footpoint motion of. At the photosphere boundary ... on the separatrix. Force-free equilibrium. The growth rate ...
A null and the associated separatrix. Continuous footpoint motion of. At the photosphere boundary ... on the separatrix. Force-free equilibrium. The growth rate ...
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Numerical simulations of largeamplitude Alfvn waves in the solar corona PowerPoint PPT Presentation
Numerical simulations of largeamplitude Alfvn waves in the solar corona - EGS meeting, Nice, March 2001 - Colloque ... Both magnetic field and temperature determine the flow. ... Distance-Latitude map of the velocity field (close up) ...
EGS meeting, Nice, March 2001 - Colloque ... Both magnetic field and temperature determine the flow. ... Distance-Latitude map of the velocity field (close up) ...
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Modeling the Intermittent Dynamics of Alfvn Waves in the Solar Wind PowerPoint PPT Presentation
Modeling the Intermittent Dynamics of Alfvn Waves in the Solar Wind - National Institute for Space Research ... Relevance of intermittency and chaos in the solar ... Spatiotemporal solutions of the Kuramoto-Sivashinsky ...
National Institute for Space Research ... Relevance of intermittency and chaos in the solar ... Spatiotemporal solutions of the Kuramoto-Sivashinsky ...
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Nonlinear coupling of Alfvn Waves to the Quasi Coherent Mode PowerPoint PPT Presentation
Nonlinear coupling of Alfvn Waves to the Quasi Coherent Mode - Er0 spectra at separatrix: k =0, f=1400 kHz. Electron geodesic-acoustic mode ... dn spectra at separatrix. kq=-1.3 cm-1, f=100 kHz. Quasi-Coherent Mode. Alcator ...
Er0 spectra at separatrix: k =0, f=1400 kHz. Electron geodesic-acoustic mode ... dn spectra at separatrix. kq=-1.3 cm-1, f=100 kHz. Quasi-Coherent Mode. Alcator ...
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Research of Alfvn wave heating and current drive on the SUNIST spherical tokamak PowerPoint PPT Presentation
Research of Alfvn wave heating and current drive on the SUNIST spherical tokamak - Task list. Impedance analysis. RF generator design & manufacture. Basic antenna design ... No mechanical vibration observed (fm fRF). Shield or limiter ...
Task list. Impedance analysis. RF generator design & manufacture. Basic antenna design ... No mechanical vibration observed (fm fRF). Shield or limiter ...
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Kinetic Alfvn Waves Dynamics and Substorm Onset Andreas Keiling Pi2 pulsations in the nearEarth plas PowerPoint PPT Presentation
Kinetic Alfvn Waves Dynamics and Substorm Onset Andreas Keiling Pi2 pulsations in the nearEarth plas - Kinetic Alfv n Waves Dynamics and Substorm Onset Andreas Keiling. Pi2 pulsations in the near-Earth plasma sheet ... Velocity vorticity and FAC Larry Kepko ...
Kinetic Alfv n Waves Dynamics and Substorm Onset Andreas Keiling. Pi2 pulsations in the near-Earth plasma sheet ... Velocity vorticity and FAC Larry Kepko ...
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Hull PowerPoint PPT Presentation
Hull - ... frakt lok No spectral transfer Dispersion relation Generation: MHD or kinetic Alfv n waves Ion cyclotron (3.1 ...
... frakt lok No spectral transfer Dispersion relation Generation: MHD or kinetic Alfv n waves Ion cyclotron (3.1 ...
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Historical Solar Cycle Context PowerPoint PPT Presentation
Historical Solar Cycle Context - Changing Relationship Between F10.7 Flux and Sunspot Number Changing Relationship Between Solar Wind Alfv n Mach Number and Sunspot Number Sunspot umbras ...
Changing Relationship Between F10.7 Flux and Sunspot Number Changing Relationship Between Solar Wind Alfv n Mach Number and Sunspot Number Sunspot umbras ...
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Evolution of                  Interplanetary Coronal Mass Ejections for Different Solar Wind Conditions PowerPoint PPT Presentation
Evolution of Interplanetary Coronal Mass Ejections for Different Solar Wind Conditions - Radial and axial expansion: different ... Strong Alfv n waves activity after the MC Modelling the magnetic flux rope IAU Symposium 257 Universal ...
Radial and axial expansion: different ... Strong Alfv n waves activity after the MC Modelling the magnetic flux rope IAU Symposium 257 Universal ...
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RFA Experiments on the T2R RFP PowerPoint PPT Presentation
RFA Experiments on the T2R RFP - 1) Alfv n Laboratory, KTH, EURATOM /VR Association VR, Stockholm, Sweden ... high-bandwidth audio amplifiers, output power 700 Watt ' ...
1) Alfv n Laboratory, KTH, EURATOM /VR Association VR, Stockholm, Sweden ... high-bandwidth audio amplifiers, output power 700 Watt ' ...
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A theoretical plasma physicist PowerPoint PPT Presentation
A theoretical plasma physicist - by supernovae at L ~ 100 pc. Fluctuations of velocity. and magnetic field are. Alfv nic: ... Maxwell's equations. Gyrokinetics: Kinetics of Larmor Rings ...
by supernovae at L ~ 100 pc. Fluctuations of velocity. and magnetic field are. Alfv nic: ... Maxwell's equations. Gyrokinetics: Kinetics of Larmor Rings ...
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An Unsplit Ideal MHD code with Adaptive Mesh Refinement PowerPoint PPT Presentation
An Unsplit Ideal MHD code with Adaptive Mesh Refinement - One characteristic wave speed (ion-acoustic) Tightly coupled formulation ... Three characteristic wave speeds (slow, Alfv n, fast) One degenerate eigenvalue ...
One characteristic wave speed (ion-acoustic) Tightly coupled formulation ... Three characteristic wave speeds (slow, Alfv n, fast) One degenerate eigenvalue ...
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Scaling and a FokkerPlanck approach to fluctuations in the solar wind plasma PowerPoint PPT Presentation
Scaling and a FokkerPlanck approach to fluctuations in the solar wind plasma - ... of supersonic and super-Alfv nic particles originated from ... different models of ... be used to develop sub-grid models for solar wind turbulence ...
... of supersonic and super-Alfv nic particles originated from ... different models of ... be used to develop sub-grid models for solar wind turbulence ...
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Issues PowerPoint PPT Presentation
Issues - Modifications of the ionospheric conductivity by the electron precipitation is ... Joule dissipation in Alfv nic regions mainly cusp and the auroral BPS regions; ...
Modifications of the ionospheric conductivity by the electron precipitation is ... Joule dissipation in Alfv nic regions mainly cusp and the auroral BPS regions; ...
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Kinetic instability induced fast ion losses in NSTX PowerPoint PPT Presentation
Kinetic instability induced fast ion losses in NSTX - ITER will operate with a large, super-Alfv nic, fast ion population ... Reflectometer shows 'sea of TAE' vs. a few scattered modes...
ITER will operate with a large, super-Alfv nic, fast ion population ... Reflectometer shows 'sea of TAE' vs. a few scattered modes...
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PowerPoint Presentation Standing wave mode structure PowerPoint PPT Presentation
PowerPoint Presentation Standing wave mode structure - Standing Alfv n waves are routinely observed by spacecraft. ... decreases approximately as 1/R, where R geocentric distance along a field line. ...
Standing Alfv n waves are routinely observed by spacecraft. ... decreases approximately as 1/R, where R geocentric distance along a field line. ...
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Nonlinear Ponderomotive Force by Low Frequency Waves and PowerPoint PPT Presentation
Nonlinear Ponderomotive Force by Low Frequency Waves and - the Possibility of Alfv n Wave Current Drive in Spherical Tori. Zhe Gao ... Tsypin et al 1995) and kinetic (Chan and Chiu 1993, Fukuyama et al 1993) model ...
the Possibility of Alfv n Wave Current Drive in Spherical Tori. Zhe Gao ... Tsypin et al 1995) and kinetic (Chan and Chiu 1993, Fukuyama et al 1993) model ...
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Can magnetic waves in aurorae transform into acoustic waves Jada Maxwell PowerPoint PPT Presentation
Can magnetic waves in aurorae transform into acoustic waves Jada Maxwell - ... is crucial for transporting photospheric energy to the hot corona. ... Ofman, L. 'Alfv n waves in the solar corona, the solar wind, and the magnetosphere. ...
... is crucial for transporting photospheric energy to the hot corona. ... Ofman, L. 'Alfv n waves in the solar corona, the solar wind, and the magnetosphere. ...
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Prsentation PowerPoint EGUNice2004 PowerPoint PPT Presentation
Prsentation PowerPoint EGUNice2004 - 1. Coupling siphon and solar wind flows (or how Alfv n waves accelerate wind and ... Domain: chromosphere (above transition) up to 15 solar radii. ...
1. Coupling siphon and solar wind flows (or how Alfv n waves accelerate wind and ... Domain: chromosphere (above transition) up to 15 solar radii. ...
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T' Hellsten1, T' Bergkvist1, T'Johnson1, M' Laxback1 and L'G' Eriksson2 PowerPoint PPT Presentation
T' Hellsten1, T' Bergkvist1, T'Johnson1, M' Laxback1 and L'G' Eriksson2 - 1Euratom-VR association, Alfv n Laboratory, Royal Institute of ... MHD increments for n interactions during one decorrelation time tdecorr , ntb=tdecorr ...
1Euratom-VR association, Alfv n Laboratory, Royal Institute of ... MHD increments for n interactions during one decorrelation time tdecorr , ntb=tdecorr ...
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T. Hellsten1, T. Bergkvist1, T.Johnson1, M. Lax PowerPoint PPT Presentation
T. Hellsten1, T. Bergkvist1, T.Johnson1, M. Lax - Title: Mo Author: thnt Last modified by: Nils Brenning Created Date: 5/28/2002 12:50:58 PM Document presentation format: Bildspel p sk rmen Company
Title: Mo Author: thnt Last modified by: Nils Brenning Created Date: 5/28/2002 12:50:58 PM Document presentation format: Bildspel p sk rmen Company
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MHD wave propagation in the neighbourhood of a two-dimensional null point PowerPoint PPT Presentation
MHD wave propagation in the neighbourhood of a two-dimensional null point - As the wave approaches the separatrix, it thins but keeps its original amplitude. ... along the field and accumulates at the separatrix and increases in time. ...
As the wave approaches the separatrix, it thins but keeps its original amplitude. ... along the field and accumulates at the separatrix and increases in time. ...
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Waves, structures and turbulences PowerPoint PPT Presentation
Waves, structures and turbulences - The Sun open magnetic field lines. MHD model field during Ulysses ... McDowell and Kellog, 2001. Power in grey scale in dB above noise. Electron beam driven ...
The Sun open magnetic field lines. MHD model field during Ulysses ... McDowell and Kellog, 2001. Power in grey scale in dB above noise. Electron beam driven ...
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Thayer School of Engineering PowerPoint PPT Presentation
Thayer School of Engineering - Thayer School of Engineering Dartmouth College Effects of the Active Auroral Ionosphere on Magnetosphere - Ionosphere Coupling Dimitri Pokhotelov
Thayer School of Engineering Dartmouth College Effects of the Active Auroral Ionosphere on Magnetosphere - Ionosphere Coupling Dimitri Pokhotelov
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Current filaments in PowerPoint PPT Presentation
Current filaments in - ... Direct measurement of current filament structures in a magnetic confinement fusion ... The current density filament is associated to a parallel vorticity ...
... Direct measurement of current filament structures in a magnetic confinement fusion ... The current density filament is associated to a parallel vorticity ...
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Summary of IAEA Theory Papers on Energetic Particle Physics PowerPoint PPT Presentation
Summary of IAEA Theory Papers on Energetic Particle Physics - A total of 15 papers presented ; 5 talks, 10 posters; 4 papers on low frequency modes (GAM,BAAE) ... 2 papers on nonlinear simulations of AE; 2 papers on EP ...
A total of 15 papers presented ; 5 talks, 10 posters; 4 papers on low frequency modes (GAM,BAAE) ... 2 papers on nonlinear simulations of AE; 2 papers on EP ...
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Boundaries in the auroral region --- Small scale density cavities and associated processes --- PowerPoint PPT Presentation
Boundaries in the auroral region --- Small scale density cavities and associated processes --- - steep gradient density cavities. related ... criterion a0.8 is satisfied in very localized regions (density gradients) ... with density gradients ...
steep gradient density cavities. related ... criterion a0.8 is satisfied in very localized regions (density gradients) ... with density gradients ...
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SUMMARY of FAST PARTICLE PHYSICS PowerPoint PPT Presentation
SUMMARY of FAST PARTICLE PHYSICS - SUMMARY of FAST PARTICLE PHYSICS. Boris Breizman, Raffi Nazikian & Energetic Particle Group ... Internal reflectometer measurements urgently needed! ...
SUMMARY of FAST PARTICLE PHYSICS. Boris Breizman, Raffi Nazikian & Energetic Particle Group ... Internal reflectometer measurements urgently needed! ...
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On the frequency distribution of heating events in Coronal Loops, simulating observations with Hinode/XRT PowerPoint PPT Presentation
On the frequency distribution of heating events in Coronal Loops, simulating observations with Hinode/XRT - On the frequency distribution of heating events in Coronal Loops, simulating ... Waves & Oscillations in the Solar Atmosphere: Heating and Magneto-Seismology. ...
On the frequency distribution of heating events in Coronal Loops, simulating ... Waves & Oscillations in the Solar Atmosphere: Heating and Magneto-Seismology. ...
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Parallel electric fields in space PowerPoint PPT Presentation
Parallel electric fields in space - Parallel electric fields in space
Parallel electric fields in space
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 PowerPoint PPT Presentation
- Title: PowerPoint Author: lab545 Last modified by: lab545 Created Date: 2/3/2006 4:57:04 PM Document presentation format:
Title: PowerPoint Author: lab545 Last modified by: lab545 Created Date: 2/3/2006 4:57:04 PM Document presentation format:
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MHD Simulations of the January 10-11, 1997 Magnetic Storm PowerPoint PPT Presentation
MHD Simulations of the January 10-11, 1997 Magnetic Storm - Scientific visualizations provide both scientist and the general public with ... CANOPUS magnetic, optical and radar data exhibit a coincident 1.3-mHz 'resonant' ...
Scientific visualizations provide both scientist and the general public with ... CANOPUS magnetic, optical and radar data exhibit a coincident 1.3-mHz 'resonant' ...
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Waves%20and%20turbulence%20in%20the%20solar%20wind PowerPoint PPT Presentation
Waves%20and%20turbulence%20in%20the%20solar%20wind - Waves and turbulence in the solar wind Tim Horbury PG Lectures Turbulence: the basics Turbulence in plasmas: MHD scales The solar wind context Key results
Waves and turbulence in the solar wind Tim Horbury PG Lectures Turbulence: the basics Turbulence in plasmas: MHD scales The solar wind context Key results
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Sound Waves from the Northern Lights PowerPoint PPT Presentation
Sound Waves from the Northern Lights - Title: Slide 1 Author: Jada Last modified by: E.J.Zita Created Date: 2/6/2006 8:32:16 PM Document presentation format: On-screen Show Other titles
Title: Slide 1 Author: Jada Last modified by: E.J.Zita Created Date: 2/6/2006 8:32:16 PM Document presentation format: On-screen Show Other titles
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Coronal Loop Oscillations observed by TRACE PowerPoint PPT Presentation
Coronal Loop Oscillations observed by TRACE - Coronal Loop Oscillations observed by TRACE (Newton, 2002?10??) ... Nakariakov et al. 1999, Science, 285, 862. Aschwanden ... (Re,spot = 0.90, Re, plage = 0.94) ...
Coronal Loop Oscillations observed by TRACE (Newton, 2002?10??) ... Nakariakov et al. 1999, Science, 285, 862. Aschwanden ... (Re,spot = 0.90, Re, plage = 0.94) ...
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Auroral Acceleration Region PowerPoint PPT Presentation
Auroral Acceleration Region - Are closure currents longitudinal (zonal) or latitudinal (meridional) ... Is there a region of zonal flow at high latitudes that is associated with the ...
Are closure currents longitudinal (zonal) or latitudinal (meridional) ... Is there a region of zonal flow at high latitudes that is associated with the ...
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