'broken' flux tube The magnetic surface separates into various sheets At break ... Magnetic field topology: sites of magnetic lines exponential separation ...
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 ...
Spatiotemporal chaos can be described in terms of UPOs. Christiansen et al., Nonlinearity 1997 ... Spatiotemporal phase dynamics of Alfven waves. Chian et al. ...
Plasmas in Laboratory and Astrophysics. Alfven Wave Turbulence and Heating. ... fine scale mixing - jagged f. Less collisions more jagged f. Entropy production ...
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 ...
A low temperature plasma containing disperse particles of solid material, ... If dust particles are charged, they interact with the waves, and give rise ...
A null and the associated separatrix. Continuous footpoint motion of. At the photosphere boundary ... on the separatrix. Force-free equilibrium. The growth rate ...
The method of coronal seismology (Uchida 1970; Roberts et al 1984) based on ... We used the observed properties of the waves for coronal seismology. ...
National Institute for Space Research ... Relevance of intermittency and chaos in the solar ... Spatiotemporal solutions of the Kuramoto-Sivashinsky ...
EGS meeting, Nice, March 2001 - Colloque ... Both magnetic field and temperature determine the flow. ... Distance-Latitude map of the velocity field (close up) ...
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 ...
PHYSICAL PROBLEM: how transverse motions (Alfv n waves) drive parallel motion ... large injection of compressive waves, large reflexion at boundary ...
Reproduced 124764 - (higher current) possibly higher D-fraction. Attempted beam voltage scan in D, too difficult to stay out of H-mode, plagued by MHD. ...
Kinetic Alfv n Waves Dynamics and Substorm Onset Andreas Keiling. Pi2 pulsations in the near-Earth plasma sheet ... Velocity vorticity and FAC Larry Kepko ...
Changing Relationship Between F10.7 Flux and Sunspot Number Changing Relationship Between Solar Wind Alfv n Mach Number and Sunspot Number Sunspot umbras ...
... of supersonic and super-Alfv nic particles originated from ... different models of ... be used to develop sub-grid models for solar wind turbulence ...
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 ...
Modifications of the ionospheric conductivity by the electron precipitation is ... Joule dissipation in Alfv nic regions mainly cusp and the auroral BPS regions; ...
... 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. ...
1Euratom-VR association, Alfv n Laboratory, Royal Institute of ... MHD increments for n interactions during one decorrelation time tdecorr , ntb=tdecorr ...
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
Magnetic & Acoustic Waves in the Aurora Jada Maxwell Photo: Michael Klensch Courtesy of http:www.nordlys.com Magnetic & Acoustic Waves in the Aurora Can magnetic ...
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 ...
Photosphere. Spectroscopic observations. 2) origin of the dv2 -1/2 ... Photosphere. Resolution scale. LOS depth. 23. Are low q/m ions hotter than the others ? ...
CLUSTER SATELLITE OBSERVATIONS OF FIELD LINE RESONANCES IN THE DAYSIDE MAGNETOSPHERE Background Assume wave propagation on the ... Radial polarisation of the ...
A Joint Australian Fusion Energy Initiative Strategic plan for Fusion Science ITER forum Capability, infrastructure, Flagship Diagnostic? Initial ISL projects ...
The Australian Plasma Fusion Research Facility: Overview and Upgrade Plans (is there potential to be an additional training platform in diagnostics and plasma physics ...
Turbulent transport in fusion plasmas is intermittent, because it is dominated ... have been observed in the magnetosphere by the 4-spaceship Cluster mission. ...
Next Generation of Magnetosphere-Ionosphere-Thermosphere Coupling Models P. Song University of Massachusetts Lowell Acknowledgments: V. M. Vasyli nas, and J. Tu
SUMMARY of FAST PARTICLE PHYSICS. Boris Breizman, Raffi Nazikian & Energetic Particle Group ... Internal reflectometer measurements urgently needed! ...
Modeling the Solar Wind: A survey of theoretical ideas for the origins of fast & slow streams Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics
Are closure currents longitudinal (zonal) or latitudinal (meridional) ... Is there a region of zonal flow at high latitudes that is associated with the ...
Elected FRS (Academician) 1668 (age 30) Appointed 1st regius prof maths at St Andrews (1668) ... Given hall as lab -- see line for telescope along meridian ...
Modulate the beams on the confinement time scale (60 ms) to observe changes in ... visible in the NPA, ions less than the full energy are conspicuously absent. ...
'Synergy means behavior of whole systems unpredicted by the behavior of their ... Buckminster Fuller. What creates the aurora? Sound waves from the aurora ...