Therefore there is a dynamic alignment of otherwise independent elsasser vectors ... Alignment have an intermittent nature, being stronger in regions with large wave ...
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. ...
Breakup always corresponds (in space&time) to tailward Alfvenic outflows (XNL reconnection? ... deceleration of incoming electrons crossing the separatrix. ...
Some shocks are very efficient accelerators 50% Magnetic amplification mG- mG ... Most CRs decompress until. expansion sub-Alfvenic. Pulsars, stars more complex! ...
(Sergeev et al.) twisted or sheared magnetic field field-aligned current flow Macro-scale ... and auroral arcs Earthward moving bubble Current layers Large ...
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 ...
Solar Wind-Magnetosphere Interaction for Northward Interplanetary Magnetic Field Paul Song Center for Atmospheric Research University of Massachusetts Lowell
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 ...
Discrepancy between average WMAP observed and ROSAT predicted Sunyaev-Zel'dovich ... The S-Z effect may be probe of cluster non-thermal processes, not cosmology. ...
Magnetic fields in Orion's Veil. T. Troland. Physics & Astronomy Department ... Orion Nebula - optical extinction. O'Dell & Yusef-Zadeh, 2000, contours at Av = 1, 2 ...
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 ...
Basal acoustic flux: 108 erg/cm2/s (equiv. ' piston' v = 0.3 km/s) ... http://cfa-www.harvard.edu/~scranmer/ Turbulent Origins of the Solar Wind. Steven R. Cranmer ...
Passively stable at =4.1% to kink, ballooning, vertical, Mercier, ... May not be compatible with inboard-launch ... of trim coils, both signs. Zeff ...
First Order Fermi Acceleration: a Primer. Return Probability from UP=1 ... Energy is channelled to CRs then the adiabatic index changes from 5/3 to 4/3. ...
University of Sheffield. Solar Physics & Space Plasma. Research ... Dutch Open Telescope, La Palma. 12. Sept. 1999 [S tterlin & Rutten] 25 000 km x 38 000 km ...
Eliminate Bn, then Bt, ut to find. Rankine-Hugoniot (Jump) Conditions: 4 ... Time (UT) f (Hz) Power. E(V/m) Electron. Flux. N(cm-3) B(nT) Predicted Radio ...
loop strands with isothermal cross-sections, at FWHM widths of ... in the CELTIC model is consistent. with a semi-Gaussian distribution. with a Gaussian width of ...
Generic picture of an accreting system (pm,swift) A collapse of a rotating envelope ... Timing is good as SWIFT is to be launched soon. It used to be used ...
Dispersion diagrams of chromospheric MHD waves in a 2D simulation. Chris Dove ... Brigham, E. Oran, The Fast Fourier Transform, Prentice-Hall, 1974 ...
Brief review of transport studies, scaling laws, similarity experiments, ... The ETG adiabatic response. does not allow strong zonal. flow generation: STREAMERS ...
Ground-based cosmic ray data from the Global Muon Detection Network (GMDN) ... Cosmic-ray storms. Isotropic intensity depression. Forbush Decrease. Enhanced anisotropy ...
National Centre for Radio Astrophysics. Tata Institute of Fundamental Research ... such that its pressure equals the rate of change of the momentum of the diver. ...
... I am going to discuss, so bear with me if I say something trivial ... source located several AU closer to the sun. and closer to the pole than Voyager 1 ...
Coupling to dispersive waves in dissipation region at small scales produces fast ... Dissipation mechanism. What balances Ep during guide field reconnection? ...
of Stochastic Magnetic Fields. PhD Thesis Research Plan. PhD candidate: ... detected at Earth is very isotropic ( 5 10-4 anisotropy) can't see the source. ...
Particle-in-Cell Simulations of Electron Transport from Plasma Turbulence: Recent Progress in ... currently ES but later EM (solve GK Poisson equation & Ampere's law) ...
A Joint Australian Fusion Energy Initiative Strategic plan for Fusion Science ITER forum Capability, infrastructure, Flagship Diagnostic? Initial ISL projects ...
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