Magnetopause PowerPoint PPT Presentations

IMAGE: Imager for MagnetopausetoAurora

TP developed in late 80 & 90s using AMPTE data. Ne/Te (particularly Te ... electron anisotropy (|| - )/ (Why does it work? Reconnection! The anti-correlation ...

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Magnetic reconnection at the Earths magnetopause: CLUSTER spacecraft observations at different scale

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. ...

Two observations selected at random, permit us to inspect the ... Betas. Neural networks units. 9/5/09. 17. Steps in the modeling process (continued) ...

The shape of Saturn's magnetopause (MP), and those of ... CASSINI MAGNETOMETER TEAM ... field strength measured by the Cassini magnetometer at each crossing. ...

Detection of magnetic compressions in front of magnetopause indentations: ... subsolar mp structure [Phan and Pashmann, Ampte results] October 2001. Cluster Workshop ...

Nutation damper inoperative at low spin periods. Magnetic torquers to control nutation fully operational. Now in Initial Orbital Checkout ...

Such periods with frequent encounters are usually indicative of a rapidly moving ... Well-determined MVA structures for MP encounters often appear over a wide range ...

Averaged in space, the jets carry the momentum difference between measured and ... In the structured plasma jets ion kinetic energy density (Wkin) and plasma flux ...

Conjugate response of the dayside magnetopause and dawn/dusk flanks using Cluster-THEMIS conjunctions and Ground based observations

Reconnection occurs at the magnetopause, on the sun, on all scales in ... Shay, M.A., J.F. Drake, B.N. Rogers, and R.E. Denton J. Geophys. Res., 106, 3759, (2001) ...

Thin current sheets: separation of regions of oppositely ... magnetic field hodograph. ion drift velocity hodograph. LHD waves at the sheared magnetopause ...

Upstream particle events (E 1 MeV) stream ... AMIs were observed close to the bow-shock and close to the magnetopause as well ... Possible sources of AMIs ...

More about flows in Poster previews! Modelers using these data to simulate eruptions! ... (BACK) Petrinec et al. (1998) Movie of Bow Shock, Magnetopause (BACK) ...

Solar Wind-Magnetosphere Interaction for Northward Interplanetary Magnetic Field Paul Song Center for Atmospheric Research University of Massachusetts Lowell

Polar THEMIS Collaboration Opportunities. Spacecraft Locations post launch ... When THEMIS is launched, Polar will be near the noon meridian, probing the ...

The Bimodal Solar Wind-Magnetosphere-Ionosphere System George Siscoe Center for Space Physics Boston University Vasyliunas Dichotomization Momentum transfer via ...

Title: PowerPoint Presentation Last modified by: hiroshih Created Date: 1/1/1601 12:00:00 AM Document presentation format: Other titles

Plasma Vorticity in. Saturnian Magnetosphere. Daniel Morozoff. Raymond Walker. Steven Joy ... Probably not vorticity. Note 11 hour periodicity. ...

Total-P perturbation in the vortex Wavelet spectrum of Total-P Summary ... It most likely resulted from local reconnection at the current sheet thinned by vortex flow.

Sun pulse brightens considerably at time of solar wind density enhancement. ... Signatures associated with reconnection are observed at IMAGE and by the Tiger ...

Normal conditions Typical concentration of particles near Earths ~1 particle / cm3 ... and b/c Earth s magnetic field is not uniform If you are an ...

Solar wind plasma and magnetic field are excluded from the bubble. ... Separatrix. The Ring Current. Current = Moving Charge. J (electric current) ...

Using the Cusp to Study Magnetic Reconnection

Ringing the Magnetospheric Bell. Units: 1 nT; 0.1 mV/m. Magnetospheric eigen ... a) Solar wind buffeting causes ringing of the magneto- sphere ...

PRESSURE, CURRENTS AND THEIR RETRIEVABILITY: A STATUS REPORT ... Anisotropy: Assimilate PADs and/or use multi vantage point observations. IRIDIUM - HENA ...

Small- meso-scale simulations with nongyrotropic corrections ... Subsolar Region |Y| 1 Re. med resolution (1/4 Re) (1/4 Re) high resolution (1/16 Re) ...

AMI events show one, two or three narrow lines in the energy range from 120 to ... mean duration time is 4 minutes. only ~20% of 60 AMI events were ...

Layers of the Atmosphere

... of ULF turbulence. L. Rezeau. CETP/IPSL/Universit Pierre et Marie Curie. F. Sahraoui, D. Atti ... It can create the small scales where micro-physical ...

Title: Slide 1 Author: tims Last modified by: johandk Created Date: 8/22/2005 12:32:21 PM Document presentation format: A4 (210 x 297 mm) Company: BIRA-IASB

Local Time distribution of Polar Time-Energy Dispersion Events. Karra and ... subsolar point, energetic particles were observed to be precipatating into the ...

A new magnetization model for Mars. A magnetic history of Mars ... Mars' most intense magnetic fields. Purucker, 2002. Structural ... External field at Mars ...

Correlation of earthquake swarm activity with weather. A) Temperatures at Paradise and Camp Muir, B) cumulative precipitation at Paradise, C) Streamgage heights for ...

The Magnetospheric Cusp: A Quadrupole Trap and Stochastic Accelerator at the Planets Ravi Kinnera, Rob Sheldon University of Alabama in Huntsville

Lab. de Fis. Corpuscular -FIW474 sondas ! Prof. Marcelo Sant Anna Sala A-310 (LaCAM) e-mail: mms@if.ufrj.br

This April special section is first of two Polar special sections to be ... Polar flies through the region of emission seen by IMAGE: ...

Anomalous resistivity and the non-linear evolution of the ion-acoustic instability Panagiota Petkaki British Antarctic Survey, Cambridge Magnetic Reconnection Theory

Supersonic Field-Aligned Flow. On Reconnected Field Line. Distance along the field line ... 4. Supersonic ( 2.1 2.4) field-aligned flow in the wedge. 5. Axial ...

SOLAR EXTREME EVENTS AND GRATE GEOMAGNETIC STORMS. E.E. Antonova, M.V. Stepanova ... peak intensity of fluxes of relativistic electrons during grate magnetic storm. ...

Mona Kessel, NASA HQ Contributions by Jacob Bortnik, Seth Claudepierre, Nicola Fox, Shri Kanekal, Kris Kersten, Craig Kletzing, Lou Lanzerotti, Tony Lui, Barry Mauk ...

Title: PowerPoint Presentation Author: Freeman Last modified by: Luis Diaz-Santana Created Date: 3/16/2001 3:17:32 PM Document presentation format

(1) Finnish Meteorological Institute, Helsinki, Finland ... Dipolarization events. simultaneous at GOES and. POLAR and with injections ...

Princeton Plasma Physics Laboratory. In collaboration with Hantao Ji, ... separatrix. ion flow. electron flow. symmetry axes. Max ion speed is 1.084 vA at ...

... Region 2 system magnetometers see smaller scale FACs associated with discrete auroral formations What do ... Highest energy ions at poleward ...

Solar wind is made up of plasma, or a soup of charged particles. ... colorful sheet in the front shows the density and the balls represent points of ...

... to Jiasheng Chen, Jon Niehof, Mike Klida, Kate Whitaker, Brian Walsh, Charlotte Wong, Zhang Hui, ... the CDCs the field and particle pressures are strongly ...

Large and SmallScale Dynamics of Saturns Magnetosphere Nick Achilleos, Atmospheric Physics Laborator

Bow shock: - conversion of kinetic energy into thermal energy; ... Often the jets head towards the MP (in one case with a 20 angle relative to the ...

Part 1: Pre-THEMIS Launch ... THEMIS observed a hot flow anomaly (HFA) ... Polar should remain operational through THEMIS tail phase (confirm or disprove ...

Overview of Results from the Radio Plasma Imager RPI on IMAGE

Sponge: List the six layers of the Earth.

Once Upon a Time in the Electron Radiation Belts R. Friedel, G. Reeves, J. Koller, Y Chen, S. Zaharia, V. Jordanova ISR-1, Los Alamos National Laboratory, USA

Anomalously strong signal in high energy bins... electron tail? Soft x-ray array assembly ... Clear detection of Hall electromagnetic fields ...