'Termination shock' diaporamas de présentation

cosmic ray acceleration and shocks in heliosphere

cosmic ray acceleration and shocks in heliosphere. chung-ming ko institute of astronomy and department of physics, national central university, taiwan (R.O.C.). SC4, Lebedev Institute, Moscow, Russia, 2009.05.18. a short discussion on. cosmic ray acceleration basics propagation

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MHD Shocks and Collisionless Shocks

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Niagara Falls

Energetic Ion Fluxes in the TNO Region The New Outer Heliosphere Meets the New Outer Solar System John F. Cooper

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Outline Our place in the Galaxy The Local Interstellar Cloud (LIC)

The Voyagers at the Edge of the Heliospheric Bubble John D. Richardson (MIT) With thanks to the Voyager team and E. Mobius. Outline Our place in the Galaxy The Local Interstellar Cloud (LIC) The Solar Wind - LIC interaction The Voyagers at the Termination Shock The Future.

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observational evidences of CR acceleration at shocks

observational evidences of CR acceleration at shocks. chung-ming ko institute of astronomy and department of physics, national central university, taiwan. KAW4, KASI, Daejeon, Korea, 2006.05.17. shocks, shocks everywhere.

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5. Heliosphere and Intersteller gas

5. Heliosphere and Intersteller gas. Outline. Global Heliosphere; Neutral Intersteller gas; ENA imaging; IBEX mission and observation CASSINI mission and observation Summary. The Sun and Local Interstellar Medium (LISM). Image courtesy of L. Huff/P. Frisch. Our Heliosphere. Heliosphere.

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Niagara Falls

Energetic Ion Fluxes in the TNO Region The New Outer Heliosphere Meets the New Outer Solar System John F. Cooper

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Superdiffusive Transport at Shocks in Space Plasmas

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Electron Acceleration in the Solar Corona

Electron Acceleration in the Solar Corona. Gottfried Mann Astrophysikalisches Institut Potsdam, D-14482 Potsdam e-mail: GMann@aip.de. The Sun is an active star. flare ? heating the coronal plasma ? mass motions (jets, CMEs) ? enhanced emission of electromagnetic radiation

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Particle acceleration in Pulsar Wind Nebulae

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Cosmic Ray Acceleration Beyond the Knee up to the Ankle in the Galactic Wind Halo

Cosmic Ray Acceleration Beyond the Knee up to the Ankle in the Galactic Wind Halo. V.N. Zirakashvili 1,2 1 Institute for Terrestrial Magnetism, Ionosphere and Radiowave Propagation, Russian Academy of Sciences, 142190 Troitsk, Moscow Region, Russia

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Pulsar Wind Nebulae

Observations of. Pulsar Wind Nebulae. Jet/Torus Structure in PWNe. Anisotropic flux with maximum energy flux in equatorial zone - radial particle outflow - striped wind from Poynting flux decreases away from equator Wind termination shock is farther from

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Particle acceleration in collisionless shock with large scale magnetic field variation

Particle acceleration in collisionless shock with large scale magnetic field variation. Fan Guo, J. R. Jokipii and Jozsef Kota Lunar & Planetary Laboratory, Department of Planetary Sciences University of Arizona. Presentation at SHINE meeting, July 27th 2010.

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Electron Acceleration at the Solar Flare Reconnection Outflow Shocks

Electron Acceleration at the Solar Flare Reconnection Outflow Shocks. Gottfried Mann, Henry Aurass, and Alexander Warmuth Astrophysikalisches Institut Potsdam, An der Sternwarte 16, D-14482 Potsdam, Germany e-mail: GMann@aip.de. Huge solar event on October 28, 2003

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2003 Fall AGU San Francisco, CA 8 December 2003

Observations of the Anisotropies of Enhanced MeV Ion Fluxes at Voyager 1 at 85 AU A. C. Cummings and E. C. Stone, Caltech L. F. Burlaga, GSFC N. F. Ness , Bartol F. B. McDonald, U. Md. W. R. Webber, NMSU. 2003 Fall AGU San Francisco, CA 8 December 2003. Summary.

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Particle Acceleration at a Blunt Termination Shock Nathan Schwadron (BU) Marty Lee ( UNH)

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(relativistic) magneto-hydrodynamics of plerions basic paradigm and issues

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(relativistic) magneto-hydrodynamics of plerions basic paradigm and issues

86 views • 8 slides