Dense plasma - PowerPoint PPT Presentation

Exploring the Solar Wind with Ultraviolet Light

Exploring the Solar Wind with Ultraviolet Light. Steven R. Cranmer and the UVCS/SOHO Team Harvard-Smithsonian Center for Astrophysics. Outline: Motivation &amp; history How does the Sun “expel” the hot solar wind? Modern space-based observations: SOHO (Solar and Heliospheric Observatory)

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518 views • 35 slides

M up

M up. Oscar Straniero &amp; Luciano Piersanti --------- INAF - Osservatorio di Teramo. where: Z o =0.02 Y o =0.28. Becker and Iben 1979. Status of the art. CLASSICAL MODELS (bare Schwarzschild criterion). In order of appearance: Siess 2007. versus

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426 views • 31 slides

Abstract

Computationally efficient description of relativistic electron beam transport in dense plasma Oleg Polomarov*, Adam Sefkov**, Igor Kaganovich** and Gennady Shvets* *IFS, The University of Texas at Austin, TX, 78712; **PPPL, Princeton, NJ 08543 . Abstract.

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374 views • 21 slides

Plumes in the Inner Magnetosphere

Plumes in the Inner Magnetosphere. INNER MAGNETOSPHERE Even very simple m odels do a pretty good job of predicting plumes in the inner magnetosphere. The trick is to extend those predictions to the magnetopause. Example of a Very Simple Model: Plasmapause Test Particle (PTP) Code

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240 views • 3 slides

INTRODUCTION

(Å). H 2. H 2. 1 2. Group Equilibrium and Transport in Plasmas Department of Applied Physics P.O. Box 513, 5600 MB Eindhoven The Netherlands. Ro-vibrational excitation of hydrogen formed by association in a very dense expanding plasma. P. Vankan , D.C. Schram, S.B.S. Heil, and R. Engeln.

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115 views • 1 slides

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