'Dense plasma' presentation slideshows

Exploring the Solar Wind with Ultraviolet Light

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M up

M up. Oscar Straniero & 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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Abstract

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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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INTRODUCTION

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