'Solar wind pressure' diaporamas de présentation

First panel is the EFW spin fit (10.5 s) electric field in ~ dawn-dusk direction.

First panel is the EFW spin fit (10.5 s) electric field in ~ dawn-dusk direction. This measurement is dominated by waves with amplitudes >32 mV/m ptp during during every storm as indicated by SYM H (third panel). The second panel is the dawn-dusk electric field averaged

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The Origin of the Solar System

Note that the following lectures include animations and PowerPoint effects such as fly ins and transitions that require you to be in PowerPoint's Slide Show mode (presentation mode). The Origin of the Solar System. Chapter 19. Guidepost.

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20 09, December 12

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Bernard V. Jackson, P. Paul Hick, Andrew Buffington, Mario M. Bisi, John M. Clover

Bernard V. Jackson, P. Paul Hick, Andrew Buffington, Mario M. Bisi, John M. Clover Center for Astrophysics and Space Sciences, University of California at San Diego, LaJolla, CA, USA and Munetoshi Tokumaru Solar-Terrestrial Environment Laboratory, Nagoya University, Japan. Bernie.

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The Sun

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Chapter 7: Asteroids and Comets

Chapter 7: Asteroids and Comets. composition, origin, fate tail formation; the physics of sublimation. Review: asteroids. Mostly rocky bodies Found in the asteroid belt between Mars and Jupiter Also the Trojans at the Jupiter Lagrangian points The source of most meteorites

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B. CME in In-situ data sets at Earth

B. CME in In-situ data sets at Earth. Yuko Hada Chi- Ju Wu 2012/01/24. We select 4 events from CME catalog. ? All events are Halo CMEs. Today, I show you only March event. (Because I cannot study deeply. ). 2012/03/04. Left: SOHO/LASCO C2 Right: SOHO/LASCOC3.

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Spacedesign Asteroid Initiative Presentation

Spacedesign Asteroid Initiative Presentation. By Joseph M. Clay Presenter: Joseph M. Lepore Spacedesign Corporation 914 Main St. Suite 913 Houston, TX 77002 www.spacedesign.com. Forces on Asteroids. Summary of Orbital forces on an asteroid Gravity Collisions

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