The Solar Wind.pdf

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• <strong>The</strong> sector structure inferred from IMP satelliteobservations. Plus signs are away from the Sun andminus signs are toward the Sun.
Page 1 and 2: ESS 200CLectures 6 and 7The Solar W
Page 3 and 4: • Solar wind speeds (heavy lines)
Page 5 and 6: • It is useful to describe the so
Page 8 and 9: • The transition from subsonic to
Page 10 and 11: • For the solar wind to continue
Page 12 and 13: • Waves and turbulence?- One poss
Page 15: • In summary the outer layer of t
Page 19: ω > Sunv ϕϕSun r r- At large dis
Page 25 and 26: • The solar wind speed and densit
Page 27 and 28: • The Archimedean spiral associat
Page 30 and 31: • Until the 1990’s our knowledg
Page 32 and 33: • The heliospheric current sheet
Page 34 and 35: • Observations of a CME in space-
Page 36 and 37: • In some CMEs there areboth forw
Page 38 and 39: • Observations from Voyager 1 as

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