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Solar and Heliospheric Physics CSI 769 / ASTR 769 Spring 2008 Jie Zhang What Physics? •Plasma Physics •MHD (Magnetohydrodynamics) Physics •Magnetism •Magnetic Reconnection •Particle Acceleration The Cosmological Context We are located in the middle of the Milky Way Galaxy 28,000 light years from the center One of 200 billion stars in our Galaxy The Sun: an Ordinary Star •An ordinary main sequence star •5 billion years old •5 billion years more to go Local Interstellar space Solar wind creates a big teardropshaped heliosphere around the solar system, by interacting with the interstellar wind Local Interplanetary Space The Earth 3rd planet from the Sun 1 AU = 150 million km Travel time: By light -8 minutes By Solar Wind- ~ 100 hrs What Practical Usage? "Space weather describes the conditions in space that affect Earth and its technological systems. Our space weather is a consequence of the behavior of the sun, the nature of Earth's magnetic field, and our location in the solar system” ----National Academy of Science, 1997 Space Weather: the Process It starts from an eruption from the Sun. Prediction depends on how it propagates Space Weather: effects Aurora; Geomagnetic Storm From Space Space Weather: effects An adverse effect Power failure due to March 1989 storm Damaged transformer Space Weather: effects On Human Space Exploration On crew and passengers of polar-route airplanes Space Weather: effects On Satellite Operation Space Weather: effects On Communication and Navigation Space Weather: the Systems The Source of the Energy? Planet Magnetic energy through magnetic field generated by solar dynamo, which has 11-year solar cycle Solar Cycle Storage of Energy? Planet Energy stored and released in magnetic field Release of Energy and the driver? Planet Coronal mass ejections Heliosphere: solar wind Planet Spiral solar wind magnetic field: radial motion of solar wind combined with Sun’s rotation Sprinkler Analogy Magnetosphere Planet A cometshaped region around the Earth Magnetosphere Planet Electric Currents in Magnetosphere Magnetosphere Planet Energetic particles in Van Allen radiation belt Ionosphere Planet Density fluctuation affects radio wave reflection and transmission Neutral Upper Atmosphere Planet It is coupled with ionosphere Re-focus on Physics •Energy Storage: magnetism •Energy Release: magnetic reconnection •Energy Transportation The End