Observing the Solar Wind with Interplanetary Scintillation

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The Sun's Atmosphere The Solar Corona (March 2006 eclipse). The Solar Wind: Expansion at supersonic speeds of the Corona through the solar system. Often two streams: “Fast” at ~750km/s and “slow” at ~350km/s. Space Weather: The impact of the solar wind and solar events such as Coronal Mass Ejections on the Earth's magnetic field and ionosphere.
Radio Measurements Line of sight to radio source Scintillation due to turbulent-scale density variations in the Solar Wind Time Lag ● Simultaneous measurements by two antennas show similar patterns of scintillation. ● Time-lag for maximum cross-correlation gives estimate of solar wind outflow speed.
Page 1: Observing the Solar Wind with Inter
Page 5 and 6: Cross-Correlation Cross-correlation
Page 7 and 8: Longer Baselines If longer baseline
Page 9 and 10: Tomography ● Many observations ta
Page 11 and 12: Tomography Co-rotating analysis Com
Page 13 and 14: Why EISCAT? ● ● ● ● Observi
Page 15 and 16: Radio Source Tracking ● ● ●
Page 17 and 18: Filter Settings Power Central Filte
Page 19 and 20: Median Sampling ● ● Data usuall
Page 21 and 22: 1420MHz System
Page 23: Summary ● EISCAT used for observi

Observing the Solar Wind with Interplanetary Scintillation

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