Remote Sensing of the Solar Wind with Radio Scattering and Scintillation Measurements
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The performance of an Earth-to-Space optical telecommunications system is degraded by distortion of the beam as it propagates through the turbulent atmosphere.
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Since radio propagation measurements using either natural or spacecraft radio signals are essentially our only means for probing the solar wind in the vicinity of the Sun, they represent a key tool for studying the interplanetary consequences of solar structure and dynamic phenomena.
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