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Observing the Solar Wind with Interplanetary Scintillation

Observing the Solar Wind with Interplanetary Scintillation

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Tomography<br />

●<br />

Many observations taken as Sun<br />

rotates results, in <strong>the</strong> Sun's<br />

frame of reference, in many<br />

overlapping lines of sight<br />

between antennas and radio<br />

sources.<br />

●<br />

These used to create a<br />

“tomographic” image of <strong>the</strong> inner<br />

heliosphere in both g-level and<br />

solar wind speed.<br />

After Manoharan, 2008

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