The Cassini 2000 solar conjunction: ka-band and X-band signal propagation through the solar corona
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A change in the paradigm of coronal structure has emerged as a result of definitive measurements made with radio occultation, white-light (SOHO/LASCO), ultraviolet (SOHO/UVCS), and soft X-ray (Yohkoh) measurements.
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This experiment was part of a telecommunications demenstration to evaluate the advantage of Ka-band (32 GHz)over X-band (8.4 GHz).
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The Cassini spacecraft and its ground segment are currently testing a novel radio frequency multilink technology to perform radio science experiments.
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