The entry probe of the Galileo mission to Jupiter entered the planet's atmosphere in 1995 in fiery fashion, generating enough heat to cause plasma reactions on its surface. The data relayed about the burning of its heat shield differed from the effects predicted in fluid dynamics models, and new work examines what might have caused such a discrepancy. Researchers now report their findings from new fluid radiative dynamics models.
from Top Technology News -- ScienceDaily https://ift.tt/2Bax7u9
Tuesday, 15 October 2019
Analysis of Galileo's Jupiter entry probe reveals gaps in heat shield modeling
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