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The radiative flux from the Huygens probe during entry into Titan is modeled. This simulated radiative flux directed back to Earth is shown to be below the lower limit of a measurement made during Huygens entry. This result is consistent with the lack of a measurable shock-layer component being seen in this measurement.
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This page is a summary of: Analysis of Huygens Entry Observation to Inform Titan Shock-Layer Radiation Models, Journal of Thermophysics and Heat Transfer, November 2021, American Institute of Aeronautics and Astronautics (AIAA),
DOI: 10.2514/1.t6453.
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