1968
DOI: 10.1007/978-3-642-48927-3_5
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Entry Radiative Transfer

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Cited by 2 publications
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“…A strong function of orbital velocity, radiative heat flux starts to dominate stagnation heat flux for re-entry velocities approaching that of approximately 11.2 km∕s for a parabolic orbit [34]. Since orbital velocities associated with skip entry maneuvers are less than this threshold, then the convective mode of heat flux is considered to be the dominant form of energy transfer, with all radiative heat flux assumed to be negligible [35,36]. From this assumption, an estimate of convective, stagnation heat flux as a function of atmospheric density and orbital velocity is given by Eq.…”
Section: Deceleration and Heat Fluxmentioning
confidence: 99%
“…A strong function of orbital velocity, radiative heat flux starts to dominate stagnation heat flux for re-entry velocities approaching that of approximately 11.2 km∕s for a parabolic orbit [34]. Since orbital velocities associated with skip entry maneuvers are less than this threshold, then the convective mode of heat flux is considered to be the dominant form of energy transfer, with all radiative heat flux assumed to be negligible [35,36]. From this assumption, an estimate of convective, stagnation heat flux as a function of atmospheric density and orbital velocity is given by Eq.…”
Section: Deceleration and Heat Fluxmentioning
confidence: 99%