Influence of atmospheric composition on heat transfer and ablation is studied together with equilibrium convective heating, including boundary-layer mass addition; gas properties at relatively low temperatures near wall control heating rate and precise definition of transport properties at stagnation temperatures associated with entry is not necessary; correlation equation, in terms of relatively low-temperature freestream gas properties and suitably defined mass-addition parameter, is given; heating rates for no mass addition in Martian atmospheres are from 10 to 25% higher than those in nitrogen.


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    Title :

    Laminar convective heating and ablation in mars atmosphere


    Additional title:

    AIAA J


    Contributors:
    Marvin, J.G. (author) / Pope, R.B. (author)

    Published in:

    AIAA Journal ; 5 , n 2


    Publication date :

    1967


    Size :

    9 pages


    Type of media :

    Article (Journal)


    Type of material :

    Print


    Language :

    English


    Keywords :


    LAMINAR CONVECTIVE HEATING AND ABLATION IN THE MARS ATMOSPHERE

    MARVIN, JOSEPH / POPE, RONALD | AIAA | 1966



    Erratum: Laminar Convective Heating and Ablation in the Mars Atmosphere

    JOSEPH G. MARVIN AND RONALD B. POPE | AIAA | 1968


    METHOD OF HEATING MARS ATMOSPHERE

    POPOV ALEKSANDR FEDOROVICH | European Patent Office | 2017

    Free access