• Home
  • Current congress
  • Public Website
  • My papers
  • root
  • browse
  • IAC-08
  • E2
  • 1
  • paper
  • Numerical Simulation of Nitrogen Nozzle Expansion using Kinetic and Continuum Approaches

    Paper number

    IAC-08.E2.1.4

    Author

    Mr. Martin Grabe, DLR German Aerospace Center, Germany

    Year

    2008

    Abstract
    Attitude control of satellites is often accomplished by expanding a gas through the nozzle of small thrusters. The
    very low background pressure leads to a heavily underexpanded plume, which may impinge on the surrounding
    surfaces causing contamination, thermal loads and unwanted forces. A thorough understanding of the plume
    expansion is thus of high importance for the design of the spacecraft and its mission.
    Experimental investigations of nozzle expansion in a spacelike
    environment are quite intricate and numerical
    methods may help to evaluate many technical configurations much more quickly. A gas expansion into vacuum
    involves a drastic decrease in density over several orders of magnitude, which causes the continuum assumption
    inherent in the wellknown
    NavierStokesequations
    of fluid mechanics to fail. Hence the classical methods of
    Computational Fluid Dynamics (CFD), relying on these equations, will produce wrong results in the domain of
    high rarefaction, where nonequilibrium
    effects prevail.
    The well tried engineering method of choice for rarefied gas flows is termed Direct Simulation Monte Carlo
    (DSMC), a probabilistic simulation method which recognizes the molecular nature of the gas. DSMC is capable
    to accurately simulate gas flows over a wide range of densities and is able to capture nonequilibrium
    effects
    without additional modelling and assumptions. However, the method is computationally expensive, particularly
    in regions of high density. It is thus attempted to use CFD to model the nearisentropic
    core of the nozzle flow
    and use DSMC for the nonequilibrium
    regions to save on computer resources and time. The line along which
    the two methods are coupled is determined by a suitable continuumbreakdown
    parameter from the CFD
    solution. Since the expanding flow is for the most part hypersonic, it is initially assumed that the DSMC solution
    will not influence the flow in the continuum domain (downstream coupling). Density, temperature and velocity
    are extracted along the coupling boundary from the continuum solution and set as boundary values for the
    particle method.
    In the investigated case of the axisymmetric nitrogen expansion from a conical nozzle, the isolines of the applied
    breakdownparameters
    were found to be nearly parallel to the flow for most part of the expansion. This
    corresponds to a de facto effusion if viewed from a point moving with the flow, i. e. a considerable number of
    particle leaves the DSMC domain towards the continuum zone simply because of their thermal velocity
    component. This particle flux is not accounted for in a pure downstream coupling and leads to an unphysical
    discontinuity in density over the boundary between the two domains. While the results thus obtained are not
    satisfactory near the nozzle exit plane, they agree well with experimental results in the farfield of the plume.
    A simple downstream coupling of kinetic and continuum approaches to accurately and efficiently simulate a gas
    expanding into vacuum is found to be insufficient, contrary to previous assumptions. Better results in the
    nearfield of the plume may be obtained by continuously updating the solution in the continuum domain using
    the results of the DSMC solution.
    Abstract document

    IAC-08.E2.1.4.pdf

    Manuscript document

    IAC-08.E2.1.4.pdf (🔒 authorized access only).

    To get the manuscript, please contact IAF Secretariat.