****************** Stochastic Forcing ****************** There is an option to apply a stochastic force field. See Nyx/Exec/DrivenTurbulence for an example; note that :: nyx.do_forcing = 1 must be set in the inputs file. The external forcing term in the momentum equation  (`[eq:momt] <#eq:momt>`__) is then given by .. math:: {\bf S}_{\rho \Ub} = \rho_b \mathbf{f} where the acceleration field :math:`\mathbf{f}(\mathbf{x},t)` is computed as inverse Fourier transform of the forcing spectrum :math:`\widehat{\mathbf{f}}(\mathbf{k},t`). The time evolution of each wave mode is given by an Ornstein-Uhlenbeck process (see :raw-latex:`\cite{SchmHille06,Schmidt14}` for details). Since the real space forcing acts on large scales :math:`L`, non-zero modes are confined to a narrow window of small wave numbers with a prescribed shape (the forcing profile). The resulting flow reaches a statistically stationary and isotropic state with a root-mean-square velocity of the order :math:`V=L/T`, where the integral time scale :math:`T` (also known as large-eddy turn-over time) is usually set equal to the autocorrelation time of the forcing. It is possible to vary the force field from solenoidal (divergence-free) if the weight parameter :math:`\zeta=1` to dilational (rotation-free) if :math:`\zeta=0`. To maintain a nearly constant root-mean-square Mach number, a simple model for radiative heating and cooling around a given equilibrium temperature :math:`T_0` is applied in the energy equation (`[eq:energy] <#eq:energy>`__): .. math:: S_{\rho E} = S_{\rho e} + \Ub \cdot {\bf S}_{\rho \Ub} = -\frac{\alpha k_{\rm B}(T-T_0)}{\mu m_{\rm H}(\gamma-1)} + \rho_b\Ub\cdot\mathbf{f} The parameters :math:`T_0` and :math:`\alpha` correspond to temp0 and alpha, respectively, in the probin file (along with rho0 for the mean density, which is unity by default). While the gas is adiabatic for :math:`\alpha=0`, it becomes nearly isothermal if the cooling time scale given by :math:`1/\alpha` is chosen sufficiently short compared to :math:`T`. For performance reasons, a constant composition (corresponding to constant molecular weight :math:`\mu`) is assumed. List of Parameters ================== +-------------------------+--------------------+-----------------+-------------+ | Parameter | Definition | Acceptable | Default | | | | Values | | +=========================+====================+=================+=============+ | **forcing.seed** | seed of the | Integer | 27011974 | | | random number | :math:`>0` | | | | generator | | | +-------------------------+--------------------+-----------------+-------------+ | **forcing.profile** | shape of | 1 (plane), 2 | 3 | | | forcing | (band), 3 | | | | spectrum | (parabolic) | | +-------------------------+--------------------+-----------------+-------------+ | **forcing.alpha** | ratio of domain | Integer | 2 2 2 | | | size :math:`X` | :math:`>0` | | | | to integral | | | | | length | | | | | :math:`L=X/\alpha` | | | | | | | | +-------------------------+--------------------+-----------------+-------------+ | **forcing.band_width** | band width of | Real | 1.0 1.0 1.0 | | | the forcing | :math:`\ge 0` | | | | spectrum | and | | | | relative to | :math:`\le 1` | | | | alpha | | | +-------------------------+--------------------+-----------------+-------------+ | **forcing.intgr_vel** | characteristic | Real | must be set | | | velocity | :math:`> 0` | | | | :math:`V` | | | +-------------------------+--------------------+-----------------+-------------+ | **forcing.auto_corrl** | autocorrelation | Real | 1.0 1.0 1.0 | | | time in units | :math:`> 0` | | | | of | | | | | :math:`T=L/V` | | | +-------------------------+--------------------+-----------------+-------------+ | **forcing.soln_weight** | weight | Real | 1.0 | | | :math:`\zeta` | :math:`\ge 0` | | | | of solenoidal | and | | | | relative to | :math:`\le 1` | | | | dilatational | | | | | modes | | | +-------------------------+--------------------+-----------------+-------------+ Triples for forcing.alpha, forcing.band_width, forcing.intgr_vel, and forcing.auto_corrl correspond to the three spatial dimensions.