Source code for pyrfu.pyrf.pid_4sc

#!/usr/bin/env python
# -*- coding: utf-8 -*-

# 3rd party imports
import numpy as np
import xarray as xr

# Local imports
from ..mms.rotate_tensor import rotate_tensor
from .avg_4sc import avg_4sc
from .c_4_grad import c_4_grad
from .trace import trace
from .ts_scalar import ts_scalar
from .ts_tensor_xyz import ts_tensor_xyz

__author__ = "Louis Richard"
__email__ = "louisr@irfu.se"
__copyright__ = "Copyright 2020-2023"
__license__ = "MIT"
__version__ = "2.4.2"
__status__ = "Prototype"


[docs]def pid_4sc(r_mms, v_mms, p_mms, b_mms): r"""Compute Pi-D term using definition of [1]_ as : .. math:: Pi-D = - \Pi_{ij}D_{ij} with :math:`\Pi_{ij}` the deviatoric part of the pressure tensor : .. math:: \Pi_{ij} = P_{ij} - p\delta_{ij} p = \frac{1}{3}P_{ii} and :math:`D_{ij}` the deviatoric part of the strain tensor : .. math:: D_{ij} = \frac{1}{2}\left ( \partial_i u_j + \partial_j u_i \right ) - \frac{1}{3}\theta\delta_{ij} \theta = \nabla . u Parameters ---------- r_mms : list of xarray.DataArray Time series of the position of the 4 spacecraft. v_mms : list of xarray.DataArray Time series of the bulk velocities of the 4 spacecraft. p_mms : list of xarray.DataArray Time series of the pressure tensor of the 4 spacecraft. b_mms : list of xarray.DataArray Time series of the background magnetic field of the 4 spacecraft. Returns ------- pid : xarray.DataArray Time series of the Pi-D. References ---------- .. [1] Yang, Y., Matthaeus, W. H., Parashar, T. N., Wu, P., Wan, M., Shi, Y., et al. (2017). Energy transfer channels and turbulence cascade in Vlasov-Maxwell turbulence. Physical Review E, 95, 061201. doi : https://doi.org/10.1103/PhysRevE.95.061201 """ # Compute pressure tensor and background magnetic field at the center of # mass of the tetrahedron p_xyz = avg_4sc(p_mms) b_xyz = avg_4sc(b_mms) # Compute divergence and gradient tensor of the bulk velocity. Yang's # notation theta = c_4_grad(r_mms, v_mms, "div") grad_u = c_4_grad(r_mms, v_mms, "grad") # Define identity tensor identity_3d = np.zeros((len(grad_u), 3, 3)) np.einsum("jii->ji", identity_3d)[:] = 1 # strain tensor eps_xyz = (grad_u.data + np.transpose(grad_u.data, [0, 2, 1])) / 2 # Deviatoric part of the strain tensor d_xyz = eps_xyz - theta.data[:, np.newaxis, np.newaxis] * identity_3d / 2 d_xyz = ts_tensor_xyz(v_mms[0].time.data, d_xyz) # Convert tensors to field aligned coordinates d_fac = rotate_tensor(d_xyz, "fac", b_xyz, "pp") p_fac = rotate_tensor(p_xyz, "fac", b_xyz, "pp") # Isotropic scalar pressure press = trace(p_fac) / 3 # Deviatoric part of the pressure tensor pi_fac = p_fac.data - press.data[:, np.newaxis, np.newaxis] * identity_3d pi_fac = ts_tensor_xyz(v_mms[0].time.data, pi_fac) # Compute Pi-D pid = np.sum(np.sum(pi_fac.data * d_fac.data, axis=1), axis=1) pid = ts_scalar(v_mms[0].time.data, pid) # Flatten tensors d_flat = np.reshape(d_fac.data, [len(d_fac), 9]) pi_flat = np.reshape(pi_fac.data, [len(pi_fac), 9]) d_flat = d_flat[:, [0, 4, -1, 1, 2, 5]] pi_flat = pi_flat[:, [0, 4, -1, 1, 2, 5]] # Compute components of the double contraction sum d_coeff = xr.DataArray( d_flat * pi_flat, coords=[p_xyz.time.data, np.arange(1, 7)], dims=["time", "index"], ) return pid, d_coeff