source: codes/icosagcm/devel/Python/test/py/RSW_MPAS_W02.py @ 682

Last change on this file since 682 was 680, checked in by dubos, 6 years ago

devel/unstructured : moved mesh partitioning code into meshes.py

File size: 2.8 KB
Line 
1print 'Loading DYNAMICO modules ...'
2from dynamico import unstructured as unst
3from dynamico.meshes import MPAS_Format, Unstructured_Mesh
4from dynamico import time_step
5print '...Done'
6
7print 'Loading modules ...'
8import math as math
9import matplotlib.pyplot as plt
10import numpy as np
11print '...Done'
12
13grid, llm, nqdyn = 10242, 1,1 # 2562, 10242, 40962
14Omega, radius, g, gh0 = 2.*np.pi/86400., 6.4e6, 1., 2.94e4
15N, T, courant = 40, 10800., 1.2 # simulation length = N*T
16
17print 'Omega, planetary PV', Omega, 2*Omega/gh0
18
19def f(lon,lat): return 2*Omega*np.sin(lat) # Coriolis parameter
20print 'Reading MPAS mesh ...'
21meshfile = MPAS_Format('grids/x1.%d.grid.nc'%grid)
22mesh=Unstructured_Mesh(meshfile, llm, nqdyn, radius, f)
23print '...Done'
24lon, lat = mesh.lon_i, mesh.lat_i
25x,y,z = np.cos(lat)*np.cos(lon), np.cos(lat)*np.sin(lon), np.sin(lat)
26
27unst.setvar('g',g)
28caldyn = unst.Caldyn_RSW(mesh)
29
30c0 = math.sqrt(gh0) # phase speed of barotropic mode
31dx = mesh.de.min()
32dt = courant*dx/c0
33nt = int(math.ceil(T/dt))
34dt = T/nt
35#scheme = time_step.RKn_simple(1,caldyn.bwd_fast_slow, dt)
36scheme = time_step.RK4(caldyn.bwd_fast_slow, dt)
37   
38print dx, dt, dt*c0/dx
39print T, nt
40
41#mesh.plot_e(mesh.le_de) ; plt.title('le/de') ; plt.show()
42#mesh.plot_i(mesh.Ai) ; plt.title('Ai') ; plt.show()
43
44#Phi0 = gh0*(1+0.1*np.exp(-2000.*(y+1.)**2))
45#flow = (Phi0,mesh.field_u())
46#for i in range(N):
47#    h,u=flow
48#    plot_i(h) ; plt.title('h'); plt.show()
49#    junk, fast, slow = caldyn.bwd_fast_slow(flow,0.)
50#    print i
51#    flow = scheme.advance(flow, nt)
52
53u0 = Omega*radius/12. # cf Williamson (1991), p.13
54gh1 = radius*Omega*u0+.5*u0**2
55print 'Williamson (1991) test 2, u0=', u0
56ulon = u0*np.cos(mesh.lat_e)
57Phi0 = gh0 - gh1*(np.sin(mesh.lat_i)**2)
58zeta0 = (2*u0/radius+2*Omega)*np.sin(mesh.lat_v)
59Phi0v = gh0 - (radius*Omega*u0+.5*u0**2)*(np.sin(mesh.lat_v)**2)
60q0 = zeta0/Phi0v
61fu_perp = mesh.ucov2D(0.*ulon,2*Omega*np.sin(mesh.lat_e)*ulon)
62
63flow = (Phi0,mesh.ucov2D(ulon,0.*ulon))
64for i in range(N):
65    h,u=flow
66    mesh.plot_i(h-Phi0) ; plt.title('err(gh)'); 
67    plt.savefig('fig_RSW_MPAS_W02/err_gh_%02d.png'%i)
68    plt.close()
69#    junk, fast, slow = caldyn.bwd_fast_slow(flow,0.)
70#    plot_i(slow[0]) ; plt.title('dh/dt'); plt.show()
71#    plot_e(slow[1]+fast[1]) ; plt.title('du/dt'); plt.show()
72#    plt.figure(); plt.plot(fu_perp,slow[1],'.');
73#    plt.xlabel('fu_perp'); plt.ylabel('u_slow'); plt.show()
74#    plt.figure(); plt.plot(fu_perp,fast[1],'.');
75#    plt.xlabel('fu_perp'); plt.ylabel('u_fast'); plt.show()
76#    plot_e(fast[1]) ; plt.title('u_fast'); plt.show()
77#    plot_e(slow[1]) ; plt.title('u_slow'); plt.show()
78#    plt.figure(); plt.plot(q0,caldyn.qv,'.');
79#    plt.xlabel('q0'); plt.ylabel('qv'); plt.show()
80    print i, h.min(), h.max()
81    flow = scheme.advance(flow, nt)
82
83print 'Time spent in DYNAMICO (s) : ', unst.getvar('elapsed')
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