Commit f6b28544 authored by Jason Reneuve's avatar Jason Reneuve
Browse files

changed strings to rstrings to avoid escape warnings

parent 4a59d2a0cb9f
Pipeline #3444 passed with stage
in 12 minutes and 51 seconds
......@@ -259,7 +259,7 @@ class SpectralEnergyBudgetNS3D(SpecificOutput):
if ax is None:
fig, ax = self.output.figure_axe()
ax.set_xlabel("$\kappa_h$")
ax.set_xlabel(r"$\kappa_h$")
ax.set_ylabel("$k_z$")
ax.set_title(
f"{key}, solver {self.output.name_solver}, nx = {self.nx:5d}"
......@@ -333,7 +333,7 @@ class SpectralEnergyBudgetNS3D(SpecificOutput):
fig, ax = self.output.figure_axe()
xlbl = "k_" + key_k[1]
ylbl = "$\Pi(" + xlbl + ")/\epsilon$"
ylbl = r"$\Pi(" + xlbl + r")/\epsilon$"
xlbl = "$" + xlbl + "$"
ax.set_xlabel(xlbl)
ax.set_ylabel(ylbl)
......@@ -342,11 +342,11 @@ class SpectralEnergyBudgetNS3D(SpecificOutput):
)
ax.semilogx(
k_plot, flux_tot / eps, "k", linewidth=2, label="$\Pi/\epsilon$"
k_plot, flux_tot / eps, "k", linewidth=2, label=r"$\Pi/\epsilon$"
)
ax.semilogx(k_plot, D / eps, "k--", linewidth=2, label="$D/\epsilon$")
ax.semilogx(k_plot, D / eps, "k--", linewidth=2, label=r"$D/\epsilon$")
ax.semilogx(
k_plot, (flux_tot + D) / eps, "k:", label="$(\Pi+D)/\epsilon$"
k_plot, (flux_tot + D) / eps, "k:", label=r"$(\Pi+D)/\epsilon$"
)
ax.legend()
......@@ -242,7 +242,7 @@ class SpectraNS3D(Spectra):
if ax is None:
fig, ax = self.output.figure_axe()
ax.set_xlabel("$\kappa_h$")
ax.set_xlabel(r"$\kappa_h$")
ax.set_ylabel("$k_z$")
ax.set_title(
"log 3D spectra, solver "
......
......@@ -264,6 +264,7 @@ class SpatialMeansNS3DStrat(SpatialMeansBase):
epsA_hypo = dict_results["epsA_hypo"]
eps_tot = dict_results["eps_tot"]
# fig 1 : energies
fig, ax = self.output.figure_axe()
fig.suptitle("Energy")
ax.set_ylabel("$E(t)$")
......@@ -275,13 +276,14 @@ class SpatialMeansNS3DStrat(SpatialMeansBase):
ax.legend()
# figure 2 : dissipations
fig, ax = self.output.figure_axe()
fig.suptitle("Dissipation of energy")
ax.set_ylabel(r"$\epsilon_K(t)$")
ax.plot(t, epsK, "r", linewidth=1, label=r"$\epsilon_K$")
ax.plot(t, epsA, "b", linewidth=1, label=r"$\epsilon_A$")
ax.plot(t, eps_tot, "k", linewidth=2, label=r"$\epsilon$")
ax.plot(t, epsK, "r", linewidth=1, label=r"$\epsilon_K$", zorder=10)
ax.plot(t, epsA, "b", linewidth=1, label=r"$\epsilon_A$", zorder=10)
ax.plot(t, eps_tot, "k", linewidth=2, label=r"$\epsilon$", zorder=10)
eps_hypo = epsK_hypo + epsA_hypo
if max(eps_hypo) > 0:
......@@ -291,7 +293,7 @@ class SpatialMeansNS3DStrat(SpatialMeansBase):
PK_tot = dict_results["PK_tot"]
PA_tot = dict_results["PA_tot"]
ax.plot(t, PK_tot, "r--", label=r"$P_K$")
ax.plot(t, PA_tot, "b--", label=r"$P_A$")
ax.plot(t, PK_tot, "r--", label=r"$P_K$", zorder=0)
ax.plot(t, PA_tot, "b--", label=r"$P_A$", zorder=0)
ax.legend()
......@@ -151,7 +151,7 @@ class SpectralEnergyBudgetNS3DStrat(SpectralEnergyBudgetNS3D):
fig, ax = self.output.figure_axe()
xlbl = "k_" + key_k[1]
ylbl = "$\Pi(" + xlbl + ")/\epsilon$"
ylbl = r"$\Pi(" + xlbl + r")/\epsilon$"
xlbl = "$" + xlbl + "$"
ax.set_xlabel(xlbl)
ax.set_ylabel(ylbl)
......@@ -160,16 +160,16 @@ class SpectralEnergyBudgetNS3DStrat(SpectralEnergyBudgetNS3D):
)
ax.semilogx(
k_plot, flux_tot / eps, "k", linewidth=2, label="$\Pi/\epsilon$"
k_plot, flux_tot / eps, "k", linewidth=2, label=r"$\Pi/\epsilon$"
)
ax.semilogx(k_plot, D / eps, "k--", linewidth=2, label="$D/\epsilon$")
ax.semilogx(k_plot, D / eps, "k--", linewidth=2, label=r"$D/\epsilon$")
ax.semilogx(
k_plot, (flux_tot + D) / eps, "k:", label="$(\Pi+D)/\epsilon$"
k_plot, (flux_tot + D) / eps, "k:", label=r"$(\Pi+D)/\epsilon$"
)
ax.semilogx(k_plot, flux_K / eps, "r", label="$\Pi_K/\epsilon$")
ax.semilogx(k_plot, flux_A / eps, "b", label="$\Pi_A/\epsilon$")
ax.semilogx(k_plot, DK / eps, "r--", label="$D_K/\epsilon$")
ax.semilogx(k_plot, DA / eps, "b--", label="$D_A/\epsilon$")
ax.semilogx(k_plot, CK2A / eps, "m", linewidth=2, label="$B/\epsilon$")
ax.semilogx(k_plot, flux_K / eps, "r", label=r"$\Pi_K/\epsilon$")
ax.semilogx(k_plot, flux_A / eps, "b", label=r"$\Pi_A/\epsilon$")
ax.semilogx(k_plot, DK / eps, "r--", label=r"$D_K/\epsilon$")
ax.semilogx(k_plot, DA / eps, "b--", label=r"$D_A/\epsilon$")
ax.semilogx(k_plot, CK2A / eps, "m", linewidth=2, label=r"$B/\epsilon$")
ax.legend()
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