nonos is a Python 2D visualization library for planet-disk numerical simulations. It supports vtk-formatted data from Pluto and Idefix, and dat-formatted data for Fargo-adsg and Fargo3D.
For more, read the documentation !
We list here the accepted formats for the data: Pluto and Idefix: data.****.vtk Fargo-adsg: gasdens.dat, gasvy*.dat, gasvx*.dat Fargo3D: same as Fargo-adsg + gasvz*.dat
nonos
is considered public beta software: we are actively improving the
design and API, but we are not at the point where we want to bless the
current state as stable yet. We are trying to keep breaking changes to a
minimum, and run deprecation cycles to minimize the pain, however they might
happen in any minor release, so if you rely on nonos
for your own work
(thank you !), we strongly encourage you to follow along releases and
upgrade frequently, so we have more opportunities to discuss if something
breaks.
Get nonos and its minimal set of dependencies as
python -m pip install nonos
Optionally, you can install with the companion command line interface too
python -m pip install "nonos[cli]"
or, to also get all optional dependencies (CLI included)
python -m pip install "nonos[all]"
from nonos.api import GasDataSet
import matplotlib.pyplot as plt
plt.close("all")
# We use GasDataSet which takes as argument the output number of the output file given by idefix/pluto/fargo
# contains in particular a dictionary with the different fields.
ds = GasDataSet(43, geometry="polar", directory="nonos/tests/data/idefix_planet3d")
# We select the GasField "RHO", then
# we perform a vertical slice in the midplane,
# and make the result plotable in the xy plane,
# rotating the grid given the planet number 0
# (which orbit is described in the planet0.dat file).
dsop = ds["RHO"].vertical_at_midplane().map("x", "y", planet_corotation=0)
fig, ax = plt.subplots()
# dsop is now a Plotable object.
# We represent its log10, with a given colormap,
# and we display the colorbar by adding the argument title.
dsop.plot(fig, ax, log=True, cmap="inferno", title=r"$\rho_{\rm mid}$")
ax.set_aspect("equal")
# This time, we perform a latitudinal projection,
# i.e. the integral of "RHO" between -theta and theta,
# and then an azimuthal average,
# before mapping it in the radial ("R") direction.
dsop = ds["RHO"].latitudinal_projection(theta=3*0.05).azimuthal_average().map("R")
fig, ax = plt.subplots()
# We display the y-axis by adding the argument title.
dsop.plot(fig, ax, c="k", title=r"$\Sigma$")
plt.show()
requires matplotlib >= 3.7
nonos
CLI uses a custom style that can be reused programmatically, without
importing the package, using matplotlib API
import matplotlib.pyplot as plt
plt.style.use("nonos.default")
See matplotlib.style
's documentation for more.