Note
Click here to download the full example code
Sampling data from a 3D model
In this example we’ll see how to sample a 3D model output at arbitrary points within the model domain.
First, load the required modules.
from psipy.model import MASOutput
from psipy.data import sample_data
import astropy.constants as const
import astropy.units as u
import matplotlib.pyplot as plt
import numpy as np
Load a set of MAS output files, and get the number density variable from the model run.
Out:
Files Downloaded: 0%| | 0/3 [00:00<?, ?file/s]
rho002.hdf: 0%| | 0.00/8.02M [00:00<?, ?B/s]
vr002.hdf: 0%| | 0.00/7.96M [00:00<?, ?B/s]
br002.hdf: 0%| | 0.00/7.94M [00:00<?, ?B/s]
rho002.hdf: 0%| | 100/8.02M [00:00<2:48:31, 793B/s]
vr002.hdf: 0%| | 100/7.96M [00:00<2:52:23, 769B/s]
rho002.hdf: 1%| | 51.7k/8.02M [00:00<00:32, 248kB/s]
vr002.hdf: 0%| | 11.2k/7.96M [00:00<02:34, 51.5kB/s]
rho002.hdf: 3%|3 | 266k/8.02M [00:00<00:08, 903kB/s]
vr002.hdf: 1%| | 53.2k/7.96M [00:00<00:45, 175kB/s]
rho002.hdf: 9%|9 | 761k/8.02M [00:00<00:03, 2.12MB/s]
vr002.hdf: 2%|1 | 144k/7.96M [00:00<00:20, 384kB/s]
rho002.hdf: 21%|##1 | 1.69M/8.02M [00:00<00:01, 4.32MB/s]
vr002.hdf: 5%|4 | 385k/7.96M [00:00<00:08, 913kB/s]
rho002.hdf: 33%|###3 | 2.66M/8.02M [00:00<00:00, 5.94MB/s]
rho002.hdf: 43%|####3 | 3.45M/8.02M [00:00<00:00, 5.94MB/s]
vr002.hdf: 8%|8 | 656k/7.96M [00:00<00:06, 1.11MB/s]
rho002.hdf: 51%|##### | 4.07M/8.02M [00:01<00:01, 3.69MB/s]
vr002.hdf: 10%|9 | 762k/7.96M [00:01<00:11, 648kB/s]
rho002.hdf: 59%|#####9 | 4.73M/8.02M [00:01<00:00, 4.25MB/s]
vr002.hdf: 15%|#4 | 1.16M/7.96M [00:01<00:05, 1.20MB/s]
rho002.hdf: 66%|######5 | 5.26M/8.02M [00:01<00:00, 4.21MB/s]
vr002.hdf: 17%|#6 | 1.34M/7.96M [00:01<00:05, 1.23MB/s]
rho002.hdf: 72%|#######1 | 5.76M/8.02M [00:01<00:00, 4.08MB/s]
vr002.hdf: 20%|#9 | 1.57M/7.96M [00:01<00:04, 1.46MB/s]
rho002.hdf: 78%|#######7 | 6.22M/8.02M [00:01<00:00, 3.97MB/s]
rho002.hdf: 83%|########2 | 6.65M/8.02M [00:01<00:00, 3.36MB/s]
rho002.hdf: 88%|########7 | 7.02M/8.02M [00:01<00:00, 3.12MB/s]
rho002.hdf: 92%|#########1| 7.36M/8.02M [00:02<00:00, 2.43MB/s]
br002.hdf: 0%| | 100/7.94M [00:02<50:33:19, 43.6B/s]
rho002.hdf: 95%|#########5| 7.64M/8.02M [00:02<00:00, 2.41MB/s]
br002.hdf: 0%| | 10.7k/7.94M [00:02<21:18, 6.20kB/s]
br002.hdf: 1%| | 51.3k/7.94M [00:02<03:34, 36.7kB/s]
br002.hdf: 2%|2 | 164k/7.94M [00:02<00:55, 141kB/s]
vr002.hdf: 22%|##2 | 1.76M/7.96M [00:02<00:13, 476kB/s]
br002.hdf: 7%|6 | 535k/7.94M [00:02<00:12, 572kB/s]
vr002.hdf: 24%|##4 | 1.92M/7.96M [00:02<00:10, 556kB/s]
br002.hdf: 14%|#4 | 1.13M/7.94M [00:02<00:05, 1.35MB/s]
vr002.hdf: 29%|##8 | 2.29M/7.96M [00:02<00:06, 899kB/s]
vr002.hdf: 37%|###6 | 2.92M/7.96M [00:03<00:03, 1.60MB/s]
rho002.hdf: 99%|#########8| 7.90M/8.02M [00:03<00:00, 1.05MB/s]
Files Downloaded: 33%|###3 | 1/3 [00:03<00:07, 3.51s/file]
br002.hdf: 20%|## | 1.59M/7.94M [00:03<00:06, 1.02MB/s]
vr002.hdf: 40%|#### | 3.22M/7.96M [00:03<00:04, 1.10MB/s]
vr002.hdf: 43%|####3 | 3.45M/7.96M [00:03<00:03, 1.16MB/s]
br002.hdf: 23%|##2 | 1.82M/7.94M [00:03<00:06, 944kB/s]
vr002.hdf: 48%|####7 | 3.80M/7.96M [00:03<00:02, 1.44MB/s]
br002.hdf: 27%|##7 | 2.16M/7.94M [00:03<00:04, 1.21MB/s]
vr002.hdf: 57%|#####6 | 4.51M/7.96M [00:03<00:01, 2.35MB/s]
br002.hdf: 35%|###4 | 2.74M/7.94M [00:03<00:02, 1.87MB/s]
vr002.hdf: 64%|######3 | 5.07M/7.96M [00:04<00:00, 2.95MB/s]
br002.hdf: 42%|####2 | 3.34M/7.94M [00:04<00:01, 2.57MB/s]
vr002.hdf: 74%|#######4 | 5.91M/7.96M [00:04<00:00, 4.01MB/s]
br002.hdf: 47%|####7 | 3.75M/7.94M [00:04<00:01, 2.87MB/s]
vr002.hdf: 87%|########7 | 6.93M/7.96M [00:04<00:00, 5.41MB/s]
br002.hdf: 56%|#####6 | 4.48M/7.94M [00:04<00:00, 3.73MB/s]
Files Downloaded: 67%|######6 | 2/3 [00:04<00:02, 2.01s/file]
br002.hdf: 62%|######2 | 4.96M/7.94M [00:04<00:01, 1.84MB/s]
br002.hdf: 67%|######7 | 5.33M/7.94M [00:05<00:01, 1.97MB/s]
br002.hdf: 74%|#######4 | 5.88M/7.94M [00:05<00:00, 2.50MB/s]
br002.hdf: 85%|########4 | 6.75M/7.94M [00:05<00:00, 3.60MB/s]
br002.hdf: 92%|#########2| 7.33M/7.94M [00:05<00:00, 3.89MB/s]
br002.hdf: 99%|#########8| 7.85M/7.94M [00:05<00:00, 3.02MB/s]
Files Downloaded: 100%|##########| 3/3 [00:05<00:00, 1.69s/file]
Files Downloaded: 100%|##########| 3/3 [00:05<00:00, 1.92s/file]
Choose a set of 1D points to interpolate the model output at.
Here we keep a constant radius, and a set of longitudes that go all the way from 0 to 360 degrees. Then we choose two different, but close latitude values, and plot the results.
As expected, the values at 0 and 360 degrees are the same, and the profiles are similar, but different, due to the small difference in latitude.
fig, ax = plt.subplots()
npoints = 1000
r = 50 * np.ones(npoints) * const.R_sun
lon = np.linspace(0, 360, npoints) * u.deg
for latitude in [0, 1] * u.deg:
lat = latitude * np.ones(npoints)
samples = rho.sample_at_coords(lon, lat, r)
ax.plot(lon, samples, label='lat = ' + str(latitude))
ax.legend()
ax.set_xlim(0, 360)
ax.set_ylim(bottom=0)
ax.set_xlabel('Longitude (deg)')
ax.set_ylabel(r'$\rho$ (cm$^{-3}$)')
ax.set_xticks([0, 90, 180, 270, 360])
plt.show()
Total running time of the script: ( 0 minutes 6.200 seconds)