volume-density-mapper 0.1.0

Reconstructs 3D density distributions from 2D column density maps using constrained diffusion.

This project provides Python functions to reconstruct a 3D density distribution from a 2D column density map using a multi-scale decomposition approach based on constrained diffusion. This method is particularly useful in astrophysics for analyzing gas and dust distributions.

Features

• compute_mean_density_width(column_density, dx): Derives the mean density and characteristic widths from a column density map.

• density_reconstruction_3d(data_in, dx): The main function to perform the full 3D density reconstruction from a 2D column density map.

Installation

To use this code, you need to install the following Python packages:

• numpy

• scipy

• matplotlib

• astropy

• constrained-diffusion (This is the cdd module used for the core decomposition.)

You can install these using pip:

pip install numpy scipy matplotlib astropy
pip install constrained-diffusion

If constrained-diffusion is a custom package, clone and install it from its repository:

git clone https://github.com/gxli/Volume-Density-Mapper
cd Volume-Density-Mapper
pip install .

pip install -e .

Example Usage

This example demonstrates how to:

• Estimate characteristic widths and mean density using compute_mean_density_width.

• Construct a 3D density cube using density_reconstruction_3d.

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

import matplotlib.pyplot as plt
import numpy as np
from astropy.io import fits
from volume_density_mapper import *

# --- Load Data and Define Constants ---
nh = fits.getdata('IC348_nh.fits')
header = fits.getheader('IC348_nh.fits')
mh2 = 1.34 * 3.34e-24  # Mass of H2 molecule in g
pc = 3.08e18           # Parsec in cm
dx = header['CDELT2'] / 180 * np.pi * 270 * pc  # Pixel size in cm

# --- Compute Mean Density and Width ---
input_map = nh * mh2
density, width = compute_mean_density_width(input_map, dx)

# --- Reconstruct 3D Density Structure ---
data3d = density_reconstruction_3d(input_map, dx)

print(np.shape(data3d))

Example

import matplotlib.pyplot as plt
import matplotlib as mpl
from matplotlib import cm
import numpy as np
from astropy.io import fits
from astropy import constants as cons
from volume_density_mapper import *



nh = fits.getdata('IC348_nh.fits')
header = fits.getheader('IC348_nh.fits')
mh2 = 1.34*3.34e-24
pc = 3.08e18

plt.figure(dpi = 100)
plt.imshow(np.log10(nh * mh2), origin = 'lower')

plt.colorbar(label=r'Log(surface density ($\rm g cm^{-2}$))')



# charactersitic scale (width) measurements
input_map = nh.copy() * mh2
dx = header['CDELT2']/180*np.pi*270 * pc
#pixel size, the same unit with that of output
density, width = compute_mean_density_width(input_map, dx)

plt.figure(dpi = 100)
plt.imshow(np.log10(density), origin = 'lower')
plt.colorbar(label = r'log(Volume Density (r$g\;cm^{-3}$))')


plt.figure(dpi = 100)
plt.imshow(np.log10(width), origin = 'lower',cmap = 'magma')
plt.colorbar(label = r'log(width (cm))')

plt.show()

# restructure the density structure in 3D space

data_in = nh * mh2 # convert to cgs unit
dx = header['CDELT2']/180*np.pi*270 * pc #pixel size, unit as cm (cgs unit)
data3d = density_reconstruction_3d(data_in, dx)

print(np.shape(data3d))

License

This project is open-source and available under the MIT License.