diff options
Diffstat (limited to 'fg21sim/galactic')
| -rw-r--r-- | fg21sim/galactic/__init__.py | 1 | ||||
| -rw-r--r-- | fg21sim/galactic/freefree.py | 227 |
2 files changed, 228 insertions, 0 deletions
diff --git a/fg21sim/galactic/__init__.py b/fg21sim/galactic/__init__.py index 4fe2659..ebf7999 100644 --- a/fg21sim/galactic/__init__.py +++ b/fg21sim/galactic/__init__.py @@ -2,3 +2,4 @@ # MIT license from .synchrotron import Synchrotron +from .freefree import FreeFree diff --git a/fg21sim/galactic/freefree.py b/fg21sim/galactic/freefree.py new file mode 100644 index 0000000..9a51777 --- /dev/null +++ b/fg21sim/galactic/freefree.py @@ -0,0 +1,227 @@ +# Copyright (c) 2016 Weitian LI <liweitianux@live.com> +# MIT license + +""" +Diffuse Galactic free-free emission simulations. +""" + +import os +import logging +from datetime import datetime, timezone + +import numpy as np +from astropy.io import fits +import astropy.units as au +import healpy as hp + +from ..utils import read_fits_healpix, write_fits_healpix + + +logger = logging.getLogger(__name__) + + +class FreeFree: + """Simulate the diffuse Galactic free-free emission. + + The [Dickinson2003] method is followed to derive the free-free template. + The H\alpha survey map [Finkbeiner2003] is first corrected for dust + absorption using the infrared 100-\mu{}m dust map [Schlegel1998], + and then converted to free-free emission map (brightness temperature). + + Parameters + ---------- + configs : ConfigManager object + An `ConfigManager` object contains default and user configurations. + For more details, see the example config specification. + + Attributes + ---------- + ??? + + References + ---------- + .. [Dickinson2003] + Dickinson, C.; Davies, R. D.; Davis, R. J., + "Towards a free-free template for CMB foregrounds", + 2003, MNRAS, 341, 369, + http://adsabs.harvard.edu/abs/2003MNRAS.341..369D + + .. [Finkbeiner2003] + Finkbeiner, Douglas P., + "A Full-Sky Hα Template for Microwave Foreground Prediction", + 2003, ApJS, 146, 407, + http://adsabs.harvard.edu/abs/2003ApJS..146..407F + + .. [Schlegel1998] + Schlegel, David J.; Finkbeiner, Douglas P.; Davis, Marc, + "Maps of Dust Infrared Emission for Use in Estimation of Reddening + and Cosmic Microwave Background Radiation Foregrounds", + 1998, ApJ, 500, 525, + http://adsabs.harvard.edu/abs/1998ApJ...500..525S + """ + def __init__(self, configs): + self.configs = configs + self._set_configs() + self._load_halphamap() + self._load_dustmap() + + def _set_configs(self): + """Load the configs and set the corresponding class attributes.""" + self.halphamap_path = self.configs.get_path( + "galactic/freefree/halphamap") + self.halphamap_unit = au.Unit( + self.configs.getn("galactic/freefree/halphamap_unit")) + self.dustmap_path = self.configs.get_path( + "galactic/freefree/dustmap") + self.dustmap_unit = au.Unit( + self.configs.getn("galactic/freefree/dustmap_unit")) + # output + self.prefix = self.configs.getn("galactic/freefree/prefix") + self.save = self.configs.getn("galactic/freefree/save") + self.output_dir = self.configs.get_path( + "galactic/freefree/output_dir") + self.filename_pattern = self.configs.getn("output/filename_pattern") + self.use_float = self.configs.getn("output/use_float") + self.clobber = self.configs.getn("output/clobber") + logger.info("Loaded and set up configurations") + + def _load_halphamap(self): + """Load the H{\alpha} map, and upgrade/downgrade the resolution + to match the output Nside.""" + self.halphamap, self.halphamap_header = read_fits_healpix( + self.halphamap_path) + halphamap_nside = self.halphamap_header["NSIDE"] + logger.info("Loaded H[alpha] map from {0} (Nside={1})".format( + self.halphamap_path, halphamap_nside)) + # TODO: Validate & convert unit + if self.halphamap_unit != au.Unit("Rayleigh"): + raise ValueError("unsupported Halpha map unit: {0}".format( + self.halphamap_unit)) + # Upgrade/downgrade resolution + if halphamap_nside != self.nside: + self.halphamap = hp.ud_grade(self.halphamap, nside_out=self.nside) + logger.info("Upgrade/downgrade H[alpha] map from Nside " + "{0} to {1}".format(halphamap_nside, self.nside)) + + def _load_dustmap(self): + """Load the dust map, and upgrade/downgrade the resolution + to match the output Nside.""" + self.dustmap, self.dustmap_header = read_fits_healpix( + self.dustmap_path) + dustmap_nside = self.dustmap_header["NSIDE"] + logger.info("Loaded dust map from {0} (Nside={1})".format( + self.dustmap_path, dustmap_nside)) + # TODO: Validate & convert unit + if self.dustmap_unit != au.Unit("MJy / sr"): + raise ValueError("unsupported dust map unit: {0}".format( + self.dustmap_unit)) + # Upgrade/downgrade resolution + if dustmap_nside != self.nside: + self.dustmap = hp.ud_grade(self.dustmap, nside_out=self.nside) + logger.info("Upgrade/downgrade dust map from Nside " + "{0} to {1}".format(dustmap_nside, self.nside)) + + def _correct_dust_absorption(self): + """Correct the H{\alpha} map for dust absorption using the + 100-{\mu}m dust map. + + References: [Dickinson2003], Eq.(3) + """ + if hasattr(self, "dust_corrected") and self.dust_corrected: + return + # + # Effective dust fraction in the LoS actually absorbing Halpha + f_dust = 0.33 + halphamap_corr = self.halphamap * 10**(self.dustmap * 0.0185 * f_dust) + self.halphamap = halphamap_corr + self.dust_corrected = True + + def _calc_ratio_a(self, Te, nu_GHz): + """Calculate the ratio factor a(T, nu), which will be used to + transform the Halpha emission (Rayleigh) to free-free emission + brightness temperature (mK). + + References: [Dickinson2003], Eq.(8) + """ + term1 = 0.366 * nu_GHz**0.1 * Te**(-0.15) + term2 = np.log(4.995e-2 / nu_GHz) + 1.5*np.log(Te) + a = term1 * term2 + return a + + def _simulate_frequency(self, frequency): + """Simulate the free-free map at the specified frequency. + + References: [Dickinson2003], Eq.(11) + + NOTE: [Dickinson2003], Eq.(11) may wrongly have the "10^3" term. + """ + # Assumed electron temperature [ K ] + Te = 7000.0 + T4 = Te / 1e4 + nu = frequency * self.freq_unit.to(au.GHz) # frequency [ GHz ] + ratio_a = self._calc_ratio_a(T4, nu) + # NOTE: ignored the "10^3" term in the referred equation + ratio_mK_R = (8.396 * ratio_a * nu**(-2.1) * + T4**0.667 * 10**(0.029/T4) * (1+0.08)) + # Use "Kelvin" as the brightness temperature unit + ratio_K_R = ratio_mK_R * au.mK.to(au.K) + hpmap_f = self.halphamap * ratio_K_R + return hpmap_f + + def _make_header(self): + """Make the header with detail information (e.g., parameters and + history) for the simulated products. + """ + header = fits.Header() + header["COMP"] = ("Galactic free-free emission", + "Emission component") + header["CREATOR"] = (__name__, "File creator") + # TODO: + history = [] + comments = [] + for hist in history: + header.add_history(hist) + for cmt in comments: + header.add_comment(cmt) + self.header = header + logger.info("Created FITS header") + + def output(self, hpmap, frequency): + """Write the simulated free-free map to disk with proper header + keywords and history. + """ + if not os.path.exists(self.output_dir): + os.mkdir(self.output_dir) + logger.info("Created output dir: {0}".format(self.output_dir)) + # + filename = self.filename_pattern.format(prefix=self.prefix, + frequency=frequency) + filename += ".fits" + filepath = os.path.join(self.output_dir, filename) + if not hasattr(self, "header"): + self._make_header() + header = self.header.copy() + header["FREQ"] = (frequency, "Frequency [ MHz ]") + header["DATE"] = ( + datetime.now(timezone.utc).astimezone().isoformat(), + "File creation date" + ) + if self.use_float: + hpmap = hpmap.astype(np.float32) + write_fits_healpix(filepath, hpmap, header=header, + clobber=self.clobber) + logger.info("Write simulated map to file: {0}".format(filepath)) + + def simulate(self, frequencies): + """Simulate the free-free map at the specified frequencies.""" + self._correct_dust_absorption() + # + hpmaps = [] + for f in np.array(frequencies, ndmin=1): + logger.info("Simulating free-free map at {0} ({1}) ...".format( + f, self.freq_unit)) + hpmap_f = self._simulate_frequency(f) + hpmaps.append(hpmap_f) + if self.save: + self.output(hpmap_f, f) + return hpmaps |