From eb660ae70db40d36418f1e4eb886fd9bb02af1a7 Mon Sep 17 00:00:00 2001 From: Aaron LI Date: Fri, 23 Jun 2017 10:37:15 +0800 Subject: utils/convert.py: Use 'utils.units' module --- fg21sim/utils/convert.py | 13 +++++++------ 1 file changed, 7 insertions(+), 6 deletions(-) (limited to 'fg21sim/utils/convert.py') diff --git a/fg21sim/utils/convert.py b/fg21sim/utils/convert.py index fc9a228..1ada6ae 100644 --- a/fg21sim/utils/convert.py +++ b/fg21sim/utils/convert.py @@ -1,14 +1,15 @@ -# Copyright (c) 2016 Weitian LI +# Copyright (c) 2016-2017 Weitian LI # MIT license """ Utilities for conversion among common astronomical quantities. """ -import numpy as np import astropy.units as au import numba +from .units import (Constants as AC, UnitConversions as AUC) + def Fnu_to_Tb(Fnu, omega, freq): """Convert flux density to brightness temperature, using the @@ -92,11 +93,11 @@ def Sb_to_Tb_fast(Sb, freq): Calculated brightness temperature, unit [ K ] """ # NOTE: `radian` is dimensionless - rad2_to_deg2 = np.rad2deg(1.0) * np.rad2deg(1.0) + rad2_to_deg2 = AUC.rad2deg ** 2 Sb_rad2 = Sb * rad2_to_deg2 # unit: [ Jy/rad^2 ] -> [ Jy ] - c = 29979245800.0 # speed of light, [ cm/s ] - k_B = 1.3806488e-16 # Boltzmann constant, [ erg/K ] - coef = 1e-35 # take care the unit conversions + c = AC.c # speed of light, [ cm/s ] + k_B = AC.k_B # Boltzmann constant, [ erg/K ] + coef = 1e-35 # unit conversion factor Tb = coef * (Sb_rad2 * c*c) / (2 * k_B * freq*freq) # unit: [ K ] return Tb -- cgit v1.2.2