Source code for pysme.atmosphere.krzfile

# -*- coding: utf-8 -*-
import re
from os.path import basename

import numpy as np

from ..abund import Abund
from .atmosphere import Atmosphere


# Atmoic mass from mendeleev package.
atmoic_mass = {
    'H': 1.008, 'He': 4.002602, 'Li': 6.94, 'Be': 9.0121831, 'B': 10.81, 'C': 12.011, 'N': 14.007, 'O': 15.999, 'F': 18.998403163, 'Ne': 20.1797, 'Na': 22.98976928, 'Mg': 24.305, 'Al': 26.9815385, 'Si': 28.085, 'P': 30.973761998, 'S': 32.06, 'Cl': 35.45, 'Ar': 39.948, 'K': 39.0983, 'Ca': 40.078, 'Sc': 44.955908, 'Ti': 47.867, 'V': 50.9415, 'Cr': 51.9961, 'Mn': 54.938044, 'Fe': 55.845, 'Co': 58.933194, 'Ni': 58.6934, 'Cu': 63.546, 'Zn': 65.38, 'Ga': 69.723, 'Ge': 72.63, 'As': 74.921595, 'Se': 78.971, 'Br': 79.904, 'Kr': 83.798, 'Rb': 85.4678, 'Sr': 87.62, 'Y': 88.90584, 'Zr': 91.224, 'Nb': 92.90637, 'Mo': 95.95, 'Tc': 97.90721, 'Ru': 101.07, 'Rh': 102.9055, 'Pd': 106.42, 'Ag': 107.8682, 'Cd': 112.414, 'In': 114.818, 'Sn': 118.71, 'Sb': 121.76, 'Te': 127.6, 'I': 126.90447, 'Xe': 131.293, 'Cs': 132.90545196, 'Ba': 137.327, 'La': 138.90547, 'Ce': 140.116, 'Pr': 140.90766, 'Nd': 144.242, 'Pm': 144.91276, 'Sm': 150.36, 'Eu': 151.964, 'Gd': 157.25, 'Tb': 158.92535, 'Dy': 162.5, 'Ho': 164.93033, 'Er': 167.259, 'Tm': 168.93422, 'Yb': 173.045, 'Lu': 174.9668, 'Hf': 178.49, 'Ta': 180.94788, 'W': 183.84, 'Re': 186.207, 'Os': 190.23, 'Ir': 192.217, 'Pt': 195.084, 'Au': 196.966569, 'Hg': 200.592, 'Tl': 204.38, 'Pb': 207.2, 'Bi': 208.9804, 'Po': 209.0, 'At': 210.0, 'Rn': 222.0, 'Fr': 223.0, 'Ra': 226.0, 'Ac': 227.0, 'Th': 232.0377, 'Pa': 231.03588, 'U': 238.02891, 'Np': 237.0, 'Pu': 244.0, 'Am': 243.0, 'Cm': 247.0, 'Bk': 247.0, 'Cf': 251.0, 'Es': 252.0, 'Fm': 257.0, 'Md': 258.0, 'No': 259.0, 'Lr': 262.0, 'Rf': 267.0, 'Db': 268.0, 'Sg': 271.0, 'Bh': 274.0, 'Hs': 269.0, 'Mt': 276.0, 'Ds': 281.0, 'Rg': 281.0, 'Cn': 285.0, 'Nh': 286.0, 'Fl': 289.0, 'Mc': 288.0, 'Lv': 293.0, 'Ts': 294.0, 'Og': 294.0
    }

[docs]class KrzFile(Atmosphere): """Read .krz atmosphere files""" def __init__(self, filename, source=None): super().__init__() if source is None: self.source = basename(filename) else: self.source = source self.method = "embedded" self.citation_info = r""" @MISC{2017ascl.soft10017K, author = {{Kurucz}, Robert L.}, title = "{ATLAS9: Model atmosphere program with opacity distribution functions}", keywords = {Software}, year = "2017", month = "Oct", eid = {ascl:1710.017}, pages = {ascl:1710.017}, archivePrefix = {ascl}, eprint = {1710.017}, adsurl = {https://ui.adsabs.harvard.edu/abs/2017ascl.soft10017K}, adsnote = {Provided by the SAO/NASA Astrophysics Data System}} """ self.load(filename)
[docs] def load(self, filename): """ Load data from krz files. The code will automatically judge the file source of ATLAS or MARCS. Parameters ---------- filename : str name of the file to load """ kB, mH = 1.380649e-16, 1.6735575e-24 # Judge the file source: ATLAS or MARCS with open(filename, "r") as file: header = file.readline() + file.readline() if "MARCS" in header: # File format: # 1..2 lines header # 3 line opacity # 4..13 elemntal abundances # 14.. Table data for each layer # Rhox Temp XNE XNA RHO with open(filename, "r") as file: header1 = file.readline() header2 = file.readline() opacity = file.readline() abund = [file.readline() for _ in range(10)] table = file.readlines() # Combine the first two lines header = header1 + header2 # Parse header # vturb try: self.vturb = float(re.findall(r"VTURB=?\s*(\d)", header, flags=re.I)[0]) except IndexError: self.vturb = 0 try: self.lonh = float(re.findall(r"L/H=?\s*(\d+.?\d*)", header, flags=re.I)[0]) except IndexError: self.lonh = 0 self.teff = float(re.findall(r"T ?EFF=?\s*(\d+.?\d*)", header, flags=re.I)[0]) self.logg = float( re.findall(r"GRAV(ITY)?=?\s*(\d+.?\d*)", header, flags=re.I)[0][1] ) model_type = re.findall(r"MODEL TYPE=?\s*(\d)", header, flags=re.I)[0] self.model_type = int(model_type) model_type_key = {0: "rhox", 1: "tau", 3: "sph"} self.depth = model_type_key[self.model_type] self.geom = "pp" self.wlstd = float(re.findall(r"WLSTD=?\s*(\d+.?\d*)", header, flags=re.I)[0]) # parse opacity i = opacity.find("-") opacity = opacity[:i].split() self.opflag = np.array([int(k) for k in opacity]) # parse abundance pattern = np.genfromtxt(abund).flatten()[:-1] pattern[1] = 10 ** pattern[1] self.abund = Abund(monh=0, pattern=pattern, type="sme") # parse table self.table = np.genfromtxt(table, delimiter=",", usecols=(0, 1, 2, 3, 4)) self.rhox = self.table[:, 0] self.temp = self.table[:, 1] self.xne = self.table[:, 2] self.xna = self.table[:, 3] self.rho = self.table[:, 4] else: with open(filename, "r") as file: header = file.readline() + file.readline() opacity = file.readline() _ = file.readline() # Read in abund abun_list = '' temp = file.readline() abun_list = abun_list + temp[42:].replace('E', '') temp = file.readline() while 'ABUNDANCE CHANGE' in temp: abun_list = abun_list + temp[temp.index('ABUNDANCE CHANGE')+16:] temp = file.readline() abun = np.array(abun_list.split(), dtype='f').reshape(int(len(abun_list.split())/2), 2) # Read the model lines temp = temp.split() model_lines = [] for _ in range(int(temp[2])): model_lines.append(file.readline().split()) model_lines = np.array(model_lines, dtype=np.float64) try: self.monh = float(re.findall(r"\[\s*([+-]?\d+(?:\.\d*)?)\s*\]", header)[0]) except IndexError: self.monh = 0.0 try: self.vturb = float(re.findall(r"VTURB=?\s*(\d)", header, flags=re.I)[0]) except IndexError: self.vturb = 0 try: self.lonh = float(re.findall(r"L/H=?\s*(\d+.?\d*)", header, flags=re.I)[0]) except IndexError: self.lonh = 0 self.teff = float(re.findall(r"T ?EFF=?\s*(\d+.?\d*)", header, flags=re.I)[0]) self.logg = float( re.findall(r"GRAV(ITY)?=?\s*(\d+.?\d*)", header, flags=re.I)[0][1] ) self.depth = 'RHOX' self.geom = "pp" self.wlstd = 5000. # parse opacity opacity_numbers = re.findall(r'OPACITY IFOP\s+([\d\s]+)', opacity, flags=re.I) if opacity_numbers: self.opflag = np.array([int(k) for k in opacity_numbers[0].split()]) else: # Back to old weird method i = opacity.find("-") opacity = opacity[:i].split() self.opflag = np.array([int(k) for k in opacity]) # parse abundance pattern = abun[:, 1] self.abund = Abund(monh=self.monh, pattern=pattern, type="kurucz") # parse table self.table = model_lines self.rhox = self.table[:, 0] self.temp = self.table[:, 1] self.xne = self.table[:, 3] self.P_gas = self.table[:, 2] self.xna = self.P_gas / (kB * self.temp) atmoic_mu = self.get_mu_from_abund() self.rho = self.P_gas * atmoic_mu * mH / (kB * self.temp)
# This is not used since it is tau_ross instead of tau_5000 # self.abross = self.table[:, 4] # self.tau = np.zeros_like(self.rhox) # self.tau[1:] = np.cumsum(0.5 * (self.abross[1:] + self.abross[:-1]) * np.diff(self.rhox))
[docs] def get_mu_from_abund(self): abun = self.abund.pattern X, Y = abun['H'], abun['He'] # 1. 预处理金属 metals = {el: 10.0**val for el, val in abun.items() if el not in ('H', 'He')} R = sum(ri * atmoic_mass[el] for el, ri in metals.items()) # ∑ ri mi # 2. r = N_He / N_H mH, mHe = atmoic_mass['H'], atmoic_mass['He'] r = (mH/X - mH - R) / (mHe + R) if r <= 0: raise ValueError("r≤0") # 3. 归一化取 N_H = 1 NH = 1.0 NHe = r * NH Ni = {el: (1+r) * NH * ri for el, ri in metals.items()} M_metals = sum(Ni[el] * atmoic_mass[el] for el in Ni) N_metals = sum(Ni.values()) mu = (mH + r * mHe + M_metals) / (1.0 + r + N_metals) return mu