#!/usr/bin/env python
# -*- coding: utf-8 -*-
"""
Internal TauModel class.
"""
from __future__ import (absolute_import, division, print_function,
unicode_literals)
from future.builtins import * # NOQA
from future.utils import native_str
from collections import OrderedDict
import os
from copy import deepcopy
from itertools import count
from math import pi
import numpy as np
from .helper_classes import DepthRange, SlownessModelError, TauModelError
from .slowness_model import SlownessModel
from .tau_branch import TauBranch
from .velocity_model import VelocityModel
[docs]class TauModel(object):
"""
Provides storage of all the TauBranches comprising a model.
"""
[docs] def __init__(self, s_mod, radius_of_planet, is_spherical=True, cache=None,
debug=False, skip_calc=False):
self.debug = debug
# Depth for which tau model as constructed.
self.source_depth = 0.0
self.radius_of_planet = radius_of_planet
# True if this is a spherical slowness model. False if flat.
self.is_spherical = is_spherical
# Ray parameters used to construct the tau branches. This may only be
# a subset of the slownesses/ray parameters saved in the slowness
# model due to high slowness zones (low velocity zones).
self.ray_params = None
# 2D NumPy array containing a TauBranch object
# corresponding to each "branch" of the tau model, First list is P,
# second is S. Branches correspond to depth regions between
# discontinuities or reversals in slowness gradient for a wave type.
# Each branch contains time, distance, and tau increments for each ray
# parameter in ray_param for the layer. Rays that turn above the branch
# layer get 0 for time, distance, and tau increments.
self.tau_branches = None
self.s_mod = s_mod
# Branch with the source at its top.
self.source_branch = 0
# Depths that should not have reflections or phase conversions. For
# instance, if the source is not at a branch boundary then
# no_discon_depths contains source depth and reflections and phase
# conversions are not allowed at this branch boundary. If the source
# happens to fall on a real discontinuity then it is not included.
self.no_discon_depths = []
if cache is None:
self._depth_cache = OrderedDict()
elif cache is not False:
self._depth_cache = cache
else:
self._depth_cache = None
if not skip_calc:
self.calc_tau_inc_from()
[docs] def calc_tau_inc_from(self):
"""
Calculates tau for each branch within a slowness model.
"""
# First, we must have at least 1 slowness layer to calculate a
# distance. Otherwise we must signal an exception.
if self.s_mod.get_num_layers(True) == 0 \
or self.s_mod.get_num_layers(False) == 0:
raise SlownessModelError(
"Can't calculate tauInc when get_num_layers() = 0. "
"I need more slowness samples.")
self.s_mod.validate()
# Create an array holding the ray parameter that we will use for
# constructing the tau splines. Only store ray parameters that are
# not in a high slowness zone, i.e. they are smaller than the
# minimum ray parameter encountered so far.
num_branches = len(self.s_mod.critical_depths) - 1
self.tau_branches = np.empty((2, num_branches), dtype=TauBranch)
# Here we find the list of ray parameters to be used for the tau
# model. We only need to find ray parameters for S waves since P
# waves have been constructed to be a subset of the S samples.
ray_num = 0
min_p_so_far = self.s_mod.s_layers[0]['top_p']
temp_ray_params = np.empty(2 * self.s_mod.get_num_layers(False) +
len(self.s_mod.critical_depths))
# Make sure we get the top slowness of the very top layer
temp_ray_params[ray_num] = min_p_so_far
ray_num += 1
for curr_s_layer in self.s_mod.s_layers:
# Add the top if it is strictly less than the last sample added.
# Note that this will not be added if the slowness is continuous
# across the layer boundary.
if curr_s_layer['top_p'] < min_p_so_far:
temp_ray_params[ray_num] = curr_s_layer['top_p']
ray_num += 1
min_p_so_far = curr_s_layer['top_p']
if curr_s_layer['bot_p'] < min_p_so_far:
# Add the bottom if it is strictly less than the last sample
# added. This will always happen unless we are
# within a high slowness zone.
temp_ray_params[ray_num] = curr_s_layer['bot_p']
ray_num += 1
min_p_so_far = curr_s_layer['bot_p']
# Copy tempRayParams to ray_param while chopping off trailing zeros
# (from the initialisation), so the size is exactly right. NB
# slicing doesn't really mean deep copy, but it works for a list of
# doubles like this
self.ray_params = temp_ray_params[:ray_num]
if self.debug:
print("Number of slowness samples for tau:" + str(ray_num))
for wave_num, is_p_wave in enumerate([True, False]):
# The minimum slowness seen so far.
min_p_so_far = self.s_mod.get_slowness_layer(0, is_p_wave)['top_p']
# for critNum, (topCritDepth, botCritDepth) in enumerate(zip(
# self.s_mod.critical_depths[:-1],
# self.s_mod.critical_depths[1:])):
# Faster:
for crit_num, top_crit_depth, bot_crit_depth in zip(
count(), self.s_mod.critical_depths[:-1],
self.s_mod.critical_depths[1:]):
top_crit_layer_num = top_crit_depth['p_layer_num'] \
if is_p_wave else top_crit_depth['s_layer_num']
bot_crit_layer_num = (
bot_crit_depth['p_layer_num']
if is_p_wave else bot_crit_depth['s_layer_num']) - 1
self.tau_branches[wave_num, crit_num] = \
TauBranch(top_crit_depth['depth'], bot_crit_depth['depth'],
is_p_wave)
self.tau_branches[wave_num, crit_num].debug = self.debug
self.tau_branches[wave_num, crit_num].create_branch(
self.s_mod, min_p_so_far, self.ray_params)
# Update minPSoFar. Note that the new minPSoFar could be at
# the start of a discontinuity over a high slowness zone,
# so we need to check the top, bottom and the layer just
# above the discontinuity.
top_s_layer = self.s_mod.get_slowness_layer(top_crit_layer_num,
is_p_wave)
bot_s_layer = self.s_mod.get_slowness_layer(bot_crit_layer_num,
is_p_wave)
min_p_so_far = min(
min_p_so_far, min(top_s_layer['top_p'],
bot_s_layer['bot_p']))
bot_s_layer = self.s_mod.get_slowness_layer(
self.s_mod.layer_number_above(bot_crit_depth['depth'],
is_p_wave), is_p_wave)
min_p_so_far = min(min_p_so_far, bot_s_layer['bot_p'])
# Here we decide which branches are the closest to the Moho, CMB,
# and IOCB by comparing the depth of the top of the branch with the
# depths in the Velocity Model.
best_moho = 1e300
best_cmb = 1e300
best_iocb = 1e300
for branch_num, t_branch in enumerate(self.tau_branches[0]):
if abs(t_branch.top_depth - self.s_mod.v_mod.moho_depth) <= \
best_moho:
# Branch with Moho at its top.
self.moho_branch = branch_num
best_moho = abs(t_branch.top_depth -
self.s_mod.v_mod.moho_depth)
if abs(t_branch.top_depth - self.s_mod.v_mod.cmb_depth) < best_cmb:
self.cmb_branch = branch_num
best_cmb = abs(t_branch.top_depth - self.s_mod.v_mod.cmb_depth)
if abs(t_branch.top_depth - self.s_mod.v_mod.iocb_depth) < \
best_iocb:
self.iocb_branch = branch_num
best_iocb = abs(t_branch.top_depth -
self.s_mod.v_mod.iocb_depth)
# Now set moho_depth etc. to the top of the branches we have decided
# on.
self.moho_depth = self.tau_branches[0, self.moho_branch].top_depth
self.cmb_depth = self.tau_branches[0, self.cmb_branch].top_depth
self.iocb_depth = self.tau_branches[0, self.iocb_branch].top_depth
self.validate()
[docs] def __str__(self):
desc = "Delta tau for each slowness sample and layer.\n"
for j, ray_param in enumerate(self.ray_params):
for i, tb in enumerate(self.tau_branches[0]):
desc += (
" i " + str(i) + " j " + str(j) + " ray_param " +
str(ray_param) +
" tau " + str(tb.tau[j]) + " time " +
str(tb.time[j]) + " dist " +
str(tb.dist[j]) + " degrees " +
str(tb.dist[j] * 180 / pi) + "\n")
desc += "\n"
return desc
[docs] def validate(self):
# Could implement the model validation; not critical right now
return True
[docs] def depth_correct(self, depth):
"""
Called in TauPTime. Computes a new tau model for a source at depth
using the previously computed branches for a surface source. No
change is needed to the branches above and below the branch
containing the depth, except for the addition of a slowness sample.
The branch containing the source depth is split into 2 branches,
and up going branch and a downgoing branch. Additionally,
the slowness at the source depth must be sampled exactly as it is an
extremal point for each of these branches. Cf. [Buland1983]_, page
1290.
"""
if self.source_depth != 0:
raise TauModelError("Can't depth correct a TauModel that is not "
"originally for a surface source.")
if depth > self.radius_of_planet:
raise TauModelError("Can't depth correct to a source deeper than "
"the radius of the planet.")
return self.load_from_depth_cache(depth)
[docs] def load_from_depth_cache(self, depth):
# Very simple and straightforward LRU cache implementation.
if self._depth_cache is not None:
# Retrieve and later insert again to get LRU cache behaviour.
try:
value = self._depth_cache.pop(depth)
except KeyError:
value = self._load_from_depth_cache(depth)
self._depth_cache[depth] = value
# Pop first key-value pairs until at most 128 elements are still
# in the cache.
while len(self._depth_cache) > 128:
self._depth_cache.popitem(last=False)
return value
else:
return self._load_from_depth_cache(depth)
[docs] def _load_from_depth_cache(self, depth):
depth_corrected = self.split_branch(depth)
depth_corrected.source_depth = depth
depth_corrected.source_branch = depth_corrected.find_branch(depth)
depth_corrected.validate()
return depth_corrected
[docs] def split_branch(self, depth):
"""
Returns a new TauModel with the branches containing depth split at
depth. Used for putting a source at depth since a source can only be
located on a branch boundary.
"""
# First check to see if depth happens to already be a branch
# boundary, then just return original model.
for tb in self.tau_branches[0]:
if tb.top_depth == depth or tb.bot_depth == depth:
return deepcopy(self)
# Depth is not a branch boundary, so must modify the tau model.
index_p = -1
p_wave_ray_param = -1
index_s = -1
s_wave_ray_param = -1
out_s_mod = self.s_mod
out_ray_params = self.ray_params
# Do S wave first since the S ray param is > P ray param.
for is_p_wave in [False, True]:
split_info = out_s_mod.split_layer(depth, is_p_wave)
out_s_mod = split_info.s_mod
if split_info.needed_split and not split_info.moved_sample:
# Split the slowness layers containing depth into two layers
# each.
new_ray_param = split_info.ray_param
# Insert the new ray parameters into the ray_param array.
above = out_ray_params[:-1]
below = out_ray_params[1:]
index = (above > new_ray_param) & (new_ray_param > below)
if np.any(index):
index = np.where(index)[0][0] + 1
out_ray_params = np.insert(out_ray_params, index,
new_ray_param)
if is_p_wave:
index_p = index
p_wave_ray_param = new_ray_param
else:
index_s = index
s_wave_ray_param = new_ray_param
# Now add a sample to each branch above the depth, split the branch
# containing the depth, and add a sample to each deeper branch.
branch_to_split = self.find_branch(depth)
new_tau_branches = np.empty((2, self.tau_branches.shape[1] + 1),
dtype=TauBranch)
for i in range(branch_to_split):
new_tau_branches[0, i] = deepcopy(self.tau_branches[0, i])
new_tau_branches[1, i] = deepcopy(self.tau_branches[1, i])
# Add the new ray parameter(s) from splitting the S and/or P
# wave slowness layer to both the P and S wave tau branches (if
# splitting occurred).
if index_s != -1:
new_tau_branches[0, i].insert(s_wave_ray_param, out_s_mod,
index_s)
new_tau_branches[1, i].insert(s_wave_ray_param, out_s_mod,
index_s)
if index_p != -1:
new_tau_branches[0, i].insert(p_wave_ray_param, out_s_mod,
index_p)
new_tau_branches[1, i].insert(p_wave_ray_param, out_s_mod,
index_p)
for p_or_s in range(2):
new_tau_branches[p_or_s, branch_to_split] = TauBranch(
self.tau_branches[p_or_s, branch_to_split].top_depth, depth,
p_or_s == 0)
new_tau_branches[p_or_s, branch_to_split].create_branch(
out_s_mod,
self.tau_branches[p_or_s, branch_to_split].max_ray_param,
out_ray_params)
new_tau_branches[p_or_s, branch_to_split + 1] = \
self.tau_branches[p_or_s, branch_to_split].difference(
new_tau_branches[p_or_s, branch_to_split],
index_p, index_s, out_s_mod,
new_tau_branches[p_or_s, branch_to_split].min_ray_param,
out_ray_params)
for i in range(branch_to_split + 1, len(self.tau_branches[0])):
for p_or_s in range(2):
new_tau_branches[p_or_s, i + 1] = \
deepcopy(self.tau_branches[p_or_s, i])
if index_s != -1:
# Add the new ray parameter from splitting the S wave
# slownes layer to both the P and S wave tau branches.
for p_or_s in range(2):
new_tau_branches[p_or_s, i + 1].insert(
s_wave_ray_param, out_s_mod, index_s)
if index_p != -1:
# Add the new ray parameter from splitting the P wave
# slownes layer to both the P and S wave tau branches.
for p_or_s in range(2):
new_tau_branches[p_or_s, i + 1].insert(
p_wave_ray_param, out_s_mod, index_p)
# We have split a branch so possibly source_branch, moho_branch,
# cmb_branch and iocb_branch are off by 1.
out_source_branch = self.source_branch
if self.source_depth > depth:
out_source_branch += 1
out_moho_branch = self.moho_branch
if self.moho_depth > depth:
out_moho_branch += 1
out_cmb_branch = self.cmb_branch
if self.cmb_depth > depth:
out_cmb_branch += 1
out_iocb_branch = self.iocb_branch
if self.iocb_depth > depth:
out_iocb_branch += 1
# No overloaded constructors - so do it this way to bypass the
# calc_tau_inc_from in the __init__.
tau_model = TauModel(
out_s_mod,
radius_of_planet=out_s_mod.v_mod.radius_of_planet,
is_spherical=self.is_spherical, cache=False,
debug=self.debug, skip_calc=True)
tau_model.source_depth = self.source_depth
tau_model.source_branch = out_source_branch
tau_model.moho_branch = out_moho_branch
tau_model.moho_depth = self.moho_depth
tau_model.cmb_branch = out_cmb_branch
tau_model.cmb_depth = self.cmb_depth
tau_model.iocb_branch = out_iocb_branch
tau_model.iocb_depth = self.iocb_depth
tau_model.ray_params = out_ray_params
tau_model.tau_branches = new_tau_branches
tau_model.no_discon_depths = self.no_discon_depths + [depth]
tau_model.validate()
return tau_model
[docs] def find_branch(self, depth):
"""Finds the branch that either has the depth as its top boundary, or
strictly contains the depth. Also, we allow the bottom-most branch to
contain its bottom depth, so that the center of the planet is contained
within the bottom branch."""
for i, tb in enumerate(self.tau_branches[0]):
if tb.top_depth <= depth < tb.bot_depth:
return i
# Check to see if depth is centre of the planet.
if self.tau_branches[0, -1].bot_depth == depth:
return len(self.tau_branches) - 1
else:
raise TauModelError("No TauBranch contains this depth.")
[docs] def get_tau_branch(self, branch_nu, is_p_wave):
if is_p_wave:
return self.tau_branches[0, branch_nu]
else:
return self.tau_branches[1, branch_nu]
[docs] def get_branch_depths(self):
"""
Return an array of the depths that are boundaries between branches.
:return:
"""
branch_depths = [self.get_tau_branch(0, True).top_depth]
branch_depths += [
self.get_tau_branch(i - 1, True).bot_depth
for i in range(1, len(self.tau_branches[0]))]
return branch_depths
[docs] def serialize(self, filename):
"""
Serialize model to numpy npz binary file.
Summary of contents that have to be handled during serialization::
TauModel
========
cmb_branch <type 'int'>
cmb_depth <type 'float'>
debug <type 'bool'>
iocb_branch <type 'int'>
iocb_depth <type 'float'>
moho_branch <type 'int'>
moho_depth <type 'float'>
no_discon_depths <type 'list'> (of float!?)
radius_of_planet <type 'float'>
ray_params <type 'numpy.ndarray'> (1D, float)
s_mod <class 'obspy.taup.slowness_model.SlownessModel'>
source_branch <type 'int'>
source_depth <type 'float'>
is_spherical <type 'bool'>
tau_branches <type 'numpy.ndarray'> (2D, type TauBranch)
TauBranch
=========
debug <type 'bool'>
bot_depth <type 'float'>
dist <type 'numpy.ndarray'>
is_p_wave <type 'bool'>
max_ray_param <type 'float'>
min_ray_param <type 'float'>
min_turn_ray_param <type 'float'>
tau <type 'numpy.ndarray'>
time <type 'numpy.ndarray'>
top_depth <type 'float'>
SlownessModel
=============
debug <type 'bool'>
p_layers <type 'numpy.ndarray'>
p_wave <type 'bool'>
s_layers <type 'numpy.ndarray'>
s_wave <type 'bool'>
allow_inner_core_s <type 'bool'>
critical_depths <type 'numpy.ndarray'>
fluid_layer_depths <type 'list'> (of DepthRange)
high_slowness_layer_depths_p <type 'list'> (of DepthRange)
high_slowness_layer_depths_s <type 'list'> (of DepthRange)
max_delta_p <type 'float'>
max_depth_interval <type 'float'>
max_interp_error <type 'float'>
max_range_interval <type 'float'>
min_delta_p <type 'float'>
radius_of_planet <type 'float'>
slowness_tolerance <type 'float'>
v_mod <class 'obspy.taup.velocity_model.VelocityModel'>
VelocityModel
=============
cmb_depth <type 'float'>
iocb_depth <type 'float'>
is_spherical <type 'bool'>
layers <type 'numpy.ndarray'>
max_radius <type 'float'>
min_radius <type 'int'>
model_name <type 'unicode'>
moho_depth <type 'float'>
radius_of_planet <type 'float'>
"""
# a) handle simple contents
keys = ['cmb_branch', 'cmb_depth', 'debug', 'iocb_branch',
'iocb_depth', 'moho_branch', 'moho_depth', 'no_discon_depths',
'radius_of_planet', 'ray_params', 'source_branch',
'source_depth', 'is_spherical']
arrays = {k: getattr(self, k) for k in keys}
# b) handle .tau_branches
i, j = self.tau_branches.shape
for j_ in range(j):
for i_ in range(i):
# just store the shape of self.tau_branches in the key names
# for later reconstruction of array in deserialization.
key = 'tau_branches__%i/%i__%i/%i' % (j_, j, i_, i)
arrays[key] = self.tau_branches[i_][j_]._to_array()
# c) handle simple contents of .s_mod
dtypes = [(native_str('debug'), np.bool_),
(native_str('p_wave'), np.bool_),
(native_str('s_wave'), np.bool_),
(native_str('allow_inner_core_s'), np.bool_),
(native_str('max_delta_p'), np.float_),
(native_str('max_depth_interval'), np.float_),
(native_str('max_interp_error'), np.float_),
(native_str('max_range_interval'), np.float_),
(native_str('min_delta_p'), np.float_),
(native_str('radius_of_planet'), np.float_),
(native_str('slowness_tolerance'), np.float_)]
slowness_model = np.empty(shape=(), dtype=dtypes)
for dtype in dtypes:
key = dtype[0]
slowness_model[key] = getattr(self.s_mod, key)
arrays['s_mod'] = slowness_model
# d) handle complex contents of .s_mod
arrays['s_mod.p_layers'] = self.s_mod.p_layers
arrays['s_mod.s_layers'] = self.s_mod.s_layers
arrays['s_mod.critical_depths'] = self.s_mod.critical_depths
for key in ['fluid_layer_depths', 'high_slowness_layer_depths_p',
'high_slowness_layer_depths_s']:
data = getattr(self.s_mod, key)
if len(data) == 0:
arr_ = np.array([])
else:
arr_ = np.vstack([data_._to_array() for data_ in data])
arrays['s_mod.' + key] = arr_
# e) handle .s_mod.v_mod
dtypes = [(native_str('cmb_depth'), np.float_),
(native_str('iocb_depth'), np.float_),
(native_str('is_spherical'), np.bool_),
(native_str('max_radius'), np.float_),
(native_str('min_radius'), np.int_),
(native_str('model_name'), np.str_,
len(self.s_mod.v_mod.model_name)),
(native_str('moho_depth'), np.float_),
(native_str('radius_of_planet'), np.float_)]
velocity_model = np.empty(shape=(), dtype=dtypes)
for dtype in dtypes:
key = dtype[0]
velocity_model[key] = getattr(self.s_mod.v_mod, key)
arrays['v_mod'] = velocity_model
arrays['v_mod.layers'] = self.s_mod.v_mod.layers
# finally save the collection of (structured) arrays to a binary file
np.savez_compressed(filename, **arrays)
@staticmethod
[docs] def deserialize(filename, cache=None):
"""
Deserialize model from numpy npz binary file.
"""
# XXX: Make this a with statement when old NumPy support is dropped.
npz = np.load(filename)
try:
model = TauModel(s_mod=None,
radius_of_planet=float(npz["radius_of_planet"]),
cache=cache, skip_calc=True)
complex_contents = [
'tau_branches', 's_mod', 'v_mod',
's_mod.p_layers', 's_mod.s_layers', 's_mod.critical_depths',
's_mod.fluid_layer_depths',
's_mod.high_slowness_layer_depths_p',
's_mod.high_slowness_layer_depths_s', 'v_mod.layers']
# a) handle simple contents
for key in npz.keys():
# we have multiple, dynamic key names for individual tau
# branches now, skip them all
if key in complex_contents or key.startswith('tau_branches'):
continue
arr = npz[key]
if arr.ndim == 0:
arr = arr[()]
setattr(model, key, arr)
# b) handle .tau_branches
tau_branch_keys = [key for key in npz.keys()
if key.startswith('tau_branches_')]
j, i = tau_branch_keys[0].split("__")[1:]
i = int(i.split("/")[1])
j = int(j.split("/")[1])
branches = np.empty(shape=(i, j), dtype=np.object_)
for key in tau_branch_keys:
j_, i_ = key.split("__")[1:]
i_ = int(i_.split("/")[0])
j_ = int(j_.split("/")[0])
branches[i_][j_] = TauBranch._from_array(npz[key])
# no idea how numpy lays out empty arrays of object type,
# make a copy just in case..
branches = np.copy(branches)
setattr(model, "tau_branches", branches)
# c) handle simple contents of .s_mod
slowness_model = SlownessModel(v_mod=None,
skip_model_creation=True)
setattr(model, "s_mod", slowness_model)
for key in npz['s_mod'].dtype.names:
# restore scalar types from 0d array
arr = npz['s_mod'][key]
if arr.ndim == 0:
arr = arr.flatten()[0]
setattr(slowness_model, key, arr)
# d) handle complex contents of .s_mod
for key in ['p_layers', 's_layers', 'critical_depths']:
setattr(slowness_model, key, npz['s_mod.' + key])
for key in ['fluid_layer_depths', 'high_slowness_layer_depths_p',
'high_slowness_layer_depths_s']:
arr_ = npz['s_mod.' + key]
if len(arr_) == 0:
data = []
else:
data = [DepthRange._from_array(x) for x in arr_]
setattr(slowness_model, key, data)
# e) handle .s_mod.v_mod
velocity_model = VelocityModel(
model_name=native_str(npz["v_mod"]["model_name"]),
radius_of_planet=float(npz["v_mod"]["radius_of_planet"]),
min_radius=float(npz["v_mod"]["min_radius"]),
max_radius=float(npz["v_mod"]["max_radius"]),
moho_depth=float(npz["v_mod"]["moho_depth"]),
cmb_depth=float(npz["v_mod"]["cmb_depth"]),
iocb_depth=float(npz["v_mod"]["iocb_depth"]),
is_spherical=bool(npz["v_mod"]["is_spherical"]),
layers=None
)
setattr(slowness_model, "v_mod", velocity_model)
setattr(velocity_model, 'layers', npz['v_mod.layers'])
finally:
if hasattr(npz, 'close'):
npz.close()
else:
del npz
return model
@staticmethod
[docs] def from_file(model_name, cache=None):
if os.path.exists(model_name):
filename = model_name
else:
filename = os.path.join(os.path.dirname(__file__), "data",
model_name.lower() + ".npz")
return TauModel.deserialize(filename, cache=cache)