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Solar envelope


#!pip install ipynb

Importing the packages

import os
import topogenesis as tg
import pyvista as pv
import trimesh as tm
import numpy as np
from ladybug.sunpath import Sunpath
from scipy.interpolate import RegularGridInterpolator

import resources.functions as f

# convert mesh to pv_mesh
def tri_to_pv(tri_mesh):
    faces = np.pad(tri_mesh.faces, ((0, 0),(1,0)), 'constant', constant_values=3)
    pv_mesh = pv.PolyData(tri_mesh.vertices, faces)
    return pv_mesh

Import meshes

envelope_path = os.path.relpath('../data/new_envelope.obj')
context_path = os.path.relpath('../data/immediate_context.obj')

# load the mesh from file
envelope_mesh = tm.load(envelope_path)
context_mesh = tm.load(context_path)

# Check if the mesh is watertight

Importing the envelope lattice

# loading the lattice from csv
lattice_path = os.path.relpath('../data/envelope_lowres.csv')
envelope_lattice = tg.lattice_from_csv(lattice_path)
envelope_lattice_one = envelope_lattice * 0 + 1

Sun vectors

Compute sun vectors

# initiate sunpath
sp = Sunpath(longitude=4.3571, latitude=52.0116)

# define sun hours : A list of hours of the year for each sun vector
# there are 8760 hours in a year, so the following integers refer to specific hours throughout the year
hoys = []
sun_vectors = []
day_multiples = 80
# for each day of the year ...
for d in range(365):
    # if it is one of the multiples
    if d%day_multiples==0:
        # for each hour of the day ...
        for h in range(24):
            # compute the hoy (hour of the year)
            hoy = d*24 + h
            # compute the sun object
            sun = sp.calculate_sun_from_hoy(hoy)
            # extract the sun vector (the direction that the sun ray travels toward)
            sun_vector = sun.sun_vector.to_array()
            # evidently, if the Z component of sun vector is positive, 
            # the sun is under the horizon 
            if sun_vector[2] < 0.0:

sun_vectors = np.array(sun_vectors)
# compute the rotation matrix 
Rz = tm.transformations.rotation_matrix(np.radians(36.324), [0,0,1])
# Rotate the sun vectors to match the site rotation
sun_vectors = tm.transform_points(sun_vectors, Rz)

Visualize sun points

# initiating the plotter
p = pv.Plotter(notebook=True)

# fast visualization of the lattice

# adding the meshes
p.add_mesh(tri_to_pv(context_mesh), opacity=0.1, style='wireframe')

# add the sun locations, color orange
p.add_points( - sun_vectors * 300, color='#ffa500')

# plotting

Compute intersection of sun rays with context mesh

Preparing the list of ray directions and origins

# constructing the sun direction from the sun vectors in a numpy array
sun_dirs = -np.array(sun_vectors)
# exract the centroids of the envelope voxels
vox_cens = envelope_lattice_one.centroids
# next step we need to shoot in all of the sun directions from all of the voxels, todo so, we need repeat the sun direction for the number of voxels to construct the ray_dir (which is the list of all ray directions). We need to repeat the voxels for the 
ray_dir = []
ray_src = []
for v_cen in vox_cens:
    for s_dir in sun_dirs:
# converting the list of directions and sources to numpy array
ray_dir = np.array(ray_dir)
ray_src = np.array(ray_src)

print("number of voxels to shoot rays from :",vox_cens.shape)
print("number of rays per each voxel :",sun_dirs.shape)
print("number of rays to be shooted :",ray_src.shape)

Computing the intersection

# computing the intersections of rays with the context mesh
tri_id, ray_id = context_mesh.ray.intersects_id(ray_origins=ray_src, ray_directions=ray_dir, multiple_hits=False)

Aggregate simulation result in the sun access lattice

Compute the percentage of time that each voxel sees the sun

# initializing the hits list full of zeros
hits = [0]*len(ray_dir)

# setting the rays that had an intersection to 1
for id in ray_id:
    hits[id] = 1

sun_count = len(sun_dirs)
vox_count = len(vox_cens)
# initiating the list of ratio
vox_sun_acc = []

# iterate over the voxels
for v_id in range(vox_count):
    # counter for the intersection
    int_count = 0
    invert_int_count = 0
    # iterate over the sun rays
    for s_id in range(sun_count):
        # computing the ray id from voxel id and sun id
        r_id = v_id * sun_count + s_id

        # summing the intersections
        int_count += hits[r_id]

    # computing the percentage of the rays that DID NOT have 
    # an intersection (aka could see the sun)
    sun_access = int_count/sun_count

    # add the ratio to list

hits = np.array(hits)
vox_sun_acc = np.array(vox_sun_acc)

Store sun access information in a lattice

# getting the condition of all voxels: are they inside the envelop or not
env_all_vox = envelope_lattice_one.flatten()

# all voxels sun access
all_vox_sun_acc = []

# v_id: voxel id in the list of only interior voxels
v_id = 0

# for all the voxels, place the interiority condition of each voxel in "vox_in"
for vox_in in env_all_vox:
    # if the voxel was outside...
    if vox_in == True:
        # read its value of sun access and append it to the list of all voxel sun access
                # add one to the voxel id so the next time we read the next voxel
        v_id += 1
    # if the voxel was not inside... 
        # add 0.0 for its sun access

# convert to array
sunacc_array = np.array(all_vox_sun_acc)

# reshape to lattice shape
sunacc_array = sunacc_array.reshape(envelope_lattice_one.shape)

# convert to lattice
sun_lattice = tg.to_lattice(sunacc_array, envelope_lattice_one)

# invert the values of the lattice (1 = a lot of sun, 0 = no sun)
sunacc_lattice = (1 - sun_lattice) * envelope_lattice

Visualize the sun access lattice

f.visualize((1 - sun_lattice), "Sun access", "../data/sun_acc_lowres")

Interpolate lowres lattice to highres

Import highres lattice

# loading highres lattice
highres_lattice_path = os.path.relpath('../data/envelope_highres.csv')
highres_lattice = tg.lattice_from_csv(highres_lattice_path)

Define interpolation function

def interpolate(lowres_field):
    # loading highres lattice
    highres_lattice_path = os.path.relpath('../data/envelope_highres.csv')
    highres_lat = tg.lattice_from_csv(highres_lattice_path)
    highres_lattice = highres_lat * 0 + 1 

    # line spaces
    x_space = np.linspace(lowres_field.minbound[0], lowres_field.maxbound[0],lowres_field.shape[0])
    y_space = np.linspace(lowres_field.minbound[1], lowres_field.maxbound[1],lowres_field.shape[1])
    z_space = np.linspace(lowres_field.minbound[2], lowres_field.maxbound[2],lowres_field.shape[2])

    # interpolation function
    interpolating_function = RegularGridInterpolator((x_space, y_space, z_space), lowres_field, bounds_error=False, fill_value=None)

    # high_res lattice
    full_lattice = highres_lattice + 1

    # sample point
    sample_points = full_lattice.centroids

    # interpolation
    interpolated_values = interpolating_function(sample_points)

    # lattice construction
    interpolated_lattice = tg.to_lattice(interpolated_values.reshape(highres_lattice.shape), highres_lattice)

    # nulling the unavailable cells
    interpolated_lattice *= highres_lattice

    return interpolated_lattice

Interpolate closeness lattice

highres_sunacc = interpolate(1 - sun_lattice)

# multipy by lattice to exclude the voxels which are outside the envelope
highres_sunacc_lattice = highres_sunacc * highres_lattice

Save interpolated field to csv

# save the sun access latice to csv
csv_path = os.path.relpath('../data/sun_acc.csv')

Visualize highres field

f.visualize(highres_sunacc, "Sun access", "../data/sun_acc_highres.png")


__author__ = "Shervin Azadi and Pirouz Nourian"
__license__ = "MIT"
__version__ = "1.0"
__url__ = ""
__summary__ = "Spatial Computing Design Studio Workshop on Solar Envelope"