示例#1
0
dt = (t1 - t0) / n

# maps [0, n) -> colors
# generate a linear interpolation of temperatures
# then map the temperatures to colors using black body
# color predictions
colors = np.zeros(n, dtype=(np.float32, 3))
for i in range(n):
    temperature = t0 + i * dt
    x, y, z = galaxy_specrend.spectrum_to_xyz(galaxy_specrend.bb_spectrum,
                                              temperature)
    r, g, b = galaxy_specrend.xyz_to_rgb(galaxy_specrend.SMPTEsystem, x, y, z)
    r = min((max(r, 0), 1))
    g = min((max(g, 0), 1))
    b = min((max(b, 0), 1))
    colors[i] = galaxy_specrend.norm_rgb(r, g, b)


# load the PNG that we use to blend the star with
# to provide a circular look to each star.
def load_galaxy_star_image():
    fname = io.load_data_file('galaxy/star-particle.png')
    raw_image = io.read_png(fname)

    return raw_image


class Canvas(app.Canvas):
    def __init__(self):
        # setup initial width, height
        app.Canvas.__init__(self, keys='interactive', size=(800, 600))
示例#2
0
dt = (t1 - t0) / n

# maps [0, n) -> colors
# generate a linear interpolation of temperatures
# then map the temperatures to colors using black body
# color predictions
colors = np.zeros(n, dtype=(np.float32, 3))
for i in range(n):
    temperature = t0 + i * dt
    x, y, z = galaxy_specrend.spectrum_to_xyz(galaxy_specrend.bb_spectrum,
                                              temperature)
    r, g, b = galaxy_specrend.xyz_to_rgb(galaxy_specrend.SMPTEsystem, x, y, z)
    r = min((max(r, 0), 1))
    g = min((max(g, 0), 1))
    b = min((max(b, 0), 1))
    colors[i] = galaxy_specrend.norm_rgb(r, g, b)


# load the PNG that we use to blend the star with
# to provide a circular look to each star.
def load_galaxy_star_image():
    fname = io.load_data_file('galaxy/star-particle.png')
    raw_image = io.read_png(fname)

    return raw_image


class Canvas(app.Canvas):

    def __init__(self):
        # setup initial width, height