Example #1
0
File: vmi.py Project: stggh/PyAbel
def calculate_speeds(IM, origin=None, Jacobian=False, dr=1, dt=None):
    """ Angular integration of the image.

        Returning the one-dimentional intensity profile as a function of the 
        radial coordinate. 
        
     Parameters
     ----------
     IM: rows x cols 2D np.array
         The data image.

     origin: tuple 
         Image center coordinate relative to *bottom-left* corner
         defaults to (rows//2+rows%2,cols//2+cols%2).

     Jacobian: boolean 
         Include r*sinθ in the angular sum (integration).

     dr: float 
         Radial coordinate grid spacing, in pixels (default 1).

     dt: float
         Theta coordinate grid spacing in degrees, defaults to rows//2.
      
     Returns
     -------
      1D np.array 
         Integrated intensity array (vs radius).

      1D np.array 
         Corresponding radial coordinates

     """

    polarIM, r_grid, theta_grid = reproject_image_into_polar(IM,
                                                             origin,
                                                             Jacobian=Jacobian,
                                                             dr=dr,
                                                             dt=dt)
    theta = theta_grid[0, :]  # theta coordinates
    r = r_grid[:, 0]  # radial coordinates

    if Jacobian:  #  x r sinθ
        sintheta = np.abs(np.sin(theta))
        polarIM = polarIM * sintheta[np.newaxis, :]
        polarIM = polarIM * r[:, np.newaxis]

    speeds = np.sum(polarIM, axis=1)
    n = speeds.shape[0]

    return speeds, r[:n]  # limit radial coordinates range to match speed
Example #2
0
File: vmi.py Project: stggh/PyAbel
def calculate_speeds(IM, origin=None, Jacobian=False, dr=1, dt=None):
    """ Angular integration of the image.

        Returning the one-dimentional intensity profile as a function of the 
        radial coordinate. 
        
     Parameters
     ----------
     IM: rows x cols 2D np.array
         The data image.

     origin: tuple 
         Image center coordinate relative to *bottom-left* corner
         defaults to (rows//2+rows%2,cols//2+cols%2).

     Jacobian: boolean 
         Include r*sinθ in the angular sum (integration).

     dr: float 
         Radial coordinate grid spacing, in pixels (default 1).

     dt: float
         Theta coordinate grid spacing in degrees, defaults to rows//2.
      
     Returns
     -------
      1D np.array 
         Integrated intensity array (vs radius).

      1D np.array 
         Corresponding radial coordinates

     """

    polarIM, r_grid, theta_grid = reproject_image_into_polar(IM, origin,
                                              Jacobian=Jacobian, dr=dr, dt=dt)
    theta = theta_grid[0, :]   # theta coordinates
    r = r_grid[:, 0]           # radial coordinates

    if Jacobian:   #  x r sinθ    
        sintheta = np.abs(np.sin(theta))
        polarIM = polarIM*sintheta[np.newaxis, :]
        polarIM = polarIM*r[:, np.newaxis]

    speeds = np.sum(polarIM, axis=1)
    n = speeds.shape[0]   

    return speeds, r[:n]   # limit radial coordinates range to match speed
Example #3
0
File: vmi.py Project: stggh/PyAbel
def calculate_angular_distributions(IM, radial_ranges=None):
    """ Intensity variation in the angular coordinate, theta.

    This function is the theta-coordinate complement to 'calculate_speeds(IM)'

    (optionally and more useful) returning intensity vs angle for defined
    radial ranges.

    Parameters
    ----------
    IM: 2D np.array 
        Image data

    radial_ranges: list of tuples
        [(r0, r1), (r2, r3), ...] 
        Evaluate the intensity vs angle for the radial ranges 
                                            r0_r1, r2_r3, etc. 

    Returns
    --------
    2D np.array 
       Intensity vs angle distribution for each selected radial range.

    1D np.array 
       Angle coordinates, referenced to vertical direction.

    """

    polarIM, r_grid, theta_grid = reproject_image_into_polar(IM)

    theta = theta_grid[0, :]  # theta coordinates
    r = r_grid[:, 0]  # radial coordinates

    if radial_ranges is None:
        radial_ranges = [
            (0, r[-1]),
        ]

    intensity_vs_theta_at_R = []
    for rr in radial_ranges:
        subr = np.logical_and(r >= rr[0], r <= rr[1])

        # sum intensity across radius of spectral feature
        intensity_vs_theta_at_R.append(np.sum(polarIM[subr], axis=0))

    return intensity_vs_theta_at_R, theta
Example #4
0
File: vmi.py Project: stggh/PyAbel
def calculate_angular_distributions(IM, radial_ranges=None):
    """ Intensity variation in the angular coordinate, theta.

    This function is the theta-coordinate complement to 'calculate_speeds(IM)'

    (optionally and more useful) returning intensity vs angle for defined
    radial ranges.

    Parameters
    ----------
    IM: 2D np.array 
        Image data

    radial_ranges: list of tuples
        [(r0, r1), (r2, r3), ...] 
        Evaluate the intensity vs angle for the radial ranges 
                                            r0_r1, r2_r3, etc. 

    Returns
    --------
    2D np.array 
       Intensity vs angle distribution for each selected radial range.

    1D np.array 
       Angle coordinates, referenced to vertical direction.

    """

    polarIM, r_grid, theta_grid = reproject_image_into_polar(IM)

    theta = theta_grid[0, :]  # theta coordinates
    r = r_grid[:, 0]          # radial coordinates

    if radial_ranges is None:
        radial_ranges = [(0, r[-1]), ]

    intensity_vs_theta_at_R = []
    for rr in radial_ranges:
        subr = np.logical_and(r >= rr[0], r <= rr[1])

        # sum intensity across radius of spectral feature
        intensity_vs_theta_at_R.append(np.sum(polarIM[subr], axis=0))

    return intensity_vs_theta_at_R, theta