def get_header(filepath):
"""Returns the header for a given file"""
hdulist = pyfits.open(filepath)
hdulist.verify('silentfix')
comment = "".join(hdulist[0].header.get_comment()).strip()
header = MapHeader(hdulist[0].header)
header['comment'] = comment
return header
def get_header(filepath):
"""Reads the header in and saves it as a dictionary"""
xmlstring = read_xmlbox(filepath, "fits")
pydict = xml_to_dict(xmlstring)["fits"]
#Fix types
for k, v in pydict.items():
if v.isdigit():
pydict[k] = int(v)
elif is_float(v):
pydict[k] = float(v)
# Remove newlines from comment
pydict['comment'] = pydict['comment'].replace("\n", "")
return MapHeader(pydict)
def __init__(self, data, header):
self._original_header = MapHeader(header)
# Set naxis1 and naxis2 if not specified
if header.get('naxis1') is None:
header['naxis1'] = self.shape[0]
if header.get('naxis2') is None:
header['naxis2'] = self.shape[1]
# Parse header and set map attributes
for attr, value in list(self.get_properties(header).items()):
setattr(self, attr, value)
# Addition properties based on data
self.byte_scaled = self.dtype == np.uint8
# Validate properties
self._validate()
def read(filepath):
"""Reads in the file at the specified location"""
hdulist = pyfits.open(filepath)
hdulist.verify('silentfix')
fits_comment = hdulist[0].header.get_comment()
# PyFITS 2.x
if len(fits_comment) > 0 and isinstance(fits_comment[0], basestring):
comments = [val for val in fits_comment]
else:
# PyFITS 3.x
comments = [card.value for card in fits_comment]
comment = "".join(comments).strip()
header = MapHeader(hdulist[0].header)
header['comment'] = comment
return hdulist[0].data, header
class BaseMap(np.ndarray):
"""
BaseMap(data, header)
A spatially-aware data array based on the SolarSoft Map object
Parameters
----------
data : numpy.ndarray, list
A 2d list or ndarray containing the map data
header : dict
A dictionary of the original image header tags
Attributes
----------
fits_header : dict
Dictionary representation of the original FITS header
carrington_longitude : str
Carrington longitude (crln_obs)
center : dict
X and Y coordinate of the center of the map in units.
Usually represents the offset between the center of the Sun and the
center of the map.
cmap : matplotlib.colors.Colormap
A Matplotlib colormap to be applied to the data
coordinate_system : dict
Coordinate system used for x and y axes (ctype1/2)
date : datetime
Image observation time
detector : str
Detector name
dsun : float
The observer distance from the Sun.
exptime : float
Exposure time of the image in seconds.
heliographic_latitude : float
Heliographic latitude in degrees
heliographic_longitude : float
Heliographic longitude in degrees
instrument : str
Instrument name
measurement : str, int
Measurement name. In some instances this is the wavelength of image.
name: str
Human-readable description of map-type
nickname: str
An abbreviated human-readable description of the map-type; part of
the Helioviewer data model
observatory : str
Observatory name
reference_coordinate : float
Reference point WCS axes in data units (crval1/2)
reference_pixel : float
Reference point axes in pixels (crpix1/2)
rsun_arcseconds : float
Radius of the sun in arcseconds
rsun_meters : float
Radius of the sun in meters
scale : dict
Image scale along the x and y axes in units/pixel (cdelt1/2).
units : dict
Image coordinate units along the x and y axes (cunit1/2).
Examples
--------
>>> aia = sunpy.Map(sunpy.AIA_171_IMAGE)
>>> aia.T
AIAMap([[ 0.3125, 1. , -1.1875, ..., -0.625 , 0.5625, 0.5 ],
[-0.0625, 0.1875, 0.375 , ..., 0.0625, 0.0625, -0.125 ],
[-0.125 , -0.8125, -0.5 , ..., -0.3125, 0.5625, 0.4375],
...,
[ 0.625 , 0.625 , -0.125 , ..., 0.125 , -0.0625, 0.6875],
[-0.625 , -0.625 , -0.625 , ..., 0.125 , -0.0625, 0.6875],
[ 0. , 0. , -1.1875, ..., 0.125 , 0. , 0.6875]])
>>> aia.units['x']
'arcsec'
>>> aia.show()
>>> import matplotlib.cm as cm
>>> import matplotlib.colors as colors
>>> aia.show(cmap=cm.hot, norm=colors.Normalize(1, 2048))
See Also
--------
numpy.ndarray Parent class for the Map object
References
----------
| http://docs.scipy.org/doc/numpy/reference/arrays.classes.html
| http://docs.scipy.org/doc/numpy/user/basics.subclassing.html
| http://docs.scipy.org/doc/numpy/reference/ufuncs.html
| http://www.scipy.org/Subclasses
"""
def __new__(cls, data, header):
"""Creates a new BaseMap instance"""
if isinstance(data, np.ndarray):
obj = data.view(cls)
elif isinstance(data, list):
obj = np.asarray(data).view(cls)
else:
raise TypeError('Invalid input')
return obj
def __init__(self, data, header):
self._original_header = MapHeader(header)
# Set naxis1 and naxis2 if not specified
if header.get('naxis1') is None:
header['naxis1'] = self.shape[0]
if header.get('naxis2') is None:
header['naxis2'] = self.shape[1]
# Parse header and set map attributes
for attr, value in list(self.get_properties(header).items()):
setattr(self, attr, value)
# Addition properties based on data
self.byte_scaled = self.dtype == np.uint8
# Validate properties
self._validate()
@classmethod
def get_properties(cls, header):
"""Parses a map header and determines default properties."""
return {
"cmap": cm.gray, # @UndefinedVariable
"date": parse_time(header.get('date-obs', None)),
"detector": header.get('detector', ''),
"dsun": header.get('dsun_obs', constants.au),
"exposure_time": header.get('exptime', 0.),
"instrument": header.get('instrume', ''),
"measurement": header.get('wavelnth', ''),
"observatory": header.get('telescop', ''),
"name": header.get('telescop', '') + " " +
str(header.get('wavelnth', '')),
"nickname": header.get('detector', ''),
"rsun_meters": header.get('rsun_ref', constants.radius),
"rsun_arcseconds": header.get('rsun_obs', header.get('solar_r',
header.get('radius',
constants.average_angular_size))),
"coordinate_system": {
'x': header.get('ctype1', 'HPLN-TAN'),
'y': header.get('ctype2', 'HPLT-TAN')
},
"carrington_longitude": header.get('crln_obs', 0.),
"heliographic_latitude": header.get('hglt_obs',
header.get('crlt_obs',
header.get('solar_b0', 0.))),
"heliographic_longitude": header.get('hgln_obs', 0.),
"reference_coordinate": {
'x': header.get('crval1', 0.),
'y': header.get('crval2', 0.),
},
"reference_pixel": {
'x': header.get('crpix1', (header.get('naxis1') + 1) / 2.),
'y': header.get('crpix2', (header.get('naxis2') + 1) / 2.)
},
"scale": {
'x': header.get('cdelt1', 1.),
'y': header.get('cdelt2', 1.),
},
"units": {
'x': header.get('cunit1', 'arcsec'),
'y': header.get('cunit2', 'arcsec')
}
}
def __array_finalize__(self, obj):
"""Finishes instantiation of the new map object"""
if obj is None:
return
if hasattr(obj, '_original_header'):
properties = ['_original_header', 'cmap', 'date', 'detector', 'dsun',
'exposure_time', 'instrument', 'measurement', 'name',
'observatory', 'rsun_arcseconds', 'rsun_meters',
'scale', 'units', 'reference_coordinate',
'reference_pixel', 'coordinate_system',
'heliographic_latitude', 'heliographic_longitude',
'carrington_longitude']
for attr in properties:
setattr(self, attr, getattr(obj, attr))
def __array_wrap__(self, out_arr, context=None):
"""Returns a wrapped instance of a Map object"""
return np.ndarray.__array_wrap__(self, out_arr, context)
def __getitem__(self, key):
"""Overiding indexing operation to ensure that header is updated"""
if isinstance(key, tuple) and type(key[0]) is slice:
x_range = [key[1].start, key[1].stop]
y_range = [key[0].start, key[0].stop]
return self.submap(y_range, x_range, units="pixels")
else:
return np.ndarray.__getitem__(self, key)
def __add__(self, other):
"""Add two maps. Currently does not take into account the alignment
between the two maps."""
result = np.ndarray.__add__(self, other)
return result
def __repr__(self):
if not hasattr(self, 'observatory'):
return np.ndarray.__repr__(self)
return (
"""SunPy Map
---------
Observatory:\t %s
Instrument:\t %s
Detector:\t %s
Measurement:\t %s
Obs Date:\t %s
dt:\t\t %f
Dimension:\t [%d, %d]
[dx, dy] =\t [%f, %f]
""" % (self.observatory, self.instrument, self.detector, self.measurement,
self.date.strftime("%Y-%m-%d %H:%M:%S"), self.exposure_time,
self.shape[0], self.shape[1], self.scale['x'], self.scale['y'])
+ np.ndarray.__repr__(self))
def __sub__(self, other):
"""Subtract two maps. Currently does not take into account the
alignment between the two maps.
numpy dtype nums:
1 int8
2 uint8
3 int16
4 uint16
"""
# if data is stored as unsigned, cast up (e.g. uint8 => int16)
if self.dtype.kind == "u":
dtype = "int%d" % (int(self.dtype.name[4:]) * 2)
self = self.astype(np.dtype(dtype))
if other.dtype.kind == "u":
dtype = "int%d" % (int(other.dtype.name[4:]) * 2)
other = other.astype(np.dtype(dtype))
result = np.ndarray.__sub__(self, other)
def norm():
mean = result.mean()
std = result.std()
vmin = max(result.min(), mean - 6 * std)
vmax = min(result.max(), mean + 6 * std)
return colors.Normalize(vmin, vmax)
result.norm = norm
result.cmap = cm.gray # @UndefinedVariable
return result
@property
def xrange(self):
"""Return the X range of the image in arcsec from edge to edge."""
xmin = self.center['x'] - self.shape[1] / 2 * self.scale['x']
xmax = self.center['x'] + self.shape[1] / 2 * self.scale['x']
return [xmin, xmax]
@property
def yrange(self):
"""Return the Y range of the image in arcsec from edge to edge."""
ymin = self.center['y'] - self.shape[0] / 2 * self.scale['y']
ymax = self.center['y'] + self.shape[0] / 2 * self.scale['y']
return [ymin, ymax]
@property
def center(self):
"""Returns the offset between the center of the Sun and the center of
the map."""
return {
'x': wcs.get_center(self.shape[0], self.scale['x'],
self.reference_pixel['x'],
self.reference_coordinate['x']),
'y': wcs.get_center(self.shape[0], self.scale['y'],
self.reference_pixel['y'],
self.reference_coordinate['y'])
}
def _draw_limb(self, fig, axes):
"""Draws a circle representing the solar limb"""
circ = patches.Circle([0, 0], radius=self.rsun_arcseconds, fill=False,
color='white')
axes.add_artist(circ)
return fig, axes
def _draw_grid(self, fig, axes, grid_spacing=20):
"""Draws a grid over the surface of the Sun"""
# define the number of points for each latitude or longitude line
num_points = 20
hg_longitude_deg = np.linspace(-90, 90, num=num_points)
hg_latitude_deg = np.arange(-90, 90, grid_spacing)
# draw the latitude lines
for lat in hg_latitude_deg:
hg_latitude_deg_mesh, hg_longitude_deg_mesh = np.meshgrid(
lat * np.ones(num_points), hg_longitude_deg)
x, y = wcs.convert_hg_hpc(self.rsun_meters,
self.dsun, self.heliographic_latitude,
self.heliographic_longitude,
hg_longitude_deg_mesh,
hg_latitude_deg_mesh, units='arcsec')
axes.plot(x, y, color='white', linestyle='dotted')
hg_longitude_deg = np.arange(-90, 90, grid_spacing)
hg_latitude_deg = np.linspace(-90, 90, num=num_points)
# draw the longitude lines
for lon in hg_longitude_deg:
hg_longitude_deg_mesh, hg_latitude_deg_mesh = np.meshgrid(
lon * np.ones(num_points), hg_latitude_deg)
x, y = wcs.convert_hg_hpc(self.rsun_meters,
self.dsun, self.heliographic_latitude,
self.heliographic_longitude,
hg_longitude_deg_mesh,
hg_latitude_deg_mesh, units='arcsec')
axes.plot(x, y, color='white', linestyle='dotted')
return fig, axes
def _validate(self):
"""Validates the meta-information associated with a Map.
This function includes very basic validation checks which apply to
all of the kinds of files that SunPy can read. Datasource-specific
validation should be handled in the relevant file in the
sunpy.map.sources package."""
if (self.dsun <= 0 or self.dsun >= 40 * constants.au):
raise InvalidHeaderInformation("Invalid value for DSUN")
def std(self, *args, **kwargs):
"""overide np.ndarray.std()"""
return np.array(self, copy=False, subok=False).std(*args, **kwargs)
def mean(self, *args, **kwargs):
"""overide np.ndarray.mean()"""
return np.array(self, copy=False, subok=False).mean(*args, **kwargs)
def min(self, *args, **kwargs):
"""overide np.ndarray.min()"""
return np.array(self, copy=False, subok=False).min(*args, **kwargs)
def max(self, *args, **kwargs):
"""overide np.ndarray.max()"""
return np.array(self, copy=False, subok=False).max(*args, **kwargs)
def data_to_pixel(self, value, dim):
"""Convert pixel-center data coordinates to pixel values"""
if dim not in ['x', 'y']:
raise ValueError("Invalid dimension. Must be one of 'x' or 'y'.")
size = self.shape[dim == 'x'] # 1 if dim == 'x', 0 if dim == 'y'.
return (value - self.center[dim]) / self.scale[dim] + ((size - 1) / 2.)
def get_header(self):
"""Returns an updated MapHeader instance"""
header = self._original_header.copy()
# Bit-depth
#
# 8 Character or unsigned binary integer
# 16 16-bit twos-complement binary integer
# 32 32-bit twos-complement binary integer
# -32 IEEE single precision floating point
# -64 IEEE double precision floating point
#
if not header.has_key('bitpix'):
bitdepth = 8 * self.dtype.itemsize
if self.dtype.kind == "f":
bitdepth = - bitdepth
header['bitpix'] = bitdepth
# naxis
header['naxis'] = self.ndim
header['naxis1'] = self.shape[0]
header['naxis2'] = self.shape[1]
# dsun
if header.has_key('dsun_obs'):
header['dsun_obs'] = self.dsun
# rsun_obs
if header.has_key('rsun_obs'):
header['rsun_obs'] = self.rsun_arcseconds
elif header.has_key('solar_r'):
header['solar_r'] = self.rsun_arcseconds
elif header.has_key('radius'):
header['radius'] = self.rsun_arcseconds
# cdelt
header['cdelt1'] = self.scale['x']
header['cdelt2'] = self.scale['y']
# crpix
header['crval1'] = self.reference_coordinate['x']
header['crval2'] = self.reference_coordinate['y']
# crval
header['crpix1'] = self.reference_pixel['x']
header['crpix2'] = self.reference_pixel['y']
return header
def resample(self, dimensions, method='linear'):
"""Returns a new Map that has been resampled up or down
Arbitrary resampling of the Map to new dimension sizes.
Uses the same parameters and creates the same co-ordinate lookup points
as IDL''s congrid routine, which apparently originally came from a
VAX/VMS routine of the same name.
Parameters
----------
dimensions : tuple
Dimensions that new Map should have.
Note: the first argument corresponds to the 'x' axis and the second
argument corresponds to the 'y' axis.
method : {'neighbor' | 'nearest' | 'linear' | 'spline'}
Method to use for resampling interpolation.
* neighbor - Closest value from original data
* nearest and linear - Uses n x 1-D interpolations using
scipy.interpolate.interp1d
* spline - Uses ndimage.map_coordinates
Returns
-------
out : Map
A new Map which has been resampled to the desired dimensions.
References
----------
| http://www.scipy.org/Cookbook/Rebinning (Original source, 2011/11/19)
"""
from sunpy.image import resample
# Note: because the underlying ndarray is transposed in sense when
# compared to the Map, the ndarray is transposed, resampled, then
# transposed back
# Note: "center" defaults to True in this function because data
# coordinates in a Map are at pixel centers
# Make a copy of the original data and perform resample
data = resample(np.asarray(self).copy().T, dimensions,
method, center=True)
# Update image scale and number of pixels
header = self._original_header.copy()
# Note that 'x' and 'y' correspond to 1 and 0 in self.shape,
# respectively
scale_factor_x = (float(self.shape[1]) / dimensions[0])
scale_factor_y = (float(self.shape[0]) / dimensions[1])
# Create new map instance
new_map = self.__class__(data.T, header)
# Update metadata
new_map.scale['x'] *= scale_factor_x
new_map.scale['y'] *= scale_factor_y
new_map.reference_pixel['x'] = (dimensions[0] + 1) / 2.
new_map.reference_pixel['y'] = (dimensions[1] + 1) / 2.
new_map.reference_coordinate['x'] = self.center['x']
new_map.reference_coordinate['y'] = self.center['x']
return new_map
def save(self, filepath):
"""Saves the SunPy Map object to a file.
Currently SunPy can only save files in the FITS format. In the future
support will be added for saving to other formats.
Parameters
----------
filepath : string
Location to save file to.
"""
pyfits_header = self.get_header().as_pyfits_header()
hdu = pyfits.PrimaryHDU(self, header=pyfits_header)
hdulist = pyfits.HDUList([hdu])
hdulist.writeto(os.path.expanduser(filepath))
def submap(self, range_a, range_b, units="data"):
"""Returns a submap of the map with the specified range
Parameters
----------
range_a : list
The range of the Map to select across either the x axis.
range_b : list
The range of the Map to select across either the y axis.
units : {'data' | 'pixels'}, optional
The units for the supplied ranges.
Returns
-------
out : Map
A new map instance is returned representing to specified sub-region
Examples
--------
>>> aia.submap([-5,5],[-5,5])
AIAMap([[ 341.3125, 266.5 , 329.375 , 330.5625, 298.875 ],
[ 347.1875, 273.4375, 247.4375, 303.5 , 305.3125],
[ 322.8125, 302.3125, 298.125 , 299. , 261.5 ],
[ 334.875 , 289.75 , 269.25 , 256.375 , 242.3125],
[ 273.125 , 241.75 , 248.8125, 263.0625, 249.0625]])
>>> aia.submap([0,5],[0,5], units='pixels')
AIAMap([[ 0.3125, -0.0625, -0.125 , 0. , -0.375 ],
[ 1. , 0.1875, -0.8125, 0.125 , 0.3125],
[-1.1875, 0.375 , -0.5 , 0.25 , -0.4375],
[-0.6875, -0.3125, 0.8125, 0.0625, 0.1875],
[-0.875 , 0.25 , 0.1875, 0. , -0.6875]])
"""
if units is "data":
# Check edges (e.g. [:512,..] or [:,...])
if range_a[0] is None:
range_a[0] = self.xrange[0]
if range_a[1] is None:
range_a[1] = self.xrange[1]
if range_b[0] is None:
range_b[0] = self.yrange[0]
if range_b[1] is None:
range_b[1] = self.yrange[1]
#x_pixels = [self.data_to_pixel(elem, 'x') for elem in range_a]
x_pixels = [np.ceil(self.data_to_pixel(range_a[0], 'x')),
np.floor(self.data_to_pixel(range_a[1], 'x')) + 1]
#y_pixels = [self.data_to_pixel(elem, 'y') for elem in range_b]
y_pixels = [np.ceil(self.data_to_pixel(range_b[0], 'y')),
np.floor(self.data_to_pixel(range_b[1], 'y')) + 1]
elif units is "pixels":
# Check edges
if range_a[0] is None:
range_a[0] = 0
if range_a[1] is None:
range_a[1] = self.shape[0]
if range_b[0] is None:
range_b[0] = 0
if range_b[1] is None:
range_b[1] = self.shape[0]
x_pixels = range_a
y_pixels = range_b
else:
raise ValueError(
"Invalid unit. Must be one of 'data' or 'pixels'")
# Make a copy of the header with updated centering information
header = self._original_header.copy()
# Get ndarray representation of submap
data = np.asarray(self)[y_pixels[0]:y_pixels[1],
x_pixels[0]:x_pixels[1]]
# Instantiate new instance and update metadata
new_map = self.__class__(data.copy(), header)
new_map.reference_pixel['x'] = self.reference_pixel['x'] - x_pixels[0]
new_map.reference_pixel['y'] = self.reference_pixel['y'] - y_pixels[0]
return new_map
@toggle_pylab
def plot(self, figure=None, overlays=None, draw_limb=True, gamma=None,
draw_grid=False, colorbar=True, basic_plot=False, **matplot_args):
"""Plots the map object using matplotlib
Parameters
----------
overlays : list
List of overlays to include in the plot
draw_limb : bool
Whether the solar limb should be plotted.
draw_grid : bool
Whether solar meridians and parallels
grid_spacing : float
Set the spacing between meridians and parallels for the grid
gamma : float
Gamma value to use for the color map
colorbar : bool
Whether to display a colorbar next to the plot
basic_plot : bool
If true, the data is plotted by itself at it's natural scale; no
title, labels, or axes are shown.
**matplot_args : dict
Matplotlib Any additional imshow arguments that should be used
when plotting the image.
"""
if overlays is None:
overlays = []
if draw_limb:
overlays = overlays + [self._draw_limb]
# TODO: need to be able to pass the grid spacing to _draw_grid from the
# plot command.
if draw_grid:
overlays = overlays + [self._draw_grid]
# Create a figure and add title and axes
if figure is None:
figure = plt.figure(frameon=not basic_plot)
# Basic plot
if basic_plot:
axes = plt.Axes(figure, [0., 0., 1., 1.])
axes.set_axis_off()
figure.add_axes(axes)
# Normal plot
else:
axes = figure.add_subplot(111)
axes.set_title("%s %s" % (self.name, self.date))
# x-axis label
if self.coordinate_system['x'] == 'HG':
xlabel = 'Longitude [%s]' % self.units['x']
else:
xlabel = 'X-position [%s]' % self.units['x']
# y-axis label
if self.coordinate_system['y'] == 'HG':
ylabel = 'Latitude [%s]' % self.units['y']
else:
ylabel = 'Y-position [%s]' % self.units['y']
axes.set_xlabel(xlabel)
axes.set_ylabel(ylabel)
# Determine extent
extent = self.xrange + self.yrange
# Matplotlib arguments
params = {
"cmap": self.cmap,
"norm": self.norm()
}
params.update(matplot_args)
if gamma is not None:
params['cmap'] = copy(params['cmap'])
params['cmap'].set_gamma(gamma)
im = axes.imshow(self, origin='lower', extent=extent, **params)
if colorbar and not basic_plot:
figure.colorbar(im)
for overlay in overlays:
figure, axes = overlay(figure, axes)
return figure
def show(self, figure=None, overlays=None, draw_limb=False, gamma=1.0,
draw_grid=False, colorbar=True, basic_plot=False, **matplot_args):
"""Displays map on screen. Arguments are same as plot()."""
self.plot(figure, overlays, draw_limb, gamma, draw_grid, colorbar,
basic_plot, **matplot_args).show()
def norm(self):
"""Default normalization method"""
return None
@classmethod
def parse_file(cls, filepath):
"""Reads in a map file and returns a header and data array"""
data, dict_header = read_file(filepath)
header = MapHeader(dict_header)
return header, data
@classmethod
def read(cls, filepath):
"""Map class factory
Attempts to determine the type of data associated with input and
returns an instance of either the generic BaseMap class or a subclass
of BaseMap such as AIAMap, EUVIMap, etc.
Parameters
----------
filepath : string
Path to a valid FITS or JPEG 2000 file of a type supported by SunPy
Returns
-------
out : Map
Returns a Map instance for the particular type of data loaded.
"""
header, data = cls.parse_file(filepath)
if cls.__name__ is not "BaseMap":
return cls(data, header)
for cls in BaseMap.__subclasses__():
if cls.is_datasource_for(header):
return cls(data, header)
return BaseMap(data, header)
@classmethod
def read_header(cls, filepath):
"""Attempts to detect the datasource type and returns meta-information
for that particular datasource."""
dict_header = read_file_header(filepath)
header = MapHeader(dict_header)
for cls in BaseMap.__subclasses__():
if cls.is_datasource_for(header):
properties = cls.get_properties(header)
properties['header'] = header
return properties
