本文整理汇总了Python中sunpy.cm.cm.get_cmap函数的典型用法代码示例。如果您正苦于以下问题：Python get_cmap函数的具体用法？Python get_cmap怎么用？Python get_cmap使用的例子？那么恭喜您, 这里精选的函数代码示例或许可以为您提供帮助。
在下文中一共展示了get_cmap函数的15个代码示例，这些例子默认根据受欢迎程度排序。您可以为喜欢或者感觉有用的代码点赞，您的评价将有助于系统推荐出更棒的Python代码示例。
示例1: __init__
def __init__(self, data, header):
BaseMap.__init__(self, header)
self.detector = "SWAP"
self.instrument = "SWAP"
self.observatory = "PROBA2"
self.name = "SWAP %s" % header.get('wavelnth')
self.cmap = cm.get_cmap(name='sdoaia171')示例2: __init__
def __init__(self, data, header):
BaseMap.__init__(self, header)
self.detector = "AIA"
self.instrument = "AIA"
self.observatory = "SDO"
self.cmap = cm.get_cmap('sdoaia%d' % header.get('wavelnth'))示例3: get_properties
def get_properties(cls, header):
"""Parses XRT image header"""
properties = Map.get_properties(header)
# XRT uses DATE_OBS, not date-obs.
properties["date"] = parse_time(header.get('date_obs', None))
#TODO: proper exception handling here - report to the user that there is
# an unexpected value
fw1 = header.get('EC_FW1_')
if not(fw1.lower() in [x.lower() for x in cls.filter_wheel1_measurements]):
pass
fw2 = header.get('EC_FW2_')
if not(fw2.lower() in [x.lower() for x in cls.filter_wheel2_measurements]):
pass
# All images get the same color table - IDL Red temperature (loadct, 3)
properties.update({
"detector": "XRT",
"instrument": "XRT",
"observatory": "Hinode",
"name": "XRT %s-%s " % (fw1.replace('_', ' '),
fw2.replace('_', ' ')),
"nickname": "XRT",
"cmap": cm.get_cmap(name='hinodexrt')
})
return properties示例4: __init__
def __init__(self, data, header, **kwargs):
GenericMap.__init__(self, data, header, **kwargs)
self.meta['CUNIT1'] = self.meta['CUNIT1'].lower()
self.meta['CUNIT2'] = self.meta['CUNIT2'].lower()
# Fill in some missing or broken info
datestr = "{date}T{time}".format(date=self.meta.get('date-obs',
self.meta.get('date_obs')
),
time=self.meta.get('time-obs',
self.meta.get('time_obs')
)
)
self.meta['date-obs'] = datestr
# If non-standard Keyword is present, correct it too, for compatibility.
if 'date_obs' in self.meta:
self.meta['date_obs'] = self.meta['date-obs']
self.meta['wavelnth'] = np.nan
self.meta['waveunit'] = 'nm'
self._nickname = self.instrument + "-" + self.detector
self.plot_settings['cmap'] = cm.get_cmap('soholasco{det!s}'.format(det=self.detector[1]))
self.plot_settings['norm'] = ImageNormalize(stretch=PowerStretch(0.5))示例5: get_properties
def get_properties(cls, header):
"""Parses SXT image header"""
properties = Map.get_properties(header)
# 2012/11/07 - the SXT headers do not have a value of the distance from
# the spacecraft to the center of the Sun. The FITS keyword 'DSUN_OBS'
# appears to refer to the observed diameter of the Sun. Until such
# time as that is calculated and properly included in the file, we will
# use the value of 1 AU as a standard.
properties['dsun']= constants.au
wavelnth = header.get('wavelnth')
if wavelnth == 'Al.1':
wavelnth = 'Al01'
if wavelnth.lower() == 'open':
wavelnth = 'white light'
properties.update({
"detector": "SXT",
"instrument": "SXT",
"observatory": "Yohkoh",
"name": "SXT %s" % wavelnth,
"nickname": "SXT",
"cmap": cm.get_cmap(name='yohkohsxt' + wavelnth[0:2].lower())
})
return properties 示例6: get_properties
def get_properties(cls, header):
"""Parses SXT image header"""
properties = Map.get_properties(header)
# 2012/12/19 - the SXT headers do not have a value of the distance from
# the spacecraft to the center of the Sun. The FITS keyword 'DSUN_OBS'
# appears to refer to the observed diameter of the Sun. Until such
# time as that is calculated and properly included in the file, we will
# use simple trigonometry to calculate the distance of the center of
# the Sun from the spacecraft. Note that the small angle approximation
# is used, and the solar radius stored in SXT FITS files is in arcseconds.
properties["dsun"] = constants.au
yohkoh_solar_r = header.get("solar_r", None)
if yohkoh_solar_r == None:
properties["dsun"] = constants.au
else:
properties["dsun"] = constants.radius / (np.deg2rad(yohkoh_solar_r / 3600.0))
wavelnth = header.get("wavelnth")
if wavelnth == "Al.1":
wavelnth = "Al01"
if wavelnth.lower() == "open":
wavelnth = "white light"
properties.update(
{
"detector": "SXT",
"instrument": "SXT",
"observatory": "Yohkoh",
"name": "SXT %s" % wavelnth,
"nickname": "SXT",
"cmap": cm.get_cmap(name="yohkohsxt" + wavelnth[0:2].lower()),
}
)
return properties示例7: __init__
def __init__(self, data, header):
BaseMap.__init__(self, header)
self.date = parse_time(header.get('date_obs'))
self.detector = "EUVI"
self.instrument = "SECCHI"
self.observatory = header.get('obsrvtry')
self.name = "EUVI %s" % self.meas
self.cmap = cm.get_cmap('sohoeit%d' % header.get('wavelnth'))示例8: __init__
def __init__(self, data, header, **kwargs):
GenericMap.__init__(self, data, header, **kwargs)
self._name = self.observatory + " " + self.detector + " " + str(self.measurement)
self._nickname = "{0}-{1}".format(self.detector, self.observatory[-1])
self.cmap = cm.get_cmap('stereocor%s' % self.detector[-1])示例9: __init__
def __init__(self, data, header, **kwargs):
GenericMap.__init__(self, data, header, **kwargs)
# Fill in some missing info
self.meta['detector'] = "AIA"
self._nickname = self.detector
self.plot_settings['cmap'] = cm.get_cmap(self._get_cmap_name())
self.plot_settings['norm'] = ImageNormalize(stretch=source_stretch(self.meta, AsinhStretch(0.01)))示例10: __init__
def __init__(self, data, header, **kwargs):
GenericMap.__init__(self, data, header, **kwargs)
# Fill in some missing or broken info
self._fix_date()
self._name = self.instrument + " " + self.detector
self._nickname = self.instrument + "-" + self.detector
self.cmap = cm.get_cmap('soholasco%s' % self.detector[1])示例11: __init__
def __init__(self, data, header, **kwargs):
GenericMap.__init__(self, data, header, **kwargs)
# Fill in some missing info
self.meta['detector'] = "AIA"
# self.meta['instrme'] = "AIA"
self._nickname = self.detector
self.cmap = cm.get_cmap('sdoaia%d' % self.wavelength)示例12: __init__
def __init__(self, data, header, **kwargs):
GenericMap.__init__(self, data, header, **kwargs)
# Fill in some missing info
self.meta['detector'] = "AIA"
# self.meta['instrme'] = "AIA"
self._nickname = self.detector
self._name = self.detector + " " + str(self.measurement)
self.cmap = cm.get_cmap(self._get_cmap_name())示例13: __init__
def __init__(self, data, header, **kwargs):
GenericMap.__init__(self, data, header, **kwargs)
# It needs to be verified that these must actually be set and
# are not already in the header.
self.meta['detector'] = "SWAP"
# self.meta['instrme'] = "SWAP"
self.meta['obsrvtry'] = "PROBA2"
self._nickname = self.detector
self.plot_settings['cmap'] = cm.get_cmap(name='sdoaia171')示例14: __init__
def __init__(self, data, header):
BaseMap.__init__(self, header)
self.date = parse_time(header.get('date_obs'))
self.detector = header.get('telescop')
self.instrument = header.get('telescop')
self.measurement = [header.get('energy_l'), header.get('energy_h')]
self.name = "RHESSI %d - %d keV" % (header.get('energy_l'),
header.get('energy_h'))
self.cmap = cm.get_cmap('rhessi')
self.exposure_time = (parse_time(header.get('date_end')) -
parse_time(header.get('date_obs'))).seconds示例15: __init__
def __init__(self, data, header, **kwargs):
GenericMap.__init__(self, data, header, **kwargs)
# It needs to be verified that these must actually be set and are not
# already in the header.
self.meta['detector'] = "TRACE"
self.meta['obsrvtry'] = "TRACE"
self._nickname = self.detector
# Colour maps
self.plot_settings['cmap'] = cm.get_cmap('trace' + str(self.meta['WAVE_LEN']))
self.plot_settings['norm'] = ImageNormalize(stretch=source_stretch(self.meta, LogStretch()))