本文整理汇总了Python中parallel.parallel_data_helper.ParallelDataHelper.setupIO方法的典型用法代码示例。如果您正苦于以下问题:Python ParallelDataHelper.setupIO方法的具体用法?Python ParallelDataHelper.setupIO怎么用?Python ParallelDataHelper.setupIO使用的例子?那么, 这里精选的方法代码示例或许可以为您提供帮助。您也可以进一步了解该方法所在类parallel.parallel_data_helper.ParallelDataHelper
的用法示例。
在下文中一共展示了ParallelDataHelper.setupIO方法的5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: hanningsmooth
# 需要导入模块: from parallel.parallel_data_helper import ParallelDataHelper [as 别名]
# 或者: from parallel.parallel_data_helper.ParallelDataHelper import setupIO [as 别名]
def hanningsmooth(
vis=None,
outputvis=None,
keepmms=None,
field=None,
spw=None,
scan=None,
antenna=None,
correlation=None,
timerange=None,
intent=None,
array=None,
uvrange=None,
observation=None,
feed=None,
datacolumn=None,
):
"""Hanning smooth frequency channel data to remove Gibbs ringing
"""
casalog.origin("hanningsmooth")
# Initiate the helper class
pdh = ParallelDataHelper("hanningsmooth", locals())
# Validate input and output parameters
try:
pdh.setupIO()
except Exception, instance:
casalog.post("%s" % instance, "ERROR")
return False
示例2: split2
# 需要导入模块: from parallel.parallel_data_helper import ParallelDataHelper [as 别名]
# 或者: from parallel.parallel_data_helper.ParallelDataHelper import setupIO [as 别名]
def split2(vis,
outputvis,
keepmms,
field,
spw,
scan,
antenna,
correlation,
timerange,
intent,
array,
uvrange,
observation,
feed,
datacolumn,
keepflags,
width,
timebin,
combine
):
"""Create a visibility subset from an existing visibility set"""
casalog.origin('split2')
# Initialize the helper class
pdh = ParallelDataHelper("split2", locals())
# Validate input and output parameters
try:
pdh.setupIO()
except Exception, instance:
casalog.post('%s'%instance,'ERROR')
return False
示例3: cvel2
# 需要导入模块: from parallel.parallel_data_helper import ParallelDataHelper [as 别名]
# 或者: from parallel.parallel_data_helper.ParallelDataHelper import setupIO [as 别名]
def cvel2(
vis,
outputvis,
keepmms,
passall, # hidden parameter for backwards compatibiliy
field,
spw,
scan,
antenna,
correlation,
timerange,
intent,
array,
uvrange,
observation,
feed,
datacolumn,
mode,
nchan,
start,
width,
interpolation,
phasecenter,
restfreq,
outframe,
veltype,
hanning,
):
""" This task used the MSTransform framework. It needs to use the ParallelDataHelper
class, implemented in parallel.parallel_data_helper.py.
"""
# Initialize the helper class
pdh = ParallelDataHelper("cvel2", locals())
casalog.origin("cvel2")
# Validate input and output parameters
try:
pdh.setupIO()
except Exception, instance:
casalog.post("%s" % instance, "ERROR")
return False
示例4: mstransform
# 需要导入模块: from parallel.parallel_data_helper import ParallelDataHelper [as 别名]
# 或者: from parallel.parallel_data_helper.ParallelDataHelper import setupIO [as 别名]
def mstransform(
vis,
outputvis, # output
createmms, # MMS --> partition
separationaxis,
numsubms,
tileshape, # tiling
field,
spw,
scan,
antenna,
correlation,
timerange,
intent,
array,
uvrange,
observation,
feed,
datacolumn,
realmodelcol,
keepflags,
usewtspectrum,
combinespws, # spw combination --> cvel
chanaverage, # channel averaging --> split
chanbin,
hanning, # Hanning --> cvel
regridms, # regridding to new frame --> cvel
mode,
nchan,
start,
width,
nspw, # spw separation
interpolation,
phasecenter,
restfreq,
outframe,
veltype,
timeaverage, # time averaging --> split
timebin,
timespan,
maxuvwdistance,
docallib,
callib,
douvcontsub,
fitspw,
fitorder,
want_cont,
denoising_lib,
nthreads,
niter,
disableparallel, # HIDDEN parameter to create MMS in sequential
ddistart, # HIDDEN internal parameter for the sub-table re-indexing
taql, # HIDDEN internal parameter
monolithic_processing, # HIDDEN parameter for the MMS monolithic processing
reindex # HIDDEN parameter for use in the pipeline context only
):
''' This task can replace split, cvel, partition and hanningsmooth '''
casalog.origin('mstransform')
''' HEURISTICS:
input MS --> output MS
input MMS --> output MMS
user can set createmms=True to create the following:
input MS --> output MMS
'''
# Initialize the helper class
pdh = ParallelDataHelper('mstransform', locals())
# When dealing with MMS, process in parallel or sequential
# disableparallel is a hidden parameter. Only for debugging purposes!
if disableparallel:
pdh.bypassParallelProcessing(1)
else:
pdh.bypassParallelProcessing(0)
# Validate input and output parameters
try:
pdh.setupIO()
except Exception, instance:
casalog.post('%s'%instance,'ERROR')
return False
示例5: partition
# 需要导入模块: from parallel.parallel_data_helper import ParallelDataHelper [as 别名]
# 或者: from parallel.parallel_data_helper.ParallelDataHelper import setupIO [as 别名]
def partition(vis,
outputvis,
createmms,
separationaxis,
numsubms,
flagbackup, # only for MMS
datacolumn,
field,
spw,
scan,
antenna,
correlation,
timerange,
intent,
array,
uvrange,
observation,
feed,
disableparallel, # HIDDEN parameter to create an MMS in sequential
ddistart, # HIDDEN parameter to be used when merging sub-tables
taql # HIDDEN parameter to be used for balanced partition schema
):
"""Create a multi visibility set from an existing visibility set:
Keyword arguments:
vis -- Name of input visibility file (MS)
default: none; example: vis='ngc5921.ms'
outputvis -- Name of output visibility file (MS)
default: none; example: outputvis='ngc5921_src.ms'
createmms -- Boolean flag if we're creating Multi MS
default: True
separationaxis -- what axis do we intend to split on.
default = 'auto'
Options: 'scan','spw','auto'
numsubms -- Number of sub-MSs to create.
default: 'auto'
flagbackup -- Backup the FLAG column of the output MMS
default: True
datacolumn -- Which data column to use to create the output
default='data'; example: datacolumn='data'
Options: 'data', 'corrected', 'model', 'all',
'float_data', 'lag_data', 'float_data,data', and
'lag_data,data'.
note: 'all' = whichever of the above that are present.
field -- Field name
default: field = '' means use all sources
field = 1 # will get field_id=1 (if you give it an
integer, it will retrieve the source with that index)
field = '1328+307' specifies source '1328+307'.
Minimum match can be used, egs field = '13*' will
retrieve '1328+307' if it is unique or exists.
Source names with imbedded blanks cannot be included.
spw -- Spectral window index identifier
default=-1 (all); example: spw=1
antenna -- antenna names
default '' (all),
antenna = '3 & 7' gives one baseline with antennaid = 3,7.
timerange -- Time range
default='' means all times. examples:
timerange = 'YYYY/MM/DD/hh:mm:ss~YYYY/MM/DD/hh:mm:ss'
timerange='< YYYY/MM/DD/HH:MM:SS.sss'
timerange='> YYYY/MM/DD/HH:MM:SS.sss'
timerange='< ddd/HH:MM:SS.sss'
timerange='> ddd/HH:MM:SS.sss'
scan -- Scan numbers to select.
default '' (all).
intent -- Select based on the scan intent.
default '' (all)
array -- (Sub)array IDs to select.
default '' (all).
uvrange -- uv distance range to select.
default '' (all).
observation -- observation ID(s) to select.
default '' (all).
"""
casalog.origin('partition')
# Initiate the helper class
pdh = ParallelDataHelper('partition', locals())
# Validate input and output parameters
try:
pdh.setupIO()
except Exception, instance:
casalog.post('%s'%instance,'ERROR')
return False