HIRSKLM
- class typhon.datasets.tovs.HIRSKLM(name=None, **kwargs)[source]
- __init__(*args, **kwargs)[source]
Methods
__init__
(*args, **kwargs)as_xarray_dataset
(M[, skip_dimensions, ...])Convert structured ndarray to xarray dataset
calc_time_since_last_calib
(M[, D, H, fn])Calculate time since last calibration.
calibrate
(cc, counts)Apply the standard calibration from NOAA KLM User's Guide.
check_parity
(counts)Verify parity for counts
combine
(my_data, other_obj[, other_data, ...])Combine with data from other dataset.
count_lines_since_last_calib
(M[, D, H, fn])Count scanlines since last calibration.
Find the directory containing granules/measurements at (date)time
find_granules
([dt_start, dt_end, ...])Yield all granules/measurementfiles in period
find_granules_sorted
([dt_start, dt_end, ...])Yield all granules, sorted by times.
find_most_recent_granule_before
(instant, ...)Find granule covering instant
flagscore
(M)Calculate "flag score"; higher is worse.
get_additional_field
(M, fld)Get additional field.
get_cc
(scanlines)Extract calibration coefficients from scanlines.
get_dataname
(header[, robust])Extract dataname from header.
get_definition_from_PDF
(path_to_pdf)Get HIRS definition from NWPSAF PDF.
get_dtypes
(f)Get dtypes for file.
Return dict (re.fullmatch) for granule, based on re
get_iwt
(header, elem)Get temperature of internal warm target
get_mask_from_flags
(header, lines[, max_flagged])Set mask in lines, based on header and lines info
get_other
(scanlines)Get other information from scanlines.
What extra format variables are needed in find_granules?
get_pos
(scanlines)Get lat-lon from scanlines.
Return the resolution for the subdir precision.
get_temp
(header, elem, anwrd)Get temperatures from header, element, anwrd
Get datetime objects for beginning and end of granule
get_times_for_granule
(p, **kwargs)For granule stored in path, get start and end times.
get_wn_c1_c2
(header)Read central wavenumber, c1, and c2 from header
id2name
(satid)Translate satellite id to satellite name.
id2no
(satid)Translate satellite id to satellite number.
iterate_subdirs
(d_start, d_end, **extra)Iterate through all subdirs in dataset.
rad2bt
(rad_wn, wn, c1, c2)Apply the standard radiance-to-BT conversion from NOAA KLM User's Guide.
read
([f, fields, pseudo_fields])Read granule in file and do some other fixes
read_cpids
(path)Read calibration parameters input data sets (CPIDS)
read_period
([start, end, onerror, fields, ...])Read all granules between start and end, in bulk.
seekhead
(f)Seek open file to header position.
setlocal
()Set local attributes, from config or otherwise.
verify_mandatory_fields
(extra)Attributes
aliases
basedir
concat_coor
count_end
count_start
counts_offset
datefields
default_orbit_filters
dist_space_iwct
end_date
filter_calibcounts
filter_prttemps
flag_fields
format_definition_file
granule_cache_file
granule_duration
granules_firstline_db
granules_firstline_file
mandatory_fields
max_valid_time_ptp
maxsize
my_pseudo_fields
n_calibchannels
n_channels
n_minorframes
n_perline
n_wordperframe
name
re
read_returns
refields
related
satellites
satname
scantype_fieldname
section
srf_backend_f
srf_backend_response
srf_dir
srf_rttov
start_date
subdir
temperature_fields
time_field
typ_Earth
typ_iwt
typ_space
unique_fields
valid_field_values
dict() -> new empty dictionary dict(mapping) -> new dictionary initialized from a mapping object's (key, value) pairs dict(iterable) -> new dictionary initialized as if via: d = {} for k, v in iterable: d[k] = v dict(**kwargs) -> new dictionary initialized with the name=value pairs in the keyword argument list. For example: dict(one=1, two=2).
views