List of all Input Parameters¶
The example input file input_sodankyla_example.yml contains the most relevant input parameters to run the PROFFASTpylot. However, there are several more parameters which can be used optionally. In this file all parameters are given and explained.
Site information¶
instrument_number
The serial number of your EM27/SUN.site_name
The name of the current measurement site.site_abbrev
A two-letter abbreviation to assign your site to a map file.coords
Coordinates of the measurement. Alternatively, a coordinate file can be used (see below).lat: Latitude, degrees north in decimal format
lon: Longitude, degrees east in decimal format
alt: Altitude, km over sea level
coord_file
Give the coordinates in a comma separated file. An example file can be found inexamples/input_data/coords.csv
utc_offset
The UTC-offset of your measurements. This can either be due to the measurement in a different time zone or due to an error in the syncing of the PC clock.note
Optional comment included in bin-files by PROFFAST preprocess.
Steering of the behavior:¶
min_interferogram_size
File size in MegaBytes. All interferograms smaller than the given size are skipped.igram_pattern
The file name pattern of the interferograms can be used to process only specific files in the interferogram folder. The default value is*.*
which means that all files in the interferogram folders are used for processing.start_with_spectra
True
orFalse
Start the processing chain with already available spectra. The spectra have to be located at<analysis>/SiteName_InstrumentNumber/YYMMDD/cal
where<analysis>
is the given analysis path.start_date
Date with the formatYYYY-MM-DD
.
The first date to be processed. If not given, the earliest available date is the start date.end_date
Date with the formatYYYY-MM-DD
.
The last date to be processed. If not given, the latest available date is the end date.delete_abscosbin_files
False
(default) orTrue
The*abscos.bin
file contains the the simulation of the atmosphere which is the result of the PROFFAST pcxs program. Pcxs can then be skipped if the abscos files are present from a previous run. If True the*abscos.bin
will be removed after the run otherwise they are kept inprf/wrk_fast
. If the abscos files are not deleted, the pT and VMR files are copied instead of moved to the result folder in order to be present if pcxs is skipped in a following run.delete_input_files
False
(default) orTrue
If False: The output of the PROFFAST programs will be moved to results folder.instrument_parameters
To evaluate EM27/SUN data this parameter does not have to be given explicitly.
Possible values are:em27``(default), ``tccon_ka_hr
,tccon_ka_lr
,tccon_default_hr
,tccon_default_lr
,invenio
,vertex
,ircube
or a path to an instrument-config file.
For more details refer to the Instrument Parameters article of the documentation.mapfile_wetair_vmr
default:None
(determined during runtime)
If you are using other mapfiles than the standard ggg2020 or ggg2014 files you can set if the columns are based on wet air (True
) or dry air (False
).
Path settings¶
proffast_path
The path pointing to the PROFFAST folder.interferogram_path
The path to the interferograms. The data structure must be likeYYMMDD/YYMMDD*.XXX
map_path
The path pointing to the map files.pressure_path
The path pointing to the pressure data.pressure_type_file
The path pointing to the pressure setup file. For more explanation see the article about pressure input in the documentation.analysis_path
In the analysis path the spectra produced by preprocess are written to. We recommend to call it analysis. Within this folder the PROFFASTpylot will create a folder structure likeanalysis/SiteName_InstrumentNumber/YYMMDD.
Consult also the article about folder structure in the documentation.result_path
The merged results, the log files and optionally the input files are written to the result path. Within it, PROFFASTpylot will create a folder namedSiteName_InstrumentNumber_StartDate-EndDate
.