Analysing UM outputs

Revision as of 23:24, 11 December 2019 by (talk | contribs)

The UM output files are in a binary format called 'fieldsfile'. This format consists of a set of headers describing the file as a whole, a lookup table describing the fields and a data table containing the field values. The format only supports 2D fields, 3D fields are stored as a 2D field for each vertical level.

Observation and ancillary files use mostly the same format, with some minor differences in the stored vairiables.


Xconv is a visualisation tool for working with UM & NetCDF files, found in ~access/bin. Select a variable from the list by double-clicking it, then use the Plot Data button in the upper left to visualise it. You can use the section on the right to specify a subregion to look at by e.g. swapping to the 'z' co-ordinate at the bottom, selecting a vertical level then pressing Apply to show only that level.

The selection controls in Xconv are a little unusual: left click lines to add them to the selection, middle click to select only that line and right-click to select the region between that line and where you last clicked.

You can convert fields to NetCDF format from within Xconv: select multiple fields, enter a name at the top of the screen then press the Convert button.


NetCDF converters

There are a number of tools for converting between UM files and NetCDF.


iris2netcdf uses the Met Office's Iris library to do conversion from UM fields to NetCDF. It uses the Met Office's mappings between STASH codes and CF standard names, so may not have correct names for fields added specifically to ACCESS (e.g. CABLE fields)

iris2netcdf is part of the Conda environments

module use /g/data3/hh5/public/modules
module load conda/analysis3
iris2netcdf -o uabcda.pah010 is the program used by CAWCR to convert UM output to NetCDF for CMIP5 analysis. It includes CF fieldnames for most fields required by CMIP5, it's available in ~access/bin

To use the script you first need to load some Python libraries, run the script like

module use ~access/modules
module load pythonlib/cdat-lite
module load pythonlib/ScientificPython
~access/bin/ -i uabcda.pah010 -o may have problems with some fields, e.g. zonally averaged ozone.


um2cdf uses the scripting interface of Xconv to do conversion - it is the same as using the NetCDF export from the Xconv GUI.

~access/bin/um2cdf uabcda.pah010
# Will create in the current directory


Iris is a Python library developed by the Met Office for working with climate and weather data. It is able to load UM files into numpy arrays for further processing.

To make Iris available run

module use /g/data3/hh5/public/modules
module load conda/analysis3

For basic conversion the `iris2netcdf` command can convert UM format files to compressed NetCDF

To extract a field from a UM file using Iris

#!/usr/bin/env python
import iris

Tsurf = iris.load('uabcda.pah010', 'surface_temperature'), '')


CDAT is another Python-based climate data package, it provides some support for UM output files.

To make CDAT available run

module use /g/data3/hh5/public/modules
module load conda/analysis27

To extract a field from a UM file using CDAT

#!/usr/bin/env python
import cdms2

data ='uabcda.pah010')
Tsurf = data['temp']

outfile ='','w')



Mule is a python library for working with UM format files directly. It allows you to do things like modify header values for individual fields.

To make Mule available run

module use /g/data3/hh5/public/modules
module load conda/analysis3

Example Mule scripts