PROGRAM prepbufr

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$Id: prep_bufr.html 11441 2017-04-06 22:00:44Z $



Translating NCEP PREPBUFR files into DART obs_seq.out files (input file to filter) is a 2 stage process. The first stage uses NCEP software to translate the PREPBUFR file into an intermediate text file. This is described in this document. The second step is to translate the intermediate files into obs_seq.out files, which is done by create_real_obs, as described in create_real_obs .



The prep_bufr package is free-standing and has not been completely assimilated into the DART architecture. It also requires adaptation of the sources codes and scripts to the computing environment where it will be run. It is not so robust that it can be controlled just with input parameters. It may not have the same levels of error detection and warning that the rest of DART has, so the user should very careful about checking the end product for correctness.

Overview of what needs to be built and run

More detailed instructions follow, but this section describes a quick overview of what programs you will be building and running.


Running the script will build the library and main executable. You will probably have to edit this script to set which fortran compiler is available on your system.

If you have raw unblocked PREPBUFR files you will need to convert them to blocked format (what prepbufr expects as input). The blk/ublk section of the build script compiles the cword.x converter program.

If you are running on an Intel (little-endian) based machine you will need the grabbufr byte swapping program that is also built by this script.

One-shot execution

If you are converting a single obs file, or are walking through the process by hand for the first time, you can follow the more detailed build instructions below, and then run the prep_bufr.x program by hand. This involves the following steps:

Production mode

If you have multiple days (or months) of observations that you are intending to convert, there is a script in the work subdirectory which is set up to run the converter on a sequence of raw data files, and concatenate the output files together into one output file per day. Edit the work/prepbufr.csh script and set the necessary values in the 'USER SET PARAMETERS' section near the top. This script can either be run from the command line, or it can be submitted to a batch queue for a long series of conversion runs.

Installation of the NCEP PREPBUFR decoding program

This package is currently organized into files under the DART/observations/NCEP/prep_bufr directory:

src           Source code of the NCEP PREPBUFR decoder
lib           NCEP BUFR library source    A script to install the NCEP PREPBUFR decoder and the NCEP BUFR library.
exe           Executables of the decoder and converter.
data          Where the NCEP PREPBUFR files (prepqm****) could be loaded into
              from the NCAR Mass Store (the script assumes this is the default location).
work          Where we run the script to do the decoding.
convert_bufr  Source code (grabbufr) to convert the binary big-endian PREPBUFR files to 
              little-endian files, and a script to compile the program.
blk_ublk      Source code (cwordsh) to convert between blocked and unblocked format.
docs          Some background information about NCEP PREPBUFR observations.

The decoding program: src/prepbufr.f

The program prepbufr.f is used to decode the NCEP reanalysis PREPBUFR data into intermediate text files. This program was originally developed by NCEP. It has been modified to output surface pressure, dry temperature, specific humidity, and wind components (U/V) of conventional radiosonde, aircraft reports, and satellite cloud motion derived wind. There are additional observation types on the PREPBUFR files, but using them they would require significant modifications of prepbufr and require detailed knowledge of the NCEP PREPBUFR files. The NCEP quality control indexes for these observations based on NCEP forecasts are also output and used in DART observation sequence files. The NCEP PREPBUFR decoding program is written in Fortran 77 and has been successfully compiled on Linux computers using pgi90, SGI® computers with f77, IBM® SP® systems with xlf, and Intel® based Mac® with gfortran.

If your operating system uses modules you may need to remove the default compiler and add the one desired for this package. For example

To compile the BUFR libraries and the decoding program, set the CPLAT variable in the script to match the compilers available on your system. CPLAT = linux is the default. Execute the script to complete the compilations for the main decoding program, the NCEP BUFR library, and the conversion utilities.

The executables (i.e., prepbufr.x, prepbufr_03Z.x) are placed in the ../exe directory.

Platforms tested:

The byte-swapping program convert_bufr/grabbufr.f

For platforms with little-endian binary file format (e.g. Intel, AMD®, and non-MIPS SGI processors) the program grabbufr.f is used to convert the big-endian format NCEP PREPBUFR data into little-endian format. The grabbufr.f code is written in Fortran 90, and has been compiled can be compiled with the pgf90 compiler on a Linux system, with gfortran on an Intel based Mac, and the ifort compiler on other Linux machines. More detailed instructions for building it can be found in convert_bufr/README, but the base install script should build this by default. In case of problems, cd into the convert_bufr subdirectory, edit convert_bufr.csh to set your compiler, and run it to compile the converter code (grabbufr).

This program reads the whole PREPBUFR file into memory, and needs to know the size of the file (in bytes). Unfortunately, the system call STAT() returns this size as one number in an array, and the index into that array differs depending on the system and sometimes the word size (32 vs 64) of the compiler. To test that the program is using the right offset into this array, you can compile and run the stat_test.f program. It takes a single filename argument and prints out information about that file. One of the numbers will be the file size in bytes. Compare this to the size you see with the 'ls -l' command for that same file. If the numbers do not agree, find the right index and edit the grabbufr.f source file. Look for the INDEXVAL line near the first section of executable code.

If grabbufr.f does not compile because the getarg() or iargc() subroutines are not found or not available, then either use the arg_test.f program to debug how to get command line arguments into a fortran program on your system, or simply go into the grabbufr.f source and comment out the section which tries to parse command line arguments and comment in the hardcoded input and output filenames. Now to run this program you must either rename the data files to these predetermined filenames, or you can use links to temporarily give the files the names needed.

The blocking program blk_ublk/cword.x

The prepbufr.x program expects to read a blocked input file, which is generally what is available for download. However, if you have an unblocked file that you need to convert, there is a conversion program. The script will try to build this by default, but in case of problems you can build it separately. Change directories into the blk_ublk subdirectory and read the README_cwordsh file for more help. The cwordsh shell-script wrapper shows how to run the executable cwordsh.x executable.

Note that if you can get the blocked file formats to begin with, this program is not needed.

Getting the NCEP Reanalysis PREPBUFR format data from NCAR HPSS.

The NCEP PREPBUFR files (prepqmYYMMDDHH) can be found within the NCEP reanalysis dataset, ds090.0, on NCAR Mass Store System (HPSS).

To find the files:

Depending on the year you select, the prepqm files can be weekly, monthly, or semi-monthly. Each tar file has a unique dataset number of the form "A#####". For example, for January of 2003, the 4 HPSS TAR files are: A21899, A21900, A21901, A21902. After September 2003, these files include AIRCRAFT data (airplane readings taken at cruising elevation) but not ACARS data (airplane readings taken during takeoff and landing). There are different datasets which include ACARS data but their use is restricted and you must contact the RDA group to get access.

If you are running on a machine with direct access to the NCAR HPSS, then change directories into the prep_bufr/data subdirectory and run:

> hsi get /DSS/A##### rawfile

where ##### is the data set number you want.

These files may be readable tar files, or they may require running the cosconvert program first. See if the tar command can read them:

> tar -tvf rawfile

If you get a good table of contents then simply rename the file and untar it:

> mv rawfile data.tar
> tar -xvf data.tar

However, if you get an error from the tar command you will need to run the cosconvert program to convert the file into a readable tar file. On the NCAR machine yellowstone, run:

> /glade/u/home/rdadata/bin/cosconvert -b rawfile data.tar

On other platforms, download the appropriate version from: . Build and run the converter and then you should have a tar file you can unpack.

The output of tar should yield individual 6-hourly NCEP PREPBUFR data files for the observations in the +/- 3-hour time windows of 00Z, 06Z, 12Z, and 18Z of each day. Note that DART obs_seq files are organized such that a 24 hour file with 4 observation times would contain observations from 3:01Z to 3:00Z of the next day, centered on 6Z, 12Z, 18Z and "24Z". In addition, there are some observations at 3:00Z on the PREPBUFR file labelled with 06Z. Then, in order to make a full day intermediate file incorporating all the required obs from the "next" day, you'll need the PREPBUFR files through 6Z of the day after the last day of interest. For example, to generate the observation sequence for Jan 1, 2003, the decoded NCEP PREPBUFR text files for Jan 1 and 2, 2003 are needed, and hence the PREPBUFR files

are needed.

Running the NCEP PREPBUFR decoding program

In prep_bufr/work/prepbufr.csh set the appropriate values of the year, month, first day, and last day of the period you desire, and the variable "convert" to control conversion from big- to little-endian. Confirm that the raw PREPBUFR files are in ../data, or that prepbufr.csh has been changed to find them. Execute prepbufr.csh in the work directory. It has code for running in the LSF batch environment, but not PBS.

Currently, this script generates decoded PREPBUFR text data each 24 hours which contains the observations within the time window of -3:01 hours to +3:00Z within each six-hour synoptic time. These daily output text files are named as temp_obs.yyyymmdd. These text PREPBUFR data files can then be read by DART/observations/NCEP/ascii_to_obs/work/create_real_obs to generate the DART daily observation sequence files.

There is an alternate section in the script which creates a decoded PREPBUFR text data file each 6 hours (so they are 1-for-1 with the original PREPBUFR files). Edit the script prepbufr.csh and look for the commented out code which outputs 4 individual files per day. Note that if you chose this option, you will have to make corresponding changes in the create_obs_seq.csh script in step 2.



This is a piece of code that is intended to be 'close' to the original, as such, we have not modified it to use the DART build mechanism. This code does not use any DART modules.



This namelist is read from the file input.nml. Namelists start with an ampersand '&' and terminate with a slash '/'. Character strings that contain a '/' must be enclosed in quotes to prevent them from prematurely terminating the namelist.

   obs_window       = 1.5,
   obs_window_upa   = 1.5,
   obs_window_air   = 1.5,
   obs_window_sfc   = 0.8,
   obs_window_cw    = 1.5,
   land_temp_error  = 2.5,
   land_wind_error  = 3.5,
   land_moist_error = 0.2,
   otype_use        = missing,
   qctype_use       = missing,

Item Type Description
obs_window real Window of time to include observations. If > 0, overrides all the other more specific window sizes. Set to -1.0 to use different time windows for different obs types. The window is +/- this number of hours, so the total window size is twice this value.
obs_window_upa real Window of time to include sonde observations (+/- hours) if obs_window is < 0, otherwise ignored.
obs_window_air real Window of time to include aircraft observations (+/- hours) if obs_window is < 0, otherwise ignored.
obs_window_sfc real Window of time to include surface observations (+/- hours) if obs_window is < 0, otherwise ignored.
obs_window_cw real Window of time to include cloud wind observations (+/- hours) if obs_window is < 0, otherwise ignored.
otype_use real(300) Report Types to extract from bufr file. If unspecified, all types will be converted.
qctype_use integer(300) QC types to include from the bufr file. If unspecified, all QC values will be accepted.
land_temp_error real observation error for land surface temperature observations when none is in the input file.
land_wind_error real observation error for land surface wind observations when none is in the input file.
land_moisture_error real observation error for land surface moisture observations when none is in the input file.





DART/observations/NCEP/prep_bufr/docs/* (NCEP text files describing the PREPBUFR files)


Various, see the source code, doc directory, and README files for more help.


none at this time



This converter could be combined with the DART library code to go directly from PREPBUFR files to DART obs_sequence files.

The converter should make an output file with a fully qualified date in the name, so constructing files that start at 21Z and continue to 3Z the next day are not as difficult to process. There are currently two separate versions of the converter only because one deals with the date wrap. This shouldn't be needed.


Terms of Use

DART software - Copyright UCAR. This open source software is provided by UCAR, "as is", without charge, subject to all terms of use at

Contact: Hui Liu
Revision: $Revision: 11441 $
Source: $URL: $
Change Date: $Date: 2017-04-06 16:00:44 -0600 (Thu, 06 Apr 2017) $
Change history:  try "svn log" or "svn diff"