------------------------------
MADIS Satsnddump Program Usage
------------------------------


1.0  Introduction
-----------------

The MADIS satsnddump program can be used to read satellite soundings metadata,
observations, and quality control (QC) information for a single time, and dump 
this to an output text file.  The operation of the program is controlled by a 
text parameter file that allows the user to exercise all of the options included 
in the MADIS system for satellite soundings data.  The program can be run as 
needed to access any MADIS data stored on your system, or can be run as a 
time-scheduled task to get data keyed to the current time.

This document describes how to setup the parameter file, how to run the 
program, and what to expect in the way of outputs.  Fortran programmers who 
wish to write their own programs to read MADIS data can find much of the same 
information in the satsnddump.f source code in the src directory.  In addition to 
being used for the dump utility, the code is annotated to provide a tutorial for 
programmers.


2.0  How to Run
---------------

1.  Make sure you have the necessary environment variables defined:

    - MADIS_STATIC  points to the MADIS static files directory

    - MADIS_DATA    points to the top-level MADIS data directory

    AWIPS users should point MADIS_DATA to FXA_DATA.

    See the INSTALL.* files for information on how to set environment 
    variables on your system.

2.  Setup the desired parameters in a satsnddump parameter file.

3.  Move to the directory in which you'll be running the program.

4.  Copy the parameter file to the run directory, and make sure that its 
    name is "satsnddump.par".

5.  Run the program.  (bin/satsnddump.exe on Unix/Linux, bin/satsnddump on 
    Windows)

6.  Outputs:

    a.  An activity log showing the selections made from the parameter file,
        as well as any errors that resulted will be written to standard output.
    
    b.  The data that's been obtained will be written to satsnddump.txt in the
        run directory.


3.0  How to Setup the Parameter File
------------------------------------

These sample parameter files can be found in the doc directory:

- satsnddump.par    Dumps all variables, using defaults for all options.

- satsnddump1.par   Example of how to specify that data be dumped for only 
                    certain data providers, and for only a few variables.

The parameter file is split into several sections, with each section delimited
by a line of "----------"'s.  With a couple of exceptions noted below, you
must include all lines that are within each section (in other words, the 
sections are "fixed length").  Each of the sections is described below, in the 
order in which they appear in the parameter file.


3.1  Database Section
---------------------

---------------------------------------------------------------------------------
              Database                                    FIXED LENGTH SECTION
              --------
FSL           'FSL' or 'AWIPS'
---------------------------------------------------------------------------------

If you have obtained MADIS files from FSL, leave the line as shown above.  If
you're reading AWIPS data, enter AWIPS at the beginning of the line.


3.2  Time Window Section
------------------------

---------------------------------------------------------------------------------
              Time Window (use 0,0,0 for default)         FIXED LENGTH SECTION
              -----------
-150          Number of minutes relative to nominal time at which to start window
30            Number of minutes relative to nominal time at which to end window
4             0 - return all records within the file containing nominal time
              4 - return all records within *window*
---------------------------------------------------------------------------------

The user selects the nominal time of the data to be returned in the Time
Selection section below.  Time "windowing" is used so that the program will
know how close in time each station's (i.e., satellite) observation time needs 
to be to the nominal time in order to be included.  The time window is specified 
by selecting the number of minutes before and after the nominal time to be used 
for the window.

If the default values (0,0,0) are selected, then all records will be returned 
from the file containing the nominal time.  Each file contains one hour, with
observation times from 29 minutes before the top of the hour through 30 
minutes after the top of the hour.

The sounding products are available for the different satellites, and for the 
different types of sounding products.  The observation times vary, and the 
latency ranges from about one and a half to three hours (latency is defined 
as the time the data are available minus the observation time).  

The settings shown in the sample section above (-150,30,4) will return all 
records within 2.5 hours before and 0.5 hours after the nominal time.

If you are running the program as a scheduled task with the nominal time
keyed to the current time, one recommended window setting would be -150,0,4.
This would return the observations for every satellite soundings product 
that had been made available within the last 2.5 hours.

The maximum window is 180 minutes.  Also note that the window is inclusive,
that is, using start & end minutes -30,30 with a nominal time of 12:00 will
return observations with times ranging from 11:30 through 12:30.


3.3  Provider Section
---------------------

---------------------------------------------------------------------------------
              Providers (see doc/satsnd_providers.txt)    VARIABLE LENGTH SECTION
              ---------
0             0 - all providers 
              N - list of N provider names follow this line 
---------------------------------------------------------------------------------

Satellite sounding datasets are available for different satellites.  In MADIS 
parlance, these are specified by "provider".  If desired, the user can select 
only a subset of the total by specifying which providers are to be included or 
excluded.

The default (shown above) is to enable both POES satellites.

See satsnddump1.par for an example of how to edit this variable-length section
to specify a list of providers to be enabled.

Here's the list of provider names recognized by MADIS:

  'ALL-POES'     All POES satellites
  'NOAA-15'      NOAA-15
  'NOAA-16'      NOAA-16
  'NOAA-18'      NOAA-18


3.4  Domain Filter Section
--------------------------

---------------------------------------------------------------------------------
              Domain Filter                               FIXED LENGTH SECTION
              -------------
0             0 - don't filter
              1 - return stations within latitude/longitude corners
              2 - return stations within specified Polar Stereographic grid
              3 - return stations within specified Lambert Conformal Conic grid

              Latitude/Longitude Corners (lines skipped if not Domain Filter 1)
              --------------------------
37.0          SW corner latitude (north)   
-109.0        SW corner longitude (east)
41.0          NE corner latitude (north)
-102.0        NE corner longitude (east)

              Polar Stereo Specification (lines skipped if not Domain Filter 2)
              --------------------------
190500.0      Grid box size (meters)
7.838         Latitude (north) of 1st grid point (lower left = SW)
-141.028      Longitude (east) of 1st grid point (lower left = SW)
-95.0         Orientation longitude (east)                 
33.0          I-coordinate of pole
45.0          J-coordinate of pole
60.0          Lat (north) at which X-Y scale is true
65            Number of grid points in X-direction (I dimension)
43            Number of grid points in Y-direction (J dimension)

              Lambert Conformal Conic Specification (lines skipped if not Domain Filter 3)
              -------------------------------------
40635.25      Grid box size (meters)
12.19         Latitude (north) of 1st grid point (lower left = SW)
-133.459      Longitude (east) of 1st grid point (lower left = SW)
-95.0         Orientation longitude (east)
25.0          Latitude (north) of first Lambert Conformal tangent
25.0          Latitude (north) of second Lambert Conformal tangent
185           Number of grid points in X-direction (I dimension)
129           Number of grid points in Y-direction (J dimension)
---------------------------------------------------------------------------------

The horizontal domain can be limited to match one of two map projections (polar 
stereographic, Lambert conformal conic) or it can be limited to a 
latitude/longitude rectangle.  Only stations within the domain will be returned.  
If one of the map projections is selected, any soundings (of any form) returned 
will be rotated to match the projection.  

If the default is selected (as above), no domain filtering will be performed,
and all available stations will be returned, regardless of their location.

(The example Latitude/Longitude specification shown above is for the state of
Colorado, the example Polar Stereographic specification defines AWIPS grid 202 
(NATIONAL-CONUS), and the example Lambert Conformal specification defines AWIPS 
grid 212 (REGIONAL-CONUS-DOUBLE RESOLUTION).)
 
If one of the map projections has been selected for the horizontal domain, the 
station latitude and longitude will be converted to a grid index into the 
2-dimensional grid (RI,RJ).  Note that this works for grids laid out this way:

                     NE (I=NX,J=NY)

  SW (I=1,J=1)

The calculated index will appear in satsnddump.txt in the "Grid I" and "Grid J"
columns.  If a map projection isn't being used, Grid I and Grid J will be
output as zeros.


3.5  QC Filter Section
----------------------

---------------------------------------------------------------------------------
              QC Filter                                   FIXED LENGTH SECTION    
              ---------
0              0 - none
               1 - coarse
              99 - highest possible
---------------------------------------------------------------------------------

The primary variables in all MADIS datasets have been screened by
automated quality control (QC) checks.  Different variables have
different levels of QC, or "stages", applied to them.  In addition to
the QC processing done by the satellite provider (who generally toss
observations that are below their own quality thresholds), currently
the satellite sounds have a MADIS level 1 validity check applied to
the temperature and level 1 and 2 applied to the dewpoint temperature
(calculated from the mixing ratio).  See satsnd_qc_variable_list.txt
for more information.  (Level 1 checks = "coarse".)

Each variable that gets dumped will also have its associated QC
information written to satsnddump.txt.  This includes a QC data
descriptor (a single character summarizing the info), and bitmasks
showing which QC checks were applied and the results of the checks.
These appear in the "QCD", "QCA", and "QCR" columns of the output.
For details on how to interpret these items see qc_info.txt.

If the user doesn't want to interpret the QC info, he or she can limit
the returned obs to selectable levels of quality.  In that case, obs
that don't meet the selected QC level will be omitted.

There are three ways that the user can request and process the QC information:

  1) Use the default setting (shown above) which will disable QC filtering.
     Then you can examine the QC info before deciding whether or not to use 
     each observation.  This allows for the maximum amount of control over 
     what's available.  

  2) If you know ahead of time that the same level of QC is available for all 
     variables you'll be using, select that level.

  3) To require that all variables pass the highest level of QC that are 
     specified for them, select QC level 99.

User's of MADIS data who want the data filtered by QC results, but don't want to
interpret the QC information themselves, should select QC level 99.


3.6  Time Selection Section
---------------------------

---------------------------------------------------------------------------------
	      Time Selection                              FIXED LENGTH SECTION
              --------------
1             0 - Julian format (YYJJJHHMM)
              1 - Month/Day format (YYYYMMDD_HHMM)
0             0 - Use the nominal time line below
              1 - Use the current time as the nominal time
20040324_1200 Nominal time (in selected format)
---------------------------------------------------------------------------------

All MADIS data are time-stamped in Universal Coordinated Time (also called GMT).
Two formats are supported, both for inputting the nominal time in the 
parameter file, and for outputting the time in the satsnddump.txt output file.

"Julian format" is in the form of "YYJJJHHMM", where:

  YY  = 2-digit year (good from 1980 - 2179)
  JJJ = Julian date of the year (001-366)
  HH  = Hour (00-23)
  MM  = Minute (00-59)

"Month/Day" format uses "YYYYMMDD_HHMM", where:

  YYYY = 4-digit year (still only good from 1980 - 2179)
  MMDD = Month/Day 
  HHMM = Hour/Minute 

The nominal time shown above in the Month/Day format translates to 040841200
in the Julian format.

Nominal times can be specified at any minute, not just at the top of the hour 
(minute 00).

To run the program as a scheduled task, specify that the current time be
used as the nominal time and set an appropriate time window.


3.7  Variables Section
----------------------

---------------------------------------------------------------------------------
              Variables (1 per line, until end of file)   VARIABLE LENGTH SECTION
              --------- (see doc/satsnd_variable_list.txt)
T
WVMR
---------------------------------------------------------------------------------

This is the last section in the parameter file.  The code names for the variables
to be dumped are listed, one per line, until the end of file is reached.  (The
section delimiter line shown here is simply for readability.  If you have this 
line or any other non-variable line in the real parameter file you'll get an 
error.)

The list of code names is found in the first column of satsnd_variable_list.txt,
along with the units for each variable, the maximum QC level, and many other
details.

In the above example, note that we're dumping the temperature and mixing ratio.  
For many variables, you can select multiple forms and MADIS will do the 
calculations for you.  For full information on what variables are available 
and how to interpret them, see satsnd_variable_list.txt.
