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The South China Sea Monsoon Experiment took place between the period of 1
May - 30 June 1998. There was a network of two ground-based radars, which was
among the many instruments that were deployed during the experiment. The radar
network was located in the center of the experimental area and was positioned
about 300 km SE of Hong Kong in the South China Sea. Both radars were 5cm
wavelength and had Doppler capability. The BMRC CPOL had the additional
capability of being polarimetric. TOGA was located about 40 km SSE of CPOL.
Radar data collection started on 4 May 1998 and ended on 25 June 1998. This
document describes the quality controlled (QC) TOGA and CPOL radar datasets.
The remaining sections of the document will describe the file naming convention and organization, a brief description of the QC
corrections, and contact information.
The distribution of these data sets is funded by NASA's
Earth Science Enterprise. The data are not copyrighted;
however, we request that when you
publish data or results using these data, please
acknowledge as follows:
The authors wish to thank Jian-Jian Wang of the Mesoscale Atmospheric
Processes Branch (Code 912), Goddard Space Flight Center, Greenbelt, Maryland
and Thomas Keenan, BMRC, Melbourne, Victoria, Australia for the production of
these data and the Data and Information Services Center(Code 610.2) at the Goddard
Space Flight Center, which archives and distributes them
under sponsorship of NASA's Earth Science Enterprise.
QC Corrections
This section only briefly highlights the corrections. A more detailed
analysis of the corrections (especially for TOGA) will be published in a
separate manuscript, but these are the main corrections the user should be
aware of.
A. TOGA Radar
TOGA had several problems that were discovered during and after the
experiment and during post_experiment analysis. A major problem occurred in
the second half of the experiment (intensive operation phase 2 (IOP2)). Water
leaked into the cables that drive the antenna causing problems in knowing the
exact location of the antenna. The geolocation of the data recorded during
IOP2 (4 June - 25 June, 1998 FOR TOGA) are not known with any certainty and are
therefore excluded from the QC dataset.
- Doppler Velocity
Incorrect sign convention The Doppler velocity
stored in the raw data had the incorrect sign (+/-). By convention, Doppler
radial velocities towards the radar are negative values and away are positive.
They were opposite in the raw data.
Ship motion correction Normally, ship motion is
subtracted out of the Doppler velocity by feeding in the ship motion obtained
by an independent inertial navigation unit (INU). This setting was not turned
on in the radar processing software. Fortunately, ship motion is stored in
every ray of data and has been subtracted from the data. The ship motion was
not large during IOP1. The maximum value seen in QC tests was about 0.4 m/s.
Radar Reflectivity
- Known engineering offset After the experiment,
engineering tests of the radar discovered a mismatch in the bandpass filter.
This mismatch caused the TOGA radar to have a 5.5dB decrease in the returned
power. Therefore, a +5.5dB offset needed to be added to the reflectivity data
for this correction.
- Unknown source offset
Extensive comparisons with CPOL, raingauge, and disdrometer data revealed that TOGA reflectivity was still too low. It is +8.0dB based on these comparisons. The source of this offset is still under investigation.
CORRECTIONS TO RAW TOGA DATA
| Parameter | Error | Correction |
| Doppler velocity | Signs reversed(+/-) | Signs reset to standard |
| Ship motion not accounted for in raw doppler velocities | Corrected using information stored in ray of data |
| Radar reflectivity | Known engineering offset: bandpass filter mismatch caused 5.5dB
deficit in returned power | Applied +5.5dB to each
reflectivity value |
| Unknown source offset: CPOL and gauge comparisons indicate remaining 8.0dB reflectivity deficit | Applied +8.0dB to each reflectivity value |
B. CPOL Radar
CPOL had very few documented problems during SCSMEX. It operated almost
continuously from 4 May 1998 to 25 June 1998. The only major problem occurred
with the elevation servo on the antenna. It was not operating between 27 May
1998 and 8 June 1998. During this time, CPOL could only operate in
surveillance mode (lowest scan only.) The following is a brief description of
the corrections, which was provided by Tom Keenan.
Doppler Velocity
The sign was flipped just like TOGA. This problem was discovered and
corrected in the software on May 17. The correction had been applied to the
data before this time. Also, it was discovered that Transmit/Receive (T/R)
switch failed on 16 May. This affected the data out to 10 KM. After 16 May,
the problem was corrected.
Radar Reflectivity
No corrections made.
Polarimetric Variables The only correction that was applied
to the QC dataset was for the T/R problem discovered on 16 May. It also
affected the ADR field out to a range of 10 KM.
CORRECTIONS TO RAW CPOL DATA
| Parameter | Error | Correction |
| Doppler velocity | Signs reversed(+/-) | Signs reset to standard |
| Radar reflectivity | No corrections |
| Polarimetric values | Transmit/receive switch failure affecting data out to 10km before May 16 |
The QC radar dataset have been converted to the standard radar universal format (UF) and compressed using the standard UNIX gzip utility.
Naming Convention
For both radars, data is stored in daily directories. For example, the directory 980515/ contains all the data for 15 May 1998.
A. TOGA radar
- Volume scans
Volume scan data have the following naming convention:
SITE_scantype_YYMMDD_HHMN.uf.gz
where:
SITE: TOGA for TOGA radar
scantype: vol for volume scan
YY: Year
DD: Day
HH: Hour (UTC)
MN: Minute (start of the scan)
uf: Universal Format file
gz: gzipped
For example, TOGA_vol_980515_0400.uf.gz
is a TOGA volume scan that was recorded on 15 May 1998 at 04:00 UTC and is stored as a compressed UF file.
- Surveillance Scans
Surveillance scan data have the same naming convention as volume scans
except the scantype identifier is sur instead of vol
where
YY = year (1999)
MM = month
DD = day of month
HH = UTC hour
mm = minutes after the hour
B. CPOL radar
- Volume and Surveillance Scans
- Both volume and surveillance scans have the same naming convention. The QC
UF files from the CPOL radar were generated by a QC program provided by Dr. Tom
Keenan. This program was applied to the raw CPOL files and no attempt was made
to modify the code or outpur naming convention. The filenames have the
following format:
ufYYMMDD_HHMMSS.PPI.gz
where:
uf = Universal Format file
YY = year (1999)
MM = month
DD = day of month
HH = UTC hour
MN = minutes (start of scan)
SS = Second (start of scan)
PPI = PPI (Plan Position Indicator file (i.e. volume or surveillance as opposed to RHI (Range Height Indicator) file)
gz = gzipped
The TOGA and CPOL radar data may be ordered by email from the Hydrology Data Support Team,
NASA Goddard (see below).
The Principal Investigator for the SCSMEX radar data is
Jian-Jian Wang Mesoscale Processes, Code 912 NASA
Goddard Space Flight Center Greenbelt, Maryland 20771 jwang@radar.gsfc.nasa.gov
Co-Investigator for the CPOL radar data is
Tom Keenan
Bureau of Meteorology (BMRC)
PO Box 1289k,
Melbourne, Victoria 3001
Australia
T.Keenan@BoM.GOV.AU
Fax : +61-(0)3-9669-4660
For technical questions on the radar data contact:
Paul Kucera The University of Iowa Iowa City, IA
52242 pakucera@mail.iihr.uiowa.edu
For SCSMEX user services at the DISC contact
Hydrology Data Support Team (Goddard DISC), Code 610.2
NASA Goddard Space Flight Center
Greenbelt, Maryland 20771
hydrology-disc@listserv.gsfc.nasa.gov
(301) 614-5165 (voice)
(301) 614-5268 (fax)
Last update:Thu Aug 15 13:56:43 EDT 2002
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