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Overview of the TEFLUN A & B field campaigns
(based on the TEFLUN science objective document at NASA/ARC TEFLUN
Home Page)
Introduction
The TExas and FLorida UNderflights (TEFLUN) Experiment is a mission to
obtain validation measurements for the Tropical Rain Measuring Mission
(TRMM). TRMM is a NASA and National Space Development Agency of Japan
(NASDA) coordinated mission that launched the TRMM satellite
on 28 November 1997 with a unique complement of sensors to remotely
observe rainfall throughout the global tropics. TEFLUN is the first in
a series of experiments using a combination of airborne and surface-based
measurements to complement the satellite data. Among these, are important
measurements aboard the NASA high-altitude aircraft, similar to those on the
TRMM satellite. They are used for direct intercomparisons with TRMM
overflights where possible, but more frequently to simulate TRMM data by
flying over precipitation systems within the experimental domain. These,
along with in situ aircraft data, surface-based measurements and
computer models, will make unique contributions to our understanding of
the tropical precipitation spectrum.
Scientific Objectives
TRMM field campaigns (FCs) aim at validation of the ground validation
products derived from radars and rain gauges, TRMM-derived Levels 2 and 3
radiometer, rain and rain profile products, and vertical profiles of
latent heating. Since latent heating profiles cannot be directly measured,
numerical cloud models are used in TRMM algorithms to provide the link
between the latent heating profiles, TRMM radar and radiometer observations.
Consequently, an important part of the campaign is to provide comprehensive
observations of the structure and evolution of Mesoscale Convective Systems
(MCS), individual convective events, and their environment. Cloud and
mesoscale models require these data sets for initialization and the
subsequent model results must be validated for realism of vertical
structure and latent heating. While the TRMM instantaneous and monthly
algorithms can be evaluated through intercomparison with ground
validation (GV) and other data sets, the campaigns will provide additional
observations required for a more thorough validation and guidance for
improving the algorithms.
- The overarching scientific objective of TEFLUN is to obtain a database
suitable for case studies of a few MCSs, early in the TRMM lifetime, from
which cloud-resolving models and forward radiative transfer models can be
used to understand and improve the performance of the satellite and GV
algorithms.
- Perform underflights of TRMM by the ER-2 and DC-8 with high-resolution
radar and passive microwave instruments to assist in evaluating the effects of
resolution and sensitivity on algorithms using the Precipitation Radar (PR)
and TRMM Microwave Imager (TMI) data. (Since underflight opportunities
are limited, similar flight lines to simulate TRMM data should be performed
over precipitation targets more frequently.)
- Evaluate and improve algorithms using ground-based radar data [i.e., GV
algorithms] for estimating rain rates, vertical profiles of hydrometors, and
separation of convective and stratiform precipitation regions by using a
combination of augmented ground-based measurements and aircraft overflights.
- Provide guidance for improving the assumptions in algorithms using TRMM
satellite data as inputs to estimate rainfall and latent heating profiles,
particularly the ones which involve microphysics, i.e., vertical distribution of
hydrometeors.
TEFLUN-A will be conducted between April 1 and May 15, 1998, principally
focused on the Texas ground validation site. The NASA ER-2 aircraft
participation is planned for April 8 - May 8, 1998 based at Eglin AFB, FL.
A cloud physics aircraft based within or near the TX site will also participate.
There is close coordination with the Houston and other WSR-88Ds, the Texas
A&M ADRAD Doppler radar, the NOAA ETL X-band polarization radar (X-
POL), and the NOAA AL Profiler system. These ground-based facilities are
integrated with dense rain gauge networks and disdrometers. Soundings will be
obtained from two mobile systems to provide initialization and validation data
for models at strategic times and locations.
TEFLUN-B will be conducted between 1 August and 30 September 1998,
principally focused on the Florida ground validation site. ((DC-8 actually arrives
around the 10th)) It will be conducted in close coordination with the 3rd
Convection And Moisture Experiment (CAMEX-3), both involving NASA ER-2
and DC-8 aircraft, and a cloud physics aircraft, all based at Patrick AFB, FL. There is
close coordination with the Melbourne and other WSR-88Ds, the NCAR S-band
polarization radar (S-POL) radar, the array of facilities at the Kennedy Space
Center, and the NOAA AL Profiler system. Soundings will be obtained from
two mobile systems to provide initialization and validation data for models at
strategic times and locations. A dense network of ground-based facilities
measurements will also be utilized in TEFLUN-B.
NASA Aircraft
Instruments
The ER-2 and the DC-8 during TEFLUN-B,
will carry instruments associated with TRMM objectives. The instruments most
relevant to TRMM are a subset of the payloads carried by each aircraft.
Primary TRMM-related instruments on the ER-2
ER-2 Doppler Radar (EDOP) is a dual-beam 9.6 GHz Doppler radar that will
provide vertical profiles of reflectivity, vertical hydrometeor motions, horizontal
winds along the aircraft track, and polarization measurements which provide
microphysical information. This instrument will be used to examine vertical
precipitation structure and resolution limitations of the PR.
Advanced Microwave Precipitation Radiometer (AMPR), with frequencies similar to
TMI (10 - 85 GHz), will provide information on precipitation structure through
the rain emission and ice scattering signals.
Lightning Instrument Package (LIP) provides measurements of the three-
dimensional electric field and conductivity. This information will be related to
the LIS measurements on the TRMM satellite.
Multispectral Atmospheric Mapping Sounder (MAMS) provides high resolution
mapping with 11 channels visible, near-IR, and IR a 6.7 m moisture channel
similar to that flown on GOES.
Millimeter Imaging Radiometer (MIR) is a cross-scanning radiometer at frequencies
from 90 GHz to 325 GHz.
Primary TRMM-related instruments on the DC-8
Airborne Rain Mapping Radar (ARMAR) simulates the TRMM Precipitation Radar
(i.e., 14 GHz frequency and cross-track scanning). It provides information on the
three-dimensional structure of reflectivity and hydrometeor motions, as well as
polarization and Doppler measurements.
Polarimetric Scanning Radiometer (PSR) is a new conical scanning radiometer at the
TRMM Microwave Imager frequencies, and for the first time, provides a closer
simulation to the SSM/I and TMI conical scanning and polarization
measurements.
Airborne Multichannel Microwave Radiometer (AMMR) is a suite of fixed-beam
radiometers GHz that will be used to help understand microwave emission from
rain. It will have channels at 18 and 37 GHz (up-looking) and 37 GHz (nadir-
looking).
Cloud/Aerosol Particle Characterization (CAPAC) provides microphysical
information using Particle Measurement Systems 2D-C, 2D-P, and FSSP probes.
Dropsondes will be launched using the GPS system developed by National
Center for Atmospheric Research.
There are several additional instruments that will be flown on the DC-8 as part of
CAMEX-3. These instruments will provide valuable information for the TRMM
objectives.
More detailed descriptions of the full ER-2 and DC-8 instrument complements
TEFLUN-B/CAMEX-3 are given on the TEFLUN-A/B and CAMEX3 web sites:
TEFLUN-A/B: http://cloud1.arc.nasa.gov/teflun
CAMEX-3: http://www.ghrc.msfc.nasa.gov/camex3
TEFLUN-B Network
Surface-based facilities which will form part of the database for TeFLUN-B
incllude the Melbourne and other WSR-88Ds, the NCAR S-band polarization radar
(S-POL), the array of facilities at the Kennedy Space Center, and the NOAA AL
Profiler system. These ground-based facilities are integrated with dense rain
gauge networks and disdrometers. Soundings will be obtained from the two
mobile systems. The enhanced surface network for TEFLUN-B is shown
in the following figure:
In addition to the enhanced TEFLUN-B surface network near the S-POL radar,
the TRMM Florida GV network with the WSR-88D's will also be used as part of the
flight region for the aircraft. This network covers most of Florida.
A more detailed description of the TEFLUN-B GV network can be found at the TRMM
Office web site:
http://trmm.gsfc.nasa.gov/trmm_office/field_campaigns/teflun/teflunb/teflunb_gv.html
- NCAR S-Band polarimetric radar
Overview:
In 1996 the Natiional Center for Atmosphereic Research (NCAR) began a program
in radar hydrology and in particle discrimination. Hydrological goals are to
improve Z-R relationship technology for estimating precipitation and to evaluate
the potential of dual-polarization measurements for estimating precipitation.
Other programmatic goals seek to develop techniq;yes for the remote detection of
precipitation particle types (raindrops, snow crystals, graupel, and hail).
The corner stone of the program is NCAR's S-band, dual-polarization radar (S-POL).
Measureables include radar reflectivity, differential reflectivity, differential
propagation phase, the correlation coefficient between reflectivity an hoizontal
and vertical polarization, the linear depolarization ratio, and the radial
velocity. More details concerning the radar can be found at:
Http://www.atd.ucar.edu/rsf/spol/spol.html
Operations and Realtime
Products:
S-Pol will be located at longitude 80° 44.736 min and latitude 27° 53.360'
(200° and 26 km from the WSR-88D at Melbourne) and will operate from
approximately 20 July until 30 September 1998. Operations will be conducted
whenever precipitation is observed or forecast within the S-Pol umbrella. It is
expected that a large number of hydrologic events will be collected. In addition
S-Pol will support TRMM activities. A number of realtime products are available.
Precipitation estimates (maps) are generated from radar reflectivity, specific
differential phase, a combination of differential reflectivity and reflectivity,
and from a combination of all three polarimetric variables. Accumulation times
can be as short as ten minutes and as long as storm duration. There is a realtime
hail detection algorithm. A recent addition is a particle discrimination product
which will make designations in eleven categories.
Scanning Strategies:
For hydrological experiments S-Pol will be operated in full PPI or sector mode.
A number of experiments are planned:
- NEXRAD mode: For some experiments the radar will be operated at elevation
angles of 0.5, 1.45, 2.4 and 3.35°. This strategy permits duplication of
precipitation products with the WSR-88D.
- Continuous sammpling: In this mode the radar will operate continuously at a
constant low elevation angle ( most likely 0.5°). The purpose is to determine
the benefits of more frequent temporal sampling. The likely sampling interval
is 55 sec.
- Three-dimensional mode: The radar will operate in a fixed sector mode over a
concentrated network of gages. The measurements support neural network approaches
to rainfall estimation.
- Doubled sampling: Normally 60 samples are collected at each polarization.
For some experiments the radar will be operated in sector mode with double
the number of samples.
The radar can be operated in either sector or vertical cross-section modes.
Antenna speeds are 6.5°/sec in sector mode and 3-4°/sec in RHI mode.
Data collections are flexible in terms of sector and elevation limits.
Some examples with approximate scan durations are:
- 60° azimuthal sector with 20 elevation angles: 3 min 20 sec
- 120° azimuthal sector with 15 elevation angles: 5 min
- 180° azimuthal sector with 15 elevation angles: 7 min 20 sec.
An RHI scan for an azimuthal sector of 30°, with elevation angles from
0 to 40°, and an azimuthal increment of 1° will take 6 min 40 sec at
an antenna speed of 3°/sec and 5 min at 4°/sec. Full RHI's
(horizon-zenith-horizon) are not possible. A proxy can be accomplished by
stringing two RHI scans with elevation angles of 0 to 85° and a null sector
width. Such a scan will take approximately 1 min 15 sec to complete.
- NOAA/AL Doppler radar profilers
(see above)
- IIHR Mobile Rainfall Observatory
The Iowa Institute of Hydraulic Research (IIHR) of the University of Iowa,
operates the so-called Mobile Rainfall Observatory, which includes a trailer-based
vertically pointing X-band radar (owned jointly with the Hydrologic Research Center
of san Diego, California), a 2-D video disrrometer, dual-design tipping-bucket
raingages, and other surface meteorological instruments. The instrumentation is
described below. Pictures of the instrumentation appear on the web at:
http://www.iihr.uiowa.edu/trailer/
- Vertically Pointing Radar
The basic specifications of the vertically pointing radar are shown in Table 1.
The radar was built at the McGill Radar Weather Observatory, McGill University,
Canada. The microwave part of the radar is essentially a widely-used navigation
radar manufactured by Decca. It is controlled by a PC equipped with a PCIP-SCOPE
digital oscilloscope card, maunfactured by Keithly Metrab;yte, and software
written by the developers of the radar at McGill University. The radar data
acquisition software provides a rudimentary display program that is useful for
confirming operation of the radar. Additional C library routines that enable
reading, plotting, converting the data to a format that is easier to distribute,
and analyzing the data, has been developed at IIHR. Recently, the radar was
upgraded to Doppler capability using a PIRAC card developed at NCAR.
Table1. McGill X-band Vertically Pointing Radar
| Parameter | Value |
| Wavelength/Frequency | 3.2 cm (9410 MHz ± 30 MHz) |
| Peak power | 25 kW |
| Dish diameter | 1.2 m |
| Pulse length | 250 ns |
| Pulse repetition frequency | 1300 Hz |
| Pulses averaged | 1200 |
| Minimum height | 100 m |
| Maximum height | 8000 m |
| Bin size | 15 m |
- 2-D Video Disdrometer
IIHR's video disdrometer is one of only a handfull of such instruments worldwide.
It was specially manufactured for IIHR by Johanneum Research at The Institute for
Applied Systems Technology, Inffeldgrasse, Austria. Two light sources generate
orthogonal light sheets that are projected through narrow slits onto two line
scan cameras. The optics are designed so that, seen through the camera lens,
the slits appear evenly and brightly lit. Particles falling through the beams
of light appear as dark silhouettes against this background. The light sources
and cameras form the sensor unit that is exposed to the precipitation.
The electronics and embedded computer that control the cameras and record the
slit images are housed in a separate, weatherproof outdoor electronics unit.
A second, indoor, PC communicates with this embedded computer via TCP/IP
protocols. After copying the raw image information from the outdoor unit, the
software running on the indoor PC reconstructs the shapes of the hydrometeros.
The software also estimates the falling velocity, horizontal velocity, oblateness,
and equivalent water content, for each individual hydrometeor. In addition to
this information, aggregate information such as drop size distribution, rainrate
versus time, vertical velocity versus time, oblateness versus diameter, etc. are
computed and displayed in real-time. IIHR's disdrometer has been in operation
since the middle of summer 1997, and we have collected data and written software
to facilitate off-line analysis.
- Mobile Platform
The instruments described above (i.e. vertically pointing radar, raingauges, and
2-D video disdrometer) are carried around on a 16 ft. trailer, called IIHR
Mobile Rainfall Observatory. The trailer permanently houses the vertically
pointing radar and accommodates the on-site data collection by the 2-D video
disdrometer. For the raingauges, it merely serves as a hauling platform, but it
houses the data acquisition and power distribution system too. We do not
recommend, due to safety reasons, operating the radar while the trailer is in
motion.
The trailer is outfitted with a dual voltage electric wiring (12V DC and 120V AC).
This way an external power supply can be provided by a cable from a permanent
facility, or from a diesel powered generator or a set of batteries. On-site computer
data acquisition system allows long term operation and storage of large volume of
data. The radar antenna is covered with a fiberglass dome, which mitigates the
effect of attenuation by the layer of water collected on the cover during rainfall.
- Rain gauge networks
There will be approximately 30 rain gauges deployed in two separate clusters.
Approximately 10 rain gauges will be installed at existing field mill sites
within Kennedy Space Center (KSC). These rain gauges will enhance the
existing network at KSC. Because the average gauge spacing is ~5km, the
information provided by the KSC rain gauge network will help determine the
mesoscale variabilith of rainfall across Cape Canaveral and provide ground
truth for scanning radar. Indeed, the KSC rain gauge network is currently
used to calibrate radar reflectivity (Z) - rainfall (R) estimates of rainfall
for TRMM from the Melbourne NEXRAD.
The spacing of the KSC gauges is too course to provide detailed statistics of
rainfall at the convective scale in TEFLUN-B. Also, it was recognized that there
exists a signigicant amount of restricted airspace in the vicinity of KSC,
thus hampering the ability of aircraft to sample convection in this area.
Because an important component of TRMM TEFLUN B is to provide
combined aircraft and ground-based sampling of Florida convection, an
additional site was selected for the placement of a dense rain gauge network
(DRGN). A tentative site for the DRGN was chosen near the town of
Hollopaw, Fl. These gauges will be used to examine variability of raingall at
0.5-2.0 km scales and should provide information on the range-dependency of
scanning radar Z-R estimates of rainfall (as well as Z_DR-R, K_DP-R and
other polarimetric relations). Moreover, profiler-pair will be able to provide
vertical structure information on the precipitation characteristics (including
drop size distributions) that can serve as calibration for the scanning radars.
The combination of the DRGN, profiler and scanning radars will provide a
unique picture of the vertical and horizontal variability during the TEFLUN
B campaign.
- Rain Gauges & Disdrometers
The rain gauges are tipping bucket type (Qualimetric). A number of disdrometers will also be deployed as part of the TEFLUN B
ground validation program. Three types of disdrometers will be used: 2-D
video, Joss, and APL. The 2-D and Joss will be deployed at the profiler
site in conjunction with an APL and a tipping bucket rain gauge. The
purpose of having all 3 disdrometer types at the profiler types will be to not
only compare the surface based measurements of drop size distribution
characteristics with the vertical structure (profiler), but also to compare
the surface measurements collected by each disdrometer to address the strengths
and weaknesses of each unit (address low end sensitivity of the APL
disrometer).
Approximately 5-10 additional APL disdrometers will be used in TEFLUN B.
These disdrometers represent a new technology in disdrometer design. They
are capable of storing several weeks of data at a time and will be stand-alone
units. However, it should be noted that these systems are relatively new
(being only deployed in TEFLUN A) and their reliability is not known. Also,
as it currently stands, the low-end sensitivity of the APL disdrometer is
approximately 1 mm and may therefore bias the retrieved DSD characteristics.
Cloud Microphysics
Aircraft
The UND Cessna Citation II aircraft has a number of design
and performance characteristics which make it a versatile and comparatively
low cost platform for a wide range of atmospheric studies. The Citation II is
a twin engine fanjet with an operating ceiling of 43,000 feet (12.1 km).
The turbofan engines provide sufficient power to cruise at speeds of up to
340 knots (175 m/s) or climb at 3300 feet/min (16.8 m/s). The fanjet
engines have relatively low fuel consumption at all altitudes, giving the
Citation an on-station time of up to 4 hours or more, depending on mission
type. Long wings allow it to be operated out of relatively short airstrips and
to be flown at ths slower speeds (140 kts or 72 m/s) necessary for many types
of measurements. The Citation is certified for flight into known icing conditions.
The cabin measures approximately five feet in diameter and more than 16 feet
in length. The minimum flight crew is pilot, co-pilot and data system
operator. Two additional seats are avbailable for scientific observers.
A series of structural modifications have been made to the basic airplane
including the following:
- pylons under the wing tips for a variety of probes in the undisturbed
air flow away from the fuselage;
- a heated Radome with a five hole system for wind measurement;
- side-facing camera mounts for time lapse cameras;
- optically flat glass windows for photography;
- and an air inlet port for air sampling inside the pressurized cabin.
More details about the UND Citation can be found at
the University of North Dakota aerospace research site.
Instrumentation:
The basic instrumentation package measures temperature, dew point temperature,
pressure, wind and cloud microphysical characteristics along with
aircraft position, attitude and performance parameters. The three dimensional
wind field is derived from measurements of acceleration, pitch,
roll and yaw combined with angles of attack and sideslip and indicated
airspeed. An LTN-76 inertial navigation system and a global positioning
system (GPS) supply the aircraft parameters. Turbulence intensity can be
derived from differential pressure transducers and accelerometer outputs.
Cloud microphysical measurements are made with an array of Particle
Measuring Systems probes (FSSP, 1D-C, 2D-C, 1D-P) mounted on the wing tip pylons.
These probes measure concentrations and sizes of particles from one µ
to several millimeters in diameter. In addition, there are probes to
measure both liquid water content (CSIRO) and icing rate (Rosemount icing meter).
For TRMM two new instruments will be available, a Cloud Particle Imager (CPI)
and a High Volume Particle Sampler (HVPS), both from SPEC, Inc. These will
provide improved resolution above that which is achieved from the PMS probes.
The CPI will provide microscopic quality images of small ice particles. The
HVPS will replace the 1D-C probe and it will provide improved sample volumn
for detection and imaging of large particles. A PMS 2D-P probe may also be
used for periods when the HVPS is not available.
A forward or side-looking video camera is also used to provide a vbisual
record of flight conditions and for recording of cockpit conversation.
A Bendix-King vertical profiling forward looking weather radar can be viewed
in the conkpit and recorded on videotape.
Data Acquisition and Display:
The data collected by the Citaiton can be sampled at various rates from
1 to 25 Hz. The sampling is controlled by the on-board computer system,
which also displays the data in real time in graphic and alphanumeric
formats while recording them on magnetic tape. The data system is based on
a projetc-customized windows system to allow flexibility in data acquisition
and instrumentation in order to accommodate specific research demands. The
data system and power distribution systems were upgraded during 1996, which
produced a substantial improvement in flexibility. also, an improved
version of the data system was leased and adapted to fit the instruments.
This provided a significant gain in weight and power availability.
When in the field, the Citation is accompained by a mobile operations
support trailer. This vehicle houses thchnical support facilities, including
calibration equipment for on-site quality control, and a workstation/
minicomputer system. The meteorological data collected on a research
flight can thus be processed and examined within 24 hours.
Data Availability & Summary:
TEFLUN Data Category
TEFLUN Priority Days
Data Availability Schedule
Tables of Flight Logs & Measurements
Coincidences of Ground, Aircraft & Satellite
Measurements
TEFLUN-B/CAMEX-3 Flight Scenarios
Data Access:
TEFLUN data resides on DISC
anonymous FTP. You may access the files from this document,
TEFLUN Data
or directly via FTP at
ftp disc2.nascom.nasa.gov
login: anonymous
password: < your internet address >
cd data/TEFLUNB/
Last update:Tue Jan 6 08:21:27 EST 2004 >
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