Global Tropospheric Wind Sounder (GTWS): A Strategy for Obtaining Operational Wind Profiles from Space
Farzin Amzajerdian (NASA/LaRC)
Robert Atlas (NASA/GSFC)
Wayman Baker (NOAA/NWS)
James Barnes (NASA/LaRC)
David Emmitt (Simpson Weather Associates)
Bruce Gentry (NASA/GSFC)
Ingrid Guch (NOAA/NESDIS)
Michael Hardesty (NOAA/OAR)
Michael Kavaya (NASA/LaRC)
Stephen Mango (NPOESS/IPO)
Kenneth Miller (Mitretek Systems)
Stephen Neeck (NASA/HQ)
John Pereira (NOAA/NESDIS)
Frank Peri (NASA/LaRC)
Upendra Singh (NASA HQ)
Gary Spiers (NASA/JPL)
James G. Yoe (NOAA/NESDIS)
June 10, 2003
3.
Hybrid Doppler Wind Lidar (Emmitt)
3.1 Notional Hybrid DWL Concept
Table
3.3-1. General mission parameters for IPO Hybrid feasibility study
Parameter
|
IPO Study Missions |
|
Orbit Height |
400 km |
|
Orbit Inclination |
98 degrees |
|
Nadir viewing angle |
45 degrees |
|
Duty cycle |
100% |
Table
3.3-2. IPO Coherent Detection Subsystem Parameters
Instrument Parameters |
IPO
Baseline
|
IPO Hybrid |
|
Wavelength
(nm) |
2054 |
Same |
|
Pulse
Energy (Joules) |
8 |
0.5 |
|
Pulse
Duration (sec) |
1.80.0E-09 |
Same |
|
Pulse
Repetition Frequency (prf) (Hz) |
12 |
Same |
|
Laser
Wallplug Efficiency (factor) |
0.02 |
Same |
|
Shot
Integration (Number) |
60 |
Same |
|
Azimuths
in Sample Sequence (number of scan positions) |
8 |
Same |
|
Energy
per LOS Data Product (Joules) |
480 |
30 |
|
Average
Laser Power ( |
4800 |
300 |
|
Telescope
Area (m2) |
0.45 |
0.2 |
|
Optical
Transmission 2-way (factor) |
0.50 |
Same |
|
Detector
Quantum Efficiency (factor) |
0.80 |
Same |
|
Mixing
Efficiency (factor) |
0.40 |
Same |
|
Data
Rate (bits/hour) |
26.2E+09 |
Same |
|
Mass
of Instrument (kg) |
? |
? |
|
Total
Instrument (including scanner) Average
Power (watts) |
5251 |
600 |
Table
3.3-3 contains the system parameters for the IPO Baseline and Hybrid Direct
Detection Subsystem alternatives compared to the baseline from the GSFC Direct
Detection Reference Design. The important differences are found in greatly
reduced pulse energy, pulse repetition frequency (prf), telescope area and mass,
and total average power for the instrument. All of these improvements address
key technology concerns in the Direct DWL Reference Design. Two alternative
hybrid configurations are considered for the direct detection hybrid sub-system,
IPO1 and IPO2. IPO2 used a lower prf and 4 azimuths per LOS Data Product instead
of 8 (e.g., 2 cross track bi-perspective observation lines instead of 4, which
equates to some reduction in horizontal resolution across track relative to the
stated requirements). IPO1 represents a system that meets the GTWS requirements
with no negotiation. It must be noted that the system efficiencies used for the
direct detection trade study were those that have been demonstrated in field
lidars times a factor of two. For direct detection, in particular, improvements
in system photon efficiencies of at least a factor of two are expected using
techniques such as photon recycling.
Table
3.3-3. IPO
Baseline and Hybrid Direct Detection Subsystem Parameters
Instrument Parameters |
IPO
Baseline |
IPO1
Hybrid |
IPO2
Hybrid |
|
Wavelength
(nm) |
355 |
Same |
Same |
|
Pulse
Energy (Joules) |
1 |
0.2 |
0.2 |
|
Pulse
Duration (sec) |
20E-09 |
Same |
Same |
|
PRF
(Hz) |
125 |
60 |
30 |
|
Laser
Wallplug Efficiency (factor) |
0.016 |
Same |
Same |
|
Shot
Integration (Number) |
633 |
300 |
600 |
|
Azimuths
in Sample Sequence (number of scan positions) |
8 |
8 |
4 |
|
Energy
per LOS Data Product (Joules) |
635 |
60 |
60 |
|
Average
Laser Power ( |
7812 |
750 |
375 |
|
Telescope
Area (m2) |
1.23 |
0.78 |
0.5 |
|
Optical
Transmission 2-way (factor) |
0.034 |
Same |
Same |
|
Detector
Quantum Efficiency (factor) |
0.80 |
Same |
Same |
|
Data
Rate (bits/hour) |
0.88E+09 |
0.44E+09 |
0.44E+09 |
|
Mass
of Instrument (kg) |
? |
? |
? |
|
Total
Average Power of Instrument (including scanner (watts) |
8112 |
1050 |
675 |
|
Size
(m) |
3 x 1.5 x 1.5 |
|
|
Instrument ParametersCombined IPO Hybrid
|
IPO1
H(DD,CD)* |
IPO2
H(DD,CD) |
|
Average
Laser Power ( |
750+300=1050 |
375+300=675 |
|
Effective
Telescope Area (m2) |
0.78
0.2 |
0.5
0.2 |
|
Data
Rate (bits/hour) |
26 E09 |
26 E09 |
|
Mass
of Instrument (kg) |
TBD |
TBD |
|
Total
Average Instrument Power ( |
1050+600=1650 |
675+600=1275 |
* DD is Direct Detection, CD is Coherent Detection
3.4
Simulated Data Products for IPO Study Concepts

Figure
3.4-1 is a performance (or data) profile for the IPO coherent detection baseline
system described in Column 2 of Table 3.3-2. In this case, and in all cases
shown here, the T213 Nature Run provided by the
In
Figure 3.4-1, the background mode of aerosols is used for the design atmosphere
for a stand-alone coherent DWL. The gray areas represent no data, due primarily
to cloud obscuration and the very cleanest tail on the background mode
distribution. The hatched areas denote useful returns from the tops of dense
clouds and within thin cirrus clouds. The error shown here is the LOS
measurement error projected on to the horizontal plane (HLOS). The color of the
error is directly related to the SNR and modeled atmospheric variance as used in
an algorithm (provided in part by Rod Frehlich, CIRES,

Figure 3.4-2 Performance
profile for IPO direct detection (double edge) baseline, molecular backscatter
only
Figure 3.4-2 is the
performance profile for the IPO direct detection baseline system (molecular
backscatter only). A double-edge detector is used in this case. Adding an
aerosol detector that would meet data requirements in the lower troposphere
would increase the power demands. Note that 125 watts at .355 microns would
require 300-400 watts at the fundamental of 1.06 microns. In this case, the
direct detection system is being sized to get as much of the power as is
“reasonable” for the technology. Alternative direct detection approaches
remain to be studied.
Figure 3.4-3 is the
performance profile for a hybrid system and the background mode of aerosols.
In this case we have a 6 watt (optical) / .5 meter aerosol coherent
subsystem combined with a 36 watt (at .1.06 micron) / 1.0 meter molecular direct
detection subsystem. It is clear that the hybrid not only meets the threshold
requirements but exceeds them in accuracy where the coherent system has the
sensitivity.

Figure 3.4-3 Performance
profile for hybrid system using background aerosol backscatter
Figure 3.4-4 is for the same instrument configuration as that in Figure 3.4-3 except the enhanced backscatter mode is used. In this case, the objective data accuracies are met with the coherent DWL over nearly 70% of the troposphere below 12km. The direct detection fills in most of the remaining volume with threshold accuracies. Together, the two systems meet the science data requirements (with margin) while reducing the power, weight and size (all cost determinants) from that of either stand-alone concept.
Figure
3.4-4
Performance profile for hybrid system using enhanced aerosol backscatter