HR: 1340h
AN: SF43A-0783 [Abstracts]
TI: Laser Sounder for Global Measurement of CO2 Concentrations in the Lower Troposphere from Space:
Progress
AU: * Abshire, J B
EM: james.abshire@gsfc.nasa.gov
AF: NASA Goddard Space Flight Center, Laboratory for Terrestrial Physics
Mail Code 920, Greenbelt, MD 20771
United States
AU: Krainak, M A
AF: NASA Goddard Space Flight Center, Laboratory for Terrestrial Physics
Mail Code 920, Greenbelt, MD 20771
United States
AU: Riris, H
AF: NASA Goddard Space Flight Center, Laboratory for Terrestrial Physics
Mail Code 920, Greenbelt, MD 20771
United States
AU: Sun, X
AF: NASA Goddard Space Flight Center, Laboratory for Terrestrial Physics
Mail Code 920, Greenbelt, MD 20771
United States
AU: Burris, J
AF: NASA Goddard Space Flight Center, Laboratory for Terrestrial Physics
Mail Code 920, Greenbelt, MD 20771
United States
AU: Gates, A
AF: NASA Goddard Space Flight Center, Laboratory for Terrestrial Physics
Mail Code 920, Greenbelt, MD 20771
United States
AU: Collatz, J
AF: NASA Goddard Space Flight Center, Laboratory for Terrestrial Physics
Mail Code 920, Greenbelt, MD 20771
United States
AB:
We describe progress toward developing a laser-based technique for the remote measurement of the tropospheric CO2
concentrations from orbit. Our goal is to demonstrate a lidar technique and instrument technology that will permit
measurements of the CO2 column abundance in the lower troposphere from aircraft at the few ppm level, with a capability of
scaling to permit global CO2 measurements from orbit.
Accurate measurements of the tropospheric CO2 mixing ratio from space are challenging due to the many potential error
sources. These including possible interference from other trace gas species, the effects of temperature, clouds, aerosols &
turbulence in the path, changes in surface reflectivity, and variability in dry air density caused by changes in atmospheric
pressure, water vapor and topographic height. Some potential instrumental errors include frequency drifts in the transmitter,
small transmission and sensitivity drifts in the instrument. High signal-to-noise ratios and measurement stability are
needed for mixing ratio estimates at the few ppm level.
We have been developing a laser sounder approach as a candidate for a future space mission. It utilizes multiple different
laser transmitters to permit simultaneous measurement of CO2 and O2 extinction, and aerosol backscatter in the same
measurement path. It directs the narrow co-aligned laser beams from the instrument's fiber lasers toward nadir, and measures
the energy of the strong laser echoes reflected from the Earth's land and water surfaces. During the measurement its narrow
linewidth lasers are rapidly tuned on- and off- selected CO2 line near 1572 nm and an O2 absorption line near 770 nm. The
receiver measures the energies of the laser echoes from the surface and any clouds and aerosols in the path with photon
counting detectors. Ratioing the on- to off-line echo pulse energies for each gas permits the column extinction and column
densities of CO2 and O2 to be estimated simultaneously via the differential absorption lidar technique.
For the on-line wavelengths, the side of the selected absorption lines are used, which due to pressure broadening, weights
the measurements to the lower troposphere, where CO2 variations caused by surface sources and sinks are largest. Simultaneous
measurements of O2 column abundance are made using an identical approach using an O2 line. The laser backscatter profiles
from clouds and aerosols are measured with other lidar channels, which permits identifying measurements influenced by clouds
and/or aerosol scattering in the path.
For space use, our lidar would continuously measure at nadir in near polar circular orbit. Using dawn and dusk measurements
made over the same region will make it possible to sample the diurnal variations in CO2 mixing ratios. A 1-m diameter
telescope is used for the receiver for all wavelengths. When averaging over 50 seconds, our calculations show a SNR of ~1500
is achievable for each gas at each on- and off-line measurement. Measurements from such a mission can be used to generate
monthly global maps of the lower tropospheric CO2 column abundance.
We have demonstrated some key elements of the laser, detector and receiver approaches in the laboratory and with measurements
over a 206 m horizontal path. These including stable measurements of CO2 line shapes in an absorption cell using a fiber
laser amplifier seeded by a tunable diode laser, measurement of small amplitude changes at low optical signal levels with the
PMT receiver, and comparison of the horizontal path measurements of CO2 against those from an in-situ instrument.
DE: 1694 Instruments and techniques
DE: 0368 Troposphere--constituent transport and chemistry
DE: 0394 Instruments and techniques
DE: 0933 Remote sensing
SC: Special Focus: Advances in Data Acquisition, Management, Analysis and Display [SF]
MN: 2004 AGU Fall Meeting