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Scientific and Technical Aerospace Reports Volume 39 April 6, 2001

Scientific and Technical Aerospace Reports Volume 39 April 6, 2001

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Atmospheric radiation in the infrared (IR) 8-13 microns spectral region contains a wealth of information that is very useful<br />

for the retrieval of ice cloud properties from aircraft or space-borne measurements. to provide the scattering <strong>and</strong> absorption properties<br />

of nonspherical ice crystals that are fundamental to the IR retrieval implementation, we use the finite-difference time domain<br />

(FDTD) method to solve for the extinction efficiency, single-scattering albedo, <strong>and</strong> the asymmetry parameter of the phase function<br />

for ice crystals smaller than 40 microns. For particles larger than this size, the improved geometric optics method (IGOM) can<br />

be employed to calculate the asymmetry parameter with an acceptable accuracy, provided that we properly account for the inhomogeneity<br />

of the refracted wave due to strong absorption inside the ice particle. A combination of the results computed from the<br />

two methods provides the asymmetry parameter for the entire practical range of particle sizes between 1 micron <strong>and</strong> 10000<br />

microns over wavelengths ranging from 8 microns to 13 microns. For the extinction <strong>and</strong> absorption efficiency calculations, several<br />

methods including the IGOM, Mie solution for equivalent spheres (MSFES), <strong>and</strong> the anomalous diffraction theory (ADT) can<br />

lead to a substantial discontinuity in comparison with the FDTD solutions for particle sizes on the order of 40 microns. to overcome<br />

this difficulty, we have developed a novel approach called the stretched scattering potential method (SSPM). For the IR 8-13<br />

microns spectral region, we show that SSPM is a more accurate approximation than ADT, MSFES, <strong>and</strong> IGOM. The SSPM solution<br />

can be further refined numerically. Through a combination of the FDTD <strong>and</strong> SSPM, we have computed the extinction <strong>and</strong> absorption<br />

efficiency for hexagonal ice crystals with sizes ranging from 1 to 10000 microns at 12 wavelengths between 8 <strong>and</strong> 13 microns<br />

Calculations of the cirrus bulk scattering <strong>and</strong> absorption properties are performed for 30 size distributions obtained from various<br />

field campaigns for midlatitude <strong>and</strong> tropical cirrus cloud systems. Parameterization of these bulk scattering properties is carried<br />

out by using second-order polynomial functions for the extinction efficiency <strong>and</strong> the single-scattering albedo <strong>and</strong> the power law<br />

expression for the asymmetry parameter. We note that the volume-normalized extinction coefficient can be separated into two<br />

parts: one is inversely proportional to effective size <strong>and</strong> is independent of wavelength, <strong>and</strong> the other is the wavelength-dependent<br />

effective extinction efficiency. Unlike conventional parameterization efforts, the present parameterization scheme is more accurate<br />

because only the latter part of the volume-normalized extinction coefficient is approximated in terms of an analytical expression.<br />

After averaging over size distribution, the single-scattering albedo is shown to decrease with an increase in effective size<br />

for wavelengths shorter than 10.0 microns whereas the opposite behavior is observed for longer wavelengths. The variation of<br />

the asymmetry parameter as a function of effective size is substantial when the effective size is smaller than 50 microns. For effective<br />

sizes larger than 100 microns, the asymmetry parameter approaches its asymptotic value. The results derived in this study<br />

can be useful to remote sensing applications involving IR window b<strong>and</strong>s under cirrus cloud conditions.<br />

Author<br />

Atmospheric Radiation; Cloud Physics; Cirrus Clouds; Infrared Radiation; Infrared Windows; Remote Sensing<br />

<strong>2001</strong>0025275 NASA Goddard Space Flight Center, Greenbelt, MD USA<br />

Tropospheric Ozone <strong>and</strong> Biomass Burning<br />

Ch<strong>and</strong>ra, Sushil, NASA Goddard Space Flight Center, USA; Ziemke, J. R., NASA Goddard Space Flight Center, USA; Bhartia,<br />

P. K., NASA Goddard Space Flight Center, USA; [<strong>2001</strong>]; 22p; In English; No Copyright; Avail: CASI; A03, Hardcopy; A01,<br />

Microfiche<br />

This paper studies the significance of pyrogenic (e.g., biomass burning) emissions in the production of tropospheric ozone<br />

in the tropics associated with the forest <strong>and</strong> savanna fires in the African, South American, <strong>and</strong> Indonesian regions. Using aerosol<br />

index (Al) <strong>and</strong> tropospheric column ozone (TCO) time series from 1979 to 2000 derived from the Nimbus-7 <strong>and</strong> Earth Probe<br />

TOMS measurements, our study shows significant differences in the seasonal <strong>and</strong> spatial characteristics of pyrogenic emissions<br />

north <strong>and</strong> south of the equator in the African region <strong>and</strong> Brazil in South America. In general, they are not related to the seasonal<br />

<strong>and</strong> spatial characteristics of tropospheric ozone in these regions. In the Indonesian region, the most significant increase in TCO<br />

occurred during September <strong>and</strong> October 1997, following large-scale forest <strong>and</strong> savanna fires associated with the El Nino-induced<br />

dry season. However, the increase in TCO extended over most of the western Pacific well outside the burning region <strong>and</strong> was<br />

accompanied by a decrease in the eastern Pacific resembling a west-to-east dipole about the date-line. The net increase in TCO<br />

integrated over the tropical region between 15 deg N <strong>and</strong> 15 deg S was about 6-8 Tg (1 Tg = 10(exp 12) gm) over the mean climatological<br />

value of about 72 Tg. This increase is well within the range of interannual variability of TCO in the tropical region <strong>and</strong><br />

does not necessarily suggest a photochemical source related to biomass burning. The interannual variability in TCO appears to<br />

be out of phase with the interannual variability of stratospheric column ozone (SCO). These variabilities seem to be manifestations<br />

of solar cycle <strong>and</strong> quasibiennial oscillations.<br />

Author<br />

Biomass Burning; Emission; Troposphere; Photochemical Reactions; Ozone; Combustion<br />

205

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