G. Echle et al., OPTICAL AND MICROPHYSICAL PARAMETERS OF THE MT. PINATUBO AEROSOL AS DETERMINED FROM MIPAS-B MID-IR LIMB EMISSION-SPECTRA, J GEO RES-A, 103(D15), 1998, pp. 19193-19211
High-resolution mid-IR limb emission spectra were recorded during a fl
ight of the Michelson interferometer for passive atmospheric sounding,
balloon-borne version (MIPAS-B) from Kiruna, northern Sweden (68 degr
ees N) on March 14/15, 1992. These spectra are affected by the Mt. Pin
atubo stratospheric aerosol, which caused an enhanced continuum emissi
on, especially in spectra of low tangent altitudes. Aerosol extinction
coefficients were retrieved from MIPAS-B spectra at approximately 60
spectral positions in the 750-980 cm(-1) and 1180-1380 cm(-1) spectral
ranges. Retrieved aerosol extinction coefficients range from 6x10(-4)
km(-1) to 3x10(-3) km(-1) in tangent altitudes 11.3 km and 14.5 km an
d from 5x10(-5) km(-1) to 1x10(-3) km(-1) in 16.1 km. Their distinct s
pectral shape indicates the presence of H2SO4-H2O droplets. Compositio
ns and size distribution parameters were retrieved by least squares fi
tting of Mie-generated spectral extinction coefficients to the ones de
rived from the spectra. Estimated spectral, single-scattering albedos
between 0.08 and 0.3 indicate the significance of thermal multiple sca
ttering. Multiple-scattering corrections led to an increase of spectra
l extinction coefficients by 5-50% with highest changes at lowest tang
ent altitudes. Accordingly, estimated volume densities have increased
by 4-20% to values of 3.66, 2.85, and 0.93 mu m(3) cm(-3) for tangent
altitudes 11.3, 14.5, and 16.1 km, respectively. Retrieved H2SO4 weigh
ts of 66-70% are in good agreement with values derived from stratosphe
ric temperatures and water vapor partial pressures. Estimated surface
densities are systematically low in comparison with in situ size distr
ibution measurements. This finding is explained by the underestimation
of small particles by the use of a monomodal size distribution in the
analysis. Retrieved effective radii of up to 0.8 mu m were found to b
e consistent with the temporal evolution of the Mt. Pinatubo aerosol.