H. Harder et al., STRATOSPHERIC BRO PROFILES MEASURED AT DIFFERENT LATITUDES AND SEASONS - ATMOSPHERIC OBSERVATIONS, Geophysical research letters, 25(20), 1998, pp. 3843-3846
Stratospheric BrO profiles were measured at different latitudes and in
different seasons in 1996/97 during three flights of the LPMA/DOAS ba
lloon gondola (LPMA/Laboratoire Physique Moleculaire et Application an
d DOAS/Differential Optical Absorption Spectrometry). Using direct sun
light DOAS spectrometry the following BrO mixing ratios were measured;
(1) 9 to 14 ppt in the height range from 20 to 30 km (at solar zenith
angles, SZA < 88 degrees) during;ascent, (2) about (14+/- 2) ppt for
altitudes above the balloon float altitude at 30.6 km, 30.0 km, and 39
.8 km, and (3) 5 to 10 ppt in the 20-30 km region during sunset. The l
ower BrO concentrations during sunset than those observed prior at day
time indicate a conversion of BrO into nighttime reservoir species (Br
ONO2, HOBr, and BrCl). The overall agreement of our UV spectroscopic B
rO profiles with recent measurements using the chemical conversion/res
onance fluorescence technique is good. Our BrO profiles are also in re
asonable agreement with the present stratospheric Br-y burden and chem
istry. Conversily collocated ground-based and satellite column measure
ments, however show significantly more total atmospheric BrO (50 - 100
%) than the integrated stratospheric BrO balloon profiles can account
for. This indicates a global tropospheric BrO background, estimated at
1-2 ppt.