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@ARTICLE{Cirisan:154628,
author = {Cirisan, A. and Luo, B. P. and Engel, I. and Wienhold, F.
G. and Sprenger, M. and Krieger, U. K. and Weers, U. and
Romanens, G. and Levrat, G. and Jeannet, P. and Ruffieux, D.
and Philipona, R. and Calpini, B. and Spichtinger, P. and
Peter, T.},
title = {{B}alloon-borne match measurements of midlatitude cirrus
clouds},
journal = {Atmospheric chemistry and physics},
volume = {14},
number = {14},
issn = {1680-7324},
address = {Katlenburg-Lindau},
publisher = {EGU},
reportid = {FZJ-2014-03918},
pages = {7341 - 7365},
year = {2014},
abstract = {Observations of high supersaturations with respect to ice
inside cirrus clouds with high ice water content (> 0.01 g
kg−1) and high crystal number densities (> 1 cm−3) are
challenging our understanding of cloud microphysics and of
climate feedback processes in the upper troposphere.
However, single measurements of a cloudy air mass provide
only a snapshot from which the persistence of ice
supersaturation cannot be judged. We introduce here the
"cirrus match technique" to obtain information about the
evolution of clouds and their saturation ratio. The aim of
these coordinated balloon soundings is to analyze the same
air mass twice. To this end the standard radiosonde
equipment is complemented by a frost point hygrometer,
"SnowWhite", and a particle backscatter detector, "COBALD"
(Compact Optical Backscatter AerosoL Detector). Extensive
trajectory calculations based on regional weather model
COSMO (Consortium for Small-Scale Modeling) forecasts are
performed for flight planning, and COSMO analyses are used
as a basis for comprehensive microphysical box modeling
(with grid scale of 2 and 7 km, respectively). Here we
present the results of matching a cirrus cloud to within
2–15 km, realized on 8 June 2010 over Payerne,
Switzerland, and a location 120 km downstream close to
Zurich. A thick cirrus cloud was detected over both
measurement sites. We show that in order to quantitatively
reproduce the measured particle backscatter ratios, the
small-scale temperature fluctuations not resolved by COSMO
must be superimposed on the trajectories. The stochastic
nature of the fluctuations is captured by ensemble
calculations. Possibilities for further improvements in the
agreement with the measured backscatter data are
investigated by assuming a very slow mass accommodation of
water on ice, the presence of heterogeneous ice nuclei, or a
wide span of (spheroidal) particle shapes. However, the
resulting improvements from these microphysical refinements
are moderate and comparable in magnitude with changes caused
by assuming different regimes of temperature fluctuations
for clear-sky or cloudy-sky conditions, highlighting the
importance of proper treatment of subscale fluctuations. The
model yields good agreement with the measured backscatter
over both sites and reproduces the measured saturation
ratios with respect to ice over Payerne. Conversely, the
$30\%$ in-cloud supersaturation measured in a massive 4 km
thick cloud layer over Zurich cannot be reproduced,
irrespective of the choice of meteorological or
microphysical model parameters. The measured supersaturation
can only be explained by either resorting to an unknown
physical process, which prevents the ice particles from
consuming the excess humidity, or – much more likely –
by a measurement error, such as a contamination of the
sensor housing of the SnowWhite hygrometer by a
precipitation drop from a mixed-phase cloud just below the
cirrus layer or from some very slight rain in the boundary
layer. This uncertainty calls for in-flight checks or
calibrations of hygrometers under the special humidity
conditions in the upper troposphere.},
cin = {IEK-7},
ddc = {550},
cid = {I:(DE-Juel1)IEK-7-20101013},
pnm = {234 - Composition and Dynamics of the Upper Troposphere and
Stratosphere (POF2-234)},
pid = {G:(DE-HGF)POF2-234},
typ = {PUB:(DE-HGF)16},
UT = {WOS:000339934900013},
doi = {10.5194/acp-14-7341-2014},
url = {https://juser.fz-juelich.de/record/154628},
}