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@PHDTHESIS{Gensch:2112,
author = {Gensch, Iulia},
title = {{W}ater and nitric acid in cirrus clouds:microphysical
kinetical modeling and a closure to field observations},
volume = {4286},
school = {Univ. Wuppertal},
type = {Dr. (Univ.)},
address = {Jülich},
publisher = {Forschungszentrum Jülich GmbH Zentralbibliothek, Verlag},
reportid = {PreJuSER-2112, Juel-4286},
series = {Berichte des Forschungszentrums Jülich},
pages = {IX, 105 p.},
year = {2008},
note = {Record converted from VDB: 12.11.2012; Wuppertal, Univ.,
Diss., 2008},
abstract = {Upper tropospheric relative humidities over ice
(RH$_{ice}$) of up to 200\% have been reported frequently in
recent times. This unexpectedly high supersaturation out-
and inside of cold cirrus clouds may have significant impact
on the Earth’s climate. In the first case, clear sky
supersaturation could be justified when the critical
supersaturation for ice cloud formation is higher than until
now assumed. This would lead to a decrease in high cloud
cover and thus impact on the radiation budget. In the second
case, high supersaturation inside of cirrus clouds could
suggest the existence of unknown microphysical and radiative
properties with consequences for climate and the vertical
redistribution of water and nitric acid. Peter et al. (2006)
summarized possible reasons for the observed supersaturation
in a ’supersaturation puzzle’, calling into question
whether this puzzle can be solved by solely using the
conventional ice cloud microphysics. Another important
question raised in this study is whether the supersaturation
may result from uncertainties or flaws in the water
measurements. The aim of this PhD thesis is to puzzle out
these questions. Therefore upper tropospheric field
observations are simulated with an adequate conventional
kinetic model in order to analyze the origin and persistence
of high ice supersaturation, particularly inside cold cirrus
clouds. The proposed $\underline{M}$odel for
$\underline{A}$erosol and $\underline{I}$ce
$\underline{D}$ynamics (MAID) handles widely aerosol and ice
microphysics, including: gas-diffusive particle growth and
evaporation, homogeneous and heterogeneous ice nucleation,
water vapor deposition and nitric acid uptake on growing ice
crystal. Special emphasis of MAID is the exact balancing of
chemical species among different physical states. MAID is
validated here, based on observations during the field
campaign POLSTAR–1 1997 (Polar Stratospheric Aerosol
Experiment). Further, a detailed analysis of cirrus cloud
observations during CR-AVE 2006, the tropical Costa Rica –
Aura Validation Experiment, is performed with MAID. The
model is initialized with different aerosol properties,
water mixing ratios, accommodation factors of water on ice
and amplitudes of mesoscale temperature fluctuations. A
notable feature here is to vary the freezing mechanism in
the simulations. The model results indicate high sensitivity
of the cloud microphysical evolution to the freezing
pathway. The ice microphysics, as well as the partitioning
of water and nitric acid inside the cloud derived from all
sensitivity studies are compared at last with the the
microphysical and chemical in-situ observations, to
determine the most probable constellation of initial
conditions and processes that led to the very cold,
sub-visible tropical cirrus cloud observed during CR–AVE.
The best agreement between model results and measurements is
given when the cirrus cloud forms heterogeneously, with
total accommodation of water on ice. By varying the freezing
pathway, the accommodation factor of water on ice, or the
amount of available water, clouds with completely different
microphysical properties form. As a summary, this work
demonstrates that it is possible to simulate significant
supersaturation inside cold cirrus (T<200 K) with
conventional microphysics when assuming heterogeneous ice
nucleation as the freezing mechanism. Thus, heterogeneous
freezing appears to be an important pathway for cold cirrus
cloud formation. More generally, a freezing mechanism
producing low number densities of ice crystals could explain
the frequent high supersaturation inside cirrus clouds
observed in this temperature range.},
cin = {ICG-1},
cid = {I:(DE-Juel1)VDB790},
pnm = {Atmosphäre und Klima},
pid = {G:(DE-Juel1)FUEK406},
typ = {PUB:(DE-HGF)11},
url = {https://juser.fz-juelich.de/record/2112},
}