Dubrovsky M., 1992: Freezing nucleus spectra in the rain samples and their possible application on cloud conditions. In: Nucleation and Atmospheric Aerosols (ed.: Fukuta N. and Wagner P.E.), (Proceedings of 13th Int. Conf. on Nucleation and Atmospheric Aerosols, Salt Lake City, Utah) A. Deepak Publishing, p.321-324.
Martin Dubrovsky
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Institute of Atmospheric Physics, Hradec Kralove Czech
Republic
The basic findings following from evaluation of freezing nucleus spectra in 351 daily precipitation samples are: 1. The freezing nucleus spectrum may be expressed as a superposition of background and supplementary spectra. The background spectrum is quite conservative and smooth, the supplementary spectrum is expressed by steps superposed on the background spectrum. 2. Concentration of highly active supplementary nuclei increases with increasing instability of stratification of the atmosphere. Supported by similar findings referred in literature, it is hypothesized that the highly active nuclei have their origin from local sources. Regarding their supposed crucial role in cloud glaciation, author suggests to take them into consideration in prediction and modelling the cloud development.
The drop freezing technique provides the freezing
nucleus spectrum of hydrosol particles contained in the
aqueous sample. The very laboratory procedure gives very
accurate picture of the freezing nucleus content in the
aqueous sample. The great problems however arise when one
tries to relate the results of the drop freezing
experiments applied on precipitation samples to cloud
conditions (Rosinski et al., 1974; Rosinski et al., 1973).
Firstly, ice nuclei (IN) detected in the precipitation
sample are generally not identical with those playing
active role in cloud glaciation, and secondly, four
heterogeneous ice nucleation modes may function in the
cloud, but only immersion freezing is detected by drop
freezing experiments. Consequently, one can hardly
reconstruct the origin of hydrosolized particles and
their possible role in cloud process based on the results
of the drop freezing experiment.
This contribution presents findings following from the
evaluation of freezing nucleus spectra measured in 351
cumulative precipitation samples collected at the ground
level. Supporting the findings with those referred in the
literature, and considering these findings rather
qualitatively instead of quantitatively, author suggests
application on cloud conditions.
Sampling site is situated on the low elevation (about 50 m above the nearly completely flat terrain), relatively far from the main local sources of air pollutants, at the southern margin of Hradec Kralove. The freezing nucleus content in the precipitation sample is determined by a computer-driven drop freezing technique (Dubrovsky and Skoloud, 1989). The single drop freezing experiment consists in freezing the set (N=100) of 0.001 ml drops resting on the cold stage the surface temperature of which linearly decreases at a rate of 0.05 Ks-1. The primary outcome of the experiment is a distribution function P(T) being a fraction of drops frozen at temperature above T. Cumulative freezing nucleus spectrum nf(T) (number of freezing nuclei active above T) may be derived from P(T) according to the relation (Vali, 1971): nf(T) = - (1/v) ln[1 - P(T)], where v is a volume of a single drop.
Evaluation of freezing nucleus spectra determined on 351 daily precipitation samples1
1 The measurements were performed only on precipitation samples of volume greater than 40 ml due to the technique of forming the drops. Two separate measurements were performed on each sample with subsequent cumulation of drop freezing temperatures.
collected during 1983-1987 indicates following, worth
mentioning findings: 1. The freezing nucleus spectrum may
be expressed as a superposition of background and
supplementary spectra. Background spectrum is quite
conservative and smooth (possible to be parametrized as nf0(T)
= a[exp(-bT) - 1], where a = 10-16mm-3,
b = 1.8 K-1), the supplementary population of
freezing nuclei is often expressed by steps superposed on
background spectrum. 2. Concentration of highly active
supplementary nuclei increases with increasing
instability of stratification of the atmosphere.
Some illustrative examples are given in Fig.1. Sample
belonging to 84/01/09 is a typical sample containing only
background spectrum, while the other samples contain some
amount of the supplementary IN effective at warmer
temperatures (referred to as super IN in next). Worth to
mention is the step-wise character of some distribution
functions, with frequent occurrence of -9 C step. The
dependence of super IN concentration on stability of
atmospheric stratification manifests itself also in a
generally lower content of super IN in the winter
precipitation samples, while the samples belonging to the
stormy summer days with high-intensity showers often
contain great concentrations of IN active at temperatures
-9 C and warmer.
These findings well correspond with those of other
authors: Rosinski and co-authors (Rosinski et al, 1971;
Rosinski and Nagamoto, 1976) distinguish two populations
of aerosol particles in severe convective storms: the
normal background aerosol and aerosolized soil particles.
Large aerosol particles of the latter population
entrained into the cloud due to the convective activity
then give an origin to the warm-temperature peaks on the
freezing nucleus spectra. The presence of highly active
freezing nuclei in the convective precipitation samples,
including the hail samples, is also expressed in
measurements by Vali [Vali and Stansbury (1966), Vali (1968,
1969, 1971)]. Some measurements of both authors exhibit
the significant nucleation activity maximum belonging to
nuclei active at temperatures close to -9 C. Freezing
nuclei with activity close to -9 C were also detected in
soil samples by Rosinski et al. (1973).
The curve in Fig.1 belonging to the bacterial suspension
(Dubrovskþ et al., 1989) evokes idea on the biogenic
origin of the atmospheric IN (cf. Schnell and Vali, 1976;
Vali et al., 1976). Unfortunately, in time of our
measurements no tests were made to learn an origin of the
super IN.
It follows from above that the IN population in the atmosphere consists of background population which may be the rather large-scale property of the air mass, and the supplementary population having origin from local sources. This "local population" may be ingested into the cloud due to the convective activity and may involve giant aerosol particles functioning as highly active IN. Although our measurements do not allow to determine an origin of highly active freezing nuclei in the precipitation samples and their possible role in cloud development, based on Vali (1974)1 and Rosinski et al (1971)2 it appears that at least the part of the super IN found in the
1 who compared the nucleus
spectra for near-simultaneous samples at cloud base and
at ground level and concludes, that the majority of
freezing nuclei found in the rain have entered the
precipitation elements during the formative stages of the
precipitation.
2 who found highly active IN in
the centres of hailstones, indicating that IN active at
higher temperatures nucleate some of the hail embryos in
severe storms.
precipitation samples played an active role in the
cloud glaciation. In case the super IN are ingested into
the totally water cloud, the effect of the super IN would
resemble the cloud seeding: the type of super IN
determines the onset temperature of cloud glaciation and
the concentration of super IN determines the initial
concentration of ice particles. Due to the scarcity of
the super IN and sufficient time delay between the
activation of the super IN and background IN (as
indicated by length of step on some distribution
functions in Fig.1) the ice particles formed on super IN
have enough time and enough water to grow to give rise to
hail embryos. Consequently, presence of even limited
concentration of highly active IN may be of great
importance for glaciation process and should be paid
corresponding attention.
Prediction of rain. In fact, information on the
probability (or onset, course) of cloud glaciation may
help while giving prediction of probability of occurrence
(or onset, character) of precipitation event. In view of
the above findings, the process of the cloud glaciation
may be under suitable conditions incited (and in fact
governed) by supplementary ingredient of the IN spectrum.
The task is then to estimate the shape of the IN spectrum
probable to occur in the cloud. The type of IN could be
deduced on the basis of knowledge of possible sources of
atmospheric aerosol (local sources may predominate in
case of the local convective clouds) and the amount of
particulate matter ingested into the cloud could be
estimated as a function of the actual meteorological
conditions with a stress upon the stability of the
stratification and wind speed.
Regarding the frequent usage of predictors based on level
of intensive crystallization (LIC, often taken as -12 C
level) in prediction of convective phenomena, one can
consider the LIC temperature as variable dependent upon
local weather and local sources of IN.
Parametrization of ice formation. Ice formation
rate is usually parametrized to monotonously increase
with decreasing temperature. In view of the possible role
of super IN, the supplementary population of highly
effective ice nuclei of limited concentration is
suggested to be considered. The total cumulative IN
spectrum n(T) may take the form n(T) = n0(T) +
n'(T), where n0(T) is a background spectrum
and n'(T) is a supplementary spectrum. Background
spectrum may be parametrized by some exponential or power-law
function, the supplementary spectrum can be parametrized
by simple step-wise function, e.g., n'(T) = SUMi=1,..,r
ci{1 - exp[-(T/Ti)ai]},
where r is number of types of supplementary IN, ci
is the concentration of the IN of the i-th kind; Ti,
ai are parameters of the activity spectrum of
the IN of the i-th kind (Ti is a
characteristic activation temperature and ai
characterizes dispersion of the actual activation
temperatures around Ti). It is not obvious how
to turn the results obtained with a drop freezing
technique referred in the previous chapter into the
quantitative expression of the IN spectra associated with
the individual nucleation modes. In a first approach one
may take r = 1; T1 = -9 C (for immersion
freezing; should be suitably modified for other
nucleation modes); a1 = infinity.
Concentration c1 should be given some
realistic value. The test of sensitivity upon varying
parameters T1 and c1 could be of great value for proper
evaluation of possible role of super IN in cloud
development.
The presence of supplementary IN population may be also
reflected in adequate form in the bulk parametrization
schemes by adding some steps of variable hight and
characteristic temperature (being possibly dependent upon
atmospheric conditions and locality) to ice formation
governing functions.
Fig.
1 Distribution functions of the drop freezing
temperatures. Triangles, asterices, filled squares, empty
squares, x: daily precipitation samples; line : bacterial
suspension (Pseudomonas syringae); Thunderstorms
occurred on 84/04/16, 84/05/21 and 84/05/23.