Observations continue to highlight the importance of heterogeneous reactions on
sulfate aerosols, and implicate N
O
hydrolysis [ Van Doren
et al, 1991] as the most important process for altering the gas-phase photochemical
balance of ozone-destroying radical species in the mid-latitude lower
stratosphere. This reaction produces the
photochemically stable HNO
, so it is a sink for NO
. This, in turn,
leads to enhancements of reactive halogen oxide and HO
radicals relative to
their abundances if only gas-phase reactions are considered. Rodriguez et
al. [1991] and King et al. [1991] were the first
to cite enhancements of ClO in the high-latitude lower stratosphere in winter
as evidence for the potential importance of this process. Based on a
comparison of a ClO balloon profile to results from a model
constrained by empirical tracer interrelationships, Avallone et al.
[1993a] confirmed the importance of this reaction over a broader
altitude range. However, these initial studies were limited by the lack of
simultaneous measurements of NO
.
Because N
O
is rapidly photolyzed in daylight to produce NO
,
that rate of formation of HNO
by N
O
hydrolysis depends upon formation of
N
O
after sunset and subsequent heterogeneous conversion in darkness. In
the presence of high abundances of aerosols the latter step is sufficiently
fast that production of N
O
, a process limited by the
temperature-dependent formation of NO
from NO
+ O
, largely
determines the rate of HNO
production. At low aerosol abundances the
reaction probability, available aerosol surface, and photolysis of N
O
become the limiting factors. Consequently, the importance of N
O
hydrolysis depends on temperature and available sunlight (i.e. on altitude,
latitude, and season) in a fairly complex way.
In regions of high aerosol loading, Fahey et al. [1993] and
Mills et al. [1993] observed non-linear reductions in NO
at mid-latitudes. These decreases, which were reproduced well by models
incorporating N
O
hydrolysis on sulfate, reached ``saturation'' as
modeled by Prather [1992]. At different altitudes, saturation is
limited by formation of N
O
at different aerosol surface loadings.
Perliski and Solomon [1992] showed that dramatic decreases in
NO
columns, even those at high solar zenith angles, could not have been due
to aerosol-induced changes in atmospheric radiation. Thus, column measurements from
the ground and from aircraft [ Coffey and Mankin, 1993] are valid
and indicate that the perturbation to NO
extended over a wide altitude
range.
The response of ClO to decreased NO
due to
Pinatubo aerosol has been observed by aircraft, balloons, and satellite
[ Fahey et al., 1993, Wilson et al., 1993, Avallone
et al., 1993b, Dessler et al., 1993, and Waters et al., 1995b].
In addition, obsevations of ClO from the ER-2 and UARS [ Toohey
et al., 1991,1993b and Waters et al., 1995b]
have revealed a seasonal dependence of mid-latitude ClO that is
inverse to what would be expected in the absence
of heterogeneous chemistry. Avallone et al.
[1993b] showed that the largest enhancements of ClO were observed at
lower latitudes, consistent with the saturation effects displayed by NO
.
Solomon et al. [1994] reported that NO
reductions were
observed from McMurdo even during the polar summer, and suggested that
excursions of air to dark regions or direct conversion of NO
to
N
O
could be responsible.
The increases in aerosol surface area due to Pinatubo should also have enhanced
the rates of other heterogeneous reactions. Perhaps most important is the
hydrolysis of ClONO
to HOCl and HNO
on sulfate. Because ClO from
photolysis of HOCl can titrate any remaining NO
, this process can
potentially reduce NO
abundances below those of reactive chlorine.
The efficiency of this reaction varies strongly with aerosol composition
[{ Hanson et al., 1994], and hence temperature, such that
it is likely to be most important in cold regions where nitric acid
photochemistry is slow (i.e., near the tropopause or in the winter polar
regions). Ground-based observations [ Solomon et al.,
1993] have implicated this process over Antarctica, and it may have
contributed to additional ozone depletion observed there in 1992 [
Hofmann et al. 1993].
Whether ClONO
hydrolysis is important at
mid-latitudes is less clear. Fahey et al. [1993] and Dessler
et al. [1993] argued that this process did not contribute
significantly to NO
and ClO abundances they observed outside the arctic
vortex under volcanic conditions. However, both of these studies examined this
issue with zonally symmetric models which, in light of the work of Kawa
et al. [1993] and Solomon et al. [1994],
could have accentuated the effects of other heterogeneous reactions,
thereby masking the potential
importance of ClONO
hydrolysis. In addition, the ClO abundances at
lower altitudes reported by Dessler et al. [1993] were
systematically higher than those observed by the ER-2 and UARS outside the
vortex during the same winter. Thus, it remains unclear whether ClONO
hydrolysis at northern middle and high latitudes was an important process at
the peak of Pinatabo loading.
Hanson et al. [1994] has outlined a procedure for
incorporating into models the various reactions on sulfate aerosols. Those
involving HCl must
be carefully parameterized because of the temperature dependence of HCl
solubility. Their calculations suggest that reactions of HCl with ClONO
and
HOCl on sulfate could have contributed to enhancements of reactive chlorine
during Pinatubo years, such as those observed by Solomon et al.
[1993], and would be most important in regions that do not quite
reach NAT temperatures, such as just outside the antarctic vortex. Such
reactions could help explain the increase in size of the antarctic ozone hole,
both vertically and horizontally, in the years immediately following the
eruption of Pinatubo.