Extended abstract - to appear in the
Proceedings of the 1st General Assembly of the WCRP Project 'Stratospheric
Processes and their Role in Climate' (SPARC), Melbourne, Australia, 2-6
December 1996.
LOWER STRATOSPHERIC WATER VAPOUR AT LOW LATITUDES AS OBSERVED BY HALOE
D.R Jackson1, S.J Driscoll1,*, E.J Highwood2,
J.E Harries1 and J.M Russell III3
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1 Blackett Laboratory, Imperial College, London, U.K.
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2 Department of Meteorology, University of Reading, Reading,
U.K.
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3 Hampton University, Hampton, Va, USA.
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* Current affiliation: UK Meteorological Office, Bracknell,
U.K
ABSTRACT
In this paper we present observations of water vapour in the lower equatorial
stratosphere made by the Halogen Occultation Experiment (HALOE) instrument,
which flies on the Upper Atmosphere Research Satellite (UARS). These data
make an important new contribution to the observational knowledge of this
region, since lower stratospheric water vapour has largely been observed
to date using in-situ instruments, and the only global longitudinally-resolving
satellite observations of this region to be reported are those from the
Stratospheric Aerosol and Gas Experiment II (SAGE II). Here, we use the
HALOE data to provide insight into the amount of cross-isentropic flow
in the Asian monsoon region. In addition, the interannual variability in
the water vapour distribution in boreal winter is examined, and linked
to the long-lived 1990-1995 El Nino Southern Oscillation (ENSO).
1. INTRODUCTION
It is widely accepted that most water vapour enters the stratosphere near
the tropical tropopause, and hence tropical tropopause conditions have
a strong impact on the stratospheric water vapour distribution. However,
it is not exactly clear how the cross-tropopause transport of water vapour
occurs. This has been the subject of much recent research (see Potter and
Holton, 1995, and references therein). A problem with the study of such
troposphere to stratosphere transport is the paucity of observations. The
dehydration of the lower stratosphere has largely been investigated using
in situ measurements, which, although usually very accurate, suffer from
limited temporal and spatial coverage. Much more extensive coverage of
water vapour in this region has come from Limb Infrared Monitor of the
Stratosphere (LIMS) (see eg Jones et al, 1986) and Stratospheric Aerosol
and Gas Experiment II (SAGE II) (Rind et al, 1993) satellite observations.
However, the LIMS dataset is short (Oct. 1978 - May 1979) and of low accuracy
near the tropopause, whilst Rind et al did not in general discuss interannual
variability in the SAGE II retrievals. Further observations of middle atmosphere
water vapour have recently become available via the Halogen Occultation
Experiment (HALOE), which flies on the Upper Atmosphere Research Satellite
(UARS). HALOE can observe at lower stratospheric levels located very close
to the tropical tropopause, and in addition is highly suitable for studying
interannual variability, since it is still in operation at the time of
writing. Therefore, the HALOE dataset extends the observational knowledge
of lower stratospheric water vapour, and in particular provides valuable
new information about its interannual variability.
2. INSTRUMENT DESCRIPTION
HALOE views solar infrared radiation in the 2.5 to 10.0 µm region
by means of solar occultation, and measures a variety of atmospheric constituents,
plus temperature and aerosol extinction (see Russell et al, 1993). The
water vapour channel is at 6.60 µm. HALOE is capable of observing
water vapour from the tropopause up to the upper mesosphere with a vertical
resolution of approximately 2 km, and with an accuracy of +_ 10 % between
0.1 and 100 mb, rising to +_ 30 % at the boundaries of the observational
range (Harries et al, 1996). Because HALOE is a solar occultation experiment,
observations are made only at sunset and sunrise. 15 observations at both
sunset and sunrise are made each day, and are clustered around two rings
of latitude (one for sunrise, one for sunset). As the orbit drifts, these
latitudes slowly change and may pass each other and reverse, with a period
of order one month. Details of the calculation of monthly and seasonal
fields appear in Jackson et al (1996).
3. LOWER STRATOSPHERIC WATER VAPOUR IN THE ASIAN SUMMER MONSOON REGION
Three years of HALOE data, from December 1992 to November 1995, were used
to create seasonal plots of water vapour. A full comparison of these fields
with the seasonal climatology of SAGE II data reported by Rind et al (1993)
appears in Jackson et al (1996). Here, we concentrate on the region of
the lower stratosphere affected by the Asian summer monsoon. In June -
July - August (JJA) at 129 mb (Figure 1a) the area of the highest water
vapour values (greater than 6.0 ppmv) is located between 15oS
and 30oN, with a distinct region of high water vapour located
over Asia, which is caused by strong tropospheric convection linked with
the Asian Monsoon. This region of high water vapour is also observed in
JJA at both 100 mb (not shown) and 83 mb (Figure 1b). At both 129 and 100
mb, water vapour values are a maximum at low latitudes. However, at 83
mb this pattern has reversed, with lowest values now found over the equatorial
region. This differing pattern occurs firstly because the Asian monsoon
acts to hydrate the lower stratosphere in JJA at both 129 and 100 mb, and
secondly because the annually varying pattern in water vapour present at
100 mb (with a minimum in December - January - February (DJF)) and a maximum
in JJA) propagates slowly upwards with time (see Mote et al, 1996). Therefore,
it is likely that much of the low equatorial water vapour seen at 83 mb
in JJA entered the stratosphere in the previous season and propagated slowly
upwards.

Figure 1 - Three-year mean of HALOE water vapour mixing ratio in
JJA. Contour interval: 0.4 ppmv. Values less than 3.2 ppmv and greater
than 6.0 ppmv are shaded. Shade lines run from bottom left to top right
for values less than 3.2 ppmv, and from bottom right to top left for values
greater than 6.0 ppmv. Values less than 2.4 ppmv and greater than 8.8 ppmv
have denser shading. Regions not sampled by HALOE are left blank. a) 129
mb; b) 83 mb.
Dynamical interpretation of the JJA Asian monsoon is easier if the data
are expressed on isentropic surfaces, since in the middle atmosphere parcels
of air are transported approximately along such surfaces. The 375 K isentropic
surface is located between the 100 and 129 mb pressure levels under mean
conditions in the region of the JJA monsoon. Figure 2a shows that in JJA
on the 375 K isentropic surface the region of high water vapour over Asia
is still present, indicating that significant cross-isentropic transport
of moist air takes place at that level. However, at stratospheric levels
more distant from the tropopause, this pattern changes; at 420 K (Figure
2b) this region of moist air has almost completely disappeared. Since under
mean conditions the 420 K isentropic level is located near 83 mb, this
suggests that the region of moist air to the north and west of India at
83 mb (Figure 1b) is due to a localised upward bulge in the isentropic
surfaces, rather than to any transport across the 420 K isentrope.

Figure 2 - Three-year mean HALOE water vapour for JJA, expressed
on an isentropic surface. Contour interval: 0.4 ppmv. Regions of shading
are as described in Figure 1.a) 375 K; b) 420 K.
4. INTERANNUAL VARIABILITY
Figures 3a and 3b show HALOE water vapour on the 375 K isentropic surface
for DJF 93/94 and DJF 94/95, respectively. In both years there is a belt
of low water vapour at low latitudes located between the Indian Ocean and
the central Pacific. An interesting difference is that in 93/94 the water
vapour is a minimum near Indonesia, whereas in 94/95 there is a local maximum
near Indonesia, with lower water vapour mixing ratios located to the east
and to the west of there. Examination of individual monthly fields shows
that such features are persistent. Sea surface temperature (SST) anomalies
(calculated by Reynolds and Smith, 1994) for January 1994 and 1995 show
that cold SST anomalies often coincide with local maxima in the water vapour
fields in the Indonesian region. Therefore, if it is assumed that cooler
SSTs lead to less deep convection, and hence a greater tropopause temperature
minimum, then the SST anomalies may explain the behaviour of the water
vapour field near Indonesia in DJF 93/94 and 94/95. We recognise that,
although this assumption is often true, closer inspection shows that the
relationship between deep convection and SSTs can often be more complicated
(see eg Zhang (1993) and references therein). However, the results do suggest
that interannual variability in SSTs can influence water vapour mixing
ratios near the tropopause. Since such fluctuations in Pacific SSTs are
associated with the long-lived 1990-1995 El Nino Southern Oscillation (ENSO),
this means that El Nino signals may be being seen in equatorial water vapour
fields at levels just above the tropopause.

Figure 3 - HALOE water vapour on the 375 K isentropic surface. Contour
interval: 0.4 ppmv. Regions of shading are as described in Figure 1. a)
DJF 93/94; b) DJF 94/95.
Acknowledgements
We would like to acknowledge the support and assistance of the HALOE Project
and Science Teams. The HALOE data were obtained through the British Atmospheric
Data Centre (BADC) facility. DRJ, SJD and EJH received financial support
from the UK Natural Environment Research Council.
References
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J.M III, 1996: Lower stratospheric water vapour at low latitudes as observed
by HALOE, 1992-1995. Submitted to Quart. J. Roy. Meteor. Soc.
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