Abstract

Abstract. We present in situ measurements of the trace gas composition of the upper tropospheric (UT) Asian summer monsoon anticyclone (ASMA) performed with the High Altitude and Long Range Research Aircraft (HALO) in the frame of the Earth System Model Validation (ESMVal) campaign. Air masses with enhanced O3 mixing ratios were encountered after entering the ASMA at its southern edge at about 150 hPa on 18 September 2012. This is in contrast to the presumption that the anticyclone's interior is dominated by recently uplifted air with low O3 in the monsoon season. We also observed enhanced CO and HCl in the ASMA, which are tracers for boundary layer pollution and tropopause layer (TL) air or stratospheric in-mixing respectively. In addition, reactive nitrogen was enhanced in the ASMA. Along the HALO flight track across the ASMA boundary, strong gradients of these tracers separate anticyclonic from outside air. Lagrangian trajectory calculations using HYSPLIT show that HALO sampled a filament of UT air three times, which included air masses uplifted from the lower or mid-troposphere north of the Bay of Bengal. The trace gas gradients between UT and uplifted air masses were preserved during transport within a belt of streamlines fringing the central part of the anticyclone (fringe), but are smaller than the gradients across the ASMA boundary. Our data represent the first in situ observations across the southern part and downstream of the eastern ASMA flank. Back-trajectories starting at the flight track furthermore indicate that HALO transected the ASMA where it was just splitting into a Tibetan and an Iranian part. The O3-rich filament is diverted from the fringe towards the interior of the original anticyclone, and is at least partially bound to become part of the new Iranian eddy. A simulation with the ECHAM/MESSy Atmospheric Chemistry (EMAC) model is found to reproduce the observations reasonably well. It shows that O3-rich air is entrained by the outer streamlines of the anticyclone at its eastern flank. Back-trajectories and increased HCl mixing ratios indicate that the entrained air originates in the stratospherically influenced TL. Photochemical ageing of air masses in the ASMA additionally increases O3 in originally O3-poor, but CO-rich air. Simulated monthly mean trace gas distributions show decreased O3 in the ASMA centre only at the 100 hPa level in July and August, but at lower altitudes and in September the ASMA is dominated by increased O3. The combination of entrainment from the tropopause region, photochemistry and dynamical instabilities can explain the in situ observations, and might have a larger impact on the highly variable trace gas composition of the anticyclone than previously thought.

Highlights

  • The Earth System Model Validation (ESMVal) field experiment with the High Altitude and Long Range Research Aircraft (HALO, http://www.halo.dlr.de) was conducted during 10–24 September 2012 in close cooperation with the HALO TACTS mission (Jurkat et al, 2014; Vogel et al, 2015; Müller et al, 2016)

  • The in situ measurements considered in our study show enhanced carbon monoxide (CO) mixing ratios in the Asian summer monsoon anticyclone (ASMA), but instead of decreased O3 we found significantly increased O3 mixing ratios – relative to the upper tropospheric (UT) air encountered south of the anticyclone

  • Our study contributes to the so far sparse ASMA in situ measurements, allowing us to address some of the aspects of this important UT phenomenon that were recently identified as poorly understood (Randel et al, 2016): dynamical and chemical coupling with convection, composition/reactive chemistry in the monsoon region, and mixing of higher latitude lower-stratospheric air into the tropical tropopause layer (TL) by the ASMA

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Summary

Introduction

The Earth System Model Validation (ESMVal) field experiment with the High Altitude and Long Range Research Aircraft (HALO, http://www.halo.dlr.de) was conducted during 10–24 September 2012 in close cooperation with the HALO TACTS mission (Jurkat et al, 2014; Vogel et al, 2015; Müller et al, 2016). The accompanying paper is mainly based on EMAC simulations, which show that our in situ data reflect rather common processes in the ASMA Both studies shall help to explain the highly variable composition of the ASMA and its outflow, addressing the following key aspects of the ASMA that were recently identified as poorly understood (Randel et al, 2016): dynamical and chemical coupling with convection, composition/reactive chemistry in the monsoon region, mixing of higher-latitude lower-stratospheric air into the tropical TL by the ASMA.

In situ measurement techniques
Atmospheric dynamics and chemistry simulations
Lagrangian trajectory calculations
Mixing of different reservoirs during POI3
Processes reflected by nitrogen oxides during POI3
Synthesis for POI3 and related UT measurements
Entraining the TL
Air masses of POI3 at the eastern ASMA flank
Photochemical O3 production
Findings
Summary
Full Text
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