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2.4. DOAS TOMOGRAPHY GROUP 63<br />

2.4.6 2D and 3D tomographic LP-DOAS measurements of trace gas distributions<br />

in Heidelberg over an area of 4 ∗ 4 km 2<br />

Participating scientists Denis Poehler, Alexander Stelzer, Irene Pundt<br />

Abstract A configuration of three Multibeam LP-DOAS Instruments and 20 different light paths<br />

to retro reflector arrays was established for long term 2D and 3D measurements of NO2, SO2, O3,<br />

HCHO, and HONO over an area of a 4 ∗ 4 km 2 above the city centre of Heidelberg.<br />

Figure 2.30: 3 Dimensional view on all light paths of the measurement over an area of 4 ∗ 4 km 2 with<br />

three telescope locations: IUP, SAS and HD-Druck.<br />

Background LP-DOAS (Long Path Differential<br />

Absorption Spectroscopy) is a well known<br />

technique for measuring average concentrations of<br />

tropospheric trace gases along a light path extending<br />

between a telescope and a retro reflector. But<br />

single path measurements are often not sufficient<br />

(as well as single point measurements), if smallscale<br />

variations exist or transport is important.<br />

To obtain informations of the dispersion, it is necessary<br />

to measure along a couple of light paths.<br />

The development of the ”Multibeam LP-DOAS<br />

telescope” (Pundt and Mettendorf, 2005), allows<br />

the measurement along up to 6 light paths simultaneously.<br />

With the suitable combination of<br />

two or more Multibeam LP-DOAS telescopes and<br />

the use of tomographic reconstruction techniques<br />

good quality 2D and 3D reconstructions of the<br />

measured trace gases can be achieved.<br />

Funding German Ministry of Research and Education<br />

, AFO 2000-C, project 07 ATC-03<br />

Methods and results The experimental setup<br />

consists of 3 Multibeam telescopes located on top<br />

of high buildings in the city (IUP, HD-Druck and<br />

SAS) and 20 retro reflector arrays. This work focuses<br />

on the one hand on the telescope location<br />

HD-Druck, where a Multibeam Instrument was<br />

installed and modified, to allow automatic measurements<br />

from this place.<br />

Each of the three telescopes uses a Xe-Arc lamp as<br />

light source, which creates up to 6 parallel light<br />

beams using different mirrors. Each light beam<br />

can be redirected to different retro reflector arrays<br />

which reflect parts of the light back into the<br />

telescope. The received light is measured with a<br />

Czerny Turner Spectrograph and contains information’s<br />

of the trace gas absorptions. With the<br />

measurement between 285 nm and 365 nm and<br />

the use of the DOAS technique reconstruction of<br />

NO2, SO2, O3, HCHO, and HONO are made<br />

along each light path.<br />

During the first measurements it was mostly impossible<br />

to run all three telescopes simultaneously,<br />

due to many breakdowns of the sensitive experimental<br />

setup. But since simultaneous measurements<br />

of all light paths are necessary for tomographic<br />

inversions, the hardware was modified and<br />

new controller software was coded to improve the<br />

stability. First simultaneous measurements were<br />

performed in September 2005, but are not completely<br />

analysed yet.<br />

Outlook/Future work The system will be run<br />

continuously over a time scale of several months.<br />

For the periods of simultaneous measurement<br />

data, 2 dimensional trace gas distributions will<br />

be reconstructed.<br />

Main publication Poehler et al. [2005]

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