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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]