University of Bremen IUP DOAS


DOAS HOME
NEWS
blog
PUBLICATIONS
POSTER GALLERY
EDUCATION
SEMINAR
MEMBERS
MEETINGS
INTERNAL
LINKS

Research

PROJECTS
SATELLITE
GROUND-BASED
AIRBORNE
DATA PRODUCTS

Navigate

Up
AMAX-DOAS
IDOAS

Airborne Multi Axis DOAS measurements (AMAXDOAS)


Introduction    References    Links    Contact

Top Introduction:

As part of the German contribution to the validation of the SCIAMACHY instrument on board of ENVISAT, a set of instruments was flown on the DLR FALCON in several campaigns in high, middle and low latitudes. The instruments involved are the ozone and aerosol LIDAR OLEX (operated by DLR Oberpfaffenhofen), the microwave radiometer ASUR (operated by the University of Bremen) and the multi axis DOAS instrument AMAXDOAS (operated by the Universities of Bremen and Heidelberg).

 

The AMAXDOAS instrument is similar to the DOAS instruments used on the ground but observes the atmosphere simultaneously in different directions, both upwards and downwards. The rationale for using different viewing directions is to derive information not only on the total column of absorbers, but also on their vertical distribution. The most straightforward information comes from the difference between nadir and zenith viewing measurements that enables tropospheric and stratospheric columns to be separated. These quantities are of particular interest as SCIAMACHY will measure total columns and stratospheric profiles of O3, NO2, BrO, H2O and other trace species quasi simultaneously. The difference between total column and integrated profile yields the tropospheric column. The AMAXDOAS instrument provides direct validation of these partial columns. Additional information can be retrieved from the slant viewing geometries, but this is a more experimental measuring mode that still has to be developed further.

The experimental set-up of the AMAXDOAS consist of two imaging grating spectrometers, one for the UV and one for the visible wavelength region. Two domes are mounted on top and below the FALCON, each housing several small telescopes pointing in the atmosphere at different angles. Quartz fibres conduct the light from the telescopes to the spectrometers, where the spectra from the individual viewing directions are projected on different parts of the CCD detectors. With this set-up, spectra from light with very different optical paths through the atmosphere can be measured simultaneously.

Apart from the possibility to separate tropospheric from stratospheric columns, air borne measurements have other important advantages for the validation of SCIAMACHY measurements. In contrast to balloon borne experiments, measurements from the FALCON can provide continuous time series along the satellite track. Also, the horizontal inhomogeneity of SCIAMACHY ground pixels can be explored by selecting a flight track perpendicular to the satellite orbit. To optimise the output of the experiments, FALCON measurements were closely co-ordinated in space and time with balloon launches during the SCIAMACHY validation campaigns.

Top References:

Top Links:

Top Contact:

If you are interested in more information on the AMAXDOAS instrument, please contact Ping Wang or Andreas Richter.

web master:  folkard@iup.physik.uni-bremen.de      Last Update: 25-05-18      Data Privacy