Title: Multi-axis differential absorption spectroscopy (MAX-DOAS) at the And
1Multi-axis differential absorption spectroscopy
(MAX-DOAS) at the Andøya Rocket Range in February
and March 2003
- Folkard Wittrock, Hilke Oetjen, Andreas Richter,
and John P. Burrows
2Structure
- Focus of DOAS observations
- DOAS analysis
- Introduction to MAX-DOAS
- Selected results from Andøya campaign
- BREDOM
- Summary and outlook
3DOAS observations Focus
- Determination of atmospheric trace gases
- Ozone, NO2, NO3, OClO, BrO, IO, HCHO
- Validation of satellites (GOME, SAGE, SCIAMACHY)
and of model calculations - standard data products
- vertical columns of ozone and NO2
- slant columns of OClO, BrO, HCHO and IO
- further data products
- vertical columns of BrO, OClO, HCHO
- tropospheric amounts e.g. for NO2, BrO
4Differential Optical Absorption Spectroscopy
(DOAS)
- Only narrowband, i. e. differential structures
of the spectra are used to detect the absorbers. - Broadband absorption and other broadband
structures like instrumental features and
features caused by Mie and Rayleigh scattering
are removed by a polynomial. - Basically, all kind of light sources can be
used. - Here Light scattered in the zenith or at
the horizon
5DOAS Equation
- Radiation in matter is attenuated according to
the Lambert-Beer-Law - The current intensity I(l) is compared to a
reference I0(l) - A polynomial is added to compensate for
scattering and other broadband structures - Slant columns of several absorbers (with known
absorption cross sections si) can be retrieved
simultaneously - The slant column is the density of the absorber
along the photon path and depends on the SZA -
6Multi Axis (MAX)-DOAS
- Extension of the light path in the troposphere
- High sensitivity for tropospheric absorbers,
similar path through the stratosphere - 3 angles to describe the geometry
- 1. elevation angle 2. SZA 3.
relative azimuth
7Radiative Transfer and Vertical Columns
- Light path is simulated by a radiative transfer
model - The air mass Factor (AMF) weights the absorption
due to the changing SZA, viewing angle, azimuth - Vertical column (V) is the vertical density of
the absorber - Here SCIATRAN (CDIPI-Version) by A. Rozanov
- Input
- viewing geometry
- profile of absorbers
- T and p profiles
- wavelength region
- albedo
- aerosols
8 2 Instruments Asymmetric Czerny-Turner
Spectrometer CCD
- CCDs
- 1320x400 pixel
- 1024x256 pixel
- Wavelength
- region
- 325 413 nm
- 330 490 nm
- FWHM
- 0.45 nm
- 0.60 nm
- Integration
- time
- 1 min
9Multi-Axis Telescopeon the roof of the old
Lidar-Building
- Commercial stainless steel box
- Shadings to avoid direct sun
- Pointing of telescope towards NNW
10MAX-DOAS telescope
Automated measurements in 4 directions 3,
7.5, 12.5 and zenith
- Different viewing directions given by moving
mirror - Box is heated to ensure operation of the motor
and ice free windows - Calibration unit with lamps Tungsten and HgCd
- Quartz fiber bundle adapter
11MAX-DOAS measurements data analysis
- Basic idea
- Use O4 to find correct model settings
- derive slant columns of O4 for given directions
- simulate O4 slant columns (vertical column is
known) and vary aerosol scenario and surface
albedo until closure for all lines of sight and
also solar zenith angles is obtained - Use information from different lines of sight to
derive profile information for the absorber of
interest - simulate absorbers slant column using aerosol
and albedo settings from O4 retrieval and vary
profile until good agreement with retrieved slant
columns is reached for all directions - RTM SCIATRAN full spherical, multiple
scattering, refraction
12MAX-DOAS measurements O4
13MAX-DOAS measurements NO2
14MAX-DOAS measurements BrO
15Andøya MAX-DOAS Summary and Outlook
- Results
- Multi Axis DOAS measurements from 4 different
groups are being performed during the campaign - O3, NO2, BrO columns can be retrieved
- tropospheric amounts of BrO and NO2 have been
estimated - Andoya measurements are very valuable to check
the consistency of different MAX-DOAS setups
Analysis still ongoing - Problems
- clouds make the analysis very complex
- automated profile retrieval still under
development
16Acknowledgments
- We like to thank the whole ARI staff for there
great support and especially - Reidar, Michael, June, Petter
- Tusen takk!
17Bremian DOAS network for atmospheric measurements
(BREDOM)
- Three tropical stations
- Similar setup for all measurement sites
- High-sensitivity DOAS-instruments for stand-alone
operation - Multiple viewing directions (MAX-DOAS)
- Retrieval of ozone and NO2 as well as minor
absorbers (e.g. BrO, OClO, SO2, HCHO)
18What is the rationale behind BREDOM?
- For the validation of satellites (e.g. SCIAMACHY
on ENVISAT), we need - long term validation
- of many trace species
- on a global scale
- From recent validations (e.g. GOME) we learned,
that - DOAS UV/visible instruments can provide such
validation - that tropical stations are mandatory
- that tropospheric products need extra validation
- Build on the existing DOAS network, extend the
range of species, add stations in the tropics,
add capability to monitor troposphere
19Bremian DOAS network for atmospheric measurements
(BREDOM)
- Three tropical stations
- Similar setup for all measurement sites
- High-sensitivity DOAS-instruments for stand-alone
operation - Multiple viewing directions (MAX-DOAS)
- Retrieval of ozone and NO2 as well as minor
absorbers (e.g. BrO, OClO, SO2, HCHO)
- Campaign instrument
- Kaashidhoo (5 N, 73 W, 5m asl) February
March 1999 - Po area (46 N, 9 E, 400m asl) JulyAugust
2002, - SeptemberOctober 2003
- Andoya (69 N, 16 E, 20m asl) FebruaryMarch
2003