Rugged optical mirrors for Fourier transform spectrometers operated in harsh environments
The Total Carbon Column Observing Network (TCCON) and the Network for the Detection of Atmospheric Composition Change (NDACC) operate a number of Fourier transform spectrometers (FTSs) that measure trace gases in the atmosphere by observing solar spectra. To guide the sunlight into the FTS, a solar...
| Main Authors: | , , , |
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| Format: | Article |
| Language: | English |
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Copernicus Publications
2016-05-01
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| Series: | Atmospheric Measurement Techniques |
| Online Access: | http://www.atmos-meas-tech.net/9/2381/2016/amt-9-2381-2016.pdf |
| _version_ | 1818064368592486400 |
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| author | D. G. Feist S. G. Arnold F. Hase D. Ponge |
| author_facet | D. G. Feist S. G. Arnold F. Hase D. Ponge |
| author_sort | D. G. Feist |
| collection | DOAJ |
| description | The Total Carbon Column Observing Network (TCCON) and the Network for the
Detection of Atmospheric Composition Change (NDACC) operate a number of
Fourier transform spectrometers (FTSs) that measure trace gases in the
atmosphere by observing solar spectra. To guide the sunlight into the FTS,
a solar tracker has to be placed outside. This device needs high-quality
optical mirrors with good reflectance in the near and mid-infrared.<br><br>More and more FTS stations are operated in remote locations with harsh
environments. Optical mirrors are usually made for laboratory conditions and
might not last very long there. At the TCCON site on Ascension Island which
is operated by the Max Planck Institute for Biogeochemistry (MPI-BGC),
several mirrors from different optical manufacturers were destroyed within
weeks.<br><br>To continue operation, the MPI-BGC had to develop rugged mirrors that could
sustain the harsh conditions for months or even years. While commercially
available mirrors are typically made from a substrate covered with a thin
reflective coating, these rugged mirrors were made from stainless steel with
no additional coating. Except for their lower reflectance (which can easily
be compensated for), their optical properties are comparable to existing
mirrors. However, their rugged design makes them mostly immune to corrosion
and scratching. Unlike most coated mirrors, they can also be cleaned easily. |
| first_indexed | 2024-12-10T14:34:53Z |
| format | Article |
| id | doaj.art-a2ab35e3ff254947ab6b38123e80451d |
| institution | Directory Open Access Journal |
| issn | 1867-1381 1867-8548 |
| language | English |
| last_indexed | 2024-12-10T14:34:53Z |
| publishDate | 2016-05-01 |
| publisher | Copernicus Publications |
| record_format | Article |
| series | Atmospheric Measurement Techniques |
| spelling | doaj.art-a2ab35e3ff254947ab6b38123e80451d2022-12-22T01:44:51ZengCopernicus PublicationsAtmospheric Measurement Techniques1867-13811867-85482016-05-01952381239110.5194/amt-9-2381-2016Rugged optical mirrors for Fourier transform spectrometers operated in harsh environmentsD. G. Feist0S. G. Arnold1F. Hase2D. Ponge3Max Planck Institute for Biogeochemistry (MPI-BGC), Jena, GermanyMax Planck Institute for Biogeochemistry (MPI-BGC), Jena, GermanyKarlsruhe Institute of Technology (KIT), Institute of Meteorology and Climate Research (IMK-ASF), Karlsruhe, GermanyMax-Planck-Institut für Eisenforschung GmbH, Düsseldorf, GermanyThe Total Carbon Column Observing Network (TCCON) and the Network for the Detection of Atmospheric Composition Change (NDACC) operate a number of Fourier transform spectrometers (FTSs) that measure trace gases in the atmosphere by observing solar spectra. To guide the sunlight into the FTS, a solar tracker has to be placed outside. This device needs high-quality optical mirrors with good reflectance in the near and mid-infrared.<br><br>More and more FTS stations are operated in remote locations with harsh environments. Optical mirrors are usually made for laboratory conditions and might not last very long there. At the TCCON site on Ascension Island which is operated by the Max Planck Institute for Biogeochemistry (MPI-BGC), several mirrors from different optical manufacturers were destroyed within weeks.<br><br>To continue operation, the MPI-BGC had to develop rugged mirrors that could sustain the harsh conditions for months or even years. While commercially available mirrors are typically made from a substrate covered with a thin reflective coating, these rugged mirrors were made from stainless steel with no additional coating. Except for their lower reflectance (which can easily be compensated for), their optical properties are comparable to existing mirrors. However, their rugged design makes them mostly immune to corrosion and scratching. Unlike most coated mirrors, they can also be cleaned easily.http://www.atmos-meas-tech.net/9/2381/2016/amt-9-2381-2016.pdf |
| spellingShingle | D. G. Feist S. G. Arnold F. Hase D. Ponge Rugged optical mirrors for Fourier transform spectrometers operated in harsh environments Atmospheric Measurement Techniques |
| title | Rugged optical mirrors for Fourier transform spectrometers operated in harsh environments |
| title_full | Rugged optical mirrors for Fourier transform spectrometers operated in harsh environments |
| title_fullStr | Rugged optical mirrors for Fourier transform spectrometers operated in harsh environments |
| title_full_unstemmed | Rugged optical mirrors for Fourier transform spectrometers operated in harsh environments |
| title_short | Rugged optical mirrors for Fourier transform spectrometers operated in harsh environments |
| title_sort | rugged optical mirrors for fourier transform spectrometers operated in harsh environments |
| url | http://www.atmos-meas-tech.net/9/2381/2016/amt-9-2381-2016.pdf |
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