Characterization and potential for reducing optical resonances in Fourier transform infrared spectrometers of the Network for the Detection of Atmospheric Composition Change (NDACC)

oleh: T. Blumenstock, F. Hase, A. Keens, D. Czurlok, O. Colebatch, O. Garcia, D. W. T. Griffith, M. Grutter, J. W. Hannigan, P. Heikkinen, P. Jeseck, N. Jones, R. Kivi, E. Lutsch, M. Makarova, H. K. Imhasin, J. Mellqvist, I. Morino, T. Nagahama, J. Notholt, I. Ortega, M. Palm, U. Raffalski, M. Rettinger, J. Robinson, M. Schneider, C. Servais, D. Smale, W. Stremme, K. Strong, R. Sussmann, Y. Té, V. A. Velazco

Format: Article
Diterbitkan: Copernicus Publications 2021-02-01

Deskripsi

<p><span id="page1240"/>Although optical components in Fourier transform infrared (FTIR) spectrometers are preferably wedged, in practice, infrared spectra typically suffer from the effects of optical resonances (“channeling”) affecting the retrieval of weakly absorbing gases. This study investigates the level of channeling of each FTIR spectrometer within the Network for the Detection of Atmospheric Composition Change (NDACC). Dedicated spectra were recorded by more than 20 NDACC FTIR spectrometers using a laboratory mid-infrared source and two detectors. In the indium antimonide (InSb) detector domain (1900–5000 <span class="inline-formula">cm<sup>−1</sup></span>), we found that the amplitude of the most pronounced channeling frequency amounts to 0.1 <span class="inline-formula">‰</span> to 2.0 <span class="inline-formula">‰</span> of the spectral background level, with a mean of (<span class="inline-formula">0.68±0.48</span>) <span class="inline-formula">‰</span> and a median of 0.60 <span class="inline-formula">‰</span>. In the mercury cadmium telluride (HgCdTe) detector domain (700–1300 <span class="inline-formula">cm<sup>−1</sup></span>), we find even stronger effects, with the largest amplitude ranging from 0.3 <span class="inline-formula">‰</span> to 21 <span class="inline-formula">‰</span> with a mean of (<span class="inline-formula">2.45±4.50</span>) <span class="inline-formula">‰</span> and a median of 1.2 <span class="inline-formula">‰</span>. For both detectors, the leading channeling frequencies are 0.9 and 0.11 or 0.23 <span class="inline-formula">cm<sup>−1</sup></span> in most spectrometers. The observed spectral frequencies of 0.11 and 0.23 <span class="inline-formula">cm<sup>−1</sup></span> correspond to the optical thickness of the beam splitter substrate. The 0.9 <span class="inline-formula">cm<sup>−1</sup></span> channeling is caused by the air gap in between the beam splitter and compensator plate. Since the air gap is a significant source of channeling and the corresponding amplitude differs strongly between spectrometers, we propose new beam splitters with the wedge of the air gap increased to at least 0.8<span class="inline-formula"><sup>∘</sup></span>. We tested the insertion of spacers in a beam splitter's air gap to demonstrate that increasing the wedge of the air gap decreases the 0.9 <span class="inline-formula">cm<sup>−1</sup></span> channeling amplitude significantly. A wedge of the air gap of 0.8<span class="inline-formula"><sup>∘</sup></span> reduces the channeling amplitude by about 50 <span class="inline-formula">%</span>, while a wedge of about 2<span class="inline-formula"><sup>∘</sup></span> removes the 0.9 <span class="inline-formula">cm<sup>−1</sup></span> channeling completely. This study shows the potential for reducing channeling in the FTIR spectrometers operated by the NDACC, thereby increasing the quality of recorded spectra across the network.</p>