Minimum Noise Fraction Analysis of TGO/NOMAD LNO Channel High-Resolution Nadir Spectra of Mars
| dc.contributor.author | Oliva, F. | |
| dc.contributor.author | D’Aversa, E. | |
| dc.contributor.author | Bellucci, G. | |
| dc.contributor.author | Carrozzo, F.G. | |
| dc.contributor.author | Ruiz Lozano, L. | |
| dc.contributor.author | Karatekin, Ö. | |
| dc.contributor.author | Daerden, F. | |
| dc.contributor.author | Thomas, I.R. | |
| dc.contributor.author | Ristic, B. | |
| dc.contributor.author | Patel, M.R. | |
| dc.contributor.author | Lopez-Moreno, J.J. | |
| dc.contributor.author | Vandaele, A.C. | |
| dc.contributor.author | Sindoni, G. | |
| dc.date | 2023 | |
| dc.date.accessioned | 2023-12-18T12:56:25Z | |
| dc.date.available | 2023-12-18T12:56:25Z | |
| dc.identifier.uri | https://orfeo.belnet.be/handle/internal/11224 | |
| dc.description | NOMAD is a suite of spectrometers on the board of the ESA-Roscosmos Trace Gas Orbiter (TGO) spacecraft and is capable of investigating the Martian environment at very high spectral resolution in the ultraviolet–visible and infrared spectral ranges by means of three separate channels: UVIS (0.2–0.65 μm), LNO (2.2–3.8 μm), and SO (2.3–4.3 μm). Among all channels, LNO is the only one operating at infrared wavelengths in nadir-viewing geometry, providing information on the whole atmospheric column and on the surface. Unfortunately, the LNO data are characterized by an overall low level of signal-to-noise ratio (SNR), limiting their contribution to the scientific objectives of the TGO mission. In this study, we assess the possibility of enhancing LNO nadir data SNR by applying the Minimum Noise Fraction (MNF), a well-known algorithm based on the Principal Components technique that has the advantage of providing transform eigenvalues ordered with increasing noise. We set up a benchmark process on an ensemble of synthetic spectra in order to optimize the algorithm specifically for LNO datasets. We verify that this optimization is limited by the presence of spectral artifacts introduced by the MNF itself, and the maximum achievable SNR is dependent on the scientific purpose of the analysis. MNF application study cases are provided to LNO data subsets in the ranges 2.627–2.648 μm and 2.335–2.353 μm (spectral orders 168 and 189, respectively) covering absorption features of gaseous H2O and CO and CO2 ice, achieving a substantial enhancement in the quality of the observations, whose SNR increases up to a factor of 10. While such an enhancement is still not enough to enable the investigation of spectral features of faint trace gases (in any case featured in orders whose spectral calibration is not fully reliable, hence preventing the application of the MNF), interesting perspectives for improving retrieval of both atmospheric and surface features from LNO nadir data are implied. | |
| dc.language | eng | |
| dc.title | Minimum Noise Fraction Analysis of TGO/NOMAD LNO Channel High-Resolution Nadir Spectra of Mars | |
| dc.type | Article | |
| dc.subject.frascati | Physical sciences | |
| dc.audience | Scientific | |
| dc.subject.free | noise reduction | |
| dc.subject.free | minimum noise fraction technique | |
| dc.subject.free | infrared spectroscopy | |
| dc.subject.free | Mars | |
| dc.subject.free | atmosphere | |
| dc.subject.free | surface | |
| dc.source.title | Remote Sensing | |
| dc.source.volume | 15 | |
| dc.source.issue | 24 | |
| dc.source.page | 15253-15267 | |
| Orfeo.peerreviewed | Yes | |
| dc.identifier.doi | 10.3390/rs15245741 | |
| dc.identifier.url |
