دورية أكاديمية
Optical and radiometric models of the NOMAD instrument part II: the infrared channels - SO and LNO.
| العنوان: | Optical and radiometric models of the NOMAD instrument part II: the infrared channels - SO and LNO. |
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| المؤلفون: | Thomas IR, Vandaele AC, Robert S, Neefs E, Drummond R, Daerden F, Delanoye S, Ristic B, Berkenbosch S, Clairquin R, Maes J, Bonnewijn S, Depiesse C, Mahieux A, Trompet L, Neary L, Willame Y, Wilque V, Nevejans D, Aballea L, Moelans W, De Vos L, Lesschaeve S, Van Vooren N, Lopez-Moreno JJ, Patel MR, Bellucci G |
| مؤلفون مشاركون: | NOMAD Team |
| المصدر: | Optics express [Opt Express] 2016 Feb 22; Vol. 24 (4), pp. 3790-805. |
| نوع المنشور: | Journal Article; Research Support, Non-U.S. Gov't |
| اللغة: | English |
| بيانات الدورية: | Publisher: Optica Publishing Group Country of Publication: United States NLM ID: 101137103 Publication Model: Print Cited Medium: Internet ISSN: 1094-4087 (Electronic) Linking ISSN: 10944087 NLM ISO Abbreviation: Opt Express Subsets: PubMed not MEDLINE |
| أسماء مطبوعة: | Publication: Washington, DC : Optica Publishing Group Original Publication: Washington, DC : Optical Society of America, 1997- |
| مستخلص: | NOMAD is a suite of three spectrometers that will be launched in 2016 as part of the joint ESA-Roscosmos ExoMars Trace Gas Orbiter mission. The instrument contains three channels that cover the IR and UV spectral ranges and can perform solar occultation, nadir and limb observations, to detect and map a wide variety of Martian atmospheric gases and trace species. Part I of this work described the models of the UVIS channel; in this second part, we present the optical models representing the two IR channels, SO (Solar Occultation) and LNO (Limb, Nadir and Occultation), and use them to determine signal to noise ratios (SNRs) for many expected observational cases. In solar occultation mode, both the SO and LNO channel exhibit very high SNRs >5000. SNRs of around 100 were found for the LNO channel in nadir mode, depending on the atmospheric conditions, Martian surface properties, and observation geometry. |
| فهرسة مساهمة: | Investigator: AC Vandaele; JJ Lopez Moreno; G Bellucci; M Patel; M Allen; F Altieri; S Aoki; S Bolsée; T Clancy; E Cloutis; F Daerden; C Depiesse; A Fedorova; V Formisano; B Funke; D Fussen; M Garcia-Comas; A Geminale; JC Gérard; D Gillotay; M Giuranna; F Gonzalez-Galindo; N Ignatiev; J Kaminski; O Karatekin; Y Kasaba; F Lefèvre; S Lewis; M López-Puertas; M López-Valverde; A Mahieux; J Mason; J McConnell; M Mumma; L Neary; E Neefs; R Novak; E Renotte; S Robert; G Sindoni; M Smith; IR Thomas; S Trokhimovsky; J Vander Auwera; G Villanueva; J Whiteway; Y Willame; V Wilquet; M Wolff; G Alonso-Rodrigo; B Aparicio del Moral; P Barzin; A BenMoussa; S Berkenbosch; D Biondi; S Bonnewijn; P Candini Gian; R Clairquin; J Cubas; S Delanoye; B Giordanengo; S Gissot; A Gomez; JJ Zafra; M Leese; J Maes; E Mazy; A Mazzoli; J Meseguer; R Morales; A Orban; Mdel C Pastor-Morales; I Perez-Grande; B Ristic; J Rodriguez-Gomez; B Saggin; V Samain; A Sanz Andres; R Sanz; JF Simar; T Thibert |
| تواريخ الأحداث: | Date Created: 20160624 Date Completed: 20160709 Latest Revision: 20190516 |
| رمز التحديث: | 20231215 |
| DOI: | 10.1364/oe.24.003790 |
| PMID: | 27333621 |
| قاعدة البيانات: | MEDLINE |
Full Text Finder | تدمد: | 1094-4087 |
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| DOI: | 10.1364/oe.24.003790 |