NOMAD, an Integrated Suite of Three Spectrometers for the ExoMars Trace Gas Mission: Technical Description, Science Objectives and Expected Performance
書誌事項
- 公開日
- 2018-06-19
- 資源種別
- journal article
- 権利情報
-
- https://creativecommons.org/licenses/by/4.0
- DOI
-
- 10.1007/s11214-018-0517-2
- 公開者
- Springer Science and Business Media LLC
この論文をさがす
説明
The NOMAD (“Nadir and Occultation for MArs Discovery”) spectrometer suite on board the ExoMars Trace Gas Orbiter (TGO) has been designed to investigate the composition of Mars’ atmosphere, with a particular focus on trace gases, clouds and dust. The detection sensitivity for trace gases is considerably improved compared to previous Mars missions, compliant with the science objectives of the TGO mission. This will allow for a major leap in our knowledge and understanding of the Martian atmospheric composition and the related physical and chemical processes. The instrument is a combination of three spectrometers, covering a spectral range from the UV to the mid-IR, and can perform solar occultation, nadir and limb observations. In this paper, we present the science objectives of the instrument and explain the technical principles of the three spectrometers. We also discuss the expected performance of the instrument in terms of spatial and temporal coverage and detection sensitivity.© 2018, The Author(s).
The NOMAD experiment is led by the Royal Belgian Institute for Space Aeronomy (IASB-BIRA), assisted by Co-PI teams from Spain (IAA-CSIC), Italy (INAF-IAPS), and the United Kingdom (Open University). This project acknowledges funding by the Belgian Science Policy Office (BELSPO), with the financial and contractual coordination by the ESA Prodex Office (PEA 4000103401, 4000121493), by Spanish MICINN through its Plan Nacional and by European funds under grant ESP2015-65064-C2-1-P (MINECO/FEDER), as well as by UK Space Agency through grants ST/R005761/1, ST/P001262/1, ST/R001405/1 and ST/R001405/1 and Italian Space Agency through grant 2018-2-HH.0. The research was performed as part of the >Excellence of Science> project >Evolution and Tracers of Habitability on Mars and the Earth> (30442502). SA acknowledge support from the FNRS, Be.
Open Access This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/)
収録刊行物
-
- Space Science Reviews
-
Space Science Reviews 214 (5), 80-, 2018-06-19
Springer Science and Business Media LLC
- Tweet
キーワード
- Solar occultation
- Physique atomique et moléculaire
- Dust
- 520
- ExoMars
- Nadir observations
- [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
- [SDU.ASTR.IM] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
- Spectroscopie [électromagnétisme, optique, acoustique]
- Mars atmosphere
- Visible
- Chimie
- Infrared
- Methane
- Composition; Dust; ExoMars; Infrared; Mars atmosphere; Methane; Nadir observations; Solar occultation; Spectroscopy; Ultraviolet; Visible
- Spectroscopy
- Composition
- Ultraviolet
詳細情報 詳細情報について
-
- CRID
- 1360567181389174528
-
- ISSN
- 15729672
- 00386308
-
- 資料種別
- journal article
-
- データソース種別
-
- Crossref
- KAKEN
- OpenAIRE
