• Aucun résultat trouvé

NOMAD on ExoMars TGO: Data processing and public release viathe ESA Planetary Science Archive

N/A
N/A
Info
Télécharger
Protected

Academic year: 2021

Partager "NOMAD on ExoMars TGO: Data processing and public release viathe ESA Planetary Science Archive"

Copied!
1
0
0

Chargement.... (Voir le texte intégral maintenant)

Texte intégral

(1)

EPSC Abstracts

Vol. 14, EPSC2020-521, 2020 https://doi.org/10.5194/epsc2020-521 Europlanet Science Congress 2020

© Author(s) 2020. This work is distributed under the Creative Commons Attribution 4.0 License.

NOMAD on ExoMars TGO: Data processing and public release via the ESA Planetary Science Archive

Ian Thomas

1

, Ann Carine Vandaele

1

, Frank Daerden

1

, Bojan Ristic

1

, Yannick Willame

1

, Cedric Depiesse

1

, Shohei Aoki

1,2

, Loic Trompet

1,3

, Justin Erwin

1

, Severine Robert

1,4

, Arianna Piccialli

1

, Lori Neary

1

, Sebastien Viscardy

1

, Jon Mason

5

, Manish Patel

5

, Giancarlo Bellucci

6

, and Jose Juan Lopez- Moreno

7

1

Belgian Institute for Space Aeronomy (BIRA-IASB), Brussels, Belgium

2

Université de Liège, Liège, Belgium

3

University of Namur, Namur, Belgium

4

ICMN, Université Catholique de Louvain, Louvain-la-Neuve, Belgium

5

Open University, Milton Keynes, UK

6

IAPS-INAF, Rome, Italy

7

IAA-CSIC, Granada, Spain

NOMAD is a suite of three spectrometers on-board the ExoMars Trace Gas Orbiter. The spectrometers operate in solar occultation, nadir and limb observing modes, measuring in the infrared (2.2-4.3um in occultation; 2.2-3.8um in nadir) and UV-visible (0.2-0.65um) spectral regions. The nominal science phase began on 21st April 2018; since then NOMAD has collected over one Martian year of data.

Due to the very high spectral and spatial resolution of NOMAD, an enormous amount of data has already been generated - including tens of millions of solar occultation and nadir spectra - which currently total around four terabytes and are spread across almost half a million files. To serve the scientific community, all calibrated data will eventually be made publicly available in PDS4 format via the ESA Planetary Science Archive at

At the time of writing, the NOMAD data collection has successfully passed peer review, and data from two of the three channels will be available very shortly. This first release will consist of: 1) infrared solar occultation data; 2) UV-visible solar occultation data; and 3) UV-visible nadir data.

The infrared nadir and infrared and UV-visible limb data will be released later, once the calibration is finalised. In this presentation I will update the scientific community on the current status of the NOMAD PSA archive, including a description of the data and how to start using it.

Powered by TCPDF (www.tcpdf.org)

Références

Télécharger maintenant ( PDF - 1 Page - 126.19 KB )

Documents relatifs

Mars dust properties by means of TGO/NOMAD UVIS and LNO channels data analysis.

We present a method to exploit the combined datasets of the UVIS and LNO channels of NOMAD to study the microphysical properties of Martian dust, allowing to

2. Status of the instrument

The NOMAD (“Nadir and Occultation for MArs Discovery”) spectrometer suite on board the ExoMars Trace Gas Orbiter (TGO) has been designed to investigate the

1. The NOMAD instrument

Nadir and Occultation for Mars Discovery (NOMAD) onboard ExoMars Trace Gas Orbiter (TGO) has started the science measurements on 21 April, 2018.. We present the preliminary

Science objectives of the NOMAD spectrometer on ExoMars Trace Gas Orbiter

NOMAD will continue and extend the monitoring of the major seasonal cycles on Mars which were done by successive space missions in the past decade.. NOMAD will be

Strong seasonal and diurnal variability of water D/H on Mars as revealed with ExoMars/NOMAD

We present the first complete dataset of retrievals of water and D/H vertical profiles derived from the Nadir and Occultation for MArs Discovery (NOMAD) instrument, onboard

The climatology of carbon monoxide on Mars as observed by NOMAD nadir-geometry observations

The nadir-geometry LNO observations taken by the NOMAD instru- ment enable the characterization of the climatology of the column- averaged volume mixing ratio of

Update on CO2 and temperature profiles from NOMAD-SO on boardExoMars TGO

The GEM-Mars GCM provides the a priori profiles of CO 2 local density, pressure and temperature.. We then apply Tikhonov linear regularization on the slant column to derive a

Water vapor vertical profiles on Mars: Results from the first fullMars Year of TGO/NOMAD science operations

The extended dataset also includes the period when the global dust storm occurred the year before; this will allow us to compare the water vapor distributions under global dust