A dataset provided by the European Space Agency

NOMAD

NOMAD is a 3-channel spectrometer designed to perform high-sensitivity orbital identification of atmospheric components, concentration and temperature, their sources, loss, and cycles. It measures the sunlight reflected from the surface and atmosphere of Mars, and analyses its wavelength spectrum to identify the components of the Martian atmosphere that may suggest a biological source.
This spectrometer consists of three channels: solar occultation (SO), limb nadir and occultation (LNO), and ultraviolet and visible spectrometer (UVIS). The first two channels work in the infrared (2.2 to 4.3 μm); the third channel (UVIS) works in the UV-visible range (0.2 to 0.65 μm), which is able to measure ozone, sulphuric acid, and perform aerosol studies. Measurements are carried out during solar occultation, i.e. the instrument points toward the sunset as the orbiter moves toward or away the dark side of Mars. It also measures in nadir mode, i.e. looking directly at the sunlight reflected from the surface and atmosphere of Mars. The Principal Investigator is Ann Carine Vandaele, from the Belgian Institute for Space Aeronomy (BIRA).

The Calibrated_Data Collection

The Calibrated data collection contains science data from the instrument which is processed to the calibrated stage, and this represents the highest level of processing within the PSA. Calibrated data is defined as having all instrument related artifacts removed. The data are delivered to the PSA from BIRA and any data older than six months is immediately released publically. (Note all LNO data is not yet publically available so can not be downloaded from any time period) Physically the collection is organised by science phase, then orbit range in groups of 100 orbits, then orbit. Different data types e.g. HK plus science from different channels may be mixed in this time related directory. A description of the calibrated data products can be found in the NOMAD Experiment to Archive ICD (EAICD). This can be found under documents in the user interface or via the Document Collection in the PSA ftp distribution. A quick start guide can also be found at:

ExoMars 2016 Mission Overview

Mission Phases