Planetary

Global Emission Spectra

The GlobES application allows to ingest climatological data from a variety of General Circulation Models (GCM) and to accurately synthesize planetary spectra. The 3D and temporal atmospheric data is aggregated and mapped into a 2D projected observationally grid that is fed to the Planetary Spectrum Generator (PSG). More information here.
 

Variable Tsurf Temperature winds Weight Pressure CO2 N2 O2 CO H2O O3 Dust WaterIce Dust_size WaterIce_sizeNone Altitude Surface 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 Topography Earth's topographyMars' topographyNone   Show winds 2D Interpolation Show POIs   GCM data Select a source Upload PSG/GCM file CAM_Aqua Earth_MERRA Earth_json LMD_THAI Mars_GEM Mars_MCD ROCKE3D UM_THAI Date/time (UT) Load data

Atmospheric data: Mars Climate Database v5.3 (Millour+2015) Variable (100 to 400 m/s)

Parameters of the spectroscopic 3D synthesis The parameters of the (exo)planet and its host star are as defined in the Target and Geometry section of PSG. This also includes the observational conditions (e.g., distance to the object, inclination, phase), while in this section, the user can also quickly define observational mode (i.e., transit, direct imaging and phase). However, it is important that the user verifies the parameters in the Target and Geometry section. The atmosphere and surface information will be as defined in the Atmosphere and Surface section, while the algorithm will use the 3D atmospheric data defined in this section to establish the vertical profiles at each location.   Geometry    Current: Disk emission   Primary transit Disk emission Phase:   Atmosphere   Molecules: CO2,N2,O2,CO,H2O,O3   Aerosols: Dust,WaterIce  Change   Instrument     Wavelength: 2702.561073-2742.447073 cm, resolution 32000 RP   Change   Spatial binning   Higher binning leads to faster calculations, yet degraded regional details

Generate 3D Spectra