GhoSST Samples and Spectra
Data currently in the GhoSST database
Near/Mid/Far IR transmission or absorbance spectra of ices:
- NIR: NO, NO2
- MIR: H2O Ih, CH4-II, C6H6
- FIR: H2O Ih,
Vis, Near/Mid/Far IR absorption coefficient or optical constants of ices
- Vis: CH4-I & II, CH4 liq
- NIR: H2O Ih & liq, α- & β-N2, α-CO, CO in β-N2, CO2, CH4-I & II, CH4 liq, HC3N, SO2
- MIR: H2O Ih & Ia, NH3am, CH3OH am, CO, CO2, CH4-I & II, C2H4, C2H6, C6H6, H2S am, SO2
- FIR: H2O Ih & Ia, NH3am, NH3cr, CO2
Vis-NIR bidirectionnal reflectance spectra + spectral BRDF of surfaces:
- Ices: wet snow
- Minerals: Palagonite JSC Mars-1 (+H2O ads), Smectite STx-1, Na-Montmorillonite SWy-1, Smectite SWy-2 (+H2O ads)
Near/Mid/Far IR transmission or absorbance spectra of minerals:
- NIR:
- MIR: Portlandite (+CO2)
- FIR:
Mid-IR transmission or absorbance spectra of Cosmo-materials:
- Meteorites: Allende, ALH83100, ALH84044, ALH85002, Bells, Boriskino, DOM03183, DOM08003, EET92002, EET92042, EET96029, Essebi, GRA06100, GRA95229, GRO03116, GRO95577, Grosnaja, Ivuna, Kaba, LAP02342, LEW85311, LEW87022, LON94101, Maralinga, MCY05230, MET00426, MIL07700, Mokoia, Murchison, Nogoya, Niger, Orgueil, PCA02010, PCA91008, PCA91082, QUE97990, QUE99177, QUE99355, RBT04133, Renazzo, Vigarano, WIS91600
- IDPs: DC06-09-21 (Sc-AMM), DC06-09-54/74/83/110/157/158/164/194/248 (Fg-AMM)
Raman spectra:
- Meteorites: Allende, Axtell, Bali, Efremovka, Kaba, Leoville, Mokoia, Vigarano
Types of samples & spectra measured at IPAG (and formerly at LGGE & LPG) for the GhoSST database
(to be ingested)
Near-IR to Mid/Far IR transmission spectra of:
- ices, minerals/rocks, organic molecules and materials, optical materials
- meteorites (mostly chondrites so far: in bulk and matrices) and Antarctic MicroMeteorites (in bulk)
Near-IR to Mid/Far IR optical constants and bandlists of:
- ices, organic molecules
Vis-NIR bidirectionnal reflectance spectra + spectral BRDF of surfaces:
- snows, ices, sulfur, …
- minerals/rocks, salts, …
- natural and synthetic organic materials, …
NIR+MIR microscopic spectra of:
- carbonaceous materials,
- minerals/rocks
UV-Vis Raman + Fluorescence spectra of:
- organic molecules,
- natural et synthetic carbonaceous materials,
- meteorites (mostly chondrites) and Antarctic MicroMeteorites
Fe-XANES spectra of:
- chondrites