Solid Spectroscopy Hosting Architecture of Databases and Expertise
EXPERIMENT_CF_20200813_000 : VIS-NIR reflectance spectra of binary mixtures of silicon dioxide (SiO2) particles (0.5 - 10 µm) and Juniper charcoal particles (less than 50 µm) | BYPASS database
EXPERIMENT_CF_20200723_000 : Vis BRDF of binary mixtures of silicon dioxide (SiO2) particles (0.5 - 10 µm) and Juniper charcoal particles (less than 50 µm) | BYPASS database
EXPERIMENT_JC_20220615_001 : Y K edge XAS transmission and XAS fluorescence of Yttrium components at 20K | FAME database
EXPERIMENT_LB_20221102_001 : Average Raman spectra (λ = 532 nm) obtained on fragments of individual particles and aggregates from Chamber A and Chamber C Ryugu samples (Hayabusa2 mission) | GhoSST database
EXPERIMENT_LB_20231006_001 : Vis-NIR reflectance spectra (i = 0°, e = 30°) of three raw chips of the Orgueil CI chondrite under ambient conditions | GhoSST database
BANDLIST_RAMAN_alpha_Na2CaCO3-2 : Raman bandlist of synthetic alpha-Na2Ca(CO3)2 (Nyerereite)
BANDLIST_RAMAN_beta_K2CaCO3-2 : Raman bandlist of synthetic beta-K2Ca(CO3)2 (Fairchildite)
BANDLIST_RAMAN_alpha_K2CaCO3-2 : Raman bandlist of synthetic alpha-K2Ca(CO3)2 (Bütschliite)
BANDLIST_RAMAN_alpha_Na2CaCO3-2 : Raman bandlist of synthetic alpha-Na2Ca(CO3)2
BANDLIST_RAMAN_Nyerereite : Raman bandlist of natural Nyerereite
SSHADE is an interoperable Solid Spectroscopy database infrastructure (www.sshade.eu) providing spectral and photometric data obtained by various spectroscopic techniques over the whole electromagnetic spectrum from gamma to radio wavelengths, through X, UV, Vis, IR, and mm ranges. The measured samples include ices, minerals, rocks, organic and carbonaceous materials... and also liquids. They are either synthesized in the laboratory, natural terrestrial analogs collected or measured in the field, or extraterrestrial samples collected on Earth or on planetary bodies: (micro-)meteorites, IDPs, lunar soils...
SSHADE contains a set of specialized databases from various research groups, mostly from Europe. It is developed under the H2020 European programs* "Europlanet 2020 RI" and now "Europlanet 2024 RI" with the help of OSUG, CNRS/INSU, IPAG, and CNES. It is hosted by the OSUG data center / Université Grenoble Alpes, France. It can also be searched through the Virtual European Solar and Planetary Access (VESPA) virtual observatory.
(*) Europlanet 2020 RI and Europlanet 2024 RI have received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreements N°654208 and N°871149