urn:nasa:pds:context:instrument:pgl.ocean_optics-uvflame 1.3 1.25.0.0 Product_Context Ocean Optics UV-Flame 2026-07-07 1.3 Removed duplicate Internal_Reference entries from Reference_List. 2025-12-24 1.2 Updated schema version. Removed instrument_to_investigation references. Adding missing "facility" references. 2025-01-02 1.1 Updated schema version. Adding missing "investigation" references. Adding missing "facility" references. 2023-08-28 1.0 Initial version. urn:nasa:pds:context:facility:laboratory.pgl instrument_to_facility Planetary Geosciences Laboratory Ocean Optics UV-Flame Spectrometer UV-VNIR The Ocean Optics UV-Flame is located at the Planetary Geosciences Laboratory at the Planetary Science Institute in Tucson, AZ. It is a portable, compact spectrometer designed to measure light across ultraviolet (UV) and visible wavelengths, typically ranging from 200 to 850 nm. It is commonly used for flame spectroscopy applications, where it analyzes the light emitted by flames to identify chemical elements and their concentrations. This spectrometer is equipped with a high-sensitivity detector and can be connected to a computer for data analysis and visualization. It's widely used in research, industrial, and environmental settings to monitor combustion processes or perform chemical analysis.