Spectrum

MIR spectrum of Diopside

Title
MIR spectrum of Diopside
DOI
10.26302/SSHADE/EXPERIMENT_ZED_20241126_01
Data reference
Charlier, Jean (2023): MIR reflectance spectra of mineral standards. SSHADE/DAYSY (OSUG Data Center). Dataset/Spectral Data. https://doi.org/10.26302/SSHADE/EXPERIMENT_ZED_20241126_01
Publications
Database
Experimentalists
Experiment type
laboratory measurement
Type
reflectance factor
Intensity unit
no unit
Instrument
SMIS NEXUS 6700 - confocal reflexion Mid-IR
Standard medium
vacuum
Observation mode
spectrum
Spectral range type(s)
MIR
Valid spectral range(s)
Min - Max ($cm^{-1}$) Sampling ($cm^{-1}$) Resolution ($cm^{-1}$) Position accuracy ($cm^{-1}$) Absorption edge
#1 400.0 - 4000.0 4.0 4.0
Observation geometry
confocal
Observation mode
fixed angles
Incidence angle
0.0°
Emergence angle
0.0°
Azimuth angle
180.0°
Phase angle
0.0°
Resolution illumination
12.0°
Resolution observation
12.0°
Observation mode
single spot
Objective type
x32
Comments
The terrestrial standards were measured in a 60x60 µm window, but the meteorite hibonite was taken with a 40x40 µm window, and the meteorite diopsides / Ca-pyroxenes with a 20x20 µm window.The resolution changes with the wavelength according to the Abbe's equation.
Experiment
MIR reflectance spectra of mineral standards
Date begin
2023-01-01
Release date
2025-01-10 14:16:47+0000 UTC
Version (Date)
#1 (2025-01-10 14:16:47+0000 UTC, Updated: 2025-01-13 07:59:28+0000 UTC)
History
Date Mode Version Status Comments
2024-12-04 17:14:16+0000 UTC first import #1 valid version
Analysis
The reflectance factor spectrum was obtained by dividing by a reference spectrum collected on a gold surface gold mirror under the same observation conditions.
Quality flag
4
Validator(s)