Spectrum

MIR spectrum of an irradiated area of the Murchison meteorite chip at 4 keV

Title
MIR spectrum of an irradiated area of the Murchison meteorite chip at 4 keV
DOI
10.26302/SSHADE/EXPERIMENT_ZED_20240701_01
Data reference
Lantz, Cateline (2022): MIR spectra of carbonaceous chondrites irradiated by He+ ions. SSHADE/DAYSY (OSUG Data Center). Dataset/Spectral Data. https://doi.org/10.26302/SSHADE/EXPERIMENT_ZED_20240701_01
Publications
Database
Experimentalists
Experiment type
laboratory measurement
Type
normalized reflectance
Intensity unit
no unit
Reference position
948.8059 cm1
Instrument
SMIS Cary 670 - confocal reflection Mid-IR
Standard medium
vacuum
Observation mode
spectrum
Spectral range type(s)
MIR
Valid spectral range(s)
Min - Max (cm1) Sampling (cm1) Resolution (cm1) Position accuracy (cm1) Absorption edge
#1 800.0 - 1250.0 4.0 1.0
Observation geometry
specular
Observation mode
fixed angles
Incidence angle
0.0°
Emergence angle
0.0°
Azimuth angle
180.0°
Phase angle
0.0°
Comments
numerical aperture of 0.62
Observation mode
averaged
Objective type
x15
Image size
13000.0 x 13000.0 μm
Comments
The resolution changes with the wavelength according to the Abbe's equation.
Name
Murchison chip
Comments
Area of the pellet irradiated by He+ ions at 20 keV and a total fluence of 6.1016ions.cm2
Experiment
MIR spectra of carbonaceous chondrites irradiated by He+ ions
Date begin
2024-01-01
Release date
2025-01-22 17:12:11+0000 UTC
Version (Date)
#1 (2025-01-22 17:12:11+0000 UTC, Updated: 2025-01-28 12:51:29+0000 UTC)
History
Date Mode Version Status Comments
2024-12-17 15:12:56+0000 UTC first import #1 valid version 2024-07-01: First import
Analysis
A baseline correction has been performed and then the spectrum has been normalized by adjusting the height of the maximum of the Si-O band to 1 and the band minimum (Christensen feature) to 0. Some reflectance features are present for wavenumber below 350 cm-1, they are due to non perfect compensation of athmospheric contribution.
Quality flag
4
Validator(s)