Olivine Laboratory Infrared Absorbance Spectra
Laboratory measurements quantifying the
effect of Fe substituting for Mg in olivine are necessary to
distinguish compositional from temperature, grain size and grain shape
effects in observational data. This dataset presents room temperature
(18-19 degrees Celsius) diamond anvil cell thin film absorption
spectra of a large suite of olivines evenly spaced across Mg and Fe
compositions at infrared wavelengths.
Release Date: 2020-08-14
Data Set Info
| PDS4 version | urn:nasa:pds:gbo.olivines.pitman.lab-spectra::1.0 | Browse | Download (707 KB) |
| PDS3 version | EAR-X-I1485-3-OLIVSPEC-V1.0 | Browse | Download (700 KB) |
The PDS4 bundle was migrated from the PDS3 data set in August 2020. The data content is unchanged.
Use the following citation to reference this data set:
Pitman, K.M., Dijkstra, C., Hofmeister,
A.M., and Speck, A.K. (2020). Olivine Laboratory Infrared Absorbance Spectra
V1.0. urn:nasa:pds:gbo.olivines.pitman.lab-spectra::1.0. NASA Planetary Data System; https://doi.org/10.26033/p5r9-9181.