Spectroscopy of synthetic Mg‐Fe pyroxenes I: Spin‐allowed and spin‐forbidden crystal field bands in the visible and near‐infrared

By R. Klima, Carle M. Pieters, Melinda Darby Dyar. 2007

293 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/d12f1753843f94263f2ebfc8051cb55564a2fb2f

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In Astronomy and Astrophysics

1. Patrick Pinet
2. James F. Bell III
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1. Paul Mann
2. Edward A. Cloutis

Citations in the corpus

• Near-infrared spectra of ferrous mineral mixtures and methods for their identification in planetary surface spectra (2014, background): “The complex 1 lm band is actually a combination of two or three distinct bands centered near 0.94, 1.03, and 1.15 lm due to Fe2+ in both the M1 and M2 sites (Schade et al., 2004; Klima et al., 2007, 2011b).”
• A new systematic approach using the Modified Gaussian Model: Insight for the characterization of chemical composition of olivines, pyroxenes and olivine-pyroxene mixtures (2011, methodology): “9a: 998 case of synthetic pyroxenes (Klima et al., 2007): (1) refers to Enstatite (En97Fs2) (RELAB C1DL64A), (2) 999 refers to Ferrosilite (En0Fs100) endmember (RELAB C1DL61A).”