Compositional dependence of infrared absorption spectra of crystalline silicate: II. Natural and synthetic olivines

By C. Koike, H. Chihara, A. Tsuchiyama, H. Suto, H. Sogawa, Hiromichi Okuda. 2003

160 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science, Geophysics

View Paper: https://www.semanticscholar.org/paper/dc2f57cd42c8a9583200067ffb0ed6dc3ea8eee0

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. W. Koeppen
2. V. Hamilton
3. B. Sargent
4. D. Watson
5. G. Sloan
6. W. Forrest
7. J. Najita
8. Michael Jura

In Atmospheric Science

1. W. Koeppen
2. V. Hamilton

In Geophysics

1. W. Koeppen
2. V. Hamilton

Citations in the corpus

• Global distribution, composition, and abundance of olivine on the surface of Mars from thermal infrared data (2008, background): “The Mg/ Fe content of olivine within this series is denoted by its forsteritenumber(Fo#),whichisdefinedasmolarMg/(Mg+ Fe) � 100.Spectralvariationinthermalinfraredobservations of olivine has been documented by several authors and correlates with its Mg/Fe content [e.g., Duke and Stephens, 1964; Burns”
• Spitzer IRS Spectroscopy of IRAS-discovered Debris Disks (2006, methodology): “In these cases, we modeled the sub-micron dust components using laboratory measured opacities of crushed forsterite (Mg2SiO4, Koike et al. 2003) and enstatite (Mg0.”
• Thermal infrared (vibrational) spectroscopy of Mg–Fe olivines: A review and applications to determining the composition of planetary surfaces (2010, methodology): “3a illustrates absorption band positions and trends using band positions derived from the transmission spectra of Duke and Stephens (1964), Burns and Huggins (1972), Salisbury et al. (1991b), Koike et al. (2003), and Hofmeister and Pitman (2007).”