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Analysis of rocks by spectral infrared emission (8 to 25 microns)

Lyon, R. J. P.·1965·Economic Geology

Abstract

Igneous rock types can be roughly determined from the wavelength position of the minima of absorption and emission, or the maxima of reflection, in their infrared spectra. Emission analysis is the method most attractive for field operations, particularly from aircraft or orbiting vehicles. The usefulness of the method is severely limited by surface roughness, small particle size (less than 50 microns), and physical discontinuities within the emitting surface.

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Metadata

Authors
Lyon, R. J. P.
Venue
Economic Geology
Published
1965-06-01
Volume
60
Issue
4
Pages
715-736
ISSN
  • 0361-0128 (ISSN-L)
  • 1554-0774
OpenAlex
W2123859765
Cited by
259
References
0
FWCI
9.27
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Analysis of rocks by spectral infrared emission (8 to 25 microns). https://app.cochat.ai/papers/10.2113/gsecongeo.60.4.715
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Lyon, R. J. P. (1965). Analysis of rocks by spectral infrared emission (8 to 25 microns). Economic Geology. https://doi.org/10.2113/gsecongeo.60.4.715

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.