Computer Science
Scientific paper
Oct 1974
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974lssf.nasa..453a&link_type=abstract
"In its Lunar Soil from the Sea of Fertility (NASA-TT-F-15881) p 453-467 (SEE N75-11814 02-91) Transl. into ENGLISH from the bo
Computer Science
Infrared Spectra, Lunar Soil, Microstructure, Chemical Composition, Lunar Maria, Lunar Surface, Lunik 16 Lunar Probe, Minerals
Scientific paper
Spectra of reflection, emission, and transmission of regolith returned by the Luna 16 automatic station were investigated in the 1.8-13 micrometers region. A reflection maximum was shown to be present in the region 3 to 5 micrometer, along with a corresponding minimum in the emission coefficient. The spectra were interpreted based on a comparison of the optical properties with the chemical and structural properties of the regolith. The regolith in the entire array of properties in the infrared region differs appreciably from terrestrial objects. Spectra of diffuse reflection and the spectra at angles of incidence 0 deg and angles of reflection 15 and 30 deg with samples of the regolith returned by the Apollo 11 and Apollo 12 missions revealed a similarity of the infrared reflection characteristics of the regolith from different lunar mare regions.
Akhmanova M. V.
Dementyev B. V.
Kartashev A. V.
Karyakin A. V.
Markov M. N.
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