Physics
Scientific paper
Mar 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979jgr....84.1025g&link_type=abstract
Journal of Geophysical Research, vol. 84, Mar. 10, 1979, p. 1025-1030.
Physics
1
Ferromagnetic Resonance, Lunar Soil, Soil Science, Lunar Composition, Quantitative Analysis, Samples, Samples, Lunar, 65701, 67701, 66031, 12001, 74121, Soils, Ferromagnetic Resonance, Moon, Exposure Ages, Vesicles, Spherules, Absorption Spectra, Particles, Anistrophy, Magnetic Properties, Apollo 16, Regolith, Spectrometers, Spectrum
Scientific paper
Quantitative ferromagnetic resonance (FMR) measurements at 9.5 and 35 GHz were made on lunar fines in order to determine the amount of single domain FE(0) and to ascertain the effect of sample quantity on the results of these experiments. Samples containing more than 10 micrograms of Fe(0) in an X-band TE(104) cavity, or more than 0.11 micrograms in a Ka-band cavity can cause errors greater than 1% in the quantitative determination of Fe(0), as well as cause anomalous broadening of the FMR line. Theoretical calculations were derived to show this effect which results from a nonlinear response of the FMR experiment with the sample quantity. Using samples of nominal weights, the amount of Fe(0) determined at 34 GHz was 1.1-1.8 times greater than at 9.5 GHz, while the linewidths increased by a factor of 1.2. As the particle size increases, the ratio of Fe(0) determined at 35 GHz to that determined at 9.5 GHz increases, suggesting that the additional iron is due to larger spheroidal particles which change from multidomain to single domain at the larger fields.
Cirlin E. H.
Crowe H. R.
Goldberg I. B.
Housley R. M.
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