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Detailed Reference Information |
Lucey, P.G., Blewett, D.T. and Jolliff, B.L. (2000). Lunar iron and titanium abundance algorithms based on final processing of Clementine ultraviolet-visible images. Journal of Geophysical Research 105: doi: 10.1029/1999JE001117. issn: 0148-0227. |
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A one-dimensional model of meridional water vapor transport is used to evaluate the factors that control the spatial and temporal variations of oxygen (Δ 18O) and hydrogen (ΔD) isotopic ratios in global precipitation. The model extends Rayleigh descriptions of isotopes in precipitation by including (1) effects of recharge to air masses by evaporation and (2) horizontal transport by both eddy fluxes and advection. Globally, spatial variations in precipitation Δ 18O and ΔD depend on the ratio of evaporation to the product of horizontal moisture flux and horizontal temperature gradient. At low latitudes, where this ratio is large, precipitation Δ 18O and ΔD are closely tied to the isotopic ratios of oceanic evaporation. At high latitudes the ratio is small, and Δ 18O and ΔD are controlled by the ratio of advective transport to eddy transport. Transport by eddy fluxes induces less fractionation than transport by advection, resulting in a smaller gradient of isotopic ratios with temperature. The model-predicted temporal relationships between Δ 18O (or ΔD) of Antarctic precipitation and temperature do not necessarily coincide with the modern spatial relationship and depend strongly on the proximity of the precipitation site to the ocean evaporation source. Sensitivity of Δ 18O to temporal changes in local surface temperature is low at coastal sites and increases with distance inland. These results suggest a possible explanation of the apparent discrepancy between borehole temperature inversion estimates of glacial temperatures and temperatures inferred from the modern spatial Δ 18O-surface temperature relationship. ¿ 2000 American Geophysical Union |
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Abstract |
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Keywords
Planetology, Solid Surface Planets, Composition, Planetology, Solid Surface Planets, Remote sensing, Planetology, Solid Surface Planets, Surface materials and properties, Planetology, Solar System Objects, Moon |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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