938 resultados para United States artillery. 102d field artillery. Battery E., 1917-1919.
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Lettered on cover: Roster of Maine in the World War.
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Issues for <, Jan. 1895>-June 1922 called also whole no. <14>-190.
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Mode of access: Internet.
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"Privately published."
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Mode of access: Internet.
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Mode of access: Internet.
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Printed for the use of the Committee on Agriculture and Forestry.
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Mode of access: Internet.
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"Committee charged with the compliation ... Major W. A Sawtell ... Capt. Frank R. Jeffrey ... Lieut. W. S. Griscom ... Lieut. Wm. R. Wright ... brigade historian."--p. 371.
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Includes bibliography.
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Errata slip inserted.
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"March 1980."
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Mode of access: Internet.
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Potential Desiccation Polygons (PDPs), tens to hundreds of meters in size, have been observed in numerous regions on Mars, particularly in ancient (>3Gyr old) terrains of inferred paleolacustrine/playa geologic setting, and in association with hydrous minerals such as smectites. Therefore, a better understanding of the conditions in which large desiccation polygons form could yield unique insight into the ancient climate on Mars. Many dried lakebeds/playas in western United States display large (>50m wide) desiccation polygons, which we consider to be analogues for PDPs on Mars. Therefore, we have carried out fieldwork in seven of these dried lakes in San Bernardino and the Death Valley National Park regions complemented with laboratory and spectral analysis of collected samples. Our study shows that the investigated lacustrine/playa sediments have (a) a soil matrix containing 40-75% clays and fine silt (by volume) where the clay minerals are dominated by illite/muscovite followed by smectite, (b) carbonaceous mineralogy with variable amounts of chloride and sulfate salts, and significantly, (c) roughly similar spectral signatures in the visible-near-infrared (VIS-NIR) range. We conclude that the development of large desiccation fractures is consistent with water table retreat. In addition, the comparison of the mineralogical to the spectral observations further suggests that remote sensing VIS-NIR spectroscopy has its limitations for detailed characterization of lacustrine/playa deposits. Finally, our results imply that the widespread distribution of PDPs on Mars indicates global or regional climatic transitions from wet conditions to more arid ones making them important candidate sites for future in situ missions.