From: Dennis Schafroth Date: Thu, 18 Aug 2011 16:24:38 +0000 (+0200) Subject: Correct Primo data X-Git-Tag: v1.5.7~3 X-Git-Url: http://sru.miketaylor.org.uk/?a=commitdiff_plain;h=398fafc67effab14293bc23f143e16ec915aec63;p=pazpar2-moved-to-github.git Correct Primo data --- diff --git a/test/primo.xml b/test/primo.xml index 400a259..a4f32a0 100644 --- a/test/primo.xml +++ b/test/primo.xml @@ -1,29 +1,2878 @@ - - - - - - - - - - - - 17813302 - english - 0036-8075 - 00368075 - MEDLINE - medline - nlm_medline - MEDLINE - medline - nlm_medline - - - - - - - - + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + + 21294516 + medline + TN_medline21294516 + XML + Other + + + article + Glassy nature of water in an ultraconfining disordered material: the case of calcium-silicate-hydrate + Youssef, Mostafa ; Pellenq, Roland J-M ; Yildiz, Bilge + Journal of the American Chemical Society, Mar, 2011, Vol.133(8), p.2499-510 + E-ISSN: 1520-5126 ; ISSN: 0002-7863 ; PMID: 21294516]]> + Calcium -- chemistry; Silicates -- chemistry; Water -- chemistry + We present the structural and dynamic nature of water ultraconfined in the quasi-two-dimensional nanopores of the highly disordered calcium-silicate-hydrate (C-S-H), the major binding phase in cement. Our approach is based on classical molecular simulations. We demonstrate that the C-S-H nanopore space is hydrophilic, particularly because of the nonbridging oxygen atoms on the disordered silicate chains which serve as hydrogen-bond acceptor sites, directionally orienting the hydrogen atoms of the interfacial water molecules toward the calcium-silicate layers. The water in this interlayer space adopts a unique multirange structure: a distorted tetrahedral coordination at short range up to 2.7 Å, a disordered structure similar to that of dense fluids and supercooled phases at intermediate range up to 4.2 Å, and persisting spatial correlations through dipole-dipole interactions up to 10 Å. A three-stage dynamics governs the mean square displacement (MSD) of water molecules, with a clear cage stage characteristic of the dynamics in supercooled liquids and glasses, consistent with its intermediate-range structure identified here. At the intermediate time scales corresponding to the β-relaxation of glassy materials, coincident with the cage stage in MSD, the non-Gaussian parameter indicates a significant heterogeneity in the translational dynamics. This dynamic heterogeneity is induced primarily because of the heterogeneity in the distribution of hydrogen bond strengths. The strongly attractive interactions of water molecules with the calcium silicate walls serve to constrain their motion. Our findings have important implications on describing the cohesion and mechanical behavior of cement from its setting to its aging. + eng + MEDLINE (NLM) + peer_reviewed + 3 + + + $$Topenurl_article + $$Uhttp://pubmed.gov/21294516$$DView this record at the National Library of Medicine site. + $$Topenurlfull_article + $$Uhttp://primo-central-3.saas.exlibrisgroup.com:1701/primo_library/libweb/aboutMedline.html$$DView the National Library of Medicine Copyright Statement + + + Youssef, Mostafa + Pellenq, Roland J-M + Yildiz, Bilge + Glassy nature of water in an ultraconfining disordered material: the case of calcium-silicate-hydrate. + We present the structural and dynamic nature of water ultraconfined in the quasi-two-dimensional nanopores of the highly disordered calcium-silicate-hydrate (C-S-H), the major binding phase in cement. Our approach is based on classical molecular simulations. We demonstrate that the C-S-H nanopore space is hydrophilic, particularly because of the nonbridging oxygen atoms on the disordered silicate chains which serve as hydrogen-bond acceptor sites, directionally orienting the hydrogen atoms of the interfacial water molecules toward the calcium-silicate layers. The water in this interlayer space adopts a unique multirange structure: a distorted tetrahedral coordination at short range up to 2.7 Å, a disordered structure similar to that of dense fluids and supercooled phases at intermediate range up to 4.2 Å, and persisting spatial correlations through dipole-dipole interactions up to 10 Å. A three-stage dynamics governs the mean square displacement (MSD) of water molecules, with a clear cage stage characteristic of the dynamics in supercooled liquids and glasses, consistent with its intermediate-range structure identified here. At the intermediate time scales corresponding to the β-relaxation of glassy materials, coincident with the cage stage in MSD, the non-Gaussian parameter indicates a significant heterogeneity in the translational dynamics. This dynamic heterogeneity is induced primarily because of the heterogeneity in the distribution of hydrogen bond strengths. The strongly attractive interactions of water molecules with the calcium silicate walls serve to constrain their motion. Our findings have important implications on describing the cohesion and mechanical behavior of cement from its setting to its aging. + Calcium -- chemistry + Silicates -- chemistry + Water -- chemistry + 21294516 + english + medline + medline21294516 + 15205126 + 1520-5126 + 00027863 + 0002-7863 + article + 2011 + Journal of the American Chemical Society + medline + nlm_medline + MEDLINE + medline + nlm_medline + MEDLINE + + + Glassy nature of water in an ultraconfining disordered material: the case of calcium-silicate-hydrate + 2011 + Youssef, Mostafa ; Pellenq, Roland J-M ; Yildiz, Bilge + + + eng + 2011 + Calcium -- chemistry + Silicates -- chemistry + Water -- chemistry + MEDLINE (NLM) + articles + articles + Youssef, Mostafa + Pellenq, Roland J-M + Yildiz, Bilge + Journal of the American Chemical Society + peer_reviewed + 5922086293338298705 + 5 + + + 2 + 2011 + 00027863 + 15205126 + 133 + 8 + 2499 + journal of the american chemical society + glassy nature of water in an ultraconfining disordered material the case of calcium silicate hydrate + glassynatureofwateridrate + 21294516 + mostafayoussef + youssefmostafa + + + Remote Search Resource + no_fulltext + + + 1 + 1 + aggregator + + + Youssef + Pellenq + Yildiz + Mostafa + Roland J-M + Bilge + Youssef, Mostafa + Pellenq, Roland J-M + Yildiz, Bilge + Glassy nature of water in an ultraconfining disordered material: the case of calcium-silicate-hydrate. + Journal of the American Chemical Society + 20110302 + 20110302 + 133 + 8 + 2499 + 2499-510 + 0002-7863 + 1520-5126 + journal + article + JOUR + We present the structural and dynamic nature of water ultraconfined in the quasi-two-dimensional nanopores of the highly disordered calcium-silicate-hydrate (C-S-H), the major binding phase in cement. Our approach is based on classical molecular simulations. We demonstrate that the C-S-H nanopore space is hydrophilic, particularly because of the nonbridging oxygen atoms on the disordered silicate chains which serve as hydrogen-bond acceptor sites, directionally orienting the hydrogen atoms of the interfacial water molecules toward the calcium-silicate layers. The water in this interlayer space adopts a unique multirange structure: a distorted tetrahedral coordination at short range up to 2.7 Å, a disordered structure similar to that of dense fluids and supercooled phases at intermediate range up to 4.2 Å, and persisting spatial correlations through dipole-dipole interactions up to 10 Å. A three-stage dynamics governs the mean square displacement (MSD) of water molecules, with a clear cage stage characteristic of the dynamics in supercooled liquids and glasses, consistent with its intermediate-range structure identified here. At the intermediate time scales corresponding to the β-relaxation of glassy materials, coincident with the cage stage in MSD, the non-Gaussian parameter indicates a significant heterogeneity in the translational dynamics. This dynamic heterogeneity is induced primarily because of the heterogeneity in the distribution of hydrogen bond strengths. The strongly attractive interactions of water molecules with the calcium silicate walls serve to constrain their motion. Our findings have important implications on describing the cohesion and mechanical behavior of cement from its setting to its aging. + 21294516 + + + + + + + 21294516&rft_id=info:oai/]]> + http://pubmed.gov/21294516 + + 21294516&rft_id=info:oai/]]> + http://primo-central-3.saas.exlibrisgroup.com:1701/primo_library/libweb/aboutMedline.html + + + 21294516&rft_id=info:oai/]]> + http://pubmed.gov/21294516 + + 21294516&rft_id=info:oai/]]> + http://primo-central-3.saas.exlibrisgroup.com:1701/primo_library/libweb/aboutMedline.html + + + + + + + TN_medline9452380 + XML + medline + 9452380 + Other + + + Jennings, D E ; Sada, P V + Absorption lines of hot water have been identified in the infrared spectra of Betelgeuse (alpha Orionis) and Antares (alpha Scorpii) near 12.3 micrometers (811 to 819 wavenumbers). The water lines originate in the atmospheres of the stars, not in their circumstellar material. The spectra are similar in structure to umbral sunspot spectra. Pure rotation water lines of this type will occur throughout the spectra of cool stars at wavelengths greater than 10 micrometers. From the water spectra, the upper limit for the temperature in the line formation region in both stars is 2800 kelvin. The water column density in both stars is (3 +/- 2) x 10(18) molecules per square centimeter, yielding an abundance relative to atomic hydrogen of n(H2O)/n(H) approximately 10(-)7. + <b>ISSN:</b> 0036-8075 ; <b>PMID:</b> 9452380 + Science (New York, N.Y.), Feb, 1998, Vol.279(5352), p.844-7 + eng + peer_reviewed + MEDLINE (NLM) + Astronomy; Water -- analysis + Water in Betelgeuse and Antares + article + 3 + + + $$Uhttp://primo-central-3.saas.exlibrisgroup.com:1701/primo_library/libweb/aboutMedline.html$$DView the National Library of Medicine Copyright Statement + $$Uhttp://pubmed.gov/9452380$$DView this record at the National Library of Medicine site. + $$Topenurl_article + $$Topenurlfull_article + + + Science (New York, N.Y.) + 1998 + Sada, P V + Jennings, D E + Absorption lines of hot water have been identified in the infrared spectra of Betelgeuse (alpha Orionis) and Antares (alpha Scorpii) near 12.3 micrometers (811 to 819 wavenumbers). The water lines originate in the atmospheres of the stars, not in their circumstellar material. The spectra are similar in structure to umbral sunspot spectra. Pure rotation water lines of this type will occur throughout the spectra of cool stars at wavelengths greater than 10 micrometers. From the water spectra, the upper limit for the temperature in the line formation region in both stars is 2800 kelvin. The water column density in both stars is (3 +/- 2) x 10(18) molecules per square centimeter, yielding an abundance relative to atomic hydrogen of n(H2O)/n(H) approximately 10(-)7. + 9452380 + english + 0036-8075 + 00368075 + medline9452380 + article + MEDLINE + medline + nlm_medline + MEDLINE + medline + nlm_medline + medline + Water -- analysis + Astronomy + Water in Betelgeuse and Antares. + + + Jennings, D E ; Sada, P V + 1998 + Water in Betelgeuse and Antares + + + MEDLINE (NLM) + 1998 + Sada, P V + Jennings, D E + Science (New York, N.Y.) + eng + articles + articles + Water -- analysis + Astronomy + peer_reviewed + 2091482702775654597 + 5 + + + 1998 + 9452380 + d ejennings + jenningsd e + 00368075 + 279 + 5352 + 844 + science (new york, ny) + water in betelgeuse antares + waterinbetelgeuseantares + 2 + 1998 + + + Remote Search Resource + no_fulltext + + + 1 + 1 + aggregator + + + Absorption lines of hot water have been identified in the infrared spectra of Betelgeuse (alpha Orionis) and Antares (alpha Scorpii) near 12.3 micrometers (811 to 819 wavenumbers). The water lines originate in the atmospheres of the stars, not in their circumstellar material. The spectra are similar in structure to umbral sunspot spectra. Pure rotation water lines of this type will occur throughout the spectra of cool stars at wavelengths greater than 10 micrometers. From the water spectra, the upper limit for the temperature in the line formation region in both stars is 2800 kelvin. The water column density in both stars is (3 +/- 2) x 10(18) molecules per square centimeter, yielding an abundance relative to atomic hydrogen of n(H2O)/n(H) approximately 10(-)7. + Water in Betelgeuse and Antares. + Jennings, D E + Sada, P V + D E + P V + Sada + Jennings + 19980206 + journal + article + 0036-8075 + 5352 + Science (New York, N.Y.) + 844-7 + 9452380 + 19980206 + JOUR + 844 + 279 + + + + + + + 9452380&rft_id=info:oai/]]> + http://pubmed.gov/9452380 + + 9452380&rft_id=info:oai/]]> + http://primo-central-3.saas.exlibrisgroup.com:1701/primo_library/libweb/aboutMedline.html + + + 9452380&rft_id=info:oai/]]> + http://pubmed.gov/9452380 + + 9452380&rft_id=info:oai/]]> + http://primo-central-3.saas.exlibrisgroup.com:1701/primo_library/libweb/aboutMedline.html + + + + + + + TN_medline15060287 + XML + medline + 15060287 + Other + + + Wernet, Ph ; Nordlund, D ; Bergmann, U ; Cavalleri, M ; Odelius, M ; Ogasawara, H ; Näslund, L A ; Hirsch, T K ; Ojamäe, L ; Glatzel, P ; Pettersson, L G M ; Nilsson, A + X-ray absorption spectroscopy and x-ray Raman scattering were used to probe the molecular arrangement in the first coordination shell of liquid water. The local structure is characterized by comparison with bulk and surface of ordinary hexagonal ice Ih and with calculated spectra. Most molecules in liquid water are in two hydrogen-bonded configurations with one strong donor and one strong acceptor hydrogen bond in contrast to the four hydrogen-bonded tetrahedral structure in ice. Upon heating from 25 degrees C to 90 degrees C, 5 to 10% of the molecules change from tetrahedral environments to two hydrogen-bonded configurations. Our findings are consistent with neutron and x-ray diffraction data, and combining the results sets a strong limit for possible local structure distributions in liquid water. Serious discrepancies with structures based on current molecular dynamics simulations are observed. + E-ISSN: 1095-9203 ; ISSN: 0036-8075 ; PMID: 15060287]]> + Science (New York, N.Y.), May, 2004, Vol.304(5673), p.995-9 + eng + peer_reviewed + MEDLINE (NLM) + Water -- chemistry + The structure of the first coordination shell in liquid water + article + 5 + + + $$Uhttp://primo-central-3.saas.exlibrisgroup.com:1701/primo_library/libweb/aboutMedline.html$$DView the National Library of Medicine Copyright Statement + $$Uhttp://pubmed.gov/15060287$$DView this record at the National Library of Medicine site. + $$Topenurl_article + $$Topenurlfull_article + + + Science (New York, N.Y.) + 2004 + Hirsch, T K + Cavalleri, M + Nordlund, D + Pettersson, L G M + Ogasawara, H + Odelius, M + Wernet, Ph + Glatzel, P + Bergmann, U + Nilsson, A + Ojamäe, L + Näslund, L A + X-ray absorption spectroscopy and x-ray Raman scattering were used to probe the molecular arrangement in the first coordination shell of liquid water. The local structure is characterized by comparison with bulk and surface of ordinary hexagonal ice Ih and with calculated spectra. Most molecules in liquid water are in two hydrogen-bonded configurations with one strong donor and one strong acceptor hydrogen bond in contrast to the four hydrogen-bonded tetrahedral structure in ice. Upon heating from 25 degrees C to 90 degrees C, 5 to 10% of the molecules change from tetrahedral environments to two hydrogen-bonded configurations. Our findings are consistent with neutron and x-ray diffraction data, and combining the results sets a strong limit for possible local structure distributions in liquid water. Serious discrepancies with structures based on current molecular dynamics simulations are observed. + 15060287 + english + 10959203 + 0036-8075 + 00368075 + 1095-9203 + medline15060287 + article + MEDLINE + medline + nlm_medline + MEDLINE + medline + nlm_medline + medline + Water -- chemistry + The structure of the first coordination shell in liquid water. + + + Wernet, Ph ; Nordlund, D ; Bergmann, U ; Cavalleri, M ; Odelius, M ; Ogasawara, H ; Näslund, L A ; Hirsch, T K ; Ojamäe, L ; Glatzel, P ; Pettersson, L G M ; Nilsson, A + 2004 + The structure of the first coordination shell in liquid water + + + MEDLINE (NLM) + 2004 + Hirsch, T K + Cavalleri, M + Nordlund, D + Pettersson, L G M + Ogasawara, H + Odelius, M + Wernet, Ph + Glatzel, P + Bergmann, U + Nilsson, A + Ojamäe, L + Näslund, L A + Science (New York, N.Y.) + eng + articles + articles + Water -- chemistry + peer_reviewed + 6992613260451631498 + 5 + + + 2004 + 15060287 + phwernet + wernetph + 10959203 + 00368075 + 304 + 5673 + 995 + science (new york, ny) + structure of the first coordination shell in liquid water + structureofthefirstcwater + 2 + 2004 + + + Remote Search Resource + no_fulltext + + + 1 + 1 + aggregator + + + X-ray absorption spectroscopy and x-ray Raman scattering were used to probe the molecular arrangement in the first coordination shell of liquid water. The local structure is characterized by comparison with bulk and surface of ordinary hexagonal ice Ih and with calculated spectra. Most molecules in liquid water are in two hydrogen-bonded configurations with one strong donor and one strong acceptor hydrogen bond in contrast to the four hydrogen-bonded tetrahedral structure in ice. Upon heating from 25 degrees C to 90 degrees C, 5 to 10% of the molecules change from tetrahedral environments to two hydrogen-bonded configurations. Our findings are consistent with neutron and x-ray diffraction data, and combining the results sets a strong limit for possible local structure distributions in liquid water. Serious discrepancies with structures based on current molecular dynamics simulations are observed. + The structure of the first coordination shell in liquid water. + Wernet, Ph + Nordlund, D + Bergmann, U + Cavalleri, M + Odelius, M + Ogasawara, H + Näslund, L A + Hirsch, T K + Ojamäe, L + Glatzel, P + Pettersson, L G M + Nilsson, A + L G M + U + D + T K + A + P + L + M + L A + H + Ph + Cavalleri + Nilsson + Hirsch + Nordlund + Ogasawara + Wernet + Pettersson + Glatzel + Odelius + Bergmann + Ojamäe + Näslund + 20040514 + 1095-9203 + journal + article + 0036-8075 + 1095-9203 + 5673 + Science (New York, N.Y.) + 995-9 + 15060287 + 20040514 + JOUR + 995 + 304 + + + + + + + 15060287&rft_id=info:oai/]]> + http://pubmed.gov/15060287 + + 15060287&rft_id=info:oai/]]> + http://primo-central-3.saas.exlibrisgroup.com:1701/primo_library/libweb/aboutMedline.html + + + 15060287&rft_id=info:oai/]]> + http://pubmed.gov/15060287 + + 15060287&rft_id=info:oai/]]> + http://primo-central-3.saas.exlibrisgroup.com:1701/primo_library/libweb/aboutMedline.html + + + + + + + TN_medline17885125 + XML + medline + 17885125 + Other + + + McEwen, A S ; Hansen, C J ; Delamere, W A ; Eliason, E M ; Herkenhoff, K E ; Keszthelyi, L ; Gulick, V C ; Kirk, R L ; Mellon, M T ; Grant, J A ; Thomas, N ; Weitz, C M ; Squyres, S W ; Bridges, N T ; Murchie, S L ; Seelos, F ; Seelos, K ; Okubo, C H ; Milazzo, M P ; Tornabene, L L ; Jaeger, W L ; Byrne, S ; Russell, P S ; Griffes, J L ; Martínez-Alonso, S ; Davatzes, A ; Chuang, F C ; Thomson, B J ; Fishbaugh, K E ; Dundas, C M ; Kolb, K J ; Banks, M E ; Wray, J J + Water has supposedly marked the surface of Mars and produced characteristic landforms. To understand the history of water on Mars, we take a close look at key locations with the High-Resolution Imaging Science Experiment on board the Mars Reconnaissance Orbiter, reaching fine spatial scales of 25 to 32 centimeters per pixel. Boulders ranging up to approximately 2 meters in diameter are ubiquitous in the middle to high latitudes, which include deposits previously interpreted as finegrained ocean sediments or dusty snow. Bright gully deposits identify six locations with very recent activity, but these lie on steep (20 degrees to 35 degrees) slopes where dry mass wasting could occur. Thus, we cannot confirm the reality of ancient oceans or water in active gullies but do see evidence of fluvial modification of geologically recent mid-latitude gullies and equatorial impact craters. + E-ISSN: 1095-9203 ; ISSN: 0036-8075 ; PMID: 17885125]]> + Science (New York, N.Y.), Sep, 2007, Vol.317(5845), p.1706-9 + eng + peer_reviewed + MEDLINE (NLM) + Mars; Water + A closer look at water-related geologic activity on Mars + article + 4 + + + $$Uhttp://primo-central-3.saas.exlibrisgroup.com:1701/primo_library/libweb/aboutMedline.html$$DView the National Library of Medicine Copyright Statement + $$Uhttp://pubmed.gov/17885125$$DView this record at the National Library of Medicine site. + $$Topenurl_article + $$Topenurlfull_article + + + Science (New York, N.Y.) + 2007 + Weitz, C M + Thomson, B J + McEwen, A S + Davatzes, A + Murchie, S L + Byrne, S + Okubo, C H + Wray, J J + Delamere, W A + Mellon, M T + Banks, M E + Jaeger, W L + Seelos, F + Tornabene, L L + Thomas, N + Seelos, K + Russell, P S + Grant, J A + Griffes, J L + Kirk, R L + Bridges, N T + Martínez-Alonso, S + Chuang, F C + Gulick, V C + Squyres, S W + Milazzo, M P + Dundas, C M + Herkenhoff, K E + Kolb, K J + Hansen, C J + Fishbaugh, K E + Eliason, E M + Keszthelyi, L + Water has supposedly marked the surface of Mars and produced characteristic landforms. To understand the history of water on Mars, we take a close look at key locations with the High-Resolution Imaging Science Experiment on board the Mars Reconnaissance Orbiter, reaching fine spatial scales of 25 to 32 centimeters per pixel. Boulders ranging up to approximately 2 meters in diameter are ubiquitous in the middle to high latitudes, which include deposits previously interpreted as finegrained ocean sediments or dusty snow. Bright gully deposits identify six locations with very recent activity, but these lie on steep (20 degrees to 35 degrees) slopes where dry mass wasting could occur. Thus, we cannot confirm the reality of ancient oceans or water in active gullies but do see evidence of fluvial modification of geologically recent mid-latitude gullies and equatorial impact craters. + 17885125 + english + 10959203 + 0036-8075 + 00368075 + 1095-9203 + medline17885125 + article + MEDLINE + medline + nlm_medline + MEDLINE + medline + nlm_medline + medline + Mars + Water + A closer look at water-related geologic activity on Mars. + + + McEwen, A S ; Hansen, C J ; Delamere, W A ; Eliason, E M ; Herkenhoff, K E ; Keszthelyi, L ; Gulick, V C ; Kirk, R L ; Mellon, M T ; Grant, J A ; Thomas, N ; Weitz, C M ; Squyres, S W ; Bridges, N T ; Murchie, S L ; Seelos, F ; Seelos, K ; Okubo, C H ; Milazzo, M P ; Tornabene, L L ; Jaeger, W L ; Byrne, S ; Russell, P S ; Griffes, J L ; Martínez-Alonso, S ; Davatzes, A ; Chuang, F C ; Thomson, B J ; Fishbaugh, K E ; Dundas, C M ; Kolb, K J ; Banks, M E ; Wray, J J + 2007 + A closer look at water-related geologic activity on Mars + + + MEDLINE (NLM) + 2007 + Weitz, C M + Thomson, B J + McEwen, A S + Davatzes, A + Murchie, S L + Byrne, S + Okubo, C H + Wray, J J + Delamere, W A + Mellon, M T + Banks, M E + Jaeger, W L + Seelos, F + Tornabene, L L + Thomas, N + Seelos, K + Russell, P S + Grant, J A + Griffes, J L + Kirk, R L + Bridges, N T + Martínez-Alonso, S + Chuang, F C + Gulick, V C + Squyres, S W + Milazzo, M P + Dundas, C M + Herkenhoff, K E + Kolb, K J + Hansen, C J + Fishbaugh, K E + Eliason, E M + Keszthelyi, L + Science (New York, N.Y.) + eng + articles + articles + Mars + Water + peer_reviewed + -7003185421639602274 + 5 + + + 2007 + 17885125 + a smcewen + mcewena s + 10959203 + 00368075 + 317 + 5845 + 1706 + science (new york, ny) + closer look at water-related geologic activity on mars + closerlookatwater-renmars + 2 + 2007 + + + Remote Search Resource + no_fulltext + + + 1 + 1 + aggregator + + + Water has supposedly marked the surface of Mars and produced characteristic landforms. To understand the history of water on Mars, we take a close look at key locations with the High-Resolution Imaging Science Experiment on board the Mars Reconnaissance Orbiter, reaching fine spatial scales of 25 to 32 centimeters per pixel. Boulders ranging up to approximately 2 meters in diameter are ubiquitous in the middle to high latitudes, which include deposits previously interpreted as finegrained ocean sediments or dusty snow. Bright gully deposits identify six locations with very recent activity, but these lie on steep (20 degrees to 35 degrees) slopes where dry mass wasting could occur. Thus, we cannot confirm the reality of ancient oceans or water in active gullies but do see evidence of fluvial modification of geologically recent mid-latitude gullies and equatorial impact craters. + A closer look at water-related geologic activity on Mars. + McEwen, A S + Hansen, C J + Delamere, W A + Eliason, E M + Herkenhoff, K E + Keszthelyi, L + Gulick, V C + Kirk, R L + Mellon, M T + Grant, J A + Thomas, N + Weitz, C M + Squyres, S W + Bridges, N T + Murchie, S L + Seelos, F + Seelos, K + Okubo, C H + Milazzo, M P + Tornabene, L L + Jaeger, W L + Byrne, S + Russell, P S + Griffes, J L + Martínez-Alonso, S + Davatzes, A + Chuang, F C + Thomson, B J + Fishbaugh, K E + Dundas, C M + Kolb, K J + Banks, M E + Wray, J J + K E + F + F C + K J + A + J J + L + A S + N + J L + M T + V C + K + S W + W A + N T + J A + S + E M + S L + C H + C J + B J + W L + M P + M E + P S + C M + R L + L L + Fishbaugh + Chuang + Squyres + Thomson + Wray + Eliason + Kirk + Herkenhoff + Thomas + Grant + Delamere + Banks + Murchie + McEwen + Bridges + Jaeger + Seelos + Keszthelyi + Martínez-Alonso + Tornabene + Milazzo + Mellon + Byrne + Russell + Griffes + Dundas + Davatzes + Weitz + Kolb + Okubo + Hansen + Gulick + 20070921 + 1095-9203 + journal + article + 0036-8075 + 1095-9203 + 5845 + Science (New York, N.Y.) + 1706-9 + 17885125 + 20070921 + JOUR + 1706 + 317 + + + + + + + 17885125&rft_id=info:oai/]]> + http://pubmed.gov/17885125 + + 17885125&rft_id=info:oai/]]> + http://primo-central-3.saas.exlibrisgroup.com:1701/primo_library/libweb/aboutMedline.html + + + 17885125&rft_id=info:oai/]]> + http://pubmed.gov/17885125 + + 17885125&rft_id=info:oai/]]> + http://primo-central-3.saas.exlibrisgroup.com:1701/primo_library/libweb/aboutMedline.html + + + + + + + TN_medline7761830 + XML + medline + 7761830 + Other + + + Wallace, L ; Bernath, P ; Livingston, W ; Hinkle, K ; Busler, J ; Guo, B ; Zhang, K + High-resolution infrared spectra of sunspot umbrae have been recorded with the 1-meter Fourier transform spectrometer on Kitt Peak. The spectra contain a very large number of water absorption features originating on the sun. These lines have been assigned to the pure rotation and the vibration-rotation transitions of hot water by comparison with high-temperature laboratory emission spectra. + <b>ISSN:</b> 0036-8075 ; <b>PMID:</b> 7761830 + Science (New York, N.Y.), May, 1995, Vol.268(5214), p.1155-8 + eng + peer_reviewed + MEDLINE (NLM) + Solar System; Water + Water on the sun + article + 5 + + + $$Uhttp://primo-central-3.saas.exlibrisgroup.com:1701/primo_library/libweb/aboutMedline.html$$DView the National Library of Medicine Copyright Statement + $$Uhttp://pubmed.gov/7761830$$DView this record at the National Library of Medicine site. + $$Topenurl_article + $$Topenurlfull_article + + + Science (New York, N.Y.) + 1995 + Zhang, K + Busler, J + Livingston, W + Guo, B + Hinkle, K + Bernath, P + Wallace, L + High-resolution infrared spectra of sunspot umbrae have been recorded with the 1-meter Fourier transform spectrometer on Kitt Peak. 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