排序方式： 共有46条查询结果，搜索用时 15 毫秒
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T. Guillot L. Abe A. Agabi J.‐P. Rivet J.‐B. Daban D. Mkarnia E. Aristidi F.‐X. Schmider N. Crouzet I. Gonalves C. Gouvret S. Ottogalli H. Faradji P.‐E. Blanc E. Bondoux F. Valbousquet 《Astronomische Nachrichten》2015,336(7):638-656
The installation and operation of a telescope in Antarctica represent particular challenges, in particular the requirement to operate at extremely cold temperatures, to cope with rapid temperature fluctuations and to prevent frosting. Heating of electronic subsystems is a necessity, but solutions must be found to avoid the turbulence induced by temperature fluctuations on the optical paths. ASTEP 400 is a 40cm Newton telescope installed at the Concordia station, Dome C since 2010 for photometric observations of fields of stars and their exoplanets. While the telescope is designed to spread star light on several pixels to maximize photometric stability, we show that it is nonetheless sensitive to the extreme variations of the seeing at the ground level (between about 0′′.1 and 5′′) and to temperature fluctuations between –30°C and –80 °C. We analyze both day‐time and night‐time observations and obtain the magnitude of the seeing caused by the mirrors, dome and camera. The most important effect arises from the heating of the primary mirror which gives rise to a mirror seeing of 0′′.23 K–1. We propose solutions to mitigate these effects. (© 2015 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim) 相似文献
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Pascal Bonnefond Pierre Exertier Olivier Laurain Amandine Guillot Nicolas Picot Mathilde Cancet 《Marine Geodesy》2015,38(3):171-192
The geodetic Corsica site was set up in 1998 in order to perform altimeter calibration of the TOPEX/Poseidon (T/P) mission and subsequently, Jason-1 and OSTM/Jason-2. The scope of the site was widened in 2005 in order to undertake the calibration of the Envisat mission and most recently of SARAL/AltiKa. Here we present the first results from the latter mission using both indirect and direct calibration/validation approaches. The indirect approach utilizes a coastal tide gauge and, as a consequence, the altimeter derived sea surface height (SSH) needs to be corrected for the geoid slope. The direct approach utilizes a novel GPS-based system deployed offshore under the satellite ground track that permits a direct comparison with the altimeter derived SSH. The advantages and disadvantages of both systems (GPS-based and tide gauges) and methods (direct or indirect) will be described and discussed. Our results for O/IGD-R data show a very good consistency for these three kinds of products: their derived absolute SSH biases are consistent within 17 mm and their associated standard deviation ranges from 31 to 35 mm. The AltiKa absolute SSH bias derived from GPS-zodiac measurement using the direct method is ?54 ±10 mm based on the first 13 cycles. 相似文献
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Fabien Deschamps Stéphane Guillot Marguerite Godard Catherine Chauvel Muriel Andreani Kéiko Hattori 《Chemical Geology》2010,269(3-4):262-277
The Tso Morari serpentinites in the Ladakh area, northwest Himalaya, originated from the forearc mantle overlying the northward subducting Neo-Tethys lithosphere and the margin of the Indian continent. The serpentinites are characterized by high concentration of fluid-mobile elements (FME: As, Sb, B, Li, and U) compared to ophiolitic or abyssal serpentinites. The Pb isotopic compositions of serpentinites show influence of the subducted Indian continental lithosphere. Trace element concentrations of antigorite determined in situ with Laser Ablation High Resolution Inductively Coupled Mass Spectrometer (LA-HR-ICP-MS) show high contents of FME including Pb, in contrast to the spatially associated iron oxides. Rare earth elements (REE) and compatible elements, such as Sc and Co, remained immobile during the hydration, allowing the identification of the primary minerals (olivine or orthopyroxene) from which serpentine formed. Serpentinized olivine displays higher Sb and As concentrations (up to 1000 × PM) than serpentinized orthopyroxenes that are enriched in Pb, Cs and Li (2 to up to 10 × PM).We propose that the observed FME distribution in two types of serpentine reflect the differential incorporation of FME during the downward movement of the serpentinite along the subduction plane. At temperature lower than 400 °C, at shallow depths, olivine is preferentially serpentinized and incorporates elements that are fluid soluble at low temperatures, such as Sb and As. Above 400 °C, orthopyroxene is hydrated and incorporates Pb, Cs, Li and possibly Ba. Boron and U are incorporated in both types of serpentine suggesting that they are released from slabs at temperatures around 300–400 °C. The serpentine acts as a sink for water, but also for FME and transports them to deeper and hotter levels in the mantle, down to the isotherm 600–650 °C where dehydration occurs. 相似文献
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Gweltaz Maho Xavier Fayoux Stphane Guillot Eduardo Garzanti Paul Capiez Georges Mascle 《Journal of Asian Earth Sciences》2006,26(6):695-707
In the Ladakh–Zanskar area, relicts of both ophiolites and paleo-accretionary prism have been preserved in the Sapi-Shergol mélange zone. The paleo-accretionary prism, related to the northward subduction of the northern Neo-Tethys beneath the Ladakh Asian margin, mainly consists of tectonic intercalations of sedimentary and blueschist facies rocks. Whole rock chemical composition data provide new constraints on the origin of both the ophiolitic and the blueschist facies rocks. The ophiolitic rocks are interpreted as relicts of the south Ladakh intra-oceanic arc that were incorporated in the accretionary prism during imbrication of the arc. The blueschist facies rocks were previously interpreted as oceanic island basalts (OIB), but our new data suggest that the protolith of some of the blueschists is a calc-alkaline igneous rock that formed in an arc environment. These blueschists most likely originated from the south Ladakh intra-oceanic arc. This arc was accreted to the southern margin of Asia during the Late Cretaceous and the buried portion was metamorphosed under blueschist facies conditions. Following oceanic subduction, the external part of the arc was obducted to form the south Ladakh ophiolites or was incorporated into the Sapi-Shergol mélange zone. The incorporation of the south Ladakh arc into the accretionary prism implies that the complete closure of the Neo-Tethys likely occurred by Eocene time. 相似文献
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Origin and evolution of the Escambray Massif (Central Cuba): an example of HP/LT rocks exhumed during intraoceanic subduction 总被引：2，自引：0，他引：2
J. Schneider D. Bosch P. Monié S. Guillot A. García-Casco J. M. Lardeaux R. Luís Torres-Roldán G. Millán Trujillo 《Journal of Metamorphic Geology》2004,22(3):227-247
High‐pressure (HP) metabasites from the Sancti Spiritus dome (Escambray massif, Central Cuba) have been studied in order to better understand the origin and evolution of the Northern Caribbean boundary plate during the Cretaceous, in a global subduction context. Geochemical and petrological studies of these eclogites reveal two groups with contrasting origins and pre‐subduction metamorphic histories. Eclogites collected from exotic blocks within serpentinite (mélange zone) originated from a N‐MORB type protolith, do not record pre‐eclogitic metamorphic history. Conversely eclogites intercalated in Jurassic metasedimentary rocks (non‐mélange zone) have a calc‐alkaline arc‐like origin and yield evidence for a pre‐subduction metamorphic event in the amphibolite facies. However, all the studied Escambray eclogites underwent the same eclogitic peak (around 600 °C at 16 kbar), and followed a cold thermal gradient during their exhumation (estimated at around 13.5 °C km?1), which can suggest that this exhumation was coeval with subduction. Concordant geochronological data (Rb/Sr and Ar/Ar) support that the main exhumation of HP/LT rocks from the Sancti Spiritus dome occurred at 70 Ma by top to SW thrusting. The retrograde trajectory of these rocks suggests that the north‐east subduction of the Farallon plate continued after 70 Ma. The set‐off to the exhumation can be correlated with the beginning of the collision between the Bahamas platform and the Cretaceous island arc that induced a change of the subduction kinematics. The contrasting origin and ante‐subduction history of the analysed samples imply that the Escambray massif consists of different geological units that evolved in different environments before their amalgamation during exhumation to form the present unit III of the massif. 相似文献
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Xavier Guillot Muzahim Al-Mukhtar Faiza Bergaya Jean-Marie Fleureau 《Comptes Rendus Geoscience》2002,334(2):105-109
Porosity measurements on a clay material, carried out through various microscopic techniques, show a significant difference with the total porosity macroscopically estimated. Analyses have allowed to assign this difference, whose importance is linked to the hydromechanical stresses sustained by the material, to microporous spaces lower than 2 nm and to closed pore volumes, not accessible by the used techniques. Besides, the role of the drying methods of samples, which do not allow the removal of a part of the water, is highlighted. Its elimination would lead to irreversible microtextural modifications, prejudicial to the understanding of the macroscopic behaviour of the material. To cite this article: X. Guillot et al., C. R. Geoscience 334 (2002) 105–109. 相似文献
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Descamp P Holon F Ballesta L Guilbert A Guillot M Boissery P Raimondino V Deter J 《Marine pollution bulletin》2011,62(2):284-292
Posidonia oceanica is an endemic seagrass from the Mediterranean Sea. It is an indicator of water quality and of the ecological state of coastal ecosystems. The aim of this paper is to test acoustic telemetry for monitoring the position of P. oceanica meadow limits with varied types. After evaluating the accuracy of the system, we present results from a spatiotemporal survey of P. oceanica meadows on nine sites located on the French coast. The method has been demonstrated to be highly efficient for high precision underwater mapping regardless of meadow type, with 1 cm accuracy for a distance of 40 m between the base and the pointer. A temporal survey led at Cerbere-Banyuls shows a weak global progression of 4 m2 (progression of 26 m2 - regression of 22 m2) between 2006 and 2010. Finally, we discuss the cost and efficiency of this method, and wether it should be generalized for further studies. 相似文献
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Stéphane Schwartz Jean-Marc Lardeaux Stéphane Guillot Pierre Tricart 《Geodinamica Acta》2013,26(2-3):169-188
RésuméLe complexe ophiolitique du Monviso représente un témoin essentiel de la lithosphère océanique subduite puis exhumée dans les Alpes occidentales. Ce complexe est classiquement subdivisé en unités lithologiques, qui ont toutes subi une évolution structurale caractérisée par la succession de trois événements dans des environnements (1) éclogitique, (2) schistes bleus puis (3) schistes verts. Cependant la quantification des conditions physiques du métamorphisme éclogitique au sein de trois unités à lithologies comparables (Viso Mozzo, Passo Gallarino et Lago Superiore), montrent clairement l’existence d’une hétérogénéité des conditions éclogitiques enregistrée par l’ensemble des unités, indépendamment de la chimie de la roche initiale. Les conditions estimées sont de 450 ± 40 °C et de 12 ± 3 kb pour l’unité du Viso Mozzo et du Passo Gallarino contre 580 ± 40°C et 19 ± 2 kb pour l’unité du Lago Superiore. De plus l’analyse structurale combinée révèle que c’est au cours de l’exhumation, dans les conditions du faciès des schistes bleus, que les différentes unités vont être juxtaposées et vont suivre une histoire tectono-métamorphique commune. Ces nouvelles données, impliquent une réinterprétation des modèles géodynamiques existants et couramment admis pour le Monviso. Ce dernier doit être considéré comme un complexe résultant de l’accrétion de différents morceaux d’une lithosphère océanique subduite, qui se sont détachés à différentes profondeurs pour venir se stocker à 25 km de profondeur dans les conditions du faciès des schistes bleus. © 2000 Éditions scientifiques et médicales Elsevier SAS 相似文献
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