Pollen‐based biome reconstructions for Colombia at 3000, 6000, 9000, 12 000, 15 000 and 18 000 14C yr ago: Late Quaternary tropical vegetation dynamics     

Robert Marchant  Hermann Behling  Juan‐Carlos Berrio  Antoine Cleef  Joost Duivenvoorden  Henry Hooghiemstra  Peter Kuhry  Bert Melief  Elisabeth Schreve‐Brinkman  Bas Van Geel  Thomas Van der Hammen  Guido Van Reenen  Michael Wille 《第四纪科学杂志》2002,17(2):113-129

Colombian biomes are reconstructed at 45 sites from the modern period extending to the Last Glacial Maximum (LGM). The basis for our reconstruction is pollen data assigned to plant functional types and biomes at six 3000‐yr intervals. A reconstruction of modern biomes is used to check the treatment of the modern pollen data set against a map of potential vegetation. This allows the biomes reconstructed at past periods to be assessed relative to the modern situation. This process also provides a check on the a priori assignment of pollen taxa to plant functional types and biomes. For the majority of the sites, the pollen data accurately reflect the potential vegetation, even though much of the original vegetation has been transformed by agricultural practices. At 18 000 ¹⁴C yr BP, a generally cool and dry environment is reflected in biome, assignments of cold mixed forests, cool evergreen forests and cool grassland–shrub; the latter extending to lower altitudes than presently recorded. This signal is strongly recorded at 15 000 and 12 000 ¹⁴C yr BP, the vegetation at these times also reflecting a relatively cool and dry environment. At 9000 ¹⁴C yr BP there is a shift to biomes thought to result from slightly cooler environmental conditions. This trend is reversed by 6000 ¹⁴C yr BP; most sites, within a range of different environmental settings, recording a shift to more xeric biome types. There is an expansion of steppe and cool mixed‐forest biomes, replacing tropical dry forest and cool grassland–shrub biomes, respectively. These changes in biome assignments from the modern situation can be interpreted as a biotic response to mid‐Holocene climatic aridity. At 3000 ¹⁴C yr BP the shift is mainly to biomes characteristic of slightly more mesic environmental conditions. There are a number of sites that do not change biome assignment relative to the modern reconstruction, although the affinities that these sites have to a specific biome do change. These ‘anomalies’ are interpreted on a site‐by‐site basis. Spatially constant, but differential response of the vegetation to climatic shifts are related to changes in moisture sources and the importance of edaphic controls on the vegetation. The Late Quaternary reconstruction of large‐scale vegetation dynamics in Colombia allows an understanding of the environmental controls on these to be developed. In particular, shifts in the character of the main climatic systems that influence Colombian vegetation are described. Copyright © 2002 John Wiley & Sons, Ltd.  相似文献   

Earth and space-based NEO survey simulations: prospects for achieving the spaceguard goal   总被引：1，自引：0，他引：1  

Robert Jedicke  Alessandro Morbidelli  Jean-Marc Petit 《Icarus》2003,161(1):17-33

We have used an improved model of the orbit and absolute magnitude distribution of Near Earth Objects (NEOs) to simulate the performance of asteroid surveys. Our results support general conclusions of previous studies using preliminary Near Earth Asteroid (NEA) orbit and magnitude distributions and suggest that meeting the Spaceguard Goal of 90% completion for Near Earth Objects (NEOs) greater than 1 km diameter by 2008 is impossible given contemporary surveying capabilities.The NEO model was derived from NEO detections by the Spacewatch Project. For this paper we developed a simulator for the Catalina Sky Survey (CSS) for which we had a complete pointing history and NEO detection efficiency. The good match between the output of the simulator and the actual CSS performance gives confidence that both the NEO model and simulator are correct. Then, in order to determine if existing surveys can meet the Spaceguard Goal, we developed a simulator to mimic the LINEAR survey, for which detailed performance characteristics were unavailable. This simulator serendipitously provided an estimate for the currently undiscovered population of NEOs upon which we base all our estimates of time to 90% completion. We also developed a set of idealized NEO surveys in order to constrain the best possible survey performance in contrast to more realistic systems.A 100% efficient, all-sky, every night survey, subject only to the constraints of detection above a specified air mass and when the Sun is 18° below the horizon provides a benchmark from which to examine the effect of imposing more restrictions and the efficacy of some simple survey strategies. Such a survey must have a limiting V-magnitude of 20.1 ± 0.2 to meet the Spaceguard Goal.More realistic surveys, limited by latitude, the galaxy, minimum rates of NEO motion, etc., require fainter limiting magnitudes to reach the same completion. Our most realistic simulations, which have been normalized to the performance of the LINEAR detector system’s operation in the period 1999-2000, indicate that it would take them another 33 ± 5 years to reach 90% completeness for the larger asteroids (?1 km diameter). They would need to immediately increase the limiting magnitude to about 24 in order to meet the Spaceguard Goal.The simulations suggest that there may be little need for distributing survey telescopes in longitude and latitude as long as there is sufficient sky coverage from a telescope or network of telescopes which may be geographically close. An idealized space-based survey, especially from a satellite orbit much interior to Earth, would offer an advantage over their terrestrial counterparts. We do not consider a cost-benefit analysis for any of the simulations but suspect that a local-area network of telescopes capable of covering much of the sky in a month to V ∼ 21.5 may be administratively, financially, and scientifically the best compromise for reaching 90% completion of NEOs larger than 1 km diameter.  相似文献   

IR band intensities of DC₃N and HC₃N: Implication for observations of Titan's atmosphere     

Yves Bénilan  Antoine Jolly  Jean-Claude Guillemin 《Planetary and Space Science》2006,54(6):635-640

We have obtained the infrared spectra and the corresponding absolute band intensities for two HC₃N isotopomers: DC₃N and HC₃¹⁵N. Our results for DC₃N are in good agreement with previous measurements except for the ν₂ and ν₃ stretching modes. For HC₃¹⁵N, this study is the first including intensity measurements.We have also studied the possible detection of these isotopomers in Titan's atmosphere using the CIRS spectrograph onboard the Cassini spacecraft. Our simulation of the expected spectra shows that for a signal-to-noise ratio better than 100, the ¹⁵N isotopomer of HC₃N could be detected. But, further study of HC₃N hot bands are needed since some of them overlap the HC₃¹⁵N Q-branch.  相似文献   

Status of the eLISA on table (LOT) electro-optical simulator for space based,long arms interferometers     

Pierre Grüning  Hubert Halloin  Pierre Prat  Sylvain Baron  Julien Brossard  Christelle Buy  Antoine Petiteau  Gerhard Heinzel  Iouri Bykov 《Experimental Astronomy》2015,39(2):281-302

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Can the optical very large array be coupled with the JNLT?     

Isabelle Bosc  Denis Mourad  Antoine Labeyrie 《Astrophysics and Space Science》1989,160(1-2):355-360

Coupling the JNLT with the Keck telescope is of considerable interest. Further enhancement may be possible with auxiliary small telescopes, as planned for ESO's VLT. Current plans for installing the optical very large array at Mauna Kea provide opportunities for extra OVLA telescopes near the JNLT.A coudé field slicer is proposed for interferometric observing of a reference star together with the main object. Additions to the JNLT coudé spectrograph are also suggested for use as a speckle camera with multiple spectral channels.Paper presented at the Symposium on the JNLT and Related Engineering Developments, Tokyo, November 29–December 2, 1988.  相似文献   

Formation of hybrid-oligomers between anthropogenic chemicals and humic acid derivatives     

Jean-Marc Bollag  Shu-Yen Liu 《Organic Geochemistry》1985,8(1):131

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Conditioning Surface-Based Geological Models to Well and Thickness Data   总被引：2，自引：1，他引：1  

Antoine Bertoncello  Tao Sun  Hongmei Li  Gregoire Mariethoz  Jef Caers 《Mathematical Geosciences》2013,45(7):873-893

Geostatistical simulation methods aim to represent spatial uncertainty through realizations that reflect a certain geological concept by means of a spatial continuity model. Most common spatial continuity models are either variogram, training image, or Boolean based. In this paper, a more recent spatial model of geological continuity is developed, termed the event, or surface-based model, which is specifically applicable to modeling cases with complex stratigraphy, such as in sedimentary systems. These methods rely on a rule-based stacking of events, which are mathematically represented by two-dimensional thickness variations over the domain, where positive thickness is associated with deposition and negative thickness with erosion. Although it has been demonstrated that the surface-based models accurately represent the geological variation present in complex layered systems, they are more difficult to constrain to hard and soft data as is typically required of practical geostatistical techniques. In this paper, we develop a practical methodology for constraining such models to hard data from wells and thickness data interpreted from geophysics, such as seismic data. Our iterative methodology relies on a decomposition of the parameter optimization problem into smaller, manageable problems that are solved sequentially. We demonstrate this method on a real case study of a turbidite sedimentary basin.  相似文献   

Specialization for amphibiosis in Brachyodus onoideus (Artiodactyla, Hippopotamoidea) from the Early Miocene of France     

Maeva J. Orliac  Pierre-Olivier Antoine  Anne-Lise Charruault  Sophie Hervet  Frédéric Prodeo  Francis Duranthon 《Swiss Journal of Geoscience》2013,106(2):265-278

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Extension syn-convergence,poinçonnement vertical et unités métamorphiques contrastées en bordure ouest du Grand Paradis (Alpes Franco-Italiennes)     

Yann Rolland  Jean-Marc Lardeaux  Stéphane Guillot  Christian Nicollet 《Geodinamica Acta》2013,26(2-3):133-148

Résumé

À la bordure occidentale du massif du Grand Paradis (Alpes occidentales), la zone Piémontaise est constituée des unités océaniques des schistes lustrés et de l’unité continentale du Grand Paradis. Une étude métamorphique nous permet de préciser et de discuter des discontinuités de pression et des conditions de rétro-morphose de trois unités piémontaises déjà distinguées antérieurement. L’unité supérieure des schistes lustrés (LS) métamorphisée dans le faciès des schistes bleus (9.5 ± 2 kbar, 340 ± 30 °C). L’unité inférieure des schistes lustrés (LI) métamorphisée dans le faciès des éclogites (12.5±3 kbar, 480±50 °C). L’unité continentale du Grand Paradis (GP) métamorphisée dans le faciès des éclogites de plus haute pression (12 à 20 kbar, 500 ± 50 °C). L’ensemble des unités enregistre une décompression dans les conditions du faciès amphibolite à épidote, et donc avec une légère augmentation tardive de température, pour les unités LI et GP, et dans celles des schistes verts pour l’unité LS. L’étude des inclusions fluides dans les fentes de tension et dans les plans de cisaillement, en parallèle à l’élude des paragenèses rétromorphiques permet de montrer que c’est tardivement (4 ± 1 kbar, 400 ± 50 °C) que l’histoire tectonomélamor-phique devient commune à l’ensemble des unités. L’étude du champ de la déformation finie met en évidence une tectonique en extension qui débute en conditions ductiles dans le faciès amphibolite à épidote pour LI, et schiste vert pour LS, et se poursuit en conditions fragiles. La déformation ductile se traduit par des trajectoires en dômes et bassins de la foliation, avec une partition entre des domaines en aplatissement au c?ur des dômes et des domaines en cisaillement simple en bordure des dômes, au contact entre les différentes unités. La déformation fragile correspond au continuum plus tardif de la déformation extensive ductile. Cette tectonique extensive n’est qu’en partie responsable des sautes de pression entre les trois unités étudiés. Elle correspond à l’accommodation, en surface, au poinçonnement vertical des unités de haute pression, en contexte de convergence, par l’écaillage progressif de la croûte européenne à l’avant du butoir mantellique apulien. © 2000 Editions scientifiques et médicales Elsevier SAS  相似文献   

A new patchwork simulation method with control of the local-mean histogram   总被引：3，自引：3，他引：0  

Corentin Faucher  Antoine Saucier  Denis Marcotte 《Stochastic Environmental Research and Risk Assessment (SERRA)》2013,27(1):253-273

We present a new stochastic simulation method that builds two-dimensional images by assembling together square image pieces called blocks. The blocks are taken from a reference image. Our method, called patchwork simulation method (PSM), enforces pattern continuity in the image. Moreover, PSM allows to control the image local-mean histogram. This histogram bin-frequencies can be set to user-defined target values that may differ from the reference image local-mean histogram. This flexibility enhances the PSM generality by enlarging the set of all possible simulations. The local-mean histogram control is achieved by adjusting suitably the transition probabilities that associate a new block to an existing neighborhood in the partly simulated image. For several types of synthetic images and one polymer blend image, we show that PSM reproduces faithfully the reference image visual appearance (i.e. patterns are correctly shaped) and that simulated images are statistically compatible with the target local-mean histogram. Moreover, we show that our method has the ability to produce simulations that respect conditional hard data as well as a target local-mean histogram.  相似文献