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排序方式: 共有431条查询结果,搜索用时 15 毫秒
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Sea level rise, deltaic progradation, and floodplain aggradation have changed the landscape in the vicinity of ancient Troy during the past 10,000 years. With the waning of the last major world glaciation and resultant sea level rise and fluctuation, a marine embayment protruded nearly 10 kilometers south of the site of Troy at Hisarlik in the Troad of northwest Turkey. As the sea approached its present level approximately 6000 years ago, fluvial and marine deposition caused a northerly migration of the delta and floodplain of the Scamander and Simois Rivers past the site of Troy toward the present-day coast about 6 kilometers north of the site. In view of these major changes in morphology, interpretations of ancient geographies related to historical or historical-mythological settings must be changed. A number of paleogeographic maps have been reconstructed with the use of subsurface data that records the continuing landscape change since the first occupancy of the site at Troy 5000 years ago. These show that ancient Troy was located on an embayment of the sea. If the Trojan War occurred, then the axis of the battlefield and associated events must be relocated to the south and west of Troy. 相似文献
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Schawinski K Justham S Wolf C Podsiadlowski P Sullivan M Steenbrugge KC Bell T Röser HJ Walker ES Astier P Balam D Balland C Carlberg R Conley A Fouchez D Guy J Hardin D Hook I Howell DA Pain R Perrett K Pritchet C Regnault N Yi SK 《Science (New York, N.Y.)》2008,321(5886):223-226
Massive stars undergo a violent death when the supply of nuclear fuel in their cores is exhausted, resulting in a catastrophic "core-collapse" supernova. Such events are usually only detected at least a few days after the star has exploded. Observations of the supernova SNLS-04D2dc with the Galaxy Evolution Explorer space telescope reveal a radiative precursor from the supernova shock before the shock reached the surface of the star and show the initial expansion of the star at the beginning of the explosion. Theoretical models of the ultraviolet light curve confirm that the progenitor was a red supergiant, as expected for this type of supernova. These observations provide a way to probe the physics of core-collapse supernovae and the internal structures of their progenitor stars. 相似文献
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Suzanne Higgins Saskia D. Keesstra Žydrė Kadziuliene Lionel Jordan-Meille David Wall Alessandra Trinchera Heide Spiegel Taru Sandén Andreas Baumgarten Johannes L. Jensen Juliane Hirte Frank Liebisch Susanne Klages Philipp Löw Katrin Kuka Maarten De Boever Karoline D'Haene Sevinc Madenoglu Hesna Özcan Wieke Vervuurt Janjo de Haan Willem van Geel Bo Stenberg Pascal Denoroy Rok Mihelič Alar Astover Raquel Mano Cristina Sempiterno Fatima Calouro Giuseppe Valboa Helena Aronsson Tore Krogstad Stanislav Torma Jose Gabriel Peter Laszlo Nils Borchard Bartosz Adamczyk Anna Jacobs Beata Jurga Bożena Smreczak Bruno Huyghebaert Morgan Abras Raimonds Kasparinskis Eloise Mason Claire Chenu 《European Journal of Soil Science》2023,74(5):e13422
The European Commission has set targets for a reduction in nutrient losses by at least 50% and a reduction in fertiliser use by at least 20% by 2030 while ensuring no deterioration in soil fertility. Within the mandate of the European Joint Programme EJP Soil ‘Towards climate-smart sustainable management of agricultural soils’, the objective of this study was to assess current fertilisation practices across Europe and discuss the potential for harmonisation of fertilisation methodologies as a strategy to reduce nutrient loss and overall fertiliser use. A stocktake study of current methods of delivering fertilisation advice took place across 23 European countries. The stocktake was in the form of a questionnaire, comprising 46 questions. Information was gathered on a large range of factors, including soil analysis methods, along with soil, crop and climatic factors taken into consideration within fertilisation calculations. The questionnaire was completed by experts, who are involved in compiling fertilisation recommendations within their country. Substantial differences exist in the content, format and delivery of fertilisation guidelines across Europe. The barriers, constraints and potential benefits of a harmonised approach to fertilisation across Europe are discussed. The general consensus from all participating countries was that harmonisation of fertilisation guidelines should be increased, but it was unclear in what format this could be achieved. Shared learning in the delivery and format of fertilisation guidelines and mechanisms to adhere to environmental legislation were viewed as being beneficial. However, it would be very difficult, if not impossible, to harmonise all soil test data and fertilisation methodologies at EU level due to diverse soil types and agro-ecosystem influences. Nevertheless, increased future collaboration, especially between neighbouring countries within the same environmental zone, was seen as potentially very beneficial. This study is unique in providing current detail on fertilisation practices across European countries in a side-by-side comparison. The gathered data can provide a baseline for the development of scientifically based EU policy targets for nutrient loss and soil fertility evaluation. 相似文献
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