Vertical variations of wave-induced radiation stress tensor   总被引：3，自引：0，他引：3  

Zheng Jinhai  Yan Yixin 《海洋学报(英文版)》2001,20(4):597-605

INTRODUcrIONThe concept of radiation stress was deve1oPed by tonguet--Higgins and Stewart (1964 ),who intreduced the definition of radiation stress as the excess mornentum due to the presence ofwaves, on the basis of time-averaged laws of Newtonian fluid mechanics and the assmption ofa unifOrm velocity distribution over depth. Subequently, the theory has been applied success-fully in the investigation of phenomena such as wave set-up and set--down (Bowen et al.,l968), longshore currents …  相似文献   

辐射应力对台风风暴潮预报的影响和数值研究   总被引：2，自引：0，他引：2  

刘秋兴  于福江  王培涛  董剑希 《海洋学报》2011,33(5):47-53

台风过程期间,风暴潮和海浪是相伴相生的,相互作用的.波致辐射应力对于近岸风暴增、减水起着十分重要的作用,传统的海浪模式计算辐射应力耗时较多,不能满足业务化预报的要求.根据已有波浪辐射应力的理论表达式,经过严密的数学推导,适当的简化处理,提出了一个较为简单的波浪辐射应力表达式,并将其应用到业务化风暴潮数值预报模式中去,通...  相似文献   

Twenty-five years of spectral UV-B measurements over Canada,Europe and Japan: Trends and effects from changes in ozone,aerosols, clouds,and surface reflectivity     

《Comptes Rendus Geoscience》2018,350(7):393-402

Spectral UV records of solar irradiance at stations over Europe, Canada, and Japan were used to study long-term trends at 307.5 nm for a 25-year period, from 1992 to 2016. Ground-based measurements of total ozone, as well as satellite measurements of the Aerosol Index, the Total Cloud Cover and the surface reflectivity were also used in order to attribute the estimated changes of the UV to the corresponding changes of these factors. The present study shows that over the Northern Hemisphere, the long-term changes in UV-B radiation reaching the Earth's surface vary significantly over different locations, and that the main drivers of these variations are changes in aerosols and total ozone. At high latitudes, part of the observed changes may also be attributed to changes in the surface reflectivity. Over Japan, the UV-B irradiance at 307.5 nm has increased significantly by ∼3%/decade during the past 25 years, possibly due to the corresponding significant decrease of its absorption by aerosols. It was found that the greatest part of this increase took place before the mid-2000s. The only European station, over which UV radiation increases significantly, is that of Thessaloniki, Greece. Analysis of the clear-sky irradiance for the particular station shows increasing irradiance at 307.5 nm by ∼3.5%/decade during the entire period of study, with an increasing rate of change during the last decade, possibly again due to the decreasing absorption by aerosols.  相似文献   

锆石辐射损伤测年方法研究进展与应用     

范明璞  柳小明  孙圣思 《地质论评》2022,68(5):2022102003-2022102003

锆石辐射损伤测年是一种新兴的低温热年代学方法（封闭温度为~230 ± 25 ℃）,其原理是依据拉曼半高宽（ν3）计算出锆石所累积的α通量,结合U、Th含量,得出锆石辐射损伤的累积时间,即锆石辐射损伤年龄。相较于其他低温年代学方法,锆石辐射损伤测年具有测试简便、高效、低成本、双（多）定年等优势,在地学研究中展现出广泛的应用前景,现已成功应用于示踪物源区和揭示岩体热事件等领域。然而,该方法尚存几个关键问题有待解决,例如,微区测试的空间不匹配性、封闭温度存有争议、较大的年龄偏差等,这无疑阻碍其在地球科学领域中更进一步的推广和应用。本文系统地介绍了锆石辐射损伤测年方法的起源、原理和测试方法,总结了相关应用的重要进展,阐述了锆石辐射损伤测年方法的尚存问题,并对该方法的发展趋势作以展望,以期为年代学的发展提供新的技术手段。  相似文献   

Extinctions, Morphological Gaps, Major Transitions, Stem Groups, and the Origin of Major Clades, with a Focus on Early Animals     

XIAO Shuhai 《《地质学报》英文版》2022,96(6):1821-1829

Systematic extinctions can leave major morphological gaps between living crown-group clades. Such morphological gaps would be perceived, from a neontological point of view, as major evolutionary transitions. In order to fill these morphological gaps and to map the evolutionary steps toward major evolutionary transitions, we need to integrate extinct stem-group taxa in phylogenetic studies. However, the recognition of stem group has not been widely adopted in the study of early animal fossils, despite that all fossils are stem groups at one level or another. Part of the difficulty is that stem groups may not have all features that collectively diagnose the respective crown group, and they can have unique (autapomorphic) features, making them tantalizingly similar to and frustratingly different from the crown group (e.g., stem-group eukaryotes can be prokaryotic and stem-group animals can be protistan). The need to embrace stem groups and to implement the PhyloCode, in order to achieve phylogenetic clarity and to offer key paleontological insights into the origin and early animal evolution, is illustrated in debates on several controversial Ediacaran and Cambrian fossils.  相似文献   

个旧东区变基性火山岩型铜矿成因分析     

郑世红 《云南地质》2012,(3):325-330

有证据表明,个旧矿区矿产除与花岗岩密切相关外,基性火山或喷流沉积作用也较明显,变基性火山岩型铜矿的发现及研究增添不少理由。该型Cu矿层状、似层状,赋存于个旧组下段卡房段,矿层多,具同生沉积构造,从而对个旧矿区成矿理论增添新看法。  相似文献   

Development dynamics of intense solar proton flares     

A. B. Struminsky  I. V. Zimovets 《Astronomy Letters》2007,33(9):615-621

We consider the relationship of electromagnetic radiation in the three most intense flares of solar cycle 23, more specifically, those of October 28, 2003, January 20, 2005, and September 7, 2005, to the acceleration and release of protons into interplanetary space. The impulsive phase of these flares lasted ～ 20 min and consisted of at least three energy release episodes, which differed by their manifestation in the soft (1–8 Å, GOES) and hard (>150 keV, INTEGRAL) X-ray ranges as well as at radio frequencies of 245 MHz and 8.8 GHz. The protons and electrons were accelerated in each episode, but with a different efficiency; the relativistic protons were accelerated only after 5–6min of impulsive-phase development after the onset of a coronal mass ejection. It is at this time that maximum hard X-ray fluxes were observed in the September 7, 2005 event, which exceeded severalfold those for the other two flares considered. We associate the record fluxes of protons with energies > 200MeV observed in the heliosphere in the September 7, 2005 event with the dynamics of the impulsive phase. The extreme intensities of the microwave emission in the October 28, 2003 and January 20, 2005 events were probably attributable to the high-energy electron trapping conditions and did not reflect the acceleration process.  相似文献   

Evidence of the Link between Broad Emission Line Regions and Accretion Disks in Active Galactic Nuclei     

Yun Xu    Xin-Wu Cao Shanghai Astronomical Observatory  Chinese Academy of Sciences  Shanghai  Graduate School of Chinese Academy of Sciences  Beijing 《中国天文和天体物理学报》2007,7(1):63-70

1 INTRODUCTION Most bright active galactic nuclei (AGNs) exhibit broad emission lines, with full width at half maximum (FWHM ≥ 103 km s?1) (Peterson et al. 1999). Some type 1 AGNs could have very broad emission lines (FWHM≥ 20 000 km s?1). Type 2 AGNs s…  相似文献   

An Annular Gap Acceleration Model for γ-ray Emission of Pulsars     

Guo-Jun Qiao  Ke-Jia Lee  Bing Zhang  Hong-Guang Wang  Ren-Xin Xu 《中国天文和天体物理学报》2007,7(4)

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基于Kongsberg EM多波束的Snippet数据处理方法     

胡俊  吴永亭  豆虎林  李治远 《海洋科学进展》2020,38(4):717-724

多波束声呐记录的海底后向散射片段(Snippet)数据处理成角度响应曲线和地理编码(Mosaic)图像可以 帮助识别海底底质类型和反映地貌形态,这一过程包括辐射校正、角度响应改正(AVG)和几何地理编码,但不同的多波束系统硬件在辐射校正和角度响应改正方法上存在差异且传统处理方法忽略了声呐系统本身的指向性模型随时间变化的事实。以声呐方程为基础,针对Kongsberg EM 多波束系统提出了一套完整的Snippet数据处理流程,并分析了各步骤中存在的可变性,给出了每一步的处理建议,最后将此方法应用于EM2040浅水多波束实测数据,并验证了该方法的有效性和实用性。  相似文献