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  • AMS (American Meteorological Society)  (1)
  • American Institute of Physics (AIP)  (1)
  • Oxford :Taylor & Francis Group,  (1)
  • Public Library of Science  (1)
Publisher
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Years
  • 1
    Keywords: Astronomy, Chinese-History. ; Electronic books.
    Description / Table of Contents: This book offers a new insight into one of the most interesting and long-lived institutions known to historians of science, the Chinese imperial Astronomical Bureau, which for two millennia observed, recorded, interpreted and predicted the movements of the celestial bodies.
    Type of Medium: Online Resource
    Pages: 1 online resource (276 pages)
    Edition: 1st ed.
    ISBN: 9781000728224
    Series Statement: Needham Research Institute Series
    DDC: 520.951
    Language: English
    Note: Intro -- List of Tables -- List of Figures -- Acknowledgments -- Reign Titles of the Qing Emperors (1644-1911) -- 1 Introduction -- 2 The Organization of the Qing Astronomical Bureau -- 3 From the Old Method to the New Method -- 4 Kangxi Calendar Dispute -- 5 Emperors and the He Brothers -- 6 The Solar Eclipse of 1730 -- 7 Knowledge Reproduction -- 8 Maintaining a Familial Career -- 9 The Decline of Missionary Influence and the Nineteenth-Century Reforms of the Astronomical Bureau -- 10 Conclusion -- Appendix A Reconstructed Family Tree of the Baos 204 -- Appendix B The Ge Family -- Appendix C The He Family -- Appendix D The Zhou Family -- Appendix E The Huang Family -- Appendix F The Si Family -- Appendix G Register of Metropolitan Officials According to the Shunzhi Imperial Screen -- Appendix H Units Used in the Qing Era -- Index.
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  • 2
    Publication Date: 2022-05-26
    Description: © The Author(s), 2017. This article is distributed under the terms of the Creative Commons Attribution License. The definitive version was published in PLoS ONE 12 (2017): e0184849, doi:10.1371/journal.pone.0184849.
    Description: Diatoms are important components of marine ecosystems and contribute greatly to the world's primary production. Despite their important roles in ecosystems, the molecular basis of how diatoms cope with oxidative stress caused by nutrient fluctuations remains largely unknown. Here, an isobaric tags for relative and absolute quantitation (iTRAQ) proteomic method was coupled with a series of physiological and biochemical techniques to explore oxidative stress- and cell fate decision-related cellular and metabolic responses of the diatom Thalassiosira pseudonana to nitrate (N) and inorganic phosphate (P) stresses. A total of 1151 proteins were detected; 122 and 56 were significantly differentially expressed from control under N- and P-limited conditions, respectively. In N-limited cells, responsive proteins were related to reactive oxygen species (ROS) accumulation, oxidative stress responses and cell death, corresponding to a significant decrease in photosynthetic efficiency, marked intracellular ROS accumulation, and caspase-mediated programmed cell death activation. None of these responses were identified in P-limited cells; however, a significant up-regulation of alkaline phosphatase proteins was observed, which could be the major contributor for P-limited cells to cope with ambient P deficiency. These findings demonstrate that fundamentally different metabolic responses and cellular regulations are employed by the diatom in response to different nutrient stresses and to keep the cells viable.
    Description: This study was funded by the National Natural Science Foundation of China (41576138, 41076080, 41576138) to Dr. Jun-Rong Liang; the Woods Hole Center for Oceans and Human Health, National Science Foundation (OCE-1314642) to Dr. DonaldM Anderson; the National Institute of Environmental Health Sciences (1-P01-ES021923- 01) to Dr. DonaldM Anderson; and the ERC Advanced Award Diatomite and ANR project DiaDomOil to Dr. Chris Bowler.
    Repository Name: Woods Hole Open Access Server
    Type: Article
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  • 3
    Publication Date: 2019-02-01
    Description: Well-known problems trouble coupled general circulation models of the eastern Atlantic and Pacific Ocean basins. Model climates are significantly more symmetric about the equator than is observed. Model sea surface temperatures are biased warm south and southeast of the equator, and the atmosphere is too rainy within a band south of the equator. Near-coastal eastern equatorial SSTs are too warm, producing a zonal SST gradient in the Atlantic opposite in sign to that observed. The U.S. Climate Variability and Predictability Program (CLIVAR) Eastern Tropical Ocean Synthesis Working Group (WG) has pursued an updated assessment of coupled model SST biases, focusing on the surface energy balance components, on regional error sources from clouds, deep convection, winds, and ocean eddies; on the sensitivity to model resolution; and on remote impacts. Motivated by the assessment, the WG makes the following recommendations: 1) encourage identification of the specific parameterizations contributing to the biases in individual models, as these can be model dependent; 2) restrict multimodel intercomparisons to specific processes; 3) encourage development of high-resolution coupled models with a concurrent emphasis on parameterization development of finer-scale ocean and atmosphere features, including low clouds; 4) encourage further availability of all surface flux components from buoys, for longer continuous time periods, in persistently cloudy regions; and 5) focus on the eastern basin coastal oceanic upwelling regions, where further opportunities for observational–modeling synergism exist.
    Type: Article , PeerReviewed , info:eu-repo/semantics/article
    Format: text
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  • 4
    Publication Date: 2014-06-28
    Description: A nonlinear theory is developed to describe the cylindrical Richtmyer-Meshkov instability (RMI) of an impulsively accelerated interface between incompressible fluids, which is based on both a technique of Padé approximation and an approach of perturbation expansion directly on the perturbed interface rather than the unperturbed interface. When cylindrical effect vanishes (i.e., in the large initial radius of the interface), our explicit results reproduce those [Q. Zhang and S.-I. Sohn, Phys. Fluids 9, 1106 (1996)] related to the planar RMI. The present prediction in agreement with previous simulations [C. Matsuoka and K. Nishihara, Phys. Rev. E 73 , 055304(R) (2006)] leads us to better understand the cylindrical RMI at arbitrary Atwood numbers for the whole nonlinear regime. The asymptotic growth rate of the cylindrical interface finger (bubble or spike) tends to its initial value or zero, depending upon mode number of the initial cylindrical interface and Atwood number. The explicit conditions, directly affecting asymptotic behavior of the cylindrical interface finger, are investigated in this paper. This theory allows a straightforward extension to other nonlinear problems related closely to an instable interface.
    Print ISSN: 1070-664X
    Electronic ISSN: 1089-7674
    Topics: Physics
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