Showing 61 - 80 results of 41,222 for search '"observation"', query time: 0.07s Refine Results
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    Revealing the limitations of 10-year MACE observations: 20-year observed total cardiovascular burden in the EPIC-Norfolk study by Frank LJ Visseren, Harald T Jorstad, Marjolein Snaterse, S Matthijs Boekholdt, Tinka J van Trier, Jannick AN Dorresteijn, Manon van den Bogaart, Wilma JM Scholte op Reimer, Ron JG Peters

    Published 2025-02-01
    “…Ratios between 10-year MACE and 20-year total CVD varied substantially, ranging from 3-fold in (older men) to 10-fold (younger women).Conclusions The observed incidence of CVD roughly triples from 10 to 20 years of follow-up, with 10-year MACE observations underestimating 20-year total CVD burden by a factor ranging from 3 (older men) to 10 (younger women). …”
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    The Impact of Assimilating Ionosphere and Thermosphere Observations on Neutral Temperature Improvement: Observing System Simulation Experiments Using EnKF by Jianhui He, Xinan Yue, Zhipeng Ren

    Published 2021-10-01
    “…In this work, the impact of different ionosphere and thermosphere observing systems on the improvement of neutral temperature of the data assimilation model has been investigated by a series of observing system simulation experiments. …”
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    Virtual Integration of Satellite and In-situ Observation Networks (VISION) v1.0: In-Situ Observations Simulator (ISO_simulator) by M. R. Russo, M. R. Russo, S. L. Bartholomew, S. L. Bartholomew, D. Hassell, D. Hassell, A. M. Mason, E. Neininger, A. J. Perman, D. A. J. Sproson, D. Watson-Parris, D. Watson-Parris, N. L. Abraham, N. L. Abraham

    Published 2025-01-01
    “…A standalone code, In-Situ Observations Simulator, or ISO_simulator for short, is described here: this software reads modelled variables and observational data files and outputs model data interpolated in space and time to match observations. …”
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    Sealing Capability and SEM Observation of the Implant-Abutment Interface by Fabio C. Lorenzoni, Paulo G. Coelho, Gerson Bonfante, Ricardo M. Carvalho, Nelson R. F. A. Silva, Marcelo Suzuki, Thelma Lopes Silva, Estevam A. Bonfante

    Published 2011-01-01
    “…Gaps in the implant-abutment interface were observed along with leakage increased at the 144 hrs evaluation period.…”
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    Observation of anomalously large Nernst effects in conducting polymers by Yingqiao Ma, Xinglong Ren, Ye Zou, Wenrui Zhao, Dongyang Wang, Zhen Ji, Juncheng Fan, Chaoyi Yan, Lanyi Xiang, Gaoyang Ge, Xiaojuan Dai, Fengjiao Zhang, Ting Lei, Henning Sirringhaus, Chong-an Di, Daoben Zhu

    Published 2025-02-01
    “…Here, we challenge this notion by observing an anomalously large Nernst effect in a range of conducting polymers. …”
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  15. 75

    Asymptotic Distribution of the Number for Error in the Time of Random Observation by Lu Chuanlai

    Published 1986-01-01
    “…In this paper, it is discussed that the distribution of sum for errors in the random time of observation is approached to a normal distribution, when the sequence {X1} of errors in an unit time is a m-dependent.…”
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    Observations of Radio Magnetars with the Deep Space Network by Aaron B. Pearlman, Walid A. Majid, Thomas A. Prince

    Published 2019-01-01
    “…We describe the DSN’s capabilities for carrying out these types of observations. We also present results from observations of three radio magnetars, PSR J1745–2900, PSR J1622–4950, and XTE J1810–197, and the transitional magnetar candidate, PSR J1119–6127, using the DSN radio telescopes near Canberra, Australia.…”
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    Evaluating Auroral Forecasts Against Satellite Observations by M. K. Mooney, M. S. Marsh, C. Forsyth, M. Sharpe, T. Hughes, S. Bingham, D. R. Jackson, I. J. Rae, G. Chisham

    Published 2021-08-01
    “…The operational implementation of the OVATION‐Prime 2013 model at the UK Met Office delivered a 30‐min forecast of the location of the auroral oval and the probability of observing the aurora. Using weather forecast evaluation techniques, we evaluate the ability of the OVATION‐Prime 2013 model forecasts to predict the location and probability of the aurora occurring by comparing the forecasts with auroral boundaries determined from data from the IMAGE satellite between 2000 and 2002. …”
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