996 resultados para Wang, Yiyuan.
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Sans nom d'auteur ni date.
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Sans nom d'auteur ni date.
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Vieille édition avec illustrations en haut des pages.Livre 20 et début du livre 21 (hui 99 à 102).
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Figures de l'éclipse de lune du 7 avril 1735. Textes mantchou et Chinois ; figures de l'éclipse pour diverses provinces.
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Par le P. Verbiest (1669), contre Yang Guang xian. Notes dans la marge supérieure.
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Par le P. Verbiest (1669) ; texte avec annotations dans la marge supérieure. Gravé de nouveau à Canton, au Da yuan tang.
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Dirigée contre Yang Guang xian et les devins, par le P. Verbiest (1669). Gravé de nouveau à Canton, au Da yuan tang.A la table, 17sections ; manquent les sections 3 à 17 ; toutefois le volume, paraît complet. — Cordier, Imprimerie Sino-européenne, 358.
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Contient : I刪註脈訣規正Shan zhu mo jue gui zheng.Le Mo jue corrigé ; II圖註八十一難經Tu zhu ba shi yi nan jing.Le Nan jing illustré, en 81 sections
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Contient : I闢釋氏諸妄Pi shi shi zhu wang ; II闢畧說條駁Pi lüe shuo tiao bai
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Office des morts.Par le P. Buglio, avec introduction.28 feuillets.
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One of the primary goals of the Center for Integrated Space Weather Modeling (CISM) effort is to assess and improve prediction of the solar wind conditions in near‐Earth space, arising from both quasi‐steady and transient structures. We compare 8 years of L1 in situ observations to predictions of the solar wind speed made by the Wang‐Sheeley‐Arge (WSA) empirical model. The mean‐square error (MSE) between the observed and model predictions is used to reach a number of useful conclusions: there is no systematic lag in the WSA predictions, the MSE is found to be highest at solar minimum and lowest during the rise to solar maximum, and the optimal lead time for 1 AU solar wind speed predictions is found to be 3 days. However, MSE is shown to frequently be an inadequate “figure of merit” for assessing solar wind speed predictions. A complementary, event‐based analysis technique is developed in which high‐speed enhancements (HSEs) are systematically selected and associated from observed and model time series. WSA model is validated using comparisons of the number of hit, missed, and false HSEs, along with the timing and speed magnitude errors between the forecasted and observed events. Morphological differences between the different HSE populations are investigated to aid interpretation of the results and improvements to the model. Finally, by defining discrete events in the time series, model predictions from above and below the ecliptic plane can be used to estimate an uncertainty in the predicted HSE arrival times.