931 resultados para Siglos IV-V
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合成三个系列的新型表面活性剂，制备了三个系列的聚乙烯接枝共聚物。第一系列的表面活性剂是将Tween8O、span80，聚氧乙烯肉桂醇醚，PEO（400），PEO（1000），PEO（2000）OCOC1’7H35和PEO（6000）-OCOC17H35引入双键而使其功能化，然后接枝到聚乙烯分子链上，表面活性剂的引入改变了聚乙烯的表面性能，使其亲水性增加。前三者为商品防雾滴剂，实验发现防雾滴剂的聚乙烯接枝共聚物膜的防雾滴性不如物理共混法制备的聚乙烯防雾滴膜的效果好。接枝聚乙烯共聚物LLDPE-g-PEO和LLDPE-g-PEO-sterate，由于结构差别，共聚物表面组成不同。前者随着支链长度的增加，支链柔性降低，共聚物表面氧的富集量趋于减少；而后者由于疏水基硬脂酸中碳链的存在，随着支链的增加，共聚物表面氧的富集量增加。LLDPE-g-PEO（400）和LLDPE-g-PEO（1000）的等温结晶速率都比空白聚乙烯的快。由于PEO与聚乙烯不相容，支链PEo在接枝共聚物中起异相成核剂的作用，使结晶速率加快。LLDPE-g-PEO（2000）-stearate的等温结晶速率与聚乙烯的接近，但比空白聚乙烯的略慢。这是由于支链末端硬脂酸碳链是柔性的疏水链，且与聚乙烯有较好的相容性，在本体聚乙烯非晶区中活动性较强，带动聚氧乙烯支链向相同的方向运动，使支链在聚乙烯中分散且伸展，对聚乙烯分子起惰性稀释剂的作用而导致结晶速率降低；但聚氧乙烯（2000）又具有结晶性，在本体聚乙烯中起异相成核剂的作用，使聚乙烯结晶速率加快，这两种作用消长的结果，使LLDPE-g-PEO（2000）-stearte接枝共聚物的结晶速率接近聚乙烯，但比聚乙烯的结晶速率略慢。LLDPE-g-PEO（6000）-stearate接枝共聚物的结晶速率比聚乙烯的快，这是由于聚氧乙烯（6000）的结晶性较强，活动性较强的硬脂酸基团很难使其伸展，其晶粒在本体聚乙烯中主要起异相成核剂的作用，导致其结晶速率比聚乙烯的快。为了弄清表面活性剂接枝到大分子链上的作用机理，特设计第二、第三系列的表面活性剂。第二系列的新型表面活性剂是I、II、III、IV和V，以及含有不饱和键的表面活性剂A-I、A-II和A-III。这些表面活性剂是以聚乙二醇、乙二醇、1，6-己二醇和1，10-癸二醇为主要的起始原料制得的。实验结果发现这些表面活性剂的表面张力随着疏水链长度的增加而增加。以A-I、A-II和A-II作为接枝单体，将其成功接枝到聚乙烯分子链上，从而改善了聚乙烯的表面性能。 由FTIR确定了其接枝率。由DSc对其等温结晶行为的研究发现：接枝链在本体聚合物中起异相成核剂的作用，加速了结晶过程，但没有改变聚乙烯晶格结构（WXA）。随着接枝链中的疏水链长度的增加，等温结晶速率加快。在低剪切速率时，空白聚乙烯具有牛顿流体的特性，而接枝聚乙烯表现出非牛顿流体行为。接枝聚合物在低剪切速率具有剪切变稠、高剪切速率时剪切变稀的现象。第三系列的新型表面活性剂是含氟和聚氧乙烯的特种表面活性剂：productIII（600-4600）。以FTIR和1HNMR表征其结构。以productIII（600-4600）为接枝单体，成功制得含氟接枝聚乙烯共聚物，亲水性表面活性剂的引入，同样改变了聚乙烯的表面性能。当PEO分子量较低时，含氟接枝聚乙烯共聚物的表面极性随着接枝链的分子量增加，极性增加，在ProductIII（1500）时，达到最大值，分子量继续增加，极性反而降低。这是由于支链结晶增加而影响分子链的迁移。含氟接枝聚乙烯共聚物的等温结晶速率比空白LLDPE的高，而且接枝共聚物的结晶速率随着支链分子量的增加而加快。这是由于含氟聚氧乙烯的接枝链在结晶体系中起成核剂的作用，使结晶过程加速。由于接枝率低，接枝链在接枝共聚物起异相成核剂的作用，虽然加速了结晶速率，但没有破坏聚乙烯晶格。
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本论文“分光光度法则测定钛和钒的价态”包括互相独立的两部分工作：一、关于钛，经比较选用2－噻吩甲酰三氟丙酮作为Ti(III)的显色剂。在含二氯化锡的盐酸介质中，形成具有M:R = 1:3的稳定络合物，在685和485nm处有两个吸收峰，摩尔吸光系数分别为1.10 * 10~3和1.79 * 10~3。在685nm处测定Ti(III)有很高的选择性，百倍量的Ti(IV)和除氧化剂外的毫克量的多数常见离子无影响。0－300微克Ti(III)/10毫升范围内遵守比尔定律。应用本法测定了三氯化钛氧化剂和异丙橡胶中的Ti(III)和Ti(IV)。另外建立了新的配制和保存Ti(III)标准溶液的方法。二、关于钒、用磷钼杂多酸－罗丹明B作试剂，在存在聚乙烯醇的情况下，水相分光光度测定了三、四、五价钒。V（▽）与试剂形成四元络合物R_4[Mo_(11)V(▽)PO_(40)], V(IV)无显色反应，V(III)还原磷钼杂多酸成磷钼等，再与罗凡明B形成三元络合物R_5[Mo_(10)(VI)Mo_2(▽)PO_(40)]，过剩磷钼杂多酸由加入柠檬酸掩蔽。当V(IV)与V(▽)共存时，将其氧化成V(▽)，测合量后减去V(▽)而得V(IV)含量；当V(IV)与V(III)共存时，将其还原成V(III)，测合量后减去V(III)而得V(IV)含量。试剂最大吸收峰在555nm，两种络合物最大吸收峰都在586nm处，络合物的摩尔吸光系数分别为2.80 * 10~5和2.16 * 10~5。0-3.0微克V(▽)和0-4.0微克V(III)/25毫升遵守比尔定律。仅钛、锆、铌和钽及氧化、还原剂有影响。一个体系能高灵敏的测定三、四、五价钒，本工作还是首次。
Resumo:
Three novel polyoxometalate derivatives decorated by transition metal complexes have been hydrothermally synthesized. Compound 1 consists of [(PMo6Mo2V8O44)-Mo-VI-V-V-O-IV{CO (2,2'-bipy)(2)(H2O)}(4)](3+) polyoxocations and [(PMo4Mo4V8O44)-Mo-IV-V-V-O-IV{Co(2,2'-bipy)(2)(H2O)}(2)](3-) polyoxoanions, which are both built on mixed-metal tetracapped [PMo8V8O44] subunits covalently bonded to four or two {Co(2,2'-bpy)(2)(H2O)}(2+), clusters via terminal oxo groups of the capping V atoms. Compound 2 is built on [(PMo8V6O42)-V-VI-O-IV{Cu-I(phen)}(2)](5-) clusters constructed from mixed-metal bicapped [(PMo8V6O42)-V-VI-O-IV](7-) subunits covalently bonded to two {Cu(phen)}(+) fragments in the similar way to 1. The structure of 3 is composed of [(PMo9Mo3O40)-Mo-VI-O-V](6-) units capped by two divalent Ni atoms via four bridging oxo groups.
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Three new cage-like mixed-valent polyoxovanadates [Ni(1,10'-phen)(3)](2)[V10O26] 1, [Zn(2,2'-biPY)(3)](3)[V15O36Cl](.)3H(2)O (2) and [Co(2,2'-biPY)(3)](3)[V15O36Cl](.)3H(2)O (3) have been hydrothermally synthesized for the first time and characterized by elemental analyses, IR, EPR spectra, TG analyses and single crystal X-ray diffraction. The polyoxoanion of I exhibits an interesting empty ellipsoidal [V-2(IV) V-8(V) O-26](4-) 'host' shell, while the oxo vanadium clusters of 2 and 3 possess a spherical [V-8(IV) V-7(V) O36Cl](6-) cage with a Cl- ion encapsulated. The structure-directing role of organic templates (1,10'-phen and 2,2'-bipy) on the formation of the polyoxoanion structures is discussed.
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上芒岗金矿床位于三江褶皱系怒江大断裂西南段，龙陵～瑞丽大断裂(F_1)南东盘，上芒岗次级断裂(F_4)之中。赋矿地层为下二叠统沙子坡组(P_(1s))和中侏罗统勐嘎组(J_(2m))。矿石主要有两种类型，硅质矿石和粘土质矿石；前者主要由石英和少量黄铁矿所组成，金品位平均为2 * 10~(-6)；后者主要由伊利石、高岭石和黄铁矿所组成，金品位一般为2 * 10~(-6) ～ 4 * 10~(-6)。矿石中金星次显微状态，主要元素组合为Au、Ag、As、Sb、Hg、Ba。矿床以强烈的黄铁粘土岩化为特征，热液蚀变作用过程即是金矿化作用过程。根据热液蚀变的矿物共生组合及其生成序次，将金矿化作用过程分为五个阶段：黄铁矿-石英阶段(I)；镁贝得-白云石阶段(II)；辉锑矿-石英阶段(IlI)：黄铁矿-高岭石-伊利石阶段(IV)；网脉状石英阶段(V)。其中黄铁矿-高岭石-伊利石阶段(IV)是金矿化的主成矿阶段。该矿床属于卡林型金矿床。由石英流体包裹体获得不同成矿阶段的温度为，成矿阶段I：210～170 ℃、成矿阶段III：190～160 ℃、成矿阶段V：173～144 ℃。伊利石-水氢同位素温度计测得成矿阶段IV的温度为165 ℃。石英流体包裹体液相成分以K~+、Na~+和Cl~- (F~-)为主，其次为Ca~(2+)、Mg~(2+)和HC0_3~-，由早到晚K~+、Na~+和Cl~-降低，而Ca~(2+)、Mg~(2+)和HC0_3~-升高；气相组分以C0_2为主。石英流体包裹体成分富F，其含量高达8.03 * 10~(-3) mol／kg，正是由于成矿热液富含F，Al才可以与F形成络合物进入热液迁移，即Al成为活动组份，从而形成该矿床所独特的强烈粘土岩化蚀变。稀土元素特征方面，矿石和赋矿地层下二叠统沙子坡以及中侏罗统勐嘎组岩石的稀土配分曲线十分相似，均为右倾型，但是两者的稀土元素总量不同，前者的相对较高。矿石和蚀变岩具有相似的稀土元素配分曲线，但是矿石的稀土元素总量相对较高。与勐嘎组泥岩相比，粘土质蚀变岩和矿石更加富集轻稀土元素，并且更富Eu。这些特征表明，粘土质蚀变岩和矿石是由热液作用形成的，而不是风化作用的产物；矿石与赋矿地层在物质来源上有亲缘关系。不同矿段、不同阶段和不同类型矿石和蚀变岩的Au、Ag、As以及Sb的含量同步变化，这表明在整个成矿作用过程中，成矿流体来源统一，且在成矿体系起主导作用。不同类型的矿石及蚀变岩中Au与Al_20_3，和TFe的含量呈正相关，表明黄铁粘土岩化与成矿关系最为密切。矿石铅同位素~(208)Pb／~(204)Pb、~(207)Pb／~(204)Pb和~(206)Pb/~(204)Pb比值分别为39.12～39.54、15.85～15.95、19.75～20.33；沙子坡组(P_(1s))岩石铅同位素比值分别为:38.407～37.868、15.921～15.589、22.685～22.367;孟嘎组(J_(2m))岩石铅同位素比值分别为：39.499～39.222，15.821～15.772、19.207～18.709。在铅同位素组成相关图中矿石与地层铅的投影点分别集中成群分布。矿石铅与地层铅呈线性分布，而且矿石铅的集中区位于沙子坡组铅集中区和勐嘎组铅集中区之间。这些特征表明矿石铅系由沙子坡组铅和勐嘎组铅混合而成。成矿热液的δ~(18)O由早到晚逐渐升高，I、III、IV、V阶段流体的δ~(18)O值分别为-4.2‰，+0.59‰；+0.76‰，+1.98‰，表现出明显的漂移特征；而δD则表现出高度的一致性，变化范围为-82.5 ～ 79.48‰。由此认为成矿热液系大气降水起源。成矿热液氢、氧同位素组成的这种规律性变化还说明，成矿热液的演化具有继承性和连续性。应用CHILLERR软件包，对上芒岗金矿床的成矿作用过程进行化学反应途径数字模拟。所展示的成矿作用过程为：大气降水沿断裂带下渗，加热循环，获取成矿物质(但不排除有深源成矿物质加入的可能性)；形成起始成矿热液：T = 200℃ P = 228.8bar；pH = 4.4；fs_2 = 10~(-9.89); fo_2 = 10~(-41.28)；aAu(HS)_2~- = 10~(-9.64)，aAuCl_2~- = 10~(-17.86);富含F、Al和Au，贫As、Hg、Zn、Cu和Pb。成矿热液在构造作用的驱动下，上升进入上芒岗断裂上部含水构造破碎带，并与下渗雨水混合而淬冷，形成沿上芒岗断裂呈线状分布的早期硅化石英岩(成矿阶段I)，成矿热液与下渗雨水之比为16:l(成矿阶段I)；继而热液扩散进入下盘破碎带，与白云岩反应，形成矿体下盘的白云石化，水:岩比为193:l(成矿阶段II)。此后成矿热液上升充填裂隙空间，由于热传导而缓慢冷却，成矿体系的温度由189 ℃降为165 ℃，形成含辉锑矿的梳状石英脉(成矿阶段1II)。成矿热液继续上升进入上盘碎屑岩破碎带，停积于构造揉皱的泥质岩，并与之反应，形成上芒岗矿床金矿化的主体—粘占土质矿石，水:岩比为29:1(成矿阶段IV)。最后成矿残液逐渐冷却, 同时伴随C0_2的起泡，形成晚期石英网脉(成矿阶段V)，至此热液金矿化过程结束。由上述可见上芒岗金矿床的成矿作用过程经历了：(初始)成矿热液与下渗大气降水混合(I) → 成矿热液与沙子坡组白云岩反应(II) → 成矿热液缓慢冷却(III) → 成矿热液与勐嘎组泥质岩石反应(IV) → 成矿热液冷却沸腾(V)等5个演化阶段。模拟结果进一步证实了上芒岗金矿床的热液成因。上芒岗金矿床成作用过程化学反应途径数字模拟与地质事实高度吻合，与地球化学研究结果相互印证，再现了上芒岗金矿床的成矿作用过程。由矿床的地质地球化学特征及成矿作用过程化学反应途径模拟结果，归纳出上芒岗金矿床成矿作用过程模型。
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New R-matrix calculations of electron impact excitation rates for Fe XI are used to determine theoretical emission line ratios applicable to solar and stellar coronal observations. These are subsequently compared to solar spectra of the quiet Sun and an active region made by the Solar EUV Rocket Telescope and Spectrograph (SERTS-95), as well as Skylab observations of two flares. Line blending is identified, and electron densities of 10(9.3), 10(9.7), greater than or equal to 10(10.8), and greater than or equal to 10(11.3) cm(-3) are found for the quiet Sun, active region, and the two flares, respectively. Observations of the F5 IV-V star Procyon, made with the Extreme Ultraviolet Explorer (EUVE) satellite, are compared and contrasted with the solar observations. It is confirmed that Procyon's average coronal conditions are very similar to those seen in the quiet Sun, with N-e = 10(9.4) cm(-3). In addition, although the quiet Sun is the closest solar analog to Procyon, we conclude that Procyon's coronal temperatures are slightly hotter than solar. A filling factor of 25(-12)(+38)% was derived for the corona of Procyon.
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El presente trabajo intenta mostrar de qué manera Plotino refuta la noción aristotélica del tiempo como «número» o «medida del movimiento», cuáles son las aporías que plantea, cómo las compulsa con sus propios argumentos y qué soluciones propone con respecto a esa misma confrontación. Todo esto será encauzado a partir de un estudio descriptivo y analítico, acompañado de una lectura a la vez hermenéutica y crítica de los textos seleccionados para esta ocasión.
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Emission line fluxes from cool stars are widely used to establish an apparent emission measure distribution, EmdApp(Te), between temperatures characteristic of the low transition region and the low corona. The true emission measure distribution, EmdTrue(Te), is determined by the energy balance and geometry adopted and, with a numerical model, can be used to predict EmdApp(Te), to guide further modelling. The scaling laws that exist between coronal parameters arise from the dimensions of the terms in the energy balance equation. Here, analytical approximations to numerical solutions for EmdTrue(Te) are presented, which show how the constants in the coronal scaling laws are determined. The apparent emission measure distributions show a minimum value at some T0 and a maximum at the mean coronal temperature Tc (although in some stars, emission from active regions can contribute). It is shown that, for the energy balance and geometry adopted, the analytical values of the emission measure and electron pressure at T0 and Tc depend on only three parameters: the stellar surface gravity and the values of T0 and Tc. The results are tested against full numerical solutions for e Eri (K2 V) and are applied to Procyon (a CMi, F5 IV/V). The analytical approximations can be used to restrict the required range of full numerical solutions, to check the assumed geometry and to show where the adopted energy balance may not be appropriate. © 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS.
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The importance of partial redistribution (PRD) in the modelling of the Lyman a and Lyman ß emission lines of hydrogen in stellar atmospheres is examined using simple atmospheric models of a range of late-type stars. These models represent the subgiant Procyon (F5 IV-V), and the two giants ß Gem (K0 III) and a Tau (K5 III). These stars are selected to span a wide range of surface gravities: 1.25 <log g <4.00. The calculations are performed using the computer code MULTI with the modifications made by Hubeny & Lites. It is found that PRD effects are highly significant, both in the direct prediction of the Lyman line profiles and in the application of hydrostatic equilibrium to calculate the atmospheric electron density in static atmospheric models.
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Despite previous attempts at codification of international law regarding international responses to natural and human-made disasters, there is currently no binding international legal framework to regulate the provision of humanitarian assistance outside armed conflicts. Nevertheless, since the International Law Commission (ILC) included the protection of persons in the event of disasters on its programme of work in 2006, it has provisionally adopted eleven draft articles that have the potential to create binding obligations on states and humanitarian actors in disaster settings. Draft articles adopted include the definition of ‘a disaster’, the relationship of the draft articles to the international humanitarian law of armed conflict, recognition of the inherent dignity of the human person, and the duty of international cooperation. However, the final form of the draft articles has not been agreed. The Codification Division of the UN Office of Legal Affairs has proposed a framework convention format, which has seen support in the ILC and the UN General Assembly Sixth Committee. The overall aim of this article is to provide an analysis of the potential forms of international regulation open to the ILC and states in the context of humanitarian responses to disasters. However to avoid enchanting the ILC draft articles with unwarranted power, any examination of form requires an understanding of the substantive subject matter of the planned international regulation. The article therefore provides an overview of the international legal regulation of humanitarian assistance following natural and human-made disasters, and the ILC’s work to date on the topic. It then examines two key issues that remain to be addressed by the ILC and representatives of states in the UN General Assembly Sixth Committee. Drawing on the UN Guiding Principles on Internal Displacement, the development and implications of binding and non-binding international texts are examined, followed by an analysis of the suggested framework convention approach identified by the Special Rapporteur as a potential outcome of the ILC work.
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Embora o objetivo principal da proteção internacional dos solos seja proteger tanto as funções quanto a estrutura do solo, a atual abordagem trata principalmente da proteção ao nível estrutural. Há uma carência de estudos que contemplem a ligação das funções do solo com os níveis da comunidade. Além disso, é ainda desconhecido se as variáveis ambientais (ex: tipos de solo, condições climáticas) atuam nas funções do solo da mesma maneira que influenciam sua estrutura biológica. Ademais, as alterações climáticas poderão ter sozinhas ou combinadas com os poluentes, um grande efeito nos ecossistemas terrestres. O presente trabalho propõe estudar as funções e a estrutura biológica do solo quando impactados devido a estresse tóxico (poluição por Cu) e/ou alterações a fatores como a temperatura e abundância de organismos, de maneira a simular possíveis variações regionais ou climáticas. Para alcançar os objetivos principais 3 experiências utilizando diferentes densidades de E. crypticus e 2 gerações foram feitas (Capítulos II e III). Duas experiências com mesocosmos (SMS) decorreram durante 3 meses sob uma gama de diversas temperaturas (10 – 29°C), que representam temperaturas médias para Portugal e Dinamarca (Capítulos IV e V). Duas experiências de campo também foram realizadas com intuito de validar os SMSs (Capítulo VI). Resultados demonstraram que os efeitos do Cu na reprodução dos enquitraídeos dependem da densidade inicial de organismos, especialmente na 2ª geração. Entretanto, nos SMSs expostos a Cu, a densidade inicial é menos importante nos resultados finais. O aumento da temperatura alterou majoritariamente a fase inicial de crescimento populacional. Em períodos mais longos, a abundância estabilizou tornando-se menos influenciada pelas temperaturas. Períodos longos de exposição reforçaram os efeitos da temperatura, como por ex: diversas espécies foram similarmente afetadas a 29 ou 26°C quando expostas durante 28 ou 61 dias respectivamente. De forma geral, o Cu reduziu a abundância da maioria das espécies ao longo do tempo, com poucas exceções. Os resultados da decomposição da matéria orgânica (MO) e atividade alimentar associaram-se com a abundância de organismos em baixas temperaturas (10-23°C). Entretanto, com o aumento das temperaturas (19-29°C), este comportamento não foi claro e a abundância de espécies e atividade alimentar diminuíram enquanto a decomposição da MO aumentou. Além disso, os resultados observados nos SMSs foram confirmados no campo. Mais especificamente, alterações ocorreram na fase de crescimento (correspondente à Primavera) e a exposição ao Cu diminuiu os efeitos da temperatura. Metodologias mais complexas (ex: mais gerações e experiências com múltiplas espécies) apresentam muitos benefícios, mas também proporcionam respostas mais complexas, as quais exigem um maior “peso” de evidências para serem comprovadas.
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F. 1-8 De vitio proprietatis religiosorum. « Jhesus, Maria, Franciscus. Sequitur... vicio proprietatis religiosorum » (titre effacé, lisible en partie à la lumière ultra-violette). « Manifestum videtur esse quod persone religiose viri et femine ordinem approbatum professe pro proprietatis vicio alligate nullo modo possint salvari... — ... nec continue. Vide Johannem Andree in regulam Non est obligatorium in novella super librum sextum et sic est finis ». F. 9-279 [BARTHOLOMAEUS DE RINONICO PISANUS] Liber de conformitatibus. « Incipit liber de conformitatibus beati Francisci quamvis plurimum breviatus tres partiales libros complectens... » (éd. dans Analecta franciscana sive chronica, IV-V, Quaracchi, 1906-1912). L. I, Conformitatum I-XII secundae partes : « Prima conformitas. Franciscus declaratur, expositio sequitur. Declarata prima parte primi fructus conformitatis que fuit de Christo (que [sic] ego pro nunc scribere non intendo sed solum que spectant ad beatum Franciscum etc.) manifestat nunc consequenter secundam partem ipsius enodare... — ... lucem Christum perveniamus. Amen. Sic ergo prelibatis apparet declarata secunda pars istius 12mi [sic] conformitatis videlicet Franciscus reserator... tam in isto duodecimo quam in precedentibus et subsequentibus conformitatibus sit laus Deo. Amen » (éd. cit., IV, 33-60, 69-82, 95-100, 108-113, 116-124, 138-149, 156-164, 175-364, 369-457, 464-485, 493-564, 580-632) (9-177v) ; — L. II, Conformitates I-XII, incomplet : « Incipit secundus liber et sequitur secunda pars prime conformitatis secundi libri videlicet Franciscus divulgatur. Expositio. Magister summus et verax... — ... patet ad fratres » (177v-224v), avec variantes et lacunes : Conformitas I, pars 2, incomplète de la fin par lacune matérielle (ibid., V, 10-13) (177v-178v) ; II et III, manquent par lacune matérielle ; IV, pars 2 (ibid., 100-123) (179-189) ; pars 1, fragm. (ibid., 97-100) (189-190v) ; V, texte abrégé (ibid., 123-144) (190v-199v) ; VI, pars 2, texte abrégé (ibid., 159-182) (199v-206) ; VII, pars 2, texte abrégé (ibid., 189-198) (206-208v) ; VIII, pars 2, texte abrégé (ibid., 208-211) (208v-209v) ; IX, texte abrégé (ibid., 211-226) (209v-213) ; X, pars 2 (ibid., 232-233) (213-214) ; XI, texte abrégé (ibid., 233-259) (214-224) ; XII, pars 2, texte abrégé (ibid., 275-277) (224-224v) ; — L. III, Conformitates I-IX, incomplet de la fin : « Incipit liber tercius de conformitate vite beati Francisci ad vitam Jhesu Christi. Fructus primus et conformitas et 2us in ordine Jhesus cum suis comedens, Franciscus emulatur. Expositio prime partis... Virtus illa et sapientia divina qua omnia a Deo fiunt... — ... ad orandum. Lc. XI in quo fuit captus... » (ibid., 333-459) (225-279). Ce texte a été aussi publié sous le nom de BARTHOLOMAEUS ALBISIUS PISANUS ; cf. Sbaralea, Supplementum, I, 114-117. Au contreplat supérieur, cote : « 87 » de l'inventaire après décès de Claude Hardy ; cf. ms. Latin 9363, f. 139. Acheté par Baluze pour la bibliothèque de Colbert ; cf. ibid., f. 145v et add. du ms. Latin 3114A.
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Contient : IDa xi xi tai li xian sheng xing ji ; II思及先生行蹟Si ji xian sheng xing ji ; III思及艾先生語錄Si ji ai xian sheng yu lu ; IV V楊淇園先生事蹟Yang qi yuan xian sheng shi ji.Vie de Yang Qi yuan ; VI-VIII張彌格爾遺蹟Zhang mi ke er yi ji ; IX悌尼削世紀Di ni xiao shi ji.Vie de Denis
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Contient : I創世歴代傳Zhuan shi li dai zhuan ; II出以至比多地傳Chu yi zhi bi duo di zhuan ; III利未氐古傳書（alias 書傳）Li wei di gu chuan shu (alias shu zhuan) ; IV算民數書傳 ; V複講法律傳Fou jiang fa lü zhuan ; VI若書亞之傳Ruo shu ya zhi zhuan ; VII審司書傳Shen si shu zhuan ; VIII路得氏傳書Lu de shi chuan shu ; IX撒母以勒書Sa mu yi le shu ; X列王書傳Lie wang shu zhuan ; XI歷代史紀書傳Li dai shi ji shu zhuan ; XII以士拉傳書Yi shi la chuan shu ; XIII尼希米亞之書Ni xi mi ya zhi shu ; XIV以士得耳之書Yi shi de er zhi shu ; XV若百之書Ruo bo zhi shu ; XVI神詩書Shen shi shu ; XVII諺語傳書Yan yu chuan shu ; XVIII宣道傳Xuan dao zhuan ; alias : 倚基理西亞書Yi ji li xi ya shu ; XIX所羅門之歌Suo luo men zhi ge ; XX先知以賽亞書Xian zhi yi sai ya shu ; XXI先知耶利米亞書Xian zhi ye li mi ya shu ; alias : 達未來者耶利米亞傳書Da wei lai zhe ye li mi ya chuan shu ; XXII耶利米亞悲難歌Ye li mi ya bei tan ge ; XXIII先知依西其理書Xian zhi yi xi qi li shu ; XXIV先知（alias 達未來者）但依理書Xian zhi (alias Da wei lai zhe) dan yi li shu ; XXV十二先知者之傳書。何西亞之書Shi er xian zhi zhe zhi chuan shu. He xi ya zhi shu ; XXVI若以利之書Ruo yi li zhi shu ; XXVII亞麼士書Ya mo shi shu ; XXVIII阿巴氐亞書E ba di ya shu ; XXIX若拿傳書Ruo na chuan shu ; XXX米加傳書Mi jia chuan shu ; XXXI拿戶馬傳書Na hu ma chuan shu ; XXXII夏巴古傳書Xia ba gu chuan shu ; XXXIII洗法尼亞傳書Xi fa ni ya chuan shu ; XXXIV夏哀傳書Xia ai chuan shu ; XXXV洗革利亞傳書Xi ke li ya chuan shu ; XXXVI達未來者馬拉其傳書Da wei lai zhe ma la qi chuan shu ; XXXVII救世我主耶穌新遺詔書。聖馬竇傳福音書Jiu shi wo zhu ye su xin yi zhao shu. Sheng ma dou chuan fu yin shu ; XXXVIII聖馬耳可傳福音書Sheng ma er ke chuan fu yin shu ; XXXIX聖路加傳福音書Sheng lu jia chuan fu yin shu ; XL聖若翰傳福音之書Sheng ruo han chuan fu yin zhi shu ; XLI使徒行傳Shi tu xing zhuan ; XLII聖保羅使徒書Sheng bao luo shi tu shu ; XLIII者米士或稱牙可百之公書Zhe mi shi huo cheng ya ke bai zhi gong shu ; XLIV聖彼多羅之公書Sheng bi duo luo zhi gong shu ; XLV聖若翰之書Sheng ruo han zhi shu ; XLVI聖如大或稱如大士之公書Sheng ru da huo cheng ru da shi zhi gong shu ; XLVII聖若翰現示之書Sheng ruo han xian shi zhi shu
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Contient : I創世歴代傳Zhuan shi li dai zhuan ; II出以至比多地傳Chu yi zhi bi duo di zhuan ; III利未氐古傳書（alias 書傳）Li wei di gu chuan shu (alias shu zhuan) ; IV算民數書傳 ; V複講法律傳Fou jiang fa lü zhuan ; VI若書亞之傳Ruo shu ya zhi zhuan ; VII審司書傳Shen si shu zhuan ; VIII路得氏傳書Lu de shi chuan shu ; IX撒母以勒書Sa mu yi le shu ; X列王書傳Lie wang shu zhuan ; XI歷代史紀書傳Li dai shi ji shu zhuan ; XII以士拉傳書Yi shi la chuan shu ; XIII尼希米亞之書Ni xi mi ya zhi shu ; XIV以士得耳之書Yi shi de er zhi shu ; XV若百之書Ruo bo zhi shu ; XVI神詩書Shen shi shu ; XVII諺語傳書Yan yu chuan shu ; XVIII宣道傳Xuan dao zhuan ; alias : 倚基理西亞書Yi ji li xi ya shu ; XIX所羅門之歌Suo luo men zhi ge ; XX先知以賽亞書Xian zhi yi sai ya shu ; XXI先知耶利米亞書Xian zhi ye li mi ya shu ; alias : 達未來者耶利米亞傳書Da wei lai zhe ye li mi ya chuan shu ; XXII耶利米亞悲難歌Ye li mi ya bei tan ge ; XXIII先知依西其理書Xian zhi yi xi qi li shu ; XXIV先知（alias 達未來者）但依理書Xian zhi (alias Da wei lai zhe) dan yi li shu ; XXV十二先知者之傳書。何西亞之書Shi er xian zhi zhe zhi chuan shu. He xi ya zhi shu ; XXVI若以利之書Ruo yi li zhi shu ; XXVII亞麼士書Ya mo shi shu ; XXVIII阿巴氐亞書E ba di ya shu ; XXIX若拿傳書Ruo na chuan shu ; XXX米加傳書Mi jia chuan shu ; XXXI拿戶馬傳書Na hu ma chuan shu ; XXXII夏巴古傳書Xia ba gu chuan shu ; XXXIII洗法尼亞傳書Xi fa ni ya chuan shu ; XXXIV夏哀傳書Xia ai chuan shu ; XXXV洗革利亞傳書Xi ke li ya chuan shu ; XXXVI達未來者馬拉其傳書Da wei lai zhe ma la qi chuan shu ; XXXVII救世我主耶穌新遺詔書。聖馬竇傳福音書Jiu shi wo zhu ye su xin yi zhao shu. Sheng ma dou chuan fu yin shu ; XXXVIII聖馬耳可傳福音書Sheng ma er ke chuan fu yin shu ; XXXIX聖路加傳福音書Sheng lu jia chuan fu yin shu ; XL聖若翰傳福音之書Sheng ruo han chuan fu yin zhi shu ; XLI使徒行傳Shi tu xing zhuan ; XLII聖保羅使徒書Sheng bao luo shi tu shu ; XLIII者米士或稱牙可百之公書Zhe mi shi huo cheng ya ke bai zhi gong shu ; XLIV聖彼多羅之公書Sheng bi duo luo zhi gong shu ; XLV聖若翰之書Sheng ruo han zhi shu ; XLVI聖如大或稱如大士之公書Sheng ru da huo cheng ru da shi zhi gong shu ; XLVII聖若翰現示之書Sheng ruo han xian shi zhi shu
