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Business Continuity Management,Operational Resilience,and Organizational Resilience:Commonalities,Distinctions,and synthesis

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International Journal of Disaster Risk science 2023年第5期14卷 713-721页

作者： s.E.Galaitsi elizaveta Pinigina Jeffrey M.Keisler Gianluca Pescaroli Jesse M.Keenan Igor Linkov Us Army Engineer Research and Development Center VicksburgMS39180USA College of Management University of Massachusetts BostonBostonMA02125USA Institute for Risk and Disaster Reduction University College LondonLondonWC1E 6BTUK school of Architecture Tulane UniversityNew OrleansLA70118USA

The concepts of business continuity management,operational resilience,and organizational resilience each refer to actions that businesses and organizations can take in anticipating and responding to ***,the existing definitions and usages are difficult to differentiate due to overlapping objectives,implementation processes,and *** article examines definitions and approaches for these three concepts and suggest a framework to operationalize methods and tools relevant to *** definitions emphasize three dyads:risk versus resilience;organizational processes versus assets;and normal operating conditions versus crisis *** these dyads to differentiate the concepts of business continuity management,operational resilience,and organizational resilience can support planners in clarifying objectives and identifying which approach will be most beneficial as businesses or organizations plan for and encounter *** article evaluates these concepts by examining illustrative examples of disruptions and responses.

关键词： Business continuity management Disruptions Operational resilience Organizational resilience

Analysis of X-Ray Emission from OB stars. IV. About X-Ray Emission from Inhomogeneous Winds of OB stars

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Research in Astronomy and Astrophysics 2023年第10期23卷 387-405页

作者： elizaveta Ryspaeva Alexander Kholtygin Crimean Astrophysical Observatory NauchnyCrimeaRussia saint-Petersburg state University Saint-PetersburgRussia

We study the origin of X-ray emission from OB stars due to collisions of stellar winds and/or inhomogeneities in the winds. The low-resolution X-ray spectra of a big sample of OB stars were fitted by both the stationary APEC/MEKAL models and by this model with an additional PsHOCK component describing the nonstationary X-ray emission. These spectra were also described by two-temperature PsHOCK models. More than ~50% of considered spectra can be described by the above-mentioned model combinations including the PsHOCK model and the quality of the fits appears to be better for O stars. The plasma temperature of the PsHOCK component is about 1–5 keV with the ionization timescale τ_(u)~ 10^(8)–10^(13)s cm^(-3). The temperature of the PsHOCK component increases with the momentum and kinetic energy of the stellar wind by a power law with an index ~0.12–*** dependencies were not revealed through modeling by the stationary APEC/MEKAL models only. At the same time the X-ray luminosity of OB stars depends on momentum and kinetic energy of their winds similarly either for stationary or for nonstationary models. We conclude that many O stars and some B stars can be sources of the nonstationary X-rays formed in their inhomogeneous stellar wind.

关键词： stars:early-type stars:statistics X-rays:stars

Nitroxy-and azidomethyl azofurazans as advanced energetic materials

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Defence Technology（防务技术） 2022年第8期18卷 1369-1381页

作者： Aleksei B.sheremetev svetlana F.Mel'nikova elizaveta s.Kokareva Ruslan E.Nekrutenko Kirill V.strizhenko Kyrill Yu suponitsky Thanh Dat Pham Alla N.Pivkina Valery P.sinditskii Zelinsky Institute of Organic Chemistry Russian Academy of Sciences47 Leninsky ProspMoscow119991Russia saint Petersburg state Institute of Technology 26 Moskovskii PrSt Petersburg190013Russia Mendeleev University of Chemical Technology Moscow125047Russia N.N.semenov Federal Research Center for Chemical Physics Russian Academy of Sciences4 Kosygina Str119991MoscowRussia

Progress in the rocket industry is only possible on the basis of new, higher performance and more environmentally friendly materials compared to up-to-date propellant ingredients for liquid, solid, gelled and hybrid propellant systems. In this work, synthetic methods have been developed for the preparation of new energetic azofurazans bearing nitroxymethyl or azidomethyl groups. All prepared compounds were fully characterized by multinuclear NMR and IR spectroscopies, as well as elemental analyses. An analysis of the structural features based on the X-ray single-crystal diffraction made it possible to discuss their influence on the densities of the azofurazans of this study. Thermal decomposition and combustion of nitroxymethyl and azidomethyl azofurazans were studied using a number of complementary experimental techniques, namely thermogravimetry, differential scanning calorimetry, manometry, microthermocouple measurements in the combustion wave. The structural and physical characteristics of these new energetic analogues illustrate the extent to which the nature of the explosophoric groups can be used to tune the performace of the azofurazan framework. These azofurazans possess positive calculated enthalpy of formation and are promising candidates for new environmentally friendly energetic materials.

关键词： Azofurazan Azide Nitrate ester X-ray Combustion

Analysis of the X-ray emission of OB stars II: B stars

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Research in Astronomy and Astrophysics 2019年第8期19卷 143-150页

作者： elizaveta Ryspaeva Alexander Kholtygin Crimean Astrophysical Observatory NauchnyCrimeaRussia saint-Petersburg state University Saint-PetersburgRussia Institute of Astronomy Russian Academy of SciencesRussia

This paper is the second part of an investigation into the mechanism for the origin of X-rays in early-type stars. Archival X-ray observations of 25 B stars, obtained by the XMM-Newton satellite, are analysed. We check two hypotheses on the origin of X-ray emission: the Magnetically Confined Wind shock Model(MCWs) and Pollock’s paradigm. For all studied stars, the mean ratio of the half widths at half maximum to the terminal velocities appears to be R ≈ 0.15-0.20 in contradiction to Pollock’s hypothesis that R ≈ 0.5. We checked three possible consequences of the MCWs model: correlations between the hardness of the X-ray spectra for B stars and terminal wind velocities, mass loss rates and magnetic *** was shown that such correlations are marginal or even absent both for magnetic and non-magnetic B stars.

关键词： stars:early-type stars:spectra:X-ray

Analysis of the X-ray emission of OB stars:O stars

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Research in Astronomy and Astrophysics 2018年第8期18卷 121-134页

作者： elizaveta Ryspaeva Alexander Kholtygin Main(Pulkovo)Astronomical Observatory 196140 Saint PetersburgRussia saint Petersburg state University 198504 Saint PetersburgRussia

We investigate the global properties of X-ray emission from O stars, analyzing the X-ray spec- tra of 32 O stars from archival data of the XMM-Newton space observatory. We examine two hypotheses about of the origin of X-ray emission from O stars. The first is a paradigm proposed by Pollock, that was revealed from an analysis of the （ Ori X-ray observation. The second is the magnetically confined wind-shock （MCWs） model. For checking Pollock＇s hypothesis, we determine the distribution of the ratio of half width at half maximum （HWHM） to the wind terminal velocity for lines in spectra of all examined stars. In addition, we check three probable consequences from the MCWs model. We analyze if a correlation exists between the spectral hardness and such stellar parameters as the wind terminal velocity, stellar magnetic field and mass loss rate. The result showed that Pollock＇s hypothesis is not correct. We also established that not all consequences of the MCWs model considered by us are con- firmed. In addition, our spectral analysis method indicated that O stars probably have clumped stellar winds with spherical clumps.

关键词： stars early-type - stars spectra X-ray

Gold nanorods with a hematoporphyrin-loaded silica shell for dual-modality photodynamic and photothermal treatment of tumors in vivo

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纳米研究：英文版 2014年第3期7卷 325-337页

作者： Georgy Terentyuk elizaveta Panfilova Vitaly Khanadeev Daniil Chumakov Elina Genina Alexey Bashkatov Valery Tuchin Alia Bucharskaya Galina Maslyakova Nikolai Khlebtsov Boris Khlebtsov saratov state University 83 Astrakhanskaya Saratov 410012 Russia Institute of Biochemistry and Physiology of Plants and Microorganisms 13 pr. Entuziastov Saratov 410049 Russia Institute of Precise Mechanics and Control of RAs 24 Rabochaya Saratov 410028 Russia Ulyanovsk state University 42 Lev Tolstoy Ulyanovsk 432017 Russia Optoelectronics andMeasurement Techniques Laboratory UniversityofOulu P.O. Box4500 Oulu FIN-90014 Finland saratov state Medical University 112 Bolshaya Kazachia Saratov 410012 Russia

由一个金 nanorod 核心和与 hematoporphyrin (HP ) 做的 mesoporous 硅石壳组成的 Nanocomposites (NC ) 被制作了以便由在 vivo 联合 photothermal 和光力学的治疗(太平洋夏季时间 + PTT ) 改进癌症治疗的效率。除了 810830 nm 附近... 详细信息

由一个金 nanorod 核心和与 hematoporphyrin (HP ) 做的 mesoporous 硅石壳组成的 Nanocomposites (NC ) 被制作了以便由在 vivo 联合 photothermal 和光力学的治疗(太平洋夏季时间 + PTT ) 改进癌症治疗的效率。除了 810830 nm 附近的长波长的电浆子回声，制作 NC 展出了相应的一座 400-nm 吸收度山峰围住 HP，在 632.5-nm Q 乐队附近在 633-nm 刺激下面产生了汗衫氧，并且生产了在 808-nm 下面的热在红外线附近(NIR ) 激光照耀。这些形式被用于联合太平洋夏季时间 + PTT 治疗大(大约 3 cm3 ) 在有一只 xenorafted 肿瘤老鼠的 vivo 的稳固的肿瘤当模特儿。NC 直接被注入肿瘤并且与 633-nm 和 808-nm 激光同时照耀刺激联合光力学并且 NC 的 photothermal 活动。联合治疗的效率被光连贯断层摄影术评估，组织学的分析，并且由肿瘤体积生长的大小在一个 21 天的时期期间。调停 NC 的太平洋夏季时间在组织组织学并且到导致了弱变化一中等在肿瘤体积的 20% 减少。相反，联合太平洋夏季时间 + PTT 处理导致了大区域的肿瘤坏死并且在肿瘤体积导致了戏剧的减少。

关键词：癌症治疗纳米棒血卟啉肿瘤体内光热双模式外壳

Neo-Kantian Philosophy of Law of Novgorodtsev and Marxism

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Neo-Kantian Philosophy of Law of Novgorodtsev and Marxism

Optical magnetic field enhancement using ultrafast azimuthally polarized laser beams and tailored metallic nanoantennas

作者： elizaveta Frolova Faculty of Law Lomonosov Moscow state University

The article gives an assessment of Marxist ideology in the philosophy of law of the Russian representative of the Baden school of Novgorodtsev's neo-Kantianism. The evolution of classical Marxism at the turn of the 19 th and 20 th centuries in the interpretation of Novgorodtsev is shown. On the example of Novgorodtsev's concept and the political theory of Marxism, the ratio of the neo-Kantian philosophy of law in Russia at the end of the 19 th and beginning of the 20 th century and the sociology of law and the state are presented. The author draws a conclusion about the conceptual divergence of the neo-Kantian philosophy of law with Marxist ideology.

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Photonics Research 2024年第5期12卷 1078-1092页

作者： RODRIGO MARTIN-HERNANDEZ LORENZ GRUNEWALD LUIs sANCHEZ-TEJERINA LUIs PLAJA ENRIQUECONEJERO JARQUE CARLOs HERNANDEZ-GARCIA sEBAsTIAN MAI Grupo de Investigacion en Aplicaciones del Laser y Fotonica Departamento de Fisica AplicadaUniversidad de SalamancaE-37008 SalamancaSpain Unidad de Excelencia en Luz y Materia Estructuradas(LUMEs) Universidad de SalamancaE-37008 SalamancaSpain Institute of Theoretical Chemistry Faculty of ChemistryUniversity of Vienna1090 ViennaAustria Vienna Doctoral school in Chemistry(DosChem) Faculty of ChemistryUniversity of Vienna1090 ViennaAustria Departamento de Electricidad y Electrónica Universidad de Valladolid47011 ValladolidSpain

*** *** thank Valentina shumakova,elizaveta Gangrskaia,Alessandra Bellissimo,Audrius Pugzlys,and Andrius Baltu?ka for fruitful discussions and computational support by the Vienna scientific Cluster(VsC 4).The authors thankfully acknowledge the computer resources at MareNostrum and sCAYLE,and the technical support provided by Barcelona supercomputing Center(REs-FI-2022-3-0041).R.M.-H.,L.s.-T.,L.P.,E.C.J.,and C.H.-*** funding from the European Research Council(ERC)under the European Union’s Horizon 2020 research and innovation program(Grant Agreement No.851201)and support from Ministerio de Ciencia e Innovación(PID2022-142340NB-I00,PID2019-106910GB-I00).This research was funded in whole or in part by the Austrian science Fund(FWF)(10.55776/ZK91).For open access purposes,the author has applied a CC BY public copyright license to any author accepted manuscript version arising from this submission.

关键词： metallic polarized discussions

Biochemical mechanisms implemented by human acute myeloid leukemia cells to suppress host immune surveillance

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Cellular & Molecular Immunology 2018年第11期15卷 989-991页

作者： Inna M.Yasinska Isabel Gonçalves silva svetlana sakhnevych Bernhard F.Gibbs Ulrike Raap elizaveta Fasler-Kan Vadim V.sumbayev Medway school of Pharmacy Universities of Kent and GreenwichChatham MaritimeUK Department of Dermatology and Allergy University of OldenburgOldenburgGermany Department of Pediatric surgery and Department of Biomedical Research Children’s HospitalInselspitalUniversity of BernBernSwitzerland Department of Biomedicine University Hospital Basel and University of Basel BaselSwitzerland

Acute myeloid leukaemia(AML)is a blood/bone marrow cancer originating from myeloid cell precusors capable of *** cells implement biochemical mechanisms which allow them not only to survive,but also to successfully escape immune *** this work,we discuss crucial molecular mechanisms used by human AML cells in order to evade immune attack.

关键词： Acute myeloid leukaemia Immune surveillance Tim-3 galectin-9