Документы 61 - 70 из 138
61.
Автор:

Ответственность: Романова Оксана Дмитриевна

Количество страниц: 5 с.

Human resource outsourcing has become the first choice of many enterprises, and the overall outsourcing field has also been significantly expanded and extended. At the initial stage of human resource outsourcing, most of the outsourcing fields focused on manufacturing and traditional information industry, but in the new era of development, human resource outsourcing is developing faster and faster, covering a wider range. In the process of realizing modern operation, most enterprises improve their comprehensive competitive strength and promote the integrated utilization and allocation of high-quality human resources through human resource outsourcing. The management layer focuses on the core of the organization operationand human resource management, and gradually implements the enterprise technical resource management and personnel management through the enterprise human resource outsourcing, improves the overall operation quality, and reasonably controls the early operation cost.

Wang Senhao.
How to promote the outsourcing of human resources management in the public sector / Wang Senhao ; научный руководитель О. Д. Романова ; Северо-Восточный федеральный университет им. М. К. Аммосова, Финансово-экономический институт // Аргуновские чтения - 2023 : материалы IX Международной конференции (workshop), посвященной обсуждению "Основ государственной политики по сохранению и укреплению традиционных российских духовно-нравственных ценностей" (Указ Президента РФ от 9 ноября 2022 г.). - Якутск : НБ РС (Я), 2023. - (Культура Арктики ; вып. 14). - С. 645-649.

62.

Количество страниц: 8 с.

The group composition of asphaltene-resin-paraffin deposits (ARPD) in the Irelyakh field and their solubility in the composite solvents on the hexane base with the additives consisting of nonionic surface-active substances (NSAS) and concentrates of aromatic hydrocarbons is determined. The results of the investigations show that the additives Neonol AF-9-10 and liquid products of pyrolysis (LPP) are most efficient. The use of these additives allows to increase the efficiency of ARPD breaking and dissolving by 1,3 – 1,6 times as compared with a base solvent. It is shown that the increase in the concentration of individual additives from 0,5 to 3 % causes a decrease in the efficiency of detergent compounds.

Ivanova, I. K. Hydrocarbon solvents on the hexane base for oil organic deposits elimination of the irelyakh gas and oil field / Izabella K. Ivanova, Elena Yu. Shitz // Нефтегазовое дело. - 2008, N 1. - С. 9.

63.

Количество страниц: 13 с.

The preservation of endangered languages is a widely discussed issue nowadays. Languages represent essential cultural heritage and can provide valuable botanical, biological, and geographical information. Therefore, it is necessary to develop efficient measures to preserve and revitalize endangered languages. However, the languageshift process is complex and requires an interdisciplinary approach, including mathematical modeling techniques. This paper develops a new mathematical model that extends previous works on this topic. We introduce the factor of ethnic identity, which is a proxy for a more complex nexus of variables involved in an individual’sself-identity and/or a group’s identity. This proxy is socially constructed rather than solely inherited, shaped by community-determined factors, with language both indexing and creating the identity. In our model, we divide speakers into groups depending on with which language they identify themselves with. Moreover, every group includes monolinguals and bilinguals. The proposed model naturally allows us to consider cases of language coexistence and describe a broader class of linguistic situations. For example, the simulation results show that our model can result in cyclic language dynamics, drawing a parallel to cell population models. In this way, the proposed mathematical model can serve as a useful tool for developing efficient measures for language preservation and revitalization.
Сохранение исчезающих языков является широко обсуждаемой проблемой в настоящее время. Языки представляют собой важное культурное наследие и могут предоставить ценную ботаническую, биологическую и географическую информацию. Поэтому необходимо разработать эффективные меры по сохранению и возрождению исчезающих языков. Однако процесс смены языка сложен и требует междисциплинарного подхода, включая методы математического моделирования. В этой статье разрабатывается новая математическая модель, которая расширяет предыдущие работы по этой теме. Мы вводим фактор этнической идентичности, который является прокси для более сложной связи переменных, вовлеченных в самоидентификацию человека и/или идентичность группы. Этот прокси социально сконструирован, а не только унаследован, сформирован факторами, определяемыми сообществом, при этом язык как индексирует, так и создает идентичность. В нашей модели мы делим говорящих на группы в зависимости от того, с каким языком они себя идентифицируют. Более того, каждая группа включает монолингвов и билингвов. Предлагаемая модель естественным образом позволяет нам рассматривать случаи сосуществования языков и описывать более широкий класс языковых ситуаций. Например, результаты моделирования показывают, что наша модель может привести к циклической языковой динамике, проводя параллель с моделями клеточной популяции. Таким образом, предлагаемая математическая модель может служить полезным инструментом для разработки эффективных мер по сохранению и возрождению языка.

Ammosov, Dmitry А.
Identity-based language shift modeling / Dmitry A. Ammosov, Yalchin Efendiev, Lenore Grenoble ; Khalifa University of Science and Technology, Texas A&M University, University of Chicago // Арктика. XXI век. - 2025. - N 1 (39). - С. 6-18. - DOI: 10.25587/2310-5453-2025-39-1-6-18
DOI: 10.25587/2310-5453-2025-39-1-6-18

64.
Автор:

Ответственность: Михайлова Анна Викторовна (Научный руководитель)

Количество страниц: 8 с.

With the intensification of market competition, it further optimizes the internal management style of enterprises and provides a very important impetus for the development of enterprises. The establishment of a perfect incentive mechanism to protect human resources performance assessment, making a substantial increase in the level of business operations. To fully consider the impact of talent to improve the competitiveness of enterprises, improve and protect the enthusiasm of talent, promote the development of talent is conducive to stimulate the enthusiasm of employees to work, in-depth exploration of talent potential, and generate a higher sense of corporate identity and belonging. Therefore, enterprises should build an effective incentive mechanism in order to guarantee the efficiency of human resource management.

Xi Haoting.
Incentives in human resource management / Xi Haoting ; научный руководитель А. В. Михайлова ; Северо-Восточный федеральный университет им. М. К. Аммосова, Финансово-экономический институт // Аргуновские чтения - 2023 : материалы IX Международной конференции (workshop), посвященной обсуждению "Основ государственной политики по сохранению и укреплению традиционных российских духовно-нравственных ценностей" (Указ Президента РФ от 9 ноября 2022 г.). - Якутск : НБ РС (Я), 2023. - (Культура Арктики ; вып. 14). - С. 621-628.

65.

Количество страниц: 9 с.

Incidence of socially significant infectious diseases (HIV, TB and HIV/TB coinfection) in the Arctic regions of Russia) / Z. Zagdyn, Y. Zhao, V. Tsvetkov [and etc.] // International journal of circumpolar health. - 2021. - Т. 80, N 1. - С. 1-9. - DOI: 10.1080/22423982.2021.1966924
DOI: 10.1080/22423982.2021.1966924

66.

Количество страниц: 3 с.

The Jupiter is a powerful regular source of high-energy electrons (0,2-40 MeV). In this connection their density in the near-Earth space systematically increases with a period of 399 days, which is coincident with the synodic period of Jupiter. According to our estimations, their energy is sufficient to produce a significant local reduction of the magnetic field in the IMF sector connected with the Jupiter. In this paper the evidence is presented that the electron fluxes in the Jovian sector are controlled by the general magnetic field of the Sun. A treatment of 399-day intervals of the electron fluxes and IMF, obtained from spacecraft data for the period of 1963 to 2000 has been performed by superposed epoch technique taking into account the periodic change of the solar magnetic field polarity. Having adopted the Jupiter opposition day to be an epoch zero, the changes in particle intensity and IMF components under different signs of the general magnetic field of the Sun are found by using a large dataset (9925 days). The times of 399-day variation maxima in different periods of solar activity are compared and a character of their displacement relative to Jupiter opposition momentsis discussed.

Skryabin, N. G. Influence of a change in solar magnetic field polarity on the Jovian electron flux intensity / N. G. Skryabin, S. N. Samsonov, I. Ya. Plotnikov // Physics of auroral phenomena : proceedings of the 26th annual seminar, 25 - 28 February 2003. – 2003. – P. 159-161.

67.

Количество страниц: 4 с.

The spatial-temporal distribution of westward electrojets in the northern hemisphere has been investigated using geomagnetic ground observation data for November 9-10, 2004 geomagnetic storm. It is shown that the location of the maximum westward electrojet depends on the IMF orientation. It is in the evening or morning sector when Bγ0. With the increase of positive IMF Bγ, the region of intensity maximum shifts to morning hours. Thus, the azimuthal IMF component not only controls the pattern of magnetospheric convection, but also affects the longitudinal location of the westward electrojet pattern during the magnetic storm.

Influence of IMF by on the location of western electrojets during the magnetic storm on Nov. 9-10, 2004 / R. N. Boroev, A. Du, S. I. Solovyev, W.-Y. Xu, G.-X. Chen, V. A. Velichko // Physics of auroral phenomena : proceedings of the 29th annual seminar, Apatity, 27 February–3 March 2006. – 2007. – P. 21-24.

68.

Количество страниц: 4 с.

Galactic cosmic ray (GCR) diffusion in interplanetary space depends in a certain way on the degree of regularity of the interplanetary magnetic field (IMF). The sector IMF structure is manifested in inhomogeneous GCR distribution in the heliosphere. In parallel with the usual sectors associated with solar activity, one should take into account the sectors, which are caused by the Jupiter activity. It is known that the Jupiter is a powerful regular source of high-energy electrons (0.2-40 MeV), the density of which, on the average, is many times higher than that of solar cosmic rays. The high-energy electrons are systematically registed with the 399-day period in the near-Earth space. According to estimations of the particle energy density their flux is sufficient to decrease the magnetic field in the Jovian sector and can due to corresponding large-scale inhomogeneity in the GKL distribution. Hereby, we present the evidences that the GCR diffusion is noticeably stronger in the sector where there are Jovian electrons. By data on periodic passage of those sectors near the Earth, we have treated neutron monitor data using the superposed epoch technique. The day of the Earth and Jupiter opposition is taken as a zero epoch. At large statistical data (9925 days) it is found that the GCR intensity in that period increases with an amplitude near 1%. The groud effect is manifested with the period of 399 days and its maximum time is in a certain way shifted relative to the planet opposite moment.

Skryabin, N. G. Influence of Jupiter on cosmic ray intensity variations / N. G. Skryabin, S. N. Samsonov, I. Ya. Plotnikov // Physics of auroral phenomena : proceedings of the 25th annual seminar, Apatity, 26 February – 1 March 2002. – 2002. – P. 137-139.

69.

Количество страниц: 5 с.

Впервые произведено разложение наблюдаемой анизотропии космических лучей на зональные гармоники и компоненты векторной и тензорной анизотропии. Рассмотрены события форбуш-понижений космических лучей, произошедших в ноябре 2001 г и ноябре 2004 г. Показано, что в начале форбуш-понижения преобладает конвекционный ток космических лучей, направленный от Солнца, а в период восстановления интенсивности - диффузионный ток частиц вдоль межпланетного магнитного поля в сторону Солнца. На фазах спада интенсивности космических лучей наблюдается кратковременное уменьшение величины второй зональной гармоники, которое совпадает с резкими скачками напряженности межпланетного магнитного поля и скорости солнечного ветра. Во время прохождения крупномасштабных возмущений солнечного ветра тензорная анизотропия ведет себя сложным образом, для объяснения ее поведения требуется дальнейшее детальное исследование.
The observable anisotropy of cosmic rays has first been decomposed into zonal harmonics and components of vector and tensor anisotropy. We examine Forbush decreases in cosmic rays that occurred in November 2001 and November 2004. It is shown that at the beginning of a Forbush decrease an antisunward convective current of cosmic rays predominates; and during the recovery phase, a sunward diffusive current of particles along the interplanetary magnetic field dominates. During the phase of intensity drop, short-time decreases in the second zonal harmonic take place. These decreases occur with abrupt changes of the interplanetary magnetic field intensity and solar wind speed. During the passage of large-scale solar wind disturbances, the tensor anisotropy behaves in a complicated way. To explain its behavior, a further detailed investigation is required.

Investigating tensor anisotropy of cosmic rays during large-scale solar wind disturbances = Исследование тензорной анизотропии космических лучей во время крупномасштабных возмущений солнечного ветра / P. Yu. Gololobov, P. A. Krivoshapkin, G. F. Krymsky, V. G. Grigoryev, S. K. Gerasimova // Солнечно-земная физика = Solar-Terrestrial Physics. – 2017, т. 3, N 2 : 13-я российско-китайская конференция по космической погоде. – С. 22-26.
DOI: 10.12737/22604

70.

Издательство: [s. n.]

Год выпуска: 1988

Количество страниц: 14 с.

The influence of continious CO2-laser processing on structure, composition and microhadness of plasma sprayed Ni-Cr-Si-B, Fe-C-Cr-V, Ni-Al coatings was studied. The change of chemical and phase compositions of the coatings compared with the initial sprayed ones due to alloying with elements of substrate, depending on the processing operation (input power) was determined. Laser processing of plasma sprayed coatings allows to improve substantially their adhesion and in combination with high speed cooling, gives the possibility to regulate the processes of structure formation, dispersion, phase formation, and hence, the properties of forming coatings by means of processing operation.

Laser processing of plasma sprayed coatings / Dr. V. P. Larionov, Cand. N. P. Bolotina, Eng. T. V. Argunova, Cand. V. D. Tyunin, Eng. M. P. Lebedev. — [S. l. : s. n.], 1988. — 6 c.