Типологія внутрішньоорганізаційних процесів у закладах системи соціальної роботи

The starting point of the article is the understanding that one of the most important features of modern research finding is the emergence of interdisciplinary work. Prominent among the latter, in author’s opinion, take up works with the subject which is on the verge of sociology and philosophy of management, management of social work and quality. The relevance of the past defined the development of principles of service country in Ukraine, developing social services, the need to improve the performance of providers of the latter. The purpose of the publication is to analyze the types of organizational processes to ensure implementation of the mission socially work institution. It is emphasized that the product of socially work institution is service. Providing it is a consequence of the internal organizational processes. However, the author notes that this processes are complex associated and they make fuzzy line between formal and informal sectors routine workforce. However, this is the situation, in his opinion, regardless of the internal set of social norms and values can personalize responsibility and professional relationships without significantly reducing of the rationality goal. It is proved that in the daily life of the collective labor of any organization, including socially oriented people, we can distinguish two areas ­ formal and informal. Describing the first area author emphasizes that within it are staff units, divisions or departments whose activities are coordinated and deliberately created by direction towards a common goal of instrumentally rational. In this area implemented behaviors and relationships that provided early and for legal reasons. The main feature of the formal sector, as defined in the article, is the presence of a coherent and general procedures specified individual units of the organization. Based on this, the author concludes that in the labor group of social institution in his inner life, the dynamics defined processes are not always directly related to the final product. As stated in the article, as they occur in the formal and informal sectors institution correlated with standard management functions and structure of the latter, as well as ensuring its integrity and social self­sufficiency. However, the main focus of the publication focuses on the processes of communication, decision making, implementation of power and influence, conflict management. In everyday these processes are not rigidly delineated by typical feature and create diversity of combinatorial forms. Research of the relationship of instrumentally rational and attractive qualities in them will determine not only the nature of the subculture employees socially oriented institution, but may be a prerequisite for the theoretical reproduction of social image of their professional competence. Статья раскрывает проблему динамики повседневного функционирования учреждений сферы социальной работы. Определено, что продуктом учреждений указанного типа является социальная услуга, которая выступает квинтэссенцией внутриорганизационной жизнедеятельности. Установлено, что внутриорганизационные процессы обеспечивают предоставление социальной услуги. В соответствии со сферами организационной жизни заведения сферы социальной работы предложена их типология. Критериальной основой последней стали сущность, алгоритм, акторы процессов. Охарактеризованы, таким образом, коммуникативный процесс, а также принятие решений, управление конфликтом, реализации власти и влияния. Особое внимание уделено вопросу их социального наполнения. Процессы в коммуникативном пространстве учреждения сферы социальной  работы  охарактеризованы как ключевые для понимания сущности внутриорганизационной динамики. Подчеркнуто, что структура отношений в этой разновидности социального пространства может не совпадать с формальной иерархией системы управления организации. Процессы принятия решений, управление конфликтами, реализации власти и влияния, в этом русле, рассматриваются как отличные от макроорганизационной административной динамики. Характеристика их позволяет создать основу для анализа эффективности стиля управления социальноориентированной организацией. Стаття розкриває проблему динаміки повсякденного функціонування закладів сфери соціальної роботи. Визначено, що продуктом установ означеного типу є соціальна послуга, яка виступає квінтесенцією внутрішньоорганізаційного життя. Встановлено, що внутрішньоорганізаційні процеси забезпечують надання соціальної послуги. Відповідно до сфер організаційного життя закладу сфери соціальної роботи запропонована їх типологія. Критеріальною основою останньої стали сутність, алгоритм, актори процесів. Охарактеризовані, таким чином, комунікативний процес, а також прийняття рішень, управління конфліктом, реалізації влади та впливу. Особлива увага приділена питанню їх соціального наповнення. Процеси в комунікативному просторі закладу сфери соціальної роботи охарактеризовані як ключові для розуміння сутності внутрішньоорганізаційної динаміки. Підкреслено, що структура відносин у цьому різновиді соціального простору може незбігаються з формальною ієрархією системи управління організації. Процеси прийняття рішень, управління конфліктами, реалізації влади та впливу, в цьому руслі, розглядаються як відмінні від макроорганізаційної адміністративної динаміки. Характеристика їх дозволяє створити підґрунтя для аналізу ефективності стилю управління соціально орієнтованою організацією.

Use of finite difference method for numerical solution of three-dimensional heat transfer fractional differential equation

The paper proposes a numerical solution for the mixed problem concerning a three-dimensional heat transfer fractional differential equation, based on the finite difference method. To solve this problem, an explicit difference scheme described in the paper is used. The stability of a proposed difference scheme is proved. The case of homogeneous medium and a square grid is considere

Interaction of Nitrogen-Vacancy Centers in Diamond with a Dense Ensemble of Carbon-13

The nitrogen-vacancy center in diamond attracts a lot of attention in sensing applications, mainly for temperature, magnetic field, and rotation measurements. Nuclear spins of carbon-13 surrounding the nitrogen-vacancy center can be used as a memory or sensing element. In the current work, a diamond plate with a relatively large concentration of carbon-13 was synthesized and examined. The spectrum of optically detected magnetic resonance was recorded and analyzed in a magnetic field range of 5-200 G. A strain-independent measurement technique of carbon-13 isotope concentration based on the analysis of magnetic resonance spectra was developed. Additionally, narrow features in the spectrum were detected and understood

ТЕХНОЛОГИЯ ПРОИЗВОДСТВА ОБЕДЕННЫХ БЛЮД НА ОСНОВЕ ОВОЩЕЙ ДЛЯ СОЦИАЛЬНОГО ПИТАНИЯ

The seven-day recipe composition of lunch dishes for social nutrition of target groups of consumers was developed. The main components of this recipe are vegetables.Разработан семидневный рецептурный состав обеденных блюд для социального питания целевых групп потребителей, основным компонентом которого являются овощи

The Foundation Supernova Survey: Motivation, design, implementation, and first data release

© 2017 The Author(s). The Foundation Supernova Survey aims to provide a large, high-fidelity, homogeneous, and precisely calibrated low-redshift Type Ia supernova (SN Ia) sample for cosmology. The calibration of the current low-redshift SN sample is the largest component of systematic uncertainties for SN cosmology, and new data are necessary to make progress. We present the motivation, survey design, observation strategy, implementation, and first results for the Foundation Supernova Survey. We are using the Pan-STARRS telescope to obtain photometry for up to 800 SNe Ia at z>~0.1. This strategy has several unique advantages: (1) the Pan-STARRS system is a superbly calibrated telescopic system, (2) Pan-STARRS has observed 3/4 of the sky in grizyP1 making future template observations unnecessary, (3) we have a well-tested data-reduction pipeline, and (4) we have observed ~3000 high-redshift SNe Ia on this system. Here, we present our initial sample of 225 SN Ia grizP1light curves, of which 180 pass all criteria for inclusion in a cosmological sample. The Foundation Supernova Survey already contains more cosmologically useful SNe Ia than all other published low-redshift SN Ia samples combined. We expect that the systematic uncertainties for the Foundation Supernova Sample will be two to three times smaller than other low-redshift samples.We find that our cosmologically useful sample has an intrinsic scatter of 0.111 mag, smaller than other low-redshift samples. We perform detailed simulations showing that simply replacing the current low-redshift SN Ia sample with an equally sized Foundation sample will improve the precision on the dark energy equation-of-state parameter by 35 per cent, and the dark energy figure of merit by 72 per cent

Supplement: "Localization and broadband follow-up of the gravitational-wave transient GW150914" (2016, ApJL, 826, L13)

This Supplement provides supporting material for Abbott et al. (2016a). We briefly summarize past electromagnetic (EM) follow-up efforts as well as the organization and policy of the current EM follow-up program. We compare the four probability sky maps produced for the gravitational-wave transient GW150914, and provide additional details of the EM follow-up observations that were performed in the different bands

Localization and broadband follow-up of the gravitational-wave transient GW150914

A gravitational-wave (GW) transient was identified in data recorded by the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO) detectors on 2015 September 14. The event, initially designated G184098 and later given the name GW150914, is described in detail elsewhere. By prior arrangement, preliminary estimates of the time, significance, and sky location of the event were shared with 63 teams of observers covering radio, optical, near-infrared, X-ray, and gamma-ray wavelengths with ground- and space-based facilities. In this Letter we describe the low-latency analysis of the GW data and present the sky localization of the first observed compact binary merger. We summarize the follow-up observations reported by 25 teams via private Gamma-ray Coordinates Network circulars, giving an overview of the participating facilities, the GW sky localization coverage, the timeline, and depth of the observations. As this event turned out to be a binary black hole merger, there is little expectation of a detectable electromagnetic (EM) signature. Nevertheless, this first broadband campaign to search for a counterpart of an Advanced LIGO source represents a milestone and highlights the broad capabilities of the transient astronomy community and the observing strategies that have been developed to pursue neutron star binary merger events. Detailed investigations of the EM data and results of the EM follow-up campaign are being disseminated in papers by the individual teams

Localization and Broadband Follow-up of the Gravitational-wave Transient GW150914

A gravitational-wave (GW) transient was identified in data recorded by the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO) detectors on 2015 September 14. The event, initially designated G184098 and later given the name GW150914, is described in detail elsewhere. By prior arrangement, preliminary estimates of the time, significance, and sky location of the event were shared with 63 teams of observers covering radio, optical, near-infrared, X-ray, and gamma-ray wavelengths with ground- and space-based facilities. In this Letter we describe the low-latency analysis of the GW data and present the sky localization of the first observed compact binary merger. We summarize the follow-up observations reported by 25 teams via private Gamma-ray Coordinates Network circulars, giving an overview of the participating facilities, the GW sky localization coverage, the timeline, and depth of the observations. As this event turned out to be a binary black hole merger, there is little expectation of a detectable electromagnetic (EM) signature. Nevertheless, this first broadband campaign to search for a counterpart of an Advanced LIGO source represents a milestone and highlights the broad capabilities of the transient astronomy community and the observing strategies that have been developed to pursue neutron star binary merger events. Detailed investigations of the EM data and results of the EM follow-up campaign are being disseminated in papers by the individual teams. </p

Localization and broadband follow-up of the gravitational-wave transient GW150914

A gravitational-wave transient was identified in data recorded by the Advanced LIGO detectors on 2015 September 14. The event candidate, initially designated G184098 and later given the name GW150914, is described in detail elsewhere. By prior arrangement, preliminary estimates of the time, significance, and sky location of the event were shared with 63 teams of observers covering radio, optical, near-infrared, X-ray, and gamma-ray wavelengths with ground- and space-based facilities. In this Letter we describe the low-latency analysis of the gravitational wave data and present the sky localization of the first observed compact binary merger. We summarize the follow-up observations reported by 25 teams via private Gamma-ray Coordinates Network Circulars, giving an overview of the participating facilities, the gravitational wave sky localization coverage, the timeline and depth of the observations. As this event turned out to be a binary black hole merger, there is little expectation of a detectable electromagnetic signature. Nevertheless, this first broadband campaign to search for a counterpart of an Advanced LIGO source represents a milestone and highlights the broad capabilities of the transient astronomy community and the observing strategies that have been developed to pursue neutron star binary merger events. Detailed investigations of the electromagnetic data and results of the electromagnetic follow-up campaign will be disseminated in the papers of the individual teams