cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
КРЕДИТНАЯ ИСТОРИЯ ЗАЕМЩИКОВ В УСЛОВИЯХ ПАНДЕМИИ
Creators: name: КАРЛОВА Е.А.
name: ВОЛОДЧЕВА М.И.
name: БАЛАШЕВ Н.Б.
Publisher: name: Экономика и бизнес: теория и практика
Year: 2020
Subjects: КРЕДИТНЫЕ КАНИКУЛЫ
РЕСТРУКТУРИЗАЦИЯ КРЕДИТА
ПАНДЕМИЯ КОРОНАВИРУСА
CREDIT HOLIDAYS
LOAN RESTRUCTURING
CORONAVIRUS PANDEMIC

description: Пандемия коронавируса затронула абсолютно все сферы жизни общества, экономическая - не исключение. Цель данной статьи - проанализировать динамику обращений граждан в кредитные организации с требованием реструктуризации кредита или займа в период пандемии коронавируса. Исходя из приведенного анализа, меры, экстренно принятые Правительством РФ в период «первой волны» коронавируса, были своевременны, популярны и эффективны.
Tidally-induced migration of TESS gas giants orbiting M dwarfs
Creators: name: Alvarado-Montes, Jaime A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: According to core-accretion formation models, the conditions under which gas giants will form around M dwarfs are very restrictive. Also, the correlation of the occurrence of these planets with the metallicity of host stars is still unknown due to the intrinsic faintness of M dwarfs in the optical and some intricacies in their spectra. Interestingly, NASA's TESS mission has started to create a growing sample of these systems, with eleven observed planets located in close-in orbits: contrary to what is expected for low stellar masses. Tidal interactions with the host star will play a key role in determining the fate of these planets, so by using the measured physical and orbital characteristics of these M-dwarf systems we numerically analyse the exchange of rotational and orbital angular momentum, while constraining the energy dissipation in each system to calculate whether host stars are spun up or spun down, depending on the relationship between the gain and loss of angular momentum by the stellar rotation. We also study the coupled orbital and physical evolution of their gas giant companion and calculate orbital circularization time-scales, as well as the time needed to undergo orbital decay from their current orbital position to the Roche limit. The thorough study of tidal processes occurring over short and long time-scales in star-planet systems like those studied here, can help constrain tidal dissipation rates inside the star and planet, complement tidal theories, and improve estimations of unconstrained properties of exoplanetary systems.
description: Accepted for publication in MNRAS. 11 pages, 6 figures. V2: a newly discovered M-dwarf system was added
Sonnenfleckenzeichnung Nr. 5.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 13.01.1996, 11:00, erstellt von Sergio Cortesi
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Sonnenfleckenzeichnung Nr. 54.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 17.03.1996, 09:15, erstellt von Andrea Manna
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 4.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
СОЦИАЛЬНО-ЭКОНОМИЧЕСКОЕ РАЗВИТИЕ КРАСНОДАРСКОГО КРАЯ В УСЛОВИЯХ КРИЗИСА: ВОПРОСЫ ОБЕСПЕЧЕНИЯ УСТОЙЧИВОСТИ РАЗВИТИЯ
Creators: name: ПИВЕНЬ И.Г.
name: БЕБЯ Х.В.
Publisher: name: Экономика и бизнес: теория и практика
Year: 2020
Subjects: РЕГИОН
СОЦИАЛЬНО-ЭКОНОМИЧЕСКОЕ РАЗВИТИЕ
СТРАТЕГИЯ
УСТОЙЧИВОСТЬ
КОНКУРЕНТОСПОСОБНОСТЬ
REGION
SOCIO-ECONOMIC DEVELOPMENT
STRATEGY
SUSTAINABILITY
COMPETITIVENESS

description: В статье рассмотрены подходы к формированию стратегий социально-экономического развития регионов. Выделены направления, которые позволят обеспечить устойчивость регионального развития и конкурентоспособность. Определены регионы-лидеры в России. Выделен Краснодарский край среди таких регионов. Рассмотрены итоги реализации Стратегии социально-экономического развития края на период до 2020 г. Выделено главное направление Стратегии развития региона. Определены основные пути достижения высоких результатов его развития.
Comparing the Super-Eddington accretion of SMC X-3 and RX J0209.6-7427 with Swift J0243.6+6124
Creators: name: Liu, Jiren
name: Vasilopoulos, Georgios
name: Ge, MingYu
name: Ji, Long
name: Weng, Shan-Shan
name: Zhang, Shuang-Nan
name: Hou, Xian
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We study the giant outbursts of SMC X-3 and RX J0209.6-7427 to compare their super-Eddington accretion regime with that of Swift J0243.6+6124. The high double-peak profile of SMC X-3 is found to be 0.25 phase offset from that below $2.3\times10^{38}$erg\,s$^{-1}$, which is similar to Swift J0243 (happened around $0.9\times10^{38}$erg\,s$^{-1}$). The profile of RX J0209 shows a similar 0.25 phase offset between high double-peak and low double-peak around $1.25\times10^{38}$erg\,s$^{-1}$. The 0.25 phase offset corresponds to a 90 degree angle change of the emission beam and strongly supports for a transition from a fan beam to a pencil beam. Their critical luminosities imply a surface magnetic field $\sim4\times10^{13}$ G and $2\times10^{13}$ G for SMC X-3 and RX J0209, respectively, based on the recently measured cyclotron line of Swift J0243. The spin-up rate and luminosity of SMC X-3 follows a relation of $\dotν\propto L^{0.94\pm0.03}$, while that of RX J0209 follows $\dotν\propto L^{1.00\pm0.03}$, which are similar to Swift J0243 and consistent with the prediction of a radiation-pressure-dominated (RPD) disk. These results indicate that accretion columns are indeed formed above Eddington luminosity, and the population of ULXPs likely corresponds to X-ray pulsars of highest magnetic field.
description: 9 pages, 5 figs, to appear on MNRAS
D4.4 Final version of ENVISION platform
Creators: name: Tekes, Stavros
Publisher: name: Zenodo
Year: 2023

description: Deliverable "D4.4 Final version of ENVISION platform" is the 4th deliverable of the WP4 and its main objective is to showcase how the services provided through the ENVISION project, may cover the needs of its business customers. In more detail, this deliverable aims to demonstrate the features of ENVISION platform and ENVISION mobile application, that are able to cover the specific needs of the users of each business case, as they identified in WP2 Commercial Service Requirements.
Overview of CNM LGAD results: Boron Si-on-Si and epitaxial wafers
Creators: name: Grieco, Chiara
name: García, Lucía Castillo
name: Moreno, Albert Doblas
name: Gkougkousis, Evangelos Leonidas
name: Grinstein, Sebastian
name: Hidalgo, Salvador
name: Moffat, Neil
name: Pellegrini, Giulio
name: Dominguez, Jairo Villegas
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Low Gain Avalanche Detectors (LGADs) are n-on-p silicon sensors with an extra p-layer below the collection electrode which provides signal amplification. When the primary electrons reach the amplification region new electron-hole pairs are created that enhance the generated signal. The moderate gain of these sensors, together with the relatively thin active region, provide precise time information for minimum ionizing particles. To mitigate the effect of pile-up at the HL-LHC the ATLAS and CMS experiments have chosen the LGAD technology for the High Granularity Timing Detector (HGTD) and for the End-Cap Timing Layer (ETL), respectively. A full characterization of recent productions of LGAD sensors fabricated at CNM has been carried out before and after neutron irradiation up to 2.5 $\times$ 10$^{15}$ n$_{eq}$/cm$^{2}$ . Boron-doped sensors produced in epitaxial and Si-on-Si wafers have been studied. The results include their electrically characterization (IV and bias voltage stability) and performance studies (charge and time resolution) for single pad devices with a Sr-90 radioactive source set-up. The behaviour of the Inter-Pad region for irradiated 2 $\times$ 2 LGAD arrays, using the Transient Current Technique (TCT), is shown. The results indicate that the Si-on-Si devices with higher resistivity perform better than the epitaxial ones.
Phase diagrams of binary ionic mixtures and white dwarf cooling
Creators: name: Baiko, D. A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: Phase diagrams of fully ionized binary ionic mixtures are considered within the framework of the linear mixing formalism taking into account recent advances in understanding quantum one-component plasma thermodynamics. We have followed a transformation of azeotropic phase diagrams into peritectic and eutectic types with increase of the charge ratio. For solid $^{12}$C/$^{16}$O and $^{16}$O/$^{20}$Ne mixtures, we have found extensive miscibility gaps. Their appearance seems to be a robust feature of the theory. The gaps evolve naturally into two-solid regions of eutectic phase diagrams at higher $Z_2/Z_1$. They do not depend on thermodynamic fit extensions beyond their applicability limits. The gaps are sensitive to binary mixture composition and physics, being strongly different for C/O and O/Ne mixtures and for the three variants of corrections to linear-mixing solid-state energies available in the literature. When matter cools to its miscibility gap temperature, the exsolution process takes place. It results in a separation of heavier and lighter solid solutions. This may represent a significant reservoir of gravitational energy and should be included in future white dwarf (WD) cooling simulations. Ion quantum effects mostly resulted in moderate modifications, however, for certain $Z_2/Z_1$, these effects can produce qualitative restructuring of the phase diagram. This may be important for the model with $^{22}$Ne distillation in cooling C/O/Ne WD proposed as a solution for the ultramassive WD cooling anomaly.
description: 13 pages, 8 figures, accepted in MNRAS
Distinguishing black holes and wormholes with orbiting hot spots
Creators: name: Li, Zilong
name: Bambi, Cosimo
Publisher: name: arXiv
Year: 2014
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The supermassive black hole candidates at the center of every normal galaxy might be wormholes created in the early Universe and connecting either two different regions of our Universe or two different universes in a Multiverse model. Indeed, the origin of these supermassive objects is not well understood, topological non-trivial structures like wormholes are allowed both in general relativity and in alternative theories of gravity, and current observations cannot rule out such a possibility. In a few years, the VLTI instrument GRAVITY will have the capability to image blobs of plasma orbiting near the innermost stable circular orbit of SgrA$^*$, the supermassive black hole candidate in the Milky Way. The secondary image of a hot spot orbiting around a wormhole is substantially different from that of a hot spot around a black hole, because the photon capture sphere of the wormhole is much smaller. The radius of the photon capture sphere is independent of the hot spot model, and therefore its possible detection, which is observationally challenging but not out of reach, can unambiguously test if the center of our Galaxy harbors a wormhole rather than a black hole.
description: 11 pages, 4 figures. v2: refereed version
Sonnenfleckenzeichnung Nr. 170.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 25.07.1996, 11:30, erstellt von Michele Bianda
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Transition from multipolar to dipolar dynamos in stratified systems
Creators: name: Zaire, B.
name: Jouve, L.
name: Gastine, T.
name: Donati, J-F.
name: Morin, J.
name: Landin, N.
name: Folsom, C. P.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Observations of surface magnetic fields of cool stars reveal a large diversity of configurations. Although there is now a consensus that these fields are generated through dynamo processes occurring within the convective zone, the physical mechanism driving such a variety of field topologies is still debated. This paper discusses the possible origins of dipole and multipole-dominated morphologies using three-dimensional numerical simulations of stratified systems where the magnetic feedback on the fluid motion is significant. Our main result is that dipolar solutions are found at Rossby numbers up to 0.4 in strongly stratified simulations, where previous works suggested that only multipolar fields should exist. We argue that these simulations are reminiscent of the outlier stars observed at Rossby numbers larger than 0.1, whose large-scale magnetic field is dominated by their axisymmetric poloidal component. As suggested in previous Boussinesq calculations, the relative importance of inertial over Lorentz forces is again controlling the dipolar to multipolar transition. Alternatively, we find that the ratio of kinetic to magnetic energies can equally well capture the transition in the field morphology. We test the ability of this new proxy to predict the magnetic morphology of a few M-dwarf stars whose internal structure matches that of our simulations and for which homogeneous magnetic field characterization is available. Finally, the magnitude of the differential rotation obtained in our simulations is compared to actual measurements reported in the literature for M-dwarfs. In our simulations, we find a clear relationship between anti-solar differential rotation and the emergence of dipolar fields.
description: 15 pages, 15 figures, accepted for publication in MNRAS
Sonnenfleckenzeichnung Nr. 212.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 07.09.1996, 07:30, erstellt von Sergio Cortesi
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
АНАЛИТИЧЕСКИЕ ПРОЦЕДУРЫ И ПОДХОДЫ К ОЦЕНКЕ НЕПРЕРЫВНОСТИ ДЕЯТЕЛЬНОСТИ ОРГАНИЗАЦИИ
Creators: name: ГАЛИЦКАЯ Ю.Н.
name: БЛЕЙ Е.И.
Publisher: name: Экономика и бизнес: теория и практика
Year: 2020
Subjects: НЕПРЕРЫВНОСТЬ ДЕЯТЕЛЬНОСТИ
БИЗНЕС
СИСТЕМА
ФИНАНСОВАЯ ОТЧЕТНОСТЬ
АУДИТ
ИНФОРМАЦИЯ
РИСК-ОРИЕНТИРОВАННЫЙ ПОДХОД
ФАКТОРЫ
ФИНАНСОВОЕ СОСТОЯНИЕ
БАНКРОТСТВО
GOING CONCERN
BUSINESS
SYSTEM
FINANCIAL REPORTING
AUDIT
INFORMATION
RISK-BASED APPROACH
FACTORS
FINANCIAL CONDITION
BANKRUPTCY

description: В данной статье охарактеризованы основные подходы к анализу и оценке непрерывности деятельности хозяйствующих субъектов, проводимые на базе финансовой отчетности. Принцип непрерывности деятельности - основа формирования финансовой отчетности и восприятие определения идеи деятельности компании в современной экономике, направленное на продолжение и развитие, ограниченное определенным промежутком времени или целевыми установками. Аналитические процедуры позволяют оценить и выявить существующие риски, создавать или корректировать управленческие решения относительно деятельности компании. Описаны составляющие риск-ориентированного подхода, позволяющие получить соответствующие и достаточные доказательства для выражения мнения и подготовки аудиторского отчета.
Sonnenfleckenzeichnung Nr. 227.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 25.09.1996, 07:15, erstellt von Sergio Cortesi
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Comments on N=(2,2) Supersymmetry on Two-Manifolds
Creators: name: Closset, Cyril
name: Cremonesi, Stefano
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study curved-space rigid supersymmetry for two-dimensional $\mathcal{N}=(2,2)$ supersymmetric fields theories with a vector-like $R$-symmetry by coupling such theories to background supergravity. The associated Killing spinors can be viewed as holomorphic sections of particular complex line bundles over Euclidean space-time, which severely restrict the allowed supersymmetric couplings on compact orientable Riemann surfaces without boundaries. For genus $g>1$, the only consistent non-singular couplings are the ones dictated by the topological $A$-twist. On spaces with $S^2$ topology, there exist additional supersymmetric backgrounds with $m=0$ or $\pm 1$ unit of flux for the $R$-symmetry gauge field. The $m=-1$ case includes the $Ω$-background on the sphere. We also systematically work out the curved-space supersymmetry multiplets and supersymmetric Lagrangians.
description: 38 pages+appendix; v2: new section 6.10 on NLSM Lagrangians; v3: corrected typos and added references
title: Polyphosphoramides as Highly Effective Fire Retardants for Polylactide: Green Syntheses, Properties and Mechanisms
Creators: name: Feng, Jiabing
Publisher: name: University of Southern Queensland
Year: 2022
Subjects: classificationCode: 401609
subject: Polymers and plastics
valueUri: https://www.abs.gov.au/statistics/classifications/australian-and-new-zealand-standard-research-classification-anzsrc/latest-release
classificationCode: 401602
subject: Composite and hybrid materials
valueUri: https://www.abs.gov.au/statistics/classifications/australian-and-new-zealand-standard-research-classification-anzsrc/latest-release

description: Renewable Polylactide (PLA) suffers from a high flammability that limits in its practical applications in many industrial settings. Therefore, it is imperative to develop flame-retarding PLA. Polyphosphoramides have shown a high fire-resistant efficiency in PLA, but nearly all of their existing synthesis methods involve a large volume of toxic solvents. Meanwhile, there has been a lack of in-depth understanding of their modes of actions and how they affect comprehensive properties of PLA. For these reasons, this thesis focuses on developing solvent/catalyst-free synthesis approaches for polyphosphoramides, then unveiling their modes of actions, and then investigating how the physical properties of PLA are impacted by polyphosphoramides. We pioneered developed a green strategy to synthesize three types of polyphosphoramides fire retardants (DM-H, DM-Si and DM-OHn) without use of any solvents and catalysts. DM-H and DM-Si show very high fire-retardant efficiency in PLA, only 2 and 3 wt%, respectively, enable PLA to achieve a desired UL-94 V-0 rating and a high LOI, but reduce its thermal stability. In comparison, DM-OHn makes PLA show both desired flame retardancy and enhanced thermal stability. The polyphosphoramides fire retardants mainly function in the gas phase. Moreover, they have limited impact on the mechanical strength of PLA. This work provides one new eco-benign strategy for synthesizing polyphosphoramides fire retardants and the results and findings of this work will significantly promote the green development of next-generation eco-friendly effective fire retardants and fire-retardant PLA bioplastics, thus enabling PLA to find more applications in industries.
Análise de processos jurídicos: Caso 16 - Ação Trabalhista - Rito Ordinário 0000586-85.2016.5.06.0001; Processo 820614-79.2019.4.05.8300: Inquérito Policial (JF/PE-0820614-79.2019.4.05.8300-INQ).
Creators: name: BRASIL. Ministério Da Justiça
Publisher: name: Zenodo
Year: 2023

description: Análise de processos jurídicos: Caso 16 - Ação Trabalhista - Rito Ordinário 0000586-85.2016.5.06.0001; Processo 820614-79.2019.4.05.8300: Inquérito Policial (JF/PE-0820614-79.2019.4.05.8300-INQ).
ОСНОВНЫЕ ФАКТЫ И СТАТИСТИКА РЕВОЛЮЦИИ В РОЗНИЧНОЙ ПРОДУКТОВОЙ ИНДУСТРИИ
Creators: name: ЯНОВА Е.А.
name: БОЙЦОВА Ю.С.
Publisher: name: Экономика и бизнес: теория и практика
Year: 2020
Subjects: ОТРАСЛЬ ПРОДУКТОВ ПИТАНИЯ
ТЕНДЕНЦИИ В ОБЛАСТИ ПИТАНИЯ
ПРОДУКТОВАЯ ИНДУСТРИЯ
РОЗНИЧНАЯ ТОРГОВЛЯ
ОБЪЕМ ПРОДАЖ ПРОДУКТОВ ПИТАНИЯ
FOOD INDUSTRY
FOOD TRENDS
RETAIL
FOOD SALES

description: Целью настоящей работы является оценка ключевых фактов и статистики, которые демонстрируют, как розничные продуктовые магазины работают и развиваются в нашем постоянно меняющемся мире. Торговля является ведущим рынком в наше времяи оценивался в 11,7 триллиона долларов, также по данным прогноза считается, что она будет развиваться со среднегодовым темпом роста 5,0% с 2020 по 2027 год. Что касается тенденций на сегодняшний день в продажном секторе, они затрагивают как цифровизацию, так и привлечение интереса на рынок посредством внимательности и личностной актуализации на персональный рынок потребителей. Сложившаяся ситуация 2020 года внесла значительный вклад в этот сектор, основными моментами является активная гибкость к сложившимся условиям, т.е. возможность переориентирования магазинов на новый формат. Таким образом, в данной статье были рассмотрены: статистика и факты розничной торговли продуктами питания; тенденции в розничной торговле продуктами питания; анализ розничной торговли продуктами питания в США и во всем мире; степень влияния Covid-19 на рынок.
title: A work-based study of leg strength and agility performance in adolescent female athletes participating in competitive Queensland AFLW: Implications for future practice
Creators: name: Stubbs, Jim
Publisher: name: University of Southern Queensland
Year: 2022
Subjects: classificationCode: 420702
subject: Exercise physiology
valueUri: https://www.abs.gov.au/statistics/classifications/australian-and-new-zealand-standard-research-classification-anzsrc/latest-release
classificationCode: 420799
subject: Sports science and exercise not elsewhere classified
valueUri: https://www.abs.gov.au/statistics/classifications/australian-and-new-zealand-standard-research-classification-anzsrc/latest-release
classificationCode: 390305
subject: Professional education and training
valueUri: https://www.abs.gov.au/statistics/classifications/australian-and-new-zealand-standard-research-classification-anzsrc/latest-release

description: This work-based project investigated the relationship between leg strength—bodyweight ratio and agility performance in adolescent females participating in competitive Australian Football League Women’s in Queensland. This demographic has been shown to have a higher risk of Anterior Cruciate Ligament injuries as compared to their male counterparts and some research suggests improved agility may contribute to mitigation of this risk. The project investigated these relationships in-the-field to address some of the barriers reported by adolescent females to regular participation in strength and conditioning programs which may be beneficial to them. 23 volunteer adolescent females were separated into two groups. All participants were tested for anthropometric, unilateral leg strength measures and agility before Group 1 (n=11), undertook a six-week, leg strength intervention program while Group 2 (n=12) continued a normal training protocol. The intervention took place three times per week and was conducted at the training ground. Both groups then participated in the same post-intervention testing battery. Results indicate both Group 1 (t = 2.14, p = 0.06) and Group 2 (t = 2.35, p < 0.05), improved left leg strength and Group 2 improved aggregate leg strength (t = 2.20, p = 0.05). Improvement in agility for Group 1 was statistically significant (t = −4.84, p < 0.001). Significant negative correlations between bodyweight and leg strength for all participants were observed (r = −0.44, p < 0.05) and leg strength and leg strength-bodyweight ratio were correlated with agility performance (r = −0.47, p < 0.05). Implications for future workbased practise suggest a group-led, field-based strength program may benefit adolescent female agility and, by extension, injury risk.
Sonnenfleckenzeichnung Nr. 33.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 21.02.1996, 09:00, erstellt von Sergio Cortesi
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Sonnenfleckenzeichnung Nr. 277.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 01.12.1996, 09:45, erstellt von Andrea Manna
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 2.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Análise de processos jurídicos: Caso 17 - Processo no 0503740-07.2018.4.02.5101 (2018.51.01.503740-1); JF-RJ-0503740-07.2018.4.02.5101-INQ.
Creators: name: BRASIL. Ministério Da Justiça
Publisher: name: Zenodo
Year: 2023

description: Análise de processos jurídicos: Caso 17 - Processo no 0503740-07.2018.4.02.5101 (2018.51.01.503740-1); JF-RJ-0503740-07.2018.4.02.5101-INQ.
The Impact of Phase Equilibrium Cloud Models on GCM Simulations of GJ~1214b
Creators: name: Christie, D. A.
name: Mayne, N. J.
name: Gillard, R. M.
name: Manners, J.
name: Hébrard, E.
name: Lines, S.
name: Kohary, K.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We investigate the impact of clouds on the atmosphere of GJ~1214b using the radiatively-coupled, phase-equilibrium cloud model {\sc EddySed} coupled to the {\sc Unified Model} general circulation model. We find that, consistent with previous investigations, high metallicity ($100\times$ solar) and clouds with large vertical extents (a sedimentation factor of $f_\mathrm{sed} = 0.1$) are required to best match the observations, although metallicities even higher than those investigated here may be required to improve agreement further. We additionally find that in our case which best matches the observations ($f_\mathrm{sed}=0.1$), the velocity structures change relative to the clear sky case with the formation of a superrotating jet being suppressed, although further investigation is required to understand the cause of the suppression. The increase in cloud extent with $f_\mathrm{sed}$ results in a cooler planet due to a higher albedo, causing the atmosphere to contract. This also results in a reduced day-night contrast seen in the phase curves, although the introduction of cloud still results in a reduction of the phase offset. We additionally investigate the impact the the {\sc Unified Model}'s pseudo-spherical irradiation scheme on the calculation of heating rates, finding that the introduction of nightside shortwave heating results in slower mid-latitude jets compared to the plane parallel irradiation scheme used in previous works. We also consider the impact of a gamma distribution, as opposed to a log-normal distribution, for the distribution of cloud particle radii and find the impact to be relatively minor.
description: Accepted to MNRAS
Systematic study of proton radioactivity half-lives based on the relationship between the Skyrme-Hartree-Fock and the macroscopic quantities of nuclear matter
Creators: name: Cheng, Jun-Hao
name: Zhang, Zhen
name: Wu, Xi-Jun
name: Chu, Peng-Cheng
name: Li, Xiao-Hua
Publisher: name: arXiv
Year: 2022
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: In the present work, we systematically study the proton radioactivity half-lives of 33 spherical nuclei based on the relationship between the Skyrme parameters and the macroscopic quantities of nuclear matter. Using the two-potential approach with the spherical Skyrme-Hartree-Fock model, the correlation between proton radioactivity half-life and macroscopic quantities was analyzed. Moreover, we obtained a new Skyrme parameter set by fitting the two most weighted macroscopic quantities. Compared with Skyrme parameters MSL0 and the theoretical model of proton radioactivity UDLP, the theoretical proton radioactivity half-life calculated by the new Skyrme parameter set can better reproduce the experimental data.
description: 8 pages, 3 figures
Multi-matrix models and Noncommutative Frobenius algebras obtained from symmetric groups and Brauer algebras
Creators: name: Kimura, Yusuke
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: It has been understood that correlation functions of multi-trace operators in ${\cal N}=4$ SYM can be neatly computed using the group algebra of symmetric groups or walled Brauer algebras. On the other hand such algebras have been known to construct 2D topological field theories (TFTs). After reviewing the construction of 2D TFTs based on symmetric groups, we construct 2D TFTs based on walled Brauer algebras. In the construction, the introduction of a dual basis manifests a similarity between the two theories. We next construct a class of 2D field theories whose physical operators have the same symmetry as multi-trace operators constructed from some matrices. Such field theories correspond to non-commutative Frobenius algebras. A matrix structure arises as a consequence of the noncommutativity. Correlation functions of the Gaussian complex multi-matrix models can be translated into correlation functions of the two-dimensional field theories.
description: 40 pages, 7 figures
ОПЫТ И ПЕРСПЕКТИВЫ РЕАЛИЗАЦИИ ГОСУДАРСТВЕННОЙ ПОЛИТИКИ В ОТНОШЕНИИ ДЕТЕЙ-ИНВАЛИДОВ В ХАНТЫ-МАНСИЙСКОМ АВТОНОМНОЙ ОКРУГЕ - ЮГРЕ
Creators: name: БРАГИНА Е.М.
Publisher: name: Экономика и бизнес: теория и практика
Year: 2020
Subjects: ГОСУДАРСТВЕННОЕ УПРАВЛЕНИЕ
ГОСУДАРСТВЕННАЯ ПОЛИТИКА В ОТНОШЕНИИ ИНВАЛИДОВ
ДОСТУПНАЯ СРЕДА
ИНКЛЮЗИВНОЕ ОБРАЗОВАНИЕ
ХАНТЫ-МАНСИЙСКИЙ АВТОНОМНЫЙ ОКРУГ - ЮГРА
PUBLIC ADMINISTRATION
STATE POLICY ON THE DISABLED
ACCESSIBLE ENVIRONMENT
INCLUSIVE EDUCATION
KHANTY-MANSIYSK AUTONOMOUS OKRUG - YUGRA

description: В статье рассмотрен опыт организации государственной системы социальной реабилитации детей-инвалидов в Ханты-Мансийском автономном округе - Югре. На основе статистических данных проанализировано современное состояние, выявлены проблемные вопросы, сформулированы предложения по совершенствованию государственного управления в данной сфере, направленные на увеличение финансовой, организационной помощи семьям с детьми - инвалидами, развитием доступной среды, инклюзивного образования, активизацией взаимодействия с общественными организациями.
СОВРЕМЕННОЕ СОСТОЯНИЕ И НАПРАВЛЕНИЯ СОВЕРШЕНСТОВАНИЯ ГОСУДАРСТВЕННОГО УПРАВЛЕНИЯ МУЗЕЙНЫМ ДЕЛОМ В ХАНТЫ-МАНСИЙСКОМ АВТОНОМНОМ ОКРУГЕ - ЮГРЕ
Creators: name: БУБЕНОВА Е.Л.
name: БРАГИНА Е.М.
Publisher: name: Экономика и бизнес: теория и практика
Year: 2020
Subjects: ГОСУДАРСТВЕННОЕ УПРАВЛЕНИЕ
КУЛЬТУРА
МУЗЕЙНОЕ ДЕЛО
РЕГИОНАЛЬНАЯ КУЛЬТУРНАЯ ПОЛИТИКА
ХАНТЫ-МАНСИЙСКИЙ АВТОНОМНЫЙ ОКРУГ - ЮГРА
PUBLIC ADMINISTRATION
CULTURE
MUSEUM BUSINESS
REGIONAL CULTURAL POLICY
KHANTY-MANSIYSK AUTONOMOUS OKRUG - YUGRA

description: В статье рассмотрен опыт организации государственного управления в сфере музейного дела в Ханты-Мансийском автономном округе - Югре. На основе статистических данных проанализировано современное состояние, выявлены проблемные вопросы, сформулированы предложения по совершенствованию государственного управления в данной сфере, направленные на увеличение финансирования, в том числе за счет государственно - частного партнерства, спонсорства, на совершенствование развития кадрового состава, активизацию внедрения информационно-коммуникационных технологий.
Rise and fall of silicate dust in RS Ophiuchi following the 2006 eruption
Creators: name: Rushton, M. T.
name: Woodward, C. E.
name: Gehrz, R. D.
name: Evans, A.
name: Kaminsky, B.
name: Pavlenko, Ya. V.
name: Eyres, S. P. S.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present an analysis of archival Spitzer InfraRed Spectrograph (IRS) observations of the recurrent nova RS Ophiuchi obtained on several occasions, beginning about 7 months after the outburst in 2006. These data show atomic emission lines, absorption bands due to photospheric SiO, and the well known silicate dust features at $9.7\,μ$m and $18\,μ$m. The dust emission, arising in the wind of the secondary star, is fitted by Dusty models for mass-loss rates in the range $1.0-1.7\times10^{-7}$M$_{\odot}$yr$^{-1}$. The silicate features are similar in profile to those seen in circumstellar environments of isolated late-type stars and some dusty symbiotic binaries, although the longer wavelength feature peaks at $17\,μ$m,, instead of the usual $18\,μ$m, indicating peculiar grain properties. The dust features are variable, appearing stronger in 2006-2007 during outburst than in 2008-2009 when the system was in the quiescent state. This variability is attributed to changes in the ultraviolet output and the reformation of the accretion disk, although a decline in the mass-loss rate of the red giant secondary star could also play a role. Further observations, in the aftermath of the 2021 eruption, could provide a definitive conclusion.
description: 10 pages, 8 figures. Accepted for publication in MNRAS
Sonnenfleckenzeichnung Nr. 105.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 15.05.1996, 12:30, erstellt von Sergio Cortesi
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
РЫНОК МЕЖДУНАРОДНЫХ ГРУЗОПЕРЕВОЗОК: ОЦЕНКА ВЛИЯНИЯ ПАНДЕМИИ
Creators: name: СУВОРОВА С.Д.
name: ВОРОБЬЕВА О.Т.
Publisher: name: Экономика и бизнес: теория и практика
Year: 2020
Subjects: COVID-19
ГРУЗОПЕРЕВОЗЧИКИ
ГРУЗОПОТОК
МЕЖДУНАРОДНОЕ ТОВАРОДВИЖЕНИЕ
ДЕФИЦИТ ЛОГИСТИЧЕСКИХ УСЛУГ
CARGO CARRIERS
CARGO FLOW
INTERNATIONAL COMMODITY MOVEMENT
SHORTAGE OF LOGISTICS SERVICES

description: Пандемия COVID-19 стала причиной кризиса международного масштаба, затронувшего все континенты. Меры, по пресечению распространения инфекции спровоцировали закрытие границ и введение ограничений, которые привели к снижению грузопотока и к отказу от привычных маршрутов товародвижения в глобальных масштабах, что вынудило малых и часть средних предприятий покинуть рынок. Авторы полагают, что опыт 2020 г. вынуждает руководителей хозяйствующих субъектов направить основные усилия на генерацию различных управленческих решений, помогающих преодолеть возникновение подобных ситуаций и сформировать гибкую стратегию международного товародвижения, направленную на адаптацию грузоперевозчиков и интеграцию логистических предприятий на разных уровнях, предоставляющих инновационные услуги, что, в сою очередь, поможет логистическим компаниям удержаться на рынке.
Radio interferometric imaging of RS Oph bipolar ejecta for the 2021 nova outburst
Creators: name: Munari, U.
name: Giroletti, M.
name: Marcote, B.
name: O'Brien, T. J.
name: Veres, P.
name: Yang, J.
name: Williams, D. R. A.
name: Woudt, P.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The recurrent nova and symbiotic binary RS Oph erupted again in August 2021 for its eighth known outburst. As part of a multi-epoch and frequency campaign, we observed RS Oph 34 days after the outburst at 5 GHz with the European VLBI Network (EVN). The radio image is elongated over the east-west direction for a total extension of about 90 mas (or about 240 AU at the Gaia DR3 distance d=2.68 [-0.15/+0.17] kpc), and shows a bright and compact central component coincident with the Gaia astrometric position, and two lobes east and west of it, expanding perpendicular to the orbital plane. By comparing with the evolution of emission-line profiles on optical spectra, we found the leading edge of the lobes to be expanding at 7550 km/s, and i=54 deg as the orbital inclination of the binary. The 2021 radio structure is remarkably similar to that observed following the 2006 eruption. The obscuring role of the density enhancement on the orbital plane (DEOP) is discussed in connection to the time-dependent visibility of the receding lobe in the background to the DEOP, and the origin of the triple-peaked profiles is traced to the ring structure formed by the nova ejecta impacting the DEOP.
description: A&A Letter to the Editor, in press
High resolution ALMA and HST imaging of $κ$CrB: a broad debris disc around a post-main sequence star with low-mass companions
Creators: name: Lovell, J. B.
name: Wyatt, M. C.
name: Kalas, P.
name: Kennedy, G. M.
name: Marino, S.
name: Bonsor, A.
name: Penoyre, Z.
name: Fulton, B. J.
name: Pawellek, N.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: $κ$CrB is a ${\sim}2.5\,$Gyr old K1 sub-giant star, with an eccentric exo-Jupiter at ${\sim}2.8\,$au and a debris disc at tens of au. We present ALMA Band 6 ($1.3\,$mm) and HST scattered light ($0.6\,μ$m) images, demonstrating $κ$CrB's broad debris disc, covering an extent $50{-}180\,$au in the millimetre (peaking at $110\,$au), and $51{-}280\,$au in scattered light (peaking at $73\,$au). By modelling the millimetre emission, we estimate the dust mass as ${\sim}0.016\,M{\oplus}$, and constrain lower-limit planetesimal sizes as $D_{\rm{max}}{>}1\,$km and the planetesimal belt mass as $M_{\rm{disc}}{>}1\,M_{\oplus}$. We constrain the properties of an outer body causing a linear trend in 17 years of radial velocity data to have a semi-major axis $8{-}66\,$au and a mass $(0.4{-}120)\,M_{\rm{Jup}}$. There is a large inner cavity seen in the millimetre emission, which we show is consistent with carving by such an outer massive companion with a string of lower mass planets. Our scattered light modelling shows that the dust must have a high anisotropic scattering factor ($g{\sim}0.8{-}0.9$) but an inclination ($i{\sim}30{-}40\,$degrees) that is inferred to be significantly lower than the $i{\sim}61\,$degrees millimetre inclination. The origin of such a discrepancy is unclear, but could be caused by a misalignment in the micron and millimetre sized dust. We place an upper limit on the CO gas mass of $M_{\rm{CO}}{<}(4.2{-}13){\times}10^{-7}\,M_{\oplus}$, and show this to be consistent with levels expected from planetesimal collisions, or from CO-ice sublimation as $κ$CrB begins its giant branch ascent.
description: Accepted for publication in MNRAS. 21 pages, 14 figures
Two-spinor geometry and gauge freedom
Creators: name: Canarutto, Daniel
Publisher: name: arXiv
Year: 2014
Subjects: subject: Mathematical Physics (math-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences
subject: 81R25, 81V10, 81T20

description: Gauge freedom in quantum particle physics is shown to arise in a natural way from the geometry of two-spinors (Weyl spinors). Various related mathematical notions are reviewed, and a special ansatz of the kind "the system defines the geometry" is discussed in connection with the stated results.
description: Elaboration of work presented at the workshop "Geometry and Quantum Theories", held in Florence, June 10-11, 2013, on the occasion of the retirement of Luigi Mangiarotti and Marco Modugno, International Journal of Geometric Methods in Modern Physics (2014)
Sonnenfleckenzeichnung Nr. 78.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 11.04.1996, 07:30, erstellt von Sergio Cortesi
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 4.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Spin Transfer Torque in Antiferromagnetic Spin-Valves: From Clean to Disordered Regimes
Creators: name: Saidaoui, Hamed Ben Mohamed
name: Waintal, Xavier
name: Manchon, Aurelien
Publisher: name: arXiv
Year: 2014
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Current-driven spin torques in metallic spin-valves composed of antiferromagnets are theoretically studied using the non-equilibrium Green's function method implemented on a tight-binding model. We focus our attention on G-type and L-type antiferromagnets in both clean and disordered regimes. In such structures, spin torques can either rotate the magnetic order parameter coherently (coherent torque) or compete with the internal antiferromagnetic exchange (exchange torque). We show that, depending on the symmetry of the spin-valve, the coherent and exchange torques can be either in the plane, α n\times(q \times n) or out of the plane α n \times q, where q and n are the directions of the order parameter of the polarizer and the free antiferromagnetic layers, respectively. Although disorder conserves the symmetry of the torques, it strongly reduces the torque magnitude, pointing out the need for momentum conservation to ensure strong spin torque in antiferromagnetic spin-valves
description: 10 pages, 11 figures
Sonnenfleckenzeichnung Nr. 282.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 06.12.1996, 08:30, erstellt von Sergio Cortesi
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 4.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Análise de processos jurídicos: Caso 18 - Ação Trabalhista - Rito Ordinário 0000855-16.2012.5.10.0111; Voto No 4315/2019 Procedimento No 1007626-09.2019.4.01.3400; Decisão 2019 (PGR-00374674/2019); Tomo n. 1007626-09.2019.4.01.3400; n. 1007626-09.2019.4.01.3400; (JF- Autuação:25/03/2019 / DF-1007626-09.2019.4.01.3400-RPCR).
Creators: name: BRASIL. Ministério Da Justiça
Publisher: name: Zenodo
Year: 2023

description: Análise de processos jurídicos: Caso 18 - Ação Trabalhista - Rito Ordinário 0000855-16.2012.5.10.0111; Voto No 4315/2019
 Procedimento No 1007626-09.2019.4.01.3400; Decisão 2019 (PGR-00374674/2019); Tomo n. 1007626-09.2019.4.01.3400; n. 1007626-09.2019.4.01.3400; (JF- Autuação:25/03/2019 / DF-1007626-09.2019.4.01.3400-RPCR).