cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÑÐµÐ½ÐºÐ° Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¿ÑÐ¸Ð²Ð»ÐµÐºÐ°ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ° Â«ÐÑÐµÐ»Ñ 3 Ð·Ð²ÐµÐ·Ð´Ñ Ð² Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÐµÂ»
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ¸Ð³Ð¾ÑÑÐµÐ²Ð°, ÐÐ½Ð°ÑÑÐ°ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¸
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Characterization of large area APDs for the EXO-200 detector
Creators: name: Neilson, R.
name: LePort, F.
name: Pocar, A.
name: Kumar, K.
name: Odian, A.
name: Prescott, C. Y.
name: Tenev, V.
name: Ackerman, N.
name: Akimov, D.
name: Auger, M.
name: Benitez-Medina, C.
name: Breidenbach, M.
name: Burenkov, A.
name: Conley, R.
name: Cook, S.
name: deVoe, R.
name: Dolinski, M. J.
name: Fairbank, W.
name: Farine, J.
name: Fierlinger, P.
name: Flatt, B.
name: Gornea, R.
name: Gratta, G.
name: Green, M.
name: Hall, C.
name: Hall, K.
name: Hallman, D.
name: Hargrove, C.
name: Herrin, S.
name: Hodgson, J.
name: Kaufman, L. J.
name: Kovalenko, A.
name: Leonard, D. S.
name: Mackay, D.
name: Mong, B.
name: Diez, M. Montero
name: Niner, E.
name: O'Sullivan, K.
name: Piepke, A.
name: Rowson, P. C.
name: Sinclair, D.
name: Skarpaas, K.
name: Slutsky, S.
name: Stekhanov, V.
name: Strickland, V.
name: Twelker, K.
name: Vuilleumier, J. -L.
name: Wamba, K.
name: Wichoski, U.
name: Wodin, J.
name: Yang, L.
name: Yen, Y. -R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: EXO-200 uses 468 large area avalanche photodiodes (LAAPDs) for detection of scintillation light in an ultra-low-background liquid xenon (LXe) detector. We describe initial measurements of dark noise, gain and response to xenon scintillation light of LAAPDs at temperatures from room temperature to 169K - the temperature of liquid xenon. We also describe the individual characterization of more than 800 LAAPDs for selective installation in the EXO-200 detector.
description: 10 pages, 17 figures
Modeling the Formation of Giant Planet Cores I: Evaluating Key Processes
Creators: name: Levison, H. F.
name: Thommes, E.
name: Duncan, M. J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: One of the most challenging problems we face in our understanding of planet formation is how Jupiter and Saturn could have formed before the the solar nebula dispersed. The most popular model of giant planet formation is the so-called 'core accretion' model. In this model a large planetary embryo formed first, mainly by two-body accretion. This is then followed by a period of inflow of nebular gas directly onto the growing planet. The core accretion model has an Achilles heel, namely the very first step. We have undertaken the most comprehensive study of this process to date. In this study we numerically integrate the orbits of a number of planetary embryos embedded in a swarm of planetesimals. In these experiments we have included: 1) aerodynamic gas drag, 2) collisional damping between planetesimals, 3) enhanced embryo cross-sections due to their atmospheres, 4) planetesimal fragmentation, and 5) planetesimal driven migration. We find that the gravitational interaction between the embryos and the planetesimals lead to the wholesale redistribution of material - regions are cleared of material and gaps open near the embryos. Indeed, in 90% of our simulations without fragmentation, the region near that embryos is cleared of planetesimals before much growth can occur. The remaining 10%, however, the embryos undergo a burst of outward migration that significantly increases growth. On timescales of ~100,000 years, the outer embryo can migrate ~6 AU and grow to roughly 30 Earth-masses. We also find that the inclusion of planetesimal fragmentation tends to inhibit growth.
description: Accepted to AJ, 62 pages 11 figures
Reduction theory of point clusters in projective space
Creators: name: Stoll, Michael
Publisher: name: arXiv
Year: 2009
Subjects: subject: Number Theory (math.NT)
subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics
subject: 11E10, 11H55 (primary), 14L24, 14H50, 14Q99 (secondary)

description: In this paper, we generalise results obtained earlier by John Cremona and the author on the reduction theory of binary forms, which describe positive zero-cycles in P^1, to positive zero-cycles (or point clusters) in projective spaces of arbitrary dimension. This should have applications to more general projective varieties in P^n, by associating a suitable positive zero-cycle to them in an PGL(n+1)-invariant way. We discuss this in the case of (smooth) plane curves.
description: 12 pages
The excitation of spiral density waves through turbulent fluctuations in accretion discs I: WKBJ theory
Creators: name: Heinemann, T.
name: Papaloizou, J. C. B.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study and elucidate the mechanism of spiral density wave excitation in a differentially rotating turbulent flow. We formulate a set of wave equations with sources that are only non-zero in the presence of turbulent fluctuations. We solve these in a shearing box domain using a WKBJ method. It is found that, for a particular azimuthal wave length, the wave excitation occurs through a sequence of regularly spaced swings during which the wave changes from leading to trailing form. This is a generic process that is expected to occur in shearing discs with turbulence. Trailing waves of equal amplitude propagating in opposite directions are produced, both of which produce an outward angular momentum flux that we give expressions for as functions of the disc parameters and azimuthal wave length. By solving the wave amplitude equations numerically we justify the WKBJ approach for a Keplerian rotation law for all parameter regimes of interest. In order to quantify the wave excitation completely the important wave source terms need to be specified. Assuming conditions of weak nonlinearity, these can be identified and are associated with a quantity related to the potential vorticity, being the only survivors in the linear regime. Under the additional assumption that the source has a flat power spectrum at long azimuthal wave lengths, the optimal azimuthal wave length produced is found to be determined solely by the WKBJ response and is estimated to be 2 pi H, with H being the nominal disc scale height.
description: Replaced "inertial acoustic waves" with "spiral density waves"
Normalizing Weak Boson Pair Production at the Large Hadron Collider
Creators: name: Campbell, J. M.
name: Castaneda-Miranda, E.
name: Fang, Y.
name: Kauer, N.
name: Mellado, B.
name: Wu, Sau Lan
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The production of two weak bosons at the Large Hadron Collider will be one of the most important sources of SM backgrounds for final states with multiple leptons. In this paper we consider several quantities that can help normalize the production of weak boson pairs. Ratios of inclusive cross-sections for production of two weak bosons and Drell-Yan are investigated and the corresponding theoretical errors are evaluated. The possibility of predicting the jet veto survival probability of VV production from Drell-Yan data is also considered. Overall, the theoretical errors on all quantities remain less than 5-20%. The dependence of these quantities on the center of mass energy of the proton-proton collision is also studied.
description: 11 pages; added references, minor text revisions, version to appear in Phys. Rev. D
GIT-equivalence and diagonal actions
Creators: name: Kotenkova, Polina Yu.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics

description: We describe the GIT-equivalence classes of linearized ample line bundles for the diagonal actions of the linear algebraic groups $SL(V)$ and $SO(V)$ on ${\mathbb{P}(V)^{m_1}\times \mathbb{P}(V^*)^{m_2}}$ and $\mathbb{P}(V)^m$ respectively.
Positivity in Rieffel's strict deformation quantization
Creators: name: Waldmann, Stefan
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We review a recent result on Rieffel's deformation quantization by actions of R^d: it is shown that for every state omega_0 of the undeformed C*-algebra A_0 there is a continuous section of states omega(hbar) through omega_0. We outline the physical interpretation in terms of quantization.
description: Contribution to the Proceedings of the ICMP 2009, 6 pages
title: The Democratic Purpose Of Postsecondary Education: Comparing Public, Private Nonprofit, And Private For-Profit Mission Statements For Expression Of Democratic Social Purpose
Creators: name: Youngberg, Lon
Publisher: name: Utah State University
Year: 2008

description: Thomas Jefferson envisioned a symbiotic relationship between democracy and public education because he considered educated citizens to be the critical ingredient of a successful democracy. Nevertheless, political and educational reforms over the past two centuries have not always been kind to the relationship that Jefferson envisioned. This study examines frequency that postsecondary education institutions declare a democratic social purpose in their mission statements. The DSP definition, data instrumentation, and theoretical lens for this study were situated from the Jeffersonian perspective. Although the primary concern for this study was publicly funded/subsidized postsecondary education, recent enrollment growth in private education and privatization initiatives, such as voucher programs, justifies comparison with private nonprofit and private for-profit institutions to reveal how the different types of institutional control influence DSP. The comparison also provides a sense of the non-economic consequences of reduced public education subsidy and intentional or unintentional privatization. A number of Carnegie classification variables were also examined to better understand what factors influence DSP expression. This study utilized a national random sample of undergraduate institutions, from associates colleges to research universities. The sample size was 336 and there were no cases of missing data. Interrater reliability was calculated as .873 Kappa on the dichotomous dependent variable (DSP presence or absence). The first research objective was to determine if public, private nonprofit, and private for-profit institutional mission statements differ in the frequency of DSP expression. Public institutions exhibited 36.5% DSP, private nonprofit institutions exhibited 69.1% DSP, and private for-profit institutions exhibited 11.9% DSP. Chi-square test determined that there was significant difference between each of 2x2 comparisons (p < .003). The second research objective utilized logistic regression analysis to gauge the influence of several variables on DSP frequency. Institutional control, focus, enrollment, and mission statement length were found to be significant at the p = .05 level. There are differences between public and private institutions and also between two-year and four-year institutions in the frequency of DSP expression. These differences have serious social and political implications that will likely go unnoticed as the bulk of society focuses on private and economic concerns.
Neighborhood Ethnic Composition and Social Identity Threat: The Mediating role of Perceived Discrimination
Creators: name: Camacho, Gabriel
Publisher: name: OSF Registries
Year: 2023
Subjects: subject: Social and Behavioral Sciences

description: This is the project presenting materials and the data relating to the paper entitled "Neighborhood Ethnic Composition and Social Identity Threat: The Mediating Role of Perceived Discrimination”.
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title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð»ÐºÐ¾Ð²Ð°, ÐÐ°Ð´ÐµÐ¶Ð´Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑ
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title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ»Ð¸Ð½Ð¸Ñ, ÐÐ°ÑÐ°Ð»ÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐ½Ð¸Ð²ÐµÑÑÐ°Ð»ÑÐ½ÑÐ¹ Ð¿ÐµÑÐµÐ´Ð°ÑÐ¾ÑÐ½ÑÐ¹ Ð´Ð¾ÐºÑÐ¼ÐµÐ½Ñ
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title: ÐÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð°ÑÑÐ¸Ð²Ð½ÑÑ Ð¡ÐÐ§ Ð¸Ð½ÑÐµÐ³ÑÐ°Ð»ÑÐ½ÑÑ ÑÑ ÐµÐ¼ Ð½Ð° ÑÐ¾ÑÑÐµÐ´Ð¾ÑÐ¾ÑÐµÐ½Ð½ÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ°Ñ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐµÐ¼Ð°ÑÐ°ÑÐ½Ð°, Ð¥ÐµÑÑÐ¸
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð¡ÐÐ§ ÐÐÐ¡
Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÐµ Ð¾ÑÐ²ÐµÑÐ²Ð¸ÑÐµÐ»Ð¸
Ð¿Ð°ÑÐ°Ð·Ð¸ÑÐ½ÑÐµ ÑÐ»ÐµÐ¼ÐµÐ½ÑÑ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð° ÑÐ°ÑÑÐµÑ Ð¿ÑÐ¾ÑÐ¾ÑÐ¸Ð¿Ð¾Ð² Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¾ÑÐ²ÐµÑÐ²Ð¸ÑÐµÐ»Ñ Ð½Ð° Ð¸Ð´ÐµÐ°Ð»ÑÐ½ÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ°Ñ, Ð½Ð° ÑÐ¾ÑÑÐµÐ´Ð¾ÑÐ¾ÑÐµÐ½Ð½ÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ°Ñ Ð¸ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¾ÑÐ²ÐµÑÐ²Ð¸ÑÐµÐ»Ñ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ¸ÑÑÐµÐ¼Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾
Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¡ÐÐ§ ÐÐÐ¡ Advanced Design System ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Keysight Technologies. ÐÐ»Ñ ÑÐ¼ÐµÐ½ÑÑÐµÐ½Ð¸Ñ Ð´Ð¸ÑÐ±Ð°Ð»Ð°Ð½ÑÐ° ÑÐ°Ð· Ð¸ Ð°Ð¼Ð¿Ð»Ð¸ÑÑÐ´ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¾ÑÑÐµÐ´Ð¾ÑÐ¾ÑÐµÐ½Ð½ÑÑ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÑ Ð¾ÑÐ²ÐµÑÐ²Ð¸ÑÐµÐ»ÐµÐ¹ Ñ ÑÑÐµÑÐ¾Ð¼ Ð¿Ð°ÑÐ°Ð·Ð¸ÑÐ½ÑÑ ÑÑÑÐµÐºÑÐ¾Ð² Ð² ÑÐ¾ÑÑÑÐµÐ´Ð¾ÑÐ¾ÑÐµÐ½Ð½ÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ°Ñ.
Средства выражения экспрессивности на синтаксическом уровне и их воссоздание в переводе (на примере романа Г.Ф. Лавкрафта «Случай Чарльза Декстера Варда» и его перевода на русский язык)
Creators: name: Первак, Татьяна
Publisher: name: ООО Цифра
Year: 2023
Subjects: expressiveness
evaluative
syntactic means
translation text
экспрессивность
оценочность
синтаксические средства
текст перевода

description: Международный научно-исследовательский журнал, Выпуск 5 (131) 2023
title: ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ ÑÑÐ½Ð¾ÑÐ½Ð¾Ð¹ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¾Ð±ÑÐµÐºÑÐ° Ð¶Ð¸Ð»Ð¾Ð¹ Ð½ÐµÐ´Ð²Ð¸Ð¶Ð¸Ð¼Ð¾ÑÑÐ¸
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð´Ð¾Ð»Ð¾Ð²Ð°, ÐÐ°ÑÐ³Ð°ÑÐ¸ÑÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð¾Ð±ÑÐµÐºÑ Ð¾ÑÐµÐ½ÐºÐ¸
Ð½ÐµÐ´Ð²Ð¸Ð¶Ð¸Ð¼Ð¾ÑÑÑ
Ð´Ð¾Ñ Ð¾Ð´Ð½ÑÐ¹ Ð¿Ð¾Ð´Ñ Ð¾Ð´
ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð¿Ð¾Ð´Ñ Ð¾Ð´
Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐ°ÑÑ Ð¾Ð´Ñ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð¶Ð¸Ð»Ð°Ñ Ð½ÐµÐ´Ð²Ð¸Ð¶Ð¸Ð¼Ð¾ÑÑÑ.
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Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¼ÐµÑÑÐ¾Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¾ÑÐµÐ½Ð¸Ð²Ð°ÐµÐ¼Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÐºÑÐ°. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ñ Ð²ÑÐµ ÑÐ°ÑÑÐµÑÑ, Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÑ Ð¾Ð±ÑÐµÐºÑÐ° Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð¾Ð² Ðº Ð¾ÑÐµÐ½ÐºÐµ. ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¾ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð².
The rat brain on fentanyl : assessment of cellular and molecular changes with single-cell and spatial resolution
Creators: name: Daswani, Rishika Rajender
Publisher: name: University of British Columbia
Year: 2024

description: Opioid addiction, particularly to fentanyl, presents significant public health challenges, necessitating a deeper understanding of its neurobiological underpinnings. This study employs a multiomics approach to elucidate brain circuitry changes resulting from fentanyl self-administration in rats. Over a 15-day self-administration period, with 10 days of continuous access followed by 5 days of intermittent access, we observed notable alterations in specific neuronal populations and gene expression profiles. The single-nuclei RNA sequencing (snRNA-seq) data revealed an increase in GABAergic neurons expressing the Megf11 gene and a decrease in glutamatergic neurons expressing the Hox5b gene in fentanyl-exposed rats. Fentanyl significantly downregulated genes in Cerebellar Granule Glutamatergic (CB Granule Glut) neurons including Cx3cr1, Ets1, and Dock8, and upregulated genes such as Prckg and Nudt7. In the Cerebellar Cortex Purkinje GABAergic (CBX Purkinje Gaba) neurons, we identified mostly mitochondrial genes being upregulated. Using both single-nuclei ATAC-seq (snATAC-seq) and SnRNA-seq analysis, we identified genes that were both differentially regulated and expressed, particularly Skap2, Arhgap15, Slc25a13, and Akap13. Pathway analysis revealed that fentanyl upregulates the Signal transduction of S1P receptor pathway in CB Granule Glut neurons. Additionally, spatial analysis using the NanoString CosMx Spatial Molecular Imager highlighted spatially variable genes such as Ttr and Malat1 and identified ten spatially resolved clusters. Our study is the first to utilize a multiomics approach to investigate fentanyl's impact on brain circuitry, providing a detailed map of molecular changes associated with chronic fentanyl exposure. These findings contribute to the growing body of knowledge on the neural mechanisms of opioid addiction, offering potential targets for therapeutic intervention. Future directions include exploring sex-specific differences, validating findings through gene knockouts, and exploring behavioral consequences in confirmatory studies. Such efforts will enhance our understanding of the functional roles of identified genes and aid in developing targeted treatments for opioid use disorder.
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐµÐ¶Ð¸Ð¼Ð°Ð¼Ð¸ ÑÐ°Ð±Ð¾ÑÑ ÑÐµÑÐ¼Ð¾Ñ Ð¸Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐµÐ°ÐºÑÐ¾ÑÐ°
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐµÐ½ÑÑÐ°ÐºÐ¾Ð²Ð°, ÐÐ»ÐµÐºÑÐ°Ð½Ð´ÑÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÐÐµÑÐ°ÑÐµÐ»ÑÐ½ÑÐµ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÑ ÑÐ²ÐµÑÑ Ð·Ð²ÑÐºÐ¾Ð²ÑÐµ
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active thermal protection method
thermochemical reactors
steam reforming

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐµÑÐ¼Ð¾ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐµÐ°ÐºÑÐ¾ÑÐ°, Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÑÑÐµÐ³Ð¾ ÑÑÐ¸Ð»Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐµÐ¿Ð»Ð° Ð² ÑÐ¾Ð´Ðµ ÑÐ½Ð´Ð¾ÑÐµÑÐ¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐµÐ°ÐºÑÐ¸Ð¸ Ð¿Ð°ÑÐ¾Ð²Ð¾Ð¹ ÐºÐ¾Ð½Ð²ÐµÑÑÐ¸Ð¸ ÑÐ³Ð»ÐµÐ²Ð¾Ð´Ð¾ÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ ÑÐ¾Ð¿Ð»Ð¸Ð²Ð° Ñ Ð¾Ð´Ð½Ð¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ Ð½Ð°ÑÐ°Ð±Ð¾ÑÐºÐ¾Ð¹ Ð²Ð¾Ð´Ð¾ÑÐ¾Ð´Ð°. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ ÑÐ°ÑÑÐµÑÐ½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° Ð´Ð»Ñ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÑÐ¼Ð¾ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐµÐ°ÐºÑÐ¾ÑÐ°. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¼Ð¾Ð´ÐµÐ»Ð¸ ÑÐµÑÐ¼Ð¾ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐµÐ°ÐºÑÐ¾ÑÐ°. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² ÑÐµÑÐ¼Ð¾ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐµÐ°ÐºÑÐ¾ÑÐ° Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ñ Ð³ÑÐ°Ð½Ð¸ÑÐ½ÑÐ¼Ð¸ ÑÑÐ»Ð¾Ð²Ð¸ÑÐ¼Ð¸ Ð¿ÐµÑÐ²Ð¾Ð³Ð¾ Ð¸ Ð²ÑÐ¾ÑÐ¾Ð³Ð¾ ÑÐ¾Ð´Ð°. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ ÑÐ°ÑÑÐµÑ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² ÑÐ°Ð±Ð¾ÑÑ ÑÐµÑÐ¼Ð¾ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐµÐ°ÐºÑÐ¾ÑÐ° Ð² ÑÐ¾ÑÑÐ°Ð²Ðµ ÑÑÐ±Ð°ÑÐºÐ¸ Ð¾ÑÐ»Ð°Ð¶Ð´ÐµÐ½Ð¸Ñ ÐºÐ°Ð½Ð°Ð»Ð° Ð¿ÑÑÐ¼Ð¾ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ Ð´Ð°Ð½Ð½ÑÑ Ð´Ð»Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÐ¾Ð¹ ÑÐµÑÐ¼Ð¾ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐµÐ°ÐºÑÐ¾ÑÐ°.
description: This work is devoted to the study of effective work modes of thermochemical reactor that provides recycling of heat during the endothermic reaction of steam reforming with simultaneous conversion of hydrocarbon fuels to hydrogen. The design principle of calculation complex used to simulate a thermochemical reactor is studied. Justifications of a mathematical model of thermochemical reactor are provided. Calculations of thermochemical reactor parameters study with boundary conditions of the first and second kind are executed. The calculation of operating modes of the thermochemical reactor as part of the cooling covering of ramjet engine channel is handled and a comparative analysis of acquired data is made to determine the most effective management work modes for thermochemical reactor.
Observational Evidence for Cosmological-Scale Extra Dimensions
Creators: name: Afshordi, Niayesh
name: Geshnizjani, Ghazal
name: Khoury, Justin
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We present a case that current observations may already indicate new gravitational physics on cosmological scales. The excess of power seen in the Lyman-alpha forest and small-scale CMB experiments, the anomalously large bulk flows seen both in peculiar velocity surveys and in kinetic SZ, and the higher ISW cross-correlation all indicate that structure may be more evolved than expected from LCDM. We argue that these observations find a natural explanation in models with infinite-volume (or, at least, cosmological-size) extra dimensions, where the graviton is a resonance with a tiny width. The longitudinal mode of the graviton mediates an extra scalar force which speeds up structure formation at late times, thereby accounting for the above anomalies. The required graviton Compton wavelength is relatively small compared to the present Hubble radius, of order 300-600 Mpc. Moreover, with certain assumptions about the behavior of the longitudinal mode on super-Hubble scales, our modified gravity framework can also alleviate the tension with the low quadrupole and the peculiar vanishing of the CMB correlation function on large angular scales, seen both in COBE and WMAP. This relies on a novel mechanism that cancels a late-time ISW contribution against the primordial Sachs-Wolfe amplitude.
description: 20 pages, 14 figures, added references and discussion of X-ray clusters
Infestation, Damage and Distribution of Blue Gum Chalcid on Eucalyptus camaldulensis Dehnh in Eastern Amhara, Ethiopia
Creators: name: Redae *, Tigabu
name: Tesfaye, Adane
name: Muhie, Seid
Publisher: name: Abyssinia Journal of Science and Technology
Year: 2020

description: Blue Gum Chalcid (BGC), Leptocybe invasa Fisher and La Salle (Hymenoptera: Eulophidae), causes high damages on Eucalyptus camaldulensis Dehnh in many countries including Ethiopia. This study aimed to determine the damage, damage severity and distribution of the BGC on Eucalyptus camaldulensis plantations in Eastern Amhara, Ethiopia. The assessment was conducted at Tehuledere (South Wollo zone), Habru (North Wollo Zone) and Dawa Chefa (Oromia adminstration zone) districts. These districts were selected purposively for continuous infestation. Three sites per district with a total of nine sites were selected. Assessments were done from four coppiced and five plantations. A minimum of 0.25 ha and five trees per site were assessed in a monthly interval. The assessment result revealed that BGC was found in all the three districts of the three zones. During the assessment, it was found that from five trees the damage severity were 20% nil, 15.6% low, 20% medim, 22.2 high, and 22.2% high. Severity and damage of the pest varied across the study sites and the assessment months. Lower and higher severity damages were observed at Amumo (0.48) and Passo sites (3.26) of Tehulederie district, respectively. Increment in damage severity was observed from November to February except at Amumo (from 0.48 to 0.87), with higher increments in January and February 2019 (averagely from 2.24 to 3.23).
description: Abyssinia Journal of Science and Technology, Vol. 5 No. 2 (2020)
MPEC 2024-S82 : 2024 SV1
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2024
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2024 SV1

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
title: International Business. How to start up overseas?
title: ÑÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¾Ð±Ð¸ÑÐµÐ²Ð°, ÐÐ»ÐµÐºÑÐ°Ð½Ð´ÑÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2020
Subjects: Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¸Ð¹ ÑÐ·ÑÐº
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description: Ð£ÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ° Ð´Ð»Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÐµÐ±Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Ð½Ð° Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð¼ ÑÐ·ÑÐºÐµ Â«International BusinessÂ». Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð° Ð¸Ð½ÑÑÑÑÐºÑÐ¸Ñ Ð¿Ð¾ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° X-Culture Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ. Ð£ÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÑÑ Ð±Ð°Ð·Ñ Ð´Ð»Ñ Ð¾ÑÐ²Ð¾ÐµÐ½Ð¸Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«ÐÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð±Ð¸Ð·Ð½ÐµÑÂ». ÐÐ»Ð°Ð²Ð½Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐ¼ Ð²ÑÑÐ¾Ð´Ð° ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¹ Ð½Ð° Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ ÑÑÐ½Ð¾Ðº, ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¼Ñ Ð¸ ÐºÑÐ»ÑÑÑÑÐ½Ð¾Ð¼Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ñ Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½ÑÑ ÑÑÑÐ°Ð½. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿ÑÐ¸ÑÐ¸Ð½Ñ Ð¸ ÑÐ¿Ð¾ÑÐ¾Ð±Ñ Ð²Ð¼ÐµÑÐ°ÑÐµÐ»ÑÑÑÐ²Ð° Ð¿ÑÐ°Ð²Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð² Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÑ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ñ Ð¸ Ð±Ð¸Ð·Ð½ÐµÑ. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¿ÑÐ¸Ð¼ÐµÑÑ Ð¸Ð½ÑÐµÑÐ²ÐµÐ½ÑÐ¸Ð¹ Ð² ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²Ð°Ñ Ð¸ Ð´Ð°Ð½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð´Ð°Ð½Ð½ÑÑ Ð¸Ð½ÑÐµÑÐ²ÐµÐ½ÑÐ¸Ð¹ Ð½Ð° ÑÑÐµÑÑ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ Ð±Ð¸Ð·Ð½ÐµÑÐ°. ÐÐ¾ ÐºÐ°Ð¶Ð´Ð¾Ð¼Ñ ÑÐ°Ð·Ð´ÐµÐ»Ñ Ð¸Ð¼ÐµÑÑÑÑ ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½ÑÐµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¸ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ.
Additional file 11 of Conservatively transmitted alleles of key agronomic genes provide insights into the genetic basis of founder parents in bread wheat (Triticum aestivum L.)
Creators: name: Li, Chang
name: Zhuang, Lei
name: Li, Tian
name: Hou, Jian
name: Liu, Hongxia
name: Jian, Chao
name: Li, Huifang
name: Zhao, Jing
name: Liu, Yunchuan
name: Xi, Wei
name: Hao, Pingan
name: Liu, Shujuan
name: Si, Xuemei
name: Wang, Xiaolu
name: Zhang, Xueyong
name: Hao, Chenyang
Publisher: name: figshare
Year: 2023
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 11: Figure S1. Physical location of 87 agronomically important genes for grain yield, stress resistance, adaptability, and quality among 21 chromosomes in wheat. The left side of the chromosome indicates physical position (Mb) of each gene and the right shows gene names. Genes for grain yield, stress resistance, adaptability, and quality are represented by red triangles, yellow diamonds, dark blue squares, and green circles, respectively. The physical positions (Mb) of all genes were determined using BLAST against Chinese Spring v1.0.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐ¾ÐµÐºÑÐ° Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Service Desk Ð² Ð¿Ð¾Ð´ÑÐ°Ð·Ð´ÐµÐ»ÐµÐ½Ð¸ÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐ "Ð Ð°Ð²ÐµÐ½ÑÑÐ²Ð¾")
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð°ÑÑÐ°ÐºÐ¾Ð², ÐÐ¸ÑÐ°Ð»Ð¸Ð¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: service desk
itil
helpdeskeddy
cÐ»ÑÐ¶Ð±Ð° ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ¸

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐ¢-Ð¾ÑÐ´ÐµÐ» ÐÐ Â«Ð aÐ²eÐ½ÑÑÐ²oÂ».
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ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÑÐ½ÐºÐ° ÑÐ¸ÑÑÐµÐ¼, Ð±ÑÐ»Ð° Ð²ÑÐ±ÑÐ°Ð½Ñ Ð¿Ð¾Ð¿ÑÐ»ÑÑÐ½ÑÐµ Ð³Ð¾ÑÐ¾Ð²ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ Service Desk Ð½Ð° ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¼ ÑÑÐ½ÐºÐµ Ð¿Ð¾Ð´ÑÐ¾Ð´ÑÑÐ¸Ðµ Ð¿Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÐ¼ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸ÑÐ¼.
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Reticularia jurana Meyl.
Creators: name: Kluša, Julita
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Protozoa
Mycetozoa
Myxomycetes
Cribrariales
Tubiferaceae
Reticularia
Reticularia jurana

description: Reticularia jurana Meyl.,
trauslais gļotpūpēdis
- leg. K.R.Kupfer, 1923, det. G.Adamonytė, 2003; leg. A.Arnicāns, 22 Jun 2020, Rīga, on a log without bark in a pine forest with some deciduous trees, det. J.Kluša, 2020; (NMKK), very rare.
description: Published as part of Kluša, Julita, 2023, Complete Checklist Of Myxomycetes In Latvia, pp. 127-151 in Acta Biologica Universitatis Daugavpiliensis 23 (2) on pages 127-151, DOI: 10.59893/abud.23(2).002, http://zenodo.org/record/12650118
The XMM-Newton Slew Survey: Towards The Whole X-ray Sky and the Rarest X-ray Events
Creators: name: Read, A. M.
name: Saxton, R. D.
name: Esquej, P.
name: Warwick, R. S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The data collected by XMM-Newton as it slews between pointings currently cover almost half the entire sky, and many familiar features and new sources are visible. The soft-band sensitivity limit of the Slew is close to that of the RASS, and a large-area Slew-RASS comparison now provides the best opportunity for discovering extremely rare high-variability objects.
description: To appear in Proceedings of "X-ray Astronomy 2009: Present Status, Multi-Wavelength Approach and Future Perspectives", Bologna, Italy, September 7-11, 2009, AIP, eds. A. Comastri, M. Cappi, and L. Angelini
Relativistic Simulations of Black Hole-Neutron Star Mergers: Effects of black-hole spin
Creators: name: Etienne, Zachariah B.
name: Liu, Yuk Tung
name: Shapiro, Stuart L.
name: Baumgarte, Thomas W.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Black hole-neutron star (BHNS) binary mergers are candidate engines for generating both short-hard gamma-ray bursts (SGRBs) and detectable gravitational waves. Using our most recent conformal thin-sandwich BHNS initial data and our fully general relativistic hydrodynamics code, which is now AMR-capable, we are able to efficiently and accurately simulate these binaries from large separations through inspiral, merger, and ringdown. We evolve the metric using the BSSN formulation with the standard moving puncture gauge conditions and handle the hydrodynamics with a high-resolution shock-capturing scheme. We explore the effects of BH spin (aligned and anti-aligned with the orbital angular momentum) by evolving three sets of initial data with BH:NS mass ratio q=3: the data sets are nearly identical, except the BH spin is varied between a/M = -0.5 (anti-aligned), 0.0, and 0.75. The number of orbits before merger increases with a/M, as expected. We also study the nonspinning BH case in more detail, varying q between 1, 3, and 5. We calculate gravitational waveforms for the cases we simulate and compare them to binary black-hole waveforms. Only a small disk (< 0.01 M_sun) forms for the anti-aligned spin case (a/M = -0.5) and for the most extreme mass ratio case (q=5). By contrast, a massive (M_disk is about 0.2 M_sun), hot disk forms in the rapidly spinning (a/M = 0.75) aligned BH case. Such a disk could drive a SGRB,possibly by, e.g., producing a copious flux of neutrino-antineutino pairs.
description: 28 pages, 24 figures, replaced with the published version, minor changes
The Effect of the Dosage of Table Salt on the Change of Rheological Properties of Wheat Dough
Creators: name: Kasyanov, Gennadii
Publisher: name: Cifra LLC
Year: 2023
Subjects: flour
kneading
dough
bread
Farinograf E
Strukturometr
Rheofermentometre
мука
замес
тесто
хлеб
Фаринограф Е
Структурометр
Реоферментометр

description: Международный научно-исследовательский журнал, Выпуск 5 (131) 2023
title: Transitional Flow Between Orifice and Non-Orifice Regimes at a Rectangular Canal Gate
Creators: name: Cabezas, Omar Alminagorta
Publisher: name: Utah State University
Year: 2008

description: The main objective of this research was to analyze the hydraulic transition between non-orifice and orifice flow regimes at a rectangular sluice gate through the calibration of various discharge equations, and determining the value of a coefficient, which defines the transition between orifice and non-orifice flow conditions. The second objective was to determine whether a single equation could be used to represent the stage-discharge relationship for both free and submerged non-orifice flow through a rectangular sluice gate. Several hundred data sets were collected in a hydraulic laboratory, each including the measurement of water upstream depth and downstream for five different gate openings, and 17 different steady-state discharges, from 0.02 to 0.166 m3/s. Three approaches were used to define the limits of the non-orifice-to-orifice regime transition: (1) using an empirical equation; (2) using the traditional submerged non-orifice equation; and (3) using the specific-energy equation for open-channel flow. Based on the results of this research, the latter approach was ultimately chosen to define the boundaries of the transition between orifice and non-orifice flow regimes. Once the transition limits were defined, the estimation of the non-orifice-to-orifice transition coefficient, Co , was made. The transition coefficient was defined as the ratio of gate opening to upstream water depth. The experimental results indicate that orifice flow always exists when Co is less than 0.83, and non-orifice flow always exists when Co is greater than 1.00. To identify the flow regime (orifice or non-orifice) within the range 0.83 < Co < 1.00, it is necessary to consider the submergence, S, which is the ratio of downstream to upstream water depth. With respect to the second objective, laboratory data for non-orifice flow regimes were used to test several different empirical equation forms that could potentially represent both free and submerged flow conditions. The strategy was to find a relationship among flow rate, upstream depth, downstream depth, and submergence. As a result of the analysis, one particular equation form was found to have a relatively high coefficient of determination and low standard error of the estimate. This equation fits the laboratory data for submergences up to 0.87 with a discharge error not exceeding +-10%.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿Ð»Ð°Ð½Ð° Ð»Ð¾ÐºÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð»Ð¸ÐºÐ²Ð¸Ð´Ð°ÑÐ¸Ð¸ Ð°Ð²Ð°ÑÐ¸Ð¹Ð½ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¹ Ð² ÑÐ°Ñ ÑÐ°Ñ
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð¨ÑÐ»ÑÑÐµÐ²Ð°, ÐÐ»ÑÐ³Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÐÐ¾ÑÐ½ÑÐµ ÑÐ°Ð±Ð¾ÑÑ
Ð¥Ð¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð²ÐµÑÐµÑÑÐ²Ð°
ÐÐ·ÑÑÐ²ÑÐ°ÑÑÐµ Ð²ÐµÑÐµÑÑÐ²Ð°
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Ð°Ð²Ð°ÑÐ¸Ð¹Ð½ÑÐµ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¸
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description: ÐÐ°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ Ð¸ÑÑÐ»ÐµÐ´ÑÐµÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÑ Ð¿Ð»Ð°Ð½Ð° Ð»Ð¾ÐºÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð»Ð¸ÐºÐ²Ð¸Ð´Ð°ÑÐ¸Ð¸ Ð°Ð²Ð°ÑÐ¸Ð¹Ð½ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¹ Ð² ÑÐ°ÑÑÐ°Ñ. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÐºÑÐ¸ÑÐµÑÐ¸Ð¸ Ð¸ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ Ðº Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð´Ð»Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð´Ð»ÐµÐ½Ð¸Ñ ÑÑÐ¾ÐºÐ° ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¸ Ð¸ÑÑÐ»ÐµÐ´ÑÐµÐ¼Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÐºÑÐ°.
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title: Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾ÐµÐºÑÐ°Ð¼Ð¸
title: Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ°Ð±Ð¾Ñ
titleType: Subtitle
Creators: name: ÐÐ°Ð²Ð»Ð¾Ð², ÐÐ¸ÐºÐ¾Ð»Ð°Ð¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾ÐµÐºÑÐ°Ð¼Ð¸

description: Ð¡Ð¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½ÑÐ¼ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ°Ð¼ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 38.03.02 Â«ÐÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÂ». ÐÐ°Ð±Ð¾Ñ Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÐ¼ÑÑ Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹ Ð¾ÑÐ²Ð°ÑÑÐ²Ð°ÐµÑ Ð²ÑÐµ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÑÐ°Ð¿Ñ ÑÐ°Ð±Ð¾ÑÑ Ð½Ð°Ð´ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð¼, Ð¾Ñ ÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²ÐºÐ¸ ÐµÐ³Ð¾ Ð¡Ð¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ Ð´Ð¾ Ð¾ÑÑÐ»ÐµÐ¶Ð¸Ð²Ð°Ð½Ð¸Ñ ÑÐ¾Ð´Ð° ÑÐ°Ð±Ð¾ÑÑ Ð¸ ÐµÐµ Ð·Ð°Ð²ÐµÑÑÐµÐ½Ð¸Ñ. ÐÐ°Ð¶Ð´Ð°Ñ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð° Ð½Ð° ÑÐµÑÐµÐ½Ð¸Ðµ ÐºÐ¾Ð½ÐºÑÐµÑÐ½Ð¾Ð¹ Ð·Ð°Ð´Ð°ÑÐ¸. Ð Ð½Ð°ÑÐ°Ð»Ðµ ÐºÐ°Ð¶Ð´Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÑÐµÑÑÑ Ð·Ð°Ð´Ð°Ð½Ð¸Ðµ. ÐÐ°ÑÐµÐ¼ ÐºÑÐ°ÑÐºÐ¾ Ð¸Ð·Ð»Ð°Ð³Ð°ÑÑÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐµÑÐµÐ½Ð¸Ñ, Ð¾Ð¿Ð¸ÑÑÐ²Ð°ÐµÑÑÑ Ð¿Ð¾ÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÐµÐ³Ð¾ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ. Ð ÐºÐ¾Ð½ÑÐµ Ð´Ð°ÐµÑÑÑ Ð¿ÐµÑÐµÑÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð², ÐºÐ¾ÑÐ¾ÑÑÐµ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð¸ÑÑ Ð½Ð° Ð·Ð°ÑÐ¸ÑÑ ÑÐ°Ð±Ð¾ÑÑ. Ð ÐµÐºÐ¾Ð¼ÐµÐ½Ð´ÑÐµÑÑÑ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹, Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ð¼ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾ÐµÐºÑÐ°Ð¼Ð¸Â», Â«Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¼Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ°Ð¼Ð¸Â». ÐÐ°Ð½Ð½Ð¾Ðµ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ðµ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼Ð¸-Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¸ÐºÐ°Ð¼Ð¸, Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ°Ð¼Ð¸ Ð¸ Ð¼ÐµÐ½ÐµÐ´Ð¶ÐµÑÐ°Ð¼Ð¸, ÑÑÐ¾Ð»ÐºÐ½ÑÐ²ÑÐ¸Ð¼Ð¸ÑÑ Ñ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÑÑ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ°Ð¼Ð¸.