cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÐ½ÐµÐ²Ð¼Ð¾Ð¿ÑÐ¸Ð²Ð¾Ð´ Ð·Ð°Ð¶Ð¸Ð¼Ð½Ð¾Ð³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° ÑÑÐ°Ð½ÐºÐ°
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°Ð»Ð°ÐµÐ², ÐÐ¸ÑÐ°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: Ð¼ÐµÐ¼Ð±ÑÐ°Ð½Ð½ÑÐ¹ Ð¿Ð½ÐµÐ²Ð¼Ð¾Ð¿ÑÐ¸Ð²Ð¾Ð´ Ð¾Ð´Ð½Ð¾ÑÑÐ¾ÑÐ¾Ð½Ð½ÐµÐ³Ð¾ Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ
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Ð·Ð°Ð¶Ð¸Ð¼Ð½Ð¾Ðµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾
ÑÐ°ÑÑÐµÑ ÑÐµÑÐµÐ½Ð¸Ñ Ð³Ð°Ð·Ð°

description: Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð¿Ð¾ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¾Ð´Ð½Ð¾ÑÑÐ¾ÑÐ¾Ð½Ð½ÐµÐ³Ð¾ Ð¼ÐµÐ¼Ð±ÑÐ°Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð½ÐµÐ²Ð¼Ð¾Ð¿ÑÐ¸Ð²Ð¾Ð´Ð° Ð±ÑÐ»Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÐµÐ³Ð¾ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¼Ð¾Ð´ÐµÐ»Ñ, ÑÑÐ¸ÑÑÐ²Ð°ÑÑÐ°Ñ ÑÐµÐ¶Ð¸Ð¼ ÑÐ¾ÑÐ¼Ð¾Ð¶ÐµÐ½Ð¸Ñ. ÐÑÐ±ÑÐ°Ð½Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÐµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½ÑÐµ ÑÐ°Ð·Ð¼ÐµÑÑ Ð¿Ð½ÐµÐ²Ð¼Ð¾ÑÐ¸Ð»Ð¸Ð½Ð´ÑÐ°, Ñ ÑÑÐµÑÐ¾Ð¼ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ ÑÐ°ÑÑÐµÑ Ð´Ð¸Ð°Ð¼ÐµÑÑÐ° ÑÑÑÐ±Ð¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ð° Ð¸ Ð¿ÑÐ¸ÑÐ¾ÐµÐ´Ð¸Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¾ÑÐ²ÐµÑÑÑÐ¸Ð¹, Ð¿ÑÐ¸ ÐºÐ¾ÑÐ¾ÑÑÑ Ð´Ð¾ÑÑÐ¸Ð³Ð°ÐµÑÑÑ Ð¼Ð°ÐºÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ðµ Ð±ÑÑÑÑÐ¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ðµ Ð¿Ð½ÐµÐ²Ð¼Ð¾Ð¿ÑÐ¸Ð²Ð¾Ð´Ð°. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ Ð½Ð°ÑÑÑÐ¾Ð¹ÐºÐ¸ Ð¿Ð½ÐµÐ²Ð¼Ð¾ÑÑÐµÐ¼Ñ, Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÑÑÐ¸Ðµ Ð·Ð°Ð´Ð°Ð½Ð½ÑÐµ ÑÐºÐ¾ÑÐ¾ÑÑÑ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð½ÐµÐ²Ð¼Ð¾Ð¿ÑÐ¸Ð²Ð¾Ð´Ð° Ð¸ Ð¸Ð½ÐµÑÑÐ¸Ð¾Ð½Ð½ÑÑ Ð½Ð°Ð³ÑÑÐ·ÐºÑ Ð¿ÑÐ¸ ÑÐ¾ÑÐ¼Ð¾Ð¶ÐµÐ½Ð¸Ð¸.
Shear and Magnification: Cosmic Complementarity
Creators: name: Van Waerbeke, L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The potential of cosmic shear to probe cosmology is well recognized and future optical wide field surveys are currently being designed to optimize the return of cosmic shear science. High precision cosmic shear analysis requires high precision photometric redshift. With accurate photometric redshifts, it becomes possible to measure the cosmic magnification on galaxies by galaxies and use it as a probe of cosmology. This type of weak lensing measurement will not use galaxy shapes, instead it will strongly rely on precise photometry and detailed color information. In this work it is shown that such a measurement would lead to competitive constraints of the cosmological parameters, with a remarkable complementarity with cosmic shear. Future cosmic shear surveys could gain tremendously from magnification measurements as an independent probe of the dark matter distribution leading to a better control of observational and theoretical systematics when combined with shear.
description: 8 pages, submitted to MNRAS
Hard X-ray Properties of the Merging Cluster Abell 3667 as Observed with Suzaku
Creators: name: Nakazawa, Kazuhiro
name: Sarazin, Craig L.
name: Kawaharada, Madoka
name: Kitaguchi, Takao
name: Okuyama, Sho
name: Makishima, Kazuo
name: Kawano, Naomi
name: Fukazawa, Yasushi
name: Inoue, Susumu
name: Takizawa, Motokazu
name: Wik, Daniel R.
name: Finoguenov, Alexis
name: Clarke, Tracy E.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Wide-band Suzaku data on the merging cluster Abell 3667 were examined for hard X-ray emission in excess to the known thermal component. Suzaku detected X-ray signals in the wide energy band from 0.5 to 40 keV. The hard X-ray (> 10 keV) flux observed by the HXD around the cluster center cannot be explained by a simple extension of the thermal emission with average temperature of ~7 keV. The emission is most likely an emission from a very hot (kT > 13.2 keV) thermal component around the cluster center, produced via a strong heating process in the merger. In the north-west radio relic, no signature of non-thermal emission was observed. Using the HXD, the overall upper-limit flux within a 34'x34' field-of-view around the relic is derived to be 5.3e-12 erg s-1 cm-2 in the 10-40 keV band, after subtracting the ICM contribution estimated using the XIS or the XMM-Newton spectra. Directly on the relic region, the upper limit is further tightened by the XIS data to be less than 7.3e-13 erg s-1 cm-2, when converted into the 10--40 keV band. The latter value suggest that the average magnetic field within the relic is higher than 1.6 uG. The non-thermal pressure due to magnetic fields and relativistic electrons may be as large as ~20% of the thermal pressure in the region.
description: 18 pages, 13 figures, to be appeared in PASJ 2008
title: Windows, atmospheres and experience in medieval Cypriot castles
Creators: name: Jamieson, Erin
Publisher: name: University of Glasgow
Year: 2021
Subjects: subject: Cyprus, medieval archaeology, castles, castle archaeology, medieval Cyprus, spatial archaeology, windows, past experiences, experiential archaeology, crusader archaeology, the crusades, the latin levant.

description: Although often overlooked in archaeology, windows play an important role in past experiences of buildings. In this thesis I am aiming to understand the importance of windows to the experience of medieval Cypriot buildings. To do this I will develop the study of atmospheres as a methodology – initially used as an alternative to phenomenology in prehistoric archaeology, I will show how it can be well suited to historical archaeology, and the study of historical buildings in particular. By using all sources available to us, from historical documents to the standing buildings, contemporary art to personal impressions, we can begin to understand not just what people were experiencing in terms of sensory information, but also what this information meant. Not just holes in walls, windows allow sensory information from other spaces – something which is central in the experience of the spaces in the past, playing a part in social hierarchies, safety and practicality. In order to study this, I have chosen to focus on the medieval buildings of Cyprus, specifically the three castles of St Hilarion, Kyrenia and Kolossi. Experiencing these castles for myself, seen alongside medieval Cypriot, Italian and French sources, I can start to piece together aspects of the experiences of the people who lived and worked in these buildings.
Survival and movements of mule deer (Odocoileus hemionus) in southern British Columbia
Creators: name: Wright, Chloe Antonia
Publisher: name: University of British Columbia
Year: 2024

description: Human induced landscape change has had a profound and lasting impact on the earth, leading to habitat destruction and biodiversity loss. Understanding and reversing the consequences of anthropogenic landscape change is a priority for wildlife managers. An important step in preserving biodiversity is protecting high quality habitat, which is often inferred through resource selection functions (RSFs) and does not include an explicit link between habitat and fitness, potentially leading to incorrect conclusions about what constitutes high-quality habitat for a species. ​In this dissertation, I evaluated the effects of landscape change on mule deer (Odocoileus hemionus) migration and survival in south-central British Columbia, Canada, and estimated whether RSFs correlated with survival and therefore inferred habitat quality. Specifically, I studied deer spring migration in a forested ecosystem disturbed by timber harvesting, identified how exposure to landscape disturbances affected deer survival, and integrated resource selection functions and survival models to quantify habitat quality across seasons and deer ages. To meet these objectives, I placed global positioning system collars on 201 adult female mule deer, 270 fawns, and 134 neonates from 2018 – 2022. ​I found that during spring migration, deer did not time their movements to match the pace of forage green-up, likely because green-up did not occur in a way that was conducive for deer to track. Potentially, timber harvesting has created a mosaic of early and late green-up patches, affecting the order and timing of green-up. Additionally, I found mortality risk increased in the winter when deer used areas with higher road densities and deeper snow. I also found deer that used recent burns and cutblocks had a reduced mortality risk in the summer compared to those that used these disturbances less often. ​Finally, I found that for neonates, fawns, and adults in the summer, selection positively correlated with survival, and RSFs accurately inferred habitat quality. However, for adults in the winter, I observed no relationship between predicted probabilities of use and survival. The common assumption that selection correlates with survival was not met for all deer, highlighting the importance of incorporating survival or fitness-based metrics into models that measure habitat quality.
NACO-SDI imaging of known companion host stars from the AAPS and Keck planet search surveys
Creators: name: Jenkins, J. S.
name: Jones, H. R. A.
name: Biller, B.
name: O'Toole, S. J.
name: Pinfield, D. J.
name: Close, L.
name: Tinney, C. G.
name: Butler, R. P.
name: Wittenmyer, R.
name: Carter, B.
name: Day-Jones, A. C.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Direct imaging of brown dwarfs as companions to solar-type stars can provide a wealth of well-constrained data to "benchmark" the physics of such objects, since quantities like metallicity and age can be determined from their well-studied primaries. We present results from an adaptive optics imaging program on stars drawn from the Anglo-Australian and Keck Planet Search projects, with the aim of directly imaging known cool companions. Simulations have modeled the expected contrast ratios and separations of known companions using estimates of orbital parameters available from current radial-velocity data and then a selection of the best case objects were followed-up with high contrast imaging to attempt to directly image these companions. These simulations suggest that only a very small number of radial-velocity detected exoplanets with consistent velocity fits and age estimates could potentially be directly imaged using the VLT's Simultaneous Differential Imaging system and only under favorable conditions. We also present detectability confidence limits from the radial-velocity data sets and show how these can be used to gain a better understanding of these systems when combined with the imaging data. For HD32778 and HD91204 the detectabilities help little in constraining the companion and hence almost all our knowledge is drawn from the SDI images. Therefore, we can say that these stars do not host cool methane objects, out to on-sky separations of ~2'', with contrasts less than 10-11 magnitudes. However, for HD25874, HD120780 and HD145825, the contrasts and detectabilities can rule out a number of possible solutions, particularly at low angular separations, and for the best case, down to strong methane masses of 40MJ at 1'' separation. The contrast curves constructed for these five stars show 5 sigma contrasts (Delta F1) of ~9.2-11.5 magnitudes at separations of >/=0.6'', which correspond to contrasts of ~9.7-12.0 magnitudes for companions of mid-T spectral type. Such limits allow us to reach down to 40MJ around fairly old field dwarfs that typically constitute high precision radial-velocity programs. Finally, the analysis performed here can serve as a template for future projects that will employ extreme-AO systems to directly image planets already indirectly discovered by the radial-velocity method.
description: 12 pages, 15 figures, accepted for publication in A&A
Arithmetic of Quantum Entropy Function
Creators: name: Sen, Ashoke
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Quantum entropy function is a proposal for computing the entropy associated with the horizon of a black hole in the extremal limit, and is related via AdS/CFT correspondence to the dimension of the Hilbert space in a dual quantum mechanics. We show that in N=4 supersymmetric string theories, quantum entropy function formalism naturally explains the origin of the subtle differences between the microscopic degeneracies of quarter BPS dyons carrying different torsion, i.e. different arithmetical properties. These arise from additional saddle points in the path integral -- whose existence depends on the arithmetical properties of the black hole charges -- constructed as freely acting orbifolds of the original AdS_2\times S^2 near horizon geometry. During this analysis we demonstrate that the quantum entropy function is insensitive to the details of the infrared cutoff used in the computation, and the details of the boundary terms added to the action. We also discuss the role of the asymptotic symmetries of AdS_2 in carrying out the path integral in the definition of quantum entropy function. Finally we show that even though quantum entropy function is expected to compute the absolute degeneracy in a given charge and angular momentum sector, it can also be used to compute the index. This can then be compared with the microscopic computation of the index.
description: LaTeX file, 27 pages; v2: minor corrections
Additional file 1 of Association of dementia comorbidities with caregivers’ physical, psychological, social, and financial burden
Creators: name: Zhang, Jingyi
name: Wang, Jing
name: Liu, Hua
name: Wu, Chenkai
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Mental Health

description: Additional file 1: Supplementary Table S1. Weighted sample description by year interviewed (weighted N = 1,065). Supplementary Table S2. Fullregression results of associations between caregiving burden or gain and PWD’s comorbidities in the weighted sample. Supplementary Table S3. Latent class analysis model statistics. Supplementary Table S4. Caregiving burden scores by care recipient’s latent class groups.
Additional file 30 of Transcriptome profiling of barley in response to mineral and organic fertilizers
Creators: name: Esmaeilzadeh-Salestani, Keyvan
name: Tohidfar, Masoud
name: Ghanbari Moheb Seraj, Rahele
name: Khaleghdoust, Banafsheh
name: Keres, Indrek
name: Marawne, Hashem
name: Loit, Evelin
Publisher: name: figshare
Year: 2023
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 30: Table S1. List of DEGs involved in the important KEGG pathways under different treatments.
(47171) 1999 TC36, A Transneptunian Triple
Creators: name: Benecchi, S. D.
name: Noll, K. S.
name: Grundy, W. M.
name: Levison, H. F.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We present new analysis of HST images of (47171) 1999 TC36 that confirm it as a triple system. Fits to the point-spread function consistently show that the apparent primary is itself composed of two similar-sized components. The two central components, A1 and A2, can be consistently identified in each of nine epochs spread over seven years of time. In each instance the component separation, ranging from 0.023+/-0.002 to 0.031+/-0.003 arcsec, is roughly one half of the Hubble Space Telescope's diffraction limit at 606 nm. The orbit of the central pair has a semi-major axis of a~867 km with a period of P~1.9 days. These orbital parameters yield a system mass that is consistent with Msys = 12.75+/-0.06 10^18 kg derived from the orbit of the more distant secondary, component B. The diameters of the three components are dA1= 286(+45,-38) km, dA2= 265(+41,-35 km and dB= 139(+22,-18) km. The relative sizes of these components are more similar than in any other known multiple in the solar system. Taken together, the diameters and system mass yield a bulk density of p=542(+317,-211) kg m^-3. HST Photometry shows that component B is variable with an amplitude of >=0.17+/-0.05 magnitudes. Components A1 and A2 do not show variability larger than 0.08+/-0.03 magnitudes approximately consistent with the orientation of the mutual orbit plane and tidally-distorted equilibrium shapes. The system has high specific angular momentum of J/J'=0.93, comparable to most of the known Transneptunian binaries.
description: 16 pages, 8 figures, 6 tables. Accepted to Icarus
An Architectural View Type for Elasticity Modeling and Simulation -- The Slingshot Approach
Creators: name: Klinaku, Floriment
name: Stieß, Sarah Sophie
name: Hakamian, Alireza
name: Becker, Steffen
Publisher: name: arXiv
Year: 2025
Subjects: subject: Software Engineering (cs.SE)
subject: FOS: Computer and information sciences

description: The cloud computing model enables the on-demand provisioning of computing resources, reducing manual management, increasing efficiency, and improving environmental impact. Software architects now play a strategic role in designing and deploying elasticity policies for automated resource management. However, creating policies that meet performance and cost objectives is complex. Existing approaches, often relying on formal models like Queueing Theory, require advanced skills and lack specific methods for representing elasticity within architectural models. This paper introduces an architectural view type for modeling and simulating elasticity, supported by the Scaling Policy Definition (SPD) modeling language, a visual notation, and precise simulation semantics. The view type is integrated into the Palladio ecosystem, providing both conceptual and tool-based support. We evaluate the approach through two single-case experiments and a user study. In the first experiment, simulations of elasticity policies demonstrate sufficient accuracy when compared to load tests, showing the utility of simulations for evaluating elasticity. The second experiment confirms feasibility for larger applications, though with increased simulation times. The user study shows that participants completed 90% of tasks, rated the usability at 71%, and achieved an average score of 76% in nearly half the allocated time. However, the empirical evidence suggests that modeling with this architectural view requires more time than modeling control flow, resource environments, or usage profiles, despite its benefits for elasticity policy design and evaluation.
description: Accepted to JSS Special Issue Quality in Software Architecture
Vortex splitting and phase separating instabilities of coreless vortices in F=1 spinor Bose-Einstein condensates
Creators: name: Takahashi, M.
name: Pietila, V.
name: Mottonen, M.
name: Mizushima, T.
name: Machida, K.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: The low lying excitations of coreless vortex states in F = 1 spinor Bose-Einstein condensates (BECs) are theoretically investigated using the Gross-Pitaevskii and Bogoliubov-de Gennes equations. The spectra of the elementary excitations are calculated for different spin-spin interaction parameters and ratios of the number of particles in each sublevel. There exist dynamical instabilities of the vortex state which are suppressed by ferromagnetic interactions, and conversely, enhanced by antiferromagnetic interactions. In both of the spin-spin interaction regimes, we find vortex splitting instabilities in analogy with scalar BECs. In addition, a phase separating instability is found in the antiferromagnetic regime.
description: 11 pages, 9 figures
title: Ð¡ÐµÑÐ¸ Ð­ÐÐ Ð¸ ÑÐµÐ»ÐµÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸. ÐÐ¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÑÐµÐ¹ ÑÐ²ÑÐ·Ð¸ Ñ ÐºÐ¾Ð¼Ð¼ÑÑÐ°ÑÐ¸ÐµÐ¹ Ð¿Ð°ÐºÐµÑÐ¾Ð². Network Simulator (Ð¡ÐµÑÐµÐ²Ð¾Ð¹ ÑÐ¸Ð¼ÑÐ»ÑÑÐ¾Ñ ns2)
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°Ð±Ð¾ÑÐ¾Ð²ÑÐºÐ¸Ð¹, ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ Ð¡ÐÐ±ÐÐ¢Ð£
Year: 2002
Subjects: ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÐµÑÐ¸

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ ÐÐÐ Ð¤ 10 "Ð¡ÐµÑÐ¸ Ð­ÐÐ Ð¸ ÑÐµÐ»ÐµÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸" Ð¸ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Ð¡ÐÐ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ 552813 "Ð¡ÐµÑÐ¸ Ð­ÐÐ Ð¸ ÑÐµÐ»ÐµÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸" Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ° Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 552800 "ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ° Ð¸ Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ ÑÐµÑÐ½Ð¸ÐºÐ°". ÐÐ°Ð½Ð¾ ÐºÑÐ°ÑÐºÐ¾Ðµ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ ÑÐµÑÐµÐ²Ð¾Ð³Ð¾ ÑÐ¸Ð¼ÑÐ»ÑÑÐ¾ÑÐ° ns2 (Network Simulator, Ð²ÐµÑÑÐ¸Ñ 2) - Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð¹ ÑÐ¾Ð±ÑÑÐ¸Ð¹Ð½Ð¾Ð¹ Ð¼Ð¾Ð´ÐµÐ»Ð¸, ÑÐ¸ÑÐ¾ÐºÐ¾ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼Ð¾Ð¹ Ð´Ð»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÑÐµÐ¹ Ñ ÐºÐ¾Ð¼Ð¼ÑÑÐ°ÑÐ¸ÐµÐ¹ Ð¿Ð°ÐºÐµÑÐ¾Ð². ÐÐ·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ñ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¸Ð¼Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¼Ð¾Ð´ÐµÐ»ÐµÐ¹ Ð´Ð»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð² ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½ÑÑ ÑÐµÑÑÑ Ð½Ð° ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÑÐ¾Ð²Ð½ÑÑ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ðº ÑÐ¸ÐºÐ»Ñ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ ÐÐÐ  ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½ÑÐµ Ð½Ð° ÐºÐ°ÑÐµÐ´ÑÐµ ÑÐµÐ»ÐµÐ¼Ð°ÑÐ¸ÐºÐ¸ Ð¡ÐÐ±ÐÐ¢Ð£. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÑÐ°ÑÑÐ¸Ñ ÐºÑÑÑÐ¾Ð² ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ "ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ° Ð¸ Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ ÑÐµÑÐ½Ð¸ÐºÐ°", "Ð¡ÐµÑÐ¸ Ð­ÐÐ Ð¸ ÑÐµÐ»ÐµÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸", Ð° ÑÐ°ÐºÐ¶Ðµ Ð´Ð»Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð², Ð¸Ð½ÑÐµÑÐµÑÑÑÑÐ¸ÑÑÑ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐ¼Ð¸ Ð¼ÐµÑÐ¾Ð´Ð°Ð¼Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÑÐµÐ¹ ÑÐ²ÑÐ·Ð¸ Ñ ÐºÐ¾Ð¼Ð¼ÑÑÐ°ÑÐ¸ÐµÐ¹ Ð¿Ð°ÐºÐµÑÐ¾Ð².
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Diffuse molecular gas at high redshift: Detection of CO molecules and the 2175 Å dust feature at z=1.64
Creators: name: Noterdaeme, P.
name: Ledoux, C.
name: Srianand, R.
name: Petitjean, P.
name: Lopez, S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present the detection of carbon monoxide molecules (CO) at z=1.6408 towards the quasar SDSSJ160457.50+220300.5 using the VLT Ultraviolet and Visual Echelle Spectrograph. CO absorption is detected in at least two components in the first six A-X bands and one d-X(5-0) inter-band system. This is the second detection of this kind along a quasar line of sight. The CO absorption profiles are well modelled assuming a rotational excitation of CO in the range 6
description: 6 pages, 4 figures, 2 tables, accepted for publication in A&A
title: Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑ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ÑÐµÐ¼ÑÐµÐ², ÐÐ»ÐµÐºÑÐµÐ¹
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·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½
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description: Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÐ½ÐºÐ°, ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹, ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¹ Ð¸ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÐ¹ Ð¿Ð»Ð°Ð½ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð¾ÑÐµÐ½ÐµÐ½Ð° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð·Ð°.
Development and implementation of model reference adaptive hierarchical control framework for shake table tests
Creators: name: Chen, Zhongwei
Publisher: name: University of British Columbia
Year: 2024

description: The structural response under earthquake excitation can be simulated by shake table tests. However, the performance of the shake table is affected by the Control-Structure Interaction (CSI) effect. In recent years, nonlinear control algorithms were developed to compensate for the CSI effect. In this study, a model reference adaptive control algorithm, named model reference adaptive hierarchical control (MRAHC) framework, is presented. MRAHC consists of a high (adaptive) and low (loop-shaping) level controller. The high-level controller develops the control algorithm on the system level, which directedly considers the inherent nonlinearity of the test specimen and the CSI effect. While the low-level controller develops the control algorithm to regulate the hydraulic system and make sure it can follow the reference signal generated by the high-level controller. MRAHC offers many advantages including the ability to handle the CSI effect and the structural nonlinearity. In addition, it allows users to quantify the structural properties such as mass, stiffness, and damping. To evaluate the performance of the MRAHC method, shake table tests of a multi-degree of freedom system with different masses were carried out. The performance of the MRAHC was compared with the direct loop-shaping control method (LC) and the traditional Proportional-Integral-Differentiation (PID) control method. The results show that the MRAHC can achieve better acceleration tracking compared to the LC and PID control methods. Especially, when the shake table has CSI effect and structural nonlinearity. Hence, the MRAHC can be used as an effective nonlinear controller for shake table tests.
Titan's Prolific Propane: The Cassini CIRS Perspective
Creators: name: Nixon, C. A.
name: Jennings, D. E.
name: Flaud, J. -M.
name: Bezard, B.
name: Teanby, N. A.
name: Irwin, P. G. J.
name: Ansty, T. M.
name: Coustenis, A.
name: Vinatier, S.
name: Flasar, F. M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: In this paper we select large spectral averages of data from the Cassini Composite Infrared Spectrometer (CIRS) obtained in limb-viewing mode at low latitudes (30S--30N), greatly increasing the path length and hence signal-to-noise ratio for optically thin trace species such as propane. By modeling and subtracting the emissions of other gas species, we demonstrate that at least six infrared bands of propane are detected by CIRS, including two not previously identified in Titan spectra. Using a new line list for the range 1300-1400cm -1, along with an existing GEISA list, we retrieve propane abundances from two bands at 748 and 1376 cm-1. At 748 cm-1 we retrieve 4.2 +/- 0.5 x 10(-7) (1-sigma error) at 2 mbar, in good agreement with previous studies, although lack of hotbands in the present spectral atlas remains a problem. We also determine 5.7 +/- 0.8 x 10(-7) at 2 mbar from the 1376 cm-1 band - a value that is probably affected by systematic errors including continuum gradients due to haze and also an imperfect model of the n6 band of ethane. This study clearly shows for the first time the ubiquity of propane's emission bands across the thermal infrared spectrum of Titan, and points to an urgent need for further laboratory spectroscopy work, both to provide the line positions and intensities needed to model these bands, and also to further characterize haze spectral opacity. The present lack of accurate modeling capability for propane is an impediment not only for the measurement of propane itself, but also for the search for the emissions of new molecules in many spectral regions.
description: 7 Figures, 3 Tables. Typeset in Latex with elsart.cls. In press for Planetary and Space Science
A simple mathematical proof of Boltzmann's equal a priori probability hypothesis
Creators: name: Evans, Denis J.
name: Searles, Debra J.
name: Williams, Stephen R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Using the Dissipation Theorem and a corollary of the Fluctuation Theorem, namely the Second Law Inequality, we give a first-principles derivation of Boltzmann's postulate of equal a priori probability in phase space for the microcanonical ensemble. We show that if the initial distribution differs from the uniform distribution over the energy hypersurface, then under very wide and commonly satisfied conditions, the initial distribution will relax to that uniform distribution. This result is somewhat analogous to the Boltzmann H-theorem but unlike that theorem, applies to dense fluids as well as dilute gases and also permits a nonmonotonic relaxation to equilibrium. We also prove that in ergodic systems the uniform (microcanonical) distribution is the only stationary, dissipationless distribution for the constant energy ensemble.
description: 12 pages
ENGLISH LITERATURE IN THE RENAISSANCE PERIOD
Creators: name: Tasheva, Nafisa
Publisher: name: Zenodo
Year: 2024

description: The Renaissance period, which spanned from the 14th to the 17th century, was a time of great cultural and intellectual revival in Europe. This era witnessed a significant shift in artistic and literary expression, and English literature was no exception. The impact of the Renaissance on English literature was profound, as it brought about a renewed interest in classical texts, a shift towards humanism, and a blossoming of creativity and innovation.
From kinetic theory to dissipative fluid dynamics
Creators: name: Betz, B.
name: Henkel, D.
name: Rischke, D. H.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We present the results of deriving the Israel-Stewart equations of relativistic dissipative fluid dynamics from kinetic theory via Grad's 14-moment expansion. Working consistently to second order in the Knudsen number, these equations contain several new terms which are absent in previous treatments.
description: 7 pages, proceedings of the Erice School on Nuclear Physics "Heavy Ion collisions from the Coulomb Barrier up to the Quark Gluon Plasma", Erice, Sicily, Sep. 16 - 24, 2008
The Role of Planet Accretion in Creating the Next Generation of Red Giant Rapid Rotators
Creators: name: Carlberg, Joleen K.
name: Majewski, Steven R.
name: Arras, Phil
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Rapid rotation in field red giant stars is a relatively rare but well-studied phenomenon; here we investigate the potential role of planet accretion in spinning up these stars. Using Zahn's theory of tidal friction and stellar evolution models, we compute the decay of a planet's orbit into its evolving host star and the resulting transfer of angular momentum into the stellar convective envelope. This experiment assesses the frequency of planet ingestion and rapid rotation on the red giant branch (RGB) for a sample of 99 known exoplanet host stars. We find that the known exoplanets are indeed capable of creating rapid rotators; however, the expected fraction due to planet ingestion is only ~10% of the total seen in surveys of present-day red giants. Of the planets ingested, we find that those with smaller initial semimajor axes are more likely to create rapid rotators because these planets are accreted when the stellar moment of inertia is smallest. We also find that many planets may be ingested prior to the RGB phase, contrary to the expectation that accretion would generally occur when the stellar radii expand significantly as giants. Finally, our models suggest that the rapid rotation signal from ingested planets is most likely to be seen on the lower RGB, which is also where alternative mechanisms for spin-up, e.g., angular momentum dredged up from the stellar core, do not operate. Thus, rapid rotators on the lower RGB are the best candidates to search for definitive evidence of systems that have experienced planet accretion.
description: 12 pages, 12 figures, accepted for publication in The Astrophysical Journal
Comment on `Quantum resolution to the arrow of time dilemma'
Creators: name: Jennings, David
name: Rudolph, Terry
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Recently, a substantial amount of debate has grown up around a proposed quantum resolution to the `arrow of time dilemma' that is based on the role of classical memory records of entropy-decreasing events. In this note we show that the argument is incomplete and furthermore, by providing a counter-example, argue that it is incorrect. Instead of quantum mechanics providing a resolution in the manner suggested, it allows enhanced classical memory records of entropy-decreasing events.
description: 4 pages, no figures. Comments welcome
title: The effect of instrumentation technique on the outcome of treatment for periodontitis
Creators: name: Paterson, Michael
Publisher: name: University of Glasgow
Year: 2021
Subjects: subject: hand instruments, periodontal treatment, randomized controlled trial, clinical outcomes, patient reported outcomes, systemic inflammation, ultrasonic instruments, combination approach.

description: Objective: This study sought to investigate clinical, systemic inflammatory and patient-reported outcomes comparing non-surgical treatment for periodontal disease using exclusively hand instruments, ultrasonic instruments or a combination approach. Cost implications of periodontal treatment within a UK NHS Dental Hospital are described. Methods: Fifty-five patients were treated between two studies (randomised controlled trial and cohort study) for generalised periodontitis using non-surgical periodontal therapy using hand instruments (HI), ultrasonic instruments (UI) or a combination approach (CI) with a 90 day follow up. Comparative analysis was carried out with respect to instrumentation technique at day 90. Success of treatment was objectively assessed against published criteria. Financial implications and patient reported outcomes of non-surgical periodontal therapy are explored by descriptive analyses. Results: Non-surgical periodontal treatment was clinically effective across all instrumentation approaches at Day 90 follow up (p<0.05). Inter-group comparisons demonstrated no clinically significant differences in clinical or systemic inflammatory outcomes. UI required less time to complete treatment compared to HI, mean difference 21.51 minutes (p<0.003; 95% CI 9.22 to 34.62) Objective criteria of success demonstrated a lack of agreement in defining successful clinical endpoints. UI had least associated reprocessing and maintenance costs. Conclusions: Clinical and systemic inflammatory outcomes were comparable between HI, UI and CI. Comparing HI and UI, UI had a shorter treatment time. UI was least costly on a recurring basis. Patients reported satisfaction with periodontal treatment.
Additional file 7 of Extracellular vesicles derived from EphB2-overexpressing bone marrow mesenchymal stem cells ameliorate DSS-induced colitis by modulating immune balance
Creators: name: Yu, Ting
name: Chu, Si
name: Liu, Xingxing
name: Li, Junyi
name: Chen, Qianyun
name: Xu, Meng
name: Wu, Hui
name: Li, Mingyue
name: Dong, Yalan
name: Zhu, Feng
name: Zhou, Haifeng
name: Hu, Desheng
name: Fan, Heng
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer

description: Additional file 7: Table S2. Sequences of primers for qRT-PCR analysis.
Implementation of a non-deterministic optical noiseless amplifier
Creators: name: Ferreyrol, Franck
name: Barbieri, Marco
name: Blandino, Remi
name: Fossier, Simon
name: Tualle-Brouri, Rosa
name: Grangier, Philippe
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Quantum mechanics imposes that any amplifier that works independently on the phase of the input signal has to introduce some excess noise. The impossibility of such a noiseless amplifier is rooted into unitarity and linearity of quantum evolution. A possible way to circumvent this limitation is to interrupt such evolution via a measurement, providing a random outcome able to herald a successful - and noiseless - amplification event. Here we show a successful realisation of such an approach; we perform a full characterization of an amplified coherent state using quantum homodyne tomography, and observe a strong heralded amplification, with about 6dB gain and a noise level significantly smaller than the minimal allowed for any ordinary phase-independent device.
Spin-orbit excitations of quantum wells
Creators: name: Ambrosetti, A.
name: Escartin, J. M
name: Lipparini, E.
name: Pederiva, F.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Confinement asymmetry effects on the photoabsorption of a quantum well are discussed by means of a sum-rules approach using a Hamiltonian including a Rashba spin-orbt coupling. We show that while the strength of the excitation is zero when the spin-orbit coupling is neglected, the inclusion of the spin-orbit interaction gives rise to a non zero strength and mean excitation energy in the far-infrared region. A simple expression for these quantities up to the second order in the Rashba parameter was derived. The effect of two-body Coulomb interaction is then studied by means of a Quantum Monte Carlo calculation, showing that electron-electron correlations induce only a small deviation from the independent particle model result.
title: ÐÐ¸Ð·ÐºÐ¾Ð½Ð°Ð¿Ð¾ÑÐ½ÑÐ¹ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð¾-ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð³Ð¸Ð´ÑÐ¾ÑÐ·ÐµÐ» Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð®Ð³Ð° Ð Ð¾ÑÑÐ¸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·Ð½ÑÐº, ÐÑÑÐµÐ¼
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: Ð½Ð¸Ð·ÐºÐ¾Ð½Ð°Ð¿Ð¾ÑÐ½ÑÐ¹ Ð³Ð¸Ð´ÑÐ¾ÑÐ·ÐµÐ»
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description: ÐÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ°, Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð½Ð°Ñ Ð¿Ð¾Ð´ ÑÑÐºÐ¾Ð²Ð¾Ð´ÑÑÐ²Ð¾Ð¼ Ð¿ÑÐ¾ÑÐµÑÑÐ¾ÑÐ° ÐºÐ°ÑÐµÐ´ÑÑ ÐÐ¸ÐÐ¡, Ð´.Ñ.Ð½. Ð.Ð. ÐÑÑÐ°ÑÑÐµÐ²Ð°, ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÑ Ð½Ð¸Ð·ÐºÐ¾Ð½Ð°Ð¿Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð³Ð¸Ð´ÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð³Ð¸Ð´ÑÐ¾ÑÐ·Ð»Ð° Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð®Ð³Ð° Ð Ð¾ÑÑÐ¸Ð¸. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÐÐÐ  Ð±ÑÐ» Ð·Ð°Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½ Ð½Ð¸Ð·ÐºÐ¾Ð½Ð°Ð¿Ð¾ÑÐ½ÑÐ¹ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð¾-ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð³Ð¸Ð´ÑÐ¾ÑÐ·ÐµÐ» Ð½Ð° Ð½ÐµÑÐºÐ°Ð»ÑÐ½Ð¾Ð¼ Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸, ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÐ¹ Ð½Ð° Ð®Ð³Ðµ Ð Ð¾ÑÑÐ¸Ð¸. Ð ÑÐ¾ÑÑÐ°Ð² Ð³Ð¸Ð´ÑÐ¾ÑÐ·Ð»Ð° Ð²ÑÐ¾Ð´ÑÑ Ð³ÑÑÐ½ÑÐ¾Ð²Ð°Ñ Ð¸ Ð±ÐµÑÐ¾Ð½Ð½Ð°Ñ Ð¿Ð»Ð¾ÑÐ¸Ð½Ñ, Ð·Ð´Ð°Ð½Ð¸Ðµ ÐÐ­Ð¡ Ð¸ ÑÐ»ÑÐ·. ÐÐ¾ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð·Ð½Ð°ÑÐ¸Ð¼Ð¾ÑÑÐ¸ Ð¸ Ð¾ÑÐ²ÐµÑÑÑÐ²ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ñ ÑÑÑÑÐ¾Ð¼ Ð¿Ð¾ÑÐ»ÐµÐ´ÑÑÐ²Ð¸Ð¹ ÑÐ°Ð·ÑÑÑÐµÐ½Ð¸Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð³Ð¸Ð´ÑÐ¾ÑÐ·Ð»Ð° Ð¾ÑÐ½ÐµÑÐµÐ½Ñ Ðº I ÐºÐ»Ð°ÑÑÑ. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¿ÑÐ¸ÑÐ¾Ð´Ð½ÑÐµ ÑÑÐ»Ð¾Ð²Ð¸Ñ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð°, Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ñ ÐºÐ¾Ð¼Ð¿Ð¾Ð½Ð¾Ð²Ð¾ÑÐ½Ð¾Ðµ Ð¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½Ð¾Ðµ ÑÐµÑÐµÐ½Ð¸Ñ, Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ñ ÑÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¸ Ð³Ð¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÑÐµÑÑ Ð¿Ð¾ Ð²Ð¾Ð´Ð¾ÑÐ»Ð¸Ð²Ð½Ð¾Ð¹ Ð¿Ð»Ð¾ÑÐ¸Ð½Ðµ, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð°.
title: Integration of monoterpenoids with low pressure simulating vacuum for control of diapausing Indian meal moth larvae and red flour beetle adults
Creators: name: Mbata, G.
name: Pascual-Villalobos, M. J.
Publisher: name: Julius Kühn-Institut
Year: 2010
Subjects: subject: low pressure
subject: DL-camphor
subject: estragole
subject: γ-terpinene
subject: carvone

description: Julius-Kühn-Archiv; 425; 402-406
The Relationship Between Self-Reported Hearing Measures and Group Exercise Participation
Creators: name: Rahme, Mohamed
name: Folkeard, Paula
name: Belfry, Shannon
name: Orange, J.B.
name: Scollie, Susan
Publisher: name: The Health & Fitness Journal of Canada
Year: 2022

description: Background: Hearing loss and physical inactivity among adults are well documented, but the relationship between functional hearing ability and successful communication at group exercise is not well-understood. Purpose: The purpose of the study was to investigate adults’ functional hearing ability in group exercise environments and to analyze the role of hearing accessibility on the ability to hear and communicate during group exercise classes. The study aimed to learn about the relationship between hearing accessibility (e.g., self-reported hearing loss, hearing aid use and room acoustics) and the ability to hear and communicate during group exercise classes. Methods: Participation in the study included the completion of an online survey titled Physical Activity and Communication Evaluation (P.A.C.E.). The inclusion criteria for this study were: (1) age of 18 years or older; (2) self-reported history of participation in group exercise classes; and (3) ability to complete the survey in English. Multiple stepwise linear regression was completed to describe the relationship between self-reported hearing measures and group exercise participation with age and severity of self-reported hearing loss (summed across ears) as predictors and the ability to hear and understand conversations at group exercise classes as dependent variables. Results: A total of 110 participants (age range 21-83 years) completed the online survey with 32 participants self-reporting hearing loss in at least one ear, with 10 of them using hearing aids during exercise participation. Self-reported hearing loss severity significantly affected the following variables: participants’ ability to hear other participants when more than one conversation was occurring at the same time (p=0.002), understand the spoken instructions without looking at the instructor (p<0.001), and understand the spoken instructions when the instructor was speaking to the group in quiet listening conditions (p<0.001). Conclusions: The results indicated that self-reported hearing loss affected the ability to hear and understand conversations at group exercise classes.
description: The Health & Fitness Journal of Canada, Vol. 15 No. 3 (2022)
title: Ð¤Ð¸Ð·Ð¸ÐºÐ° Ð¼Ð°ÐºÑÐ¾Ð¼Ð¾Ð»ÐµÐºÑÐ»
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÑÑÐ¸Ñ ÑÑÐµÐ±Ð½ÑÑ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹, Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ñ ÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² Â«Ð¢ÐµÑ Ð½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°Â»
titleType: Subtitle
Creators: name: ÐÐ°Ð¿ÑÐ°Ð»Ð¾Ð²Ð°, ÐÐ¸ÐºÑÐ¾ÑÐ¸Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2012
Subjects: ÐÐ°ÐºÑÐ¾Ð¼Ð¾Ð»ÐµÐºÑÐ»Ñ
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The Ly-alpha profile and center-to-limb variation of the quiet Sun
Creators: name: Curdt, W.
name: Tian, H.
name: Teriaca, L.
name: Schuehle, U.
name: Lemaire, P.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study the emission of the hydrogen Lyman-a line in the quiet Sun, its center-to-limb variation (CLV), and its radiance distribution. We also compare quasi-simultaneous Ly-a and Ly-b line profiles. We used the high spectral and spatial resolution of the SUMER spectrometer and completed raster scans at various locations along the disk. For the first time, we used a method to reduce the incoming photon flux to a 20%-level by partly closing the aperture door. We also performed a quasi-simultaneous observation of both Ly-a and Ly-b at Sun center in sit-and-stare mode. We infer the flow characteristic in the Ly-a map from variations in the calibrated 1206 Si III line centroids. We present the average profile of Ly-a, its radiance distribution, its CLV behaviour, and the signature of flows on the line profiles. Little CLV and no limb brightening are observed in the profiles of the Ly-a line. In contrast to all other lines of the Lyman series, which have a stronger red-horn, Ly-a has a dominating blue-horn asymmetry. There appears to be a brightness-to-asymmetry relationship. A similar and even clearer trend is observed in the downflow-to-asymmetry relationship. This important result is consistent with predictions from models that include flows. However, the absence of a clear CLV in the profiles may be more indicative of an isotropic field than a radial flow. It appears that the ubiquitous hydrogen behaves similar to a filter that dampens all signatures of the line formation by processes in the chromosphere and transition region.
description: 4 pages, 4 figures