cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Stemonitis splendens Rostaf.
Creators: name: Kluša, Julita
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Protozoa
Mycetozoa
Myxomycetes
Stemonitidales
Stemonitidaceae
Stemonitis
Stemonitis splendens

description: ● Stemonitis splendens Rostaf.,
spīgainā vālenīte (šokolādes gļotsēne)
- leg. M.Šlapakova-Pjankova, 06 Mar 2023, Rēzekne, on an old deciduous trunk, det. J.Kluša, conf. E.Johannesen, 2023; (NMKK), one locality.
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
Reply to "What Faster-than-traffic Characteristic Speeds Mean for Vehicular Traffic Flow"
Creators: name: Helbing, Dirk
Publisher: name: arXiv
Year: 2009
Subjects: subject: Physics and Society (physics.soc-ph)
subject: FOS: Physical sciences

description: This contribution replies to H. M. Zhang's paper "What Faster-than-traffic Characteristic Speeds Mean for Vehicular Traffic Flow", which comments on the manuscript "On the Controversy around Daganzo's Requiem for and Aw-Rascle's Resurrection of Second-Order Traffic Flow Models" published in this issue of Eurpean Physical Journal B. The author clarifies several points and agrees that suitable experiments can be a way of deciding the controversy on the existence of propagation speeds faster than the speed of vehicles. Moreover, he proposes to aim at an integrated theory, which is both, theoretically consistent and practically relevant.
description: For related work see http://www.helbing.org
Additional file 4 of Should migraine without aura be further divided? A study of 1444 female patients with migraine without aura
Creators: name: Wang, Xiaolin
name: Na, Weinan
name: Yang, Ying
name: Zhang, Wenwen
name: Zhao, Junxia
name: Zhang, Tingting
name: Zhou, Yuanji
name: Liu, Hua
name: Zhao, Dong
name: Yu, Shengyuan
Publisher: name: figshare
Year: 2023
Subjects: subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 4.
The origin of the X-ray emitting plasma in the eastern edge of the Cygnus Loop
Creators: name: Zhou, Xin.
name: Bocchino, Fabrizio.
name: Miceli, Marco.
name: Orlando, Salvatore.
name: Chen, Yang.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The Cygnus Loop is interacting with a protrusion of the cavity wall in its eastern edge (the XA region), where the X-ray emission is very bright. The complexity of the environment and the non-linear physical processes of the shock-cloud interaction make the origin of the X-ray emission still not well understood. Our purpose is to understand the physical origin of the X-ray emission in the XA region, addressing, in particular, the role of thermal conduction in the interaction process. We analyzed two XMM-Newton data sets, performing image analysis and spatially resolved spectral analysis on a set of homogeneous regions. We applied a recently developed diagnostic tool to compare spectral analysis results with predictions of theoretical models, and to estimate the efficiency of thermal conduction on the X-ray emitting shocked plasma. We found that the inhomogeneous cavity wall contains both large clumps (the protrusion) and small isolated clumps with different densities. A large indentation bent over to the south is detected. The abundance of the surrounding ISM is ~0.2 times solar value. We confirmed the important role of thermal conduction in the evolution of X-ray emitting plasma during shock-cloud interaction.
description: 7 pages, 5 figures, MNRAS in press
title: Ð£ÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾Ðµ ESG ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½ÑÑ ÑÐºÐ¾ÑÐ¸ÑÑÐµÐ¼
title: Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ñ
titleType: Subtitle
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name: ÐÐ°Ð±ÐºÐ¸Ð½, ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
name: ÐÐ¾Ð»ÑÑÐ½Ð¾Ð²ÑÐºÐ°Ñ, ÐÐ°ÑÐ¸Ð½Ð°
name: ÐÑÐ·Ð¸Ð½Ð¾Ð², Ð .
name: ÐÐ°Ð±ÐºÐ¸Ð½, ÐÐ²Ð°Ð½
name: ÐÐ°ÑÐ¸Ð»ÑÐµÐ², Ð .
name: ÐÐ»ÑÑÐ¾Ð², ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
name: ÐÐ¸Ð±ÑÐ¾Ð², Ð.
name: ÐÐ»ÑÐ¸Ð½ÑÐºÐ°Ñ, Ð.
name: ÐÐ¾Ð²ÑÐ¾Ð², Ð.
name: ÐÐ¾Ð¿ÑÑÐµÐ½ÐºÐ¾Ð²Ð°, Ð.
name: ÐÐµÐ²Ð°Ð½ÑÑÐº, Ð.
name: ÐÐ¾Ð³Ð¸Ð½Ð¾Ð², Ð.
name: ÐÑÑÐ°Ð³Ð¸Ð½, Ð.
name: ÐÑÑÐ°Ð³Ð¸Ð½, Ð.
name: ÐÐ°Ð»ÐµÐ²ÑÐºÐ°Ñ-ÐÐ°Ð»ÐµÐ²Ð¸Ñ, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
name: ÐÐ°ÑÑÐ½Ð¸Ð½, Ð®.
name: ÐÐ¾Ð²Ð¸ÐºÐ¾Ð²Ð°, Ð®.
name: ÐÐ¾Ð½Ð¾Ð¼Ð°ÑÐµÐ²Ð°, Ð.
name: Ð¡Ð°Ð´ÑÐ¸ÐµÐ², Ð.
name: Ð¡Ð°Ð¼Ð¾ÑÐ²Ð°Ð»Ð¾Ð², ÐÐ²Ð°Ð½
name: Ð¡ÑÐ¿ÐµÑÐµÐºÐ¸Ð½, Ð.
name: Ð¢ÐµÐ¿Ð»Ð¸ÑÐºÐ¸Ð¹, Ð.
name: Ð¢Ð¸ÑÐ¾Ð²Ð°, Ð.
name: Ð¢Ð¸ÑÐ¾Ð²Ð°, Ð.
name: Ð¢Ð¸ÑÐ¾Ð½Ð¾Ð²Ð°, Ð.
name: Ð¤ÐµÐ´Ð¾ÑÐ¾Ð², Ð.
name: Ð®ÑÑÐ¿Ð¾Ð²Ð°, Ð.
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2023
Subjects: ÑÐ¸ÑÑÐ¾Ð²Ð°Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸

description: Ð Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ð¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹, Ð¾ÑÑÐ°Ð¶Ð°ÑÑÐ¸Ðµ Ð½Ð°ÑÑÐ½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ð¸ ESG ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½ÑÑ ÑÐºÐ¾ÑÐ¸ÑÑÐµÐ¼ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð½Ð¾Ð²Ð¾Ð¹ ÑÐµÐ°Ð»ÑÐ½Ð¾ÑÑÐ¸, Ð¾Ð±ÑÑÐ»Ð¾Ð²Ð»ÐµÐ½Ð½ÑÑ ÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼ Ð½Ð¾Ð²Ð¾Ð³Ð¾ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾ÑÑÐ´ÐºÐ°, Ð¿ÑÐ¾ÑÐµÑÑÐ°Ð¼Ð¸ Ð³Ð»Ð¾Ð±Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ ÑÐ¸ÑÑÐ¾Ð²Ð¸Ð·Ð°ÑÐ¸Ð¸. Ð Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ð¸ Ð½Ð°ÑÐ»Ð¸ Ð¾ÑÑÐ°Ð¶ÐµÐ½Ð¸Ðµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½Ð¾Ð¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð½Ð¾Ð²Ð¾Ð³Ð¾ Ð¼Ð¸ÑÐ¾Ð¿Ð¾ÑÑÐ´ÐºÐ°, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ð¸ ÑÐ¸ÑÐºÑÐ»ÑÑÐ½Ð¾Ð¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ESG ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ, ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²ÑÐ¼ ESG ÑÐ°Ð·Ð²Ð¸ÑÐ¸ÐµÐ¼ ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ Ð¸ Ð¾ÑÑÐ°ÑÐ»ÐµÐ²ÑÑ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ¾Ð² Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð´Ð»Ñ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ESG Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð². ÐÐ¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ñ Ð¾ÑÑÐ°Ð¶Ð°ÐµÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð°Ð²ÑÐ¾ÑÐ¾Ð². ÐÐ°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ð¸ Ð±ÑÐ´ÑÑ Ð¿Ð¾Ð»ÐµÐ·Ð½Ñ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÑÐ¼, Ð½Ð°ÑÑÐ½ÑÐ¼ ÑÐ°Ð±Ð¾ÑÐ½Ð¸ÐºÐ°Ð¼, ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ°Ð¼ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹, Ð½Ð°ÑÑÐ½ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¹ Ð¸ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸Ð¹, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð¸ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ°Ð¼. ÐÐ°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ð¸ ÑÐ°Ð·Ð¼ÐµÑÐµÐ½Ñ Ð² Ð±Ð°Ð·Ðµ Ð´Ð°Ð½Ð½ÑÑ Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð³Ð¾ Ð¸Ð½Ð´ÐµÐºÑÐ° Ð½Ð°ÑÑÐ½Ð¾Ð³Ð¾ ÑÐ¸ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð° Ð¿Ð»Ð°ÑÑÐ¾ÑÐ¼Ðµ Elibrary.ru.
The Bolocam Galactic Plane Survey -- II. Catalog of the Image Data
Creators: name: Rosolowsky, Erik
name: Dunham, Miranda K.
name: Ginsburg, Adam
name: Bradley, Eric Todd
name: Aguirre, James
name: Bally, John
name: Battersby, Cara
name: Cyganowski, Claudia
name: Dowell, Darren
name: Drosback, Meredith
name: Evans, Neal J.
name: Glenn, Jason
name: Harvey, Paul
name: Stringfellow, Guy S.
name: Walawender, Josh
name: Williams, Jonathan P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a catalog of 8358 sources extracted from images produced by the Bolocam Galactic Plane Survey (BGPS). The BGPS is a survey of the millimeter dust continuum emission from the northern Galactic plane. The catalog sources are extracted using a custom algorithm, Bolocat, which was designed specifically to identify and characterize objects in the large-area maps generated from the Bolocam instrument. The catalog products are designed to facilitate follow-up observations of these relatively unstudied objects. The catalog is 98% complete from 0.4 Jy to 60 Jy over all object sizes for which the survey is sensitive (<3.5'). We find that the sources extracted can best be described as molecular clumps -- large dense regions in molecular clouds linked to cluster formation. We find the flux density distribution of sources follows a power law with dN/dS ~S^(-2.4 +/- 0.1) and that the mean Galactic latitude for sources is significantly below the midplane: =(-0.095 +/- 0.001) deg.
description: Accepted by ApJS. Data release and full resolution manuscript at http://irsa.ipac.caltech.edu/data/BOLOCAM_GPS/
Exact dynamical exchange-correlation kernel of a weakly inhomogeneous electron gas
Creators: name: Nazarov, V. U.
name: Vignale, G.
name: Chang, Y. -C.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The dynamical exchange-correlation kernel $f_{xc}$ of a non-uniform electron gas is an essential input for the time-dependent density functional theory of electronic systems. The long-wavelength behavior of this kernel is known to be of the form $f_{xc}= α/q^2$ where $q$ is the wave vector and $α$ is a frequency-dependent coefficient. We show that in the limit of weak non-uniformity the coefficient $α$ has a simple and exact expression in terms of the ground-state density and the frequency-dependent kernel of a {\it uniform} electron gas at the average density. We present an approximate evaluation of this expression for Si and discuss its implications for the theory of excitonic effects.
description: 5 pages, 2 figures
Additional file 1 of Molecular detection and genotyping of bovine viral diarrhea virus in Western China
Creators: name: Chang, Lingling
name: Qi, Yanping
name: Liu, Dan
name: Du, Qian
name: Zhao, Xiaomin
name: Tong, Dewen
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology
subject: Computational Biology

description: Additional file 1.
title: Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¾Ð±Ð¾ÑÐ¾ÑÐ½ÑÐ¼ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð¾Ð¼ Ð¸ Ð¿ÑÑÐ¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÐµÐ³Ð¾ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð° ÑÑÐ¾Ð²Ð½Ðµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð°Ð¿Ð¾Ð³Ð¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´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: 2017
Subjects: ÐºÐ°Ð¿Ð¸ÑÐ°Ð»
Ð¾Ð±Ð¾ÑÐ¾ÑÐ½ÑÐ¹ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»
Ð¾Ð±Ð¾ÑÐ¾ÑÐ½ÑÐµ Ð°ÐºÑÐ¸Ð²Ñ
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description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«Ð Ð°ÑÑÂ». Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾Ð±Ð¾ÑÐ¾ÑÐ½ÑÐ¼ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð¾Ð¼. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð° Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ¸, ÑÑÑÑÐºÑÑÑÑ Ð¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¾Ð±Ð¾ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð° ÐÐÐ Â«Ð Ð°ÑÑÂ». Ð ÑÐµÐ»ÑÑ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾Ð±Ð¾ÑÐ¾ÑÐ½ÑÐ¼ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð¾Ð¼ Ð² ÐÐÐ Â«Ð Ð°ÑÑÂ» Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¾ Ð²ÑÑÐ²Ð¸ÑÑ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ°, Ð¾Ð¿ÑÐµÐ´ÐµÐ»Ð¸ÑÑ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÐ¹ ÑÑÐ¾Ð²ÐµÐ½Ñ Ð·Ð°Ð¿Ð°ÑÐ¾Ð², Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°ÑÑ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÑÑ, Ð¾Ð¿ÑÐµÐ´ÐµÐ»Ð¸ÑÑ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÐ¹ ÑÑÐ¾Ð²ÐµÐ½Ñ Ð´ÐµÐ½ÐµÐ¶Ð½ÑÑ ÑÑÐµÐ´ÑÑÐ² Ð¸ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÐ½ÐµÐ¶Ð½ÑÐ¼Ð¸ ÑÑÐµÐ´ÑÑÐ²Ð°Ð¼Ð¸. ÐÐ½ÐµÐ´ÑÐµÐ½Ð¸Ðµ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾Ð±Ð¾ÑÐ¾ÑÐ½ÑÐ¼Ð¸ Ð°ÐºÑÐ¸Ð²Ð°Ð¼Ð¸ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ñ ÑÐ¾ÐºÑÐ°ÑÐ¸ÑÑ Ð½ÐµÐ¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð½ÑÐµ ÑÐ°ÑÑÐ¾Ð´Ñ, ÑÐ°Ð·Ð¼ÐµÑ Ð±ÐµÐ·Ð½Ð°Ð´ÐµÐ¶Ð½ÑÑ Ð´Ð¾Ð»Ð³Ð¾Ð², Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ñ ÑÐ±Ð°Ð»Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾ÑÑÑ Ð¸ ÑÐ¸Ð½ÑÑÐ¾Ð½Ð½Ð¾ÑÑÑ Ð´ÐµÐ½ÐµÐ¶Ð½ÑÑ Ð¿Ð¾ÑÐ¾ÐºÐ¾Ð².
title: An Investigation of Postzygotic Reproductive Isolation and Phenotypic Divergence in the Bark Beetle Dendroctonus Ponderosae
Creators: name: Bracewell, Ryan R.
Publisher: name: Utah State University
Year: 2009

description: Understanding reproductive isolation and divergence is the focus of speciation research. Recent evidence suggested that some Dendroctonus ponderosae populations produced hybrids with reproductive incompatibilities, a reproductive boundary undetected by phylogeographic analyses using molecular markers. Additionally, the unique bifurcated distribution of D. ponderosae and the proposed isolation-by-distance gene flow pattern around the Great Basin Desert provided a unique opportunity to investigate the evolution of postmating (postyzygotic) isolation while also understanding phenotypic divergence along latitudinal (climatic) gradients. First, I characterized the strength, biological pattern, and geographic pattern of postzygotic isolation in D. ponderosae by crossing increasingly divergent populations in a common garden environment. There was little evidence of hybrid inviability in these crosses, yet geographically distant crosses produced sterile males, consistent with expectations under Haldane's rule. Hybrid male sterility appeared at a threshold among increasingly divergent populations, was bidirectional (reciprocal crosses were affected), and less geographically distant crosses did not show significant gender-specific decreases in fitness. Second, a separate investigation of two critical phenotypic traits (body size and development time) was conducted on intrapopulation F2 generation offspring from a common garden experiment. Genetic differences contributing to phenotypic variance were interpreted within the context of the previously described reproductive incompatibilities, gene flow patterns, and latitudinal gradients. Genetic differences in development time were striking between faster developing and more synchronized northern populations and slower developing, less synchronized southern populations. Differences in development time were not detected between populations at similar latitudes. Body size, although more variable than developmental time, generally conformed to expectations, with northern populations being smaller than southern populations. Average adult size was found to be quite different between many populations and did vary between populations at similar latitudes, yet relative sexual size dimorphism was rather consistent. There was no evidence of correspondence between phenotypic traits (body size and development time) and either reproductive boundaries or gene flow patterns. The results suggest that latitudinally imposed climatic differences are likely driving phenotypic divergence between populations.
Nonlinear Schrodinger equation with chaotic, random, and nonperiodic nonlinearity
Creators: name: Cardoso, W. B.
name: Leao, S. A.
name: Avelar, A. T.
name: Bazeia, D.
name: Hussein, M. S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: In this paper we deal with a nonlinear Schrödinger equation with chaotic, random, and nonperiodic cubic nonlinearity. Our goal is to study the soliton evolution, with the strength of the nonlinearity perturbed in the space and time coordinates and to check its robustness under these conditions. Comparing with a real system, the perturbation can be related to, e.g., impurities in crystalline structures, or coupling to a thermal reservoir which, on the average, enhances the nonlinearity. We also discuss the relevance of such random perturbations to the dynamics of Bose-Einstein Condensates and their collective excitations and transport.
description: 4 pages, 6 figures
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐ¾ÑÐµÐ´ÑÑÑ Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð°ÑÐ´Ð¸ÑÐ° Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ ÐºÐ°Ð´ÑÐ¾Ð²Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐ¾Ð¼Ð¸ÑÐµÑÐ° Ð¿Ð¾ ÑÐ°ÑÐ¸ÑÐ°Ð¼ Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°)
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð¨Ð°Ð²ÐµÑÐ¾Ð²Ð°, Ð¯Ð½Ð°
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: ÐºÐ°Ð´ÑÐ¾Ð²Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ°
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description: Ð Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ Ðº Ð¿Ð¾Ð½ÑÑÐ¸Ñ ÐºÐ°Ð´ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð°ÑÐ´Ð¸ÑÐ° Ð¸ Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð°ÑÐ´Ð¸ÑÐ° Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ ÐºÐ°Ð´ÑÐ¾Ð²Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¼ÐµÑÐ¾Ð´Ñ Ð¸ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð°ÑÐ´Ð¸ÑÐ° Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ ÐºÐ°Ð´ÑÐ¾Ð²Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼ÑÐµ Ð¸ÑÐ¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¼Ð¸ Ð¾ÑÐ³Ð°Ð½Ð°Ð¼Ð¸ Ð²Ð»Ð°ÑÑÐ¸ Ð² Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ðµ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÑÐµÐ´ÑÑÑ Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð°ÑÐ´Ð¸ÑÐ° Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ ÐºÐ°Ð´ÑÐ¾Ð²Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð² ÑÐ°Ð±Ð¾ÑÑ Ð¸ÑÐ¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¾Ð² Ð²Ð»Ð°ÑÑÐ¸ Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°.
title: Factors Affecting the Longevity of the Department of Industrial Technology and Education at Utah State University 1985-2005: A Case Study
Creators: name: Cloward, Jerry
Publisher: name: Utah State University
Year: 2009

description: A qualitative case study method was used to discover the factors involved with the longevity of the Technology Education program at Utah State University. The problem was that while there were studies reporting the many Technology Education programs that have been closed there had been no studies on individual programs that have remained open. This study also contains a consolidation of relative information on the program. The primary data was obtained from interviews with the professors involved with the program during the timeframe of the study. The data obtained from the interviews was evaluated and set into themes. The factors were derived from the themes. The many factors presented in this study are evidence of the need to do this holistic study of the problem. The findings from this study provide a basis for study of other successful Technology Education programs.
Emerging bioenergy technologies : convergence and divergence of scientific literature and perspectives on X (Twitter)
Creators: name: Elnur, Rawie Ibrahim
Publisher: name: University of British Columbia
Year: 2024

description: This thesis explores two emerging technologies in the bioenergy space: Bioenergy with Carbon Capture and Storage (BECCS) and Sustainable Aviation Fuel (SAF). BECCS involves converting biomass into energy while capturing and permanently storing carbon dioxide emissions, positioning it as a negative emissions technology essential for meeting the Paris Climate Agreement's targets. SAF, derived from biomass like agricultural and forestry residues, helps reduce emissions from aviation, addressing the sector's significant contribution to global carbon emissions. Public perception, heavily influenced by social media discourse, plays a pivotal role in shaping policy support and legitimizing these technologies. Conclusions on the sustainability of bioenergy as a renewable resource depend heavily on contextual temporal-scale and spatial-scale factors, often overlooked in social media discussions. Tweets frequently make blanket statements on carbon neutrality and sustainability without sufficient context, revealing biases in online discourse. Conversely, researchers and industry stakeholders often underplay or negate the social and environmental consequences of the increasing demand for biofuel production, which threaten biodiversity and the livelihoods of rural and marginalized communities worldwide. The research objectives are to explore how these technologies are framed, compare levels of optimism and skepticism across platforms, and outline differences in discourse between BECCS and SAF despite their reliance on similar feedstocks. An automated content analysis of historical Twitter posts (n=11,314) and peer-reviewed academic articles (n=140) provides insights into these dynamics. The findings and research aim to provide insights into how scientific communication is disseminated from academia to social media, uncovering underreported knowledge gaps amidst the increasing demand for biofuel production, and to assess variations in optimism and skepticism across different technologies and media.
Planetesimals to Protoplanets II: Effect of Debris on Terrestrial Planet Formation
Creators: name: Leinhardt, Z. M.
name: Richardson, D. C.
name: Lufkin, G.
name: Haseltine, J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: In this paper we extend our numerical method for simulating terrestrial planet formation from Leinhardt and Richardson (2005) to include dynamical friction from the unresolved debris component. In the previous work we implemented a rubble pile planetesimal collision model into direct N-body simulations of terrestrial planet formation. The new collision model treated both accretion and erosion of planetesimals but did not include dynamical friction from debris particles smaller than the resolution limit for the simulation. By extending our numerical model to include dynamical friction from the unresolved debris, we can simulate the dynamical effect of debris produced during collisions and can also investigate the effect of initial debris mass on terrestrial planet formation. We find that significant initial debris mass, 10% or more of the total disk mass, changes the mode of planetesimal growth. Specifically, planetesimals in this situation do not go through a runaway growth phase. Instead they grow concurrently, similar to oligarchic growth. In addition to including the dynamical friction from the unresolved debris, we have implemented particle tracking as a proxy for monitoring compositional mixing. Although there is much less mixing due to collisions and gravitational scattering when dynamical friction of the background debris is included, there is significant inward migration of the largest protoplanets in the most extreme initial conditions.
description: 13 pages, 16 figures, 1 table, accepted for publication in MNRAS abstract shortened
Additional file 2 of Molecular detection and genotyping of bovine viral diarrhea virus in Western China
Creators: name: Chang, Lingling
name: Qi, Yanping
name: Liu, Dan
name: Du, Qian
name: Zhao, Xiaomin
name: Tong, Dewen
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology
subject: Computational Biology

description: Additional file 2.
title: ÐÐµÑÑÐ¾Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð²ÐµÐ±-Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÐº Python
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð¢Ð¸ÑÐ¾Ð½Ð¾Ð²Ð°, 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Ð¸ÑÐ¾Ð½ (Python)
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Old Main Sequence Turnoff Photometry in the Small Magellanic Cloud. II. Star Formation History and Its Spatial Gradients
Creators: name: Noel, Noelia E. D.
name: Aparicio, Antonio
name: Gallart, Carme
name: Hidalgo, Sebastian L.
name: Costa, Edgardo
name: Mendez, Rene A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a quantitative analysis of the SFH of 12 fields in the SMC. We find that there are four main periods of enhancement of star formation: a young one peaked at around 0.2-0.5 Gyr old, only present in the eastern and in the central-most fields; two at intermediate ages present in all fields (a conspicuous one peaked at 4-5 Gyr old, and a less significant one peaked at 1.5-2.5); and an old one, peaked at 10 Gyr in all fields but the western ones. In the western fields, this old enhancement splits into two, one peaked at around 8 Gyr old and another at around 12 Gyr old. This "two-enhancement" zone seems to be a robust feature since it is unaffected by our choice of stellar evolutionary library but more data covering other fields of the SMC are necessary in order to ascertain its significancy. Some correlation could exist with encounters taken from the orbit determination of Kallivayalil et al. (2006). But our results would be also fit in a first pericenter passage scenario like the one claimed by Besla et al. (2007). There is a strong dichotomy between East/Southeast and West in the current irregular shape of the SMC. We find that this dichotomy is produced by the youngest population and began about 1 Gyr ago or later. We do not find yet a region dominated by an old halo at 4.5 kpc from the SMC center, indicating either that this old stellar halo does not exist in the SMC or that its contribution to the stellar populations, at the galactocentric distances of our outermost field, is negligible. We derive the age-metallicity relation and find that the metallicity increased continuously from early epochs until now.
description: Accepted for publication in AJ, 39 pages, 13 Postscript figures. High resolution available at: http://www.iac.es/galeria/noelia/PaperII_Figures/index.html or via email to: noelia@roe.ac.uk
Magnetic field detection in the B2Vn star HR 7355
Creators: name: Rivinius, Th.
name: Szeifert, Th.
name: Barrera, L.
name: Townsend, R. H. D.
name: Stefl, S.
name: Baade, D.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The B2Vn star HR 7355 is found to be a He-rich magnetic star. Spectropolarimetric data were obtained with FORS1 at UT2 on Paranal observatory to measure the disk-averaged longitudinal magnetic field at various phases of the presumed 0.52 d cycle. A variable magnetic field with strengths between B_z = -2200 and +3200G was found, with confidence limits of 100 to 130G. The field topology is that of an oblique dipole, while the star itself is seen about equator-on. In the intensity spectra the HeI-lines show the typical equivalent width variability of He-strong stars, usually attributed to surface abundance spots. The amplitudes of the equivalent width variability of the HeI lines are extraordinarily strong compared to other cases. These results not only put HR 7355 unambiguously among the early-type magnetic stars, but confirm its outstanding nature: With v sin i = 320 km/s the parameter space in which He-strong stars are known to exist has doubled in terms of rotational velocity.
description: 6 pages, 5 figures, 1 Table. Accepted for publication in MNRAS Letters
title: Measurement and Modeling of Reduced-Gravity Fluid Distribution and Transport in Unsaturated Porous Plant-Growth Media
Creators: name: Heinse, Robert
Publisher: name: Utah State University
Year: 2009

description: The effect of reduced gravity on the balanced management of liquid, gaseous and ionic fluxes in unsaturated porous media remains a central challenge for plant-based bio-regenerative life support systems needed for long-duration space missions. This research investigated how shifting capillary and gravitational forces alter the sample-scale transport and distribution of fluids in mm-sized porous ceramic aggregates. Measurements in variably saturated media conducted on the International Space Station in microgravity ($sim1cdot10^{-3} g_{earth}$) and measurements during parabolic flight in variable gravity encompassing microgravity, terrestrial gravity and hypergravity ($sim1.8 g_{earth}$) were supported by numerical modeling based on fundamental, earth-derived soil-physical relationships. Measurements of water fluxes in rigid saturated media suggested Darcian flow unaffected by gravity. Observations of hydraulic potential and sample water content were used to estimate the primary draining and wetting water-retention characteristic (WRC). Terrestrial parameterizations of the WRC were largely unaffected by reduced gravity. However, because the WRC is hysteretic, heterogenous water-content distributions resulted within the confines of the primary draining and wetting characteristics. Ensuing distributions were fundamentally different from terrestrial observations and were stable in the absence of a significant gravity gradient. We showed that these distributions, though unexpected, could be predicted using the Richards equation. One consequence of altered water distribution could be the reduction in, and increased tortuosity of, continuous gas-filled pathways for diffusive transport compared to terrestrial estimates. Measurements of oxygen diffusion in microgravity suggested reduced diffusivities during draining. These observations, particularly for the smaller particle-sized media, were suggestive of the delayed formation of critical air-filled pathways at lower water contents. This dissertation further uses a case history of a stratified root-zone developed based on water-retention characteristics of different particle-sized media. The root-zone design provided a more uniform water-content distribution at terrestrial gravity suggested to provide more optimal conditions for root growth. Additionally, the design and testing of a novel integrated sensor for measurements of water content based on the dissipation of heat and estimation of nutrient status based on electrical resistivity are discussed. These results should provide insights into microgravity fluid distribution and transport contributing to the design and implementation of controllable plant-growth systems for use in microgravity and future planetary habitats.
title: Ð Ð°ÑÑÐµÑ ÑÑÑÐ°Ð½Ð¾Ð²Ð¸Ð²ÑÐ¸Ñ ÑÑ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð², ÑÐ¾ÐºÐ¾Ð² ÐºÐ¾ÑÐ¾ÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð¼ÑÐºÐ°Ð½Ð¸Ñ Ð¸ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ð² ÑÐ»Ð¾Ð¶Ð½Ð¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ðµ 500/330 ÐºÐ
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°ÑÐ´Ð¾, ÐÐ»ÐµÐºÑÐ°Ð½Ð´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Ð»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ¸ÑÑÐµÐ¼Ð°
ÑÑÑÐ°Ð½Ð¾Ð²Ð¸Ð²ÑÐ¸Ð¹ÑÑ ÑÐµÐ¶Ð¸Ð¼ ÑÐ°Ð±Ð¾ÑÑ
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description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð²ÐºÐ»ÑÑÐ°ÐµÑ Ð² ÑÐµÐ±Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ ÑÐ°ÑÑÐµÑ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ 500/330 ÐºÐ. Ð¡Ð¸ÑÑÐµÐ¼Ð° ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð¸Ð· Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÐ¾Ð², ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾ÑÐ¾Ð², Ð»Ð¸Ð½Ð¸Ð¹ Ð¸ Ð½Ð°Ð³ÑÑÐ·Ð¾Ðº.
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title: Fundamentals of Mountain Resort Base Village Design: A Critical Review of Existing Resort Developments with Recommendations for Future Development Practices
Creators: name: Harding, Bryan P.
Publisher: name: Utah State University
Year: 2006

description: The North American ski industry has grown over the past century from a small, family-owned and -operated industry, to a multi-billion dollar industry dominated by corporate management organizations. The rise of corporate resort ownership has led to the trend of the construction base village developments at ski resorts around the country to attract guests, and therefore revenue, to their resorts. Though many base villages have been very successful in attracting skiers, examples of poor landscape architectural design practices abound in the industry. This study examines several design elements considered to be the "fundamental elements of designed space," applies these elements to base village design throughout the country, critically examines their implementation in built examples, and presents suggestions and recommendations for future mountain resort base village design practices.
Additional file 1 of Should migraine without aura be further divided? A study of 1444 female patients with migraine without aura
Creators: name: Wang, Xiaolin
name: Na, Weinan
name: Yang, Ying
name: Zhang, Wenwen
name: Zhao, Junxia
name: Zhang, Tingting
name: Zhou, Yuanji
name: Liu, Hua
name: Zhao, Dong
name: Yu, Shengyuan
Publisher: name: figshare
Year: 2023
Subjects: subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 1.
New supersymmetric AdS4 type II vacua
Creators: name: Lust, Dieter
name: Tsimpis, Dimitrios
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Building on our recent results on dynamic SU(3)xSU(3) structures we present a set of sufficient conditions for supersymmetric AdS4xM6 backgrounds of type IIA/IIB supergravity. These conditions ensure that the background solves, besides the supersymmetry equations, all the equations of motion of type II supergravity. The conditions state that the internal manifold is locally a codimension-one foliation such that the five dimensional leaves admit a Sasaki-Einstein structure. In type IIA the supersymmetry is N=2, and the total six-dimensional internal space is locally an S^2 bundle over a four-dimensional Kaehler-Einstein base; in IIB the internal space is the direct product of a circle and a five-dimensional squashed Sasaki-Einstein manifold. Given any five-dimensional Sasaki-Einstein manifold we construct the corresponding families of type IIA/IIB vacua. The precise profiles of all the fields are determined at the solution and depend on whether one is in IIA or in IIB. In particular the background does not contain any sources, all fluxes (including the Romans mass in IIA) are generally non-zero, and the dilaton and warp factor are non-constant.
description: 19 pages; clarifications added, version to appear in JHEP
Elucidating the Black Hole - Galaxy Connection
Creators: name: Walsh, Jonelle
Publisher: name: Zenodo
Year: 2021
Subjects: AGN and black holes

description: The local BH mass function is incomplete, and we do not know exactly what roles BHs play in galaxy evolution. We need robust MBH measurements at the ends of the BH mass scale and in a wider variety of galaxies that have grown in different ways. Recent progress has been made with AO on large ground-based telescopes, new wide-field highly sensitive IFUs, ALMA, and updates to the modeling methods. Future facilities in the era of the Nancy Grace Roman Space Telescope will open up new regimes. We can study the most massive BHs in the Universe, exploring the extreme end of BH evolution. We can probe the smallest BHs in the Universe, exploring the mass function of initial BH seeds. We can directly trace redshift evolution in the BH scaling relations over a meaningful baseline, exploring when/how BHs and galaxies grow.
Garden Club at Gardiner's Island by Mr. Morton Pennypacker, September 11, 1934
Creators: name: Pennypacker, Morton
Publisher: name: Garden Club of East Hampton
Year: 1934
Subjects: Gardening
Gardens
Social organizations
Organizations
East Hampton (N.Y.)

description: This paper titled, "Garden Club at Gardiner's Island", was written by Mr. Morton Pennypacker on September 11, 1934.
The Role of Angular Momentum and Cosmic Censorship in the (2+1)-Dimensional Rotating Shell Collapse
Creators: name: Mann, Robert B.
name: Oh, John J.
name: Park, Mu-In
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We study the gravitational collapse problem of rotating shells in three-dimensional Einstein gravity with and without a cosmological constant. Taking the exterior and interior metrics to be those of stationary metrics with asymptotically constant curvature, we solve the equations of motion for the shells from the Darmois-Israel junction conditions in the "co-rotating" frame. We study various collapse scenarios with "arbitrary" angular momentum for a variety of geometric configurations, including anti-de Sitter, de Sitter, and flat spaces. We find that the collapsing shells can form a BTZ black hole, a three-dimensional Kerr-dS spacetime, and an horizonless geometry of point masses under certain initial conditions. For pressureless dust shells, the curvature singularity is "not" formed due to the angular momentum barrier near the origin. However when the shell pressure is nonvanishing, we find that for all types of shells with polytropic-type equations of state (including the perfect fluid and the generalized Chaplygin gas), collapse to a naked singularity is "possible" under generic initial conditions. We conclude that in three dimensions angular momentum does not in general guard against violation of cosmic censorship.
description: Added Comments on a caveat of three dimensions and the critical behavior (p.26); Added References; Accepted in PRD
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title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
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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: ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¸Ñ
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Ð¼Ð°Ð»ÑÐ¹ Ð¸ ÑÑÐµÐ´Ð½Ð¸Ð¹ Ð±Ð¸Ð·Ð½ÐµÑ
Ð±Ð°Ð½ÐºÐ¸

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title: The Effect of an Ambient Olfactory Intervention on Time-on-Task and Performance During Participant Interaction with an Electronic Flashcard System
Creators: name: Loewer, Aaron J.
Publisher: name: Utah State University
Year: 2009

description: The purpose of this study was to measure the influence of an ambient peppermint aroma on participants' time-on-task and performance while using FACTOR, an open-source e-Learning application. I proposed time-on-task was moderating between olfactory stimulation and performance. A 2x2 research design measured interaction of group (nonscented, scented) and gender of participants (N = 65). The learning content consisted of 28 African countries. Two methods for measuring time-on-task were employed: participant self-report at six learning intervals, and second, video recordings captured by, and stored on each participant's computer. Independent samples t tests were used to measure group and gender differences in time-on-task and performance. Relationships between time-on-task and performance were assessed using bivariate correlation and were reported as r values. Time-on-task differences between groups were not significant but garnered ES =.53. After 24 minutes of learning time, control females spent more time-on-task than control males (ES =.71), which was a statistically significant result. There was a weak to almost neutral correlation between time-on-task of all participants and performance (r =.1) where controls showed a weaker relationship (r =.05) than treatments (r =.26). The correlation between observed time-on-task and posttest performance was neutral for controls (r = .008) but moderate for treatments (r =.38). During the 40-minute learning session, the relationship between observed time-on-task and performance was r =.04 (females) and r =.55 (males), which was statistically significant. When examining time-on-task at the six measured intervals, the relationship with performance was strongest for treatments after 16 (r =.39) and 24 (r =.39) minutes of learning time. The direct influence of olfactory stimulation on performance was weak as the peppermint scent had a greater influence on time-on-task. Significant differences and notable effect sizes were not achieved by examining these variables. Analysis of the entire model showed the variables (condition, time-on-task, performance) were weakly correlated (r =.19) and that only 4% of the variance in the model was explained by its variables. As such, I failed to reject the null hypothesis, which was that time-on-task did not act as a moderator between condition and performance.