cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
EFFECTS OF ELECTIVE DELIVERY POLICY ON CLINICAL AND COST OUTCOMES
Creators: name: Wu, Su Yen
Publisher: name: Zenodo
Year: 2015

description: The United States is an increasingly attractive location for foreign mothers to deliver their babies. At one southern California medical center, many foreign mothers with late local third trimester prenatal care demanded early delivery (e.g., less than 39 weeks gestation). This led to increased numbers of infants admitted to the Neonatal Intensive Care Unit (NICU), reflecting potentially poor fetal outcomes and uncompensated costs for the facility. The hospital implemented a new elective delivery policy based on American Congress of Obstetricians and Gynecologists (AGOG) recommendations. During 2012, a team was formed to manage the processes, which included educational sessions and dissemination of the new policy to the medical and nursing staff. An evaluation that compared monthly numbers of scheduled early elective deliveries in 2011 to 2012 were compared to those from 2013 to 2014. Prior to the policy implementation, 277 elective delivery cases did not comply with ACOG recommendation standards (16% of all deliveries) compared to eight cases (0.4%) after policy implementation; 39 NICU admissions occurred prior to the implementation compared to three admissions afterwards. Uncompensated hospital costs dropped from $254, 546 pre-policy to $0 afterwards. These results indicate that the successful implementation of the policy promoted the safety and health of mothers and neonates, and decreased uncompensated costs for the hospital. Staff morale also increased due to pride in following ACOG recommendations and perceptions of enhanced neonatal safety.
Constructing Two-Dimensional Voronoi Diagrams via Divide-and-Conquer of Envelopes in Space
Creators: name: Setter, Ophir
Publisher: name: arXiv
Year: 2009
Subjects: subject: Computational Geometry (cs.CG)
subject: FOS: Computer and information sciences

description: We present a general framework for computing two-dimensional Voronoi diagrams of different classes of sites under various distance functions. The framework is sufficiently general to support diagrams embedded on a family of two-dimensional parametric surfaces in $R^3$. The computation of the diagrams is carried out through the construction of envelopes of surfaces in 3-space provided by CGAL (the Computational Geometry Algorithm Library). The construction of the envelopes follows a divide-and-conquer approach. A straightforward application of the divide-and-conquer approach for computing Voronoi diagrams yields algorithms that are inefficient in the worst case. We prove that through randomization the expected running time becomes near-optimal in the worst case. We show how to employ our framework to realize various types of Voronoi diagrams with different properties by providing implementations for a vast collection of commonly used Voronoi diagrams. We also show how to apply the new framework and other existing tools from CGAL to compute minimum-width annuli of sets of disks, which requires the computation of two Voronoi diagrams of two different types, and of the overlay of the two diagrams. We do not assume general position. Namely, we handle degenerate input, and produce exact results.
description: M.Sc. thesis. The work has been carried out at Tel-Aviv University under the supervision of Prof. Dan Halperin. 85 pages, 17 figures, 4 tables. For some reason the arXiv PDF version looks different than it should. PS is preferable
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸Ð·Ð¸ÐºÐ¾-Ð¼ÐµÑ Ð°Ð½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð¶Ð¸Ð´ÐºÐ¾ÑÑÐµÐºÐ¾Ð»ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ¼Ð¾Ð²Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¼ÐµÑÐ¸ Ð´Ð»Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¾ÑÐ¼Ð¾Ð²Ð¾ÑÐ½Ð¾Ð¹ Ð»Ð¸Ð½Ð¸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¡Ð°Ð±Ð°Ð½Ð¸Ð½ , ÐÐ°ÐºÑÐ¸Ð¼
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: ÑÐ¾ÑÐ¼Ð¾Ð²Ð¾ÑÐ½Ð°Ñ ÑÐ¼ÐµÑÑ
ÑÐ³Ð»ÐµÐºÐ¸ÑÐ»ÑÐ¹ Ð³Ð°Ð·
Ð¶Ð¸Ð´ÐºÐ¾Ðµ ÑÑÐµÐºÐ»Ð¾
Ð³Ð°Ð·Ð¾Ð¿ÑÐ¾Ð½Ð¸ÑÐ°ÐµÐ¼Ð¾ÑÑÑ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð»Ð¸ÑÐµÐ¹Ð½ÑÑ ÑÐ¾ÑÐ¼ Ð¸Ð· Ð¶Ð¸Ð´ÐºÐ¾ÑÑÐµÐºÐ¾Ð»ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ¼Ð¾Ð²Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¼ÐµÑÐ¸, Ð¾ÑÐ²ÐµÑÐ¶Ð´Ð°ÐµÐ¼Ð¾Ð¹ Ð¿ÑÐ¾Ð´ÑÐ²ÐºÐ¾Ð¹ Ð¡Ð2 Ð¸ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð½Ð¾Ð¹ Ðº Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð° Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¾ÑÐ¼Ð¾Ð²Ð¾ÑÐ½Ð¾Ð¹ Ð»Ð¸Ð½Ð¸Ð¸ Ð¿ÑÐ¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ðµ Ð±Ð¸Ð¼ÐµÑÐ°Ð»Ð»Ð¸ÑÐµÑÐºÐ¸Ñ Ð¾ÑÐ»Ð¸Ð²Ð¾Ðº..Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¼ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ°Ð¼ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð»Ð¸ÑÐµÐ¹Ð½ÑÑ ÑÐ¾ÑÐ¼ Ð¸Ð· Ð¶Ð¸Ð´ÐºÐ¾ÑÑÐµÐºÐ¾Ð»ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ¼Ð¾Ð²Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¼ÐµÑÐ¸, Ð¾ÑÐ²ÐµÑÐ¶Ð´Ð°ÐµÐ¼Ð¾Ð¹ Ð¿ÑÐ¾Ð´ÑÐ²ÐºÐ¾Ð¹ Ð¡Ð2, Ñ ÑÑÐµÑÐ¾Ð¼ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸Ðº Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¿ÑÐµÐ´ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð¼ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð»Ð¸ÑÐµÐ¹Ð½Ð¾Ð³Ð¾ ÑÐµÑÐ° Ð¿Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ñ Ð±Ð¸Ð¼ÐµÑÐ°Ð»Ð»Ð¸ÑÐµÑÐºÐ¸Ñ Ð¾ÑÐ»Ð¸Ð²Ð¾Ðº.ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð»Ð¾ÑÑ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ Ð¶Ð¸Ð´ÐºÐ¾Ð³Ð¾ ÑÑÐµÐºÐ»Ð° Ð² ÑÐ¾ÑÐ¼Ð¾Ð²Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¼ÐµÑÐ¸, Ð²ÑÐµÐ¼ÐµÐ½Ð¸ Ð¿ÑÐ¾Ð´ÑÐ²ÐºÐ¸, Ð²ÑÐµÐ¼ÐµÐ½Ð¸ Ð²ÑÐ´ÐµÑÐ¶ÐºÐ¸ Ð¿Ð¾ÑÐ»Ðµ Ð¿ÑÐ¾Ð´ÑÐ²ÐºÐ¸, ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÑ Ð¸ Ð´Ð»Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÑÑÐºÐ¸ Ð¾Ð±ÑÐ°Ð·ÑÐ¾Ð² Ð¿Ð¾ÑÐ»Ðµ Ð¾ÐºÑÐ°ÑÐºÐ¸ Ð½Ð° Ð¿ÑÐµÐ´ÐµÐ» Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÐ¸ Ð½Ð° ÑÐ°Ð·ÑÑÐ² Ð¸ Ð³Ð°Ð·Ð¾Ð¿ÑÐ¾Ð½Ð¸ÑÐ°ÐµÐ¼Ð¾ÑÑÑ ÑÐ¼ÐµÑÐ¸ Ð² ÑÑÑÐ¾Ð¼ (Ð¾ÑÐ²ÐµÑÐ¶Ð´ÐµÐ½Ð½Ð¾Ð¼) ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ð¸; Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð²ÑÐµÐ¼ÐµÐ½Ð¸ Ð²ÑÐ´ÐµÑÐ¶ÐºÐ¸ Ð¾ÑÐ»Ð¸Ð²ÐºÐ¸ Ð² ÑÐ¾ÑÐ¼Ðµ Ð½Ð° Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÑ ÑÐ¾ÑÐ¼Ð¾Ð²Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¼ÐµÑÐ¸; Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ ÑÑÐ»Ð¾Ð²Ð¸Ð¹ Ð·Ð°Ð»Ð¸Ð²ÐºÐ¸ Ð¼ÐµÑÐ°Ð»Ð»Ð° Ð½Ð° ÐºÐ°ÑÐµÑÑÐ²Ð¾ Ð»Ð¸ÑÐµÐ¹Ð½Ð¾Ð¹ ÑÐ¾ÑÐ¼Ñ. ÐÐ¾ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ°Ð¼ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¼Ð½Ð¾Ð³Ð¾ÑÐ°ÐºÑÐ¾ÑÐ½ÑÑ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ¾Ð² ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð½ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð². ÐÐ¾Ð»ÑÑÐµÐ½Ð½ÑÐµ Ð´Ð°Ð½Ð½ÑÐµ Ð¿Ð¾ Ð³ÑÐ°Ð½ÑÐ»Ð¾Ð¼ÐµÑÑÐ¸ÑÐµÑÐºÐ¾Ð¼Ñ Ð¸ ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¼Ñ ÑÐ¾ÑÑÐ°Ð²Ð°Ð¼ Ð¾ÑÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾Ð¹ ÑÐ¼ÐµÑÐ¸ Ð¼Ð¾Ð³ÑÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ñ Ð¿ÑÐ¸ ÑÐµÑÐµÐ½Ð¸Ð¸ Ð²Ð¾Ð¿ÑÐ¾ÑÐ¾Ð² Ð¾ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ ÐµÐµ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð² ÑÐ¼ÐµÐ¶Ð½ÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°Ñ.
RADIATIVE TRANSFER MODELING FOR QUANTIFYING LUNAR SURFACE MINERALS, PARTICLE SIZE AND SUBMICROSCOPIC IRON (SMFe)
Creators: name: Li, Shuai
Publisher: name: IUPUI University Library
Year: 2012
Subjects: subject: Lunar soils, Radiative transfer model, Newton method
subject: Moon -- Surface
subject: Soils
subject: Minerals

description: Indiana University-Purdue University Indianapolis (IUPUI)
description: The main objective of this work is to better quantify lunar surface minerals (agglutinate, clinopyroxene, orthopyroxene, plagioclase, olivine, ilmenite, and volcanic glass), particle sizes and the abundance of SMFe from the lunar soil characterization consortium (LSCC) dataset with our improved model based on Hapke's radiative transfer theory. The model is implemented for both forward and inverse modeling. Hapke's radiative transfer theory is implemented in the inverse model means Newton's method and least squares are jointly used to solve nonlinear questions rather than commonly used look-up Table (LUT). Although the effects of temperature and surface topography are incorporated into the implementation to improve the model performance for application of lunar spacecraft data, these effects cannot be extensively addressed in the current work because of the use of lab measured reflectance data. Our forward radiative transfer model (RTM) results show that the correlation coefficients between modeled and measured spectra are over 0.99. For the inverse model, the distribution of the calculated particle sizes is all within their measured range. The range of modeled SMFe for highland samples is 0.01% - 0.5 % and for mare samples is 0.03% - 1 %. The linear trend between SMFe and ferromagnetic resonance (Is) for all the LSCC samples is consistent with laboratory measurements. For quantifying lunar mineral abundances, the results show that the R-squared for the training samples (Is/FeO <= 65) are over 0.65 with plagioclase having highest correlation (0.94) and pyroxene the lowest (0.68). In the future work, the model needs to be improved for handling more mature lunar soil samples.
Additional file 1 of Endoscopic intraventricular hematoma evacuation surgery versus external ventricular drainage for the treatment of patients with moderate to severe intraventricular hemorrhage: a multicenter, randomized, controlled trial
Creators: name: Zhu, Junhao
name: Tang, Chao
name: Cong, Zixiang
name: Yang, Jin
name: Cai, Xiangming
name: Liu, Yuxiu
name: Ma, Chiyuan
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Science Policy

description: Additional file 1. SPIRIT 2013 Checklist: Recommended items to address in a clinical trial protocol and related documents.
Detection of the energetic pulsar PSR B1509-58 and its pulsar wind nebula in MSH 15-52 using the Fermi-Large Area Telescope
Creators: name: LAT Collaboration
name: Consortium, Pulsar Timing
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We report the detection of high energy gamma-ray emission from the young and energetic pulsar PSR B1509$-$58 and its pulsar wind nebula (PWN) in the composite supernova remnant SNR G320.4-1.2 (aka MSH 15-52). Using 1 year of survey data with the Fermi-Large Area Telescope (LAT), we detected pulsations from PSR B1509-58 up to 1 GeV and extended gamma-ray emission above 1 GeV spatially coincident with the PWN. The pulsar light curve presents two peaks offset from the radio peak by phases 0.96 $\pm$ 0.01 and 0.33 $\pm$ 0.02. New constraining upper limits on the pulsar emission are derived below 1 GeV and confirm a severe spectral break at a few tens of MeV. The nebular spectrum in the 1 - 100 GeV energy range is well described by a power-law with a spectral index of (1.57 $\pm$ 0.17 $\pm$ 0.13) and a flux above 1 GeV of (2.91 $\pm$ 0.79 $\pm$ 1.35) 10^{-9} cm^{-2} s^{-1}. The first errors represent the statistical errors on the fit parameters, while the second ones are the systematic uncertainties. The LAT spectrum of the nebula connects nicely with Cherenkov observations, and indicates a spectral break between GeV and TeV energies.
description: 14 pages, 6 figures, accepted for publication by ApJ
Constraining the energy budget of GRB 080721
Creators: name: Starling, R. L. C.
name: Rol, E.
name: van der Horst, A. J.
name: Yoon, S. -C.
name: Pal'shin, V.
name: Ledoux, C.
name: Page, K. L.
name: Fynbo, J. P. U.
name: Wiersema, K.
name: Tanvir, N. R.
name: Jakobsson, P.
name: Guidorzi, C.
name: Curran, P. A.
name: Levan, A. J.
name: O'Brien, P. T.
name: Osborne, J. P.
name: Svinkin, D.
name: Postigo, A. de Ugarte
name: Oosting, T.
name: Howarth, I. D.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We follow the bright, highly energetic afterglow of Swift-discovered GRB 080721 at z=2.591 out to 36 days or 3e6 s since the trigger in the optical and X-ray bands. We do not detect a break in the late-time light curve inferring a limit on the opening angle of theta_j >= 7.3 deg and setting tight constraints on the total energy budget of the burst of E_gamma >= 9.9e51 erg within the fireball model. To obey the fireball model closure relations the GRB jet must be expanding into a homogeneous surrounding medium and likely lies behind a significant column of dust. The energy constraint we derive can be used as observational input for models of the progenitors of long gamma-ray bursts: we discuss how such high collimation-corrected energies could be accommodated with certain parameters of the standard massive star core-collapse models. We can, however, most probably rule out a magnetar progenitor for this GRB which would require 100% efficiency to reach the observed total energy.
description: 11 pages, 6 figures (3 colour), accepted for publication in MNRAS following minor revision of Sections 4.2 and 5
The meaning of traditional small grains cultivation : generational wisdom, well-being, and food security
Creators: name: Ogura, Saori
Publisher: name: University of British Columbia
Year: 2024

description: Small grains cultivation historically contributed to humanity’s survival in different parts of the world, and has endured neglect as a viable crop in modern times, particularly as the emergence of modern industrial agricultural methods. While there has been reported decreased interest in small grains cultivation and a threat to the loss of traditional knowledge and the heirloom seeds, small grains cultivation has a key role in this time of uncertainty, given the small grains’ climate resilience, high nutritional value, and contribution to food security and food sovereignty. Using ethnography and an occupational perspective, this dissertation explores the meanings of small grains cultivation to older cultivators and younger community members in three communities in Japan. First, I use an integrative review method to understand what has been studied on traditional occupations and meaning in the existing occupational science literature. Second, I explore the meaning of small grains cultivation for 10 cultivators, to discover the reasons they continued the cultivation practice despite the laborious work and disdain by mainstream society. Third, I take a deep dive into exploring the meaning of small grains to a dedicated cultivator, presenting an individual case study that delineates how the traditional rotational farming contributes to maintaining biodiversity and forest restoration. Fourth, the meanings of small grains and related activities are explored for 10 younger community members whose involvement in small grains cultivation are transient, and outline important characteristics for how the traditional cultivation could be passed to younger generations. Fifth, using an arts-based method, I document the 20 community members’ responses to the documentary film that was created through interviews and participant observation of this study, allowing the research findings to return to the communities in an artistic, approachable format. This study supports the bridging of generational gaps and creates an unanticipated bond among the communities. This study highlights the important meanings neglected in this modern era and uncovers potential pathways to sustain the cultivation practice into the future, which would support land and community well-being. Importantly, this work provided a renewed sense of pride in community members’ engagement in the occupation of small grains cultivation.
The impact of glaciation and climate change on biogeochemical cycling and landscape development
Creators: name: Mabry, James Brice
Publisher: name: IUPUI University Library
Year: 2012
Subjects: subject: paleoclimatology, 8.2 ka event, younger dryas
subject: geochemistry, phosphorus, sediment, glacial lake
subject: Glacial lakes -- California
subject: Glacial lakes -- Illinois
subject: Climatic changes -- Environmental aspects
subject: Glacial climates
subject: Paleoclimatology

description: Indiana University-Purdue University Indianapolis (IUPUI)
description: Lake cores from Dry Lake, California and Crystal Lake, Illinois were analyzed to identify climate variability and characterize landscape response to glacial/deglacial climate transitions. Geochemical analysis of the Dry Lake sediment prior to the 8.2 kyr event revealed average values for percent total organic carbon to be 4% with a range of 0.2% to 15.2%. The average decreased to approximately 2.1% with a range of 0.4% to 5.3% during and after the event. Occluded phosphorus averaged 488 µg/g before the 8.2 kyr event and 547 µg/g after but was much lower during the event at 287 µg/g. These results were interpreted as an environment which began as warm, wet, and productive then quickly turned colder and drier during the 8.2 kyr event which resulted in a resetting of soil development. The higher temperatures returned after the 8.2 kyr event which allowed for continued soil development despite its drier climate. Previous research corroborated these conclusions. The Crystal Lake geochemical record was very different from Dry Lake. Percent total organic carbon averaged 6.7% with a range of 3.9% to 8.5% during the Younger Dryas but recorded a lower average before and after at 4.9% and 4.6% respectively. Occluded phosphorus acted similarly with a higher average during the cooling event, 2626 µg/g, and lower averages before and after, 1404 µg/g and 1461 µg/g, respectively. This was interpreted as continued productivity and soil development through the cold period which was attributed to a change in biomass.
title: Архитектура ЭВМ
Creators: name: ELS IPR BOOKS
Publisher: name: Профобразование
Year: 2025

description: В учебном пособии рассматриваются краткая история создания электронно-вычислительных машин, базовые элементы, представление информации, устройства ввода-вывода информации, терминалы, подсистема прерываний и т.д. В конце даны практические задания для изучения основных принципов построения ЭВМ. Учебное пособие предназначено для студентов, обучающихся по укрупненной группе специальностей среднего профессионального образования «Информатика и вычислительная техника», изучающих дисциплины «Архитектура аппаратных средств», «Архитектура электронно-вычислительных машин и вычислительные системы».
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«Ð ÐÐÂ»)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÐºÐ°ÑÐ¾Ð²Ð°, ÐÐµÑÐ¾Ð½Ð¸ÐºÐ°
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°Ð½Ð°Ð»Ð¸Ð·
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description: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¾ Ð½Ð° ÑÐ¸ÑÑÐµÐ¼Ð½Ð¾Ð¼ Ð¿Ð¾Ð´ÑÐ¾Ð´Ðµ, ÐºÐ°ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð¼ Ð²ÑÐ±Ð¾ÑÐµ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸. ÐÐ°Ð½Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð±ÑÐ´ÐµÑ ÑÐ¿Ð¾ÑÐ¾Ð±ÑÑÐ²Ð¾Ð²Ð°ÑÑ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ°Ð±Ð¾ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ¸ÑÑÐµÐ¼Ð½Ð¾Ð³Ð¾ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð²ÑÐµÑ Ð²Ð¸Ð´Ð¾Ð² ÐµÐµ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸.
title: ÐÐ¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÐÐ­Ð¢-ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð² Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ Ðº Ð»ÑÑÐµÐ²Ð¾Ð¼Ñ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸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¥Ð°ÑÑÐ°Ð±, Ð®ÑÑÐµÑ
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ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ðµ Ð¿ÑÐ¸Ð±Ð¾ÑÑ, Ð°Ð¿Ð¿Ð°ÑÐ°ÑÑ Ð¸ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ
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positron emission tomography
computed tomography
radiotherapy

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¼Ñ Ð±ÑÐ´ÐµÐ¼ Ð¸Ð·ÑÑÐ°ÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ ÐºÐ¾Ð¼Ð±Ð¸Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¼ÐµÐ¶Ð´Ñ ÐÐ¢ Ð¸ ÐÐ­Ð¢ Ð´Ð»Ñ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð»ÑÑÐµÐ²Ð¾Ð¹ ÑÐµÑÐ°Ð¿Ð¸Ð¸, Ð² Ð¿ÐµÑÐ²Ð¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð¼Ñ Ð±ÑÐ´ÐµÐ¼ Ð¸Ð·ÑÑÐ°ÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ°Ð´Ð¸Ð¾Ð½ÑÐºÐ»Ð¸Ð´Ð¾Ð² Ð² Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ñ Ð´Ð¸Ð°Ð³Ð½Ð¾ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ aÑÐ¿ÐµÐºÑÐ°Ñ Ð´Ð»Ñ Ð¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°, Ð²Ð¾ Ð²ÑÐ¾ÑÐ¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð¼Ñ Ð±ÑÐ´ÐµÐ¼ ÑÐ°ÐºÐ¶Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÑ Ð²ÑÐ±Ð¾Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ ÑÐ°Ð´Ð¸Ð¾Ð½ÑÐºÐ»Ð¸Ð´Ð½Ð¾Ð¹ Ð²Ð¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ñ ÑÐµÐ»ÑÑ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¿ÑÐµÐ´Ð²Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±Ð»ÑÑÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð»ÑÑÐµÐ²Ð¾Ð¹ ÑÐµÑÐ°Ð¿Ð¸Ð¸. Ð ÑÑÐµÑÑÐµÐ¹ Ð³Ð»Ð°Ð²Ðµ Ð¼Ñ Ð±ÑÐ´ÐµÐ¼ Ð¸Ð·ÑÑÐ°ÑÑ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ðµ ÑÑÐ¾ÑÐ´ÐµÐ·Ð¾ÐºÑÐ¸Ð³Ð»ÑÐºÐ¾Ð·Ñ Ð½Ð° ÑÑÐºÐ¾ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ð¼ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐµ. Ð¸ Ð² Ð¿Ð¾ÑÐ»ÐµÐ´Ð½ÐµÐ¹ Ð³Ð»Ð°Ð²Ðµ Ð¼Ñ Ð¾Ð±ÑÐµÐ´Ð¸Ð½Ð¸Ð¼ ÐÐ¢ Ð¸ ÐÐ­Ð¢ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ¸ÑÑÐµÐ¼Ñ Fusion Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°ÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°Ñ.
description: In this paper we will explore the possibility of combining between CT and PET for improved radiation therapy planning, in the first chapter, we will explore the use of radionuclides in medical diagnostic and technical aspects for their production. In the second chapter, we will also study The choice of radionuclide imaging technology for the preparation of pre-exposure to radiation therapy. In the third chapter, we will study Getting fluorodeoxyglucose from complex and accelerator, in the last chapter we combine CT and PET using Fusion system and analyze the results.
Multi-Element Abundance Measurements from Medium-Resolution Spectra. I. The Sculptor Dwarf Spheroidal Galaxy
Creators: name: Kirby, Evan N.
name: Guhathakurta, Puragra
name: Bolte, Michael
name: Sneden, Christopher
name: Geha, Marla C.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present measurements of Fe, Mg, Si, Ca, and Ti abundances for 388 radial velocity member stars in the Sculptor dwarf spheroidal galaxy (dSph), a satellite of the Milky Way. This is the largest sample of individual alpha element (Mg, Si, Ca, Ti) abundance measurements in any single dSph. The measurements are made from Keck/DEIMOS medium-resolution spectra (6400-9000 A, R ~ 6500). Based on comparisons to published high-resolution (R >~ 20000) spectroscopic measurements, our measurements have uncertainties of sigma([Fe/H]) = 0.14 and sigma([alpha/Fe]) = 0.13. The Sculptor [Fe/H] distribution has a mean = -1.58 and is asymmetric with a long, metal-poor tail, indicative of a history of extended star formation. Sculptor has a larger fraction of stars with [Fe/H] < -2 than the Milky Way halo. We have discovered one star with [Fe/H] = -3.80 +/- 0.28, which is the most metal-poor star known anywhere except the Milky Way halo, but high-resolution spectroscopy is needed to measure this star's detailed abundances. As has been previously reported based on high-resolution spectroscopy, [alpha/Fe] in Sculptor falls as [Fe/H] increases. The metal-rich stars ([Fe/H] ~ -1.5) have lower [alpha/Fe] than Galactic halo field stars of comparable metallicity. This indicates that star formation proceeded more gradually in Sculptor than in the Galactic halo. We also observe radial abundance gradients of -0.030 +/- 0.003 dex per arcmin in [Fe/H] and +0.013 +/- 0.003 dex per arcmin in [alpha/Fe] out to 11 arcmin (275 pc). Together, these measurements cast Sculptor and possibly other surviving dSphs as representative of the dwarf galaxies from which the metal-poor tail of the Galactic halo formed.
description: Accepted to ApJ on 2009 Sep 15, 22 pages, 23 figures
Modeling with Mocking
Creators: name: Stoel, Jouke
name: Storm, Van Der
name: Vinju, Jurgen
Publisher: name: Zenodo
Year: 2021
Subjects: lightweight formal specifications
bounded model checking
temporal logic

description: Writing formal specifications often requires users to abstract from the original problem. Especially when verification techniques such as model checking are used. Without applying abstraction the search space the model checker need to traverse tends to grow quickly beyond the scope of what can be checked within reasonable time. The downside of this need to omit details is that it increases the distance to the implementation. Ideally, the created specifications could be used to generate software from (either manually or automatically). But having an incomplete description of the desired system is not enough for this purpose. In this work we introduce the REBEL2 specification language. REBEL2 lets the user write full system specifications in the form of state machines with data without the need to apply abstraction while still preserving the ability to verify non-trivial properties. This is done by allowing the user to _forget_ and _mock_ specifications when running the model checker. The original specifications are untouched by these techniques. We compare the expressiveness of REBEL2 and the effectiveness of _mock_ and _forget_ by implementing two case studies: one from the automotive domain and one from the banking domain. We find that REBEL2 is expressive enough to implement both case studies in a concise manner. Next to that, when performing checks in isolation, mocking can speed up model checking significantly.
Additional file 1 of Endoscopic intraventricular hematoma evacuation surgery versus external ventricular drainage for the treatment of patients with moderate to severe intraventricular hemorrhage: a multicenter, randomized, controlled trial
Creators: name: Zhu, Junhao
name: Tang, Chao
name: Cong, Zixiang
name: Yang, Jin
name: Cai, Xiangming
name: Ma, Chiyuan
name: Liu, Yuxiu
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Science Policy

description: Additional file 1. SPIRIT 2013 Checklist: Recommended items to address in a clinical trial protocol and related documents.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ ÑÐ¾Ð±Ð¾ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ Ð½Ð°Ð¿Ð»Ð°Ð²ÐºÐ¸ Ð°Ð»ÑÐ¼Ð¸Ð½Ð¸ÐµÐ²ÑÑ Ð¿Ð¾Ð»ÑÑÐ°Ð±ÑÐ¸ÐºÐ°ÑÐ¾Ð²
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ·Ð¾Ð²ÑÐµÐ², ÐÐµÐ¾ÑÐ³Ð¸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: 2017
Subjects: Ð°Ð´Ð´Ð¸ÑÐ¸Ð²Ð½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸
ÑÐ¾Ð±Ð¾ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð°Ñ Ð½Ð°Ð¿Ð»Ð°Ð²ÐºÐ°
ÑÐ²Ð°ÑÐºÐ° Ð°Ð»ÑÐ¼Ð¸Ð½Ð¸Ñ

description: Ð Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ° Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð°Ð¿Ð»Ð°Ð²ÐºÐ¸ Ð°Ð»ÑÐ¼Ð¸Ð½Ð¸Ñ Ð² ÑÑÐµÐ´Ðµ Ð·Ð°ÑÐ¸ÑÐ½ÑÑ Ð³Ð°Ð·Ð¾Ð², Ð¿Ð¾Ð»ÑÑÐµÐ½Ñ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¼ ÑÐ²Ð°ÑÐ¾ÑÐ½Ð¾Ð¼ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¸, Ð¼ÐµÑÐ¾Ð´Ð°Ñ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸ Ð¿ÐµÑÐµÐ½Ð¾ÑÐ° Ð¼ÐµÑÐ°Ð»Ð»Ð°. ÐÐ·ÑÑÐµÐ½Ñ Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð½ÐµÑÐºÐ¾Ð»ÑÐºÐ¾ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² ÑÐ¾Ð±Ð¾ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ Ð½Ð°Ð¿Ð»Ð°Ð²ÐºÐ¸, ÑÐ¾Ð²ÐµÑÑÐµÐ½Ñ Ð¿Ð¾Ð¿ÑÑÐºÐ¸ Ðº Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¿ÑÐ¸Ð¼Ð¸ÑÐ¸Ð²Ð½ÑÑ ÑÐ¸Ð³ÑÑ. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð° Ð¾Ð±ÑÐ¸ÑÐ½Ð°Ñ Ð±Ð¸Ð±Ð»Ð¸Ð¾Ð³ÑÐ°ÑÐ¸Ñ Ð¿Ð¾ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐµÐ¼Ð°ÑÐ¸ÐºÐµ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÑÐ´ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ¾Ð², Ð´ÐµÐ¼Ð¾Ð½ÑÑÑÐ¸ÑÑÑÑÐ¸Ñ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² ÑÐ²Ð°ÑÐºÐ¸ Ð½Ð° ÐºÐ¾ÑÑÑÐ¸ÑÐ¸ÐµÐ½Ñ Ð½Ð°Ð¿Ð»Ð°Ð²ÐºÐ¸.
Cosmic Ray Spallation in Radio-Quiet Active Galactic Nuclei: A Case Study of NGC 4051
Creators: name: Turner, T. J.
name: Miller, L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We investigate conditions for and consequences of spallation in radio-quiet Seyfert galaxies. The work is motivated by the recent discovery of significant line emission at 5.44 keV in Suzaku data from NGC 4051. The energy of the new line suggests an identification as Cr I Ka emission, however the line is much stronger than would be expected from material with cosmic abundances, leading to a suggestion of enhancement owing to nuclear spallation of Fe by low energy cosmic rays from the active nucleus. We find that the highest abundance enhancements are likely to take place in gas out of the plane of the accretion disk and that timescales for spallation could be as short as a few years. The suggestion of a strong nuclear flux of cosmic rays in a radio-quiet Seyfert galaxy is of particular interest in light of the recent suggestion from Pierre Auger Observatory data that ultra-high-energy cosmic rays may originate in such sources.
description: 14 pages, 1 figure. Accepted for publication in The Astrophysical Journal
title: ÐÐ°ÑÐ¶Ð¸Ð½Ð°Ð»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¹ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ ÐµÐ³Ð¾ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð´Ð»Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¸Ð±ÑÐ»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ÐµÐ´Ð¾Ð³Ð¾Ð²Ð¾ÑÐ¾Ð²Ð°, ÐÐ°Ñ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: Ð¼Ð°ÑÐ¶Ð¸Ð½Ð°Ð»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð·
ÑÐ¾ÑÐºÐ° Ð±ÐµÐ·ÑÐ±ÑÑÐ¾ÑÐ½Ð¾ÑÑÐ¸
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ
ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÑ

description: Ð Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð° Ð¾Ð±ÑÐ°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° ÐÐÐ Â«Ð¢Ð¾ÑÐ³Ð¾Ð²ÑÐ¹ ÐÐ¾Ð¼ Â«Ð­Ð½ÐµÑÐ³Ð¾ÑÐ±ÑÑÂ», ÐµÐ³Ð¾ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ°, Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð·Ð° 2014-2016 Ð³Ð¾Ð´Ñ. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð° Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²Ð°Ñ Ð±Ð°Ð·Ð° ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ° ÐÐÐ Â«Ð¢Ð¾ÑÐ³Ð¾Ð²ÑÐ¹ ÐÐ¾Ð¼ Â«Ð­Ð½ÐµÑÐ³Ð¾ÑÐ±ÑÑÂ». ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾ÑÑÐ°Ð²Ð° Ð¸ ÑÑÑÑÐºÑÑÑÑ Ð·Ð°ÑÑÐ°Ñ ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¹ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð¼Ð°ÑÐ¶Ð¸Ð½Ð°Ð»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð·Ð°ÑÑÐ°Ñ Ð¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¾Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¾Ð²Ð°ÑÐ¾Ð² (Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ ÑÐ¾ÑÐºÐ¸ Ð±ÐµÐ·ÑÐ±ÑÑÐ¾ÑÐ½Ð¾ÑÑÐ¸, Ð·Ð°Ð¿Ð°ÑÐ° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÐ¸, Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÑÑÑÐ°Ð³Ð°). ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð¾ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¸Ð±ÑÐ»Ð¸ Ð·Ð° ÑÑÐµÑ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð² Ð´ÐµÐ¹ÑÑÐ²Ð¸Ðµ ÑÐµÐ·ÐµÑÐ²Ð¾Ð² ÑÐ¾ÑÑÐ° Ð¿ÑÐ¸Ð±ÑÐ»Ð¸ Ð² ÐÐÐ Â«Ð¢Ð¾ÑÐ³Ð¾Ð²ÑÐ¹ ÐÐ¾Ð¼ Â«Ð­Ð½ÐµÑÐ³Ð¾ÑÐ±ÑÑÂ». ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÐ¼ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹.
Three-Qubit Ground State and Thermal Entanglement of $XXZ$ Model With Dzyaloshinskii-Moriya Interaction
Creators: name: Jafari, R.
name: Langari, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We have studied the symmetric and non-symmetric pairwise ground state and thermal entanglement in three-qubit anisotropic Heisenberg (XXZ) and Ising in a magnetic field models and in the presence of Dzyaloshinskii-Moriya (DM) interaction. We have found that increasing of the DM interaction and magnetic field can enhance and reduce the entanglement of system. We have shown that the non-symmetric pairwise has higher value concurrence and critical temperature (above which the entanglement vanishes) than the symmetric pairwise. For negative anisotropy the non-symmetric entanglement is a monotonic function of DM interaction while for positive anisotropy it has a maximum versus DM parameter and vanishes for larger values of DM interaction. The conditions for the existence of thermal entanglement are discussed in details. The most remarkable result happens at zero temperature where 3-qubit ground state entanglement of the system (in spite of 2-qubit counterpart) shows the fingerprint of quantum phase transition for an infinite size system.
200SMEchallenge Partner's Handbook to Experimental Open Innovation Scheme
Creators: name: Ohland-Andersen, Mads
Publisher: name: Zenodo
Year: 2021
Subjects: Horizon2020
200SMEChallenge

description: This deliverable aims at providing project partners with all the needed guidance to set up and execute the UX Challenge, as stated in the Project Plan. The deliverable is also publicly available to external innovation agencies that might be willing to embark in the same effort, though not as part of project 200SMEchallenge. In the light of the results of the experimental pilot and RCT - Randomized Control Trial study, another more specific deliverable will be made available by the project with the specific purpose of building capacity for adoption of the piloted scheme beyond the project consortium (D2.2 Practical Guide for Innovation Agencies to adopt and scale up the scheme).
title: ÐÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° Ð´Ð»Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐ¾Ð³Ð»Ð°ÑÐµÐ½Ð¸Ð¹ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½ÑÑ ÑÐµÐµÑÑÑÐ¾Ð²
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Ð½Ð¸ÑÐ·Ð¾Ð², Ð¢Ð¸Ð¼Ñ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Ð¼Ð°ÑÑ-ÐºÐ¾Ð½ÑÑÐ°ÐºÑ
ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½ÑÐµ ÑÐµÐµÑÑÑÑ
Ð±Ð»Ð¾ÐºÑÐµÐ¹Ð½

description: Ð Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿Ð»Ð°ÑÑÐ¾ÑÐ¼Ñ, ÐºÐ¾ÑÐ¾ÑÐ°Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸Ñ Ð¸ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ðµ Ð·Ð°ÐºÐ»ÑÑÐµÐ½Ð½ÑÑ ÑÐ¾Ð³Ð»Ð°ÑÐµÐ½Ð¸Ð¹ Ð¼ÐµÐ¶Ð´Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸ÑÐ¼Ð¸. Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÐµÐºÑÑÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐµÐ½ÑÑÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÑ ÑÐµÐµÑÑÑÐ¾Ð². ÐÑÐ» Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐµÐ´ÑÑÐ² Ð´Ð»Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð´ÐµÑÐµÐ½ÑÑÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ, Ð² ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ ÐºÐ¾ÑÐ¾ÑÐ¾Ð³Ð¾ Ð±ÑÐ»Ð° Ð²ÑÐ±ÑÐ°Ð½Ð° Ð¿Ð»Ð°ÑÑÐ¾ÑÐ¼Ð° Corda. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸Ð»Ð°ÑÑ Ð½Ð° ÑÐ·ÑÐºÐµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Java. ÐÐ·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ðµ Ñ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸ÐµÐ¼-ÐºÐ»Ð¸ÐµÐ½ÑÐ¾Ð¼ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð² REST+JSON Ð¿Ð¾Ð´ÑÐ¾Ð´Ðµ.
A STUDY TO EXAMINE SELF-EFFICACY, SELF-REGULATION AND THEIR RELATIONSHIP TO OVERWEIGHT PATIENTS WHO UTILIZE A HEALTH COACH
Creators: name: Pidermann, Barbara Lea
Publisher: name: Zenodo
Year: 2014

description: The purpose of this study was to examine whether there was a positive effect on overweight individuals who utilized an exercise coach. It also explored the relationships of self-efficacy (SE) and self-regulation (SR) to exercise adherence in normal-weight and overweight individuals. A comparative descriptive design was used to study adult patients in a family practice clinic who were selected by convenience sampling during a routine visit. At that time, participants completed surveys that measured levels of general SE and exercise SR along with a demographic questionnaire. Tools utilized were the General Self-Efficacy Scale, the Self-Regulation Questionnaire for Exercise, and a self-report demographic questionnaire. Statistical analysis was completed to determine whether there was a positive effect on exercise adherence in overweight individuals who utilized an exercise coach. In addition, statistical interpretations were used to determine whether there was a relationship between SE, SR, and exercise adherence in normal- weight and overweight individuals. The results indicated a significant relationship between SR and exercise adherence but no significant relationship between SE and exercise adherence. Due to sample size, the study was unable to determine whether there was a positive effect on exercise adherence in overweight individuals who utilized an exercise coach iii In conclusion, those who had high levels of exercise adherence were high self-regulators but did not necessarily have high levels of general SE. The study was unable to determine whether there was a positive effect on overweight individuals who used an exercise coach.
3D human pose estimation with self-supervision and learnable data generation
Creators: name: Gholami, Mohsen
Publisher: name: University of British Columbia
Year: 2024

description: The estimation of 3D human body poses from 2D images is needed in a wide-ranging application across robotics, computer graphics, and patient monitoring. While Deep Learning offers promising solutions to this challenging problem, the progress has been impeded by the scarcity of annotated 3D datasets. This thesis proposes innovative strategies for training deep learning models without the need for explicit 3D annotated data. Previous approaches have proposed generating pseudo-ground-truth 3D annotated data from multi-view 2D images. While 2D images are cost-effective and easy to capture, these methods unfortunately require calibrated multi-view images. We propose a weak supervision approach that combines classical triangulation methods with a multi-view network to generate pseudo-ground-truth 3D images, demonstrating superior results without requiring camera calibration. We then investigate the generation of synthetic 3D pose data to enhance the generalizability of 3D pose models. We propose generating synthetic 2D-3D pose data that rely on random generation methods as have been previously proposed. Our method is a targeted synthetic 2D-3D pose generation that is tailored to have the resulting 3D pose models adapt to specific settings. Leveraging unlabeled images from the target domain, our method demonstrates significant performance improvements. We further extend our data generation method and generate image-3D poses using Neural Radiance Fields (NeRF). NeRFs have recently been proposed for generating novel views of humans, based on a partial set of 2D images. Unlike classical rendering methods, our method does not require 3D scans of humans. It generates out-of-distribution images for 3D pose models and significantly improves the generalizability of models on unseen datasets. We then explore a real-life application of estimating 3D body poses for monitoring Parkinson's disease patients. Here, we observe that poor generalizability of 3D pose models hinders their application to patient gait monitoring where accurate gait measurement is important. To avoid obtaining cumbersome and time-consuming clinical data, we introduce a weak supervision method that utilizes the expertise of clinicians to label the gait videos of Parkinson's patients, enhancing the applicability of 3D pose estimation in clinical settings.
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾Ð¿Ð»Ð°ÑÑ ÑÑÑÐ´Ð° Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÑÐºÐµÐ²Ð¸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: 2016
Subjects: ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾Ð¿Ð»Ð°ÑÑ ÑÑÑÐ´Ð°
ÑÐ¸ÑÑÐµÐ¼Ð° Ð¾Ð¿Ð»Ð°ÑÑ ÑÑÑÐ´Ð°
Ð¾Ð¿Ð»Ð°ÑÐ° ÑÑÑÐ´Ð° Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°

description: Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° Ð¾Ð¿Ð»Ð°ÑÑ ÑÑÑÐ´Ð° Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°, Ð²ÑÐ´ÐµÐ»ÑÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ Ðº Ð¾Ð¿Ð»Ð°ÑÐµ ÑÑÑÐ´Ð°, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼ÑÐµ Ð² Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½Ð¾Ð¹ Ð¿ÑÐ°ÐºÑÐ¸ÐºÐµ Ð¸ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¸ÑÑÑ Ð¾ÑÐµÐ½ÐºÐ° Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸. ÐÐ½Ð°Ð»Ð¸Ð·Ð¸ÑÑÐµÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ ÐÐÐ Â«ÐÐµÑÑÐ¾ÑÐµÐ½ÑÑÂ» Ð½Ð° Ð¿ÑÐµÐ´Ð¼ÐµÑ Ð¿ÑÐ¾ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾ÑÑÐ¸ Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐµÐ¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾Ð¿Ð»Ð°ÑÑ ÑÑÑÐ´Ð° Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°, Ð²ÑÑÐ²Ð»ÑÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐºÐ¸ Ð¸ Ð´Ð°ÑÑÑÑ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð¸Ñ ÑÑÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð¸ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾Ð¿Ð»Ð°ÑÑ ÑÑÑÐ´Ð° Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸.
title: ÐÐ½Ð¾ÑÑÑÐ°Ð½Ð½ÑÐ¹ ÑÐ·ÑÐº: Ð±Ð°Ð·Ð¾Ð²ÑÐ¹ ÐºÑÑÑ (Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¸Ð¹ ÑÐ·ÑÐº). Ð§. 1
title: ÑÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ±Ð°ÐºÑÐ¼Ð¾Ð²Ð°, ÐÐ°ÑÐ¸Ñ
name: ÐÐ¾Ð»ÑÑÐ°ÐºÐ¾Ð²Ð°, ÐÐ½Ð½Ð°
name: ÐÐ¾Ð»ÑÐºÐ¾Ð²Ð°, ÐÐ°Ñ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: 2018
Subjects: Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¸Ð¹ ÑÐ·ÑÐº
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÐÐÐÐ­Ð¸Ð¢ Ð¿Ð¾ Ð²ÑÐµÐ¼ Ð¿ÑÐ¾ÑÐ¸Ð»ÑÐ¼ Ð¸ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Ð¾ÑÐ½Ð¾Ð¹, Ð¾ÑÐ½Ð¾-Ð·Ð°Ð¾ÑÐ½Ð¾Ð¹ Ð¸ Ð·Ð°Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ¼ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ "ÐÐ½Ð¾ÑÑÑÐ°Ð½Ð½ÑÐ¹ ÑÐ·ÑÐº (Ð±Ð°Ð·Ð¾Ð²ÑÐ¹ ÐºÑÑÑ)". ÐÐ°Ð½Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð°Ð´ÑÐµÑÐ¾Ð²Ð°Ð½Ð¾ Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ð¼ÑÑ 1-Ð¾Ð³Ð¾ Ð¸ 2-Ð¾Ð³Ð¾ ÐºÑÑÑÐ¾Ð² ÑÑÐ¾Ð²Ð½Ñ B1 Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ ÐµÐ²ÑÐ¾Ð¿ÐµÐ¹ÑÐºÐ¾Ð¹ ÑÐºÐ°Ð»Ð¾Ð¹ ÑÑÐ¾Ð²Ð½ÐµÐ¹ Ð²Ð»Ð°Ð´ÐµÐ½Ð¸Ñ ÑÐ·ÑÐºÐ¾Ð¼. ÐÐ°Ð¶Ð´ÑÐ¹ ÑÐ°Ð·Ð´ÐµÐ» Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð´Ð²Ðµ ÑÐ°ÑÑÐ¸: ÐºÑÐ°ÑÐºÐ¸Ð¹ Ð³Ð»Ð¾ÑÑÐ°ÑÐ¸Ð¹ Ð¿Ð¾ ÑÐµÐ¼Ðµ Ð¸ ÑÐ¿ÑÐ°Ð¶Ð½ÐµÐ½Ð¸Ñ Ð½Ð° Ð¾ÑÐ²Ð¾ÐµÐ½Ð¸Ðµ Ð¸ Ð·Ð°ÐºÑÐµÐ¿Ð»ÐµÐ½Ð¸Ðµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¾ ÐºÐ»ÑÑÐ°Ð¼Ð¸ Ð² Ð²Ð¸Ð´Ðµ Ð¾ÑÐ´ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ, ÑÑÐ¾ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÑ ÐµÐ³Ð¾ ÐºÐ°Ðº Ð´Ð»Ñ Ð°ÑÐ´Ð¸ÑÐ¾ÑÐ½Ð¾Ð¹, ÑÐ°Ðº Ð¸ Ð´Ð»Ñ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ.
Interactions of the magnetospheres of stars and close-in giant planets
Creators: name: Cohen, O.
name: Drake, J. J.
name: Kashyap, V. L.
name: Saar, S. H.
name: Sokolov, I. V.
name: Manchester, W. B.
name: Hansen, K. C.
name: Gombosi, T. I.
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: Since the first discovery of an extrasolar planetary system more than a decade ago, hundreds more have been discovered. Surprisingly, many of these systems harbor Jupiter-class gas giants located close to the central star, at distances of 0.1 AU or less. Observations of chromospheric 'hot spots' that rotate in phase with the planetary orbit, and elevated stellar X-ray luminosities,suggest that these close-in planets significantly affect the structure of the outer atmosphere of the star through interactions between the stellar magnetic field and the planetary magnetosphere. Here we carry out the first detailed three-dimensional MagnetoHydroHynamics (MHD) simulation containing the two magnetic bodies and explore the consequences of such interactions on the steady-state coronal structure. The simulations reproduce the observable features of 1) increase in the total X-ray luminosity, 2) appearance of coronal hot spots, and 3) phase shift of these spots with respect to the direction of the planet. The proximate cause of these is an increase in the density of coronal plasma in the direction of the planet, which prevents the corona from expanding and leaking away this plasma via a stellar wind. The simulations produce significant low temperature heating. By including dynamical effects, such as the planetary orbital motion, the simulation should better reproduce the observed coronal heating.
Oscillations of rotating magnetised neutron stars with purely toroidal magnetic fields
Creators: name: Lander, S. K.
name: Jones, D. I.
name: Passamonti, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We investigate the oscillation spectrum of rotating Newtonian neutron stars endowed with purely toroidal magnetic fields, using a time evolution code to evolve linear perturbations in the Cowling approximation. The background star is generated by numerically solving the MHD equilibrium equations and may be nonspherical by virtue of both rotation and magnetic effects; hence our perturbations and background are fully consistent. Whilst the background field is purely toroidal, the perturbed field is mixed poloidal-toroidal. From Fourier analysis of the perturbations we are able to identify a number of magnetically-restored Alfvén (or $a$-) modes. We show that in a rotating star pure inertial and $a$-modes are replaced by hybrid magneto-inertial modes, which reduce to $a$-modes in the nonrotating limit and inertial modes in the nonmagnetic limit. We show that the $r$-mode instability is suppressed by magnetic fields in sufficiently slowly rotating stars. In addition, we determine magnetic frequency shifts in the $f$-mode. We discuss the astrophysical relevance of our results, in particular for magnetar oscillations.
description: 15 pages, 9 figures
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ ÑÐ°Ð¹ÑÐ° Ð´Ð»Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð¿Ð¾ Ð¾ÐºÐ°Ð·Ð°Ð½Ð¸Ñ ÑÑÐ»ÑÐ³ ÑÐ²ÑÐ·Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐÐÐ ÐÑÑ ÐÑ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ÑÑÐ¿ÐµÐ½ÐºÐ¾Ð², 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: Ð¸Ð½ÑÐµÑÐ½ÐµÑ
Ð²ÐµÐ±-Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð²ÐµÐ±-Ð´Ð¸Ð·Ð°Ð¹Ð½
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