cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The role of happiness in climate action
Creators: name: Radke, Jade
Publisher: name: University of British Columbia
Year: 2024

description: Despite the climate emergency, few people are acting on climate change. One potential reason for inaction is that climate communication often focuses on the negative effects of climate change and the need to make personal sacrifices. Such communication can make people retreat from the issue rather than engage with it. To address this, we combined happiness science with climate science in a new happy climate approach that focuses on the happiness benefits of climate action. In Study 1 (N=1320) presented in Chapter 2, we randomly assigned participants to read one of four messages: happy climate, neutral, disaster, or happy-only. Participants then selected the climate actions they would be willing to engage in. We found that the happy climate message resulted in the most individual and civic climate actions chosen. In Study 2 (N=779) presented in Chapter 3, participants were presented with 15 climate action statements and asked to rate how likely they are to engage in the action and how happy doing so would make them feel. These actions were either framed to emphasize what they could do more to benefit the environment or what they could do less to benefit the environment. We found that those in the do-more-good condition were significantly more likely to engage in climate action than those in the do-less-bad condition, and this effect was mediated by a boost in happiness. In Study 3 (N=302) presented in Chapter 4, participants could choose between receiving a guaranteed 10 cent refund per bottle for recycling or opt for a chance to win a higher amount of money. We found that people preferred and were happier with probabilistic rewards for recycling than certain rewards. The results from the three studies presented in this thesis highlight the importance of happiness for climate action.
The European Pulsar Timing Array: current efforts and a LEAP toward the future
Creators: name: Ferdman, Robert D.
name: van Haasteren, Rutger
name: Bassa, Cees G.
name: Burgay, Marta
name: Cognard, Ismael
name: Corongiu, Alessandro
name: D'Amico, Nichi
name: Desvignes, Gregory
name: Hessels, Jason W. T.
name: Janssen, Gemma H.
name: Jessner, Axel
name: Jordan, Christine
name: Karuppusamy, Ramesh
name: Keane, Evan F.
name: Kramer, Michael
name: Lazaridis, Kosmas
name: Levin, Yuri
name: Lyne, Andrew G.
name: Pilia, Maura
name: Possenti, Andrea
name: Purver, Mark
name: Stappers, Ben
name: Sanidas, Sotirios
name: Smits, Roy
name: Theureau, Gilles
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The European Pulsar Timing Array (EPTA) is a multi-institutional, multi-telescope collaboration, with the goal of using high-precision pulsar timing to directly detect gravitational waves. In this article we discuss the EPTA member telescopes, current achieved timing precision, and near-future goals. We report a preliminary upper limit to the amplitude of a gravitational wave background. We also discuss the Large European Array for Pulsars, in which the five major European telescopes involved in pulsar timing will be combined to provide a coherent array that will give similar sensitivity to the Arecibo radio telescope, and larger sky coverage.
description: 10 pages, 2 figures, 2 tables, Amaldi 8 conference proceedings, accepted for publication by Classical & Quantum Gravity
title: ÐÐ¾Ð»Ð¾Ð´ÐµÐ¶Ð½Ð°Ñ Ð¿ÑÐ¸ÐµÐ¼Ð½Ð°Ñ ÐºÐ°Ðº Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½Ñ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð¼Ð¸Ð´Ð¶Ð° Ð¾ÑÐ³Ð°Ð½Ð° Ð²Ð»Ð°ÑÑÐ¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐ¾Ð»Ð¾Ð´ÐµÐ¶Ð½Ð¾Ð¹ Ð¿ÑÐ¸ÐµÐ¼Ð½Ð¾Ð¹ ÐÐ´Ð¼Ð¸Ð½Ð¸ÑÑÑÐ°ÑÐ¸Ð¸ ÐÐ°Ð»Ð¸Ð½Ð¸Ð½ÑÐºÐ¾Ð³Ð¾ ÑÐ°Ð¹Ð¾Ð½Ð° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¤ÑÐ½Ð´Ð°Ð¼Ð¸Ð½ÑÐºÐ°Ñ, 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: 2017
Subjects: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³, Ð³Ð¾ÑÐ¾Ð´
PR-Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ
Ð¸Ð¼Ð¸Ð´Ð¶
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ÐÐ¾Ð»Ð¾Ð´ÐµÐ¶Ð½Ð°Ñ Ð¿ÑÐ¸ÐµÐ¼Ð½Ð°Ñ
ÐÐ°Ð»Ð¸Ð½Ð¸Ð½ÑÐºÐ¸Ð¹ ÑÐ°Ð¹Ð¾Ð½

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÐºÐ¾-Ð¼ÐµÑÐ¾Ð´Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð¸Ð¼Ð¸Ð´Ð¶Ð° Ð¾ÑÐ³Ð°Ð½Ð¾Ð² Ð²Ð»Ð°ÑÑÐ¸; Ð¾Ð¿Ð¸ÑÑÐ²Ð°ÑÑÑÑ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¸Ð¼Ð¸Ð´Ð¶Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ ÐµÐ³Ð¾ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ°, ÑÐ¸Ð¿Ñ Ð¸ ÑÑÐ½ÐºÑÐ¸Ð¸. ÐÐ·ÑÑÐ°ÑÑÑÑ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¸ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð¼Ð¸Ð´Ð¶Ð° Ð¾ÑÐ³Ð°Ð½Ð¾Ð² Ð²Ð»Ð°ÑÑÐ¸. ÐÐ°Ð½Ð° ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° ÐÐ¾Ð»Ð¾Ð´ÐµÐ¶Ð½Ð¾Ð¹ Ð¿ÑÐ¸ÐµÐ¼Ð½Ð¾Ð¹, ÐºÐ°Ðº Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ° ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð¼Ð¸Ð´Ð¶Ð° ÐÐ´Ð¼Ð¸Ð½Ð¸ÑÑÑÐ°ÑÐ¸Ð¸ ÐÐ°Ð»Ð¸Ð½Ð¸Ð½ÑÐºÐ¾Ð³Ð¾ ÑÐ°Ð¹Ð¾Ð½Ð° Ð³Ð¾ÑÐ¾Ð´Ð° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³. ÐÑÐ¾Ð³Ð¾Ð¼ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÑÑÑÑ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð¼Ð¸Ð´Ð¶Ð° ÐÐ¾Ð»Ð¾Ð´ÐµÐ¶Ð½Ð¾Ð¹ Ð¿ÑÐ¸ÐµÐ¼Ð½Ð¾Ð¹.
Radial Velocity Survey for Planets around Young stars RV-SPY
Creators: name: Zakhozhay, Olga
name: Launhardt, R.
name: Brems, S.
name: Trifonov, T.
name: Müller, A.
name: Henning, Th.
name: Kürster, M.
name: Reffert, S.
Publisher: name: Zenodo
Year: 2021

description: Planets are born in gaseous protoplanetary disks that surround young stars. Within only a few million years, protoplantary disks lose their gas due to accretion onto the star and newly formed planets, but also via disk winds. While we are now nearly every day gaining new insights into the structure and composition of circumstellar disks, detections of forming protoplanets around young stars are still extremely challenging and therefore very rare. In my talk I will present our large radial velocity search program for planets around young stars with debris disks - RV-SPY. Our sample includes over one hundred targets that we are observing with FEROS. Majority of our stars are included in NaCo- ISPY ESO-GTO direct imaging survey for planets. The synergy of both these surveys will allow us to draw the up-to-date most robust constraints on the occurrence and properties of giant planets in young debris disks. I will also overview the results of the first few semesters of high-cadence observations that is aiming to scan our targets for both stellar activity and the presence of hot Jupiters.
The Financing of Associations in the Italian Regions during the Period 2005-2022
Creators: name: Leogrande, Angelo
Publisher: name: Zenodo
Year: 2023

description: Istat calculates the value of association financing. The variable is calculated as the number of people aged 14 and over who have financed associations in the last 12 months out of the total number of people aged 14 and over. The data refers to the Italian regions between 2005 and 2022.
Supplementary Information (SI) from Rheology and electro-magnetism stimulated non-trivial deformation dynamics of viscoelastic compound droplets
Creators: name: Gupta, Pulak
name: Dhar, Purbarun
name: Samanta, Devranjan
Publisher: name: The Royal Society
Year: 2025
Subjects: classificationCode: 400499
subject: Chemical engineering not elsewhere classified
classificationCode: 401299
subject: Fluid mechanics and thermal engineering not elsewhere classified
classificationCode: 401799
subject: Mechanical engineering not elsewhere classified

description: In this research, we present an analytical model describing the deformation dynamics of viscoelastic, leaky dielectric droplet confined within a surrounding liquid under the influence of direct electric field and uniform magnetic field. We have considered various combinations of droplets and surrounding fluid, which can be either Newtonian (N) or non-Newtonian (N-N), and may mimic a compound droplet scenario too. The governing equations for conservation of charge, mass, momentum and electromagnetic phenomena are solved for the leaky dielectric theory within the Stokes flow regime and the small deformation approximation. The electrical, magnetic and viscoelastic behaviour is realized using the Cauchy momentum equation in conjunction with the Maxwell stress tensor, Lorentz force and the upper convected Maxwell (UCM) model, respectively. The changes in deformation and flow characteristics are comprehensively analysed through the variation of key non-dimensional parameters, namely the Capillary number (Ca), Weissenberg number (Wi) and electromagnetic interaction number (Em). The present work is restricted to Wi ≤ 1 and semi-analytical solutions to the complicated multi-physics phenomena is obtained. Our study reveals that in the presence of only an electric field, a flow field in the non-Newtonian fluid fails to develop if the droplet has relatively lower conductivity compared to the surrounding medium, owing to the insufficient intensity of the electric field. However, when the droplet is relatively more conductive than the surrounding medium, a flow field does arise. The analysis shows that an augmentation in the flow and deformation behaviour of the non-Newtonian fluid can be observed when the magnetic field is applied, but only in a specific direction relative to the electric field. Flow is induced in the +B direction when the droplet is relatively less conductive, and the electromagnetic force dominates over the hydrodynamic force. Conversely, in the −B direction, flow is induced when the droplet is relatively more conductive, as both the electric and electromagnetic forces act work together. Such findings provide intricate insights into understanding electro-magneto-hydrodynamics (EMHDs) with non-Newtonian confined droplets, and may enable avenues towards realizing precision industrial and scientific microfluidic technologies via manipulation of the movement, deformation and coalescence of droplets.
Cavity phenomena in mesas of cuprate high-$T_c$ superconductors under voltage bias
Creators: name: Hu, Xiao
name: Lin, Shizeng
Publisher: name: arXiv
Year: 2009
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Modeling a single crystal of cuprate high-$T_c$ superconductor, such as $\rm{Bi_2Sr_2CaCu_2O_{8+δ}}$, as a stack of intrinsic Josephson junctions, we formulate explicitly the cavity phenomenon of plasma oscillations and electromagnetic (EM) waves in mesas of cylindrical and annular shapes. When the mesa thickness is small compared with the EM wavelength, the boundary condition for the inductively coupled sine-Gordon equations is the Neumann-type one to a good approximation, addressed first theoretically and verified in a recent experiment. This renders the superconductor mesa a cavity. Biasing a dc voltage in the $c$ direction, a state with $\pmπ$ kinks in the superconductivity phase difference piled up alternatively along the c axis is stabilized. The $\pmπ$ phase kinks provide inter-lock between superconductivity phases in adjacent junctions, taking the advantage of huge inductive couplings inherent in the cuprate superconductors, which establishes the coherence across the whole system of more than $\sim 600$ junctions. They also permit a strong coupling between the lateral cavity mode and the transverse Josephson plasma, enhance the plasma oscillation significantly at the cavity modes which radiates EM waves in the terahertz band when the lateral size of mesa is set to tens of micrometers. In order to overcome the heating effect, we propose to use annular geometry. The dependence of frequency on the aspect ratio is analyzed, which reveals that the shape tailor is quite promising for improving the present technique of terahertz excitation. The annular geometry may be developed as a waveguide resonator, mimic the fiber lasers for visible lights.
description: 10 pages, 13 figures
title: ÐÑÐ¸ÑÑÐ°Ð»Ð»Ð¾Ð³ÑÐ°ÑÐ¸Ñ
title: ÑÑÐµÐ±Ð½Ð¸Ðº 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 Â«ÐÐ°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð¸ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð½Ð¾Ð²ÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð²Â»
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ¸Ð»ÑÐµÐ², ÐÐ¼Ð¸ÑÑÐ¸Ð¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ Ð¡ÐÐ±ÐÐ¢Ð£
Year: 1996
Subjects: ÐÑÐ¸ÑÑÐ°Ð»Ð»Ð¾Ð³ÑÐ°ÑÐ¸Ñ

description: Ð£ÑÐµÐ±Ð½Ð¸Ðº Ð¿Ð¾ÑÐ²ÑÑÐµÐ½ Ð³ÐµÐ¾Ð¼ÐµÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¸ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¾Ð³ÑÐ°ÑÐ¸Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¾ÑÐ¸Ð¼Ð¸Ð¸. ÐÐ·Ð»Ð¾Ð¶ÐµÐ½Ñ ÑÐ»ÐµÐ¼ÐµÐ½ÑÑ Ð»Ð¸Ð½ÐµÐ¹Ð½Ð¾Ð¹ Ð°Ð»Ð³ÐµÐ±ÑÑ Ð¸ ÑÐµÐ¾ÑÐ¸Ð¸ Ð³ÑÑÐ¿Ð¿, Ð·Ð½Ð°Ð½Ð¸Ðµ ÐºÐ¾ÑÐ¾ÑÑÑ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ Ð´Ð»Ñ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¾Ð³ÑÐ°ÑÐ¸Ð¸. Ð ÐµÑÐµÐ½Ð¸Ñ Ð·Ð°Ð´Ð°Ñ Ð³ÐµÐ¾Ð¼ÐµÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¾Ð³ÑÐ°ÑÐ¸Ð¸ Ð´Ð°ÐµÑÑÑ Ð² Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¸ Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¾ÑÐ¼Ðµ. Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÑÑÑÐ¾ÐµÐ½Ð¸Ðµ Ð¸Ð´ÐµÐ°Ð»ÑÐ½ÑÑ ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¾Ð², ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¾Ð² Ñ Ð´ÐµÑÐµÐºÑÐ°Ð¼Ð¸ Ð¸ ÐºÐ²Ð°Ð·Ð¸ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¾Ð². Ð¢ÐµÐ½Ð·Ð¾ÑÐ½Ð¾Ðµ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¾Ð² Ð´Ð°ÐµÑÑÑ Ð² Ð±ÐµÑÐºÐ¾Ð¾ÑÐ´Ð¸Ð½Ð°ÑÐ½Ð¾Ð¹ Ð¸ ÐºÐ¾Ð¾ÑÐ´Ð¸Ð½Ð°ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ¼Ð°Ñ. ÐÐµÑÐ²Ð¾Ðµ Ð¸Ð·Ð´Ð°Ð½Ð¸Ðµ ÐºÐ½Ð¸Ð³Ð¸ Ð²ÑÑÐ»Ð¾ Ð² 1972 Ð³., Ð²ÑÐ¾ÑÐ¾Ðµ â Ð² 1981 Ð³. ÐÐ½Ð¸Ð³Ð° Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð° Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ Ð²ÑÐ·Ð¾Ð² Ð¸ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ¾Ð², Ð·Ð°Ð½Ð¸Ð¼Ð°ÑÑÐ¸ÑÑÑ Ð¸Ð·ÑÑÐµÐ½Ð¸ÐµÐ¼ ÑÐ²Ð¾Ð¹ÑÑÐ² ÑÐ²ÐµÑÐ´Ð¾Ð³Ð¾ ÑÐµÐ»Ð°. ÐÐ¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð° Ð´Ð»Ñ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¾Ð³ÑÐ°ÑÐ¸Ð¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°Ð¼Ð¸, Ð¼Ð°Ð³Ð¸ÑÑÑÐ°Ð¼Ð¸, Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ°Ð¼Ð¸ Ð¸ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ°Ð¼Ð¸, ÑÐ°Ð±Ð¾ÑÐ°ÑÑÐ¸Ð¼Ð¸ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ (material science) Ð¸ ÑÐ¸Ð·Ð¸ÐºÐ¸ ÑÐ²ÐµÑÐ´Ð¾Ð³Ð¾ ÑÐµÐ»Ð°.
Orbiting Configurable Artificial Star (ORCAS) for Visible Adaptive Optics from the Ground
Creators: name: Milam, Stefanie
name: Mather, John
name: Peretz, Eliad
name: Kain, Isabel
name: Slonaker, Richard
name: O'Meara, John
name: Seager, Sara
name: Hoerbelt, Tiffany
Publisher: name: Zenodo
Year: 2021

description: Enabling Adaptive Optics (AO) for a variety of targets across the sky at visible wavelengths for a range of telescopes on the ground could transform many key areas in astronomy. As a result, a 30th magnitude star could be imaged within minutes and the surfaces of planets, satellites, and asteroids could be mapped without visiting them. Cameras and spectrographs would have pixel areas reduced by factors of 104 to 105, and the isoplanatic patch could be resolved into ~100 megapixels for a Nyquist-sampled camera. The Keck telescopes, GMT, TMT, and E-ELT could reach nearly diffraction limited angular resolution, achieving up to an order of magnitude better performance than the Hubble Space Telescope. The Orbiting Configurable Artificial Star (ORCAS) is a small-scale mission composed of four wavelength-configurable artificial star small satellites propelled by ion engines and controlled from a ground station. This mission would overcome some major challenges in order to enable visible band AO such as: 1) insufficient brightness; 2) the cone effect; and 3) Tip-Tilt correction limitation. The mission overview and applications to planetary science will be presented.
Baron Munchhausen's Sequence
Creators: name: Khovanova, Tanya
name: Knop, Konstantin
name: Radul, Alexey
Publisher: name: arXiv
Year: 2010
Subjects: subject: Combinatorics (math.CO)
subject: Discrete Mathematics (cs.DM)
subject: Data Structures and Algorithms (cs.DS)
subject: History and Overview (math.HO)
subject: FOS: Mathematics
subject: FOS: Computer and information sciences
subject: 11B99, 00A08, 00A08

description: We investigate a coin-weighing puzzle that appeared in the all-Russian math Olympiad in 2000. We liked the puzzle because the methods of analysis differ from classical coin-weighing puzzles. We generalize the puzzle by varying the number of participating coins, and deduce a complete solution, perhaps surprisingly, the objective can be achieved in no more than two weighings regardless of the number of coins involved.
description: 26 pages
title: ÐÐ±ÑÐ°Ð· ÑÐ°ÑÑ Ð¾Ð±ÐµÐ·ÑÑÐ½ Ð¡ÑÐ½Ñ Ð£-ÐºÑÐ½Ð° Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ ÐºÐ¸ÑÐ°Ð¹ÑÐºÐ¾Ð¹ ÐºÑÐ»ÑÑÑÑÐµ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÐºÐ¾Ð²Ð°, ÐÐ¾Ð»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¡ÑÐ½Ñ Ð£-ÐºÑÐ½
ÐºÐ¸ÑÐ°Ð¹ÑÐºÐ°Ñ ÐºÑÐ»ÑÑÑÑÐ°
ÑÐ°ÑÑ Ð¾Ð±ÐµÐ·ÑÑÐ½
ÐÐÐ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÑÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¾Ð±ÑÐ°Ð·Ð° Ð¡ÑÐ½Ñ Ð£-ÐºÑÐ½Ð° Ð² ÑÑÐ°Ð´Ð¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¸ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ ÐºÑÐ»ÑÑÑÑÐ°Ñ ÐÐ¸ÑÐ°Ñ. ÐÐ·ÑÑÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð¶Ð° Ð² Ð´Ð²ÑÑ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ½ÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð¸ÑÑ: ÐºÐ»Ð°ÑÑÐ¸ÑÐµÑÐºÐ¾Ð¼ ÑÐ¾Ð¼Ð°Ð½Ðµ XVI Ð². Â«ÐÑÑÐµÑÐµÑÑÐ²Ð¸Ðµ Ð½Ð° ÐÐ°Ð¿Ð°Ð´Â» Ð¸ ÑÐ°ÑÐ¸ÑÐ¸ÑÐµÑÐºÐ¾Ð¼ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ XVII Ð². Â«ÐÐ¾Ð¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ðµ Ðº ÐÑÑÐµÑÐµÑÑÐ²Ð¸Ñ Ð½Ð° ÐÐ°Ð¿Ð°Ð´Â». Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ»Ð¸ÑÐ¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÐµÑÑÑ ÑÐ°ÑÑ Ð¾Ð±ÐµÐ·ÑÑÐ½ Ð² ÑÑÑÑ ÑÑÐµÑÐ°Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ ÐºÑÐ»ÑÑÑÑÑ ÐÐÐ : ÑÐµÐ»Ð¸Ð³Ð¸Ð¸, ÐºÐ¸Ð½ÐµÐ¼Ð°ÑÐ¾Ð³ÑÐ°ÑÐµ Ð¸ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐµ.
"AH WRONG SPEECH": PERSUASION OF GRAMMAR USED IN PRESIDENT JOKO WIDODO'S SPEECH AT THE ECOSPERITY WEEK SPEECH IN SINGAPORE
Creators: name: Dian Luthfiyati
name: Widyastuti
name: Suhartono
Publisher: name: Zenodo
Year: 2024
Subjects: Grammar, Persuasion, President Joko Widodo, Speech.

description: Abstract

This article is an analysis of the nature of propositions built in President Joko Widodo's persuasive speech about investment in the nation's capital from the perspective of mood analysis. This research also reveals how the speaker divides ethos, pathos and logos to the audience. This research uses discourse analysis with a qualitative approach to see how President Joko Widodo structures ethos, pathos and logos clauses grammatically. The results show that 1) ethos clauses are built with a declarative mood to show his credibility; 2) pathos clauses are formed with a declarative mood with the realization of the statement function and imperative mood to arouse the emotions of the audience; 3) logos clauses are structured with a declarative mood to provide a statement of the basis of the argumentation he conveyed.
title: ÐÐ²Ð¸Ð³Ð°ÑÐµÐ»Ð¸ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÑ Ð¼Ð°ÑÐ¸Ð½
title: Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¿Ð¾ ÐºÑÑÑÐ¾Ð²Ð¾Ð¼Ñ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐÐÐ¡
titleType: Subtitle
Creators: name: Ð ÑÑÐ¸Ð½Ð¾Ð², Ð Ð¾ÑÑÐ¸ÑÐ»Ð°Ð²
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2007
Subjects: ÐÐ²Ð¸Ð³Ð°ÑÐµÐ»Ð¸ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ³Ð¾ ÑÐ³Ð¾ÑÐ°Ð½Ð¸Ñ

description: ÐÐ°Ð½Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¼Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼Ñ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ Ð¸ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 190100 Â«ÐÐ°Ð·ÐµÐ¼Ð½ÑÐµ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÐµ ÑÐ¸ÑÑÐµÐ¼ÑÂ» Ð¸ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 190200 Â«Ð¢ÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ Ð¸ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð¾-ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÑÂ», 190201 Â«ÐÐ²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ðµ- Ð¸ ÑÑÐ°ÐºÑÐ¾ÑÐ¾ÑÑÑÐ¾ÐµÐ½Ð¸ÐµÂ», 190202 Â«ÐÐ½Ð¾Ð³Ð¾ÑÐµÐ»ÐµÐ²ÑÐµ Ð³ÑÑÐµÐ½Ð¸ÑÐ½ÑÐµ Ð¸ ÐºÐ¾Ð»ÐµÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½ÑÂ». ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÐ¹ Ð² Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐºÐ°Ð·Ð°Ð½Ð¸ÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð» ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¾ÑÑÐ°Ð²Ð½Ð¾Ð¹ ÑÐ°ÑÑÑÑ Ð»ÐµÐºÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÐºÑÑÑÐ° Ð¿Ð¾ Ð¿Ð¾ÑÑÐ½ÐµÐ²ÑÐ¼ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»ÑÐ¼ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ³Ð¾ ÑÐ³Ð¾ÑÐ°Ð½Ð¸Ñ (ÐÐÐ¡) Ð¸ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð´Ð°Ð½Ð½ÑÐµ, Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐµ Ð´Ð»Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÐºÑÑÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»ÐµÐ¹ (Ð²ÑÐ±Ð¾Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² Ð¸ ÑÐ°Ð·Ð¼ÐµÑÐ¾Ð² Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ Ð¸ ÑÑÑÐ±Ð¾ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÐ°, ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð¹ Ð¸ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ°ÑÑÐµÑÑ, Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐ°Ð²Ð½Ð¾Ð²ÐµÑÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ, ÑÑÐµÐ±ÑÐµÐ¼ÑÐ¹ Ð¾Ð±ÑÐµÐ¼ Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ°Ð±Ð¾Ñ). ÐÐ»Ñ Ð¶ÐµÐ»Ð°ÑÑÐ¸Ñ ÑÐ³Ð»ÑÐ±Ð¸ÑÑ ÑÐ²Ð¾Ð¸ Ð¿Ð¾Ð·Ð½Ð°Ð½Ð¸Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐµÐ¾ÑÐ¸Ð¸ Ð¸ ÑÐ°ÑÑÐµÑÐ° ÐÐÐ¡ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÑ ÑÐ²Ð¾Ð¹ ÐºÑÑÑÐ¾Ð²Ð¾Ð¹ Ð¿ÑÐ¾ÐµÐºÑ Ð¾ÑÐ¸Ð³Ð¸Ð½Ð°Ð»ÑÐ½ÑÐ¼Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ°Ð¼Ð¸ Ð¿Ð¾ ÑÐ°ÑÑÐµÑÑ ÑÐ¸ÑÑÐµÐ¼ Ð²Ð¿ÑÑÑÐºÐ° ÑÐ¾Ð¿Ð»Ð¸Ð²Ð° (Ð´Ð¸Ð·ÐµÐ»Ð¸), Ð°Ð½Ð°Ð»Ð¸Ð·Ñ Ð¿ÑÐ¾Ð¿ÑÑÐºÐ½Ð¾Ð¹ ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ ÑÐ¸ÑÑÐµÐ¼ Ð³Ð°Ð·Ð¾ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ñ Ð¿ÑÑÐµÐ¹ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð³Ð¾ ÑÐ¸ÐºÐ»Ð° Ð´Ð¸Ð·ÐµÐ»ÐµÐ¹ Ð¿ÑÐ¸ Ð¸Ð½ÑÑ, Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ð¸Ð°Ð»ÑÐ½Ð¾ Ð½Ð¾Ð²ÑÑ Ð¿ÑÑÑÑ ÐµÐ³Ð¾ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸. Ð¡Ð¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑÐ¸Ðµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð² Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¸. ÐÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ñ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÑÐ°ÑÑÐ¸Ñ ÐºÑÑÑÐ¾Ð² ÑÐ½ÐµÑÐ³Ð¾Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ¾Ð² Ð²ÑÑÑÐ¸Ñ ÑÑÐµÐ±Ð½ÑÑ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹ Ð¸ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÐµÐ¹ - ÐºÐ¾Ð½ÑÑÐ»ÑÑÐ°Ð½Ñ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 Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
The central energy source of 70micron-selected galaxies: Starburst or AGN?
Creators: name: Symeonidis, M.
name: Rosario, D.
name: Georgakakis, A.
name: Harker, J.
name: Laird, E. S.
name: Page, M. J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present the first AGN census in a sample of 61 galaxies selected at 70microns, a wavelength which should strongly favour the detection of star-forming systems. For the purpose of this study we take advantage of deep Chandra X-ray and Spitzer infrared (3.6-160micron) data, as well as optical spectroscopy and photometry from the Deep Extragalactic Evolutionary Probe 2 (DEEP2) survey for the Extended Groth Strip (EGS) field. We investigate spectral line diagnostics ([OIII]/Hbeta and [NeIII]/[OII] ratios, Hdelta Balmer absorption line equivalent widths and the strength of the 4000Ang break), X-ray luminosities and spectral energy distributions (SEDs). We find that the 70micron sources are undergoing starburst episodes and are therefore characterised by a predominance of young stars. In addition, 13 per cent of the sources show AGN signatures and hence potentially host an AGN. When the sample is split into starbursts (SBs, 10^10
description: 20 pages, 14 figures, accepted for publication in MNRAS
Arecibo Observatory: a ground and space joint effort in support of small bodies exploration
Creators: name: Venditti, Flaviane
name: Virkki, Anne
name: Marshall, Sean
name: Hickson, Dylan
name: Taylor, Patrick
name: Zambrano, Luisa
Publisher: name: Zenodo
Year: 2021

description: We present how the planetary radar program at the Arecibo Observatory (AO) works in synergy with other ground-based and space telescopes, as well as planetary mission support. The AO's S-band radar system (2.38 GHz, 1 MW) is crucial for orbit refinement and characterization of near-Earth asteroids (NEAs), providing information about shape, spin, size, surface properties, and revealing natural satellites. Radar observations rely on optical and space infrared NEA surveys, allowing for rapid post-discovery orbit refinement, which can decrease orbit uncertainty and extend the predictability window. Furthermore, missions to small bodies use radar characterization to select suitable targets, such as NASA's OSIRIS-REx to 101955 Bennu, and JAXA's Hayabusa to 25143 Itokawa. The upcoming NASA's DART mission, part of the pioneer international collaboration AIDA, will test the kinetic impact on the secondary component of the binary system Didymos in 2022, becoming the first asteroid mitigation strategy performed. AO's radar system can measure speed and distance with incomparable precision, and will be actively supporting this deflection mission for a few weeks after the impact in real time.
The Earth-Based Observational Program for Juno Mission Support
Creators: name: Orton, Glenn
name: Tabataba-Vakili, Fachreddin
name: Momary, Thomas
Publisher: name: Zenodo
Year: 2021

description: The Juno mission has promoted and coordinated a network of Earth-based observations, including both space- and ground-based facilities, to extend and enhance observations made by the Juno mission. The spectral region and timeline of all of these observations are summarized in the web site: https://www.missionjuno.swri.edu/planned-observations. The purpose of these observations is fourfold. (1) The observations complement the spectral coverage of Juno's instruments by extending the spectral coverage and resolution of its instruments. (2) They also extend the spatial coverage of Juno's instruments, which is usually extremely limited. (3) Measurements of Jupiter over time also provide a measurements of the evolution of atmospheric features and phenomena over time that Juno typically only observes once. (4) The support program also includes quasi-continuous surveys of properties not directly observed by Juno that nonetheless exert an influence over the phenomena it is observing. A summary of the results of this effort will be illustrated with specific examples.
PIERNIK mhd code - a multi-fluid, non-ideal extension of the relaxing-TVD scheme (I)
Creators: name: Hanasz, Michał
name: Kowalik, Kacper
name: Wóltański, Dominik
name: Pawłaszek, Rafał
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a new multi-fluid, grid MHD code PIERNIK, which is based on the Relaxing TVD scheme. The original scheme has been extended by an addition of dynamically independent, but interacting fluids: dust and a diffusive cosmic ray gas, described within the fluid approximation, with an option to add other fluids in an easy way. The code has been equipped with shearing-box boundary conditions, and a selfgravity module, Ohmic resistivity module, as well as other facilities which are useful in astrophysical fluid-dynamical simulations. The code is parallelized by means of the MPI library. In this paper we shortly introduce basic elements of the Relaxing TVD MHD algorithm, following Trac & Pen (2003) and Pen et al. (2003), and then focus on the conservative implementation of the shearing box model, constructed with the aid of the Masset's (2000) method. We present results of a test example of a formation of a gravitationally bounded object (planet) in a self-gravitating and differentially rotating fluid.
description: 6 pages, 3 figures, conference proceedings of the Torun Exoplanets 2008
title: ÐÐ½Ð°Ð»Ð¸Ð· Ð¿Ð¾ÑÑÐµÐ±Ð¸ÑÐµÐ»ÑÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ², ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ð° ÐºÐ°ÑÐµÑÑÐ²Ð° ÑÐµÐ»ÑÐ´Ð¸ ÑÐ¾Ð»ÐµÐ½Ð¾Ð¹ Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸ ÑÑÐ±Ð½ÑÐ¼Ð¸ ÑÐ¾Ð²Ð°ÑÐ°Ð¼Ð¸ Ð² ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð¼ ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¼ Ð¿ÑÐµÐ´Ð¿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Ð¾Ð´Ð½ÐµÐ²ÑÐºÐ°Ñ, ÐÐ¸ÑÐ°Ð»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: ÑÐµÐ»ÑÐ´Ñ ÑÐ¾Ð»ÐµÐ½Ð°Ñ
ÑÐ¸Ð·Ð¸ÐºÐ¾-Ñ Ð¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÐºÐ°ÑÐµÑÑÐ²Ð°
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ÑÑÐ±Ð½ÑÐ¹ ÑÑÐ½Ð¾Ðº Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°
ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ð° ÐºÐ°ÑÐµÑÑÐ²Ð°

description: 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¸Ð·ÑÑÐµÐ½Ð¸Ðµ ÑÐ¾Ð²Ð°ÑÐ¾Ð²ÐµÐ´Ð½Ð¾Ð¹ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ Ð¸ Ð¾ÑÐµÐ½ÐºÐ° ÐºÐ°ÑÐµÑÑÐ²Ð° ÑÐ¾Ð»ÐµÐ½Ð¾Ð¹ ÑÐµÐ»ÑÐ´Ð¸. ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐµÐ»ÑÐ´Ñ ÑÐ¾Ð»ÐµÐ½Ð°Ñ, ÑÐµÐ°Ð»Ð¸Ð·ÑÐµÐ¼Ð°Ñ Ð² ÑÐ¾Ð·Ð½Ð¸ÑÐ½ÑÑ ÑÐ¾ÑÐ³Ð¾Ð²ÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸ÑÑ Ð¡Ð°Ð½ÐºÑâÐÐµÑÐµÑÐ±ÑÑÐ³Ð°. Ð Ð¿ÐµÑÐ²Ð¾Ð¹ ÑÐ°ÑÑÐ¸ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÑÑÑÑÑ
Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ½ÑÐµ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¸, Ð¸ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ð° ÐºÐ°ÑÐµÑÑÐ²Ð° ÑÐ¾Ð»ÐµÐ½Ð¾Ð¹ ÑÐµÐ»ÑÐ´Ð¸ Ð½Ð° Ð¿ÑÐµÐ´Ð¼ÐµÑ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ñ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ð½Ð° Ð¼Ð°ÑÐºÐ¸ÑÐ¾Ð²ÐºÐµ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¾ÑÐ³Ð°Ð½Ð¾Ð»ÐµÐ¿ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸ ÑÐ¸Ð·Ð¸ÐºÐ¾-ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹
ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸ÑÐ¼ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ°. ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¹ ÑÐ°ÑÑÐ¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐ±Ð¾ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÑÐ½ÐºÐ° Ð Ð¾ÑÑÐ¸Ð¸ Ð·Ð° 2015â2017 Ð³Ð¾Ð´Ñ, Ð² ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ ÐºÐ¾ÑÐ¾ÑÐ¾Ð³Ð¾ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¾, ÑÑÐ¾ Ð¾Ð´Ð½Ð¾Ð¹ Ð¸Ð· Ð³Ð»Ð°Ð²Ð½ÑÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼ Ð¾ÑÐµÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÑÐ±Ð¾ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° ÑÐ²Ð»ÑÐµÑÑÑ Ð¾ÑÑÑÑÑÑÐ²Ð¸Ðµ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ Ð¿ÐµÑÐµÑÐ°Ð±Ð°ÑÑÐ²Ð°ÑÑÐµÐ¹ Ð±Ð°Ð·Ñ, Ð²ÑÐ»ÐµÐ´ÑÑÐ²Ð¸Ðµ ÑÐµÐ³Ð¾ Ð·Ð½Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð°Ñ ÑÐ°ÑÑÑ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ñ Ð±Ð¸Ð¾ÑÐµÑÑÑÑÐ¾Ð² Ð¾ÑÐ¿ÑÐ°Ð²Ð»ÑÐµÑÑÑ Ð·Ð° ÑÑÐ±ÐµÐ¶ Ð´Ð»Ñ Ð¿Ð¾ÑÐ»ÐµÐ´ÑÑÑÐµÐ¹ Ð¿ÐµÑÐµÑÐ°Ð±Ð¾ÑÐºÐ¸. ÐÐ´Ð½Ð¸Ð¼ Ð¸Ð· Ð²Ð°Ð¶Ð½ÐµÐ¹ÑÐ¸Ñ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¼ÐµÑ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ ÑÑÐ±Ð½Ð¾Ð¹ Ð¾ÑÑÐ°ÑÐ»Ð¸, Ð¸Ð¼ÐµÑÑÐµÐ¹ Ð·Ð½Ð°ÑÐ¸ÑÐµÐ»ÑÐ½ÑÐ¹ ÑÐºÑÐ¿Ð¾ÑÑÐ½ÑÐ¹ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð», ÑÐ²Ð»ÑÐµÑÑÑ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð¾ÑÐµÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ Ð³Ð»ÑÐ±Ð¾ÐºÐ¾Ð¹ ÑÑÐµÐ¿ÐµÐ½Ð¸ Ð¿ÐµÑÐµÑÐ°Ð±Ð¾ÑÐºÐ¸
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The Origin of Neutrino Masses and Physics Beyond the Standard Model
Creators: name: Perez, Pavel Fileviez
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We discuss the simplest models for the generation of neutrinos masses at tree level and one-loop level. The realization of the different seesaw mechanisms in the context of renormalizable SU(5) and SO(10) theories is reviewed. A new mechanism for the generation of neutrino masses at one-loop level is presented. We discuss the first realization of the Type III seesaw mechanism in the context of a renormalizable SU(5) theory, called "Adjoint SU(5)".
description: minor corrections. Plenary talk given at NuFact09, Fermilab and IIT, Chicago, July 20-25, 2009
Cutting mechanics of soft solids
Creators: name: Antarvedi Goda, Bharath
Publisher: name: University of British Columbia
Year: 2024

description: Cutting mechanics of soft solids has been of growing interest due to its promising benefits in material characterization and other industrial applications. However, a full understanding of the physical phenomena is still missing, and several questions remain outstanding. In this thesis, we explore the simple problem of wire cutting. Through finite element analysis and dimensional arguments, we obtain a simple scaling relation between the wire radius and the steady-state cutting forces. We note that, in the absence of dissipative mechanisms, steady-state cutting forces are independent of blade sharpness. However, in the presence of dissipation in the form of friction and adhesion, we show that tough materials are sensitive to friction, whereas, brittle materials are sensitive to dissipation in the form of adhesion and wear. In the regime dominated by friction, cutting forces have a weaker sensitivity to blade sharpness. But, in the regime dominated by adhesion and shear damage/ wear, we have a linear dependence between cutting force and blade sharpness. By accounting for strain-stiffening and compressibility of the soft material, we note that tough and highly strain-stiffening materials are most sensitive to frictional dissipation. Whereas, in-compressible brittle materials are most sensitive to adhesion and wear dissipation. Finally, this thesis provides important findings: Toughness can be estimated from wire-cutting experiments from the intercept of the forcewire radius linear correlation, however this only estimates cleavage toughness. In the adhesive/wear regime, a larger radius would scale the cutting fracture process zone giving rise to higher apparent toughness.
Comparison of performance between environmentally friendly and now-banned fluorinated cross-country ski wax
Creators: name: Sandberg, Joakim
name: Almqvist, Andreas
name: Kalliorinne, Kalle
name: Hindér, Gustav
name: Holmberg, Hans-Christer
name: Larsson, Roland
Publisher: name: Loughborough University
Year: 2024

description: Engineering of Sport 15 - Proceedings from the 15th International Conference on the Engineering of Sport (ISEA 2024)

In cross-country skiing the friction between the ski and snow can greatly affect the performance of the skier. One important factor influencing this friction is the wax applied to the ski base. With the recent environmental concerns surrounding fluorinated waxes, there is an increasing interest in the applicability and performance of fluor-free alternatives. This study aims to shed light on the coefficient of friction (COF) of different waxes, including the newer fluor-free alternatives, at varying conditions using a novel ski tribometer.
Physarum cinereum Pers.
Creators: name: Kluša, Julita
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Protozoa
Mycetozoa
Myxomycetes
Physarales
Physaraceae
Physarum
Physarum cinereum

description: Physarum cinereum (Batsch) Pers.,
pelēcīgā pumpurīte
- leg.&det. K.R.Kupfer, 1931; leg. E.Veinberga, 12 Aug 2021, Salaspils p., on leaves of Taraxacum officinale and zucchini in a garden, det. J.Kluša, 2021; (NMKK), very rare.
description: Published as part of Kluša, Julita, 2023, Complete Checklist Of Myxomycetes In Latvia, pp. 127-151 in Acta Biologica Universitatis Daugavpiliensis 23 (2) on pages 127-151, DOI: 10.59893/abud.23(2).002, http://zenodo.org/record/12650118
Additional file 1 of A novel inflammation-nutrition biomarker score for predicting prognosis of patients with cancer: results from a multicenter study
Creators: name: Xie, Hailun
name: Ruan, Guotian
name: Wei, Lishuang
name: Zhang, Heyang
name: Zhang, Qi
name: Ge, Yizhong
name: Lin, Shiqi
name: Song, Mengmeng
name: Zhang, Xi
name: Liu, Xiaoyue
name: Zhang, Xiaowei
name: Li, Xiangrui
name: Zhang, Kangping
name: Yang, Ming
name: Tang, Meng
name: Deng, Li
name: Shi, Hanping
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Cancer

description: Additional file 1: Table S1. The formula of inflammation and malnutrition biomarkers. Table S2. The descriptive characteristics of patients with cancer. Table S3. Cox regression analysis of systemic inflammation-related and nutrition-related markers associated with overall survival. Table S4. Logistic regression analysis of inflammation nutrition score associated with secondary outcome. Figure S1. The area under the receiver operating characteristic curve of systemic inflammation-related and nutrition-related markers. Figure S2. Pearson’s test and LASSO Cox regression model. Figure S3. The optimal threshold of systemic inflammation-related and nutrition-related markers. Figure S4. Study design. Figure S5. The proportion of tumor stages and tumor types among different INS groups. Figure S6. Kaplan-Meier curve of systemic inflammation-related and nutrition-related markers in patients with cancer. Figure S7. Stratified survival analysis of systemic inflammation-related and nutrition-related markers based on pathological stages. Figure S8. Kaplan-Meier survival curve of inflammation-malnutrition biomarker score based different tumor types and pathological stages. Figure S9. The association between systemic inflammation-related and nutrition-related markers and all-cause mortality in patients with cancer. Figure S10. The association between systemic inflammation-related and nutrition-related markers and hazard risk of overall survival in various subgroups. Figure S11. Dose-response effects of inflammatory-nutritional score based on subgroup.
title: ÐÐ¸ÑÐµÐ²Ð°Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ñ Ð¸ Ð¿ÑÐ¾Ð´Ð¾Ð²Ð¾Ð»ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ ÑÑÑÑÐµ. ÐÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ñ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ 19 ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ Ð°ÑÐ¾Ð¼Ð½Ð¾-ÑÐ¼Ð¸ÑÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¿ÐµÐºÑÑÐ¾Ð¼ÐµÑÑÐ¸Ð¸ Ñ Ð¸Ð½Ð´ÑÐºÑÐ¸Ð²Ð½Ð¾ ÑÐ²ÑÐ·Ð°Ð½Ð½Ð¾Ð¹ Ð¿Ð»Ð°Ð·Ð¼Ð¾Ð¹ ÐÐ 05-2023
Creators: name: Ð¥Ð°Ð»ÑÐ²Ð¸Ð½, Ð.
Publisher: name: Ð¤ÐÐÐ£ Â«ÐÐÐÐÐÐÂ»
Year: 2023
Subjects: Ð¡Ð¿ÐµÐºÑÑÐ¾Ð¼ÐµÑÑÐ¸Ñ
ÐÐ»Ð°Ð·Ð¼Ð° (ÑÐ¸Ð·.)
Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ñ

description: ÐÐ¾Ð²Ð¸Ð·Ð½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ñ ÐÐ 05-2023 Â«ÐÐ¸ÑÐµÐ²Ð°Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ñ Ð¸ Ð¿ÑÐ¾Ð´Ð¾Ð²Ð¾Ð»ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ ÑÑÑÑÐµ. ÐÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ñ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ 19 ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ Ð°ÑÐ¾Ð¼Ð½Ð¾-ÑÐ¼Ð¸ÑÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¿ÐµÐºÑÑÐ¾Ð¼ÐµÑÑÐ¸Ð¸ Ñ Ð¸Ð½Ð´ÑÐºÑÐ¸Ð²Ð½Ð¾ ÑÐ²ÑÐ·Ð°Ð½Ð½Ð¾Ð¹ Ð¿Ð»Ð°Ð·Ð¼Ð¾Ð¹Â» Ð·Ð°ÐºÐ»ÑÑÐ°ÐµÑÑÑ Ð² ÑÐ¾Ð¼, ÑÑÐ¾ Ð² Ð½ÐµÐ¹ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð° ÐµÐ´Ð¸Ð½Ð¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð°Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ñ Ð¼Ð°ÑÑÐ¾Ð²Ð¾Ð¹ Ð´Ð¾Ð»Ð¸ (ÐºÐ¾Ð½ÑÐµÐ½ÑÑÐ°ÑÐ¸Ð¸) 19 ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð² Ð¿Ð¸ÑÐµÐ²Ð¾Ð¼ Ð¸ Ð¿ÑÐ¾Ð´Ð¾Ð²Ð¾Ð»ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¼ ÑÑÑÑÐµ, Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ Ð°ÑÐ¾Ð¼Ð½Ð¾-ÑÐ¼Ð¸ÑÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¿ÐµÐºÑÑÐ¾Ð¼ÐµÑÑÐ¸Ð¸ Ñ Ð¸Ð½Ð´ÑÐºÑÐ¸Ð²Ð½Ð¾ ÑÐ²ÑÐ·Ð°Ð½Ð½Ð¾Ð¹ Ð¿Ð»Ð°Ð·Ð¼Ð¾Ð¹.
The calibration of the Sudbury Neutrino Observatory using uniformly distributed radioactive sources
Creators: name: Boudjemline, K.
name: Cai, B.
name: Cleveland, B. T.
name: Evans, H. C.
name: Ewan, G. T.
name: Farine, J.
name: Ford, R. J.
name: Guillian, E.
name: Hallin, A. L.
name: Hallman, E. D.
name: Howard, C.
name: Jagam, P.
name: Jelley, N. A.
name: Keeter, K. J.
name: Klein, J. R.
name: Kraus, C.
name: Krauss, C. B.
name: Lange, R.
name: Lawson, I. T.
name: Leslie, J. R.
name: Loach, J. C.
name: McDonald, A. B.
name: McGregor, G.
name: Noble, A. J.
name: O'Keeffe, H. M.
name: Peeters, S. J. M.
name: Poon, A. W. P.
name: Reitzner, S. D.
name: Rielage, K.
name: Robertson, R. G. H.
name: Rusu, V. L.
name: Seibert, S. R.
name: Skensved, P.
name: Thomson, M. J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: The production and analysis of distributed sources of 24Na and 222Rn in the Sudbury Neutrino Observatory (SNO) are described. These unique sources provided accurate calibrations of the response to neutrons, produced through photodisintegration of the deuterons in the heavy water target, and to low energy betas and gammas. The application of these sources in determining the neutron detection efficiency and response of the 3He proportional counter array, and the characteristics of background Cherenkov light from trace amounts of natural radioactivity is described.
description: 24 pages, 13 figures
title: ÐÑÑÐ¼Ð¾Ð»Ð¸Ð½ÐµÐ¹Ð½ÑÐµ ÐºÐ¾Ð»ÐµÐ±Ð°Ð½Ð¸Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐºÐ¸. Ð¢ÐµÐ¾ÑÐ¸Ñ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÐºÑÐ¼
title: ÑÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ
titleType: Subtitle
Creators: name: ÐÐ°ÑÑÐºÐ¸Ð½, Ð®ÑÐ¸Ð¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2019
Subjects: ÐÐ¸Ð½Ð°Ð¼Ð¸ÐºÐ° ÑÐ¾ÑÐºÐ¸

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¼ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð¼ ÐºÑÑÑÐµ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð», Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐ¹ Ð´Ð»Ñ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÑÐµÐ¾ÑÐ¸Ð¸ Ð¿ÑÑÐ¼Ð¾Ð»Ð¸Ð½ÐµÐ¹Ð½ÑÑ ÐºÐ¾Ð»ÐµÐ±Ð°Ð½Ð¸Ð¹ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐºÐ¸ Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð¾Ð±ÑÐµÐ³Ð¾ ÐºÑÑÑÐ° Â«Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¼ÐµÑÐ°Ð½Ð¸ÐºÐ°Â», ÑÐ¸ÑÐ°ÐµÐ¼Ð¾Ð³Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐ»ÐµÐºÑÑÐ¾Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸ ÑÐ½ÐµÑÐ³Ð¾Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¾ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ð¹ ÐÐ½ÑÑÐ¸ÑÑÑÐ° ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ¸ Ð¸ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÑ ÑÐ¸ÑÑÐµÐ¼, Ð° ÑÐ°ÐºÐ¶Ðµ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¾ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² ÐÐ½ÑÑÐ¸ÑÑÑÐ° Ð¼ÐµÑÐ°Ð»Ð»ÑÑÐ³Ð¸Ð¸, Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¸ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ°. ÐÐ°Ð»ÑÐ¹ Ð¾Ð±ÑÐµÐ¼ ÑÐ°ÑÐ¾Ð², Ð¾ÑÐ²Ð¾Ð´Ð¸Ð¼ÑÐ¹ ÑÑÐµÐ±Ð½ÑÐ¼ Ð¿Ð»Ð°Ð½Ð¾Ð¼ Ð½Ð° Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ ÑÐµÐ¾ÑÐ¸Ð¸ ÐºÐ¾Ð»ÐµÐ±Ð°Ð½Ð¸Ð¹, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐµÑ Ð²ÑÐ±Ð¾Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð° Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð¸ ÐºÐ¾Ð½ÑÐ¿ÐµÐºÑÐ¸Ð²Ð½ÑÐ¹ ÑÑÐ¸Ð»Ñ ÐµÐ³Ð¾ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ. ÐÐ° Ð±Ð°Ð·Ðµ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð° ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐ¸Ð¿Ð¾Ð²ÑÑ Ð·Ð°Ð´Ð°Ñ Ð¿Ð¾ ÑÐµÐ¾ÑÐ¸Ð¸ Ð¿ÑÑÐ¼Ð¾Ð»Ð¸Ð½ÐµÐ¹Ð½ÑÑ ÐºÐ¾Ð»ÐµÐ±Ð°Ð½Ð¸Ð¹ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐºÐ¸, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð±ÑÐ´ÑÑ Ð¿Ð¾Ð»ÐµÐ·Ð½Ñ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð² Ð¿ÐµÑÐ¸Ð¾Ð´ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ðº ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿Ð¾ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑÐµÐ¼Ñ ÑÐ°Ð·Ð´ÐµÐ»Ñ. Ð Ð·Ð°ÐºÐ»ÑÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ°ÑÑÐ¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð²Ð°ÑÐ¸Ð°Ð½ÑÑ ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ ÑÐµÐ¾ÑÐ¸Ð¸ Ð¿ÑÑÐ¼Ð¾Ð»Ð¸Ð½ÐµÐ¹Ð½ÑÑ ÐºÐ¾Ð»ÐµÐ±Ð°Ð½Ð¸Ð¹ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐºÐ¸. ÐÐ°Ð½Ð½ÑÐ¹ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐ¹ ÐºÑÑÑ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¿ÐµÑÐ²Ð¾Ð³Ð¾ Ð¸ Ð²ÑÐ¾ÑÐ¾Ð³Ð¾ ÐºÑÑÑÐ° Ð¾ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ð¹ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾-ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐ¸Ð»Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÐµÐ¹, Ð²ÐµÐ´ÑÑÐ¸Ñ ÑÐ¿ÑÐ°Ð¶Ð½ÐµÐ½Ð¸Ñ Ð² Ð³ÑÑÐ¿Ð¿Ð°Ñ.
Deterministic Minimax Impulse Control in Finite Horizon: the Viscosity Solution Approach
Creators: name: Asri, Brahim El
Publisher: name: arXiv
Year: 2010
Subjects: subject: Optimization and Control (math.OC)
subject: FOS: Mathematics

description: We study here the impulse control minimax problem. We allow the cost functionals and dynamics to be unbounded and hence the value functions can possibly be unbounded. We prove that the value function of the problem is continuous. Moreover, the value function is characterized as the unique viscosity solution of an Isaacs quasi-variational inequality. This problem is in relation with an application in mathematical finance.
title: Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¼ÐµÑ Ð°Ð½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð´ÐµÑ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°ÐºÑÐ¸Ð¼Ð¾Ð²Ð°, ÐÐ°Ð»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: 2016
Subjects: ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ
ÑÑÐ°Ð½Ð¾Ðº
ÑÐµÐ¶Ð¸Ð¼Ñ ÑÐµÐ·Ð°Ð½Ð¸Ñ
technological process
machine
cutting conditions

description: Ð Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¼ Ð¿ÑÐ¾ÐµÐºÑÐµ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð¾ Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¸Ðµ Ð´ÐµÑÐ°Ð»Ð¸ Â«ÐÐ°Ð»Â», Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð¸ ÑÑÐ»Ð¾Ð²Ð¸Ñ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¸. Ð¡ÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÐµÐ»Ð¸ Ð¸ Ð·Ð°Ð´Ð°ÑÐ¸, ÑÑÐµÐ±ÑÑÑÐ¸Ðµ ÑÐµÑÐµÐ½Ð¸Ñ Ð² Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¼ Ð¿ÑÐ¾ÐµÐºÑÐµ. ÐÑÐ±ÑÐ°Ð½ Ð¸ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½ ÑÐ¿Ð¾ÑÐ¾Ð± Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ Ð¸ÑÑÐ¾Ð´Ð½Ð¾Ð¹ Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸, Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ, ÑÐµÐ¶ÑÑÐ¸Ð¹ Ð¸ ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½Ð¾-Ð¸Ð·Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½Ñ. ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð´ÐµÑÐ°Ð»Ð¸. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ñ ÑÐµÐ¶Ð¸Ð¼Ñ ÑÐµÐ·Ð°Ð½Ð¸Ñ Ð¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð½Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ°Ð±Ð¾Ñ. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ñ Ð¸ ÑÐ¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÐµ ÑÑÐ°Ð½Ð¾ÑÐ½ÑÐµ Ð¸ ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½Ð¾-Ð¸Ð·Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ðµ Ð¿ÑÐ¸ÑÐ¿Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð¸Ñ.
description: The thesis project analyzed the details of the appointment of "Shaft ", a description of the design and operating conditions. The aims and objectives to be addressed in the thesis project. Selected and validated a method for producing the original blank, equipment, cutting, control and measuring tool. A process of machining parts. Cutting conditions are calculated and carried out the valuation process works. Designed and engineered a special machine tools and test and measurement devices.
Long Covid in Workers: main risk factors, clinical management, and management of work processes
Creators: name: Da Silva, Paola Falceta
name: Victorino, Fernando Albuquerque
name: Santos, Daniel Valente Soares Dos
name: De Cássia Oliveira Da Costa Mattos, Rita
name: Hermano Castro Albuquerque
name: Isabele Campos Costa Amaral
name: Cavalcante, Ana Luiza Michel
name: Corrêa, Maria Juliana Moura
name: Teixeira, Liliane
name: Gilvania Barreto Feitosa Coutinho
name: Silveira, Martha Silvia Martinez
name: Talita Monsores Paixão
name: Fonseca, Antonio Sergio Almeida
name: Thamiris Luiza Machado De Carvalho
name: Santos, Marcus Vinicius Corrêa Dos
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Public Health
subject: Medicine and Health Sciences
subject: Occupational Health and Industrial Hygiene
subject: prolonged symptom COVID
subject: Occupational Health
subject: Post-COVID syndrome
subject: Post-COVID Condition
subject: Long COVID
subject: Post-Acute COVID Syndrome
subject: long-term COVID
subject: Post-Coronavirus Disease
subject: Post-Acute COVID
subject: Sequelae SARS-CoV-2
subject: Sequelae COVID

description: This is a scope review protocol on Long Covid in Workers. The review question is: "What are the main risk factors, clinical management, and management of workers affected by Long Covid?”.
title: Ð¤Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÐºÑÐ»ÑÑÑÑÑ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐ´Ð° ÐºÐ°Ðº ÑÐ°ÑÑÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÐºÑÐ»ÑÑÑÑÑ Ð¸ ÐºÐ°Ð´ÑÐ¾Ð²Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð² Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸ÑÑ , Ð¿Ð¾Ð´Ð²ÐµÐ´Ð¾Ð¼ÑÑÐ²ÐµÐ½Ð½ÑÑ ÐÐ¸Ð½Ð¾Ð±ÑÐ½Ð°ÑÐºÐ¸ Ð Ð¾ÑÑÐ¸Ð¸
title: ÑÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐ¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² 20.04.01 Â«Ð¢ÐµÑ Ð½Ð¾ÑÑÐµÑÐ½Ð°Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑÂ»
titleType: Subtitle
Creators: name: Ð¤ÐµÐ´Ð¾ÑÐ¾Ð²Ð°, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
name: ÐÐ¸Ð»ÑÐºÐµÐ½, ÐÐ¸ÐºÑÐ¾ÑÐ¸Ñ
name: ÐÐ°ÑÐ°Ð½Ð¸Ð½, ÐÐ¼Ð¸ÑÑÐ¸Ð¹
name: ÐÐ°Ð±ÐºÐ¸Ð½, ÐÐ²Ð°Ð½
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2023
Subjects: ÐÑ ÑÐ°Ð½Ð° ÑÑÑÐ´Ð°

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¿Ð¾ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÑÐ»ÑÑÑÑÑ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐ´Ð° Ð² Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸ÑÑ, Ð¿Ð¾Ð´Ð²ÐµÐ´Ð¾Ð¼ÑÑÐ²ÐµÐ½Ð½ÑÑ ÐÐ¸Ð½Ð¾Ð±ÑÐ½Ð°ÑÐºÐ¸ Ð Ð¾ÑÑÐ¸Ð¸. Ð Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ð¹ ÑÐ°ÑÑÐ¸ ÑÐ°ÑÐºÑÑÐ²Ð°ÐµÑÑÑ Ð±Ð°Ð·Ð¾Ð²Ð°Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð»Ð¾Ð³Ð¸Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÑÐ¸Ð²ÐµÑÐ¶ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐµÐ½Ð½Ð¾ÑÑÐ¸ Â«Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½ÑÐ¹ ÑÑÑÐ´Â» ÐºÐ°Ðº Ð¾Ð´Ð½Ð¾Ð¹ Ð¸Ð· Ð²Ð°Ð¶Ð½ÐµÐ¹ÑÐ¸Ñ ÑÐµÐ½Ð½Ð¾ÑÑÐµÐ¹ Ð»ÑÐ±Ð¾Ð¹ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ. ÐÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ Ð¼ÐµÑÐ¾Ð´Ñ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÑÐ¾Ð²Ð½Ñ ÐºÑÐ»ÑÑÑÑÑ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐ´Ð°, ÑÐ¾ÑÐ¼Ñ Ð¸ ÑÐ°Ð±Ð»Ð¾Ð½Ñ Ð´Ð»Ñ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾ÑÐµÐ½ÐºÐ¸. Ð£ÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ°Ð¼Ð¸ ÑÐ»ÑÐ¶Ð± Ð¾ÑÑÐ°Ð½Ñ ÑÑÑÐ´Ð° Ð¸ ÑÑÐºÐ¾Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ¼Ð¸ Ð²ÑÐµÑ ÑÑÐ¾Ð²Ð½ÐµÐ¹ Ð² Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸ÑÑ, Ð¿Ð¾Ð´Ð²ÐµÐ´Ð¾Ð¼ÑÑÐ²ÐµÐ½Ð½ÑÑ ÐÐ¸Ð½Ð¾Ð±ÑÐ½Ð°ÑÐºÐ¸ Ð Ð¾ÑÑÐ¸Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐ¾ÑÐµÑÑÐ¾ÑÑÐºÐ¾-Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¸Ð¼ ÑÐ¾ÑÑÐ°Ð²Ð¾Ð¼ Ð¸ Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ð¼Ð¸ÑÑ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸, ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÑ Ñ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸ÐµÐ¼ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¸ Ð¾ÑÑÐ°Ð½Ñ ÑÑÑÐ´Ð°.