cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Glomeris mohamedanica Attems 1900
Creators: name: Golovatch, Sergei
name: Mauriès, Jean-Paul
name: Akkari, Nesrine
name: Stoev, Pavel
name: Geoffroy, Jean-Jacques
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Diplopoda
Glomerida
Glomeridae
Glomeris
Glomeris mohamedanica

description: Glomeris mohamedanica Attems, 1900 Figs 24, 25 Glomeris europaea striata var. mohamedanica Attems, 1900: 303 (D). Glomeris mohamedanica – Schubart 1953: 218 (L). Type material: Tunisia, Béja Gov., Medjez El Bab (now Mejez El Bab), date?, leg.?, ♁ lectotype (here designated) (NHMW 3913), paralectotypes: 3 ♁, 2 ♀ (NHMW 3913), 1 ♁ (MNHN CC 153). The designation of a lectotype (from 350 syntypes, see Attems 1900) seems advisable in order to ensure that the name-bearing type shows the diagnostically important characteristics of the male sex. Other material: Tunisia, Béja Gov., Nefza (30 km of Béja), 2003, leg. N. Akkari, 1 ♁, 1 ♀ (MNHN CC 153). Same locality, 36°57′61″N, 8°56′51″E, open area with scattered vegetation, under stones, 27.II.2004, leg. N. Akkari, 3 ♁, 5 ♀, 3 juv. (MNHN CC 153). Same locality, 2.X.2005, leg. N. Akkari, 1 ♁, 3 ♀ (NMNH). Tunisia, Jen- douba Gov., Beni Mtir (8 km S of Aïn Draham), mixed oak forest dominated by Quercus suber, slope, under stones, 19.II.2007, leg. N. Akkari, 10 ♁ (MNHN CC 153), 3 ♁ (ZMUM), 2 ♁ (NMNH), 2 # (FMNH). Same locality, alt. approx. 500 m, 19.II.2007, leg. N. Akkari, 2 ♁, 2 ♀ (ZMUC 200113). Tunisia, Jendouba Gov., Tabarka, 10.XII.2003, leg. N. Akkari, 1 ♀ (FMNH). Tunisia, Jendouba Gov., 40 km of Jendouba, near frontier, 17.V.1988, leg. Z. M. Cop. Exp., 2 M (ZMUC 200108). Short description: Length up to 12 mm, width up to 6.0 mm. Coloration dark brown to blackish, with contrasting yellow bands, pattern as in Figs 24A, B. ♁ legs 17, 18 and 19 (telopods) as in Figs 25 A-D. Remarks: This species is unusual among the presumably native North African Glomeris in belonging to the “ Eurypleuromeris ” type.
description: Published as part of Golovatch, Sergei, Mauriès, Jean-Paul, Akkari, Nesrine, Stoev, Pavel & Geoffroy, Jean-Jacques, 2009, The millipede genus Glomeris Latreille, 1802 (Diplopoda, Glomerida, Glomeridae) in North Africa, pp. 47-86 in ZooKeys 12 (12) on pages 75-76, DOI: 10.3897/zookeys.12.179, http://zenodo.org/record/576461
description: {"references": ["Attems C (1900) Uber die Farbung von Glomeris und Beschreibung neuer oder wenig gekannter palaearktischer Myriopoden. Archiv fur Naturgeschichte 66 (1, 3): 297 - 320.", "Schubart O (1953) Diplopoden aus Marokko, gesammelt vom Institut Scientifique Cherifien. Bulletin de la Societe des Sciences Naturelles du Maroc 32 (1): 199 - 225 (for 1952)."]}
Voli spaziali: attenti al sistema immunitario
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2015

Un gruppo di ricercatori ha dimostrato che  il volo spaziale potrebbe essere una delle cause di invecchiamento accelerato del sistema immunitario del corpo degli astronauti. Gli esperimenti sono stati effettuati tutti nei laboratori sulla Terra utilizzando la tecnica dell'hindlimb unloaded (HU)
The Diversity of Massive Star Outbursts I: Observations of SN 2009ip, UGC 2773 OT2009-1, and Their Progenitors
Creators: name: Foley, Ryan J.
name: Berger, Edo
name: Fox, Ori
name: Levesque, Emily M.
name: Challis, Peter J.
name: Ivans, Inese I.
name: Rhoads, James E.
name: Soderberg, Alicia M.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Despite both being outbursts of luminous blue variables (LBVs), SN 2009ip and UGC 2773 OT2009-1 have very different progenitors, spectra, circumstellar environments, and possibly physical mechanisms that generated the outbursts. From pre-eruption HST images, we determine that SN 2009ip and UGC 2773 OT2009-1 have initial masses of >60 and >25 M_sun, respectively. Optical spectroscopy shows that at peak SN 2009ip had a 10,000 K photosphere and its spectrum was dominated by narrow H Balmer emission, similar to classical LBV giant outbursts, also known as "supernova impostors." The spectra of UGC 2773 OT2009-1, which also have narrow H alpha emission, are dominated by a forest of absorption lines, similar to an F-type supergiant. Blueshifted absorption lines corresponding to ejecta at a velocity of 2000 - 7000 km/s are present in later spectra of SN 2009ip -- an unprecedented observation for LBV outbursts, indicating that the event was the result of a supersonic explosion, rather than a subsonic outburst. The velocity of the absorption lines increases between two epochs, suggesting that there were two explosions in rapid succession. A rapid fading and rebrightening event concurrent with the onset of the high-velocity absorption lines is consistent with the double-explosion model. A near-infrared excess is present in the spectra and photometry of UGC 2773 OT2009-1 that is consistent with ~2100 K dust emission. We compare the properties of these two events and place them in the context of other known massive star outbursts such as eta Car, NGC 300 OT2008-1, and SN 2008S. This qualitative analysis suggests that massive star outbursts have many physical differences which can manifest as the different observables seen in these two interesting objects.
description: 14 pages, 9 figures, submitted to ApJ
Schreier rewriting beyond the classical setting
Creators: name: Bahturin, Yuri
name: Olshanskii, Alexander
Publisher: name: arXiv
Year: 2008
Subjects: subject: Rings and Algebras (math.RA)
subject: Group Theory (math.GR)
subject: FOS: Mathematics
subject: 16D40;16P90;16S10;20E05;20M30

description: Using actions of free monoids and free associative algebras, we establish some Schreier-type formulas involving the ranks of actions and the ranks of subactions in free actions or Grassmann-type relations for the ranks of intersections of subactions of free actions. The coset action of the free group is used to establish the generalization of the Schreier formula to the case of subgroups of infinite index. We also study and apply large modules over free associative algebras in the spirit of the paper Olshanskii, A. Yu.; Osin, D.V., Large groups and their periodic quotients, Proc. Amer. Math. Soc., 136 (2008), 753 - 759.
description: 17 pages
The Saturation Limit of the Magnetorotational Instability
Creators: name: Vishniac, Ethan T.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Simulations of the magnetorotational instability (MRI) in a homogeneous shearing box have shown that the asymptotic strength of the magnetic field declines steeply with increasing resolution. Here I model the MRI driven dynamo as a large scale dynamo driven by the vertical magnetic helicity flux. This growth is balanced by large scale mixing driven by a secondary instability. The saturated magnetic energy density depends almost linearly on the vertical height of the typical eddies. The MRI can drive eddies with arbitrarily large vertical wavenumber, so the eddy thickness is either set by diffusive effects, by the magnetic tension of a large scale vertical field component, or by magnetic buoyancy effects. In homogeneous, zero magnetic flux, simulations only the first effect applies and the saturated limit of the dynamo is determined by explicit or numerical diffusion. The exact result depends on the numerical details, but is consistent with previous work, including the claim that the saturated field energy scales as the gas pressure to the one quarter power (which we interpret as an artifact of numerical dissipation). The magnetic energy density in a homogeneous shearing box will tend to zero as the resolution of the simulation increases, but this has no consequences for the dynamo or for angular momentum transport in real accretion disks. The claim that the saturated state depends on the magnetic Prandtl number may also be an artifact of simulations in which microphysical transport coefficients set the MRI eddy thickness. Finally, the efficiency of the MRI dynamo is a function of the ratio of the Alfvén velocity to the product of the pressure scale height and the local shear. As this approaches unity from below the dynamo reaches maximum efficiency.
description: Accepted by The Astrophysical Journal
On the extension of the mean curvature flow
Creators: name: Le, Nam Q.
name: Sesum, Natasa
Publisher: name: arXiv
Year: 2009
Subjects: subject: Differential Geometry (math.DG)
subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics

description: Consider a family of smooth immersions $F(\cdot,t): M^n\to \mathbb{R}^{n+1}$ of closed hypersurfaces in $\mathbb{R}^{n+1}$ moving by the mean curvature flow $\frac{\partial F(p,t)}{\partial t} = -H(p,t)\cdot ν(p,t)$, for $t\in [0,T)$. In \cite{Cooper} Cooper has recently proved that the mean curvature blows up at the singular time $T$. We show that if the second fundamental form stays bounded from below all the way to $T$, then the scaling invariant mean curvature integral bound is enough to extend the flow past time $T$, and this integral bound is optimal in some sense explained below.
description: 21 pages, presented self-contained proof of the main theorem
Decoding the Origin of Dark Matter
Creators: name: Liu, Zuowei
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We discuss the interplay between LHC signatures and the mechanism by which dark matter is generated in the early universe in supersymmetric theories. The LHC signatures of two of the major mechanisms for such generation of dark matter which are known to be the Stau Coannihilation (Stau-Co) region and annihilation on the Hyperbolic Branch (HB) are exhibited in detail. By analyzing the various LHC signatures, including multi leptons, hadronic jets, b-tagging, and missing transverse momentum, one can discriminate between the Stau-Co region and the HB region for the mSUGRA model. Interestingly, there are some regions of the parameter space which are beyond the current and near future reach of the dark matter direct detection experiments but will be accessible at the LHC, and vise versa.
description: 4 pages, 5 figures, based on a talk presented at SUSY 09; Boston, 5-10 June, 2009
title: Effect of Deposition from Static Test Fires on Corn and Alfalfa
Creators: name: Mendenhall, Scout
Publisher: name: Utah State University
Year: 2013

description: A greenhouse study was conducted to determine the effects of deposition from static rocket test fires on corn and alfalfa. Seeds were germinated in a wide concentration range of depositional material, called test fire soil (TFS). Additionally, the impact of chloride and aluminum, two major components of test fire soil, on germination was also evaluated. Furthermore, plants were grown in packed columns and exposed to test fire soil, either in the root zone or on foliage. Tissue was weighed and analyzed to compare biomass production and plant composition.
Corn and alfalfa exposed to test fire soil in the root zone produced less biomass than controls, but foliar treatment had no effect on biomass production. No kernels were produced by corn exposed to test fire soil in the root zone. Leaves of plants exposed to test fire soil in the root zone accumulated more metals and nutrients than controls, whereas plant tissue treated with test fire soil on the leaves contained only elevated levels of aluminum, although levels were still within reasonable concentrations for plants.
Germination of seeds was not affected below 1% test fire soil in soil; however higher concentrations of test fire soil decreased percent germination. Addition of chloride to soil also inhibits germination, but addition of aluminum has no effect on germination percentage. Corn germination was restored in test fire soil leached with 200 mm artificial rainwater.
The results of this research contribute information regarding the potential impact of test fire soil from static test fires on crop production. Test fire soil inhibits germination and growth if deposited in the root zone, and even foliar application alters tissue composition. However, plant composition is not altered significantly in terms of feed criteria, and germination can be restored by irrigating the TFS. The effects of test fire soil are attributed to high levels of chloride that induce salt stress. Crop damage may be avoided by conducting static test fires after crops are harvested or providing extra irrigation to soil impacted with the TFS.
Implementation of one-dimensional quantum walks on spin-orbital angular momentum space of photons
Creators: name: Zhang, Pei
name: Liu, Bi-Heng
name: Liu, Rui-Feng
name: Li, Hong-Rong
name: Li, Fu-Li
name: Guo, Guang-Can
Publisher: name: arXiv
Year: 2010
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Photons can carry spin angular momentum (SAM) and orbital angular momentum (OAM), which can be used to realize a qubit system and a high-dimension system respectively. This spin-orbital system is very suitable for implementing one-dimensional discrete-time quantum random walks. We propose a simple scheme of quantum walks on the spin-orbital angular momentum space of photons, where photons walk on the infinity OAM space controlled by their SAM. By employing the recent invention of an optical device, the so-called 'q-plate', our scheme is more simple and efficient than others because there is no Mach-Zehnder interferometer in the scheme.
description: 5 pages, 1 figure
Glomeris punica Attems 1900
Creators: name: Golovatch, Sergei
name: Mauriès, Jean-Paul
name: Akkari, Nesrine
name: Stoev, Pavel
name: Geoffroy, Jean-Jacques
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Diplopoda
Glomerida
Glomeridae
Glomeris
Glomeris punica

description: Glomeris punica Attems, 1900 Figs 26-28 Glomeris europaea striata var. punica Attems, 1900: 302 (D). Glomeris connexa var. punica – Attems 1908: 105 (F). Glomeris connexa punica – Brolemann 1921: 100 (L).
description: Published as part of Golovatch, Sergei, Mauriès, Jean-Paul, Akkari, Nesrine, Stoev, Pavel & Geoffroy, Jean-Jacques, 2009, The millipede genus Glomeris Latreille, 1802 (Diplopoda, Glomerida, Glomeridae) in North Africa, pp. 47-86 in ZooKeys 12 (12) on page 76, DOI: 10.3897/zookeys.12.179, http://zenodo.org/record/576461
description: {"references": ["Attems C (1900) Uber die Farbung von Glomeris und Beschreibung neuer oder wenig gekannter palaearktischer Myriopoden. Archiv fur Naturgeschichte 66 (1, 3): 297 - 320.", "Attems C (1908) Note sur les Myriapodes recueillis par M. Henri Gadeau de Kerville en Khroumirie et description de deux especes et d'une variete nouvelles provenant de cette region de la Tunisie. In: Gadeau de Kerville H (Ed) Voyage zoologique en Khroumirie (Tunisie). Rouen 1906, 103 - 116.", "Brolemann HW (1921) Liste des Myriapodes signales dans le nord de l'Afrique. Bulletin de la Societe des Sciences Naturelles du Maroc 1 (3 - 6): 99 - 110."]}
NASA, ecco il piano di spesa per il 2016
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2015

Presentato ieri dall’amministrazione Obama, il budget che la NASA sottopone al Congresso per il prossimo anno prevede finanziamenti per 18.5 miliardi di dollari, 5.3 dei quali destinati a programmi scientifici. In calendario anche una missione robotica verso Europa, la luna di Giove
Radial Fourier multipliers in high dimensions
Creators: name: Heo, Yaryong
name: Nazarov, Fedor
name: Seeger, Andreas
Publisher: name: arXiv
Year: 2009
Subjects: subject: Classical Analysis and ODEs (math.CA)
subject: FOS: Mathematics
subject: 42B15

description: Given a fixed $p\neq 2$, we prove a simple and effective characterization of all radial multipliers of $\cF L^p(\Bbb R^d)$, provided that the dimension $d$ is sufficiently large. The method also yields new $L^q$ space-time regularity results for solutions of the wave equation in high dimensions.
description: Some changes in the last section
Gravitational strings. Do we see one?
Creators: name: Krasnikov, S. V.
Publisher: name: arXiv
Year: 2008
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: I present a class of objects called gravitational strings (GS) for their similarity to the conventional cosmic strings: even though the former are just singularities in flat spacetime, both varieties are equally "realistic", they may play equally important cosmological rôle and their lensing properties are akin. I argue that the enigmatic object CSL-1 is an evidence in favor of the existence of GS.
description: The published version. Minor corrections
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Year: 2018
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title: ÐÑÐ½Ð¾Ð²Ñ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð². ÐÐ¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¼Ð¾Ð´ÐµÐ»Ð¸. ÐÐ¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾Ð´Ð½Ð¾Ð¿ÐµÑÐ¸Ð¾Ð´Ð½ÑÐµ Ð¼Ð¾Ð´ÐµÐ»Ð¸
title: Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¿Ð¾ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ°ÐµÐ², ÐÐ»ÐµÐºÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
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title: Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð²ÑÐ³Ð¸Ð½Ð°, Ð®Ð»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: 2016
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description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÑÐµÑÐ° Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð·Ð°ÑÑÐ°Ñ Ð½Ð° Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾. Ð ÑÐ°ÐºÐ¶Ðµ Ð±ÑÐ» Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½ ÑÑÐµÑ Ð·Ð°ÑÑÐ°Ñ Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð·Ð°ÑÑÐ°Ñ Ð½Ð° Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾ Ð² ÐÐÐ Â«ÐÑÐ°ÑÐ½ÑÐ¹ ÐÐºÑÑÐ±ÑÑ - ÐÐµÐ²Ð°Â». Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð·Ð°ÑÑÐ°ÑÐ°Ð¼Ð¸ Ð² ÑÐµÐ»ÑÑ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ñ Ð¿ÑÐ¸ÐµÐ¼Ð»ÐµÐ¼Ð¾Ð¹ ÑÑÑÑÐºÑÑÑÑ, ÑÐ°ÐºÐ¶Ðµ Ð¿Ð¾Ð½Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð¸Ñ Ð²ÐµÐ»Ð¸ÑÐ¸Ð½Ñ (Ð¿ÑÐ¸ ÑÑÐ»Ð¾Ð²Ð¸Ð¸ ÑÐ¾ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð²ÑÐ¿ÑÑÐºÐ°ÐµÐ¼Ð¾Ð¹ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸) Ð´Ð°ÐµÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ ÑÐ½Ð¸Ð·Ð¸ÑÑ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ Ð½Ð° Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ñ, ÑÑÐ¾ Ð¿ÑÐ¸ Ð¾ÑÑÐ°Ð»ÑÐ½ÑÑ ÑÐ°Ð²Ð½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð´Ð°ÐµÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ ÑÐ¾ÑÑÐ°Ð½Ð¸ÑÑ Ð¸Ð»Ð¸ Ð¶Ðµ Ð² ÑÐ¾Ð¼ ÑÐ¸ÑÐ»Ðµ Ð¸ Ð·Ð°ÐºÑÐµÐ¿Ð¸ÑÑ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¸ Ð½Ð° ÑÑÐ½ÐºÐµ.
Johann Caspar Rudolph Hasert: verwischte Spuren eines altlutherischen Konvertiten
Creators: name: Kelter, Gert
Publisher: name: Lutherische Beiträge
Year: 1970

description: Lutherische Beiträge, Bd. 15 Nr. 4 (2010): Lutherische Beiträge, Band 15, Heft 4
Origin and Phenomenology of Weak-Doublet Spin-1 Bosons
Creators: name: Chizhov, M. V.
name: Dvali, Gia
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study phenomenological consequences of the Standard Model extension by the new spin-1 fields with the internal quantum numbers of the electroweak Higgs doublets. We show, that there are at least three different classes of theories, all motivated by the hierarchy problem, which predict appearance of such vector weak-doublets not far from the weak scale. The common feature for all the models is the existence of an SU(3) gauge extension of the weak SU(2) group, which is broken down to the latter at some energy scale around TeV. The Higgs doublet then emerges as either a pseudo-Nambu-Goldstone boson of a global remnant of SU(3), or as a symmetry partner of the true eaten-up Goldstone boson. In the third class, the Higgs is a scalar component of a high-dimensional SU(3) gauge field. The common phenomenological feature of these theories is the existence of the electroweak doublet vectors (Z*,W*), which in contrast to well-known Z' and W' bosons posses only anomalous (magnetic moment type) couplings with ordinary light fermions. This fact leads to some unique signatures for their detection at the hadron colliders.
description: 7 pages, 5 figures
title: Ð ÐµÑÐµÐ½Ð¸Ðµ Ð¿Ð¾Ð»Ð¸Ð½Ð¾Ð¼Ð¸Ð°Ð»ÑÐ½ÑÑ Ð¸ ÑÑÐ°Ð½ÑÑÐµÐ½Ð´ÐµÐ½ÑÐ½ÑÑ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ð¹, ÑÐ¸ÑÑÐµÐ¼ Ð»Ð¸Ð½ÐµÐ¹Ð½ÑÑ Ð¸ Ð½ÐµÐ»Ð¸Ð½ÐµÐ¹Ð½ÑÑ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ÑÑÐµÐ´ÑÑÐ²Ð¾Ð¼ ÑÑÐ½ÐºÑÐ¸Ð¹ ÐÐ°ÑÐ»Ð°Ð±Ð° Ð¸ ÑÐ¾Ð·Ð´Ð°Ð½Ð½ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÑ ÑÐµÑÐ°ÑÐµÐ»ÐµÐ¹ Ð½Ð° Ð¸Ñ Ð¾ÑÐ½Ð¾Ð²Ðµ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿Ð¾ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÐ¼ ÑÐ°Ð±Ð¾ÑÐ°Ð¼
titleType: Subtitle
Creators: name: Ð ÑÐºÐ¸Ð½, ÐÐ»ÐµÐ³
name: ÐÑÐºÐ¸ÑÐµÐ², ÐÐ½Ð´ÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2013
Subjects: ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½ÑÐµ
ÐÐ»Ð³ÐµÐ±ÑÐ°Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ
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ÐÐ¸Ð½ÐµÐ¹Ð½ÑÐµ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ
ÐÐµÐ»Ð¸Ð½ÐµÐ¹Ð½ÑÐµ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ
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description: Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð´Ð°Ð½Ð¾ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ ÑÑÐ½ÐºÑÐ¸Ð¹ ÐÐ°ÑÐ»Ð°Ð±Ð° Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÑ ÑÐµÑÐ°ÑÐµÐ»ÐµÐ¹ Ð½Ð° Ð¸Ñ Ð¾ÑÐ½Ð¾Ð²Ðµ: roots(â¦) Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð¿Ð¾Ð»Ð¸Ð½Ð¾Ð¼Ð¸Ð°Ð»ÑÐ½ÑÑ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ð¹, fzero(â¦) Ð´Ð»Ñ Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ñ Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð»Ð¾ÐºÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÑÐ°Ð½ÑÑÐµÐ½Ð´ÐµÐ½ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ, Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ ÑÐµÑÐ°ÑÐµÐ»Ñ VichVesÑhKorFx (Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ fzero) Ð´Ð»Ñ Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ñ Ð²ÑÐµÑ Ð²ÐµÑÐµÑÑÐ²ÐµÐ½Ð½ÑÑ ÐºÐ¾ÑÐ½ÐµÐ¹ Ð² Ð·Ð°Ð´Ð°Ð½Ð½Ð¾Ð¼ Ð´Ð¸Ð°Ð¿Ð°Ð·Ð¾Ð½Ðµ Ð½ÐµÐ¸Ð·Ð²ÐµÑÑÐ½Ð¾Ð¹, ÑÑÐ½ÐºÑÐ¸Ð¸ linsolve(â¦) Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼ Ð»Ð¸Ð½ÐµÐ¹Ð½ÑÑ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ð¹, ÑÑÐ½ÐºÑÐ¸Ð¸ fsolve(â¦) Ð´Ð»Ñ Ð½Ð°ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ Ð¾Ð´Ð½Ð¾Ð³Ð¾ ÑÐ¸ÑÑÐµÐ¼Ð½Ð¾Ð³Ð¾ ÐºÐ¾ÑÐ½Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð½ÐµÐ»Ð¸Ð½ÐµÐ¹Ð½ÑÑ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ Ð·Ð°Ð´Ð°Ð½Ð½Ð¾Ð¼Ñ Ð½Ð°ÑÐ°Ð»ÑÐ½Ð¾Ð¼Ñ Ð¿ÑÐ¸Ð±Ð»Ð¸Ð¶ÐµÐ½Ð¸Ñ, Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ ÑÐµÑÐ°ÑÐµÐ»Ñ FsolveSLuScX0 (Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ fsolve) Ð´Ð»Ñ Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ñ Ð²ÑÐµÑ ÑÐ¸ÑÑÐµÐ¼Ð½ÑÑ ÐºÐ¾ÑÐ½ÐµÐ¹ Ð² Ð·Ð°Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð½ÐµÐ¸Ð·Ð²ÐµÑÑÐ½ÑÑ Ð½ÐµÐ»Ð¸Ð½ÐµÐ¹Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ð¹, ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»Ñ ÐºÐ¾ÑÐ½ÐµÐ¹ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ð¹ RasprUrKrSys Ð¸Ð· ÑÐ¿Ð¸ÑÐºÐ¾Ð² ÑÐµÑÐ°ÑÐµÐ»Ñ FsolveSLuScX0 Ð¿Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸ÑÐ¼ Ð¸ Ð½ÐµÐ¸Ð·Ð²ÐµÑÑÐ½ÑÐ¼ ÑÐ¸ÑÑÐµÐ¼Ñ Ð°Ð»Ð³ÐµÐ±ÑÐ°Ð¸ÑÐµÑÐºÐ¸Ñ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ð¹ Ñ ÑÐ°Ð·Ð´ÐµÐ»ÑÑÑÐ¸Ð¼Ð¸ÑÑ ÐºÐ¾ÑÐ½ÑÐ¼Ð¸. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ, Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¸ ÑÐ¿Ð¾ÑÐ¾Ð± Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ 5 Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð² ÑÑÐµÐ±Ð½ÑÑ Ð³ÑÑÐ¿Ð¿Ð°Ñ Ð² ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ð¼ ÐºÐ»Ð°ÑÑÐµ Ñ ÑÐ¸ÑÐ»Ð¾Ð¼ Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ¾Ð² Ð¾Ñ 52 Ð´Ð¾ 80. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¸ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 27.03.05 ÐÐ½Ð½Ð¾Ð²Ð°ÑÐ¸ÐºÐ° Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ð°Ð¼ Â«Ð¡Ð¸ÑÑÐµÐ¼Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ðµ ÑÐµÑÐµÐ½Ð¸Ð¹Â» Ð¸ Â«Ð¢ÐµÐ¾ÑÐ¸Ñ Ð¸ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÂ».
A comparitve study between the degree of assimilation and the self image.
Creators: name: Adams, Margaret Belle (Baxter)
Publisher: name: University of British Columbia
Year: 2012

description: This thesis investigates the relationship between the self image and the degree of assimilation in children. There are two parts to the hypothesis: firstly, there are self image characteristics which are common to members of one national group that distinguish them from members of other national groups, and secondly, these distinguishing characteristics decrease as the members of one national group become assimilated with another national group. The hypothesis was tested in the Vancouver shool system. An interviewing program was undertaken with three matched groups of school children: German immigrants, settled Canadians, and migrant Canadians. The purpose of the first two groups was to form a basis on which to compare the self images of children who were well assimilated and children who were poorly assimilated. The main function of the third group was to provide a basis on which to distinguish any self image characteristics which may be common to all children who are 'uprooted' and not only to children who immigrate to another country. If such characteristics were found they could not be regarded as distinguishing characteristics of any one national group. The self images of the Canadian and German children were found to differ in their social and institutional identification. The poorly assimilated German children identified mainly within the home and family; while the Canadian children identified within many additional institutions and people. As the German children became better assimilated their identification broadened. Therefore, a limited amount of evidence was found to support both parts of the hypothesis.
The locally covariant Dirac field
Creators: name: Sanders, Ko
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We describe the free Dirac field in a four dimensional spacetime as a locally covariant quantum field theory in the sense of Brunetti, Fredenhagen and Verch, using a representation independent construction. The freedom in the geometric constructions involved can be encoded in terms of the cohomology of the category of spin spacetimes. If we restrict ourselves to the observable algebra the cohomological obstructions vanish and the theory is unique. We establish some basic properties of the theory and discuss the class of Hadamard states, filling some technical gaps in the literature. Finally we show that the relative Cauchy evolution yields commutators with the stress-energy-momentum tensor, as in the scalar field case.
description: 36 pages; v2 minor changes, typos corrected, updated references and acknowledgements
Electron spin relaxation in n-type InAs quantum wires
Creators: name: Lü, C.
name: Schneider, H. C.
name: Wu, M. W.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We investigate the electron spin relaxation of $n$-type InAs quantum wires by numerically solving the fully microscopic kinetic spin Bloch equations with the relevant scattering explicitly included. We find that the quantum-wire size and the growth direction influence the spin relaxation time by modulating the spin-orbit coupling. Due to inter-subband scattering in connection with the spin-orbit interaction, spin-relaxation in quantum wires can show different characteristics from those in bulk or quantum wells and can be effectively manipulated by various means.
description: 8 pages, 6 figures
Due scrigni stellari da non perdere
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2015

Due ammassi stellari, M46 e M47, possono essere osservati abbastanza agevolmente, anche solo con l’ausilio di un piccolo binocolo, nel cielo in direzione del sud.  In particolare M47, seppure composto da una cinquantina di stelle, è il più brillante della coppia per la sua minore distanza da noi. I consigli per individuare M47 e le informazioni sui fenomeni più interessanti da osservare in questo mese
The first Calends of the Julian Calendar
Creators: name: Sparavigna, Amelia Carolina
Publisher: name: Zenodo
Year: 2019
Subjects: Archaeoastronomy

description: This work is proposing an archaeo-astronomical study of the Julian calendar, a reform of the Roman calendar proposed by Julius Caesar. The calendar was inaugurated on the first of January, 45 BC (historical date). Using astronomical software CalSKY,  we can investigate if the first day of this new system of organizing the days was corresponding to a Calenda, that is, to a day of new moon. It was on January 2, 45 BC (Julian day). We can also see how the new calendar adapted itself to the following phases of the moon.
Begründung und Bedeutung einer Lehre von den Schöpfungsordnungen Gottes nach Schrift und Bekenntnis
Creators: name: Wenz, Armin
Publisher: name: Lutherische Beiträge
Year: 1970

description: Lutherische Beiträge, Bd. 15 Nr. 4 (2010): Lutherische Beiträge, Band 15, Heft 4
title: Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¾Ñ ÑÐ°Ð½Ð¾Ð¹ ÑÑÑÐ´Ð° Ð½Ð° Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð¼ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐÐÐ­Ð¤ÐÂ»)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÐ³Ð¸Ð½, ÐÐ¸ÐºÑÐ¾Ñ
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¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ
Ð¾Ñ ÑÐ°Ð½Ð° ÑÑÑÐ´Ð°
Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾
enterprise
labour protection
production

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð¾ÑÑÐ°Ð½Ð° ÑÑÑÐ´Ð° Ð½Ð° Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð¼ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ ÐÐÐ Â«ÐÐÐÐ­Ð¤ÐÂ». Ð¦ÐµÐ»Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ- Ð¿ÑÐµÐ´Ð»Ð¾Ð¶Ð¸ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾ÑÑÐ°Ð½Ð¾Ð¹ ÑÑÑÐ´Ð° Ð¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ ÑÑÑÐ´Ð°. Ð Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸Ð»Ð¾ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÐ¾Ð² Ð¿Ð¾ Ð¾ÑÑÐ°Ð½Ðµ ÑÑÑÐ´Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾ÑÑÐ°Ð½Ñ ÑÑÑÐ´Ð° Ð½Ð° ÐÐÐ Â«ÐÐÐÐ­Ð¤ÐÂ». Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð±ÑÐ»Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ ÐÐÐ Â« ÐÐÐÐ­Ð¤ÐÂ» ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾ÑÑÐ°Ð½Ð¾Ð¹ ÑÑÑÐ´Ð°.
description: The object of the research is the occupational safety at the industrial enterprise JSC "NIIEFA". The purpose of the final - to propose measures to improve occupational health and safety, as well as the enterprise for labor protection. In the process of writing, the work was to study the theoretical issues on labor protection, as well as the analysis of the organization of labor protection in JSC "NIIEFA". The results of the study suggested measures to establish a system at the enterprise JSC "NIIEFA" for safety management and occupational health.
New tools for probing the phase space structure of dark matter halos
Creators: name: Valluri, Monica
name: Debattista, Victor P.
name: Quinn, Tom
name: Moore, Ben
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We summarize recent developments in the use of spectral methods for analyzing large numbers of orbits in N-body simulations to obtain insights into the global phase space structure of dark matter halos. The fundamental frequencies of oscillation of orbits can be used to understand the physical mechanism by which the shapes of dark matter halos evolve in response to the growth of central baryonic components. Halos change shape primarily because individual orbits change their shapes adiabatically in response to the growth of a baryonic component, with those at small radii become preferentially rounder. Chaotic scattering of orbits occurs only when the central point mass is very compact and is equally effective for centrophobic long-axis tube orbits as it is for centrophilic box orbits.
description: To appear in "Hunting for the Dark: The Hidden Side of Galaxy Formation", Malta, 19-23 Oct. 2009, eds. V.P. Debattista & C.C. Popescu, AIP Conf. Ser., in press, 4 pages 3 figures
Johann Habermann, Christliche Gebete für alle Not und Stende der ganzen Christenheit (1567)
Creators: name: Junker, Thomas
Publisher: name: Lutherische Beiträge
Year: 1970

description: Lutherische Beiträge, Bd. 15 Nr. 3 (2010): Lutherische Beiträge, Band 15, Heft 3
Una Bellezza Nera marziana
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2015

NWA 7034 è uno dei più antichi meteoriti mai trovati sulla Terra. Diverso da tutti gli altri frammenti analizzati finora perché ricco d'acqua e carbonio organico, questo pesa 320 grammi ed è essenzialmente un pezzo di roccia basaltica (quindi magmatica) cementata molto scura e particolare. Ecco perché
title: Ð­Ð»ÐµÐ³Ð°Ð·Ð¾Ð²ÑÐ¹ Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÐ½ÑÐ¹ Ð²ÑÐºÐ»ÑÑÐ°ÑÐµÐ»Ñ 63 ÐºÐ Ð´Ð»Ñ ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°Ð½ÑÐ¸Ð¸ ÐÐ°ÐºÐ²Ð¸Ð¶Ð°Ñ (Ð¨ÑÐ¸âÐÐ°Ð½ÐºÐ°)
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: Ð¯Ð´Ð´ÐµÑ Ð¸Ð³Ðµ Ð Ð¸Ð²Ð¸Ð½Ð´Ñ ÐÐ°ÑÐ°Ð½ÐºÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐ»ÐµÐ³Ð°Ð·Ð¾Ð²ÑÐ¹ Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÐ½ÑÐ¹ Ð²ÑÐºÐ»ÑÑÐ°ÑÐµÐ»Ñ
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description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½ Ð¾Ð±Ð·Ð¾Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ Ð¸ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÐ½ÑÑ Ð²ÑÐºÐ»ÑÑÐ°ÑÐµÐ»ÐµÐ¹. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð²ÑÐºÐ»ÑÑÐ°ÑÐµÐ»Ñ Ñ ÑÐµÑÑÑ Ð² ÑÐµÐ¶Ð¸Ð¼Ð°Ñ ÐºÐ¾ÑÐ¾ÑÐºÐ¸Ñ Ð·Ð°Ð¼ÑÐºÐ°Ð½Ð¸Ðµ. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ ÑÐ°ÑÑÐµÑ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² Ð´ÑÐ³Ð¾Ð³Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð¸ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð¾ ÑÐ¸ÑÐ»ÐµÐ½Ð½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð² Ð´ÑÐ³Ð¾Ð³Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ð¼ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ðµ Ð¿ÑÐ¸ ÐºÐ¾Ð¼Ð¼ÑÑÐ°ÑÐ¸Ð¸. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ ÑÐ¾Ð¿Ð»Ð¾Ð²Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð²ÑÐºÐ»ÑÑÐ°ÑÐµÐ»Ñ, Ð³Ð»Ð°Ð²Ð½Ð¾Ð¹ ÐºÐ¾Ð½ÑÐ°ÐºÑÐ½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð²ÑÐºÐ»ÑÑÐ°ÑÐµÐ»Ñ Ð¸ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ Ðº Ð¿ÑÐ¸Ð²Ð¾Ð´Ñ Ð´Ð»Ñ Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð²ÑÐºÐ»ÑÑÐ°ÑÐµÐ»Ñ.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð´Ð¸Ð·Ð°Ð¹Ð½Ð° ÑÐ°Ð¹ÑÐ° Ð´Ð»Ñ Ð¼Ð°ÑÑÐµÑÑÐºÐ¾Ð¹ Ð¿Ð¾ Ñ ÑÐ´Ð¾Ð¶ÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ ÐºÐ¾Ð²ÐºÐµ Â«Ð­Ð´ÐµÐ»ÑÐ²ÐµÐ¹ÑÂ»
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÐ°Ð»ÐµÐ²ÑÐºÐ°Ñ, Ð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: ÑÐ°Ð¹Ñ
ÐºÐ¾Ð²ÐºÐ°
Ð»Ð¸ÑÑÐµ
Ð°Ð´Ð°Ð¿ÑÐ¸Ð²Ð½ÑÐ¹ Ð´Ð¸Ð·Ð°Ð¹Ð½

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¾Ð½ÐºÐ¾ÑÑÐ¸ ÐºÑÐ·Ð½ÐµÑÐ½Ð¾Ð³Ð¾ Ð´ÐµÐ»Ð° Ð¸ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ½ÑÑ ÑÐ°Ð¹ÑÐ¾Ð². Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð°Ð´Ð°Ð¿ÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ ÑÐ°Ð¹ÑÐ° Ð´Ð»Ñ Ð¼Ð°ÑÑÐµÑÑÐºÐ¾Ð¹ Â«Ð­Ð´ÐµÐ»ÑÐ²ÐµÐ¹ÑÂ». Ð Ð¿ÑÐ¾ÑÐµÑÑÐµ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸Ð»ÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐµÐ½Ð´Ð¾Ð² Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÑÐµÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ Ð¿ÑÐ¸ÑÐ¾Ð»Ð¾Ð³Ð¸Ñ Ð¿Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»Ñ Ð½Ð° ÑÐ°Ð¹ÑÐµ.
Itinerant antiferromagnetism in BaCr$_2$As$_2$
Creators: name: Singh, D. J.
name: Sefat, A. S.
name: McGuire, M. A.
name: Sales, B. C.
name: Mandrus, D.
name: VanBebber, L. H.
name: Keppens, V.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We report single crystal synthesis, specific heat and resistivity measurements and electronic structure calculations for BaCr$_2$As$_2$. This material is a metal with itinerant antiferromagnetism, similar to the parent phases of Fe-based high temperature superconductors, but differs in magnetic order. Comparison of bare band structure density of states and the low temperature specific heat implies a mass renormalization of $\sim$ 2. BaCr$_2$As$_2$ shows stronger transition metal - pnictogen covalency than the Fe compounds, and in this respect is more similar to BaMn$_2$As$_2$. This provides an explanation for the observation that Ni and Co doping is effective in the Fe-based superconductors, but Cr or Mn doping is not.
description: Additional discussion. Minor correction to Fermi velocities
Una vita alla Steve McQueen
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2015

Uno studio condotto su un insieme di quattro galassie dimostra come la loro intensa attività le renda ben presto inattive facendole invecchiare prematuramente a causa della mancanza del gas necessario per formare nuove stelle. Lo studio, pubblicato su Monthly Notices of the Royal Astronomical Society, fa luce sui quei meccanismi che determinano la fine dei processi di formazione stellare
ELIXIR 2023 Recommended Interoperability Resources
Creators: name: Garrard, Clare
name: Maccallum, Peter
name: Liberante, Fabio
Publisher: name: Zenodo
Year: 2023

description: ELIXIR Recommended Interoperability Resources are European tools, services, and registries that help make scientific research findable, accessible, interoperable and reusable (FAIR). 

Following the 2023 RIR selection process, there are now 21 Recommended Interoperability Resources, an increase of 7.In this document we outline the background to the RIRs, list the new RIRs, and publicly thank and acknowledge our reviewers and evaluators.
title: Relationships Between Classroom Schedule Types and Performance on the Algebra I Criterion-Referenced Test
Creators: name: Murray, Gregory V.
Publisher: name: Utah State University
Year: 2012

description: Public education has options with regard to educational settings and structures. States and school districts may select varying lengths for the school year, lengths for the school day, and lengths for individual class periods. In Utah, one measure of students' achievement is scores on the State's end-of-level criterion-referenced test (CRT) for Algebra I. Additionally, an option regarding educational structures is the schedule type used to deliver Algebra I classes. This study examined the relationship between student achievement as measured by Algebra I CRT scores, and the schedule type used to deliver Algebra I classes. The schedule types compared were the traditional daily schedule, trimester 3/3 schedule, trimester 2/3 schedule, and the block A/B schedule. This study sought to answer two research questions: (1) What is the relationship between mathematics instructional schedule type and student scores on Utah's CRT for Algebra I, for all students? and (2) What is the relationship between mathematics instructional schedule type and student scores on Utah's CRT for Algebra I, by individual grade levels? Data were obtained from the Utah State Office of Education and included the scores for 50,000 Utah students, from over 300 different schools, who took the identical Algebra I CRT at the end of the 2010-2011 school year. Data were also obtained from each school district to determine the schedule type of each participating student. Both a multinomial logistic regression analysis and a t-test analysis were conducted to determine relationships between Algebra I CRT scores and schedule types. The results indicated significant differences in student achievement based on the schedule type overall and for individual grade levels. Generally, the earlier the grade level the higher the CRT score. Within individual grade levels, there were both statistically significant and nonsignificant differences. The schedule types that generally score the highest (trimester 3/3 and traditional) had more time in the mathematics classroom and the students' mathematics class met daily. The results suggest the value of daily time spent in the mathematics classroom and may assist educators when considering options available to foster student achievement.
Modern Theory of Nuclear Forces
Creators: name: Epelbaum, Evgeny
name: Hammer, Hans-Werner
name: Meißner, Ulf-G.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Effective field theory allows for a systematic and model-independent derivation of the forces between nucleons in harmony with the symmetries of Quantum Chromodynamics. We review the foundations of this approach and discuss its application for light nuclei at various resolution scales. The extension of this approach to many-body systems is briefly sketched.
description: Commissioned article for Reviews of Modern Physics, 52 pp, 40 figs
title: ÐÐµÑÐ¾Ð´Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÑ ÑÐµÑÐµÐ½Ð¸Ð¹. ÐÐ¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Microsoft Excel
title: Ð¿ÑÐ°ÐºÑÐ¸ÐºÑÐ¼
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ°Ð½Ð¸Ð½, ÐÐ¼Ð¸ÑÑÐ¸Ð¹
name: ÐÑÐºÐ°ÑÐµÐ²Ð¸Ñ, ÐÐ¸ÐºÐ¸ÑÐ°
name: Ð¢Ð¸ÑÐ¾Ð½Ð¾Ð², ÐÐ¼Ð¸ÑÑÐ¸Ð¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2015
Subjects: ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½ÑÐµ
ÐÐ¸Ð½ÐµÐ¹Ð½Ð¾Ðµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ

description: Ð Ð¿ÑÐ°ÐºÑÐ¸ÐºÑÐ¼Ðµ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐ°Ð±Ð¾ÑÑ Ñ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸ÐµÐ¼ Microsoft Excel Ð¿ÑÐ¸ ÑÐµÑÐµÐ½Ð¸Ð¸ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð·Ð°Ð´Ð°Ñ (ÑÑÐ°Ð½Ð´Ð°ÑÑÐ½Ð¾Ð¹ Ð·Ð°Ð´Ð°ÑÐ¸ Ð»Ð¸Ð½ÐµÐ¹Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð¾Ð¹ Ð·Ð°Ð´Ð°ÑÐ¸, Ð·Ð°Ð´Ð°ÑÐ¸ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿Ð¾ÑÑÑÐµÐ»Ñ ÑÐµÐ½Ð½ÑÑ Ð±ÑÐ¼Ð°Ð³). ÐÐ·Ð´Ð°Ð½Ð¸Ðµ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð¾Ð²Ð°Ð½Ð¾ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð¾ÑÐ½Ð¾Ð¹, Ð¾ÑÐ½Ð¾-Ð·Ð°Ð¾ÑÐ½Ð¾Ð¹, Ð·Ð°Ð¾ÑÐ½Ð¾Ð¹ Ð¸ Ð´Ð¸ÑÑÐ°Ð½ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¾ÑÐ¼ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ 38.03.02 Â«ÐÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÂ» Ð¸ 38.03.01 Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°Â», Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«ÐÐµÑÐ¾Ð´Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÑ ÑÐµÑÐµÐ½Ð¸Ð¹Â», Ð´Ð»Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÐºÑÑÑÐ¾Ð²Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ.
Global Regularity for the Critical Dispersive Dissipative Surface Quasi-Geostrophic Equation
Creators: name: Kiselev, Alexander
name: Nazarov, Fedor
Publisher: name: arXiv
Year: 2009
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics
subject: 35B65; 35Q35

description: We consider surface quasi-geostrophic equation with dispersive forcing and critical dissipation. We prove global existence of smooth solutions given sufficiently smooth initial data. This is done using a maximum principle for the solutions involving conservation of a certain family of moduli of continuity.
description: 6 pages
Onde gravitazionali ridotte in polvere
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2015

Contrariamente a quanto annunciato la primavera scorsa, non c’è ancora alcuna prova certa della presenza di “modi B” primordiali – risalenti al Big Bang – nella polarizzazione della CMB. Questa la conclusione, dopo mesi trascorsi fianco a fianco ad analizzare i dati, dei team del satellite Planck dell’ESA e del telescopio antartico BICEP2
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ÑÐ±ÑÐ°ÑÐ¾Ðµ ÐºÐ¾Ð»ÐµÑÐ¾Â»
title: Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ
titleType: Subtitle
Creators: name: ÐÐ½ÑÐ¾Ð½Ð¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð¼ÐµÑ Ð°Ð½Ð¸ÑÐµÑÐºÐ°Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ° Ð´ÐµÑÐ°Ð»ÐµÐ¹
ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ
Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð½Ð°ÐºÐ»Ð°Ð´ÐºÐ°

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¼ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¼ Ð¿ÑÐ¾ÐµÐºÑÐµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð´ÐµÑÐ°Ð»Ð¸ Â«ÐÑÐ±ÑÐ°ÑÐ¾Ðµ ÐºÐ¾Ð»ÐµÑÐ¾Â» Ð½Ð° Ð¼ÐµÑÐ°Ð»Ð»Ð¾ÑÐµÐ¶ÑÑÐ¸Ñ ÑÑÐ°Ð½ÐºÐ°Ñ, Ð²ÑÐ±ÑÐ°Ð½ Ð²Ð¸Ð´ Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¸ Ð¼ÐµÑÐ¾Ð´ ÐµÑ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ, ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ñ Ð¿ÑÐ¸Ð¿ÑÑÐºÐ¸ Ð´Ð»Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸, ÑÐµÐ¶Ð¸Ð¼Ñ ÑÐµÐ·Ð°Ð½Ð¸Ñ, ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ð¾ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ðµ Ð¿ÑÐ¸ÑÐ¿Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð¸Ðµ. ÐÑÐ¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð±ÑÐ»Ð¸ ÑÑÑÐµÐ½Ñ: ÑÐ¸Ð¿ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°, ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð¸ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¾Ð±ÑÐ°Ð±Ð°ÑÑÐ²Ð°ÐµÐ¼Ð¾Ð³Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°, ÑÐ¾ÑÐ½Ð¾ÑÑÑ ÑÐ¾ÑÐ¼ Ð¸ ÑÐ°Ð·Ð¼ÐµÑÐ¾Ð², ÑÐµÑÐ¾ÑÐ¾Ð²Ð°ÑÐ¾ÑÑÑ, Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐ¸Ðµ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ Ð¸ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ñ. ÐÑÐ¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ð¸ ÑÑÐ´Ð° ÑÐ°Ð·Ð´ÐµÐ»Ð¾Ð² Ð¿ÑÐ¾ÐµÐºÑÐ° (ÑÐ°ÑÑÑÑ Ð¿ÑÐ¸Ð¿ÑÑÐºÐ¾Ð², ÑÐ°ÑÑÑÑ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² ÑÐµÐ·Ð°Ð½Ð¸Ñ) Ð±ÑÐ» Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÐ¹ Ð¿Ð°ÐºÐµÑ ÐÐ¾Ð¼Ð¿Ð°Ñ-3D. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»: ÑÐµÑÑÐµÐ¶Ð¸ Ð´ÐµÑÐ°Ð»Ð¸, Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸, Ð¿ÑÐ¸ÑÐ¿Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð¸Ñ, ÐºÐ°ÑÑ Ð½Ð°Ð»Ð°Ð´Ð¾Ðº, Ð°Ð»ÑÐ±Ð¾Ð¼ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ ÐºÐ°ÑÑ Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐ¼Ð¸ ÑÑÐºÐ¸Ð·Ð°Ð¼Ð¸. ÐÑÐ¸ Ð¾ÑÐ¾ÑÐ¼Ð»ÐµÐ½Ð¸Ð¸ Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð¸ Ð°Ð»ÑÐ±Ð¾Ð¼Ð° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ ÐºÐ°ÑÑ ÑÑÐ¸ÑÑÐ²Ð°Ð»Ð¸ÑÑ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ ÐÐ¡ÐÐ Ð¸ ÐÐ¡Ð¢ÐÐ.