cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Preprints: Forschungsergebnisse schnell und offen kommunizieren
Creators: name: Schmeja, Stefan
Publisher: name: Zenodo
Year: 2021
Subjects: Open Access
Publikationsprozess

description: Preprints, also Vorabversionen von wissenschaftlichen Artikeln, spielen eine immer wichtigere Rolle in der Kommunikation von Forschungsergebnissen. Während das Teilen von Preprints in der Physik dank arXiv eine 30-jährige Tradition hat, haben es andere Fachgebiete erst vor kurzem für sich entdeckt. In den Lebenswissenschaften hat insbesondere die Covid-19-Pandemie mit dem Bedarf nach einer raschen Verbreitung von Forschungsergebnissen zum SARS-CoV-2-Virus für einen Aufschwung von Preprints geführt. Da Preprints in der Regel noch kein Peer Review durchlaufen haben, gibt es aber auch Vorbehalte. In diesem Vortrag, der im Rahmen des Open Access Talk am 28.10.2021 gehalten wurde, werden die Merkmale von Preprints und Preprint-Servern vorgestellt, rechtliche Fragestellungen erörtert und die Bedeutung von Preprints für Open Science und den "grünen Weg" zu Open Access diskutiert. Folgende Fragen stehen dabei im Fokus: Welche Version meines Manuskriptes darf ich veröffentlichen? Was muss ich dabei beachten? Wo kann ich Preprints veröffentlichen? Welche Vorbehalte gibt es gegenüber Preprints? Welche Rolle spielen Preprints für Open Access?
Breast Cancer Detection using Histopathological Images
Creators: name: Maan, Jitendra
name: Maan, Harsh
Publisher: name: arXiv
Year: 2022
Subjects: subject: Image and Video Processing (eess.IV)
subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Computer and information sciences

description: Cancer is one of the most common and fatal diseases in the world. Breast cancer affects one in every eight women and one in every eight hundred men. Hence, our prime target should be early detection of cancer because the early detection of cancer can be helpful to cure cancer effectively. Therefore, we propose a saliency detection system with the help of advanced deep learning techniques, such that the machine will be taught to emulate actions of pathologists for localization of diagnostically pertinent regions. We study identification of five diagnostic categories of breast cancer by training a CNN (VGG16, ResNet architecture). We have used BreakHis dataset to train our model. We focus on both detection and classification of cancerous regions in histopathology images. The diagnostically relevant regions are salient. The detection system will be available as an open source web application which can be used by pathologists and medical institutions.
description: 6 pages, 10 figures, Published with International Journal of Computer Science Trends and Technology (IJCST)
Cielo a pecorelle attorno alle galassie
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2014

Un lavoro pubblicato su Monthly Notices of the Royal Astronomical Society e guidato da ricercatori dell'Università dell'Illinois getta nuova luce sulla struttura e i moti delle nubi giganti di gas che circondano le galassie. Guido Risaliti (INAF): "Queste osservazioni potrebbero costituire un importante nuovo 'ingrediente' per i modelli di formazione ed evoluzione delle galassie".
Quell’oggetto misterioso nel cielo
Creators: Giulia Bonelli
Publisher: name: Media Inaf
Year: 2014

Un oggetto celeste appena scoperto sfida le categorie astronomiche oggi conosciute. Individuato da un gruppo di astrofisici dell’Università di Toronto, ha alcune caratteristiche dei pianeti e altre delle nane brune. Lo studio su Astrophysical Journal Letters.
Kepler scopre altri esopianeti gonfi di gas
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2014

È tempo di bilanci in casa Kepler. Durante il meeting annuale dell'American Astronomical Society (AAS) a Washington sono stati presentati gli ultimi risultati delle ricerche del telescopio orbitante della NASA. Tra i pianeti candidati scoperti in questi quattro anni moltissimi sono gassosi. La tecnica per misurare la massa e la densità è quella delle variazioni temporanee di transito. Sempre al meeting annuale della AAS un nuovo studio ipotizza un clima più simile alla Terra di quanto finora ipotizzato per gli esopianeti denominati Super-Terre
title: ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ°. ÐÐ²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð² Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð·
title: Ð¿ÑÐ°ÐºÑÐ¸ÐºÑÐ¼
titleType: Subtitle
Creators: name: ÐÐ¾Ð»ÐºÐ¾Ð², ÐÐ¼Ð¸ÑÑÐ¸Ð¹
name: ÐÐ°Ð»ÑÐ½Ð¾Ð²Ð°, ÐÑÐµÐ½Ð¸Ñ
name: ÐÑÐ°ÑÐ½Ð¾ÑÐµÐºÐ¾Ð², ÐÐ¸ÐºÑÐ¾Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2016
Subjects: ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð·

description: Ð ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð²Ð¾Ð¿ÑÐ¾ÑÑ, ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÐµ Ñ Ð¿Ð¾Ð½ÑÑÐ¸ÑÐ¼Ð¸ Ð¼Ð½Ð¾Ð¶ÐµÑÑÐ²Ð°, ÑÑÐ½ÐºÑÐ¸Ð¸ Ð¸ Ð¿ÑÐµÐ´ÐµÐ»Ð° ÑÑÐ½ÐºÑÐ¸Ð¸ Ð¾Ð´Ð½Ð¾Ð¹ Ð¿ÐµÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹. ÐÐµÑÐ²Ð°Ñ ÑÐ°ÑÑÑ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð¸Ð· Ð¿ÑÑÐ¸ ÑÐ°Ð·Ð´ÐµÐ»Ð¾Ð², Ð² ÐºÐ¾ÑÐ¾ÑÑÑ ÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÑÑ ÐºÑÐ°ÑÐºÐ¸Ðµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¸ Ð¿ÑÐ¸Ð¼ÐµÑÑ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹. Ð¢ÐµÐºÑÑ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¸ÑÑÑ Ð¿Ð°ÑÐ°Ð»Ð»ÐµÐ»ÑÐ½Ð¾ Ð½Ð° ÑÑÑÑÐºÐ¾Ð¼ Ð¸ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð¼ ÑÐ·ÑÐºÐ°Ñ. ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¹ ÑÐ°ÑÑÐ¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ ÑÐ¾Ð±ÑÐ°Ð½Ð¾ 330 Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹ Ð¿Ð¾ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÐ¼ÑÐ¼ ÑÐµÐ¼Ð°Ð¼. ÐÑÐ»Ð¸ ÑÐ¸Ð¿Ñ Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹ Ð² ÑÐµÐ»Ð¾Ð¼ ÑÑÐ°Ð´Ð¸ÑÐ¸Ð¾Ð½Ð½Ñ, ÑÐ¾ ÑÐ°Ð¼Ð¸ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ Ð¿ÑÐµÐ¸Ð¼ÑÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾ Ð¾ÑÐ¸Ð³Ð¸Ð½Ð°Ð»ÑÐ½Ñ. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ 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Ð¼ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°Â», Â«ÐÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÂ», Â«ÐÐ¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ Ð¸ Ð¼ÑÐ½Ð¸ÑÐ¸Ð¿Ð°Ð»ÑÐ½Ð¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÂ», Â«ÐÐ¸Ð·Ð½ÐµÑ-Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ°Â», Â«Ð­Ð½ÐµÑÐ³ÐµÑÐ¸ÐºÐ°, ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ðµ Ð¸ ÑÐ»ÐµÐºÑÑÐ¾ÑÐµÑÐ½Ð¸ÐºÐ°Â», Â«ÐÐµÑÐ°Ð»Ð»ÑÑÐ³Ð¸Ñ, Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ðµ Ð¸ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ°Â», Â«Ð¢ÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÐµ ÑÑÐµÐ´ÑÑÐ²Ð°Â», Â«ÐÑÑÐ¸ÑÐµÐºÑÑÑÐ° Ð¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾Â», Â«ÐÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑ Ð¶Ð¸Ð·Ð½ÐµÐ´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸, Ð¿ÑÐ¸ÑÐ¾Ð´Ð¾Ð¾Ð±ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾ Ð¸ Ð¾ÑÑÐ°Ð½Ð° Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´ÑÂ», Ð° ÑÐ°ÐºÐ¶Ðµ Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ° Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÂ», Â«ÐÑÐ¼Ð°Ð½Ð¸ÑÐ°ÑÐ½ÑÐµ Ð½Ð°ÑÐºÐ¸Â». Ð§Ð°ÑÑÐ¸ÑÐ½Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð¼Ð¾Ð³ÑÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ñ Ð¿ÑÐ¸ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² Ð¿Ð¾ Ð³ÑÑÐ¿Ð¿Ð°Ð¼ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹: Â«Ð­Ð»ÐµÐºÑÑÐ¾Ð½Ð½Ð°Ñ ÑÐµÑÐ½Ð¸ÐºÐ°, ÑÐ°Ð´Ð¸Ð¾ÑÐµÑÐ½Ð¸ÐºÐ° Ð¸ ÑÐ²ÑÐ·ÑÂ», Â«ÐÐ²ÑÐ¾Ð¼Ð°ÑÐ¸ÐºÐ° Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÂ», Â«ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ° Ð¸ Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ ÑÐµÑÐ½Ð¸ÐºÐ°Â» Ð¸ Ð´Ñ. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¼Ð¾Ð¶ÐµÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÑÑÑ ÐºÐ°Ðº Ð¿ÑÐ¸ Ð¾Ð±ÑÑÐµÐ½Ð¸Ð¸ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², ÑÐ°Ðº Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð²-Ð¸Ð½Ð¾ÑÑÑÐ°Ð½ÑÐµÐ², Ð²Ð»Ð°Ð´ÐµÑÑÐ¸Ñ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¸Ð¼ ÑÐ·ÑÐºÐ¾Ð¼.
Controllable CVD-Growth of 2D Cr5Te8 Nanosheets with Thickness-Dependent Magnetic Domains
Creators: name: Wu, Hanxiang
name: Guo, Jianfeng
name: Zhaxi, Suonan
name: Xu, Hua
name: Mi, Shuo
name: Wang, Le
name: Chen, Shanshan
name: Xu, Rui
name: Ji, Wei
name: Pang, Fei
name: Cheng, Zhihai
Publisher: name: arXiv
Year: 2023
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: As a typical 2D magnetic material with self-intercalated structure, Cr5Te8 exhibits many fascinating magnetic properties. Although the ferromagnetism of 2D Cr5Te8 has been reported, the study of its magnetic domain is still blank. Herein, we successfully fabricated 2D Cr5Te8 nanosheets with controlled thickness and lateral size by chemical vapor deposition (CVD). Then magnetic property measurement system suggested Cr5Te8 nanosheets possessing intense out-of-plane ferromagnetism with the Curie temperature of 179 K. Most importantly, we found magnetic bubbles and thickness-dependent maze-like magnetic domains by cryogenic magnetic force microscopy (MFM) for the first time. The domain width of the maze-like magnetic domains increases rapidly with decreasing sample thickness, while domain contrast decreases. This indicates dipolar interaction is the dominant role over exchange interaction and magnetic anisotropy. Our work not only paves a way for the controllable growth of 2D magnetic materials, but also suggests new directions for controlling magnetic phases and systematically adjusting domain properties.
L’immutabile energia oscura del BOSS
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2014

Analizzando lo spettro di oltre un milione di galassie, la Baryon Oscillation Spectroscopic Survey ha realizzato la misura più precisa di sempre della scala dell’universo. Consentendo di quantificare alcune proprietà della dark energy e della curvatura. Numerosi gli italiani nella collaborazione.
title: Developing Advanced Cloud Retrievals for PACE: Building a Joint Spectro-Polarimetric Cloud Microphysics Retrieval
Creators: name: Miller, Daniel J.
name: Meyer, Kerry
name: Platnick, Steven E.
name: Zhang, Zhibo
name: Ademakinwa, Adeleke
name: Sinclair, Kenneth
name: Alexandrov, Mikhail
name: Geogdzhayev, Igor
name: Van Diedenhoven, Bastiaan
Publisher: name: NASA
Year: 2024

description: AGU Fall Meeting 2024
Thermodynamics of small systems by nanocalorimetry: from physical to biological nano-objects
Creators: name: Garden, Jean-Luc
name: Guillou, Hervé
name: Lopeandia, Aitor Fernandez
name: Richard, Jacques
name: Heron, Jean-Savin
name: Souche, Germain
name: Ong, Florian
name: Vianay, Benoit
name: Bourgeois, Olivier
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Soft Condensed Matter (cond-mat.soft)
subject: Biological Physics (physics.bio-ph)
subject: Chemical Physics (physics.chem-ph)
subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: Membrane based nanocalorimeters have been developed for ac calorimetry experiments. It has allowed highly sensitive measurements of heat capacity from solid state physics to complex systems like polymers and proteins. In this article we review what has been developed in ac calorimetry toward the measurement of very small systems. Firstly, at low temperature ac calorimetry using silicon membrane permits the measurement of superconducting sample having geometry down to the nanometer scale. New phase transitions have been found in these nanosystems illustrated by heat capacity jumps versus the applied magnetic field. Secondly, a sensor based on ultra-thin polymer membrane will be presented. It has been devoted to thermal measurements of nanomagnetic systems at intermediate temperature (20K to 300K). Thirdly, three specific polyimide membrane based sensors have been designed for room temperature measurements. One is devoted to phase transitions detection in polymer, the second one to protein folding/unfolding studies and the third one will be used for the study of heat release in living cells. The possibility of measuring systems out of equilibrium will be emphasized.
The geology of Kinskuch Lake area, British Columbia
Creators: name: Gale, Robert Earle
Publisher: name: University of British Columbia
Year: 2012

description: Kinskuch Lake area covers a fifty-square mile portion of the Portland Canal district of western British Columbia. Kinskuch Lake lies near the eastern border of the Coast Mountains, approximately twelve miles north of the port of Alice Arm. Reconnaissance mapping of the area on a scale of 1" = 1000’ was done during part of the summer of 1956. Rock specimens collected in the field were examined microscopically and the results of the latter investigation form the greater part of this thesis. The interbedded volcanic and sedimentary rocks of Kinskuch Lake area were deposited during the period of Mesozoic volcanism and sedimentation which was widespread throughout western British Columbia and southeastern Alaska. Near Kinskuch Lake, the earliest products of Mesozoic volcanism are represented by augite porphyry volcanic breccias, crystal tuffs, flows and flow breccias outcropping along the western margin of the map area. Augitic volcanics are overlain to the east by interfingering felsitic breccias and tuffs, sedimentary rocks and greenstone. East of Kinskuch Lake, the latter rocks pass gradationally into a thick overlying sequence of felsitic volcanic breccia, crystal tuffs and feldspar porphyry flows. The youngest rocks outcrop near the eastern margin of the map area. Here, argillites and conglomerates overlie felsitic volcanic breccia and interbedded tuff. The Mesozoic volcanic and sedimentary rocks were folded, faulted and intruded by keratophyric and lamprophyric dykes. As a last stage in the geological sequence of events, volcanic rocks at the southeast corner of Kinskuch Lake were altered and mineralized. Highly fractured or sheared greenstone and felsitic volcanics were altered to chlorite, pyrite, epidote, sericite quartz and calcite. Minor chalcopyrite mineralization accompanied rock alteration and many small quartz-carbonate veins cut the altered rocks. Some of the latter veins carry pyrite, chalcopyrite and traces of sphalerite and galena. Albitization of some of the igneous rocks outside the altered zone accompanied the widespread carbonate alteration.
Le tre scoperte sul podio di Hubble
Creators: Giulia Bonelli
Publisher: name: Media Inaf
Year: 2014

Quattro galassie luminosissime, l’immagine più dettagliata mai fornita di un ammasso di galassie e la probabile origine di quasi tutte le stelle osservate oggi: sono i tre risultati più importanti raggiunti dal telescopio spaziale Hubble. La presentazione al summit mondiale per lo spazio dell’American Astronomical Society.
title: Ð ÐµÑÐµÐ½Ð¸Ðµ Ð¿ÑÐ¸ÐºÐ»Ð°Ð´Ð½ÑÑ Ð·Ð°Ð´Ð°Ñ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð² ÑÐ°ÑÐºÑÐ°ÑÐºÐ¸ Ð³ÑÐ°ÑÐ¾Ð²
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡ÐµÑÐ¾Ð², 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¿Ð¾Ð¸ÑÐº Ñ ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ¸ÑÐ»Ð° Ð³ÑÐ°ÑÐ¾Ð²
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description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÑÑÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ñ ÑÐ°ÑÐºÑÐ°ÑÐºÐ¸ Ð³ÑÐ°ÑÐ¾Ð², Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ Ð¿Ð¾Ð¸ÑÐºÐ° Ð³Ð°Ð¼Ð¸Ð»ÑÑÐ¾Ð½Ð¾Ð²Ð° ÑÐ¸ÐºÐ»Ð° Ð¸ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¸Ñ ÑÐµÐ°Ð»Ð¸Ð·ÑÑÑÐ¸Ðµ. Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ ÑÐµÐ°Ð»Ð¸Ð·ÑÑÑÐµÐµ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ñ ÑÐ°ÑÐºÑÐ°ÑÐºÐ¸ Ð³ÑÐ°ÑÐ¾Ð². Ð Ð¿ÑÐ¾ÑÐµÑÑÐµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð¸ Ð¸Ð·ÑÑÐµÐ½Ñ Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ñ ÑÐ°ÑÐºÑÐ°ÑÐºÐ¸ Ð³ÑÐ°ÑÐ¾Ð², Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¸ ÑÐµÑÐµÐ½Ð¸Ð¸ Ð¿ÑÐ¸ÐºÐ»Ð°Ð´Ð½ÑÑ Ð·Ð°Ð´Ð°Ñ. ÐÑÐ»Ð¾ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð¾ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ ÑÐ¿ÑÐ¾ÑÐ°ÑÑÐµÐµ Ð²Ð²Ð¾Ð´ Ð¸ ÑÐµÐ´Ð°ÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð³ÑÐ°ÑÐ¾Ð²ÑÑ ÑÑÑÑÐºÑÑÑ. ÐÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð´Ð°ÐµÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ Ð¾ÑÐ¾Ð±ÑÐ°Ð·Ð¸ÑÑ ÑÐ°Ð¼ Ð³ÑÐ°Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐµÐ·ÑÐ»ÑÑÐ°Ñ ÐµÐ³Ð¾ ÑÐ°ÑÐºÑÐ°ÑÐºÐ¸. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð½ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ ÑÐµÑÐµÐ½Ð¸Ñ Ð¼Ð¾Ð´ÐµÐ»ÑÐ½ÑÑ Ð·Ð°Ð´Ð°Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°Ð»Ð¸ Ð½Ð°Ð´ÐµÐ¶Ð½Ð¾ÑÑÑ Ð¸ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ ÑÐ°Ð±Ð¾ÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ. ÐÐ´Ð½Ð¸Ð¼ Ð¸Ð· Ð´Ð¾ÑÑÐ¾Ð¸Ð½ÑÑÐ² ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð² ÑÑÐµÐ±Ð½ÑÑ ÑÐµÐ»ÑÑ. ÐÐ¾ÑÑÐµÐºÑÐ½Ð¾ÑÑÑ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð±ÑÐ»Ð° Ð¿ÑÐ¾Ð²ÐµÑÐµÐ½Ð° Ð½Ð° ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ ÑÐºÐ¾Ð½ÑÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¿ÑÐ¸Ð¼ÐµÑÐ°Ñ.
Il Sole debutta alla grande
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2014

Inizio d'anno con botto per il Sole. Prima una macchia solare grande come poche nell'ultimo decennio. Poi, dalla stessa regione attiva, il primo brillamento in classe X del 2014, accompagnato da un'espulsione di massa coronale. Si prevede tempesta geomagnetica di moderata entità, buona per gli amanti delle aurore polari.
Pulsar timing array projects
Creators: name: Hobbs, G.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Pulsars are amongst the most stable rotators known in the Universe. Over many years some millisecond pulsars rival the stability of atomic clocks. Comparing observations of many such stable pulsars may allow the first direct detection of gravitational waves, improve the Solar System planetary ephemeris and provide a means to study irregularities in terrestrial time scales. Here we review the goals and status of current and future pulsar timing array projects.
description: To be published in IAU261 proceedings
title: Ð­Ð²Ð¾Ð»ÑÑÐ¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð²Ð¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¸ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ ÑÐ¸ÑÐºÐ° Ð½Ð°Ð²Ð¾Ð´Ð½ÐµÐ½Ð¸Ð¹
title: Evolution of visualisation techniques in flood risk modelling
Creators: name: ÐÐ°ÑÐ¸Ð»ÑÐµÐ², ÐÐ¾Ð½ÑÑÐ°Ð½ÑÐ¸Ð½
name: "Ð¡Ð¸ÑÑÐµÐ¼Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð² Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð°Ñ Ð½Ð°ÑÑÐ½Ð°Ñ Ð¸ ÑÑÐµÐ±Ð½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (25; 2021; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2021
Subjects: ÐÐ¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
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description: ÐÐ¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÐºÐ° Ð½Ð°Ð²Ð¾Ð´Ð½ÐµÐ½Ð¸Ð¹ Ð¾ÑÐµÐ½Ñ Ð²Ð°Ð¶Ð½Ð° Ð´Ð»Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð¿Ð¾Ð½Ð¸Ð¼Ð°Ð½Ð¸Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐ¼Ð¸ Ð·Ð°Ð¸Ð½ÑÐµÑÐµÑÐ¾Ð²Ð°Ð½Ð½ÑÐ¼Ð¸ ÑÑÐ¾ÑÐ¾Ð½Ð°Ð¼Ð¸ Ð·Ð½Ð°ÑÐ¸Ð¼Ð¾ÑÑÐ¸ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÐ¸ÑÐºÐ° Ð½Ð°Ð²Ð¾Ð´Ð½ÐµÐ½Ð¸Ð¹ Ð¸ Ð¿Ð¾Ð¼Ð¾Ð³Ð°ÐµÑ Ð´Ð¾Ð½ÐµÑÑÐ¸ Ð´Ð¾ Ð½Ð¸Ñ Â«Ð¿Ð»ÑÑÑÂ» Ð¸ Â«Ð¼Ð¸Ð½ÑÑÑÂ» Ð¼ÐµÑ Ð¿Ð¾ ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ñ ÑÐ¸ÑÐºÐ° Ð½Ð°Ð²Ð¾Ð´Ð½ÐµÐ½Ð¸Ð¹. Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÑÐ°ÑÑÐµ Ð°Ð²ÑÐ¾Ñ Ð·Ð½Ð°ÐºÐ¾Ð¼Ð¸Ñ ÑÐ¸ÑÐ°ÑÐµÐ»Ñ Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐ¼Ð¸ ÑÑÐ°Ð¿Ð°Ð¼Ð¸ ÑÐ²Ð¾Ð»ÑÑÐ¸Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð²Ð¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¸ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ ÑÐ¸ÑÐºÐ° Ð½Ð°Ð²Ð¾Ð´Ð½ÐµÐ½Ð¸Ð¹. Ð ÐºÐ¾Ð½ÑÐµ ÑÐ°Ð±Ð¾ÑÑ Ð°Ð²ÑÐ¾Ñ ÑÐ°ÐºÐ¶Ðµ Ð´ÐµÐ»Ð¸ÑÑÑ Ð¼ÑÑÐ»ÑÐ¼Ð¸ Ð¾ ÑÐ¾Ð¼, ÐºÐ°Ðº Ð² Ð±ÑÐ´ÑÑÐµÐ¼ Ð¸Ð·Ð¼ÐµÐ½ÑÑÑÑÑ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ Ðº Ð²Ð¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿Ð¾Ð´Ð¾Ð±Ð½ÑÑ Ð¼Ð¾Ð´ÐµÐ»ÐµÐ¹.
description: Visualisation of the results of flood risk simulations is very important for increasing the appreciation of various stakeholders of the importance of understanding flood risk and helps convey to them the pros and cons of flood risk mitigation measures. In this paper, author takes you through the main milestones in evolution of visualisation techniques in flood risk modelling. In the end the author also provides thoughts on what the future holds for visualisation of such an output.
Even-odd effects in the $J_1-J_2$ SU($N$) Heisenberg spin chain
Creators: name: Herviou, Loïc
name: Capponi, Sylvain
name: Lecheminant, Philippe
Publisher: name: arXiv
Year: 2023
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The zero-temperature phase diagram of the $J_1-J_2$ SU($N$) antiferromagnetic Heisenberg spin chain is investigated by means of complementary field theory and numerical approaches for general $N$. A fully gapped SU($N$) valence bond solid made of $N$ sites is formed above a critical value of $J_2/J_1$ for all $N$. We find that the extension of this $N$-merized phase for larger values of $J_2$ strongly depends on the parity of $N$. For even $N$, the phase smoothly interpolates to the large $J_2$ regime where the model can be viewed as a zigzag SU($N$) two-leg spin ladder. The phase exhibits both a $N$-merized ground state and incommensurate spin-spin correlations. In stark contrast to the even case, we show that the $N$-merized phase with odd $N$ only has a finite extent with no incommensuration. A gapless phase in the SU($N$)$_1$ universality class is stabilized for larger $J_2$ that stems from the existence of a massless renormalization group flow from SU($N$)$_2$ to SU($N$)$_1$ conformal field theories when $N$ is odd.
description: Final version
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐ¾ÐµÐºÑÐ° Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð¾Ð±ÑÐµÐ¼Ð° Ð¿ÑÐ¾Ð´Ð°Ð¶ Ð² ÑÑÐµÑÐµ ÐºÐ¾Ð½ÑÐ°Ð»ÑÐ¸Ð½Ð³Ð¾Ð²ÑÑ ÑÑÐ»ÑÐ³ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐ Â«ÐÐ°Ð´Ð°ÑÂ»)
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»ÑÐ³Ð°Ð»Ð¸Ð½Ð°, ÐÐ»ÐµÐ½Ð°
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: ÐºÐ¾Ð½ÑÐ°Ð»ÑÐ¸Ð½Ð³Ð¾Ð²ÑÐµ ÑÑÐ»ÑÐ³Ð¸
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Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¿ÑÐ¾ÐµÐºÑÑ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«ÐÐ Â«ÐÐ°Ð´Ð°ÑÂ». Ð¦ÐµÐ»ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÐ²Ð»ÑÐµÑÑÑ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð·, Ð²ÐºÐ»ÑÑÐ°ÑÑÐ¸Ð¹ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, ÐµÐ³Ð¾ ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð²Ð¸Ð´ÐµÐ½Ð¸Ñ, Ð´Ð»Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð¾Ð±ÑÐµÐ¼Ð° Ð¿ÑÐ¾Ð´Ð°Ð¶.
On the Use of the Microtremor HVSR for Tracking Velocity Changes: A case study in Campo de Dalías basin (SE Spain)
Creators: name: Seivane, Helena
name: García-Jerez, Antonio
name: Navarro, Manuel
name: Molina, Luis
name: Navarro-Martínez, Francisco
Publisher: name: arXiv
Year: 2022
Subjects: subject: Geophysics (physics.geo-ph)
subject: FOS: Physical sciences

description: The stability of the low-frequency peaks (< 1 Hz) obtained in the passive seismic survey of Campo de Dalías basin (CDB) by applying the horizontal-to-vertical spectral ratio (HVSR) method was investigated. Three temporary seismic stations were installed in remote sites that enabled studying the stationarity of their characteristic microtremor HVSR (MHVSR) shapes. All stations began to operate in mid-2016 and recorded at least one year of continuous seismic ambient noise data, having up to two years in some. Each seismic station counted with a monitored borehole in their vicinity, registering the groundwater level every 30 minutes. The MHVSR curves were calculated for time windows of 150 s and averaged hourly. Four parameters have been defined to characterize the shape of the MHVSR around the main peak and to compare them with several environmental variables. Correlations between MHVSR characteristics and the groundwater level showed to be the most persistent. The robustness of MHVSR method for applications to seismic engineering was not found to be compromised since the observed variations were within the margins of acceptable deviations. Our results widen the possibilities of the MHVSR method from being a reliable predictor for seismic resonance to also being an autonomous monitoring tool, especially sensitive to the S-wave modifications.
description: 63 pages, 19 figures
Superconductivity and the Effects of Pressure and Structure in Single Crystalline SrNi$_2$P$_2$
Creators: name: Ronning, F.
name: Bauer, E. D.
name: Park, T.
name: Baek, S. -H
name: Sakai, H.
name: Thompson, J. D.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Heat capacity, magnetic susceptibility, NMR, and resistivity of SrNi2P2 single crystals are presented, illustrating a purely structural transition at 325 K with no magnetism. Bulk superconductivity is found at 1.4 K. The magnitude of the transition temperature T_c, fits to the heat capacity data, the small upper critical field $H_{c2}$ = 390 Oe, and Ginzburg-Landau parameter $κ$ = 2.1 suggests a conventional fully gapped superconductor. With applied pressure a second structural phase transition occurs which results in an 8% reduction in the c/a ratio of lattice parameters. We find that superconductivity persists into this high pressure phase, although the transition temperature is monotonically suppressed with increasing pressure. Comparison of these Ni-P data as well as layered Fe-As and Ni-As superconductor indicates that reduced dimensionality can be a mechanism for increasing the transition temperature.
description: 6 pages, 7 figures, New Title, minor changes, published in PRB as an editor's suggestion
Deep JHKs and Spitzer Imaging of Four Isolated Molecular Cloud Cores
Creators: name: Chapman, Nicholas L.
name: Mundy, Lee G.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present observations in eight wavebands from 1.25-24 microns of four dense cores: L204C-2, L1152, L1155C-2, and L1228. Our goals are to study the YSO population of these cores and to measure the mid-infrared extinction law. With our combined near-infrared and Spitzer photometry, we classify each source in the cores as, among other things, background stars, galaxies, or embedded young stellar objects (YSOs). L1152 contains three YSOs and L1228 has seven, but neither L204C-2 nor L1155C-2 appear to contain any YSOs. We estimate an upper limit of 7x10^-5 to 5x10^-4 solar luminosities for any undiscovered YSOs in our cores. We also compute the line-of-sight extinction law towards each background star. These measurements are averaged spatially, to create chi-squared maps of the changes in the mid-infrared extinction law throughout our cores, and also in different ranges of extinction. From the chi-squared maps we identify two small regions in L1152 and L1228 where the outflows in those cores appear to be destroying the larger dust grains, thus altering the extinction law in those regions. On average, however, our extinction law is relatively flat from 3.6 to 24 microns for all ranges of extinction and in all four cores. From 3.6 to 8 microns this law is consistent with a dust model that includes larger dust grains than the diffuse interstellar medium, which suggests grain growth has occurred in our cores. At 24 microns, our extinction law is 2-4 times higher than predicted by dust models. However, it is similar to other empirical measurements.
description: Accepted by ApJ. 46 pages, 20 figures, 6 tables in preprint format. For a version with full-resolution figures, see http://peggysue.as.utexas.edu/SIRTF/PAPERS/
title: Ð¢Ð¾Ð²Ð°ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð½ÐµÑÑÐ±Ð½ÑÑ Ð¾Ð±ÑÐµÐºÑÐ¾Ð² Ð¿ÑÐ¾Ð¼ÑÑÐ»Ð°
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¨ÐµÐ²ÑÐµÐ½ÐºÐ¾, ÐÐµÑÐ°
name: ÐÐ¸Ð»Ð¸Ð¿ÐµÐ½ÐºÐ¾, Ð¢Ð°ÑÑÑÐ½Ð°
name: ÐÑÑÐ¾Ð½Ð´ÑÑÑÐ¾Ð²Ð°, ÐÑÐ¸Ð½Ð°
name: ÐÐµÑÐµÐ»Ð¾Ð², ÐÐ¸ÐºÐ¾Ð»Ð°Ð¹
Publisher: name: Ð¡ÐÐ±ÐÐ¢Ð­Ð£
Year: 2012
Subjects: Ð¢Ð¾Ð²Ð°ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ
Ð½ÐµÑÑÐ±Ð½ÑÐµ Ð¾Ð±ÑÐµÐºÑÑ
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ðµ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸, Ð²ÑÑÐ°Ð±Ð°ÑÑÐ²Ð°ÐµÐ¼Ð¾Ð¹ Ð¸Ð· Ð½ÐµÑÑÐ±Ð½ÑÑ Ð¾Ð±ÑÐµÐºÑÐ¾Ð² Ð¿ÑÐ¾Ð¼ÑÑÐ»Ð°. ÐÐ¿Ð¸ÑÐ°Ð½Ñ ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ Ð¸ ÑÑÑÐ¾ÐµÐ½Ð¸Ðµ Ð¼Ð¾ÑÐµÐ¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð². Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ¾Ð²Ð°ÑÐ¾Ð²ÐµÐ´Ð½Ð°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½ÑÐ°, ÑÑÐ°Ð½Ð´Ð°ÑÑÐ¸Ð·Ð°ÑÐ¸Ñ Ð¸ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ð° ÐºÐ°ÑÐµÑÑÐ²Ð° Ð½ÐµÑÑÐ±Ð½ÑÑ Ð¾Ð±ÑÐµÐºÑÐ¾Ð² Ð¿ÑÐ¾Ð¼ÑÑÐ»Ð°.
ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ¼Ñ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 100800 Â«Ð¢Ð¾Ð²Ð°ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸ÐµÂ».
L’eclissi che non ti aspetti da 3905 Doppler
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2014

3905 Doppler è stato avvistato per la prima volta nel 1984 nella cintura di asteroidi tra Marte e Giove, ma nessuno gli aveva dato peso. Lo scorso settembre, invece, la scoperta: si tratta di una rara coppia di asteroidi orbitanti l'uno attorno all'altro e che si eclissano a vicenda periodicamente. Un gruppo di ricercatori americani ha tracciato il grafico della loro curva di luce confermando la teoria.
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÐ»Ð¾Ð², ÐÐ½Ð°ÑÐ¾Ð»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: 2017
Subjects: ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼
ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼
Ð¼ÐµÑÐ¾Ð´Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼
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description: Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ Ð½Ð° ÐÐÐ Â«ÐÐ¾ÑÐ²ÐµÑ Ð¡ÐÐÂ» Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ. ÐÐ°Ð½Ð½Ð°Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð°Ð¼ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ Ð² Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸ÑÑ. Ð Ð¿ÐµÑÐ²Ð¾Ð¹ Ð³Ð»Ð°Ð²Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð¾Ð¿Ð¸ÑÑÐ²Ð°ÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼. ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¹ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ ÐÐÐ Â«ÐÐ¾ÑÐ²ÐµÑ Ð¡ÐÐÂ», Ð¸Ð·ÑÑÐ°ÐµÑÑÑ ÑÑÑÑÐºÑÑÑÐ° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ, ÐºÐ°Ð´ÑÐ¾Ð²ÑÐ¹ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð» Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð ÑÑÐµÑÑÐµÐ¹ Ð³Ð»Ð°Ð²Ðµ Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÑÑÑÑ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼.
title: Ð Ð°ÑÑÐµÑ Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾Ð´ÑÐ¸Ð¿Ð½Ð¸ÐºÐ¾Ð² ÑÐºÐ¾Ð»ÑÐ¶ÐµÐ½Ð¸Ñ, ÑÐ°Ð±Ð¾ÑÐ°ÑÑÐ¸Ñ Ð¿ÑÐ¸ Ð³ÑÐ°Ð½Ð¸ÑÐ½Ð¾Ð¹ ÑÐ¼Ð°Ð·ÐºÐµ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÑÐµÐ¹ÑÐ¸Ðº, ÐÐ½Ð°ÑÐ¾Ð»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: 2018
Subjects: ÐÐ¾Ð´ÑÐ¸Ð¿Ð½Ð¸ÐºÐ¸ ÑÐºÐ¾Ð»ÑÐ¶ÐµÐ½Ð¸Ñ

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ 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¸Ð½Ñ Â«Ð­ÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð°Ñ Ð¼ÐµÑÐ°Ð½Ð¸ÐºÐ°Â». Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÐ°ÑÑÐµÑÐ° Ð¿Ð¾Ð´ÑÐ¸Ð¿Ð½Ð¸ÐºÐ¾Ð² ÑÐºÐ¾Ð»ÑÐ¶ÐµÐ½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÐ°ÑÑÐ¸Ñ Ð¿ÑÐ¸ Ð³ÑÐ°Ð½Ð¸ÑÐ½Ð¾Ð¹ ÑÐ¼Ð°Ð·ÐºÐµ Ð¿ÑÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¶Ð¸Ð´ÐºÐ¸Ñ Ð¸ Ð¿Ð»Ð°ÑÑÐ¸ÑÐ½ÑÑ ÑÐ¼Ð°Ð·Ð¾ÑÐ½ÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð². Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ°ÐºÐ¶Ðµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² Ð´Ð»Ñ Ð¿Ð¾Ð´ÑÐ¸Ð¿Ð½Ð¸ÐºÐ¾Ð² ÑÐºÐ¾Ð»ÑÐ¶ÐµÐ½Ð¸Ñ Ð¸ Ð¼ÐµÑÐ¾Ð´Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð¸Ð·Ð½Ð¾ÑÐ¾ÑÑÐ¾Ð¹ÐºÐ¾ÑÑÐ¸ ÑÑÐ¸Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÐµÐ½Ð¸Ñ Ð¸Ð·Ð±Ð¸ÑÐ°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÐµÑÐµÐ½Ð¾ÑÐ°, Ð² ÑÐ°ÑÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð°Ð½ÑÐ¸ÑÑÐ¸ÐºÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð¿Ð¾Ð»Ð¸Ð°Ð¼Ð¸Ð´Ð½ÑÑ Ð¿Ð¾ÐºÑÑÑÐ¸Ð¹, Ð¿Ð¾Ð»Ð¸ÑÐµÑÑÐ°ÑÑÐ¾ÑÑÑÐ¸Ð»ÐµÐ½Ð¾Ð² Ð¸ ÑÐµÐ·Ð¸Ð½. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ ÐºÑÑÑ Â«Ð­ÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð°Ñ Ð¼ÐµÑÐ°Ð½Ð¸ÐºÐ°Â» Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 15.04.01 Â«ÐÐ°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸ÐµÂ».
Esopianeti, dite ‘cheese’
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2014

E' operativo lo strumento installato al telescopio Gemini South in Cile e capace di produrre immagini dirette di esopianeti di grande taglia. Le sue prime dettagliatissime riprese, una di Beta Pictoris b e l'altra del disco di polveri attorno alla giovane stella sono state presentate al 223esimo meeting dell'American Astronomical Society.
title: ÐÑÐµÐ½ÐºÐ° Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸Ð»ÐµÑ, ÐÐ°Ð²ÐµÐ»
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¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð» Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
Ð¾ÑÐµÐ½ÐºÐ° Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°
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enterprise potential
personel assessment
competitiveness of the enterprise

description: ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð° Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿ÑÑÐ¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÐ¾Ð²Ð½Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð°. Ð¡ÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð°. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¸ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. ÐÐµÑÐ¾Ð´Ñ Ð¾ÑÐµÐ½ÐºÐ¸ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ ÑÑÐ»ÑÐ³ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð° Ð¿ÑÐ¾ÑÐµÐ´ÑÑÐ° Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð°. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð°ÑÐ¿ÐµÐºÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð¾Ð¼, ÑÑÑÐ½Ð¾ÑÑÑ Ð¸ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¾ÑÐµÐ½ÐºÐ¸ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐµÐ¹ Ð¸ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°, ÑÑÑÑÐºÑÑÑÐ° Ð·Ð°Ð´Ð°Ñ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°, Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿ÑÐ°ÐºÑÐ¸ÐºÐ¸ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð¿ÑÐ¸ Ð½Ð°Ð¹Ð¼Ðµ Ð¸ Ð¾ÑÐ±Ð¾ÑÐµ.
description: Presents an analysis of production potential of industrial enterprise. The ways of increasing the level of productive capacity. Comparison of methods of assessment of the industrial potential. The evaluations and approaches of the industrial enterprise. Methods of estimation of competitiveness of services of the enterprises. The procedure of evaluation capacity. Presents the theoretical aspects of management capabilities, the nature and the assessment of the capabilities and performance of the personnel, structure, tasks of personnel assessment, analysis of assessment practices of staff recruitment and selection.
Alla ricerca dei viaggiatori nel tempo sul web
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2014

Alcuni ricercatori della Michigan Technological University hanno deciso di cercare le prove dell'esistenza dei viaggiatori del tempo sui social network. La strategia proposta si basa sul principio della preveggenza: chi proviene dal futuro conosce già gli eventi prima che accadano. Quali sono stati i risultati della loro ricerca? L'articolo presentato all’American Astronomical Society meeting del 6 gennaio a Washington e il commento di Maria Teresa Crosta dell'INAF - Osservatorio Astrofisico di Torino.
Strong obstruction of the Berends-Burgers-van Dam spin-3 vertex
Creators: name: Bekaert, Xavier
name: Boulanger, Nicolas
name: Leclercq, Serge
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In the eighties, Berends, Burgers and van Dam (BBvD) found a nonabelian cubic vertex for self-interacting massless fields of spin three in flat spacetime. However, they also found that this deformation is inconsistent at higher order for any multiplet of spin-three fields. For arbitrary symmetric gauge fields, we severely constrain the possible nonabelian deformations of the gauge algebra and, using these results, prove that the BBvD obstruction cannot be cured by any means, even by introducing fields of spin higher (or lower) than three.
description: 19 pages, no figure
Calibration of photometry from the Gemini Multi-Object Spectrograph on Gemini North
Creators: name: Jorgensen, Inger
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: All available observations of photometric standard stars obtained with the Gemini Multi-Object Spectrograph at Gemini North in the period from August 2001 to December 2003 have been used to establish the calibrations for photometry obtained with the instrument. The calibrations presented in this paper are based on significantly more photometric standard star observations than usually used by the individual users. Nightly photometric zero points as well as color terms are determined. The color terms are expected to be valid for all observations taken prior to UT 2004 November 21 at which time the Gemini North primary mirror was coated with silver instead of aluminum. While the nightly zero points are accurate to 0.02 mag or better (random errors), the accuracy of the calibrations is limited by systematic errors from so-called "sky concentration", an effect seen in all focal reducer instruments. We conclude that an accuracy of 0.035 to 0.05 mag can be achieved by using calibrations derived in this paper. The color terms are strongest for very red objects, e.g. for objects with (r'-z')=3.0 the resulting z' magnitudes will be ~0.35 mag too bright if the color term is ignored. The calibrations are of importance to the large Gemini user community with data obtained prior to UT 2004 November 21, as well as future users of achive data from this period in time.
description: Accepted for publication in Publications of the Astronomical Society of Australia, 13 pages, 8 figures, emulateapj format
Washington: summit mondiale per lo spazio
Creators: Giovanni Bignami
Publisher: name: Media Inaf
Year: 2014

Nei prossimi giorni i vertici delle agenzie spaziali di tutto il mondo si incontreranno nella capitale degli Stati Uniti per tornare a discutere, dopo alcuni anni, del futuro dell'esplorazione spaziale. Dopo anni di crisi è il momento di tornare a gaurdare avanti, ad affrontare sfide difficili ma possibili, che possono essere vinte solo con la partecipazione di tutti.
Raggi gamma per lente gravitazionale
Creators: Francesca Aloisio
Publisher: name: Media Inaf
Year: 2014

Prime osservazioni in assoluto nei raggi gamma di una lente gravitazionale. Ad ottenerle il satellite della NASA, con forte partecipazione italiana, Fermi. Un risultato importante che apre nuove strade alla ricerca, in particolare le osservazioni di regioni di emissioni vicine ai buchi neri supermassicci.
Characteristic Lengths of Magnetic Field in Magnetohydrodynamic Turbulence
Creators: name: Cho, Jungyeon
name: Ryu, Dongsu
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: In the framework of turbulence dynamo, flow motions amplify a weak seed magnetic field through the stretching of field lines. Although the amplification process has been a topic of active research, less attention has been paid to the length scales of magnetic field. In this paper, we described a numerical study on characteristic lengths of magnetic field in magnetohydrodynamic turbulence. We considered the case of very weak or zero mean magnetic field, which is applicable to the turbulence in the intergalactic space. Our findings are as follows. (1) At saturation, the peak of magnetic field spectrum occurs at $\sim L_0/2$, where $L_0$ is the energy injection scale, while the most energy containing scale is $\sim L_0/5$. The peak scale of spectrum of projected, two-dimensional field is $\sim L_0$. (2) During the stage of magnetic field amplification, the energy equipartition scale shows a power-law increase of $\sim t^{1.5}$, while the integral and curvature scales show a linear increase. The equipartition, integral, and curvature scales saturate at $\sim L_0$, $\sim 0.3L_0$, and $\sim 0.15L_0$, respectively. (3) The coherence length of magnetic field defined in the Faraday rotation measure (RM) due to the intergalactic magnetic field (IGMF) is related to the integral scale. We presented a formula that expresses the standard deviation of RM, $σ_{RM}$, in terms of the integral scale and rms strength of the IGMF, and estimated that $σ_{RM}$ would be $\sim 100$ and $\sim$ a few rad m$^{-2}$ for clusters and filaments, respectively.
description: To appear in ApJ Letters; published version
title: Ð¤ÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÐµ Ð¸ Ð¿ÑÐ¸ÐºÐ»Ð°Ð´Ð½ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ, ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð¸ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸. Ð§. 2
title: ÑÐ±Ð¾ÑÐ½Ð¸Ðº ÑÑÑÐ´Ð¾Ð² Ð²ÑÐµÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð½Ð°ÑÑÐ½Ð¾Ð¹ Ð¸ ÑÑÐµÐ±Ð½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸
titleType: Subtitle
Creators: name: "Ð¤ÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÐµ Ð¸ Ð¿ÑÐ¸ÐºÐ»Ð°Ð´Ð½ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ, ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð¸ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸", Ð²ÑÐµÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ°Ñ Ð½Ð°ÑÑÐ½Ð°Ñ Ð¸ ÑÑÐµÐ±Ð½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (2020; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2020
Subjects: Ð½Ð°ÑÑÐ½ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°
Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ
ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ñ

description: Ð ÑÐ±Ð¾ÑÐ½Ð¸ÐºÐµ Ð¿ÑÐ±Ð»Ð¸ÐºÑÑÑÑÑ ÑÑÐ°ÑÑÐ¸ Ð¿Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°Ð¼ Ð´Ð¾ÐºÐ»Ð°Ð´Ð¾Ð², Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÑ Ð½Ð° ÑÐµÐºÑÐ¸Ð¾Ð½Ð½ÑÑ Ð·Ð°ÑÐµÐ´Ð°Ð½Ð¸ÑÑ Ð½Ð°ÑÑÐ½Ð¾Ð¹ Ð¸ ÑÑÐµÐ±Ð½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸ Â«Ð¤ÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÐµ Ð¸ Ð¿ÑÐ¸ÐºÐ»Ð°Ð´Ð½ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ, ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð¸ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸Â». Ð¡ÑÐ°ÑÑÐ¸ Ð¾ÑÑÐ°Ð¶Ð°ÑÑ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐ¹ ÑÑÐ¾Ð²ÐµÐ½Ñ
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ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð½Ð° Ð¼Ð¸ÐºÑÐ¾- Ð¸ Ð¼Ð°ÐºÑÐ¾ÑÑÐ¾Ð²Ð½ÑÑ, ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð±Ð¸Ð·Ð½ÐµÑÐ¾Ð¼.
Archaeocyatha from the Colville and Salmo area of Washington and British Columbia
Creators: name: Greggs, Robert G.
Publisher: name: University of British Columbia
Year: 2012

description: Archaeocyathids are an extinct group of animals that lived and thrived in the warm, clear marine waters of the Lower Cambrian. In general shape, they resemble rugose corals, but in skeletal details, numerous differences between these groups exist, i.e. inner and outer walls, central cavities, parieties, etc. are unique to Archaeocyathids. The Archaeocyathids which are the subject of this thesis were collected by Dr. H. Little from the South Fork of the Salmo River, and from north of Colville, Washington. In the Salmo area, they occur in a narrow band of limestone at the base of the Laib group. The Colville collection is from an outcrop of Old Dominion limestone. The identification and description of the species present in these collections are the main considerations of the thesis. Two new species are described, Ethmophyllum lineatus and Syringocnema colvillensis. The former species occurs in the Lower Cambrian limestone of the Laib group, Salmo area; the latter is reported from the Old Dominion limestone of the Colville area. Archaeocyathids may be useful in the correlation of Lower Cambrian formations, providing further accurately located (stratigraphically) collections are made. At present, insufficient stratigraphic data are available to erect Archaeocyathid zones. However, some attempt to correlate the known Archaeocyathid occurrences is made. In correlating the ten known Archaeocyathid occurrences from Washington to the Yukon Territory, it is suggested that the most southerly, Colville, Washington, is stratigraphically lower than the Salmo occurrence, and that the latter is, in turn, stratigraphically lower than the northern localities. These northern occurrences are considered to be late Lower Cambrian. The age assigned to the northern localities is, in general, based on stratigraphic and paleontological evidence other than that afforded by Archaeocyathids. The occurrences of Archaeocyathids in the northern part of the Cordillera are given below with their related lithologic unit where possible: 1) Colville, Washington - Old Dominion limestone 2) Salmo, B.C. - lower part of the Laib group 3) Dogtooth Range, B.C. - Donald formation 4) Quesnel Lake, B.C. - Cariboo series 5) Sinclair Mills, B.C. - 6) Pine Pass, B.C. - Misinchinka schists 7) Aiken Lake, B.C. - upper Wolverine complex 8) McDame Creek, B.C. - Atan group 9) Wolf Lake, Yukon Territory - Lord's group B and c units 10) Quiet Lake, Yukon Territory – It is believed that these occurrences outline the western edge of the geosyncline present in this region in Lower Cambrian time.
Topological metals constructed by sliding quantum wire arrays
Creators: name: Zuo, Zheng-Wei
name: Lv, Linxi
name: Kang, Dawei
Publisher: name: arXiv
Year: 2023
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: A general strategy of alternated slide construction to craft topological metals is proposed, where there is a relative slide between the odd and even chains in the trivial spinless quantum wire array. Firstly, taking the three-leg ladder as an example, we find that alternated slide can induce a topological phase transition from the normal metal to topological metal phases, which are protected by inversion symmetry. Remarkably, topological metal without nontrivial edge states is found, and the bulk-boundary correspondence breaks down. Secondly, the two-dimensional quantum wire arrays with alternated slide manifests similar physical behaviors. Two types of topological metal phases emerge, where there are gapless bulk bands with and without nontrivial edge states. These results could be confirmed by current experimental techniques.
description: 6 pages, 5 figures
Approaches to systematic transaction data reuse: machine learning support of information discovery
Creators: name: Hahn, Jim
Publisher: name: F1000 Research Limited
Year: 2019

description: The purpose of this poster is to detail approaches in systematic transactional data reuse using machine learning and network science visualization methods. Preliminary machine learning workflows were undertaken in WEKA and made use of the Fp-growth algorithm for seeding a recommender system for library user accounts. The resulting tables of consequent association rules are stored in a production relational database server accessed through the recommender app’s middleware. The association rule database is used at runtime for the machine learning based recommender system. As a result of the availability of databases with association rules, researchers further analyzed their properties using network analysis software were the edges of the graph are the consequent topics and the nodes are the antecedent topics. Network science can be particularly valuable in assisting the understanding of machine learning outputs by visualizing and analyzing graphs the distribution of the topic network. Several key network science metrics, including the average degree, diameter, average clustering coefficient, and total triangles were computed by way of Gephi network analytic tools.