cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Smash-nilpotent cycles on abelian 3-folds
Creators: name: Kahn, Bruno
name: Sebastian, Ronnie
Publisher: name: arXiv
Year: 2009
Subjects: subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics
subject: 14C15, 14K05

description: We show that homologically trivial algebraic cycles on a 3-dimensional abelian variety are smash-nilpotent.
description: To appear in Math. Res. Letters
Studiare il vento solare inseguendo le comete
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2016

Chandra è uno dei tre grandi telescopi orbitanti della NASA ancora attivi, con Hubble e Spitzer. Nel 2013 ha osservato nel dettaglio due famose comete per analizzare il comportamento del flusso di particelle che proviene dal Sole
The photochemistry of aldehydes in the gaseous phase
Creators: name: Sifniades, Stylianos
Publisher: name: University of British Columbia
Year: 2011

description: The object of the present work was the investigation of two separate topics, the investigation of the radical-radical termination step in the photochemical oxidation of acetaldehyde and the investigation of the photolysis of crotonaldehyde, both in the gas phase and at room temperature. A third topic, the photolysis of 3-butene-1-al, was investigated in the course of the work, in order to provide evidence in favour of the mechanism proposed for the photolysis of crotonaldehyde. In the first part of the work, mixtures of acetaldehyde and isotopically enriched oxygen containing argon as a reference gas were irradiated at 25°C with light at a wavelength of 3130 [formula omitted] and the reaction products were analyzed by gas chromatography and mass spectrometry. The major products were found to be peracetic acid and diacetyl peroxide. By following the rate of formation of these products, as well as the concentrations of the three possible kinds of oxygen in the reaction mixture, it was possible to verify McDowell and Farmer's mechanism for the photooxidation of acetaldehyde and establish a satisfactory mechanism for the chain terminating step of the reaction. In the second part of the work, crotonaldehyde was irradiated at 30°C with light at a wavelength of 2450-4000 [formula omitted], and the products analyzed by gas chromatography and infra-red spectroscopy. The only product in experiments of short duration was found to be 3-butene-1-al, thus establishing isomerization as the primary process of the reaction. In later stages CO, propylene and 1,5-hexadiene were formed. The following experimental laws were found to hold for the rate of formation of these products: d(3-butene-1-al)/dt = ႴIabs , Ⴔ = 0.095 ± 0.005 d(1, 5-hexadiene)/dt ∼ (Iabs².t)/(crotonaldehyde ) d(propylene )/dt ∼ (Iabs².t)/(crotonaldehyde)1.3-1.5 No detailed law was established for the rate of formation of CO, but whenever measured it was found to follow closely the propylene formation. These experimental laws were interpreted by means of a mechanism, in which crotonaldehyde participates in so far as it isomerizes to 3-butene-1-al. The latter was assumed to yield the three other products of the reaction through a mixed radical-molecular photochemical dissociation. Evidence was provided in favour of the proposed mechanism by studying the photolysis of 3-butene-1-al at 30°C and a wavelength of 2450-4000 [formula omitted]. The products of the reaction were found to be propylene, 1,5-hexadiene and CO, with their rates of formation obeying the following laws: d(1,5-hexadiene)/dt = Ⴔhexad. Iabs , Ⴔhexad = 0.135 ± 0.0318 d(propylene)/dt = Ⴔprop‧Iabs , Ⴔprop = 0.79 ± 0.05 CO formation was found to be approximately equal to propylene formation. These experimental laws were interpreted by means of a mixed radical-molecular photochemical dissociation of 3-butene-1-al, thus justifying the mechanism proposed for the photolysis of crotonaldehyde.
ExoMars, tra l’Italia e Marte
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2016

Il 14 marzo scorso è stata lanciata dal cosmodromo di Baikonur, in Kazakistan, la prima delle due missioni ExoMars, che arriverà per la metà di ottobre prossimo in orbita attorno a Marte. A bordo della missione il Trace Gas Orbiter e il lander Schiaparelli, per saperne di più su questa missione abbiamo organizzato una chiacchierata in diretta con due delle protagoniste della missione: Francesca Esposito dell’Osservatorio Astronomico di Capodimonte e Francesca Ferri dell’Università di Padova
Fast Hamiltonian sampling for large scale structure inference
Creators: name: Jasche, J.
name: Kitaura, F. S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: In this work we present a new and efficient Bayesian method for nonlinear three dimensional large scale structure inference. We employ a Hamiltonian Monte Carlo (HMC) sampler to obtain samples from a multivariate highly non-Gaussian lognormal Poissonian density posterior given a set of observations. The HMC allows us to take into account the nonlinear relations between the observations and the underlying density field which we seek to recover. As the HMC provides a sampled representation of the density posterior any desired statistical summary, such as the mean, mode or variance, can be calculated from the set of samples. Further, it permits us to seamlessly propagate non-Gaussian uncertainty information to any final quantity inferred from the set of samples. The developed method is extensively tested in a variety of test scenarios, taking into account a highly structured survey geometry and selection effects. Tests with a mock galaxy catalog based on the millennium run show that the method is able to recover the filamentary structure of the nonlinear density field. The results further demonstrate the feasibility of non-Gaussian sampling in high dimensional spaces, as required for precision nonlinear large scale structure inference. The HMC is a flexible and efficient method, which permits for simple extension and incorporation of additional observational constraints. Thus, the method presented here provides an efficient and flexible basis for future high precision large scale structure inference.
description: 14 pages, 7 figures
title: ÐÐ¿ÐµÑÐ°ÑÐ¸Ð²Ð½ÑÐµ Ð¿ÐµÑÐµÐºÐ»ÑÑÐµÐ½Ð¸Ñ Ð² ÑÐ»ÐµÐºÑÑÐ¾ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ°Ñ ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°Ð½ÑÐ¸Ð¹ Ð¸ Ð¿Ð¾Ð´ÑÑÐ°Ð½ÑÐ¸Ð¹
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°Ð¿Ð¸Ð´ÑÑ, ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
name: Ð¡ÐµÐ¼ÐµÐ½Ð¾Ð², ÐÐ¾Ð½ÑÑÐ°Ð½ÑÐ¸Ð½
name: Ð¡Ð¾Ð»Ð¾Ð²ÑÐµÐ²Ð°, Ð¡Ð²ÐµÑÐ»Ð°Ð½Ð°
name: Ð¨Ð°ÑÐ¾Ð²Ð°, ÐÐ°ÑÐ¸Ñ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2023
Subjects: Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸
Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÑÐ°Ð½ÑÐ¸Ð¸
Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾Ð´ÑÑÐ°Ð½ÑÐ¸Ð¸

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼Ñ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ´ÐµÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð°Ð²ÑÐ¾Ð½Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸Ñ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Â«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¸ÐºÐ¾Ð³Ð¾Â» Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² 13.03.02 Â«Ð­Ð»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ° Ð¸ ÑÐ»ÐµÐºÑÑÐ¾ÑÐµÑÐ½Ð¸ÐºÐ°Â», Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ð°Ð¼ Â«Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÑÐ°Ð½ÑÐ¸Ð¸ Ð¸ Ð¿Ð¾Ð´ÑÑÐ°Ð½ÑÐ¸Ð¸Â», Â«Ð ÐµÐ¶Ð¸Ð¼Ñ ÑÐ°Ð±Ð¾ÑÑ ÑÐ»ÐµÐºÑÑÐ¾Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°Ð½ÑÐ¸Ð¹ Ð¸ Ð¿Ð¾Ð´ÑÑÐ°Ð½ÑÐ¸Ð¹Â», Â«Ð­ÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ñ ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°Ð½ÑÐ¸Ð¹Â». Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¿ÑÐ°Ð²Ð¸Ð»Ð° Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð²Ð½ÑÑ Ð¿ÐµÑÐµÐºÐ»ÑÑÐµÐ½Ð¸Ð¹ Ð² ÑÐ»ÐµÐºÑÑÐ¾ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ°Ñ ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°Ð½ÑÐ¸Ð¹ Ð¸ Ð¿Ð¾Ð´ÑÑÐ°Ð½ÑÐ¸Ð¹. Ð Ð°ÑÐºÑÑÐ²Ð°ÑÑÑÑ Ð¿ÑÐ¸ÑÐ¸Ð½Ñ ÑÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÑÐ´ÐºÐ° Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹ ÐºÐ¾Ð¼Ð¼ÑÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐ¼Ð¸ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÐ°Ð¼Ð¸. ÐÑÐ²ÐµÑÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð²ÑÐ²Ð¾Ð´Ð° Ð² ÑÐµÐ¼Ð¾Ð½Ñ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÐµÐ¼Ñ Ð´Ð»Ñ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÑÑÑÐ¾Ð¹ÑÑÐ² ÑÐ°Ð·Ð»Ð¸ÑÐ½Ð¾Ð³Ð¾ ÑÐ¸Ð¿Ð°. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ¾Ð² Ð²ÑÐ·Ð¾Ð².
Neutroni contro il contrabbando nucleare
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2016

Proprio mentre dagli Stati Uniti arriva l'allarme per una nuova generazione di ordigni nucleari, viene descritta oggi sulle pagine di “Scientific Reports” una tecnica di imaging per reazioni a bassa energia progettata per rilevare la presenza di materiale fissile
Al via la finale delle Olimpiadi di Astronomia
Creators: Livia Giacomini
Publisher: name: Media Inaf
Year: 2016

Dal 19 al 21 aprile si svolge a Milano la finale nazionale delle Olimpiadi italiane di Astronomia. La premiazione dei dieci vincitori si terrà giovedì 21 al Museo della Scienza e della Tecnologia “Leonardo Da Vinci”
Pseudogeoplana Ogren & Kawakatsu 1990
Creators: name: Carbayo, Fernando
name: Álvarez-Presas, Marta
name: Cĺaudia T. Olivares
name: Marques, Fernando P. L.
name: Eud Óxia M. Froehlich
name: Riutort, Marta
Publisher: name: Zenodo
Year: 2013
Subjects: Biodiversity
Taxonomy
Animalia
Platyhelminthes
Turbellaria
Tricladida
Geoplanidae
Pseudogeoplana

description: Genus Pseudogeoplana Ogren & Kawakatsu, 1990 Pseudogeoplana arpi (Schirch, 1929) comb. n. Pseudogeoplana blaseri (Schirch, 1929) comb. n. Pseudogeoplana bresslaui (Schirch, 1929) comb. n. Pseudogeoplana elegans (Darwin, 1944) comb. n.
description: Published as part of Fernando Carbayo, Marta Álvarez-Presas, Cĺaudia T. Olivares, Fernando P. L. Marques, Eud Óxia M. Froehlich & Marta Riutort, 2013, Molecular phylogeny of Geoplaninae (Platyhelminthes) challenges current classification: proposal of taxonomic actions, pp. 508-528 in Zoologica Scripta 42 on page 524, DOI: 10.5281/zenodo.399812
description: {"references": ["Ogren, R. & Kawakatsu, M. (1990). Index to the species of the family Geoplanidae (Turbellaria, Tricladida, Terricola). Part I: Geoplaninae. Bulletin of the Fuji Women ' s College, 28, 79 - 166.", "Schirch, P. F. (1929). Sobre as planarias terrestres do Brasil. Boletim do Museu Nacional, 5, 27 - 38."]}
Clever people solving difficult problems - perspectives on weakness of state and nation in Papua New Guinea
Creators: name: Regan, Anthony
Publisher: name: Canberra, ACT: State, Society and Governance in Melanesia (SSGM) Program, The Australian National University
Year: 2005
Subjects: Papua New Guinea

description: The ASPI Paper argues that although the state in Papua New Guinea has become extremely weak, it has not failed or collapsed - possibly in contrast with neighbouring Solomon Islands, the subject of an earlier ASPI paper the title of which used the phrase “our failing neighbour (ASPI 2003). Poor and declining standards in delivery of basic services to the people are seen as one of the key measures of weakness. Others include corruption, increasing levels of violence, and a worsening law and order situation. The weakness is so profound that: ‘PNG has now reached the point at which its institutions are too weak themselves to undertake and sustain the kind of major reforms needed to turn the country around. If PNG is going to be strengthened, it is going to need much more help – and different kinds of help – than it has received over the past three decades. If Australia does not take the lead in offering that help, no one else will.’ (ASPI 2004:11)
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐ "ÐÐ¾Ð½ÑÐµÑÐ½ ÐÐÐ "ÐÐ²ÑÐ¾ÑÐ°")
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¨Ð¾Ð»Ð¸Ð½, ÐÐ²Ð°Ð½
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¡ÑÐ´Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾ÑÑÑ
Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸
Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸
ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼
ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¸Ñ
Ð°Ð½Ð°Ð»Ð¸Ð· Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ¹ Ð¸ Ð²Ð½ÐµÑÐ½ÐµÐ¹ ÑÑÐµÐ´Ñ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¼ Ð¿ÑÐ¾ÐµÐºÑÐµ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÐºÐ»ÑÑÐµÐ²ÑÐµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐÐÐ ÐÐ²ÑÐ¾ÑÐ°, ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸, ÑÑÑÑÐºÑÑÑÐ°, ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ, Ð° ÑÐ°Ðº Ð¶Ðµ Ð¼Ð¸ÑÑÐ¸Ñ ÐºÐ¾Ð½ÑÐµÑÐ½Ð°, Ð±ÑÐ»Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ñ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ¹ Ð¸ Ð²Ð½ÐµÑÐ½ÐµÐ¹ ÑÑÐµÐ´Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¿Ð¾ÐºÐ°Ð·Ð°Ð»Ð¸ Ð´Ð¾Ð²Ð¾Ð»ÑÐ½Ð¾ ÑÐ°ÐºÐ¸ ÑÑÐ¿ÐµÑÐ½ÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÐÐ±ÑÐµÑÑÐ²Ð°, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ Ð½ÐµÑÐºÐ¾Ð»ÑÐºÐ¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð¾Ð² ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸ÐµÐ¼. Ð¦ÐµÐ»ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð±ÑÐ»Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°, Ð² ÑÐ¾Ð´Ðµ ÐºÐ¾ÑÐ¾ÑÐ¾Ð³Ð¾ Ð±ÑÐ» Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½ ÐºÐ»Ð°ÑÑ Ð´Ð»Ñ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸, Ð·Ð°ÐºÑÐ¿Ð»ÐµÐ½Ð¾ Ð½Ð¾Ð²ÐµÐ¹ÑÐµÐµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð´Ð»Ñ Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð² Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾ Ð½Ð¾Ð²Ð¾Ð¹ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸, Ð¸ Ñ.Ð´. Ð¢Ð°Ðº Ð¶Ðµ ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ð° ÑÐµÐ»ÐµÑÐ¾Ð¾Ð±ÑÐ°Ð·Ð½Ð¾ÑÑÑ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ°, ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¸ ÑÐ¸ÑÐºÐ¸.
Tunable Kondo-Luttinger systems far from equilibrium
Creators: name: Chung, C. -H.
name: Latha, K. V. P.
name: Hur, K. Le
name: Vojta, M.
name: Woelfle, P.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We theoretically investigate the non-equilibrium current through a quantum dot coupled to one- dimensional electron leads, utilizing a controlled frequency-dependent renormalization group (RG) approach. We compute the non-equilibrium conductance for large bias voltages and address the interplay between decoherence, Kondo entanglement and Luttinger physics. The combined effect of large bias voltage and strong interactions in the leads, known to stabilize two-channel Kondo physics, leads to non-trivial modifications of the conductance. For weak interactions, we build an analogy to a dot coupled to helical edge states of two-dimensional topological insulators.
description: 4 pages, 4 figures
Circumventing the eta problem in building an inflationary model in string theory
Creators: name: Easson, Damien A.
name: Gregory, Ruth
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The eta problem is one of the most significant obstacles to building a successful inflationary model in string theory. Planck mass suppressed corrections to the inflaton potential generally lead to inflaton masses of order the Hubble scale and generate contributions of order unity to the eta slow roll parameter rendering prolonged slow roll inflation impossible. We demonstrate the severity of this problem in the context of brane anti-brane inflation in a warped throat of a Calabi-Yau flux compactification with all phenomenologically dangerous moduli stabilized. Using exact numerical solutions we show that the eta problem can be avoided in scenarios where the inflaton is non-minimally coupled to gravity and has Dirac-Born-Infeld (DBI) kinetic term. We show that the resulting cosmic microwave background (CMB) observables such as measures of non-gaussianites can, in principle, serve as a probe of scalar-gravity couplings.
description: 8 pages, 3 figures; title changed and reference added to match published version in PRD
title: Ð¡Ð¸ÑÑÐµÐ¼Ð½ÑÐ¹ Ð¿Ð¾Ð´Ñ Ð¾Ð´ Ð¿ÑÐ¸ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ð¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð² Ð¥ÐµÐ´Ð¶-Ð¤Ð¾Ð½Ð´Ðµ
title: A systematic approach to making investment decisions in a Hedge fund
Creators: name: ÐÐ¾Ð·Ð»Ð¾Ð²ÑÐºÐ°Ñ, Ð­ÑÐ°
name: Ð¨Ð°ÑÐ¸Ñ, Ð­ÑÐ¼Ð¸Ð½
name: Ð¯ÐºÐ¾Ð²Ð»ÐµÐ²Ð°, ÐÐ°ÑÑÑ
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¡Ð¸ÑÑÐµÐ¼Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð·
ÐÑÐ¸Ð½ÑÑÐ¸Ðµ ÑÐµÑÐµÐ½Ð¸Ð¹
ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ

description: Ð ÑÑÐ°ÑÑÐµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½ ÑÐ¸ÑÑÐµÐ¼Ð½ÑÐ¹ Ð¿Ð¾Ð´ÑÐ¾Ð´ Ð¿ÑÐ¸ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ð¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð² ÑÐµÐ´Ð¶-ÑÐ¾Ð½Ð´Ðµ Ð¸ ÑÐ°ÑÐºÑÑÑÑ ÑÑÐ»Ð¾Ð²Ð¸Ñ, Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¸ ÑÑÐµÐ¼Ð° Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ¸ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐµÐ¾ÑÐ¸Ð¸ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹.
description: The article substantiates a systematic approach to making investment decisions in a hedge fund and reveals the conditions, features and scheme of building a decision support system based on decision theory.
Xerapoa Froehlich 1955
Creators: name: Carbayo, Fernando
name: Álvarez-Presas, Marta
name: Cĺaudia T. Olivares
name: Marques, Fernando P. L.
name: Eud Óxia M. Froehlich
name: Riutort, Marta
Publisher: name: Zenodo
Year: 2013
Subjects: Biodiversity
Taxonomy
Animalia
Platyhelminthes
Turbellaria
Tricladida
Geoplanidae
Xerapoa

description: Genus Xerapoa Froehlich, 1955 Emended diagnosis. Geoplaninae with small-sized body, 15–30 mm in length; thin, subcylindrical body, margins nearly parallel; anterior region raised; sensory pits may open at the tip of small papillae; eyes monolobulated, marginally arranged along the body; creeping sole as wide as one-third of body width; main nervous system two-chords shaped; pharynx cylindrical; ovaries close to the pharynx; ovovitelline ducts with ascending portion, if any, posterior to female atrium and joining each other behind female atrium; genital canal horizontal, arising from the posterior region of female atrium; female atrium small, funnel-shaped. Distribution. States of Stao Paulo, Santa Catarina, in Brazil. Type species. Xerapoa hystrix Froehlich, 1955, designated by Froehlich (1955) Xerapoa species. Xerapoa hystrix Froehlich, 1955 a * Xerapoa una Froehlich, 1955 a Xerapoa pseudorhynchodemus (Riester, 1938) * comb. n. Xerapoa trina (Marcus, 1951) * comb. n.
description: Published as part of Fernando Carbayo, Marta Álvarez-Presas, Cĺaudia T. Olivares, Fernando P. L. Marques, Eud Óxia M. Froehlich & Marta Riutort, 2013, Molecular phylogeny of Geoplaninae (Platyhelminthes) challenges current classification: proposal of taxonomic actions, pp. 508-528 in Zoologica Scripta 42 on page 524, DOI: 10.5281/zenodo.399812
description: {"references": ["Froehlich, C. G. (1955 a). Sobre a morfologia e taxonomia das Geoplanidae. Boletim da Faculdade de Filoso fi a, Ci \u02c6 encias e Letras da Universidade de S t ao Paulo, S\u00b4erie Zoologia, 19, 195 - 279.", "Riester, A. (1938). Beitraege zur Geoplaniden-Fauna Brasiliens. Abhandlungen der Senckenberg Naturforsch Gesellschaft fur \u00a8 Naturforschung, 441, 1 - 88.", "Du Bois-Reymond Marcus, E. (1951). On South American geoplanids. Boletim da Faculdade de Filoso fi a, Ci \u02c6 encias e Letras da Universidade de S t ao Paulo, S\u00b4erie Zoologia, 16, 217 - 255."]}
Congestion in a macroscopic model of self-driven particles modeling gregariousness
Creators: name: Degond, Pierre
name: Navoret, Laurent
name: Bon, Richard
name: Sanchez, David
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We analyze a macroscopic model with a maximal density constraint which describes short range repulsion in biological systems. This system aims at modeling finite-size particles which cannot overlap and repel each other when they are too close. The parts of the fluid where the maximal density is reached behave like incompressible fluids while lower density regions are compressible. This paper investigates the transition between the compressible and incompressible regions. To capture this transition, we study a one-dimensional Riemann problem and introduce a perturbation problem which regularizes the compressible-incompressible transition. Specific difficulties related to the non-conservativity of the problem are discussed.
Non-Annihilation Processes, Fermion-Loop and QED Radiation
Creators: name: G. Passarino
Publisher: name: INFN Open Access Repository
Year: 2001

description: The bulk of large radiative corrections to any process can be obtained by
promoting coupling constants to be running ones and by including QED radiation
at the leading logarithmic level via structure functions evoluted at some
scale. The problem of fixing the proper scale in running coupling constants and
in structure functions for non-annihilation processes is briefly addressed and
the general solution is analyzed.
Are Constants Constant?
Creators: name: G. Passarino
Publisher: name: INFN Open Access Repository
Year: 2001

description: The prospect of a time-dependent Higgs vacuum expectation value is examined
within the standard model of electroweak interactions. It is shown that the
classical equation of motion for the Higgs field admits a solution that is a
doubly-periodic function of time. The corresponding Dirac equation for the
electron field is equivalent to a second order differential equation with
doubly-periodic coefficients. In the limit of very large primitive period of
the Higgs background this equation can be solved in WKBJ approximation, showing
plane-wave solutions with a time-dependent distortion factor which can be made
arbitrarily small.
Bayesian non-linear large scale structure inference of the Sloan Digital Sky Survey data release 7
Creators: name: Jasche, J.
name: Kitaura, F. S.
name: Li, C.
name: Ensslin, T. A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: In this work we present the first non-linear, non-Gaussian full Bayesian large scale structure analysis of the cosmic density field conducted so far. The density inference is based on the Sloan Digital Sky Survey data release 7, which covers the northern galactic cap. We employ a novel Bayesian sampling algorithm, which enables us to explore the extremely high dimensional non-Gaussian, non-linear log-normal Poissonian posterior of the three dimensional density field conditional on the data. These techniques are efficiently implemented in the HADES computer algorithm and permit the precise recovery of poorly sampled objects and non-linear density fields. The non-linear density inference is performed on a 750 Mpc cube with roughly 3 Mpc grid-resolution, while accounting for systematic effects, introduced by survey geometry and selection function of the SDSS, and the correct treatment of a Poissonian shot noise contribution. Our high resolution results represent remarkably well the cosmic web structure of the cosmic density field. Filaments, voids and clusters are clearly visible. Further, we also conduct a dynamical web classification, and estimated the web type posterior distribution conditional on the SDSS data.
description: 18 pages, 11 figures
Высшее образование сегодня,Выпуск 6 2018
Creators: name: Автономная некоммерческая организация высшего образования «Российский новый университет»
Publisher: name: Автономная некоммерческая организация высшего образования «Российский новый университет»
Year: 2018

description: Высшее образование сегодня,Выпуск 6 2018
Primo ruggito per il motore a singolo atomo
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

Un articolo apparso sull'ultimo numero della rivista Science descrive un innovativo motore termico che opera utilizzando un singolo atomo. Il risultato è il frutto del lavoro del team QUANTUM presso l’Istituto di Fisica dell’Università Johannes Gutenberg di Mainz, in collaborazione con i fisici teorici della Friedrich-Alexander-Universität di Erlangen-Norimberga
Atmospheric muons and neutrinos
Creators: name: Naumov, Vadim A.
Publisher: name: INFN Open Access Repository
Year: 2002

description: This paper is a mini-review of the atmospheric muon and neutrino flux
calculations based upon a recent version of CORT code and up-to-date data on
primary cosmic rays and hadronic interactions. A comparison of calculations
with a representative set of atmospheric muon data for momenta below 1 TeV/c is
presented. The overall agreement between the calculated muon fluxes and the
data provides an evidence in favor of the validity of adopted description of
hadronic interactions and shower development. In particular, this supports the
low-energy atmospheric neutrino fluxes predicted with CORT which are
essentially lower than those used in current analyses of the sub-GeV and
multi-GeV neutrino induced events in underground neutrino detectors.
Supersymmetric Quantum Mechanics of Magnetic Monopoles: A Case Study
Creators: name: de Vries, Erik Jan
name: Schroers, Bernd J.
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study, in detail, the supersymmetric quantum mechanics of charge-(1,1) monopoles in N=2 supersymmetric Yang-Mills-Higgs theory with gauge group SU(3) spontaneously broken to U(1) x U(1). We use the moduli space approximation of the quantised dynamics, which can be expressed in two equivalent formalisms: either one describes quantum states by Dirac spinors on the moduli space, in which case the Hamiltonian is the square of the Dirac operator, or one works with anti-holomorphic forms on the moduli space, in which case the Hamiltonian is the Laplacian acting on forms. We review the derivation of both formalisms, explicitly exhibit their equivalence and derive general expressions for the supercharges as differential operators in both formalisms. We propose a general expression for the total angular momentum operator as a differential operator, and check its commutation relations with the supercharges. Using the known metric structure of the moduli space of charge-(1,1) monopoles we show that there are no quantum bound states of such monopoles in the moduli space approximation. We exhibit scattering states and compute corresponding differential cross sections.
description: 38 pages, minor corrections and updates to references
A Living, Controllable Device:The Political Police and Informant Network in Socialist Hungary, 1956-1989
Creators: name: Kisiday, Matyas
Publisher: name: Stanford Digital Repository
Year: 2023
Subjects: subject: Hungary
subject: Socialism
subject: Police--Political activity--History
subject: Soviet Union
subject: Revolution (Hungary : 1956)
subject: Kádár, János, 1912-1989
subject: Eastern Europe

description: After coming to power in the wake of the infamous Hungarian Revolution of 1956, János Kádár built his regime upon a delicate balance between upholding socialist ideals and appeasing a disgruntled, scarred nation. The slogan that became Kádár’s central doctrine perfectly represented this balance: “those who are not against us, are with us.” Existing literature on Kádárist Hungary portrays the period’s stability as a product of the leader’s compromising personality and political cunning. While accurate, these accounts largely neglect the role of Kádár’s political police as a primary organ of two-way interaction between the party and populace. Internal informational documents from the Ministry of the Interior III. reveal that the mass informant network served as the spearhead of interaction between the party and population in the realm of national security, which was viewed as essential to the building of socialism. The informant network’s transformation alongside the political police from a crude, coercive, and inherently dishonest body into a more focused, sophisticated, and interactive machine reveal much about the implementation of János Kádár’s vision for socialist Hungary. Described as a “living, controllable device,” the political police’s informant network provided Hungarian citizens with an accessible and personally beneficial means of cooperation with the state. The network allowed Hungarians to prove themselves “not against” Kádár’s Party.
Additional file 4 of UGRP1-modulated MARCO+ alveolar macrophages contribute to age-related lung fibrosis
Creators: name: Chen, Yongyan
name: Hao, Xiaolei
name: Li, Ming
name: Tian, Zhigang
name: Cheng, Min
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 4: Figure 3.Representative DEGs of state 17 were shown.
Ghiaccio bollente su Europa
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

I ghiacci di Europa, il satellite mediceo di Giove, potrebbe trattenere più calore di quanto si pensasse. Questo il risultato di una serie di esperimenti dedicati a comprendere meglio quanto calore venga generato dalla deformazione del ghiaccio. Lo studio è stato presentato sulla rivista Earth and Planetary Science Letters
Higgs boson decay rate into gluons in a 5 dimensional calculable model
Creators: name: G. Cacciapaglia
Publisher: name: INFN Open Access Repository
Year: 2002

description: In an extension of the Standard Model with one compact extra dimension and
N=1 supersymmetry, we compute the Higgs boson decay rate into two gluons,
relevant to the Higgs production in hadronic collisions. We find that at one
loop the decay width is significantly suppressed with respect to the SM. In
particular, for a compactification radius 1/R=370 /pm 70 GeV and a Higgs mass
m_H = 127 /pm 8 GeV we find it to be less than 15% of the SM result.
title: ÐÑÐ¸ÑÑÐ°Ð»Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð°Ð»ÑÐ¼Ð¸Ð½Ð¸ÐµÐ²ÑÑ ÑÐ¿Ð»Ð°Ð²Ð¾Ð²: ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð· Ð¼Ð¸ÐºÑÐ¾ÑÑÑÑÐºÑÑÑÑ
title: Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ¾Ð±Ð¾Ñ, ÐÑÐ´Ð¼Ð¸Ð»Ð°
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: 2023
Subjects: ÐÐ»ÑÐ¼Ð¸Ð½Ð¸ÐµÐ²ÑÐµ ÑÐ¿Ð»Ð°Ð²Ñ
ÐÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð¡Ð¿Ð»Ð°Ð²Ñ

description: ÐÑÐ¾Ð´ÐµÐ¼Ð¾Ð½ÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½ ÑÐ¸ÑÑÐµÐ¼Ð½ÑÐ¹ Ð¿Ð¾Ð´ÑÐ¾Ð´ Ðº ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð°Ð´Ð°ÑÐ¸ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð·Ð° ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¾ÑÐ»Ð¸Ð²Ð¾Ðº Ð¸Ð· Ð°Ð»ÑÐ¼Ð¸Ð½Ð¸ÐµÐ²ÑÑ ÑÐ¿Ð»Ð°Ð²Ð¾Ð² Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ð³Ð¾ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¸Ñ ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ (ÑÑÐµÑ ÑÐ¾Ð¿ÑÑÐ¶ÐµÐ½Ð½ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð²ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÐ²ÐµÑÐ´Ð¾Ð¹ ÑÐ°Ð·Ñ, Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÐ¾ÑÑÐ°Ð²Ð° Ð¶Ð¸Ð´ÐºÐ¾Ð¹ ÑÐ°Ð·Ñ Ð¸ ÑÐ²Ð¾Ð»ÑÑÐ¸Ð¸ ÑÐ°Ð·Ð¼ÐµÑÐ¾Ð² Ð²ÑÐ¾ÑÐ¸ÑÐ½ÑÑ Ð¼ÐµÐ¶Ð´ÑÐ¾ÑÐ½ÑÑ Ð¿ÑÐ¾Ð¼ÐµÐ¶ÑÑÐºÐ¾Ð² Ð´ÐµÐ½Ð´ÑÐ¸ÑÐ¾Ð²). ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ð¹ ÑÐµÑÐ¼Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ¸ Ð¸ ÑÐµÐ¿Ð»Ð¾Ð¾Ð±Ð¼ÐµÐ½Ð° Ð¿ÑÐ¸ Ð·Ð°ÑÐ²ÐµÑÐ´ÐµÐ²Ð°Ð½Ð¸Ð¸ Ð¼Ð°ÐºÑÐ¾ÑÐ°Ð·Ð¼ÐµÑÐ½ÑÑ ÑÐ°ÑÐ¾Ð½Ð½ÑÑ Ð¾ÑÐ»Ð¸Ð²Ð¾Ðº ÑÑÐ¾ÑÐ½ÐµÐ½Ñ Ð³ÑÐ°Ð½Ð¸ÑÐ½ÑÐµ ÑÑÐ»Ð¾Ð²Ð¸Ñ Ð»Ð¾ÐºÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐµÐ¿Ð»Ð¾Ð¾Ð±Ð¼ÐµÐ½Ð° Ð¿ÑÐ¸ Ð¼ÐµÐ·Ð¾Ð¼Ð°ÑÑÑÐ°Ð±Ð½Ð¾Ð¼ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð½ÐµÑÐ°Ð²Ð½Ð¾Ð²ÐµÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²ÐµÑÐ´Ð¾Ð¹ ÑÐ°Ð·Ñ Ð¸ Ð¿ÐµÑÐµÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ¾Ð² Ð¼ÐµÐ¶Ð´Ñ ÑÐ°Ð·Ð°Ð¼Ð¸ Ð¿ÑÐ¸ ÐºÐ¾Ð°Ð»ÐµÑÑÐµÐ½ÑÐ¸Ð¸ Ð²ÑÐ¾ÑÐ¸ÑÐ½ÑÑ Ð´ÐµÐ½Ð´ÑÐ¸ÑÐ½ÑÑ Ð²ÐµÑÐ²ÐµÐ¹. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÑÐºÑÑÑÐ½Ð¾-ÑÐ°Ð·Ð¾Ð²ÑÑ Ð¿ÐµÑÐµÑÐ¾Ð´Ð¾Ð² Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ð° Ð°Ð´Ð´Ð¸ÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ ÑÐ¸Ð·Ð¸ÐºÐ¾-ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ¾Ð² ÑÐ¿Ð»Ð°Ð²Ð° Ð² Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð´Ð¸ÑÑÑÐ·Ð¸Ð¾Ð½Ð½Ð¾-ÐºÐ°Ð¿Ð¸Ð»Ð»ÑÑÐ½Ð¾Ð¹ Ð¼Ð¾ÑÑÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ²Ð¾Ð»ÑÑÐ¸Ð¸ Ð´ÐµÐ½Ð´ÑÐ¸ÑÐ½Ð¾Ð¹ ÑÑÑÑÐºÑÑÑÑ Ð¸ Ð»Ð¾ÐºÐ°Ð»ÑÐ½Ð¾Ð¹ Ð´ÐµÐ½Ð´ÑÐ¸ÑÐ½Ð¾Ð¹ Ð½ÐµÐ¾Ð´Ð½Ð¾ÑÐ¾Ð´Ð½Ð¾ÑÑÐ¸, ÑÑÐ¾ÑÐ°ÑÑÐ¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ°ÑÐ°ÐºÑÐµÑ Ð¸ ÑÑÐµÐ¿ÐµÐ½Ñ ÐºÐ¾ÑÐ¾ÑÐ¾Ð¹ Ð²ÑÑÐ²Ð»ÑÑÑÑÑ Ð¿ÑÐ¸ Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¸. Ð ÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½ÑÐ¹ Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ð¹ Ð´Ð»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¿Ð»Ð°Ð²Ð¾Ð², ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½ Ð½Ð° Ð°Ð½Ð°Ð»Ð¸Ð· Ð¼Ð½Ð¾Ð³Ð¾ÑÐ°ÐºÑÐ¾ÑÐ½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð»Ð¸ÑÐµÐ¹Ð½ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² Ð¸ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¼Ð¸ÐºÑÐ¾ÑÑÑÑÐºÑÑÑÑ Ð¾ÑÐ»Ð¸Ð²Ð¾Ðº.
The photochemical and thermal oxidation of hydrogen sulphide
Creators: name: Tse, Ronald Siu-Man
Publisher: name: University of British Columbia
Year: 2011

description: In order to elucidate the mechanism of hydrogen sulphide oxidation, the photo-oxidation and thermal oxidation of hydrogen sulphide were studied, using gas chromatography for the analysis of final products. Photo-oxidation was studied at 130° and 150°C. Products found were sulphur dioxide, hydrogen, water and sulphur. Production of sulphur dioxide was found to be inhibited by an increase in surface area. Whether in photo- or thermal oxidation, the yield of sulphur dioxide increased drastically with slight increases in (O₂)/H₂S) ratio. This was also observed in the yield of hydrogen in photo-oxidation. Thermal oxidation was studied at 160°, 170°, 190°, 210°, 225°, 240°, and 260°C. Products were sulphur dioxide, water, and sulphur. No hydrogen was found. An expression for the production of sulphur dioxide was obtained: [formula omitted] = k (H₂S)⁻¹→⁺¹ (O₂)³ The overall activation energy was found to be 21.2±2k.cal./mole. Comparison with previously reported works was made and a mechanism proposed.
Giocare a nascondino con le lenti gravitazionali
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2016

Questa scoperta, compiuta grazie all'Atacama Large Millimeter/submillimeter Array, apre la strada allo studio di molti oggetti simili e potrebbe aiutare gli astronomi a risolvere domande importanti sulla natura della materia oscura
title: ÐÐ½ÑÑÑÐµÐ½Ð½Ð¸Ð¹ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð¸ Ð²Ð½ÑÑÑÐµÐ½Ð½Ð¸Ð¹ Ð°ÑÐ´Ð¸Ñ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¾ÑÐ¸Ð½ÐµÐ², Ð®ÑÐ¸Ð¹
name: ÐÐ½ÑÑÑÐµÐ²Ð°, ÐÐ»ÐµÐ½Ð°
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2021
Subjects: Ð²Ð½ÑÑÑÐµÐ½Ð½Ð¸Ð¹ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ (ÑÐºÐ¾Ð½.)
Ð²Ð½ÑÑÑÐµÐ½Ð½Ð¸Ð¹ Ð°ÑÐ´Ð¸Ñ
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÐºÐ¾Ð½ÑÐµÐ¿ÑÑÐ°Ð»ÑÐ½Ð°Ñ Ð¾ÑÐ½Ð¾Ð²Ð° Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÑÐ±ÑÐµÐºÑÐ¾Ð², Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÑÑÑÐºÑÑÑÐ° ÑÐ¸ÑÑÐµÐ¼Ñ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð¸ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ðµ ÐµÐµ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð². Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¿ÑÐµÐ´ÑÑÐ²Ð»ÑÐµÐ¼ÑÐµ Ðº ÑÐ¸ÑÑÐµÐ¼Ð°Ð¼ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÑÐ±ÑÐµÐºÑÐ¾Ð² Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÐ½ÑÐ¼Ð¸ Ð¸ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½ÑÐ¼Ð¸ Ð°ÐºÑÐ°Ð¼Ð¸. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¾ Ð¼ÐµÑÑÐ¾ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ³Ð¾ Ð°ÑÐ´Ð¸ÑÐ° Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÑÐ±ÑÐµÐºÑÐ¾Ð². Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð²Ð¾Ð·Ð½Ð¸ÐºÐ½Ð¾Ð²ÐµÐ½Ð¸Ñ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ³Ð¾ Ð°ÑÐ´Ð¸ÑÐ° Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÑÑÐ°Ð¿Ð¾Ð² ÐµÐ³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ. Ð£Ð´ÐµÐ»ÐµÐ½Ð¾ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ Ð²Ð¾Ð¿ÑÐ¾ÑÐ°Ð¼ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¿ÑÐ°ÐºÑÐ¸ÐºÐ¸ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ³Ð¾ Ð°ÑÐ´Ð¸ÑÐ°, ÐµÐ³Ð¾ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ð°Ð¼ Ð¸ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ°Ð¼. Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 38.04.01 Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°Â» (Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð° 38.04.01.20 Â«Ð£ÑÐµÑ, Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ Ð°ÑÐ´Ð¸Ñ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸ÐµÐ¹Â»). ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ ÑÐ°ÐºÐ¶Ðµ Ð¿Ð¾Ð»ÐµÐ·Ð½Ð¾ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ°Ð¼ Ð¿Ð¾ Ð°ÑÐ´Ð¸ÑÑ, Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ°Ð¼ Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð´ÑÑÐ³Ð¸Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼.
Cassini, il cattura-polvere interstellare
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2016

Individuate e analizzate da un team di ricercatori guidato da Nicolas Altobelli grazie allo strumento Cosmic Dust Analyzer della missione ESA-NASA-ASI alcune particelle di polvere proveniente dall'esterno del nostro Sistema solare. Il commento di Vincenzo Della Corte (INAF)
Additional file 1: of Suv39h1 promotes facet joint chondrocyte proliferation by targeting miR-15a/Bcl2 in idiopathic scoliosis patients
Creators: name: Li, Jiong
name: Yang, Guanteng
name: Liu, Shaohua
name: Wang, Longjie
name: Liang, Zhuotao
name: Zhang, Hongqi
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Pharmacology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Hematology
subject: Virology

description: Table S1. Clinical data of study subjects. Table S2. List of antibodies from Cell Signaling Technologies. Table S3. Primers sequences for genes. (DOCX 20 kb)
The magnetic SW Sextantis star RX J1643.7+3402
Creators: name: Rodriguez-Gil, P.
name: Martinez-Pais, I. G.
name: Rodriguez, J. de la Cruz
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present time-resolved spectroscopy and circular spectropolarimetry of the SW Sex star RX J1643.7+3402. We find significant polarisation levels exhibiting a variability at a period of 19.38 +- 0.39 min. In addition, emission-line flaring is found predominantly at twice the polarimetric period. These two findings are strong evidences in favour of the presence of a magnetic white dwarf in the system. We interpret the measured periodicities in the context of our magnetic accretion model for SW Sex stars. In contrast with LS Pegasi -the first SW Sex star discovered to have modulated circular polarisation- the polarisation in RX J1643.7+3402 is suggested to vary at 2(omega - Omega), while the emission lines flare at (omega - Omega). However, a 2omega/omega interpretation cannot be ruled out. Together with LS Peg and V795 Her, RX J1643.7+3402 is the third SW Sex star known to exhibit modulated circular polarisation.
description: 7 pages, 4 figures, accepted for publication in MNRAS
Le stelle del cinema a Foligno
Creators: Francesco Rea
Publisher: name: Media Inaf
Year: 2016

Tema di quest'anno, il coraggio di conoscere. A seguire la conferenza di Roberto Battiston, presidente ASI. Venerdì 15, invece, la conferenza del presidente INAF Nichi D'Amico dal titolo «Onda su onda, la radioastronomia da Marconi ad Einstein»
Cervello umano batte supercomputer 1-0
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

Un team interdisciplinare di ricercatori dell’Università di Aarhus, in Danimarca, ha sottoposto oltre 10 mila persone a un esperimento che consisteva nel risolvere problemi complessi utilizzando il video gioco online chiamato Quantum Moves. I risultati dimostrano che il cervello umano è più efficiente di qualunque supercomputer
title: ÐÐ¸ÑÐºÑÐµÑÐ½Ð°Ñ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ°. ÐÐ²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð² ÑÐµÐ¾ÑÐ¸Ñ Ð³ÑÐ°ÑÐ¾Ð²
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¾Ð¿Ð¾Ð²Ð°, Ð¡Ð²ÐµÑÐ»Ð°Ð½Ð°
name: Ð¥Ð¾Ð´ÑÑÐµÐ², ÐÐ²Ð°Ð½
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2013
Subjects: ÐÐ¸ÑÐºÑÐµÑÐ½Ð°Ñ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ°
ÐÑÐ°ÑÐ¾Ð² ÑÐµÐ¾ÑÐ¸Ñ

description: Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ñ ÑÐµÐ¾ÑÐ¸Ð¸ Ð³ÑÐ°ÑÐ¾Ð². Ð¡Ð¾Ð´ÐµÑÐ¶Ð¸Ñ Ð²ÑÐ¿Ð¾Ð¼Ð¾Ð³Ð°ÑÐµÐ»ÑÐ½ÑÐ¹ ÑÑÐµÐ±Ð½ÑÐ¹ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð», Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð½ÑÐ¹ Ð¿Ð¾ ÑÐ¸ÑÐ»Ñ Ð²ÐºÐ»ÑÑÐµÐ½Ð½ÑÑ Ð² Ð½ÐµÐ³Ð¾ ÑÐµÐ¼. ÐÐ»Ñ Ð¿Ð¾Ð»Ð½Ð¾Ð³Ð¾ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÑÐ°Ð·Ð´ÐµÐ»Ð° Â«Ð¢ÐµÐ¾ÑÐ¸Ñ Ð³ÑÐ°ÑÐ¾Ð²Â» ÐºÑÑÑÐ° Â«ÐÐ¸ÑÐºÑÐµÑÐ½Ð°Ñ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ°Â» Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð², Ð² ÐºÐ¾ÑÐ¾ÑÑÑ ÑÐ°ÑÐºÑÑÑÑ ÑÐµÐ¼Ñ, Ð½Ðµ Ð²ÐºÐ»ÑÑÐµÐ½Ð½ÑÐµ Ð² Ð´Ð°Ð½Ð½Ð¾Ðµ ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ. ÐÐ¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð² ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð²ÑÐ¿Ð¾Ð¼Ð¾Ð³Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐµÐ±Ð½Ð¾Ð³Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð° Ð´Ð»Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ 010500 Â«ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð¸ Ð°Ð´Ð¼Ð¸Ð½Ð¸ÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼Â» Ð¸ 010500.62 Â«ÐÑÐ¸ÐºÐ»Ð°Ð´Ð½Ð°Ñ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ° Ð¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ°Â». ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¼Ð»Ð°Ð´ÑÐ¸Ñ ÐºÑÑÑÐ¾Ð² Ð²ÑÑÑÐ¸Ñ ÑÑÐµÐ±Ð½ÑÑ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹, Ð° ÑÐ°ÐºÐ¶Ðµ Ð´Ð»Ñ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸Ð¹ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÐ°Ð»Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¼Ð¸ÐºÑÐ¾Ð¿ÑÐ¾ÑÐµÑÑÐ¾ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° ÑÐµÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð¸ Ð¸ÑÐ¿ÑÑÐ°Ð½Ð¸Ð¹ ÑÑÐµÐ´ÑÑÐ² Ð Ð Ð¸ Ð, ÑÐ°Ð±Ð¾ÑÐ°ÑÑÐ¸Ñ Ð² ÑÑÐ°Ð½Ð´Ð°ÑÑÐµ ÐÐ­Ð-61850
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð¡Ð¼Ð¸ÑÐ½Ð¾Ð², 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: Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÑÐ¸ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ
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Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÐµÐ´Ð¸Ð½Ð¸ÑÑ Ð¸ ÑÑÐ°Ð»Ð¾Ð½Ñ

description: ÐÐ¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð²Ð¸ÑÑÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¸Ð±Ð¾ÑÐ°, Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÑÐµÐ¼Ð¾Ð¹ ÑÑÐµÐ´Ñ NI Labview 2015, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐµÐ³Ð¾ ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°ÑÑ Ð¿ÑÐ¾ÑÐµÑÑ Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸ Ð¼Ð³Ð½Ð¾Ð²ÐµÐ½Ð½ÑÑ Ð·Ð½Ð°ÑÐµÐ½Ð¸Ð¹ ÑÐ¾ÐºÐ° Ð¸ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸ÑÐ¼Ð¸ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ° ÐÐ­Ð 61850 -9-2. ÐÑÐ»Ð¸ Ð¸Ð·ÑÑÐµÐ½Ñ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð Ð Ð¸ Ð, Ðº ÐºÐ¾ÑÐ¾ÑÑÐ¼ Ð¿ÑÐ¸Ð¼ÐµÐ½Ð¸Ð¼Ð° Ð´Ð°Ð½Ð½Ð°Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð°. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ ÑÐ°Ð·Ð´ÐµÐ» Ð¿Ð¾ Ð¾ÑÑÐ°Ð½Ðµ ÑÑÑÐ´Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ°ÑÑÐµÑ ÑÐµÐ±ÐµÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ. Ð Ð´Ð°Ð»ÑÐ½ÐµÐ¹ÑÐµÐ¼ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ðµ Ð¿Ð¾ÑÐ¾ÐºÐ¾Ð¾Ð±ÑÐ°Ð·ÑÑÑÐµÐ³Ð¾ Ð²Ð¸ÑÑÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¸Ð±Ð¾ÑÐ°, Ñ ÑÑÐ»Ð¾Ð²Ð¸ÑÐ¼Ð¸ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ° ÐÐ­Ð 61850.
description: Dissertation is devoted to the development of virtual instrument based on programmable NI Labview 2015 environment can simulate the process of instant current and voltage values in accordance with the requirements of IEC 61850 9-2. RE devices have been studied and A, which is applicable to this program. This paper presents a section on occupational safety and health, as well as the calculation of the cost of the program. In the future, on the basis of this work can be built potokoobrazuyuschego virtual instrument, the terms of the IEC 61850 standard.
Revealing Hanny's Voorwerp: radio observations of IC 2497
Creators: name: Jozsa, G. I. G.
name: Garrett, M. A.
name: Oosterloo, T. A.
name: Rampadarath, H.
name: Paragi, Z.
name: van Arkel, H.
name: Lintott, C.
name: Keel, W. C.
name: Schawinski, K.
name: Edmondson, E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present multi-wavelength radio observations in the direction of the spiral galaxy IC 2497 and the neighbouring emission nebula known as "Hanny's Voorwerp". Our WSRT continuum observations at 1.4 GHz and 4.9 GHz, reveal the presence of extended emission at the position of the nebulosity, although the bulk of the emission remains unresolved at the centre of the galaxy. e-VLBI 1.65 GHz observations show that on the milliarcsecond-scale a faint central compact source is present in IC 2497 with a brightness temperature in excess of 4E5 K. With the WSRT, we detect a large reservoir of neutral hydrogen in the proximity of IC 2497. One cloud complex with a total mass of 5.6E9 Msol to the South of IC 2497, encompasses Hanny's Voorwerp. Another cloud complex is located at the position of a small galaxy group ~100 kpc to the West of IC 2497 with a mass of 2.9E9 Msol. Our data hint at a physical connection between both complexes. We also detect HI in absorption against the central continuum source of IC 2497. Our observations strongly support the hypothesis that Hanny's Voorwerp is being ionised by an AGN in the centre of IC 2497. In this scenario, a plasma jet associated with the AGN, clears a path through the ISM/IGM in the direction towards the nebulosity. The large-scale radio continuum emission possibly originates from the interaction between this jet and the large cloud complex that Hanny's Voorwerp is embedded in. The HI kinematics do not fit regular rotation, thus the cloud complex around IC 2497 is probably of tidal origin. From the HI absorption against the central source, we derive a lower limit of 2.8E21 +- 0.4E21 atoms/sqcm to the HI column density. However, assuming non-standard conditions for the detected gas, we cannot exclude the possibility that the AGN in the centre of IC 2497 is Compton-thick.
description: 4 pages, 5 figures, A&A, letter to the editor, accepted for publication
Cavity-enhanced dual-comb spectroscopy
Creators: name: Bernhardt, Birgitta
name: Ozawa, Akira
name: Jacquet, Patrick
name: Jacquey, Marion
name: Kobayashi, Yohei
name: Udem, Thomas
name: Holzwarth, Ronald
name: Guelachvili, Guy
name: Hänsch, Theodor W.
name: Picqué, Nathalie
Publisher: name: arXiv
Year: 2009
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: The sensitivity of molecular fingerprinting is dramatically improved when placing the absorbing sample in a high-finesse optical cavity, thanks to the large increase of the effective path-length. As demonstrated recently, when the equidistant lines from a laser frequency comb are simultaneously injected into the cavity over a large spectral range, multiple trace-gases may be identified within a few milliseconds. Analyzing efficiently the light transmitted through the cavity however still remains challenging. Here, a novel approach, cavity-enhanced frequency comb Fourier transform spectroscopy, fully overcomes this difficulty and measures ultrasensitive, broad-bandwidth, high-resolution spectra within a few tens of $μ$s. It could be implemented from the Terahertz to the ultraviolet regions without any need for detector arrays. We recorded, within 18 $μ$s, spectra of the 1.0 $μ$m overtone bands of ammonia spanning 20 nm with 4.5 GHz resolution and a noise-equivalent-absorption at one-second-averaging per spectral element of 3 10^-12 cm^-1Hz^-1/2, thus opening a route to time-resolved spectroscopy of rapidly-evolving single-events.