cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
A multi-wavelength study of the young star V1118 Orionis in outburst
Creators: name: Audard, M.
name: Stringfellow, G. S.
name: Güdel, M.
name: Skinner, S. L.
name: Walter, F. M.
name: Guinan, E. F.
name: Hamilton, R. T.
name: Briggs, K. R.
name: Baldovin-Saavedra, C.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Abriged version for astroph: The young late-type star V1118 Orionis was in outburst from 2005 to 2006. We followed the outburst with optical and near-infrared photometry; the X-ray emission was further probed with observations taken with XMM-Newton and Chandra during and after the outburst. In addition, we obtained mid-infrared photometry and spectroscopy with Spitzer at the peak of the outburst and in the post-outburst phase. The spectral energy distribution of V1118 Ori varied significantly over the course of the outburst. The optical flux showed the largest variations, most likely due to enhanced emission by a hot spot. The latter dominated the optical and near-infrared emission at the peak of the outburst, while the disk emission dominated in the mid-infrared. The X-ray flux correlated with the optical and infrared fluxes, indicating that accretion affected the magnetically active corona and the stellar magnetosphere. The thermal structure of the corona was variable with some indication of a cooling of the coronal temperature in the early phase of the outburst with a gradual return to normal values. Color-color diagrams in the optical and infrared showed variations during the outburst, with no obvious signature of reddening due to circumstellar matter. Using MC realizations of star+disk+hotspot models to fit the SED in ``quiescence'' and at the peak of the outburst, we determined that the mass accretion rate varied from about 2.5E-7 Msun/yr to 1E-6 Msun/yr; in addition the fractional area of the hotspot increased significantly as well. The multi-wavelength study of the V1118 Ori outburst helped us to understand the variations in spectral energy distributions and demonstrated the interplay between the disk and the stellar magnetosphere in a young, strongly accreting star.
description: Accepted in A&A, Tables will be published online
Additional file 3 of Comparison of the in-vivo effect of two tranexamic acid doses on fibrinolysis parameters in adults undergoing valvular cardiac surgery with cardiopulmonary bypass - a pilot investigation
Creators: name: Zhou, Zhen-feng
name: Zhai, Wen
name: Yu, Li-na
name: Sun, Kai
name: Sun, Li-hong
name: Xing, Xiu-fang
name: Yan, Min
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Physiology
subject: Pharmacology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Additional file 3: TableS3. Coagulation proteins without correcting for hemodilution at different time points between the three groups.
Dust and Star Formation in Galaxies: Not the Entire Story
Creators: name: Calzetti, Daniela
Publisher: name: Zenodo
Year: 2021
Subjects: Dust and star formation in galaxies

description: The effects of dust1 are tangled with the star formation history (SFH) of galaxies with a high degree of degeneracy in the UV—NIR wavelength range. Disentangling and constraining the two (dust attenuation and SFH) is key to deriving accurate physical properties of galaxies (SFR, mass, etc.). Availability of restframe MIR/FIR (dust emission) data helps separating the two effects, although degeneracies are still present when large regions (> 1 kpc -> multiple stellar populations) or entire galaxies are modeled. The complexity of separating the two effects will be magnified by the difficulty of securing restframe dust emission data with ALMA for the vast surveys that will become available with the NGRST, Euclid, and JWST (at z>6). Impact decreases at lower metallicities and highest redshifts (shorter t’s). Past and ongoing efforts to help chart a map to address this issue are key for progress. Mainly, this is an issue of limiting the range of solutions with physical arguments.
description: Invited Talk
Effects of neonatal lipopolysaccharide exposure on steroid regulation in the adult mouse brain and blood
Creators: name: Bajaj, Hitasha
Publisher: name: University of British Columbia
Year: 2024

description: Early-life infections can have enduring consequences on brain development and function. Bacterial infections during development increase the risk for neuropsychiatric disorders later in life. However, the mechanisms underlying how illness in early life programs the brain are unknown. Bacterial infections activate the hypothalamic-pituitary-adrenal (HPA) axis and increase glucocorticoid (GC) and mineralocorticoid (MC) secretion from the adrenal glands. Exposure to lipopolysaccharide (LPS), an endotoxin found in Gram-negative bacteria, at postnatal day (PND) 5 also induces GC production in the mouse brain. It is unclear whether neonatal endotoxin exposure (“1st hit”) alters GC and MC regulation in the brain after adult endotoxin exposure (“2nd hit”). Here, male and female C57BL/6J mice were injected intraperitoneally with saline (vehicle control) or 50ug/kg LPS at PND 4 and 6 (“1st hit”). Mice were injected again with either saline or 50ug/kg LPS in adulthood (“2nd hit”) (2x2 design). The brain and blood were collected 4 hr later (n=10/sex/group). We measured 11-deoxycorticosterone, corticosterone, 11-dehydrocorticosterone, and aldosterone in the blood and microdissected brain regions. Steroid levels were quantified in the prefrontal cortex, dorsal hippocampus, ventral hippocampus, hypothalamus, and amygdala via highly specific and sensitive liquid chromatography-tandem mass spectrometry. Results show that neonatal LPS treatment alters GC and aldosterone responses to adult LPS treatment in the blood and brain. Also, males and females show different GC and aldosterone responses to adult LPS treatment. These data clarify how neonatal endotoxin exposure produces long-term alterations in brain steroid regulation in adulthood, potentially underlying behavioural impairments seen upon subsequent immune challenges later in life.
Percolation and critical O($n$) loop configurations
Creators: name: Ding, Chengxiang
name: Deng, Youjin
name: Guo, Wenan
name: Blöte, Henk W. J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We study a percolation problem based on critical loop configurations of the O($n$) loop model on the honeycomb lattice. We define dual clusters as groups of sites on the dual triangular lattice that are not separated by a loop, and investigate the the bond-percolation properties of these dual clusters. The universal properties at the percolation threshold are argued to match those of Kasteleyn-Fortuin random clusters in the critical Potts model. This relation is checked numerically by means of cluster simulations of several O($n$) models in the range $1\leq n \leq 2$. The simulation results include the percolation threshold for several values of $n$, as well as the universal exponents associated with bond dilution and the size distribution of the diluted clusters at the percolation threshold. Our numerical results for the exponents are in agreement with existing Coulomb gas results for the random-cluster model, which confirms the relation between both models. We discuss the renormalization flow of the bond-dilution parameter $p$ as a function of $n$, and provide an expression that accurately describes a line of unstable fixed points as a function of $n$, corresponding with the percolation threshold. Furthermore, the renormalization scenario indicates the existence, in $p$ versus $n$ diagram, another line of fixed points at $p=1$, which is stable with respect to $p$.
description: 17 pages, 9 figures, 1 table
Sweeping Away the Dust: Understanding The Evolution of Attenuation up to the Peak of Cosmic Star Formation
Creators: name: Battisti, Andrew
Publisher: name: Zenodo
Year: 2021
Subjects: Dust and star formation in galaxies

description: Obtaining a detailed census of galaxy properties through cosmic time is crucial to our understanding of galaxy evolution, but depends critically on our ability to correct for the effects of dust attenuation. Dust attenuation curves appear to evolve significantly between z=0 and z=2, however, the underlying cause of this evolution remains unclear. Constraints on attenuation curves at z~1 can provide clear progress on this issue. I will present a characterization of the dust attenuation curve at z~1 based on combining rest-frame UV-to-NIR photometry with the HST WFC3 IR Spectroscopic Parallel (WISP) and 3D-HST grism surveys that have acquired dust-sensitive emission line diagnostics for several hundred galaxies at 0.7<z<1.5. I will also briefly highlight how future grism surveys with the RST and Euclid offer the means to dramatically improve our understanding on the evolution of dust attenuation in galaxies up to z~2.
title: ÐÐ¾Ð´Ð¾Ñ ÑÐ°Ð½Ð¸Ð»Ð¸ÑÐ½ÑÐ¹ Ð³Ð¸Ð´ÑÐ¾ÑÐ·ÐµÐ» Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ ÐÐ°Ð»ÑÐ½ÐµÐ³Ð¾ ÐÐ¾ÑÑÐ¾ÐºÐ°
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ÐµÐ¼ÑÐµÐ²Ð°, Ð¢Ð°ÑÑÑÐ½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð²ÑÑÐ¾ÐºÐ¾Ð½Ð°Ð¿Ð¾ÑÐ½ÑÐ¹ Ð³Ð¸Ð´ÑÐ¾ÑÐ·ÐµÐ»
ÐºÐ¾Ð¼Ð¿Ð¾Ð½Ð¾Ð²ÐºÐ°
Ð³ÑÑÐ½ÑÐ¾Ð²Ð°Ñ Ð¿Ð»Ð¾ÑÐ¸Ð½Ð°
ÑÐ°ÑÑÐµÑ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸
Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾ ÑÐ°Ð±Ð¾Ñ

description: ÐÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ°, Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð½Ð°Ñ Ð¿Ð¾Ð´ ÑÑÐºÐ¾Ð²Ð¾Ð´ÑÑÐ²Ð¾Ð¼ Ð´Ð¾ÑÐµÐ½ÑÐ° ÐºÐ°ÑÐµÐ´ÑÑ ÐÐ¸ÐÐ¡, Ðº.Ñ.Ð½. Ð.Ð. Ð¤ÑÐ¾Ð»Ð¾Ð²Ð¾Ð¹, ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÑ Ð²ÑÑÐ¾ÐºÐ¾Ð½Ð°Ð¿Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð³Ð¸Ð´ÑÐ¾ÑÐ·Ð»Ð° Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ ÐÐ°Ð»ÑÐ½ÐµÐ³Ð¾ ÐÐ¾ÑÑÐ¾ÐºÐ°. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½ Ð²Ð°ÑÐ¸Ð°Ð½Ñ ÐºÐ¾Ð¼Ð¿Ð¾Ð½Ð¾Ð²ÐºÐ¸ Ð³Ð¸Ð´ÑÐ¾ÑÐ·Ð»Ð°, Ð²ÐºÐ»ÑÑÐ°ÑÑÐ¸Ð¹ Ð² ÑÐµÐ±Ñ Ð³ÑÑÐ½ÑÐ¾Ð²ÑÑ Ð¿Ð»Ð¾ÑÐ¸Ð½Ñ, ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð¸ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð²Ð¾Ð´Ð¾ÑÐ±ÑÐ¾ÑÑ, Ð²Ð¾Ð´Ð¾Ð¿ÑÐ¸ÐµÐ¼Ð½Ð¸Ðº Ð½Ð°Ð¿Ð¾ÑÐ½Ð¾Ð¹ Ð´ÐµÑÐ¸Ð²Ð°ÑÐ¸Ð¸. ÐÐ»Ñ Ð³ÑÑÐ½ÑÐ¾Ð²Ð¾Ð¹ Ð¿Ð»Ð¾ÑÐ¸Ð½Ñ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ, Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ Ð¿Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÑÑÑÐ¾Ð·Ð¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÐ¸ Ð¸ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ð¾ÑÐºÐ¾ÑÐ¾Ð². Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½ Ð¿ÑÐ¾ÑÐµÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° ÑÐ°Ð±Ð¾Ñ. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÑÑÐµÐ¶Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð¸ Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ Ð³Ð¸Ð´ÑÐ¾ÑÐ·Ð»Ð°.
Additional file 5 of Comparison of the in-vivo effect of two tranexamic acid doses on fibrinolysis parameters in adults undergoing valvular cardiac surgery with cardiopulmonary bypass - a pilot investigation
Creators: name: Zhou, Zhen-feng
name: Zhai, Wen
name: Yu, Li-na
name: Sun, Kai
name: Sun, Li-hong
name: Xing, Xiu-fang
name: Yan, Min
Publisher: name: figshare
Year: 2021
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Physiology
subject: Pharmacology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Additional file 5: TableS5. Postoperative clinical data and Standard coagulation test.
The SIR epidemic model from a PDE point of view
Creators: name: Chalub, Fabio A. C. C.
name: Souza, Max O.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Populations and Evolution (q-bio.PE)
subject: FOS: Biological sciences

description: We present a derivation of the classical SIR model through a mean-field approximation from a discrete version of SIR. We then obtain a hyperbolic forward Kolmogorov equation, and show that its projected characteristics recover the standard SIR model. Moreover, we show that the long time limit of the evolution will be a Dirac measure. The exact position will depend on the well-know $R_0$ parameter, and it will be supported on the corresponding stable SIR equilibrium.
title: Application of the Relevance Vector Machine to Canal Flow Prediction in the Sevier River Basin
Creators: name: Flake, John T.
Publisher: name: Utah State University
Year: 2007

description: This work addresses management of the scarce water resource for irrigation in arid regions where signiﬁcant delays between the time of order and the time of delivery present major diﬃculties. Motivated by improvements to water management that will be facilitated by an ability to predict water demand, this work employs a data-driven approach to developing canal ﬂow prediction models using the Relevance Vector Machine (RVM), a probabilistic kernel-based learning machine. Beyond the RVM learning process, which establishes the set of relevant vectors from the training data, a search is performed across model attributes including input set, kernel scale parameter, and model update scheme for models providing superior prediction capability. Models are developed for two canals in the Sevier River Basin of southern Utah for prediction horizons of up to ﬁve days. Appendices provide the RVM derivation in detail.
title: Calibration and Results of the Equis II Plasma Impedance Probe (PIP)
Creators: name: Humphries, Seth D.
Publisher: name: Utah State University
Year: 2005

description: This thesis presents the calibration process and analysis results for the two Plasma Impedance Probe (PIP) units that were ﬂown as part of the NASA Equis-I I campaign from the Kwa jalein Atoll. The work of calibration that was presented by Krishna Kurra for the PIP on the Floating Potential Measurement Unit (FPMU) is improved and extended herein. The sweeping impedance probe (SIP), the instrument formerly known as plasma sweeping probe (PSP), is an integral part of the PIP. For the SIP, the calibration presented in this work, calibration error less than 5% error is achieved. The calibration is applied to the ﬂight data to yield impedance measurements. Balmain’s normalized theoretical model is ﬁt to normalized calibrated data to obtain electron density proﬁles within the range of about 2 × 103 to 5 × 106 [Ne /cm3 ]. Electron density proﬁles from the plasma frequency probe (PFP), also part of the PIP, are compared with the density proﬁles from the SIP and there is a close correlation, verifying the calibration and analysis of the SIP.
The dynamical state of brightest cluster galaxies and the formation of clusters
Creators: name: Coziol, R.
name: Andernach, H.
name: Caretta, C. A.
name: Alamo-Martinez, K. A.
name: Tago, E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: A large sample of Abell clusters of galaxies, selected for the likely presence of a dominant galaxy, is used to study the dynamical properties of brightest cluster members (BCMs). From visual inspection of Digitized Sky Survey images combined with redshift data we identify 1426 candidate BCMs in 1221 redshift components in 1169 different Abell clusters, the largest such sample published so far. By our own morphological classification we find ~92% of these BCMs to be early-type galaxies, and 48% of cD type. We confirm previous findings based on much smaller samples, namely that a large fraction of BCMs have significant peculiar velocities. For a subsample of 452 clusters with at least 10 measured radial velocities, we find a median BCM peculiar velocity of 32% of their host clusters' radial velocity dispersion. This suggests that most BCMs are not at rest in the potential well of their clusters, and that the phenomenon is thus not a special trait of clusters hosting cD galaxies. We show that the peculiar velocity of the BCM is independent of cluster richness and only slightly dependent on the Bautz-Morgan type. We also find a weak trend for the peculiar velocity to rise with the cluster velocity dispersion. The strongest dependence is with the morphological type of the BCM: cD galaxies tend to have lower relative peculiar velocities than elliptical galaxies. This result points to a connection between the formation of the BCMs and that of their clusters. Our data are qualitatively consistent with the merging-groups scenario, where BCMs in clusters formed first in smaller subsystems comparable to compact groups of galaxies. In this scenario, clusters would have formed recently from the mergers of many such groups and would still be in a dynamically unrelaxed state.
description: 114 pages, 9 figures, full version of tables 1 and 2; accepted to appear in AJ
title: ÐÐ¾Ð³Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¸Ð·Ð´ÐµÑÐ¶ÐºÐ¸ Ð² Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð·Ð°ÐºÑÐ¿Ð¾ÑÐ½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐ°ÐºÐ´Ð¾Ð½Ð°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¸ÑÐ¾ÑÐºÐ¸Ð½, ÐÐ»Ð°Ð´Ð¸ÑÐ»Ð°Ð²
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·Ð°ÐºÑÐ¿Ð¾ÑÐ½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
Ð»Ð¾Ð³Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¸Ð·Ð´ÐµÑÐ¶ÐºÐ¸
Ð¼Ð¸Ð½Ð¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ Ð·Ð°ÑÑÐ°Ñ
ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½Ð°Ñ Ð¾ÑÐµÐ½ÐºÐ°

description: Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· Ð»Ð¾Ð³Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸Ð·Ð´ÐµÑÐ¶ÐµÐº Ð² Ð·Ð°ÐºÑÐ¿Ð¾ÑÐ½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐÐ°ÐºÐ´Ð¾Ð½Ð°Ð»Ð´Ñ. ÐÑÐ»Ð° Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½Ð°Ñ Ð¾ÑÐµÐ½ÐºÐ° ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð° ÐÐ°ÐºÐ´Ð¾Ð½Ð°Ð»Ð´Ñ. Ð¡Ð´ÐµÐ»Ð°Ð½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð»Ð¾Ð³Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸Ð·Ð´ÐµÑÐ¶ÐµÐº Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐÐ°ÐºÐ´Ð¾Ð½Ð°Ð»Ð´Ñ, Ð° Ð¸Ð¼ÐµÐ½Ð½Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð· Ð°Ð´Ð¼Ð¸Ð½Ð¸ÑÑÑÐ°ÑÐ¸Ð²Ð½Ð¾-ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¸Ñ Ð¸Ð·Ð´ÐµÑÐ¶ÐµÐº, Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸Ð·Ð´ÐµÑÐ¶ÐµÐº Ð½Ð° ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ ÑÑÐ°Ð½ÐµÐ½Ð¸Ðµ Ð·Ð°Ð¿Ð°ÑÐ¾Ð² Ð¸ ÐÐ·Ð´ÐµÑÐ¶ÐµÐº, ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÑ Ñ Ð¾Ð¿Ð»Ð°ÑÐ¾Ð¹ Ð»Ð¾Ð³Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾ÑÑÐµÐ´Ð½Ð¸ÐºÐ¾Ð². ÐÐ°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ¾ÐºÑÐ°ÑÐµÐ½Ð¸Ñ Ð»Ð¾Ð³Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸Ð·Ð´ÐµÑÐ¶ÐµÐº.
Broken symmetry states and divergent resistance in suspended bilayer graphene
Creators: name: Feldman, Benjamin E.
name: Martin, Jens
name: Yacoby, Amir
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Graphene [1] and its bilayer have generated tremendous excitement in the physics community due to their unique electronic properties [2]. The intrinsic physics of these materials, however, is partially masked by disorder, which can arise from various sources such as ripples [3] or charged impurities [4]. Recent improvements in quality have been achieved by suspending graphene flakes [5,6], yielding samples with very high mobilities and little charge inhomogeneity. Here we report the fabrication of suspended bilayer graphene devices with very little disorder. We observe fully developed quantized Hall states at magnetic fields of 0.2 T, as well as broken symmetry states at intermediate filling factors $ν= 0$, $\pm 1$, $\pm 2$ and $\pm 3$. The devices exhibit extremely high resistance in the $ν= 0$ state that grows with magnetic field and scales as magnetic field divided by temperature. This resistance is predominantly affected by the perpendicular component of the applied field, indicating that the broken symmetry states arise from many-body interactions.
description: 23 pages, including 4 figures and supplementary information; accepted to Nature Physics
title: Monitoring of Indoor Relative Humidity Levels in Residential Dwellings: A Sensor Network Application
Creators: name: Lee, Lizabeth
Publisher: name: Utah State University
Year: 2008

description: Indoor Air Quality is an increasing concern in the world today. The mere presence of people in a building or residence can signiﬁcantly alter indoor air quality. Relative humidity over the range of normal indoor temperatures (66 - 80 degrees Farenheit) has been linked both directly and indirectly to various health and structural problems. The purpose of this project was to discover whether residential dwellings might beneﬁt from an indoor humidiﬁcation system. The project consisted of the deployment of three separate sensor networks consisting of 12 tmote sky modules manufactured by the Moteiv corporation, each equipped with a temperature and humidity sensor manufactured by Sensirion. Each tmote sky module continuously transmitted the raw data readings to a base station to be processed. The lifetime of each network was approximately four days of continuous data transmission. The results veriﬁed the hypothesis that relative humidity levels have a signiﬁcant affect on the indoor environment and can be linked to the health and structural problems reported by the occupants of each monitored residence. Based on the project ﬁndings residential dwellings would beneﬁt from an indoor humidiﬁcation system, given the symptoms associated with relative humidity level problems exist.
Inner CGM virialization and its implications for disk galaxies, star formation and galactic winds
Creators: name: Faucher-Giguère, Claude-André
Publisher: name: Zenodo
Year: 2021
Subjects: Dust and star formation in galaxies

description: The origin of disk galaxies is a central problem in galaxy formation. In the prevailing paradigm, disks inherit angular momentum from their host halos. However, deep HST surveys have revealed that disk galaxies are a recent phenomenon: disks start to appear in massive galaxies only around z~2 and disk settling in lower-mass galaxies is delayed until even later. Since halo spins do not depend on mass or redshift in LCDM, these observations indicate that the standard model is at best incomplete. I will summarize recent results from the FIRE cosmological simulations which support a new paradigm for the formation of large disk galaxies. The simulations show that the virialization of the inner circumgalactic medium (CGM) coincides with abrupt changes in the properties of the central galaxy and its stellar feedback: the galaxy settles into a stable rotating disk, star formation transitions from 'bursty' to 'steady,' and galactic winds are suppressed. Disk formation also appears to be associated with accelerated feeding of nuclear black holes, which we speculate drives the onset of quenching by AGN feedback. Future wide-field observations with the Roman, Rubin, Euclid, and Webb observatories will test the predictions of this new theory with unprecedented statistical power and resolution, especially at high redshift.
Vibrationally excited HC3N in NGC 4418
Creators: name: Costagliola, F.
name: Aalto, S.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We investigate the molecular gas properties of the deeply obscured luminous infrared galaxy NGC 4418. We address the excitation of the complex molecule HC3N to determine whether its unusually luminous emission is related to the nature of the buried nuclear source. We use IRAM 30m and JCMT observations of rotational and vibrational lines of HC3N to model the excitation of the molecule by means of rotational diagrams. We report the first confirmed extragalactic detection of vibrational lines of HC3N. We detect 6 different rotational transitions ranging from J=10-9 to J=30-29 in the ground vibrational state and obtain a tentative detection of the J=38-37 line. We also detect 7 rotational transitions of the vibrationally excited states v6 and v7, with angular momenta ranging from J=10-9 to 28-27. The energies of the upper states of the observed transitions range from 20 to 850 K. In the optically thin regime, we find that the rotational transitions of the vibrational ground state can be fitted for two temperatures, 30 K and 260 K, while the vibrationally excited levels can be fitted for a rotational temperature of 90 K and a vibrational temperature of 500 K. In the inner 300 pc of NGC 4418, we estimate a high HC3N abundance, of the order of 10^-7. The excitation of the HC3N molecule responds strongly to the intense radiation field and the presence of warm, dense gas and dust at the center of NGC 4418. The intense HC3N line emission is a result of both high abundances and excitation. The properties of the HC3N emitting gas are similar to those found for hot cores in Sgr B2, which implies that the nucleus (< 300 pc) of NGC 4418 is reminiscent of a hot core. The potential presence of a compact, hot component (T=500 K) is also discussed.
The therapist's dual reality : an investigation into the impact of videoconferencing psychotherapy (VCP) on therapists' perceptions of their clinical abilities
Creators: name: Wellspring, Ian
Publisher: name: University of British Columbia
Year: 2024

description: The COVID-19 pandemic has influenced an increase in Videoconferencing Psychotherapy (VCP) to deliver psychological services (Shore et al., 2020). However, there has been minimal research that has investigated whether therapists’ clinical skills in Face-to-Face (FtF) therapy transfer to VCP. There has also been ongoing consideration regarding clients’ comfort in disclosing information across communication mediums, with mixed prior research. Further, there has been minimal research considering the prevalence and reasons why clients may provide untruthful information in therapy, and therapists’ credibility assessment ability, particularly in VCP. This research aimed to consider whether, and in what potential ways, therapists’ clinical competencies are impacted by conducting therapy across different communication mediums. The perceived advantages and disadvantages of mental health applications were also considered. Study one garnered information about graduate student clinicians’ and clients’ experiences (i.e., clinical skills, comfort disclosing information) following either a FtF or VCP therapy session. Study two collected information about registered psychologists’ experiences and perceptions of their clinical competencies across communication mediums. Participants in study two were also asked to gauge the credibility of a mock VCP client. A mixed-methods survey approach was adopted. Thematic analyses revealed that psychologists perceived clients’ individual differences as being more important for disclosing information in therapy as compared to the communication medium. For example, they believed general levels of openness about one’s personal history played more of a role in disclosure, as compared to the communication medium. Across graduate student clinicians and registered psychologists, therapists reported feeling generally competent in VCP but endorsed not feeling as competent in phone therapy. Registered psychologists were found to experience significantly higher levels of boredom, inattentiveness, and drowsiness in VCP as compared to FtF therapy. Lastly, registered psychologists’ ability to detect deceit in a mock VCP session was 46.75%. This was not significantly different from chance or the deception detection accuracy of 54% found in most prior literature, which is likely reflective of a Truth Bias in most clinical settings. The present results have various implications, particularly in identifying competency areas for therapists to consider when providing mental health services across communication mediums.
title: ÐÑÐ°Ð²Ð¾Ð²Ð¾Ðµ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾ÑÐ¸Ð²Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ ÐºÐ¾ÑÑÑÐ¿ÑÐ¸Ð¸
title: Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ¾ÑÐ°ÑÐµÐ², Ð¡ÐµÑÐ³ÐµÐ¹
name: ÐÐ¾ÑÐ¾ÑÐ¾Ð², ÐÐ¼Ð¸ÑÑÐ¸Ð¹
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2019
Subjects: ÐºÐ¾ÑÑÑÐ¿ÑÐ¸Ñ
Ð±Ð¾ÑÑÐ±Ð° Ñ Ð¿ÑÐµÑÑÑÐ¿Ð½Ð¾ÑÑÑÑ
Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ðµ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ

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ÑÑÐµÐ±Ð½ÑÑ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹, Ð° ÑÐ°ÐºÐ¶Ðµ Ð´Ð»Ñ Ð²ÑÐµÑ Ð¸Ð½ÑÐµÑÐµÑÑÑÑÐ¸ÑÑÑ ÑÑÐ¸Ð¼Ð¸ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð°Ð¼Ð¸.
title: Design of a Low-Power Automatic Wireless Multi-logger Networking Device
Creators: name: Lewis, Kelly S.
Publisher: name: Utah State University
Year: 2007

description: Virtually every industry and discipline (e.g., mining, pharmaceutical, construction, agriculture, reclamation, etc.) is ﬁnding applications for wireless data acquisition for monitoring and managing processes and resources. Two sectors, namely agriculture and environmental research, are seeking ways to obtain distributed soil and plant measurements over larger areas like a watershed or large ﬁelds rather than a single site of intensive instrumentation (i.e., a weather station). Wireless sensor networks and remote sensing have been explored as a means to satisfy this need. Commercial products are readily available that have remote wireless options to support distributed senor networking. However, these systems have been designed with a ﬁeld engineer or technician as the target end-user. Equipment and operating costs, device speciﬁc programming languages, and complex wireless conﬁguration schemes have impeded the adoption of large-scale, multi-node wireless systems in these ﬁelds. This report details the development of an easy-to-use, ultra-low power wireless datalogger incorporating a scalable, intelligent data collection and transmission topology. The ﬁnal product can interface to various sensor types including SDI-12 and uses an LCD display to help simplify device setup.
title: A Formal Approach to Specifying and Verifying Spacecraft Behavior
Creators: name: McInnes, Allan I.S.
Publisher: name: Utah State University
Year: 2007

description: Process algebra can provide spacecraft designers with a mathematical formalism for specifying, understanding, analyzing, and verifying spacecraft system behavior. Although it is standard practice to mathematically model and analyze the subsystems of a spacecraft to ensure that they will function correctly when built, the system-level behavior of the spacecraft is generally understood in much less rigorous terms. This leaves the spacecraft system vulnerable to design errors which may not become apparent until the integration and test phase, when design changes are most expensive. In this dissertation, we develop a formal approach to engineering spacecraft behavior, based on mathematical models of behavior expressed using the process algebra Communicating Sequential Processes. This new approach to spacecraft behavior is intended to help spacecraft systems engineers to model and analyze proposed spacecraft system designs in a rigorous manner, and to detect subtle speciﬁcation and design errors earlier in the design process than the errors would otherwise be found.
title: Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð°Ð³ÐµÐ½ÑÑÑÐ²Ð° ÐÐ¼ÐµÐ³Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ¾Ð·Ð´Ð¾Ð²Ð° , ÐÐ¸ÐºÑÐ¾ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
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financial-economic activity of enterprise
the efficiency of the company
the reserves of increase of efficiency
economic effect

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð°Ð³ÐµÐ½ÑÑÑÐ²Ð¾ Â«ÐÐ¼ÐµÐ³Ð°Â».Ð¦ÐµÐ»ÑÑ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¾ÑÐµÐ½ÐºÐ° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð°Ð³ÐµÐ½ÑÑÑÐ²Ð° Â«ÐÐ¼ÐµÐ³Ð°Â» Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ðµ ÑÐµÐ·ÐµÑÐ²Ð¾Ð² ÐµÐµ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ. ÐÐ»Ñ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ ÑÐµÐ»Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ ÑÑÑÐ½Ð¾ÑÑÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¾ÑÐµÐ½ÐºÐ¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð°Ð³ÐµÐ½ÑÑÑÐ²Ð° Â«ÐÐ¼ÐµÐ³Ð°Â», Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ ÑÐµÐ·ÐµÑÐ²Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸. ÐÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ Ð·Ð½Ð°ÑÐ¸Ð¼Ð¾ÑÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð² ÑÐ¾Ð¼, ÑÑÐ¾ ÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÐ¸ÐµÑÑ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¼Ð¾Ð³ÑÑ ÑÐ»ÑÐ¶Ð¸ÑÑ Ð¾ÑÐ½Ð¾Ð²Ð¾Ð¹ Ð´Ð»Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð² Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð°Ð³ÐµÐ½ÑÑÑÐ²Ðµ Â«ÐÐ¼ÐµÐ³Ð°Â».
description: The object of research is the online agency "Omega". The aim is to assess the cost effectiveness of Internet agency "Omega" and the identification of reserves to im-prove it. To achieve the goal defined the essence of the effectiveness of the enterprise, the technique evaluation of the effectiveness of the company, evaluated the cost-effectiveness of the online agency "Omega", proposed reserves to increase economic efficiency. The practical significance of the study lies in the fact that contained recommendations can serve as a basis for improving the efficiency of financial activity in the Internet agency "Omega".
title: Ð¢ÐµÐ¾ÑÐ¸Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ Ð¿Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ (Ð»Ð¸Ð´ÐµÑÑÑÐ²Ð¾)
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¾Ð·Ð»Ð¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
name: ÐÐ¾Ð·Ð»Ð¾Ð², ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2013
Subjects: ÑÐµÐ¾ÑÐ¸Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸
Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ Ð¿Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ
Ð»Ð¸Ð´ÐµÑÑÑÐ²Ð¾
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

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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ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð·Ð°Ð³ÑÑÐ·ÐºÐ¸, Ð·Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐºÐ»Ð°Ð´ÑÐºÐ¸Ñ Ð¿Ð»Ð¾ÑÐ°Ð´ÐµÐ¹ Ð´Ð»Ñ Ð¤ÐÐÐ£Ð "ÐÐ½ÑÑÐ¸ÑÑÑ Ð²ÑÑÐ¾ÐºÐ¾Ð¼Ð¾Ð»ÐµÐºÑÐ»ÑÑÐ½ÑÑ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹ Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð°ÐºÐ°Ð´ÐµÐ¼Ð¸Ð¸ Ð½Ð°ÑÐº"
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÑÑÐ¾Ð½, ÐÐ¸ÑÐ°Ð»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: 2016
Subjects: Ð»Ð¾Ð³Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¸
Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ°
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸
ÑÐºÐ»Ð°Ð´ÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸
logistics operations
organizational structure
financial highlights
warehousing indicators

description: Ð Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¾ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸Ð·Ð¾Ð²Ð°Ð½Ð° Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¤ÐÐÐ£ Ð½Ð°ÑÐºÐ¸ ÐÐ½ÑÑÐ¸ÑÑÑ Ð²ÑÑÐ¾ÐºÐ¾Ð¼Ð¾Ð»ÐµÐºÑÐ»ÑÑÐ½ÑÑ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹ Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð°ÐºÐ°Ð´ÐµÐ¼Ð¸Ð¸ Ð½Ð°ÑÐº. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐºÐ»Ð°Ð´Ð¾Ð², ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ°. Ð Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð¿ÑÐ¾Ð¸Ð·Ð¾ÑÐ»Ð¾ Ð¾Ð·Ð½Ð°ÐºÐ¾Ð¼Ð»ÐµÐ½Ð¸Ðµ Ñ ÑÐ°Ð±Ð¾ÑÐ¾Ð¹ Ð¾ÑÐ´ÐµÐ»Ð° Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾-ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ñ Ð² Ð´Ð°Ð½Ð½Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸.
description: In the bachelor work is characterized the activity of the Institute of macromolecular compounds of Russian Academy of Sciences. There are depicted the financial results of the warehouse work, examined the structure of IMC RAS organization. In the process there was done the acquaintance with the operation of the Department of logistics of IMC RAS.
Quantum ESPRESSO: a modular and open-source software project for quantum simulations of materials
Creators: name: Giannozzi, P.
name: Baroni, S.
name: Bonini, N.
name: Calandra, M.
name: Car, R.
name: Cavazzoni, C.
name: Ceresoli, D.
name: Chiarotti, G. L.
name: Cococcioni, m.
name: Dabo, I.
name: Corso, A. Dal
name: Fabris, S.
name: Fratesi, G.
name: de Gironcoli, S.
name: Gebauer, R.
name: Gerstmann, U.
name: Gougoussis, C.
name: Kokalj, A.
name: Lazzeri, M.
name: Martin-Samos, L.
name: Marzari, N.
name: Mauri, F.
name: Mazzarello, R.
name: Paolini, S.
name: Pasquarello, A.
name: Paulatto, L.
name: Sbraccia, C.
name: Scandolo, S.
name: Sclauzero, G.
name: Seitsonen, A. P.
name: Smogunov, A.
name: Umari, P.
name: Wentzcovitch, R. M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Quantum ESPRESSO is an integrated suite of computer codes for electronic-structure calculations and materials modeling, based on density-functional theory, plane waves, and pseudopotentials (norm-conserving, ultrasoft, and projector-augmented wave). Quantum ESPRESSO stands for "opEn Source Package for Research in Electronic Structure, Simulation, and Optimization". It is freely available to researchers around the world under the terms of the GNU General Public License. Quantum ESPRESSO builds upon newly-restructured electronic-structure codes that have been developed and tested by some of the original authors of novel electronic-structure algorithms and applied in the last twenty years by some of the leading materials modeling groups worldwide. Innovation and efficiency are still its main focus, with special attention paid to massively-parallel architectures, and a great effort being devoted to user friendliness. Quantum ESPRESSO is evolving towards a distribution of independent and inter-operable codes in the spirit of an open-source project, where researchers active in the field of electronic-structure calculations are encouraged to participate in the project by contributing their own codes or by implementing their own ideas into existing codes.
description: 36 pages, 5 figures, resubmitted to J.Phys.: Condens. Matter
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ¸ ÑÐµÑÐµÑÐºÐ¸ Ð² ÑÐµÐ³Ð½ÐµÑÐ¾ÑÐ»ÐµÐºÑÑÐ¸ÐºÐµ ÑÐ¸ÑÐºÐ¾Ð½Ð°ÑÐ°-ÑÐ¸ÑÐ°Ð½Ð°ÑÐ° ÑÐ²Ð¸Ð½ÑÐ° 20% Ð¼ÐµÑÐ¾Ð´Ð°Ð¼Ð¸ ÑÐ°ÑÑÐµÑÐ½Ð¸Ñ Ð½ÐµÐ¹ÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ Ð¸ ÑÐ¸Ð½Ñ ÑÐ¾ÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ Ð¸Ð·Ð»ÑÑÐµÐ½Ð¸Ñ
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð§Ð°ÐºÐ¸ÑÐµÐ²Ð°, ÐÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¡ÐµÐ³Ð½ÐµÑÐ¾ÑÐ»ÐµÐºÑÑÐ¸ÐºÐ¸
Ð¡Ð²Ð¸Ð½ÐµÑ, ÑÐ¸ÑÐºÐ¾Ð½Ð°ÑÑ
Ð¡Ð²Ð¸Ð½ÐµÑ, ÑÐ¸ÑÐ°Ð½Ð°ÑÑ
Ð­Ð»ÐµÐºÑÑÐ¾Ð¼Ð°Ð³Ð½Ð¸ÑÐ½ÑÐµ Ð²Ð¾Ð»Ð½Ñ
ÐÐµÐ¹ÑÑÐ¾Ð½Ñ

description: Ð Ð°Ð±Ð¾ÑÐ° ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ, Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ½ÑÐ¹ Ð¾Ð±Ð·Ð¾Ñ, Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°, ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¸ Ð²ÑÐ²Ð¾Ð´Ñ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´Ð¸ÑÑÐ°ÐºÑÐ¸Ð¾Ð½Ð½ÑÑ ÐºÐ°ÑÑÐ¸Ð½, ÑÐ¿ÐµÐºÑÑÐ¾Ð² Ð½ÐµÑÐ¿ÑÑÐ³Ð¾Ð³Ð¾ ÑÐ°ÑÑÐµÑÐ½Ð¸Ñ, Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ñ Ð´Ð¸ÑÐ¿ÐµÑÑÐ¸Ð¾Ð½Ð½ÑÐµ ÐºÑÐ¸Ð²ÑÐµ.
Coronal Inflows and Giant Polar Plumes
Creators: name: Pinto, R.
name: Grappin, R.
name: Leorat, J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present the first results of simulations of giant polar plumes and coronal flows. We use a 2.5D axisymmetric MHD numerical model of an isothermal corona and slow solar wind. A plume is generated just above asmall magnetic bipole embedded in an unipolar flux region which is perturbed by Alfvén waves injected from the coronal base. The boundary conditions are transparent. The results are compared to those obtained previously with a 1D wind model in which plumes are generated as a consequence of variations of the heating and flux-tube expansion parameters.
description: 4 pages, 5 figures, accepted for publication in the Solar Wind 12 conference proceedings (AIP Conference Proceedings)
title: Sampling Frequencies Ratio Estimation and Symbol Timing Recovery for Baseband Binary Pulse Amplitude Modulation
Creators: name: Rodriguez, Ana A. Paniagua
Publisher: name: Utah State University
Year: 2008

description: The original intent of this pro ject was to perform real time digital communications between a personal computer (PC) as the transmitter and a digital signal processor (DSP) as the receiver using the audio band analog channel. Although transmitter and receiver were both designed with baseband binary Pulse Amplitude Modulation (PAM), a low data rate and a sampling rate of 8 kilohertz, it was not possible to achieve communication between the two with traditional synchronization algorithms because of large diﬀerences in sampling clock frequencies. This thesis explores the theory and results of implementing digital communications between systems with diﬀerent sampling frequencies. The receiver structure has no a priori knowledge of the transmitter’s sampling rate, although it is assumed to be approximately equal to that of the receiver. Therefore, a receiver structure that can correct this clock frequency oﬀset is developed. Similar sampling frequencies at the transmitter and receiver are assumed in most derivations in the literature. A search of the literature found no cases of a large diﬀerence in the sampling frequencies. In general, if the receiver knows the transmitter’s sampling rate, a resampling ﬁlter at the receiver converts the signal to one compatible with the transmitters sampling rate. However, here it is assumed that the receiver does not know the transmitter’s exact sampling frequency and must be estimated. The mathematical expressions for the signals in the system are derived. The sampling frequency oﬀset introduces errors in the correct detection of the signal when it is done through traditional synchronization algorithms. Therefore, a receiver structure that corrects the sampling frequency oﬀset based on the interpolation concept is proposed. This structure will be shown to work when the correct sampling frequency ratio is known. Later, an approach to estimate the sampling frequency ratio is explored. A feedback estimator structure is derived from the Maximum Likelihood optimum criteria. A feed forward estimator that assumes the clock frequency of the transmitter and uses a synchronization sequence is explored as well.