cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
X-ray characterization of physical-vapor-transport-grown bulk AlN single crystals
Creators: name: Wicht, Thomas
name: Müller, Stephan
name: Weingärtner, Roland
name: Epelbaum, Boris
name: Besendörfer, Sven
name: Bläß, Ulrich
name: Weisser, Matthias
name: Unruh, Tobias
name: Meissner, Elke
Publisher: name: FID GEO
Year: 2020

description: AlN slices from bulk crystals grown under low thermomechanical stress conditions via the physical vapor transport (PVT) method were analyzed by X-ray methods to study the influence of the growth mode on the crystal quality. Defect types and densities were analyzed along axial [0001] as well as lateral growth directions. X-ray diffraction (0110) rocking-curve mappings of representative wafer cuts reveal a low mean FWHM of 13.4 arcsec, indicating the generally high crystal quality. The total dislocation density of 2 × 103 cm−2 as determined by X-ray topography is low and dislocations are largely threading edge dislocations of b = 1/3⟨1120⟩ type. The absence of basal plane dislocations in homogeneous crystal regions void of macroscopic defects can be linked to the low-stress growth conditions. Under the investigated growth conditions this high crystal quality can be maintained both along the axial [0001] direction and within lateral growth directions. Exceptions to this are some locally confined, misoriented grains and defect clusters, most of which are directly inherited from the seed or are formed due to the employed seed fixation technique on the outer periphery of the crystals. Seed-shaping experiments indicate no apparent kinetic limitations for an enhanced lateral expansion rate and the resulting crystal quality, specifically with regard to the growth mode on a-face facets.
Cooking Quality and Flavor of Eggs, as Related to Candled Quality, Storage Conditions, and other Factors
Creators: name: Dawson, Elsie H.
name: Miller, Cora
name: Redstrom, Ruth A.
name: Dawson, Elsie H.
name: Miller, Cora
name: Redstrom, Ruth A.
Publisher: name: Unknown
Year: 1956
Subjects: Food Consumption/Nutrition/Food Safety
Research Methods/ Statistical Methods

description: Excerpt from the report Purpose of the Research: Eggs graded by candling have been on the market for over 30 years, but little has been known about the relationship between functional characteristics in cooking of eggs and candled grade. A coordinated research project was therefore designed for the purpose of providing new information regarding the following: (1) The reliability of the candled quality of eggs as a guide to their performance in food preparation and palatability when served alone or in combination with other ingredients; (2) The suitability of shell eggs of different candled qualities (resulting from storage conditions) for different purposes in the home preparation of foods; (3) The retention of cooking quality and palatability of eggs during storage for varying periods of time and under storage conditions commonly used ; and (4) The relation of climate or season of production to the quality of eggs.
Initial Conditions of Planet Formation: Lifetimes of Primordial Disks
Creators: name: Mamajek, Eric E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The statistical properties of circumstellar disks around young stars are important for constraining theoretical models for the formation and early evolution of planetary systems. In this brief review, I survey the literature related to ground-based and Spitzer-based infrared (IR) studies of young stellar clusters, with particular emphasis on tracing the evolution of primordial (``protoplanetary'') disks through spectroscopic and photometric diagnostics. The available data demonstrate that the fraction of young stars with optically thick primordial disks and/or those which show spectroscopic evidence for accretion appears to approximately follow an exponential decay with characteristic time ~2.5 Myr (half-life = 1.7 Myr). Large IR surveys of ~2-5 Myr-old stellar samples show that there is real cluster-by-cluster scatter in the observed disk fractions as a function of age. Recent Spitzer surveys have found convincing evidence that disk evolution varies by stellar mass and environment (binarity, proximity to massive stars, and cluster density). Perhaps most significantly for understanding the planeticity of stars, the disk fraction decay timescale appears to vary by stellar mass, ranging from ~1 Myr for >1.3 Msun stars to ~3 Myr for <0.08 Msun brown dwarfs. The exponential decay function may provide a useful empirical formalism for estimating very rough ages for YSO populations and for modeling the effects of disk-locking on the angular momentum of young stars.
description: 8 pages, 1 figure, invited review, Proceedings of the 2nd Subaru International Conference "Exoplanets and Disks: Their Formation and Diversity", Keauhou - Hawaii - USA, 9-12 March 2009
title: Ð­ÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð¿ÑÐ¸ÑÐ°Ð´Ð¾Ðº Ðº Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð¾Ð¼Ñ ÑÐ¾Ð¿Ð»Ð¸Ð²Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° ÐÐ°ÐºÐ°Ð·ÑÐ¸ÐºÐ° Ð½Ð° Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸, ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐ½Ð¾ÑÑÐ¸ Ð¸ ÑÐ¾ÐºÑÐ¸ÑÐ½Ð¾ÑÑÐ¸ Ð¾ÑÑÐ°Ð±Ð¾ÑÐ°Ð²ÑÐ¸Ñ Ð³Ð°Ð·Ð¾Ð² Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½ÑÑ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»ÐµÐ¹ Ð½Ð° Ð±Ð°Ð·Ðµ Ð¼Ð¾ÑÐ¾ÑÐ½ÑÑ ÑÑÐµÐ½Ð´Ð¾Ð²ÑÑ Ð¸ÑÐ¿ÑÑÐ°Ð½Ð¸Ð¹
title: Ð ÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¼Ð¾ÑÐ¾ÑÐ½Ð¾-ÑÑÐµÐ½Ð´Ð¾Ð²ÑÑ Ð¸ÑÐ¿ÑÑÐ°Ð½Ð¸Ð¹ Ð½Ð° Ð´Ð¸Ð·ÐµÐ»ÑÐ½Ð¾Ð¼ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ðµ (Ð·Ð°ÐºÐ»ÑÑÐ¸ÑÐµÐ»ÑÐ½ÑÐ¹)
titleType: Subtitle
title: Experimental study of the influence of the properties of additives to automotive fuel produced by the Customer on the performance, efficiency and toxicity of exhaust gases of automobile engines based on motor bench tests
Creators: name: Ð¨Ð°Ð±Ð°Ð½Ð¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2022
Subjects: Ð´Ð¸Ð·ÐµÐ»ÑÐ½ÑÐ¹ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ
Ð´Ð¸Ð·ÐµÐ»ÑÐ½Ð¾Ðµ ÑÐ¾Ð¿Ð»Ð¸Ð²Ð¾
Ð¼Ð½Ð¾Ð³Ð¾ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð°Ñ Ð¿ÑÐ¸ÑÐ°Ð´ÐºÐ°
diesel engine
diesel fuel
multifunctional additive
ÐÐ¾Ð³Ð¾Ð²Ð¾Ñ ÐÐÐ¢Ð 143248204

description: Ð Ð¾ÑÑÐµÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¼Ð¾ÑÐ¾ÑÐ½ÑÑ ÑÑÐµÐ½Ð´Ð¾Ð²ÑÑ Ð¸ÑÐ¿ÑÑÐ°Ð½Ð¸Ð¹ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¾Ð±ÑÐ°Ð·ÑÐ¾Ð² ÐºÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð¾Ð³Ð¾ Ð´Ð¸Ð·ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð¿-Ð»Ð¸Ð²Ð° ÐÐ¢-Ð-Ð5 Ñ Ð´Ð¾Ð±Ð°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼ Ð¿ÑÐ¸ÑÐ°Ð´ÐºÐ¸ BRAVOS PRIME D, Ð² ÑÐ¾Ð¿Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸ Ñ Ð±Ð°Ð·Ð¾Ð²ÑÐ¼ ÑÐ¾Ð¿Ð»Ð¸Ð²Ð¾Ð¼. ÐÑÐ¿ÑÑÐ°Ð½Ð¸Ñ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸Ð»Ð¸ÑÑ Ð´Ð»Ñ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ñ Ð¾Ð±ÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð¹ ÐºÐ°ÑÑÐ¸Ð½Ñ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð²ÑÑÐµÑÐºÐ°Ð·Ð°Ð½Ð½Ð¾Ð¹ Ð¿ÑÐ¸ÑÐ°Ð´ÐºÐ¸ Ð½Ð° ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ Ð´Ð¸Ð·ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð½Ð° Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ ÑÑÐ¾Ð²Ð½Ñ Ð·Ð°Ð³ÑÑÐ·Ð½ÐµÐ½Ð¸Ð¹ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ ÐºÐ°Ð¼ÐµÑÑ ÑÐ³Ð¾ÑÐ°Ð½Ð¸Ñ Ð¸ ÑÐ¸ÑÑÐµÐ¼ Ð²Ð¿ÑÑÐºÐ°-Ð²ÑÐ¿ÑÑÐºÐ° Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ.
description: The report presents the results of motor bench tests of comparative samples of composite automotive diesel fuel DT-L-K5 with the addition of BRAVOS PRIME D additive, in comparison with the base fuel. The tests were carried out to identify an objective picture of the effect of the above additive on the technical, economic and environmental performance of the diesel engine, as well as on the change in the level of contamination of the combustion chamber engine and engine intake and exhaust systems.
Improving Information Extraction From Simulated Discharge Using Sensitivity-Weighted Performance Criteria
Creators: name: Guse, B.
name: Pfannerstill, M.
name: Fohrer, N.
name: Gupta, H.
Publisher: name: FID GEO
Year: 2020

description: Due to seasonal or interannual variability, the relevance of hydrological processes and of the associated model parameters can vary significantly throughout the simulation period. To achieve accurately identified model parameters, temporal variations in parameter dominance should be taken into account. This is not achieved if performance criteria are applied to the entire model output time series. Even when using complementary performance criteria, it is often only possible to identify some of the model parameters precisely. We present an innovative approach to improve parameter identifiability that exploits the information available regarding temporal variations in parameter dominance. Using daily parameter sensitivity time series, we construct a set of sensitivity-weighted performance criteria, one for each parameter, whereby periods of higher dominance of a model parameter and its corresponding process are assigned higher weights in the calculation of the associated performance criterion. These criteria are used to impose constraints on parameter values. We demonstrate this approach by constraining 12 model parameters for three catchments and examine ensemble hydrological simulations generated using these constrained parameter sets. The sensitivity-weighted approach improves in particular the identifiability for parameters whose corresponding processes are dominant only for short periods of time or have strong seasonal patterns. This results overall in slight improvement of model performance for a set of 10 contrasting performance criteria. We conclude that the sensitivity-weighted approach improves the extraction of hydrologically relevant information from data, thereby resulting in improved parameter identifiability and better representation of model parameters.
The supernova rate and delay time distribution in the Magellanic Clouds
Creators: name: Maoz, Dan
name: Badenes, Carles
Publisher: name: arXiv
Year: 2010
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We use the supernova remnants (SNRs) in the Magellanic Clouds (MCs) as a supernova (SN) survey, "conducted" over tens of kyr, from which we derive the current SN rate, and the SN delay time distribution (DTD), i.e., the SN rate vs. time that would follow a hypothetical brief burst of a star formation. In Badenes, Maoz, & Draine (2010) we have compiled a list of 77 SNRs in the MCS, and argued it is a fairly complete record of the SNRs in the Sedov phase of their expansions. We recover the DTD by comparing the numbers of SNRs observed in small individual "cells" in these galaxies to the star-formation histories of each cell, as calculated from resolved stellar populations by Harris & Zaritsky. The visibility times of SNRs are the Sedov-phase lifetimes, which depend on the local ambient densities. The local densities are estimated from HI emission, from an inverse Schmidt law based on either Halpha flux or on the resolved star-formation rate, and from combinations of these tracers. In the DTD, we detect "prompt" type-Ia SNe (that explode within 330 Myr of star formation) at >99% confidence level (c.l.). The best fit for the number of prompt SNe-Ia per stellar mass formed is (2.7-11.0) x 10^{-3} /Msun, depending on the density tracer used. The 95% c.l. range for a "delayed" SN Ia component (from 330 Myr to a Hubble time) is < 1.6 x 10^{-13} SN/yr/Msun, consistent with rate measurements in old populations. The current total (core-collapse+Ia) SN rate in the MCs is 2.5-4.6 SNe per millenium (68% c.l.+systematics), or 1.7-3.1 SNuM [SNe/100 yr/10^{10}Msun], in agreement with the historical record and with rates measured in other dwarf irregulars. Conversely, assuming the SNRs are in free expansion, rather than in their Sedov phase, would impose on the SNRs a maximum age of 6 kyr, and would imply a MC SN rate per unit mass that is 5 times higher than in any type of galaxy.
description: MNRAS, in press
title: ÐÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð² Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾Ð¹ Ð³ÑÐ°ÑÐ¸ÐºÐµ. Ð§. 6
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°ÑÐºÐ¾Ð²Ð°, Ð¢Ð°ÑÑÑÐ½Ð°
name: ÐÐ¾ÑÐºÐ¾Ð², ÐÐ½Ð´ÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2021
Subjects: ÐÐ½Ð¶ÐµÐ½ÐµÑÐ½Ð°Ñ Ð³ÑÐ°ÑÐ¸ÐºÐ°
ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½ÑÐµ
ÐÐ°ÑÐ¸Ð½Ð½Ð°Ñ Ð³ÑÐ°ÑÐ¸ÐºÐ°
ÐÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ

description: Ð¡Ð¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÐ¿ÑÐ°Ð¶Ð½ÐµÐ½Ð¸Ñ, Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ðµ ÐºÐ¾ÑÐ¾ÑÑÑ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ Ð·Ð°ÐºÑÐµÐ¿Ð¸ÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð·Ð½Ð°Ð½Ð¸Ñ ÐºÑÑÑÐ° Â«ÐÐ½Ð¶ÐµÐ½ÐµÑÐ½Ð°Ñ Ð³ÑÐ°ÑÐ¸ÐºÐ°Â», Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿Ð¾ÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾ Ð¾ÑÐ²Ð¾Ð¸ÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ ÑÐ¸ÑÑÐµÐ¼Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐÐÐÐÐÐ¡-3D V18 Ð¸ ÑÑÐ°ÑÑÐµ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÑÐµÐ½Ð¸Ñ ÑÐµÑÑÐµÐ¶Ð°: Ð¿Ð¾Ð½Ð¸Ð¼Ð°Ð½Ð¸Ñ ÑÐ¾ÑÐ¼Ñ Ð¸Ð·Ð´ÐµÐ»Ð¸Ñ Ð¿Ð¾ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸ÑÐ¼ Ð½Ð° ÑÐµÑÑÐµÐ¶Ðµ. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ñ Ð¾Ð±ÑÐ¸Ðµ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ñ Ð¸ Ð¿ÑÐ¸ÐµÐ¼Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ 3D-Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð´ÐµÑÐ°Ð»Ð¸. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ Ðº ÑÑÐºÐ¸Ð·Ð°Ð¼ Ð¸ Ð¿Ð¾ÑÑÐ´Ð¾Ðº Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÑÐ¾ÑÐ¼Ð¾Ð¾Ð±ÑÐ°Ð·ÑÑÑÐ¸Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹, ÑÐ¿Ð¾ÑÐ¾Ð±Ñ Ð¾ÑÐ¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ñ Ð¸ ÑÐµÐ´Ð°ÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¼Ð¾Ð´ÐµÐ»Ð¸. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¿ÐµÑÐ²Ð¾Ð³Ð¾ ÐºÑÑÑÐ° Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹. ÐÐ¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð´Ð»Ñ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¸ÐµÐ¼Ð¾Ð² ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¾ÑÑÐºÐ¾Ð¹ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼Ð¸ Ð´ÑÑÐ³Ð¸Ñ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸.
Farmers' Mutual Fire and Windstorm Insurance in the United States
Creators: name: Botts, Ralph R.
name: Rush, John D.
name: Ellickson, John C
name: Botts, Ralph R.
name: Rush, John D.
name: Ellickson, John C
Publisher: name: Unknown
Year: 1956
Subjects: Industrial Organization
Risk and Uncertainty

description: Excerpts from the report Preface: The study reported here summarizes the results of the 1954 "benchmark" survey of the farmers’ mutual fire and windstorm insurance companies. A total of 1,476 farm mutual insurance companies cooperated in the study by filling in and returning their survey schedules. Similar surveys, though not so comprehensive, were made in 1916, 1926, 1936, and 1946. This bulletin is the result of an effort to learn more about the operating methods of the farm mutuals, by types of companies, regions, volume of insurance carried, and size of operating territory, and the extent to which these and other factors are associated with loss and expense rates, assessment income, and size of safety funds.
Numerical simulation of dark lanes in post-flare supra-arcade
Creators: name: Costa, A.
name: Elaskar, S.
name: Fernandez, C.
name: Martinez, G.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We integrate the MHD ideal equations to simulate dark void sunwardly moving structures in post--flare supra--arcades. We study the onset and evolution of the internal plasma instability to compare with observations and to gain insight into physical processes and characteristic parameters of these phenomena. The numerical approach uses a finite-volume Harten-Yee TVD scheme to integrate the 1D1/2 MHD equations specially designed to capture supersonic flow discontinuities. The integration is performed in both directions, the sunward radial one and the transverse to the magnetic field. For the first time, we numerically reproduce observational dark voids described in Verwichte et al. (2005). We show that the dark tracks are plasma vacuums generated by the bouncing and interfering of shocks and expansion waves, upstream an initial slow magnetoacoustic shock produced by a localized deposition of energy modeled with a pressure perturbation. The same pressure perturbation produces a transverse to the field or perpendicular magnetic shock giving rise to nonlinear waves that compose the kink--like plasma void structures, with the same functional sunward decreasing phase speed and constancy with height of the period, as those determined by the observations.
description: Accepted MNRAS, 6 pages, 7 figures
title: Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð² ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÑÐµÑÐµ
title: ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÑ 5.2.3. Ð ÐµÐ³Ð¸Ð¾Ð½Ð°Ð»ÑÐ½Ð°Ñ Ð¸ Ð¾ÑÑÐ°ÑÐ»ÐµÐ²Ð°Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ° (ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ð»ÑÐ½Ð°Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°)
titleType: Subtitle
Creators: name: ÐÐ¾ÑÐ¾Ð±Ð¾ÐºÐ¾Ð², ÐÐ½Ð´ÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2023
Subjects: ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð°Ñ ÑÑÐµÑÐ°
ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ð»ÑÐ½Ð°Ñ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ°
Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ Ð¸Ð¼Ð¿Ð°ÐºÑ-Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ
Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¾ÑÐµÐ½ÐºÐ¸ ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð² ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÑÐµÑÐµ

description: ÐÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð¾Ð² Ð¸ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¾ÑÐ³Ð°Ð½Ð°Ð¼Ð¸ ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¹ Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÑÐµÑÑ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð´Ð»Ñ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð² ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÑÐµÑÐµ Ð¸ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐµÑ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸; ÑÐ°ÐºÐ¶Ðµ Ð²ÑÐ²Ð¾Ð´Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ Ð¼Ð¾Ð³ÑÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ñ Ð² ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð¿ÑÐ¸ Ð¾Ð±ÑÑÐµÐ½Ð¸Ð¸ Ð¿Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð°Ð¼ Ð¼Ð°Ð³Ð¸ÑÑÑÐ°ÑÑÑÑ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°Â», Â«ÐÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÂ», Â«Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸ÑÐ¼Ð¸Â».
Volt-per-Ångstrom terahertz fields from X-ray free-electron lasers
Creators: name: Tanikawa, T.
name: Karabekyan, S.
name: Kovalev, S.
name: Casalbuoni, S.
name: Asgekar, V.
name: Bonetti, S.
name: Wall, S.
name: Laarmann, T.
name: Turchinovich, D.
name: Zalden, P.
name: Kampfrath, T.
name: Fisher, A. S.
name: Stojanovic, N.
name: Gensch, M.
name: Geloni, G.
Publisher: name: FID GEO
Year: 2020

description: The electron linear accelerators driving modern X-ray free-electron lasers can emit intense, tunable, quasi-monochromatic terahertz (THz) transients with peak electric fields of V Å−1 and peak magnetic fields in excess of 10 T when a purpose-built, compact, superconducting THz undulator is implemented. New research avenues such as X-ray movies of THz-driven mode-selective chemistry come into reach by making dual use of the ultra-short GeV electron bunches, possible by a rather minor extension of the infrastructure.
Family of exactly solvable models with an ultimative quantum paramagnetic ground state
Creators: name: Schmidt, K. P.
name: Laad, M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We present a family of two-dimensional frustrated quantum magnets solely based on pure nearest-neighbor Heisenberg interactions which can be solved quasi-exactly. All lattices are constructed in terms of frustrated quantum cages containing a chiral degree of freedom protected by frustration. The ground states of these models are dubbed ultimate quantum paramagnets and exhibit an extensive entropy at zero temperature. We discuss the unusual and extensively degenerate excitations in such phases. Implications for thermodynamic properties as well as for decoherence free quantum computation are discussed.
Impact of Bonding on the Stacking Defects in Layered Chalcogenides
Creators: name: Mio, Antonio M.
name: Konze, Philipp M.
name: Meledin, Alexander
name: Küpers, Michael
name: Pohlmann, Marc
name: Kaminski, Marvin
name: Dronskowski, Richard
name: Mayer, Joachim
name: Wuttig, Matthias
Publisher: name: FID GEO
Year: 2019

description: Abstract Phase-change materials for high-density data storage traditionally exploit the amorphous-to-crystalline phase transition. A number of these compounds are organized in blocks, separated by van der Waals-like gaps. Such layered chalcogenides are attracting interest due to their unique material properties and the possibility to change their properties upon local rearrangements at the gap, giving rise to novel applications. To better understand the behavior of layered chalcogenides, the connection between structural defects, physical properties, and the bonding situation is highlighted here using electron microscopy, X-ray diffraction, and density functional theory. In particular, stacking defects in hexagonal Ge4Se3Te, GaSe, and Sb2Te3 are characterized experimentally, followed by an investigation of the influence of observed and hypothetical stacking defects on optical and electronic properties by theoretical means. Then, a connection between observed defects and the bonding situation in these materials is drawn and related to the presence of van der Waals and metavalent bonding in chalcogenides. Finally, additional experiments are performed to validate the conclusions for other metavalently bonded layered chalcogenides. Transmission electron microscopy provides a powerful tool for direct detection of defects and, when combined with diffraction experiments and ab initio theory, it facilitates the precise investigation of the bonding mechanisms in layered chalcogenides.
title: ÐÐµÑÐ¾Ð´Ñ Ð¸ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¸Ð¼Ð¸ ÑÐµÑÑÑÑÐ°Ð¼Ð¸ Ð² ÑÐµÐ»ÑÑ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾Ð³Ð¾ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¹ Ð² ÐÐ¸ÑÐ°Ð¹ÑÐºÐ¾Ð¹ ÐÐ°ÑÐ¾Ð´Ð½Ð¾Ð¹ Ð ÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐµ
title: ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÑ 5.2.6. ÐÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ
titleType: Subtitle
Creators: name: Ð ÐÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2023
Subjects: ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¸Ð¼Ð¸ ÑÐµÑÑÑÑÐ°Ð¼Ð¸
Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¸ Ð² ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¸Ðµ ÑÐµÑÑÑÑÑ
ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¾Ð³Ð¾ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð°
ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾Ðµ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ

description: Ð ÑÐ¿Ð¾ÑÑ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸, Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð¼ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐ²Ð»ÑÑÑÑÑ Ð·Ð½Ð°Ð½Ð¸Ñ, Ð° Ð»ÑÐ´Ð¸, ÐºÐ°Ðº Ð½Ð¾ÑÐ¸ÑÐµÐ»Ð¸ Ð·Ð½Ð°Ð½Ð¸Ð¹, Ð¿ÑÐ¸Ð¾Ð±ÑÐµÑÐ°ÑÑ Ð¸ Ð±ÑÐ´ÑÑ Ð¸ Ð´Ð°Ð»ÐµÐµ Ð¿ÑÐ¸Ð¾Ð±ÑÐµÑÐ°ÑÑ Ð²ÑÑ Ð±Ð¾Ð»ÑÑÐµÐµ Ð·Ð½Ð°ÑÐµÐ½Ð¸Ðµ Ð² Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¼ Ð¿ÑÐ¾ÑÐµÑÑÐµ. ÐÐ²ÑÐ¾ÑÐµÑÐµÑÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹, Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹, Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÑ Ð½Ð° ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¸Ð¼Ð¸ ÑÐµÑÑÑÑÐ°Ð¼Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¹, Ð¾ÑÑÑÐµÑÑÐ²Ð»ÑÑÑÐ¸Ñ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð² ÐÐ¸ÑÐ°Ð¹ÑÐºÐ¾Ð¹ ÐÐ°ÑÐ¾Ð´Ð½Ð¾Ð¹ Ð ÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐµ, Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ¾Ð² Ð¾ÑÐµÐ½ÐºÐ¸ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¸Ñ ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¾Ð³Ð¾ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð° Ð¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¹ Ð² ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¸Ðµ ÑÐµÑÑÑÑÑ. Ð ÑÐ¾Ð´Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¿Ð¾Ð¼Ð¸Ð¼Ð¾ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ°Ð´Ð¸ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð², Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÑÑÑÑ ÑÑÐ°ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¼ÐµÑÐ¾Ð´Ñ: ÑÐµÐ³ÑÐµÑÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð· Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÑÐ´Ð¾Ð². ÐÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ Ð·Ð½Ð°ÑÐ¸Ð¼Ð¾ÑÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸ÑÐ¼ Ð²ÑÑÑÑÐ°Ð¸Ð²Ð°ÑÑ Ð´Ð¾Ð»Ð³Ð¾ÑÑÐ¾ÑÐ½ÑÑ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÑ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¸Ð¼Ð¸ ÑÐµÑÑÑÑÐ°Ð¼Ð¸, Ð¾Ð¿Ð¸ÑÐ°ÑÑÑ Ð½Ð° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÑÑ Ð¾ÑÐµÐ½ÐºÑ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¹ Ð² Ð½Ð¸Ñ. ÐÐ°ÑÑÐ¾ÑÑÐ¸Ð¹ Ð°Ð²ÑÐ¾ÑÐµÑÐµÑÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑ Ð¸Ð½ÑÐµÑÐµÑ Ð´Ð»Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð², Ð¸Ð½ÑÐµÑÐµÑÑÑÑÐ¸ÑÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼ ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¸Ð¼Ð¸ ÑÐµÑÑÑÑÐ°Ð¼Ð¸.
Likelihood analysis of the next-to-minimal supergravity motivated model
Creators: name: Balazs, Csaba
name: Carter, Daniel
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In anticipation of data from the Large Hadron Collider (LHC) and the potential discovery of supersymmetry, in this work we seek an answer to the following: What are the chances that supersymmetry will be found at the LHC? Will the LHC data be enough to discover a given supersymmetric model? And what other measurements can assist the LHC establish the presence of supersymmetry? As a step toward answering these general questions, we calculate the odds of the next-to-minimal version of the popular supergravity motivated model (NmSuGra) being discovered at the LHC to be 4:3 (57 %). We also demonstrate that viable regions of the NmSuGra parameter space outside the LHC reach can be covered by upgraded versions of dark matter direct detection experiments, such as super-CDMS, at 99 % confidence level. Due to the similarities of the models, we expect very similar results for the constrained minimal supersymmetric standard model (CMSSM).
description: 21 pages, 7 figures
Sprinkler Irrigation in the Pacific Northwest
Creators: name: Stippler, Henry H.
name: Stippler, Henry H.
Publisher: name: Unknown
Year: 1956
Subjects: Crop Production/Industries
Labor and Human Capital
Livestock Production/Industries
Production Economics
Resource /Energy Economics and Policy

description: Excerpts from the report Summary: Sprinkler irrigation in both the high- and low-rainfall areas of the Pacific Northwest has expanded rapidly in recent years. This report provides information on costs of sprinkler-irrigation systems as they relate to crops and climate and to design and operation. The purpose of the study reported here was to learn the physical conditions under which use of sprinklers is most satisfactory, and to ascertain the economic advantages or disadvantages of their use under various conditions. However, little information has been available so far on the economics of sprinkler irrigation -- the costs of operating sprinkler systems, the factors that affect costs, the labor requirements, or the variations in costs caused by different designs and methods of operation. To provide information of this type and to relate it properly to existing conditions and technical differences in design, early in 1949 several research agencies in agriculture pooled their resources to make a cooperative study of the economic phases of sprinkler irrigation in Oregon, Washington, and Idaho.
Zt, gamma t and t production at hadron colliders via strong flavour-changing neutral couplings
Creators: name: Aguilar-Saavedra, J. A.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We consider gq -> Zt, gq -> gamma t and gq -> t production (q=u,c) mediated by strong flavour-changing neutral interactions within an effective operator framework. We provide total cross sections for Tevatron and LHC, showing explicitly that the six processes can be described in full generality in terms of only two parameters (anomalous couplings) for q=u plus two for q=c. In our work we take into account and study in detail the effects of top quark decay. For gamma t, the inclusion of the top quark decay in the matrix element reveals an striking result: the largest contribution to the final state, e.g. gamma l nu b, with l = e, mu, tau, does not result from gq -> gamma t -> gamma l nu b but from on-shell gq -> t production with t -> gamma l nu b, being the photon radiated off the top decay products. This contribution, missed in previous literature, increases the signal cross sections by factors ranging between 3 and 6.5.
description: LaTeX 19 pages, 23 PS figures. Typos corrected in text and equations. Final version to appear in NPB.
title: Thermal Response and Safety Analysis of the Liquefied Gas Storage Tank at Low Filling Ratios
Creators: name: Ren, J.
name: Zhao, B.
name: Sun, J.
name: Bi, M.
name: International Seminar On Fire And Explosion Hazards (9; 2019; Saint Petersburg, Russia)
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2019

description: Experimental and numerical research was conducted to investigate the effect of liquid filling ratios on the
thermal response and safety of a vertical cylindrical liquefied gas storage tank. Low filling ratios were
considered to reveal the distribution characters of the medium temperature and wall temperature, as well
as the pressure rise histories. The results show that with less liquid filled, the dry wall temperature was
higher thus lead to the wet wall to be hotter and more heat transferred into the liquid medium from per
unit wall area. As a result, the temperature in the bulk liquid zone rose faster and the stratification degree
was larger and last longer. Under the combined influence of the higher pressure and the degradation of
the wall material at the higher temperature, the less filled tank can stand for shorter period in thermal
environment. Moreover, if the tank failed after the same heating period, the high grade energy retained in
the liquid medium under lower filling ratio would more likely bring serious consequence.
Climate Related Initiatives Interactions Report n.1
Creators: name: Hanlon, Helen
name: Garrett, Natalie
Publisher: name: Zenodo
Year: 2018
Subjects: MED-GOLD Horizon 2020 project

description: This report details the interactions with other initiatives as part of task 6.1. This task specifically, is pursuing dissemination synergies with other EU initiatives such as Climate-KIC, JPI Climate, FACCE-JPI, JPI Water and related ERA-NET (e.g. ERA4CS, which is the ERA-NET on Climate Services) as well as clustering with other climate service related EC funded projects via H2020 or other complementary programmes (i.e. LIFE, Copernicus, PRIMA, etc.). There is also a focus on getting involved with other agriculture-related initiatives which comprise a significant climate component. This deliverable will be updated annually to track the progress of other initiatives and our involvement with them.
Dust-Bounded ULIRGs? Model Predictions for Infrared Spectroscopic Surveys
Creators: name: Abel, N. P.
name: Dudley, C.
name: Fischer, Jacqueline
name: Satyapal, S.
name: van Hoof, P. A. M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The observed faintness of infrared fine-structure line emission along with the warm far-infrared (FIR) colors of ultraluminous infrared galaxies (ULIRGs) is a long-standing problem. In this work, we calculate the line and continuum properties of a cloud exposed to an Active Galactic Nucleus (AGN) and starburst spectral energy distribution (SED). We use an integrated modeling approach, predicting the spectrum of ionized, atomic, and molecular environments in pressure equilibrium. We find that the effects of high ratios of impinging ionizing radiation density to particle density (i.e. high ionization parameters, or U) can reproduce many ULIRG observational characteristics. Physically, as U increases, the fraction of UV photons absorbed by dust increases, corresponding to fewer photons available to photoionize and heat the gas, producing what is known as a "dust-bounded" nebula. We show that high U effects can explain the "[C II] deficit", the ~1 dex drop in the [C II] 158 micron /FIR ratio seen in ULIRGs when compared to starburst or normal galaxies. Additionally, by increasing U through increasing the ionizing photon flux, warmer dust and thus higher IRAS F(60)/F(100) ratios result. High U effects also predict an increase in [O I]63 micron /[C II] 158 micron and a gradual decline in [O III] 88 micron /FIR, similar to the magnitude of the trends observed, and yield a reasonable fit to [Ne V]14 micron /FIR ratio AGN observations.
description: 34 pages, 13 figures, accepted for publication in the Astrophysical Journal
title: Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¾Ð±ÑÐµÐºÑÐ¾Ð² ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ¸ Ð¾Ñ Ð¿Ð¾ÑÐ°Ð¶Ð°ÑÑÐµÐ³Ð¾ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¹
title: Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÑÐ¼ÐµÐ½ÑÐº, ÐÐ°ÑÐ¸Ð»Ð¸Ð¹
name: ÐÑÐ»Ð¸Ð½ÐºÐ¾Ð²Ð¸Ñ, ÐÐ»ÐµÐºÑÐµÐ¹
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2020
Subjects: Ð­Ð½ÐµÑÐ³ÐµÑÐ¸ÐºÐ°
Ð¢ÐµÑ Ð½Ð¸ÐºÐ° Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸
ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½ÑÐµ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¸

description: Ð Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ð¸ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¾Ð±ÑÐ¸Ðµ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ Ð¸ Ð·Ð°Ð´Ð°ÑÐ¸ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¾Ð±ÑÐµÐºÑÐ¾Ð² ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¾ÑÑÐ°ÑÐ»Ð¸ Ð Ð¤; Ð¸Ð·Ð»Ð°Ð³Ð°ÑÑÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð·Ð°ÑÐ¸ÑÑ Ð¾Ð±ÑÐµÐºÑÐ¾Ð² ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ¸ Ð¾Ñ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð¿Ð¾ÑÐ°Ð¶Ð°ÑÑÐ¸Ñ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² Ð§Ð¡ Ð¸ Ð¿Ð¾ÑÐ°Ð¶Ð°ÑÑÐ¸Ðµ ÑÐ°ÐºÑÐ¾ÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² Ð§Ð¡. ÐÐ±Ð¾ÑÐ½Ð¾Ð²ÑÐ²Ð°ÑÑÑÑ Ð¼ÐµÑÐ¾Ð´Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð¿Ð¾ÑÐ°Ð¶Ð°ÑÑÐ¸Ñ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² Ð§Ð¡ Ð½Ð° Ð¾Ð±ÑÐµÐºÑÑ ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð·Ð°ÑÐ¸ÑÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¾Ð±ÑÐµÐºÑÐ¾Ð² ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ¸ Ð¾Ñ Ð¿Ð¾ÑÐ°Ð¶Ð°ÑÑÐ¸Ñ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¹. ÐÐ°ÑÑÑÑ ÑÐµÑÐµÐ½Ð¸Ñ ÑÑÐ´Ð° Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸ Ð²Ð°Ð¶Ð½ÑÑ Ð·Ð°Ð´Ð°Ñ.
ÐÐ¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð° Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð² Ð¸ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð², Ð·Ð°Ð½Ð¸Ð¼Ð°ÑÑÐ¸ÑÑÑ Ð¸Ð·ÑÑÐµÐ½Ð¸ÐµÐ¼ Ð²Ð¾Ð¿ÑÐ¾ÑÐ¾Ð² Ð·Ð°ÑÐ¸ÑÑ Ð¾Ð±ÑÐµÐºÑÐ¾Ð² Ð½Ð°ÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²Ð° Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¹.
Foliations of Hyperbolic Space by Constant Mean Curvature Hypersurfaces
Creators: name: Coskunuzer, Baris
Publisher: name: arXiv
Year: 2009
Subjects: subject: Differential Geometry (math.DG)
subject: Geometric Topology (math.GT)
subject: FOS: Mathematics
subject: 53A10; 57M50

description: We show that the constant mean curvature hypersurfaces in the hyperbolic n-space spanning the boundary of a star shaped C^{1,1} domain in the asymptotic sphere give a foliation of the hyperbolic n-space. We also show that if C is a closed codimension-1 C^{2,a} submanifold in the asymptotic sphere bounding a unique constant mean curvature hypersurface S_H in the hyperbolic n-space with asymptotic boundary C for any -1
Initial phases of massive star formation in high infrared extinction clouds. I. Physical parameters
Creators: name: Rygl, K. L. J.
name: Wyrowski, F.
name: Schuller, F.
name: Menten, K. M.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The earliest phases of massive star formation are found in cold and dense infrared dark clouds (IRDCs). Since the detection method of IRDCs is very sensitive to the local properties of the background emission, we present here an alternative method to search for high column density in the Galactic plane by using infrared extinction maps. We find clouds between 1 and 5 kpc, of which many were missed by previous surveys. By studying the physical conditions of a subsample of these clouds, we aim at a better understanding of the initial conditions of massive star formation. We made extinction maps of the Galactic plane based on the 3.6-4.5 microns color excess between the two shortest wavelength Spitzer IRAC bands, reaching to visual extinctions of ~100 mag and column densities of 9x10^22 cm^-2. From this we compiled a new sample of cold and compact high extinction clouds. We used the MAMBO array at the IRAM 30m telescope to study the morphology, masses and densities of the clouds and the dense clumps within them. The latter were followed up by pointed ammonia observations with the 100m Effelsberg telescope, to determine rotational temperatures and kinematic distances. Extinction maps of the Galactic plane trace large scale structures such as the spiral arms. The 1.2 mm emission maps reveal that the high extinction clouds contain extended cold dust emission, from filamentary structures to still diffuse clouds. Most of the clouds are dark in 24 microns, but several show already signs of star formation via maser emission or bright infrared sources, suggesting that the high extinction clouds contain a variety of evolutionary stages. The observations suggest an evolutionary scheme from dark, cold and diffuse clouds, to clouds with a stronger 1.2 mm peak and to finally clouds with many strong 1.2 mm peaks, which are also warmer, more turbulent and already have some star formation signposts.
description: 26 pages, 14 figures, 9 tables. Accepted for publication in Astronomy and Astrophysics, small corrections implemented
Discriminating Electroweak-ino Parameter Ordering at the LHC and Its Impact on LFV Studies
Creators: name: Hisano, Junji
name: Nojiri, Mihoko M.
name: Sreethawong, Warintorn
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Current limit on the dark matter relic abundance may suggest that $|μ|$ should be smaller than prediction in the minimal supergravity scenario (mSUGRA) for moderate $m_0$ and $m_{1/2}$. The electroweak-ino parameter $M_1, M_2$ and $|μ|$ are then much closer to each other. This can be realized naturally in the non-universal Higgs mass model (NUHM). Since the heaviest neutralino ($\tildeχ^0_4$) and chargino ($\tildeχ^\pm_2$) have significant gaugino components, they may appear frequently in the left-handed squark decay and then be detectable at the LHC. In such a case, we showed that the hierarchy of $M_1, M_2$ and $|μ|$ can be determined. In the light slepton mass scenario with non-vanishing lepton-flavor violation (LFV) in the right-handed sector, NUHM with small $|μ|$ corresponds to region of parameter space where strong cancellation among leading contributions to $Br(μ\to eγ)$ can occur. We showed that determination of electroweak-ino hierarchy plays a crucial role in resolving cancellation point of $Br(μ\to eγ)$ and determination of LFV parameters. We also discussed test of the universality of the slepton masses at the LHC and the implications to SUSY flavor models.
description: 34 pages, 16 figures
title: ÐÐ½Ð°Ð»Ð¸Ð· Ð¼ÐµÑ Ð¿Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐµÐ³ÑÐ»Ð¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ ÑÑÐ½ÐºÐ° Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸ Ð² Ð¿ÐµÑÐ¸Ð¾Ð´ Ñ 2012 Ð¿Ð¾ 2020 Ð³Ð¾Ð´Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ»Ð¾Ð²Ð°, ÐÐ½Ð°ÑÑÐ°ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³Ð¸Ñ
ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ°
ÑÑÐ½Ð¾Ðº Ð¼Ð¾ÑÐ½Ð¾ÑÑÐµÐ¹ (ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ°)
Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾ ÑÐ½ÐµÑÐ³Ð¸Ð¸

description: ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¼ÐµÑ Ð¿Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐµÐ³ÑÐ»Ð¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ ÑÑÐ½ÐºÐ° Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸ Ð² Ð¿ÐµÑÐ¸Ð¾Ð´ Ñ 2012 Ð¿Ð¾ 2020 Ð³Ð¾Ð´ Ð´Ð»Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ ÑÑÑÑÐ°Ð½ÐµÐ½Ð¸Ñ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼.
Tunable Kondo effect in a single donor atom
Creators: name: Lansbergen, G. P.
name: Tettamanzi, G. C.
name: Verduijn, J.
name: Collaert, N.
name: Biesemans, S.
name: Blaauboer, M.
name: Rogge, S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: The Kondo effect has been observed in a single gate-tunable atom. The measurement device consists of a single As dopant incorporated in a Silicon nanostructure. The atomic orbitals of the dopant are tunable by the gate electric field. When they are tuned such that the ground state of the atomic system becomes a (nearly) degenerate superposition of two of the Silicon valleys, an exotic and hitherto unobserved valley Kondo effect appears. Together with the regular spin Kondo, the tunable valley Kondo effect allows for reversible electrical control over the symmetry of the Kondo ground state from an SU(2)- to an SU(4) -configuration.
description: 10 pages, 8 figures
title: Ð Ð°Ð·Ð²Ð¸ÑÐ¸Ðµ ÑÐºÐ¾ÑÐ¾ÑÑÐ½Ð¾-ÑÐ¸Ð»Ð¾Ð²ÑÑ ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐµÐ¹ Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð³Ð°Ð½Ð´Ð±Ð¾Ð»Ð¸ÑÑÐ¾Ðº
title: The development of speed and strength capacities of professional handball players
Creators: name: Ð Ð°Ð¼Ð·Ð°Ð¹ÑÐµÐ²Ð°, Ð.
name: "Ð¡Ð¿Ð¾ÑÑ, ÑÐµÐ»Ð¾Ð²ÐµÐº, Ð·Ð´Ð¾ÑÐ¾Ð²ÑÐµ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð½Ð°ÑÑÐ½ÑÐ¹ ÐºÐ¾Ð½Ð³ÑÐµÑÑ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2021
Subjects: ÑÐºÐ¾ÑÐ¾ÑÑÐ½Ð¾-ÑÐ¸Ð»Ð¾Ð²ÑÐµ ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸
ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ðµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ
Ð³Ð°Ð½Ð´Ð±Ð¾Ð»

description: Ð¦ÐµÐ»ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ ÑÐºÐ¾ÑÐ¾ÑÑÐ½Ð¾-ÑÐ¸Ð»Ð¾Ð²ÑÑ ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐµÐ¹ Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð³Ð°Ð½Ð´Ð±Ð¾Ð»Ð¸ÑÑÐ¾Ðº Ð·Ð° ÑÑÐµÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ¾Ð² ÑÐ¿ÑÐ°Ð¶Ð½ÐµÐ½Ð¸Ð¹ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÐºÐ»ÑÑÐµÐ½Ð¸Ðµ Ð² ÑÑÐµÐ½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½ÑÐ¹ Ð¿ÑÐ¾ÑÐµÑÑ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ¾Ð² ÑÐ¿ÑÐ°Ð¶Ð½ÐµÐ½Ð¸Ð¹ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð½Ð°Ð±Ð¸Ð²Ð½ÑÑ Ð¼ÑÑÐµÐ¹, ÑÑÐ¿Ð°Ð½Ð´ÐµÑ-ÐºÐ¾Ð»ÐµÑ Ð¸ ÑÑÐ¼Ð± ÑÐ¿Ð¾ÑÐ¾Ð±ÑÑÐ²ÑÐµÑ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ ÑÐºÐ¾ÑÐ¾ÑÑÐ½Ð¾-ÑÐ¸Ð»Ð¾Ð²ÑÑ ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐµÐ¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð³Ð°Ð½Ð´Ð±Ð¾Ð»Ð¸ÑÑÐ¾Ðº.
description: The aim of the study is to develop the speed and strength capacities of professional handball players through the use of sets of exercises using special equipment. The inclusion in the training process of exercises with stuffed balls, expander rings and plyometric boxes help to increase the performance of speed and strength capacities of professional handball players.
Growth and physiological response of Solanum nigrum L. to organic and/or inorganic fertilisers
Creators: name: Bvenura, Callistus
name: Afolayan, Anthony J.
Publisher: name: Association for Applied Botany e.V., German Society for Quality Research on Plant Foods
Year: 2014
Subjects: root
shoot ratio
stem diameter
chlorophyll
moisture
leaf area
plant height

description: Journal of Applied Botany and Food Quality; 87; 168-174
description: A pot experiment was conducted to determine the effect of fertilisers on the growth and physiological response of Solanum nigrum. The experiment was laid out in a Randomised Complete Block Design with five treatments: Control (T1); 100 kg N/ha (T2); 8.13 t manure/ ha (T3); 100 kg N/ha + 8.13 t manure/ ha (T4) and 50 kg N/ha + 4.07 t manure/ ha (T5). Plant height, total number of leaves, chlorophyll, moisture, root: shoot ratio, leaf area and stem diameter were measured using standard growth indicator methods. Fertilisers improved the yield, quality and growth of Solanum nigrum. Application of 100 kg N/ha produced the best total number of leaves; root: shoot ratio and stem diameter values; 100 kg N/ha + 8.13 t manure/ha produced the best chlorophyll values and 50 kg N/ha + 4.07 t manure/ha increased moisture, leaf area and plant height. The control showed signs of nutrient stress and inorganic fertiliser applied independently did not significantly affect the growth parameters. Although parameters responded differently to each fertiliser treatment, applying a combination of organic and inorganic fertiliser may be a good option to poor resource farmers who may not be able to afford inorganic fertilisers.
Model for coiling and meandering instability of viscous threads
Creators: name: Nagahiro, S.
name: Hayakawa, Y.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: A numerical model is presented to describe both the transient and steady-state dynamics of viscous threads falling onto a plane. The steady-state coiling frequency w is calculated as a function of fall height H. In the case of weak gravity, w ~ H^{-1} and w ~ H are obtained for lower and higher fall heights respectively. When the effect of gravity is significant, the relation w ~ H^2 is observed. These results agree with the scaling laws previously predicted. The critical Reynolds number for coil-uncoil transition is discussed. When the gravity is weak, the transition occurs with hysteresis effects. If the plane moves horizontally at a constant speed, a variety of meandering oscillation modes can be observed experimentally. The present model also can describe this phenomenon. The numerically obtained state diagram for the meandering modes qualitatively agrees with the experiment.
description: 12 pages, 10 figures
Collaborative filtering with diffusion-based similarity on tripartite graphs
Creators: name: Shang, Ming-Sheng
name: Zhang, Zi-Ke
name: Zhou, Tao
name: Zhang, Yi-Cheng
Publisher: name: arXiv
Year: 2009
Subjects: subject: Information Retrieval (cs.IR)
subject: FOS: Computer and information sciences

description: Collaborative tags are playing more and more important role for the organization of information systems. In this paper, we study a personalized recommendation model making use of the ternary relations among users, objects and tags. We propose a measure of user similarity based on his preference and tagging information. Two kinds of similarities between users are calculated by using a diffusion-based process, which are then integrated for recommendation. We test the proposed method in a standard collaborative filtering framework with three metrics: ranking score, Recall and Precision, and demonstrate that it performs better than the commonly used cosine similarity.
description: 8 pages, 4 figures, 1 table
Effect of 24-epibrassinolide on salinity-induced changes in loquat (Eriobotrya japonica Lindl)
Creators: name: Sadeghi, Fatemeh
name: Shekafandeh, Akhtar
Publisher: name: Association for Applied Botany e.V., German Society for Quality Research on Plant Foods
Year: 2014
Subjects: salt stress
24-epibrassinolide
Loquat
growth
mineral nutrients

description: Journal of Applied Botany and Food Quality; 87; 190-195
description: This study was carried out to investigate the role of 24-epibrassinolide (24-EBL) in inducing loquat plant salt tolerance. Plants were treated with five levels of salt, so that the electrical conductivity (EC) of 0.5 (control), 2, 4, 6 and 8 dS m-1 was established in pots. Then, the plants were sprayed with different concentrations of 24-EBL (0, 0.25, 0.5 and 0.75 mg l-1). Under salt stress, the plant growth parameters and chlorophyll content decreased, while the total soluble sugars and proline contents considerably increased. However, the application of 24-EBL significantly ameliorated the plant growth by reducing the adverse effects of salinity on the examined parameters. The ion concentrations showed an increase in accumulation of Na+ and Cl coupled with a decrease in K+ with increasing salinity in medium. Exogenous application of 24-EBL had a significant effect on leaf Na+, K+, Cl- contents. Out of different 24-EBL concentrations, the effects of 0.5 mg l-1 proved the best under stress conditions.