cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸
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ÑÐ·ÑÐ¼Ð¸Ð½Ð° , ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ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: 2018
Subjects: ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÑ
Ð²Ð½ÐµÑÐ½Ð¸Ð¹ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ
Ð°ÑÐ´Ð¸Ñ
Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«ÐÐ¸ÐºÑÐ¾Ð½Â».
ÐÐµÑÐ¾Ð´Ð°Ð¼Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÑÑÑÑ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ Ð¿Ð¾ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐµÐ¼Ðµ, Ð¾Ð±Ð¾Ð±ÑÐµÐ½Ð¸Ðµ Ð¸ ÑÐ¸ÑÑÐµÐ¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ñ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½Ð¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð°Ð½Ð°Ð»Ð¸Ð·Ð°, ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ, Ð´ÐµÐ´ÑÐºÑÐ¸Ð¸, Ð¸Ð½Ð´ÑÐºÑÐ¸Ð¸, ÑÐ¸Ð½ÑÐµÐ·Ð°.
Ð¦ÐµÐ»Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ â ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸ Ð¸ ÐµÐµ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð½Ð° ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÑÑÑÐµÐ¼ ÑÑÐ±ÑÐµÐºÑÐµ. ÐÑÐ½Ð¾Ð²Ð½ÑÐ¼Ð¸ Ð·Ð°Ð´Ð°ÑÐ°Ð¼Ð¸ ÑÐ²Ð»ÑÐ»Ð¸ÑÑ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ ÑÐ¾ÑÑÐ°Ð²Ð° Ð¸ Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¸Ñ ÑÐ¾ÑÐ¼ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¸Ðµ Ð¾ÑÐ½Ð¾Ð² Ð°ÑÐ´Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸ ÐÐÐ Â«ÐÐ¸ÐºÑÐ¾Ð½Â», ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹, Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÑ Ð½Ð° ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð°ÑÐ´Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸.
Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ» Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð¾Ð²Ð°Ð½ Ð¸ ÑÐ¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½ Ð¿ÑÐ¾ÑÐµÑÑ Ð°ÑÐ´Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸ ÐÐÐ Â«ÐÐ¸ÐºÑÐ¾Ð½Â», Ð¿Ð¾ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ°Ð¼ Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸ Ð±ÑÐ»Ð¸ Ð¿Ð¾Ð´Ð²ÐµÐ´ÐµÐ½Ñ Ð¸ÑÐ¾Ð³Ð¸ Ð¸ ÑÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¾ Ð¼Ð½ÐµÐ½Ð¸Ðµ Ð¾ Ð´Ð¾ÑÑÐ¾Ð²ÐµÑÐ½Ð¾ÑÑÐ¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸.
ÐÑÐ»Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¾ÑÐ½Ð¾Ð² Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸, ÑÑÐ¾ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ñ ÑÐ»ÑÑÑÐ¸ÑÑ ÐºÐ°ÑÐµÑÑÐ²Ð¾ Ð°ÑÐ´Ð¸ÑÐ¾ÑÑÐºÐ¸Ñ Ð¿ÑÐ¾Ð²ÐµÑÐ¾Ðº Ð¸, ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÐµÐ½Ð½Ð¾, Ð¿Ð¾Ð²ÑÑÐ¸Ñ ÑÑÐ¾Ð²ÐµÐ½Ñ Ð´Ð¾Ð²ÐµÑÐ¸Ñ Ð²Ð½ÐµÑÐ½Ð¸Ñ Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÐµÐ¹ Ðº Ð´Ð°Ð½Ð½ÑÐ¼ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸, ÑÑÐ¾ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐµÑ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÑÑ Ð·Ð½Ð°ÑÐ¸Ð¼Ð¾ÑÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ.
Statistical and Econometric Models for Financial Networks
Creators: name: BOYAO WU
Publisher: name: Monash University
Year: 2021
Subjects: subject: 140302 Econometric and Statistical Methods
subject: FOS: Economics and business

description: Network economics offers an innovative perspective for bridging general equilibrium theories and game theories under the same framework. However, potential interactive patterns of financial agents challenge the application of network economics in finance settings. This thesis discusses statistical and econometric models to generate and further study financial networks, which can supplement studies on financial networks by introducing novel constructing methods and general econometric models with the networking effect, which benefits wider understanding of global finance systems.
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¾Ð¿ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² ÑÐ¾Ð½ÐºÐ¸Ñ ÑÐ»Ð¾ÑÐ², ÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÐ¸Ñ Ð½Ð°Ð½Ð¾ÑÐ°ÑÑÐ¸ÑÑ ÐºÑÐµÐ¼Ð½Ð¸Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¢ÐµÐ¿Ð»ÑÐºÐ¾Ð², ÐÐ¸ÑÐ°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: 2016
Subjects: Ð½Ð°Ð½Ð¾ÑÐ°ÑÑÐ¸ÑÑ ÐºÑÐµÐ¼Ð½Ð¸Ñ
Ð½Ð°Ð½Ð¾ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¸ÑÐµÑÐºÐ¸Ð¹ ÐºÑÐµÐ¼Ð½Ð¸Ð¹
ÑÐ¾ÑÐ¾Ð»ÑÐ¼Ð¸Ð½ÐµÑÑÐµÐ½ÑÐ¸Ñ
ÑÐ¾Ð»Ð½ÐµÑÐ½ÑÐµ ÑÐ»ÐµÐ¼ÐµÐ½ÑÑ
silicon nanoparticles
nanocrystalline silicon
photoluminescence
solar cells

description: Ð¦ÐµÐ»ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐ»Ð¾ÑÑ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¾Ð¿ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² ÑÐ¾Ð½ÐºÐ¸Ñ ÑÐ»Ð¾ÑÐ², ÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÐ¸Ñ Ð½Ð°Ð½Ð¾ÑÐ°ÑÑÐ¸ÑÑ ÐºÑÐµÐ¼Ð½Ð¸Ñ, Ð° Ð¸Ð¼ÐµÐ½Ð½Ð¾, Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ðµ ÑÐ¿ÐµÐºÑÑÐ¾Ð² ÑÐ¾ÑÐ¾Ð»ÑÐ¼Ð¸Ð½ÐµÑÑÐµÐ½ÑÐ¸Ð¸ ÑÐ»Ð¾ÐµÐ², Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð¹ ÑÐ¸ÑÐ¸Ð½Ñ Ð·Ð°Ð¿ÑÐµÑÑÐ½Ð½Ð¾Ð¹ Ð·Ð¾Ð½Ñ Ð¸ ÑÑÐµÐ´Ð½Ð¸Ñ ÑÐ°Ð·Ð¼ÐµÑÐ¾Ð² Ð½Ð°Ð½Ð¾ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¾Ð² Ð² ÑÐ»Ð¾Ðµ. ÐÐ°Ð´Ð°ÑÐµÐ¹ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ» Ð¿Ð¾Ð¸ÑÐº ÑÐ°ÐºÐ¾Ð¹ Ð¾Ð¿ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÐµÐ¼Ñ Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ñ ÑÐ¾ÑÐ¾Ð»ÑÐ¼Ð¸Ð½ÐµÑÑÐµÐ½ÑÐ¸Ð¸, ÐºÐ¾ÑÐ¾ÑÐ°Ñ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ð»Ð° Ð±Ñ ÑÐ¼ÐµÐ½ÑÑÐ¸ÑÑ Ð²ÐºÐ»Ð°Ð´ ÑÐ¾ÑÐ¾Ð»ÑÐ¼Ð¸Ð½ÐµÑÑÐµÐ½ÑÐ¸Ð¸ Ð¿Ð¾Ð´Ð»Ð¾Ð¶ÐºÐ¸ Ð¸ Ð²ÑÐ´ÐµÐ»Ð¸ÑÑ Ð½Ð° ÐµÐµ ÑÐ¾Ð½Ðµ ÑÐ¿ÐµÐºÑÑ ÑÐ¾ÑÐ¾Ð»ÑÐ¼Ð¸Ð½ÐµÑÑÐµÐ½ÑÐ¸Ð¸ ÑÐ»Ð¾Ñ Ñ Ð½Ð°Ð½Ð¾ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð°Ð¼Ð¸ ÐºÑÐµÐ¼Ð½Ð¸Ñ.
description: The goal of this work was the experimental research of the optical properties of thin layers containing silicon nanoparticles, namely, measuring the photoluminescence spectra of the layers, evaluation of the effective band gap and the average size of the nanocrystals in the layer. The aim of the work was to find such an optical scheme for the photoluminescence setup, which would allow reducing the contribution of the photoluminescence of the substrate and extracting spectrum of the layer with silicon nanocrystals from the background photoluminescence.
On Odd Order Nilpotent Groups With Class 2
Creators: name: Jain, Vivek Kumar
Publisher: name: arXiv
Year: 2009
Subjects: subject: Group Theory (math.GR)
subject: FOS: Mathematics
subject: 20D15

description: Let $G$ be an odd order nilpotent group with class 2 and $e$ denotes the exponent of its commutator subgroup. Let $e=p_1^{r_1}p_2^{r_2}... p_s^{r_s}$, where $p_i$'s are odd primes and $r_i$'s are non-negative integers. Then there are at least $r_1+r_2+... +r_s$ non-isomorphic nilpotent groups with class two and the order of each of the group is equal to the order of $G$.
description: 5 pages
title: Ð¤Ð¸Ð½Ð¸ÑÐ½Ð°Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ° Ð´ÐµÑÐ°Ð»ÐµÐ¹ ÑÐµÐ½ÑÑÐ¾Ð±ÐµÐ¶Ð½Ð¾-ÑÐ¿Ð»Ð¾ÑÐ½ÐµÐ½Ð½ÑÐ¼ Ð¿Ð¾ÑÐ¾ÐºÐ¾Ð¼ ÑÐ²Ð¾Ð±Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð°Ð±ÑÐ°Ð·Ð¸Ð²Ð°
title: Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ
titleType: Subtitle
Creators: name: Ð¨Ð¸ÑÐºÐ¸Ð½, ÐÐµÐ½Ð¸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ÐµÐ½ÑÑÐ¾Ð±ÐµÐ¶Ð½Ð¾-ÑÐ¿Ð»Ð¾ÑÐ½ÐµÐ½Ð½ÑÐ¹ Ð¿Ð¾ÑÐ¾Ðº ÑÐ²Ð¾Ð±Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð°Ð±ÑÐ°Ð·Ð¸Ð²Ð°
Ð²Ð¸Ñ ÑÐµÐ²Ð¾Ð¹ Ð³Ð¸Ð´ÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ¾ÑÐ¼Ð¾Ð·
ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð°Ñ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ°
Ð°Ð±ÑÐ°Ð·Ð¸Ð²Ð½Ð¾Ðµ Ð·ÐµÑÐ½Ð¾
ÑÑÐµÐ¼ Ð¼ÐµÑÐ°Ð»Ð»Ð°
centrifugal-compacted stream free of abrasive material
vortex hydrodynamic brake
experimental setup
abrasive grain
eat metal

description: Ð Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¼ Ð¿ÑÐ¾ÐµÐºÑÐµ, ÑÐµÐ¼Ð° ÐºÐ¾ÑÐ¾ÑÐ¾Ð³Ð¾, Â«Ð¤Ð¸Ð½Ð¸ÑÐ½Ð°Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ° Ð´ÐµÑÐ°Ð»ÐµÐ¹ ÑÐµÐ½ÑÑÐ¾Ð±ÐµÐ¶Ð½Ð¾-ÑÐ¿Ð»Ð¾ÑÐ½ÐµÐ½Ð½ÑÐ¼ Ð¿Ð¾ÑÐ¾ÐºÐ¾Ð¼ ÑÐ²Ð¾Ð±Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð°Ð±ÑÐ°Ð·Ð¸Ð²Ð°Â» Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¿ÑÑÐ¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐµÐ½ÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð´ÐµÑÐ°Ð»ÐµÐ¹ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐµÐ½ÑÑÐ¾Ð±ÐµÐ¶Ð½Ð¾-ÑÐ¿Ð»Ð¾ÑÐ½ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐ¾ÐºÐ° ÑÐ²Ð¾Ð±Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð°Ð±ÑÐ°Ð·Ð¸Ð²Ð° (Ð¦Ð£ÐÐ¡Ð). ÐÐ¿Ð¸ÑÐ°Ð½Ñ Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¸Ðµ Ð¸ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿ ÑÐ°Ð±Ð¾ÑÑ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð¾Ð¹ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸, Ð² ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ñ ÐºÐ¾ÑÐ¾ÑÐ¾Ð¹ Ð²ÐºÐ»ÑÑÐµÐ½ Ð²Ð¸ÑÑÐµÐ²Ð¾Ð¹ Ð³Ð¸Ð´ÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ¾ÑÐ¼Ð¾Ð· Ð¸ ÑÐµÐ·ÐµÑÐ²ÑÐ°Ñ Ð´Ð»Ñ ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ ÑÐ¾ÑÐ¼Ð¾Ð·Ð½Ð¾Ð¹ Ð¶Ð¸Ð´ÐºÐ¾ÑÑÐ¸ Ð´Ð»Ñ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¾ÑÐ¼Ð¾Ð·Ð½Ð¾Ð³Ð¾ Ð¼Ð¾Ð¼ÐµÐ½ÑÐ°. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ ÑÑÐµÐ¼Ð° Ð¼ÐµÑÐ°Ð»Ð»Ð° Ð¾Ñ Ð³Ð»ÑÐ±Ð¸Ð½Ñ Ð¿Ð¾Ð³ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð´ÐµÑÐ°Ð»Ð¸ Ð² Ð¦Ð£ÐÐ¡Ð Ð¿ÑÐ¸ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÐ¸ÑÐ»Ð°Ñ Ð¾Ð±Ð¾ÑÐ¾ÑÐ¾Ð² ÑÐ¾ÑÐ¾ÑÐ°. ÐÑÐ» Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾Ð¹ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸, Ð¿ÑÐ¾ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¶Ð¸Ð·Ð½ÐµÐ´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸.
description: The graduate work, whose theme is, "Finishing details centrifugally compacted abrasive stream free" analyzed ways of increasing intensification of processing parts using centrifugal compressed stream free abrasive (CMSFA). Describe the purpose and operation of a pilot plant in the design which included a hydrodynamic vortex brake and a reservoir for storing brake fluid to regulate the braking torque. Experimental studies to determine metal removal depending on the depth of immersion in the details CMSFA at different rotor speed. A calculation was made of technical and economic indicators of the developed installation worked out health and safety issues.
title: ÐÐ½Ð¶ÐµÐ½ÐµÑÐ½Ð¾Ðµ Ð¾Ð±ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾ ÑÑÐ°ÑÑÐºÐ° Ð² Ð¿Ð¾ÑÐµÐ»ÐºÐµ Â«Ð¡Ð¸Ð½ÑÐ²Ð¸Ð½Ð¾Â»
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Ð½Ð¾Ð², ÐÐ½Ð°ÑÐ¾Ð»Ð¸Ð¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð¾Ð±ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾
Ð´ÑÐµÐ½Ð°Ð¶
Ð²Ð¾Ð´Ð¾Ð¾ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ðµ
Ð²Ð¾Ð´Ð¾Ð¾ÑÐ¸ÑÑÐºÐ°
ÐºÐ°Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ
Ð°ÑÑÐ¾ÑÐµÐ½Ðº
Ð´Ð°ÑÐ½ÑÐ¹ ÑÑÐ°ÑÑÐ¾Ðº

description: ÐÐ¸Ð¿Ð»Ð¾Ð¼Ð½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½ Ð²Ð¾Ð¿ÑÐ¾ÑÐ°Ð¼ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° ÑÑÐ°ÑÑÐºÐ° Ð² Ð¿Ð¾ÑÐµÐ»ÐºÐµ Â«Ð¡Ð¸Ð½ÑÐ²Ð¸Ð½Ð¾Â». ÐÑÐ¾ÐµÐºÑ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ Ð·Ð°Ð´Ð°Ð½Ð¸ÐµÐ¼ Ð½Ð° Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸ÑÐ¼Ð¸ Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐ¸Ñ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½ÑÑ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ¾Ð² Ð² ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ðµ.
A Comprehensive Study of the Spectral Variation and the Brightness Profile of Young Pulsar Wind Nebulae
Creators: name: Hu, Chin-Ping
name: Ishizaki, Wataru
name: Ng, C. -Y.
name: Tanaka, Shuta J.
name: Mong, Y. -L.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present a systematic study of particle transport by diffusion in young pulsar wind nebulae (PWNe). We selected nine bright sources that are well resolved with the Chandra X-ray Observatory. We analyzed archival data to obtain their radial profiles of photon index ($Γ$) and surface brightness ($Σ$) in a consistent way. These profiles were then fit with a pure diffusion model that was tested on Crab, 3C 58 and G21.5$-$0.9 before. In addition to the spectral softening due to the diffusion, we calculated the synchrotron power and built up the theoretical surface brightness profile. For each source, we performed separate fits to the $Γ$ and the $Σ$ profiles. We found these two profiles of most PWNe are similar, except for Crab and Vela. Both profiles can be well described by our model, suggesting that diffusion dominates the particle transport in most sampled PWNe. The discrepancy of parameters between the $Γ$ profile and $Σ$ profiles is relatively large for 3C 58 and G54.1+0.3. This difference could be attributed to the elongated shape, reflecting boundary, and the non-uniform magnetic field. Finally, we found no significant correlations between diffusion parameters and physical parameters of PWN and pulsar.
description: 15 pages, 6 figures, accepted for publication in ApJ
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸, ÑÐ°Ð±Ð¾ÑÐ°ÑÑÐµÐ¹ Ð½Ð° ÑÑÐ½ÐºÐµ ÑÐ°Ð·Ð²Ð»ÐµÐºÐ°ÑÐµÐ»ÑÐ½ÑÑ ÑÑÐ»ÑÐ³ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐ¾ÑÐ²ÐµÐ¶ÑÐºÐ¸Ð¹ ÐÐ°ÑÐºÂ»)
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: Ð¢ÑÐµÑÑÑÐºÐ¾Ð²Ð°, 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: 2018
Subjects: ÑÑÑÐ°ÑÐµÐ³Ð¸Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«ÐÐ¾ÑÐ²ÐµÐ¶ÑÐºÐ¸Ð¹ ÐÐ°ÑÐºÂ».
Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸, ÑÐ°Ð±Ð¾ÑÐ°ÑÑÐµÐ¹ Ð½Ð° ÑÑÐ½ÐºÐµ ÑÐ°Ð·Ð²Ð»ÐµÐºÐ°ÑÐµÐ»ÑÐ½ÑÑ ÑÑÐ»ÑÐ³ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐ¾ÑÐ²ÐµÐ¶ÑÐºÐ¸Ð¹ ÐÐ°ÑÐºÂ»).
ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÑÑÐµÑÑÐ²ÑÑÑÐµÐ¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð±ÑÐ»Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸.
 ÐÑÐ»Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð¡Ð´ÐµÐ»Ð°Ð½ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð· Ð²ÑÑÑÑÐºÐ¸ Ð¸ Ð·Ð°ÑÑÐ°Ñ Ð¾Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÐ¼ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ð° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹. ÐÑÐ±ÑÐ°Ð½ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½ÑÐ¹ Ð²Ð°ÑÐ¸Ð°Ð½Ñ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð´Ð»Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ.
 Ð ÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¼ÐµÑ, Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÑ Ð½Ð° ÑÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÑ Ðº ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÐ»Ð° ÐºÐ»Ð¸ÐµÐ½ÑÐ¾Ð² ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐ¾Ð¹ Ð¿ÑÐ¸Ð±ÑÐ»Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸.
Solar Photovoltaics in British Columbia: A Scoping Review of Residential, Grid-Connected Systems
Creators: name: Tynan, Sean
Publisher: name: The University of British Columbia
Year: 2016

description: This document provides information regarding recent developments in small-scale residential, grid-connected photovoltaic systems. The purpose of the document is three-fold: to explore the current status and potential of these systems within the Province of British Columbia, to identify the major barriers to PV systems, and to examine the key policy interventions that would be required to bring about widespread uptake of these systems. Research was conducted primarily through a review of the literature. This information was supplemented through a market survey and interviews with key informants from both the public and private sector. The document contains two substantive findings. Firstly, there are environmental benefits (greenhouse gas reductions) that will result from the uptake of residential PV systems within the Province. Secondly, cost is by far the largest barrier to PV system uptake. A major policy intervention to rebalance the economics of PV systems in BC would be required to support their widespread adoption within the next decade. Economic interventions to directly subsidize solar PV would likely be expensive relative to other forms of renewable energy in BC, and are therefore unlikely to be justifiable at present. If the price of PV systems reduces sufficiently over time, such measures could be considered. Over the shorter term, then, policies which support PV as well as other forms of renewable energy are recommended.
Future dark energy constraints from measurements of quasar parallax: Gaia, SIM and beyond
Creators: name: Ding, Fiona
name: Croft, Rupert A. C.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: (Abridged) A consequence of the Earth's motion with respect to the CMB is that over a 10 year period it will travel a distance of ~800 AU. As first noted by Kardashev in 1986, this baseline can be used to carry out astrometric measurements of quasar parallaxes, so that only microarcsecond precision is necessary to detect parallax shifts of objects at gigaparsec distances. Such precision will soon be approached with the launch of the astrometric satellites Gaia and SIM. We use a Fisher matrix formalism to investigate the constraints that these and future missions may be able to place on the cosmological distance scale and dark energy. We find that by observing around a million quasars as planned, an extended 10 year Gaia mission could detect quasar parallax shifts at the 2.8 sigma level and so measure the Hubble constant to within 25 km/s. For the interferometer SIMLite, a Key Project using 2.4 % of the total mission time to observe 750 quasars could detect the effect at the 2 sigma level. Gaia and a dedicated SIMLite only weakly constrain the presence of a cosmological constant at the ~1 sigma levels. We also investigate future mission concepts, such as an interferometer similar in scope and design to NASA's Terrestrial Planet Finder. This could in principle measure the dark energy parameters w_0 and w_a with high precision, yielding a Figure of Merit larger than the stage IV experiments considered by the the Dark Energy Task Force. Unlike perhaps all other probes of dark energy there appear to be no obvious astrophysical sources of systematic error. There is however uncertainty regarding the statistical errors. As well as measurement error, there will be small additional contributions from image centroiding of variable sources, quasar peculiar motions and weak microlensing by stars along the line of sight.
description: 10 pages, 3 figures, revised version: used Gaia and SIM up to date proper motion errors, MNRAS in press
title: ÐÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð±ÑÑÑÑÐ¾ÑÑ ÑÐµÐ°ÐºÑÐ¸Ð¸ Ñ Ð²ÑÐ°ÑÐ°ÑÐµÐ¹ 12-14 Ð»ÐµÑ Ð² ÑÑÑÐ±Ð¾Ð»Ðµ Ð»Ð¸Ñ Ñ ÑÐµÑÐµÐ±ÑÐ°Ð»ÑÐ½ÑÐ¼ Ð¿Ð°ÑÐ°Ð»Ð¸ÑÐ¾Ð¼
title: Development of reaction speed for 12-14 age group goalkeepers in football for people with cerebral paralysis
Creators: name: ÐÑÑÐ°Ð½Ð¾Ð²Ð°, Ð¡.
name: ÐÐºÑÐµÐ½Ð¾Ð², Ð.
name: Ð¢ÐµÑÐµÐ½ÑÑÐµÐ², 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: Ð°Ð´Ð°Ð¿ÑÐ¸Ð²Ð½ÑÐ¹ ÑÐ¿Ð¾ÑÑ
ÑÑÑÐ±Ð¾Ð»
Ð´ÐµÑÑÐºÐ¸Ð¹ ÑÐµÑÐµÐ±ÑÐ°Ð»ÑÐ½ÑÐ¹ Ð¿Ð°ÑÐ°Ð»Ð¸Ñ
Ð±ÑÑÑÑÐ¾ÑÐ° ÑÐµÐ°ÐºÑÐ¸Ð¸
ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸
Ð¿Ð¾Ð´Ð²Ð¸Ð¶Ð½ÑÐµ Ð¸Ð³ÑÑ

description: Ð ÑÑÐ°ÑÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð±ÑÑÑÑÐ¾ÑÑ ÑÐµÐ°ÐºÑÐ¸Ð¸ Ñ Ð²ÑÐ°ÑÐ°ÑÐµÐ¹ 12-14 Ð»ÐµÑ Ð² ÑÑÑÐ±Ð¾Ð»Ðµ Ð»Ð¸Ñ Ñ ÑÐµÑÐµÐ±ÑÐ°Ð»ÑÐ½ÑÐ¼ Ð¿Ð°ÑÐ°Ð»Ð¸ÑÐ¾Ð¼, ÑÑÐµÐ´ÑÑÐ²Ð°Ð¼Ð¸ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¸ Ð¿Ð¾Ð´Ð²Ð¸Ð¶Ð½ÑÑ Ð¸Ð³Ñ. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ½ÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð², Ð¿ÐµÑÐµÑÐµÐ½Ñ ÑÐµÑÑÐ¾Ð² Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½ÑÐ¹ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¿ÑÐ°Ð¶Ð½ÐµÐ½Ð¸Ð¹ Ð¸ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ.
description: The article is dedicated to the issues of development of reaction speed among goalkeepers of 12-14 years old in football for people with cerebral paralysis, means of physical training and outdoor games. An analysis of literature sources, a list of tests and a developed set of physical exercises and research results are presented.
A spatially dependent correction of Gaia EDR3 parallax zero-point offset based on 0.3 million LAMOST DR8 giant stars
Creators: name: Wang, Chun
name: Yuan, Haibo
name: Huang, Yang
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We have studied the zero-point offset of Gaia early Data Release 3 (EDR3) parallaxes based on a sample of 0.3 million giant stars built from the LAMOST data with distance accuracy better than 8.5\%. The official parallax zero-point corrections largely reduce the global offset in the Gaia EDR3 parallaxes: the global parallax offsets are $-$27.9 $μ$as and $-$26.5 $μ$as (before correction) and $+$2.6 $μ$as and $+$2.9 $μ$as (after correction) for the five- and six-parameter solutions, respectively. The bias of the raw parallax measurements is significantly dependent on the $G$ magnitudes, spectral colors, and positions of stars. The official parallax zero-point corrections could reduce parallax bias patterns with $G$ magnitudes, while could not fully account the patterns in the spaces of the spectral colors and positions. In the current paper, a spatially dependent parallax zero-point correction model for Gaia EDR3 five-parameter solution in the LAMOST footprint is firstly provided with the advantage of huge number of stars in our sample.
description: 9 pages, 6 figures, 1 table, accepted for publication in AJ
An Improvement to a Berezin-Li-Yau type inequality for the Klein-Gordon Operator
Creators: name: Yolcu, Selma Yildirim
Publisher: name: arXiv
Year: 2009
Subjects: subject: Spectral Theory (math.SP)
subject: FOS: Mathematics
subject: 35P15, 35S99

description: In this article we improve a lower bound for $\sum_{j=1}^kβ_j$ (a Berezin-Li-Yau type inequality) in [E. M. Harrell II and S. Yildirim Yolcu, Eigenvalue inequalities for Klein-Gordon Operators, J. Funct. Analysis, 256(12) (2009) 3977-3995]. Here $β_j$ denotes the $j$th eigenvalue of the Klein Gordon Hamiltonian $H_{0,Ω}=|p|$ when restricted to a bounded set $Ω\subset {\mathbb R}^n$. $H_{0,Ω}$ can also be described as the generator of the Cauchy stochastic process with a killing condition on $\partial Ω$. (cf. [R. Banuelos, T. Kulczycki, Eigenvalue gaps for the Cauchy process and a Poincare inequality, J. Funct. Anal. 211 (2) (2004) 355-423]; [R. Banuelos, T. Kulczycki, The Cauchy process and the Steklov problem, J. Funct. Anal. 234 (2006) 199-225].) To do this, we adapt the proof of Melas ([ A. D. Melas, A lower bound for sums of eigenvalues of the Laplacian, Proceedings of the American Mathematical Society, 131(2) (2002) 631-636]), who improved the estimate for the bound of $\sum_{j=1}^kλ_j$, where $λ_j$ denotes the $j$th eigenvalue of the Dirichlet Laplacian on a bounded domain in ${\mathbb R}^d$.
description: 7 pages
General Electric Quarterly Survey 79-04, Versions I , II & III and College Student Version
Creators: name: Electric, General
Publisher: name: Roper Center for Public Opinion Research
Year: 2022

description: Adult sample: Most interesting concerns (3); local community interests (1); solving community problems (2); life satisfaction (1); interest in national issues (1); national issues discussions (10); desired community changes (12); taxes for community services (12); race relations (1); future race relations (1); companies helping race relations (1); price controls (1); wage controls (1); unaffordable purchases (1); future expensive purchases (1); electricity fuels (3); future fuels (2); need for additional plants (1); power plant approvals (3); government activity changes (26); government company regulations (1); company effects (1); electricity value (1); programs affecting economy (9); nuclear plant distance (2); nuclear plant dangers (1); magazine readership (1); television viewing habits (2); courses taken (7); financial situation (2); income change (1); future plans (2); inflation (5); unemployment (1); recession (2). College student sample: Most interesting concerns (3); life satisfaction (1); interest in national issues (1); national issues discussions (10); price controls (1); wage controls (1); race relations (1); future race relations (1); companies helping race relations (1); electricity fuels (3); future fuels (2); need for additional plants (1); power plant approvals (3); inflation (1); recession (2); government activity changes (12); government company regulations (1); company effects (1); programs affecting economy (9); nuclear plant distance (2); nuclear plant dangers (1); magazine readership (1); television viewing habits (2); college attended (2); class year (1); major (1); degree (1); preferred career (2); important career aspects (9); academic standing (1).
Dynamics at barriers in bidirectional two-lane exclusion processes
Creators: name: Juhász, Róbert
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Physical sciences

description: A two-lane exclusion process is studied where particles move in the two lanes in opposite directions and are able to change lanes. The focus is on the steady state behavior in situations where a positive current is constrained to an extended subsystem (either by appropriate boundary conditions or by the embedding environment) where, in the absence of the constraint, the current would be negative. We have found two qualitatively different types of steady states and formulated the conditions of them in terms of the transition rates. In the first type of steady state, a localized cluster of particles forms with an anti-shock located in the subsystem and the current vanishes exponentially with the extension of the subsystem. This behavior is analogous to that of the one-lane partially asymmetric simple exclusion process, and can be realized e.g. when the local drive is induced by making the jump rates in two lanes unequal. In the second type of steady state, which is realized e.g. if the local drive is induced purely by the bias in the lane change rates, and which has thus no counterpart in the one-lane model, a delocalized cluster of particles forms which performs a diffusive motion as a whole and, as a consequence, the current vanishes inversely proportionally to the extension of the subsystem. The model is also studied in the presence of quenched disordered, where, in case of delocalization, phenomenological considerations predict anomalously slow, logarithmic decay of the current with the system size in contrast with the usual power-law.
description: 24 pages, 13 figures
title: Canadian job postings in digital sectors during COVID-19
Creators: name: Bellatin, Alejandra
name: Galassi, Gabriela
Publisher: name: Bank of Canada
Year: 2021

description: Digital technologies have helped maintain economic activity while allowing people to remain physically distant throughout the COVID-19 crisis. This note shows that the number of online postings for jobs related to the production of digital technologies in Canada decreased less than the number for other jobs and recovered more quickly after lockdowns were lifted.
description: Depuis le début de la pandémie de COVID-19, les technologies numériques contribuent au maintien de l’activité économique tout en facilitant la distanciation. Notre analyse montre que le nombre d’offres d’emploi publiées en ligne pour des postes liés à la production de technologies numériques au Canada a diminué moins que celui des autres offres d’emploi, et qu’il a récupéré plus rapidement après la levée des confinements.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÐµÑÑ ÑÑÐ»ÑÐ³ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Event-Ð°Ð³ÐµÐ½ÑÑÑÐ²Ð°)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°Ð±Ð¸Ð´ÑÐ»Ð»Ð¸Ð½Ð°, ÐÐ»ÐµÐ½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ ÑÑÐµÑÑ ÑÑÐ»ÑÐ³
Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ
Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¸
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ

description: Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ° ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾Ð³Ð¾ Event-Ð°Ð³ÐµÐ½ÑÑÑÐ²Ð°. ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Event-Ð°Ð³ÐµÐ½ÑÑÑÐ²Ð¾ Â«ÐÑÐµÐ»ÑÐµ Ð¼Ð¾Ð´Ð½ÑÑ ÑÐ¾ÑÐ¶ÐµÑÑÐ²Â». Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÑÑÐµÑÑ ÑÑÐ»ÑÐ³. ÐÐ°Ð½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð´Ð»Ñ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ñ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¸ ÑÐµÐ»ÐµÑÐ¾Ð¾Ð±ÑÐ°Ð·Ð½Ð¾ÑÑÐ¸ ÐµÐ³Ð¾ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸ÑÐºÐ¾Ð² Ð¿Ð¾ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¼Ñ Ð¿ÑÐ¾ÐµÐºÑÑ.
Sulphur abundances in halo stars from Multiplet 3 at 1045 nm
Creators: name: Caffau, Elisabetta
name: Sbordone, Luca
name: Ludwig, Hans-Günter
name: Bonifacio, Piercarlo
name: Spite, Monique
Publisher: name: arXiv
Year: 2010
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Sulphur is a volatile alpha-element which is not locked into dust grains in the interstellar medium (ISM). Hence, its abundance does not need to be corrected for dust depletion when comparing the ISM to the stellar atmospheres. The abundance of sulphur in the photosphere of metal-poor stars is a matter of debate: according to some authors, [S/Fe] versus [Fe/H] forms a plateau at low metallicity, while, according to other studies, there is a large scatter or perhaps a bimodal distribution. In metal-poor stars sulphur is detectable by its lines of Mult.1 at 920 nm, but this range is heavily contaminated by telluric absorptions, and one line of the multiplet is blended by the hydrogen Paschen zeta line. We study the possibility of using Mult. 3 (at 1045 nm) for deriving the sulphur abundance because this range, now observable at the VLT with the infra-red spectrograph CRIRES, is little contaminated by telluric absorption and not affected by blends at least in metal-poor stars. We compare the abundances derived from Multiplets 1 and 3, taking into account NLTE corrections and 3D effects. Here we present the results for a sample of four stars, although the scatter is less pronounced than in previous analysis, we cannot find a plateau in [S/Fe], and confirm the scatter of the sulphur abundance at low metallicity.
description: to be published in Astronomische Nachrichten
title: Method for assessing the conditions for the construction of a high-rise building on a pile foundation in a seismically hazardous area
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Kafidov, Gennady
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¡ÐµÐ¹ÑÐ¼Ð¾ÑÑÐ¾Ð¹ÐºÐ¾Ðµ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾
ÐÐ´Ð°Ð½Ð¸Ñ Ð¼Ð½Ð¾Ð³Ð¾ÑÑÐ°Ð¶Ð½ÑÐµ
Ð¤ÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÑ ÑÐ²Ð°Ð¹Ð½ÑÐµ
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description: Master's thesis is devoted to the development of methods for assessing the conditions for the construction of high-rise buildings on pile foundations in seismically hazardous areas. The paper presents an analysis of how shifts have changed with changes in power or other soil, and efforts in piles. The application of the method of approximation of the results to find the linear dependence, on the basis of which it would be possible to put forward recommendations for the construction of similar objects. These calculations were carried out in the SCAD software package. As a result, a relationship has been obtained between the movement of the building, effort in sleeping buildings and possessions or other soil. The developed method for assessing the results of construction and use of projects with related projects.
description: ÐÐ°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð¼ÐµÑÐ¾Ð´Ð° Ð¾ÑÐµÐ½ÐºÐ¸ ÑÑÐ»Ð¾Ð²Ð¸Ð¹ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð²ÑÑÐ¾ÑÐ½ÑÑ Ð·Ð´Ð°Ð½Ð¸Ð¹ Ð½Ð° ÑÐ²Ð°Ð¹Ð½ÑÑ ÑÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÐ°Ñ Ð² ÑÐµÐ¹ÑÐ¼Ð¾Ð¾Ð¿Ð°ÑÐ½ÑÑ ÑÐ°Ð¹Ð¾Ð½Ð°Ñ. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾Ð³Ð¾ ÐºÐ°Ðº Ð¼ÐµÐ½ÑÐ»Ð¸ÑÑ Ð¿ÐµÑÐµÐ¼ÐµÑÐµÐ½Ð¸Ñ Ñ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸ÐµÐ¼ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸ ÑÐ»Ð¾Ñ ÑÐ¾Ð³Ð¾ Ð¸Ð»Ð¸ Ð¸Ð½Ð¾Ð³Ð¾ Ð³ÑÑÐ½ÑÐ°, ÑÑÐ¸Ð»Ð¸Ñ Ð² ÑÐ²Ð°ÑÑ. ÐÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð° Ð°Ð¿Ð¿ÑÐ¾ÐºÑÐ¸Ð¼Ð°ÑÐ¸Ð¸ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð´Ð»Ñ Ð½Ð°ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ Ð»Ð¸Ð½ÐµÐ¹Ð½Ð¾Ð¹ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸, Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÐºÐ¾ÑÐ¾ÑÐ¾Ð¹, Ð¼Ð¾Ð¶Ð½Ð¾ Ð±ÑÐ»Ð¾ Ð±Ñ Ð²ÑÐ´Ð²Ð¸Ð½ÑÑÑ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ñ Ð¿Ð¾Ð´Ð¾Ð±Ð½ÑÑ Ð¾Ð±ÑÐµÐºÑÐ¾Ð². ÐÐ°Ð½Ð½ÑÐµ ÑÐ°ÑÑÐµÑÑ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸Ð»Ð¸ÑÑ Ð² Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð¼ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐµ SCAD. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð° Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÑ Ð¼ÐµÐ¶Ð´Ñ Ð¿ÐµÑÐµÐ¼ÐµÑÐµÐ½Ð¸ÑÐ¼Ð¸ Ð·Ð´Ð°Ð½Ð¸Ñ, ÑÑÐ¸Ð»Ð¸Ñ Ð² ÑÐ²Ð°ÑÑ Ð·Ð´Ð°Ð½Ð¸Ñ Ð¸ Ð¼Ð¾ÑÐ½Ð¾ÑÑÑÑ ÑÐ»Ð¾Ñ ÑÐ¾Ð³Ð¾ Ð¸Ð»Ð¸ Ð¸Ð½Ð¾Ð³Ð¾ Ð³ÑÑÐ½ÑÐ°. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½ÑÐ¼ Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÑÐ»Ð¾Ð²Ð¸Ð¹ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð¸ Ð´Ð°Ð½Ð½ÑÐ¼Ð¸ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸ÑÐ¼Ð¸ ÑÐ¼Ð¾Ð³ÑÑ Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÑÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ½ÑÐµ Ð¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¸ ÑÐ°ÑÑÐµÑÐµ Ð¿Ð¾Ð´Ð¾Ð±Ð½ÑÑ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÑ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¹ Ð¿Ð¾ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ ÐºÐ²ÐµÑÑ-ÑÐ°Ð·Ð²Ð»ÐµÑÐµÐ½Ð¸Ð¹
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÐ´ÑÐ»Ñ, ÐÐ»ÐµÐ½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐµ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÐµ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸
ÐºÐ²ÐµÑÑ-ÑÐ°Ð·Ð²Ð»ÐµÑÐµÐ½Ð¸Ñ
ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ñ
integrated marketing communications
quest entertainment
campaign

description: ÐÐ±ÑÑÐ¼ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ - 73 ÑÑÑÐ°Ð½Ð¸ÑÑ, Ð½Ð° ÐºÐ¾ÑÐ¾ÑÑÑ ÑÐ°Ð·Ð¼ÐµÑÐµÐ½Ñ 27 ÑÐ¸ÑÑÐ½ÐºÐ¾Ð² Ð¸ 8 ÑÐ°Ð±Ð»Ð¸Ñ. ÐÑÐ¸ Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ð¸Ð¸ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð° Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð»Ð¾ÑÑ 30 Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð². ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¸ Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ð¸Ð¸ ÑÐ°Ð±Ð¾ÑÑ Ð¿Ð¾ÑÐ»ÑÐ¶Ð¸Ð»Ð° ÐºÐ²ÐµÑÑ-ÐºÐ¾Ð¼Ð½Ð°ÑÐ° Â«ÐÐ»Ð»ÑÐ·Ð¸ÑÂ». ÐÑÐµÐ´Ð¼ÐµÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÑ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¹. Ð¦ÐµÐ»ÑÑ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐ¸ÑÑÐµÐ¼Ñ Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÑ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¹ ÐºÐ²ÐµÑÑ ÐºÐ¾Ð¼Ð½Ð°ÑÑ Â«ÐÐ»Ð»ÑÐ·Ð¸ÑÂ» Ð´Ð»Ñ Ð±Ð¾Ð»ÐµÐµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ ÑÑÐ»ÑÐ³Ð¸.
description: The volume of the thesis 73 pages containing 27 figures and 8 tables. When writing diploma was used 30 sources. The object of the study when writing work was the quest room "Allusion". The subject of research is the strategic planning of integrated marketing communications. The aim of the study is to develop a system of integrated marketing communications quest room "Allusion" for more effective promotion of services.
Cosmic age, Statefinder and $Om$ diagnostics in the decaying vacuum cosmology
Creators: name: Tong, Ming-Lei
name: Zhang, Yang
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: As an extension of $Λ$CDM, the decaying vacuum model (DV) describes the dark energy as a varying vacuum whose energy density decays linearly with the Hubble parameter in the late-times, $ρ_Λ(t) \propto H(t)$, and produces the matter component. We examine the high-$z$ cosmic age problem in the DV model, and compare it with $Λ$CDM and the Yang-Mills condensate (YMC) dark energy model. Without employing a dynamical scalar field for dark energy, these three models share a similar behavior of late-time evolution. It is found that the DV model, like YMC, can accommodate the high-$z$ quasar APM 08279+5255, thus greatly alleviates the high-$z$ cosmic age problem. We also calculate the Statefinder $(r,s)$ and the {\it Om} diagnostics in the model. It is found that the evolutionary trajectories of $r(z)$ and $s(z)$ in the DV model are similar to those in the kinessence model, but are distinguished from those in $Λ$CDM and YMC. The ${\it Om}(z)$ in DV has a negative slope and its height depends on the matter fraction, while YMC has a rather flat ${\it Om}(z)$, whose magnitude depends sensitively on the coupling.
description: 12 pages, 4 figures, with some corrections
title: ÐÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐ¾ÑÐ¾ÑÐ¸Ð¿Ð° Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð¼Ð¾Ð½Ð¸ÑÐ¾ÑÐ¸Ð½Ð³Ð° ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¿Ð¾Ð¸ÑÐºÐ¾Ð²Ð¾Ð¹ Ð²ÑÐ´Ð°ÑÐ¸ Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð½ÐµÐºÐ¾ÑÐ¾ÑÑÑ Ð¿ÑÐ¸ÐµÐ¼Ð¾Ð² seo-Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð½Ð° Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ ÑÐ°Ð¹ÑÐ° Ð² Ð¿Ð¾Ð¸ÑÐºÐ¾Ð²ÑÑ ÑÐ¸ÑÑÐµÐ¼Ð°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Ð¾ÑÑÑÐ½, ÐÐ¸ÑÐ¸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: 2017
Subjects: ÐÐ½ÑÐµÑÐ½ÐµÑ
ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¿Ð¾Ð¸ÑÐºÐ¾Ð²ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ
Ð¿Ð¾Ð¸ÑÐºÐ¾Ð²ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ
ÑÐ°ÐºÑÐ¾ÑÑ ÑÐ°Ð½Ð¶Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ
Ð¿Ð¾Ð¸ÑÐºÐ¾Ð²Ð°Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ seo-Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ðµ ÑÐ°Ð¹ÑÐ° Ð² Ð¿Ð¾Ð¸ÑÐºÐ¾Ð²ÑÑ ÑÐ¸ÑÑÐµÐ¼Ð°Ñ. Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÑ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð½ÐµÐºÐ¾ÑÐ¾ÑÑÑ Ð¿ÑÐ¸ÐµÐ¼Ð¾Ð² seo-Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð½Ð° Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ ÑÐ°Ð¹ÑÐ° Ð² Ð¿Ð¾Ð¸ÑÐºÐ¾Ð²ÑÑ ÑÐ¸ÑÑÐµÐ¼Ð°Ñ, Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¿Ð¾Ð¸ÑÐºÐ¾Ð²Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¯Ð½Ð´ÐµÐºÑ. Ð Ð¿ÑÐ¾ÑÐµÑÑÐµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð¾ Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ð¾ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ ÐºÐ¾ÑÐ¾ÑÐ¾Ð³Ð¾ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸Ð»Ð¾ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð²Ð°Ð¶Ð½Ð¾ÑÑÐ¸ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² ÑÐ°Ð½Ð¶Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÑÑÐ°Ð½Ð¸Ñ Ð¿Ð¾Ð¸ÑÐºÐ¾Ð²Ð¾Ð¹ Ð²ÑÐ´Ð°ÑÐ¸. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð±ÑÐ» ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½ ÑÐ¿Ð¸ÑÐ¾Ðº Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² ÑÐ°Ð½Ð¶Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¾ ÑÑÐµÐ¿ÐµÐ½ÑÑ Ð¸Ñ Ð²Ð°Ð¶Ð½Ð¾ÑÑÐ¸ Ð´Ð»Ñ Ð¿Ð¾Ð¸ÑÐºÐ¾Ð²Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¯Ð½Ð´ÐµÐºÑ.
title: ÐÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÐÐ¸ÑÐ°Ð¹ÑÐºÐ¾Ð¹ Ð ÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐ¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ»Ð»Ð°Ð±ÐµÑÐ´ÑÐµÐ²Ð° , ÐÐ¶ÐµÐ½Ð½ÐµÑ
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Ð¸ÑÐ°Ð¹ÑÐºÐ°Ñ Ð ÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐ°
ÑÐµÐ²Ð¾Ð»ÑÑÐ¸Ñ
ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½Ð¾Ðµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ
Ð¢Ð°Ð¹Ð²Ð°Ð½Ñ
Ð´ÐµÐ¼Ð¾ÐºÑÐ°ÑÐ¸Ñ
ÐÐ¾Ð¼Ð¸Ð½ÑÐ´Ð°Ð½
Ð´ÐµÐºÐ»Ð°ÑÐ°ÑÐ¸Ñ
Ð²ÑÐ±Ð¾ÑÑ
Republic of China
revolution
state of emergency
Taiwan
democracy
Kuomintang
declaration
elections

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ðµ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÐÐ¸ÑÐ°Ð¹ÑÐºÐ¾Ð¹ Ð ÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐ¸. Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ ÐÐ¸ÑÐ°Ð¹ÑÐºÐ¾Ð¹ Ð ÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐ¸, ÐµÐµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½Ð° Ð¢Ð°Ð¹Ð²Ð°Ð½Ðµ, Ð¸ÑÑÐ¾ÑÐ¸ÑÐµÑÐºÐ¾Ðµ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ. ÐÐ·ÑÑÐµÐ½Ð° Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° Ð½Ð° Ð¢Ð°Ð¹Ð²Ð°Ð½Ðµ Ð¿ÑÐ¸ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¾Ð¼ ÑÐµÐ¶Ð¸Ð¼Ðµ Ð¿ÑÐ¸ Ð§Ð°Ð½ ÐÐ°Ð¹ÑÐ¸, Ð° ÑÐ°ÐºÐ¶Ðµ ÐµÐµ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð²Ð¾ Ð²ÑÐ¾ÑÐ¾Ð¹ Ð¿Ð¾Ð»Ð¾Ð²Ð¸Ð½Ðµ 20 Ð²ÐµÐºÐ°. Ð¢Ð°ÐºÐ¶Ðµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ Ð¸ÑÑÐ¾ÑÐ¸Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð´ÐµÐ¼Ð¾ÐºÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð½Ð° Ð¾ÑÑÑÐ¾Ð²Ðµ, Ð½Ð°ÑÐ°Ð»ÑÐ½ÑÐµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Ð§ÑÐ½Ñ Ð¨ÑÐ¹Ð±ÑÐ½Ñ, Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð½ÑÐµ Ð±Ð¾ÑÑÐ±Ðµ Ð·Ð° Ð´ÐµÐ¼Ð¾ÐºÑÐ°ÑÐ¸Ñ. ÐÐ°Ð·Ð²Ð°Ð½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐ°Ð¹Ð²Ð°Ð½ÑÑÐºÐ¾Ð¹ Ð´ÐµÐ¼Ð¾ÐºÑÐ°ÑÐ¸Ð¸, ÐµÐµ ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ°. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½ Ð¼ÐµÑÐ¾Ð´ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Â«ÑÐ°Ð¹Ð²Ð°Ð½ÑÑÐºÐ°Ñ Ð´ÐµÐ¼Ð¾ÐºÑÐ°ÑÐ¸ÑÂ».
description: This work dedicated to the problem of political development of Republic of China. In this work discussed formation of Republic of China, formation of Republic of China in Taiwan, historical development. Also studied political system in Taiwan with the political mode under Chiang Kai-Shek, and it's changes in the second half of the 20th century. Also, the history creation of the democratic movement on the island, the initial programs of Chen Shui-bian, dedicated to the struggle for democracy. Named features of Taiwan's democracy, it's specificity. Analyzed possibility of using the model of "Taiwan's democracy".
Constraining the baryon loading factor of AGN jets: implication from the gamma-ray emission of the Coma cluster
Creators: name: Shi, Xin-Yue
name: Zhang, Yi
name: Liu, Ruo-Yu
name: Wang, Xiang-Yu
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: High-energy cosmic rays (CRs) can be accelerated in the relativistic jets of Active Galactic Nuclei (AGNs) powered by supermassive black holes. The baryon loading efficiency onto relativistic CR baryons from the accreting black holes is poorly constrained by observations so far. In this paper, we suggest that the $γ$-ray emission of galaxy clusters can be used to study the baryon loading factor of AGN jets, since CRs injected by AGN jets are completely confined in the galaxy clusters and sufficiently interact with intra-cluster medium via hadronic process, producing diffuse $γ$-rays. We study the propagation of CRs in the galaxy clusters and calculate the radial distribution of the gamma-rays in the galaxy cluster with different injection rates from AGNs. By comparison with the $γ$-ray flux and upper limits of the Coma cluster measured by $Fermi$-LAT and VERITAS, we find the upper limit of the average baryon loading factor {(defined as the efficiency with which the gravitational energy is converted into relativistic particles)} to be $η_{p, \mathrm{grav}} < 0.1$. The upper limit is much lower than that required to account for diffuse neutrino flux in the conventional blazar models.
description: 12 pages, 9 figures. Accepted for Publication in ApJ
title: Ð­Ð»ÐµÐºÑÑÐ¾Ð³Ð¸Ð´ÑÐ¾Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ½Ð°Ñ Ð²ÑÑÑÐ¶ÐºÐ°âÑÐ¾ÑÐ¼Ð¾Ð²ÐºÐ° ÑÐ¾Ð½ÐºÐ¾Ð»Ð¸ÑÑÐ¾Ð²ÑÑ Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð² Ð² Ð·Ð°ÐºÑÑÑÑÑ Ð¼Ð°ÑÑÐ¸ÑÑ
title: Ð½Ð°ÑÑÐ½ÑÐ¹ Ð´Ð¾ÐºÐ»Ð°Ð´
titleType: Subtitle
Creators: name: ÐÑÑÐµÐ½ÑÑÐµÐ²Ð°, ÐÑÐµÐ½Ð¸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: 2018
Subjects: ÐÑÑÑÐ¶ÐºÐ° Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð²
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Collisional debris as laboratories to study star formation
Creators: name: Boquien, M.
name: Duc, P. -A.
name: Wu, Y.
name: Charmandaris, V.
name: Lisenfeld, U.
name: Braine, J.
name: Brinks, E.
name: Iglesias-Páramo, J.
name: Xu, C. K.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: In this paper we address the question whether star formation is driven by local processes or the large scale environment. To do so, we investigate star formation in collisional debris where the gravitational potential well and velocity gradients are shallower and compare our results with previous work on star formation in non-interacting spiral and dwarf galaxies. We have performed multiwavelength spectroscopic and imaging observations (from the far-ultraviolet to the mid-infrared) of 6 interacting systems, identifying a total of 60 star-forming regions in their collision debris. Our analysis indicates that in these regions a) the emission of the dust is at the expected level for their luminosity and metallicity, b) the usual tracers of star formation rate display the typical trend and scatter found in classical star forming regions, and c) the extinction and metallicity are not the main parameters governing the scatter in the properties of intergalactic star forming regions; age effects and variations in the number of stellar populations, seem to play an important role. Our work suggests that local properties such as column density and dust content, rather than the large scale environment seem to drive star formation. This means that intergalactic star forming regions can be used as a reliable tool to study star formation.
description: 18 pages, 19 figures, accepted for publication in The astronomical journal