cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Oceani ovunque, persino su Plutone
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2016

I dati di New Horizon aprono le porte a una possibilità che rasenta l’incredibile: non solo Plutone potrebbe aver ospitato un oceano sotterraneo, ma questo potrebbe essere ancora lì, con acqua almeno parzialmente allo stato liquido. Intanto, un altro studio mostra che l’oceano sotterraneo di Encelado è meno in profondità del previsto: appena 5 km sotto la superficie della luna di Saturno
Deep Learning Models for Predicting IPL Cricket Scores
Creators: name: S. Rahul, Mr.
name: M. Sowndharya, Mrs.
Publisher: name: Zenodo
Year: 2025

description: Cricket score prediction remains a challenging task due to the sport’s dynamic and multifaceted nature. This study explores a deep learning-based approach utilizing linear regression to predict Indian Premier League (IPL) match scores. The model is trained on historical ball-by-ball data from 2008 to 2017, incorporating key match factors such as team performance, past statistical trends, and game conditions. A web-based application is developed to provide an interactive platform where users can register, log in, and access predictive analytics. By leveraging deep learning techniques, this research enhances the accuracy of score predictions, offering valuable insights for cricket analysts and enthusiasts. The study details the methodology, including data preprocessing, feature selection, model training, and evaluation. The integration of a web-based interface facilitates user interaction with predictive models, bridging the gap between raw cricket data and actionable insights. This research contributes to the growing field of sports analytics, demonstrating the potential of deep learning in predictive modeling and decision-making in professional cricket. Future work aims to refine model performance by incorporating additional match parameters and real-time data streams for improved predictive accuracy.
La magnetar con la nebulosa intorno
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

Un team internazionale di ricercatori, sfruttando i telescopi spaziali XMM-Newton e Swift che operano nel campo della luce ad alta energia, ha scoperto una magnetar circondata da una nebulosa. Se nel caso delle pulsar classiche questo è abbastanza comune, per le magneter è la prima volta che succede, e questa scoperta potrebbe aiutarci a comprendere come funzionino queste stelle con i campi magnetici più intensi in assoluto
title: ÐÑÑÐ¾ÑÐ¸Ñ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð½Ð°ÑÐºÐ¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¨Ð¸Ð¿ÑÐ½Ð¾Ð²Ð°, ÐÐ»ÑÐ³Ð°
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: Ð½Ð°ÑÐºÐ°
Ð¸ÑÑÐ¾ÑÐ¸Ñ Ð¿Ð¾Ð·Ð½Ð°Ð½Ð¸Ñ
Ð¼ÐµÑÐ¾Ð´Ð¾Ð»Ð¾Ð³Ð¸Ñ
ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¸Ðµ
ÑÐ¸Ð·Ð¸ÐºÐ¾-Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð½Ð°ÑÐºÐ¸
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: ÐÐ°ÑÐµÑÐ¸Ð°Ð» Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ ÑÑÐµÐ±Ð½Ð¾Ð³Ð¾ Ð¿Ð»Ð°Ð½Ð° Ð¿Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ðµ Ð¼Ð°Ð³Ð¸ÑÑÑÐ°ÑÑÑÑ Â«ÐÑÑÐ¾ÑÐ¸Ñ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð½Ð°ÑÐºÐ¸Â». Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÑÐ°Ð¿Ñ Ð¸ÑÑÐ¾ÑÐ¸Ð¸ Ð½Ð°ÑÐºÐ¸, ÑÐ²Ð¾Ð»ÑÑÐ¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð½Ð°ÑÑÐ½Ð¾Ð³Ð¾ Ð¿Ð¾Ð·Ð½Ð°Ð½Ð¸Ñ, Ð´Ð°ÐµÑÑÑ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¾ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ Ð¼ÐµÐ¶Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ð°ÑÐ½Ð¾Ð¹ Ð¼ÐµÑÐ¾Ð´Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð½Ð°ÑÐºÐ¸, Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ð°Ñ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð°ÑÐ³ÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ð¸, ÐºÑÐ»ÑÑÑÑÐµ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¼ÑÑÐ»ÐµÐ½Ð¸Ñ. ÐÐ°ÐµÑÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÑÑÐ²Ð°. ÐÐ¾Ð´ÑÐµÑÐºÐ¸Ð²Ð°ÐµÑÑÑ ÑÐ²ÑÐ·Ñ Ð½Ð°ÑÑÐ½Ð¾Ð¹ ÐºÐ°ÑÑÐ¸Ð½Ñ Ð¼Ð¸ÑÐ° Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð½Ð°ÑÐºÐ¸ Ð² ÐµÐµ Ð¸ÑÑÐ¾ÑÐ¸Ð¸. ÐÐ·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ñ Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¾Ð¹, ÑÐ»ÐµÐºÑÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹, ÐºÐ²Ð°Ð½ÑÐ¾Ð²Ð¾-Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¾Ð¹, ÐºÐ²Ð°Ð½ÑÐ¾Ð²Ð¾-Ð¿Ð¾Ð»ÐµÐ²Ð¾Ð¹ ÐºÐ°ÑÑÐ¸Ð½Ñ Ð¼Ð¸ÑÐ°, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ ÑÐ¸Ð½ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ°ÑÑÐ¸Ð½Ñ Ð¼Ð¸ÑÐ°, ÐºÐ¾ÑÐ¾ÑÐ°Ñ ÑÐ¾ÑÐ¼Ð¸ÑÑÐµÑÑÑ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ð¸ Ð³Ð»Ð¾Ð±Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ²Ð¾Ð»ÑÑÐ¸Ð¾Ð½Ð¸Ð·Ð¼Ð° Ð¸ Ð¼ÐµÐ¶Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ð°ÑÐ½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ð½Ð¾Ð¹ Ð¼ÐµÑÐ¾Ð´Ð¾Ð»Ð¾Ð³Ð¸Ð¸. ÐÐ°ÑÐµÑÐ¸Ð°Ð» ÑÑÐµÐ±Ð½Ð¸ÐºÐ° Ð¾Ð¿Ð¸ÑÐ°ÐµÑÑÑ Ð½Ð° ÑÐ¿ÑÐ°Ð²Ð¾ÑÐ½ÑÐµ Ð¸ ÑÑÐµÑÑÐ¾Ð¼Ð°ÑÐ¸Ð¹Ð½ÑÐµ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¸, ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ ÑÐ¸Ð·Ð¸ÐºÐ¸, ÑÐ¸Ð¼Ð¸Ð¸, Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¿Ð¾Ð»ÐµÐ·ÐµÐ½ Ð´Ð»Ñ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¸Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ Ð¿Ð¾ ÐµÑÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð½Ð°ÑÑÐ½ÑÐ¼ Ð¸ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¼ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸.
ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ²Ð»ÑÐµÑÑÑ 2-Ð¼ Ð¸Ð·Ð´Ð°Ð½Ð¸ÐµÐ¼ Ð¿ÑÐµÐ´ÑÐ´ÑÑÐµÐ³Ð¾: Ð¨Ð¸Ð¿ÑÐ½Ð¾Ð²Ð° Ð. Ð. ÐÑÑÐ¾ÑÐ¸Ñ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð½Ð°ÑÐºÐ¸: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ. Ð¡ÐÐ±.: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°. 2016.. â 256 Ñ. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÐÐ½ÑÑÐ¸ÑÑÑÐ° ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ¸ Ð¸ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÑ ÑÐ¸ÑÑÐµÐ¼.
Da Salerno a Stanford inseguendo i GRB
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2016

Una correlazione “3D”, fra tre dei parametri che caratterizzano i lampi di raggi gamma, ha consentito a un team di astrofisici d’individuare un campione di sorgenti candidate a svolgere il ruolo di “candele standard”. Media INAF ha raggiunto la prima autrice dello studio
Overview of Neutrino Mixing Models and Their Mixing Angle Predictions
Creators: name: Albright, Carl H.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: An overview of neutrino-mixing models is presented with emphasis on the types of horizontal flavor and vertical family symmetries that have been invoked. Distributions for the mixing angles of many models are displayed. Ways to differentiate among the models and to narrow the list of viable models are discussed.
description: 5 pages, 6 figures, written version of talk presented at the 11th International Workshop on Neutrino Factories, Superbeams and Beta Beams, Illinois Institute of Technology, Chicago, July 20-25, 2009; abbreviated version of arXiv:0905.0146 which appeared in Proceedings of the 13th International Workshop on Neutrino Telescopes, Venice, March 10-13, 2009
title: ÐÐ¾ÑÑÐ¸Ð½Ð¸ÑÐ½ÑÐ¹ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ Ð½Ð° 200 ÑÐµÐ»Ð¾Ð²ÐµÐº Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ Ð¿Ð¾Ð´Ð·ÐµÐ¼Ð½Ð¾Ð¹ Ð¿Ð°ÑÐºÐ¾Ð²ÐºÐ¾Ð¹
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ°
titleType: Subtitle
Creators: name: Ð¡ÑÐ°ÑÐ¸ÑÑÐ½Ð°, 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Ð½ÐµÑÐ³Ð¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ
ÑÐ½ÐµÑÐ³Ð¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ðµ Ð¾ÑÑÐµÐºÐ»ÐµÐ½Ð¸Ðµ
Ð¿Ð¾Ð´Ð·ÐµÐ¼Ð½ÑÐ¹ Ð¿Ð°ÑÐºÐ¸Ð½Ð³

description: ÐÐ±ÑÐµÐºÑ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° â Ð³Ð¾ÑÑÐ¸Ð½Ð¸ÑÐ½ÑÐ¹ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ 8 ÑÑÐ°Ð¶ÐµÐ¹ Ñ Ð¿ÐµÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ ÑÑÐ°Ð¶Ð½Ð¾ÑÑÑÑ Ð¸ Ð¼Ð½Ð¾Ð³Ð¾ÑÑÐ¾Ð²Ð½ÐµÐ²Ð¾Ð¹ Ð¿Ð¾Ð´Ð·ÐµÐ¼Ð½Ð¾Ð¹ ÑÑÐ¾ÑÐ½ÐºÐ¾Ð¹ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÐ¸Ð¿Ð° TRANSLO PARKING.
Ð ÑÐ¾ÑÑÐ°Ð² Ð³Ð¾ÑÑÐ¸Ð½Ð¸ÑÑ Ð²ÑÐ¾Ð´ÑÑ Ð½Ð¾Ð¼ÐµÑÐ° Ð¿ÐµÑÐ²Ð¾Ð¹ ÐºÐ°ÑÐµÐ³Ð¾ÑÐ¸Ð¸, Ð½Ð¾Ð¼ÐµÑÐ°-Ð»ÑÐºÑÑ, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐµÑÑÐ¾ÑÐ°Ð½, ÐºÐ°ÑÐµ, ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾-Ð¾Ð·Ð´Ð¾ÑÐ¾Ð²Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ Ð·Ð¾Ð½Ð°, Ð´ÐµÑÑÐºÐ¸Ðµ Ð¸Ð³ÑÐ¾Ð²ÑÐµ. ÐÐ°Ð´Ð°Ð½Ð½Ð¾Ðµ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð¾ Ð¼ÐµÑÑ Ð² Ð³Ð¾ÑÑÐ¸Ð½Ð¸ÑÐµ â 200 ÑÐµÐ». ÐÐ¾ÑÑÐ¸Ð½Ð¸ÑÐ½ÑÐ¹ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ ÑÐ°ÑÐ¿Ð¾Ð»Ð°Ð³Ð°ÐµÑÑÑ Ð¿Ð¾ Ð°Ð´ÑÐµÑÑ: Ð³. Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³, ÐÑÐ¸Ð¼Ð¾ÑÑÐºÐ¸Ð¹ ÑÐ°Ð¹Ð¾Ð½, ÐÑÐ¸Ð¼Ð¾ÑÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐ¿ÐµÐºÑ, ÑÑ. 1. ÐÑÐ¾ÐµÐºÑÐ¾Ð¼ Ð¿ÑÐµÐ´ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¾ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ðµ Ð·Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ Ñ ÑÐ°Ð·Ð¼ÐµÑÐµÐ½Ð¸ÐµÐ¼ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð¾Ð¹ ÑÑÐ¾ÑÐ½ÐºÐ¸, ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð·Ð¾Ð½Ñ, Ð·Ð¾Ð½Ñ Ð¾ÑÐ´ÑÑÐ° Ð²Ð·ÑÐ¾ÑÐ»ÑÑ Ð¸ Ð´ÐµÑÐµÐ¹, Ð·Ð¾Ð½Ñ ÑÐ¿Ð¾ÑÑÐ°, Ð¿ÑÐ¸Ð±ÑÐµÐ¶Ð½Ð¾Ð¹ Ð·Ð¾Ð½Ñ Ð¸ Ð·Ð¾Ð½Ñ Ð¾Ð·ÐµÐ»ÐµÐ½ÐµÐ½Ð¸Ñ.
Mayapan Agrarian (Rural) Life Project Informe 2015 Season
Creators: name: Masson, Marilyn
Year: 2018
Subjects: subject: Yucatan (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/762/yucatan-state-territory
subject: Mesoamerican Postclassic period
valueUri: https://core.tdar.org/browse/temporal-keyword/5618/mesoamerican-postclassic-period
subject: Postclassic Maya
valueUri: https://core.tdar.org/browse/culture-keyword/8273/postclassic-maya
subject: CLASSIC LOWLAND MAYA
valueUri: https://core.tdar.org/browse/culture-keyword/6850/classic-lowland-maya
subject: Mayapan
valueUri: https://core.tdar.org/browse/site-name/94380/mayapan
subject: Domestic Structures
valueUri: https://core.tdar.org/browse/site-type/256/domestic-structures
subject: Rural
valueUri: https://core.tdar.org/browse/site-type/2134/rural
subject: Domestic Structure or Architectural Complex
valueUri: https://core.tdar.org/browse/site-type/251/domestic-structure-or-architectural-complex
subject: Ceramic
valueUri: https://core.tdar.org/browse/material-type/1/ceramic
subject: Chipped Stone
valueUri: https://core.tdar.org/browse/material-type/2/chipped-stone
subject: Ground Stone
valueUri: https://core.tdar.org/browse/material-type/7/ground-stone
subject: Building Materials
valueUri: https://core.tdar.org/browse/material-type/8/building-materials
subject: Household Archaeology
valueUri: https://core.tdar.org/browse/other-keyword/134855/household-archaeology
subject: Archaeological Overview
valueUri: https://core.tdar.org/browse/investigation-type/1/archaeological-overview
subject: Remote Sensing
valueUri: https://core.tdar.org/browse/investigation-type/22/remote-sensing

description: Report to INAH of 2015 seasons that investigated rural houses of the Terminal Classic and Postclassic period in the Mayapan area (outside of the city walls). A follow-up project to the 2013 LiDAR season (in Spanish).
Winding number expansion for the canonical approach to finite density simulations
Creators: name: Meng, Xiangfei
name: Li, Anyi
name: Alexandru, Andrei
name: Liu, Keh-Fei
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: The canonical partition function approach was designed to avoid the overlap problem that affects the lattice simulations of nuclear matter at high density. The method employs the projections of the quark determinant on a fix quark number sector. When the quark number is large, the evaluation of the projected determinant becomes numerically unstable. In this paper a different evaluation method based on expanding the determinant in terms of loops winding around the lattice is studied. We show that this method is stable and significantly faster than our original algorithm. This greatly expands the range of quark numbers that we can simulate effectively.
description: 8 pages, 5 figures, LATTICE 2008, parallel talk
Radio Emission from Supernova Remnants: Implications for Post-Shock Magnetic Field Amplification and the Magnetic Fields of Galaxies
Creators: name: Thompson, Todd A.
name: Quataert, Eliot
name: Murray, Norman
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Using observations from the literature, we show that the non-thermal radio luminosity (L) of supernova remnants (SNRs) is a strong function of the average gas surface density (Sigma) of the galaxy in which the remnants reside, from normal spirals to luminous starbursts. We combine a simple theory for electron cooling in SNRs with the observed radio luminosities to estimate the remnant magnetic field strength (B_SNR): the correlation between L and Sigma implies that B_SNR also increases with Sigma. We explore two interpretations of this correlation: (1) B_SNR is generated by post-shock magnetic field amplification, with B_SNR^2 proportional to Sigma and (2) B_SNR results from shock-compression of the ambient ISM magnetic field (B_ISM), with B_ISM being larger in denser galaxies. We find that shock compression is, on average, sufficient to produce the observed radio emission from SNRs in the densest starbursts; amplification of post-shock magnetic fields is not required. By contrast, in normal spirals post-shock field amplification (by a factor of a few - 10) is consistent with the data; we find tentative evidence that both the Alfven speed and the ratio of B_SNR^2 to the post-shock pressure ("epsilon_B") are constant in SNRs from galaxy to galaxy. We discuss observational tests that can be used to distinguish between these two interpretations of the radio luminosities of SNRs. Regardless of which is correct, the radio emission from SNRs provides an upper limit to B_ISM that is independent of the minimum energy assumption. For the densest starbursts, the ISM magnetic energy density is below that required for hydrostatic equilibrium; thus magnetic fields are not dynamically important on the largest scales in starbursts, in contrast with spiral galaxies like our own. This dichotomy may have implications for galactic dynamo theory.
description: 11 pages, 4 figures, submitted to MNRAS, revised to reflect referee's comments
title: ÐÐ½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸ÑÐ¼Ð¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð Ð°ÑÑÐºÐ°Ð·Ð¾Ð²Ð°, ÐÐ»ÑÐ³Ð°
name: ÐÐ°Ð»Ð¸Ð½Ð¸Ð½Ð°, ÐÐ»ÑÐ³Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2017
Subjects: Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¸
Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ
ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼

description: Ð¡Ð¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ° Ð¿Ð¾ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ 38.04.02 Â«ÐÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÂ». ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ Ð°ÑÐ¿ÐµÐºÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ Ð¿Ð¾ Ð°ÐºÑÑÐ°Ð»ÑÐ½ÑÐ¼ Ð²Ð¾Ð¿ÑÐ¾ÑÐ°Ð¼ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¼Ð¸ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸ÑÐ¼Ð¸, Ð²Ð½ÑÑÑÐµÐ½Ð½Ð¸Ð¼Ð¸ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸ÑÐ¼Ð¸, Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÐºÑÐ»ÑÑÑÑÐ¾Ð¹. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÑÐ°Ð¼Ð¾Ð¾Ð±ÑÑÐ°ÑÑÐ°ÑÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ, ÐºÐ¾ÑÐ¾ÑÐ°Ñ Ð³ÐµÐ½ÐµÑÐ¸ÑÑÐµÑ ÑÑÐ»Ð¾Ð²Ð¸Ñ Ð´Ð»Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ, Ð¿ÑÐ¸Ð¾Ð±ÑÐµÑÐµÐ½Ð¸Ñ, Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸ Ð¸ ÑÐ¾ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð·Ð½Ð°Ð½Ð¸Ð¹ ÑÐ²Ð¾Ð¸Ñ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð², Ð¿Ð¾ÑÐºÐ¾Ð»ÑÐºÑ ÑÑÐ¿ÐµÑÐ½ÑÐµ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐºÐ¾Ð½ÐºÑÑÐ¸ÑÑÑÑ Ð¼ÐµÐ¶Ð´Ñ ÑÐ¾Ð±Ð¾Ð¹ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð·Ð½Ð°Ð½Ð¸Ð¹ Ð¸ ÐºÐ»ÑÑÐµÐ²ÑÑ ÐºÐ¾Ð¼Ð¿ÐµÑÐµÐ½ÑÐ¸Ð¹. ÐÐ»Ð°Ð²Ð½Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ ÐºÐ»ÑÑÐµÐ²Ð¾Ð¹ ÑÐ¾Ð»Ð¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð¿ÑÐ¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ Ð¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ð¹. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÐµÑ ÑÐ¾ÑÐ¼ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ, Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ ÐºÑÑÑ Â«ÐÐ½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸ÑÂ».
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ Ð¡Ð¾Ð²ÐµÑÐ° Ð¿Ð¾ Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð£ÑÐµÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ° ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾.
S-wave DK interactions in the chiral SU(3) quark model
Creators: name: Zhang, Dan
name: Zhao, Qiao-Yan
name: Zhang, Qiu-Yang
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The $DK$ interaction is relevant to the interpretation of the $D_{sJ}(2317)$. We dynamically investigate $S$-wave $DK$ interactions in the chiral SU(3) quark model by solving the resonating group method equation. The numerical results show an attraction between $D$ and $K$, which is from boson exchanges between light quarks. However, such an attraction is not strong enough to form a $DK$ molecule. Meanwhile, $S$ partial wave phase shifts of $DK$ elastic scattering are obtained. The case of $S$-wave $D^*K$ is rather similar to that of $DK$. To draw a definite conclusion whether a molecular state exists in $DK$ or $D^*K$ system, more details of dynamics should be considered in further study.
description: 4 pages, 3 figures
Periodic orbit analysis at the onset of the unstable dimension variability and at the blowout bifurcation
Creators: name: Pereira, Rodrigo Frehse
name: Pinto, Sandro Ely de Souza
name: Viana, Ricardo L.
name: Lopes, Sergio R.
name: Grebogi, Celso
Publisher: name: arXiv
Year: 2009
Subjects: subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Physical sciences

description: Many chaotic dynamical systems of physical interest present a strong form of nonhyperbolicity called unstable dimension variability (UDV), for which the chaotic invariant set contains periodic orbits possessing different numbers of unstable eigendirections. The onset of UDV is usually related to the loss of transversal stability of an unstable fixed point embedded in the chaotic set. In this paper, we present a new mechanism for the onset of UDV, whereby the period of the unstable orbits losing transversal stability tends to infinity as we approach the onset of UDV. This mechanism is unveiled by means of a periodic orbit analysis of the invariant chaotic attractor for two model dynamical systems with phase spaces of low dimensionality, and seems to depend heavily on the chaotic dynamics in the invariant set. We also described, for these systems, the blowout bifurcation (for which the chaotic set as a whole loses transversal stability) and its relation with the situation where the effects of UDV are the most intense. For the latter point, we found that chaotic trajectories off, but very close to, the invariant set exhibit the same scaling characteristic of the so-called on-off intermittency.
description: 32 pages (preprint format), 9 figures
Emission from a Young Protostellar Object I. Signatures of Young Embedded Outflows
Creators: name: Yamada, M.
name: Machida, M. N.
name: Inutsuka, S.
name: Tomisaka, K.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We examine emission from a young protostellar object (YPO) with three-dimensional ideal MHD simulations and three-dimensional non-local thermodynamic equilibrium (non-LTE) line transfer calculations, and show the first results. To calculate the emission field, we employed a snapshot result of an MHD simulation having young bipolar outflows and a dense protostellar disk (a young circumstellar disk) embedded in an infalling envelope. Synthesized line emission of two molecular species (CO and SiO) show that subthermally excited SiO lines as a high density tracer can provide a better probe of the complex velocity field of a YPO, compared to fully thermalized CO lines. In a YPO at the earliest stage when the outflows are still embedded in the collapsing envelope, infall, rotation and outflow motions have similar speeds. We find that the combined velocity field of these components introduces a great complexity in the line emissions through varying optical thickness and emissivity, such as asymmetric double-horn profiles. We show that the rotation of the outflows, one of the features that characterizes an outflow driven by magneto-centrifugal forces, appears clearly in velocity channel maps and intensity-weighted mean velocity (first moment of velocity) maps. The somewhat irregular morphology of the line emission at this youngest stage is dissimilar to a more evolved object such as young Class 0. High angular resolution observation by e.g., the Atacama Large Millimeter/submillimeter Array (ALMA) telescope can reveal these features.
description: 46 pages, 19 figures: accepted for publication in ApJ. High resolution figures are available at https://www.asiaa.sinica.edu.tw/~masako/preprints/ms_of_final.pdf
Mayapan PEMY Informe 2001-2004 Seasons
Creators: name: Masson, Marilyn
Year: 2008
Subjects: subject: Yucatan (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/762/yucatan-state-territory
subject: Mesoamerican Postclassic period
valueUri: https://core.tdar.org/browse/temporal-keyword/5618/mesoamerican-postclassic-period
subject: Postclassic Maya
valueUri: https://core.tdar.org/browse/culture-keyword/8273/postclassic-maya
subject: Urban
valueUri: https://core.tdar.org/browse/site-type/2131/urban
subject: Ceramic
valueUri: https://core.tdar.org/browse/material-type/1/ceramic
subject: Chipped Stone
valueUri: https://core.tdar.org/browse/material-type/2/chipped-stone
subject: Fauna
valueUri: https://core.tdar.org/browse/material-type/4/fauna
subject: Ground Stone
valueUri: https://core.tdar.org/browse/material-type/7/ground-stone
subject: political capital
valueUri: https://core.tdar.org/browse/other-keyword/166127/political-capital
subject: Household Archaeology
valueUri: https://core.tdar.org/browse/other-keyword/134855/household-archaeology
subject: Archaeological Overview
valueUri: https://core.tdar.org/browse/investigation-type/1/archaeological-overview

description: Report to INAH of 2001-2004 seasons of survey, surface collection, test-pitting and horizontal excavation of residential zone of Mayapan (in Spanish).
Lampi gamma “standard” come supernove Ia
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2016

Un metodo inedito per sfruttare le più potenti esplosioni dell’Universo, i GRB, come strumento per calibrarne la velocità d’espansione è stato messo a punto da un team di ricercatori guidato da Maria Giovanna Dainotti, ricercatrice alla Stanford University e all’INAF IASF di Bologna
title: ÐÐ¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°Ð½Ð°Ñ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: 2016
Subjects: Ð±Ð¸Ð·Ð½ÐµÑ
Ð¿Ð»Ð°Ð½
ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐ¹ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½
business
plan
electronic shop

description: ÐÐ°Ð½Ð½Ð°Ñ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð° ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð°. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿Ð¾Ð´ÑÐµÑÐºÐ¸Ð²Ð°ÐµÑÑÑ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÑ ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð° ÐºÐ°Ðº Ð½ÐµÐ¾ÑÑÐµÐ¼Ð»ÐµÐ¼Ð¾Ð¹ ÑÐ°ÑÑÐ¸ Ð²Ð½ÑÑÑÐ¸Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ»Ñ Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°Ð·Ð´ÐµÐ»Ð° Ð°Ð²ÑÐ¾ÑÑ ÑÐ´Ð°Ð»Ð¾ÑÑ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾ Ð´ÐµÑÐ°Ð»ÑÐ½Ð¾ Ð¾Ð·Ð½Ð°ÐºÐ¾Ð¼Ð¸ÑÑÑÑ Ñ ÑÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ¾Ð¹ Ð¿Ð¾ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð¾Ð². ÐÑÐ¾Ð±Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¸ ÑÑÐ¾Ð¼ ÑÐ´ÐµÐ»ÑÐ»Ð¾ÑÑ ÑÑÑÑÐºÑÑÑÐµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð° Ð¸ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ ÐºÐ°Ð¶Ð´Ð¾Ð³Ð¾ Ð¸Ð· ÑÐ°Ð·Ð´ÐµÐ»Ð¾Ð² ÑÑÐ¾Ð¹ ÑÑÑÑÐºÑÑÑÑ. ÐÐ¿Ð¸ÑÑÐ²Ð°ÑÑÑÑ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÑÐ½ÐºÐ° ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÑ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð¾Ð². ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð°, ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÐ¸ÑÐºÐ¾Ð².
description: This thesis is devoted to the creation of a business plan electronic store. The paper emphasizes the need to develop a business plan as an integral part of organizational planning. For writing theoretical part the author managed relatively get acquainted with educational-methodological literature on the development of business plans. Special attention was paid to the structure development of the business plan and the content of each section of this structure. Describes the features of development of the market of electronic stores. The work on drafting the most effective business plan, assessment of risks.
Corona-Pandemie – die Kinder- und Jugendhilfe im Stresstest – eine gewerkschaftliche Zwischenbilanz
Creators: name: Wegner, Alexander
Publisher: name: Universitäts- und Landesbibliothek Sachsen-Anhalt
Year: 2020
Subjects: subject: Corona, Arbeitsbedingungen, Arbeitsschutz, Gewerkschaft
subject: 300
subject: 360

description: Gewerkschaftliche Perspektiven auf die Arbeitsbedingungen im Bereich sozialer Dienste angesichts der Corona-Pandemie.
Il pianoforte di Einstein
Creators: Antonella Gasperini
Publisher: name: Media Inaf
Year: 2016

I colli di Firenze, Hans-Joachim Staude, le leggi razziali, Tiziano Terzani, Albert Einstein e la sua famiglia… vicende e persone che s'intrecciano attorno a un unico oggetto: un pianoforte a coda del 1899. La storia, e la musica, giovedì sera ad Arcetri
Marte: esploratori cercasi
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2016

Marte ha bisogno di te! Per andare alla conquista del rosso Pianeta c’è bisogno di esploratori, agricoltori, geometri, periti, arrotini, aggiustatutto, turnanti notturni, insegnanti. Ecco la nuova e affascinante campagna NASA
A stage in the making of a physician
Creators: name: Chang, Yunshik
Publisher: name: University of British Columbia
Year: 2012

description: The process of the socialization of first year medical students is analyzed according to a paradigm of adult socialization. This paradigm consists of three sets of variables, that is, independent variable (I), personal background characteristics, independent variable (II), elements of interpersonal relation in which students are involved, and dependent variable, the cultural content of socialization. The study shows (a) that during the first year the medical students tend to think of the first year as the least important period for their later career. Besides being least important, the first year appears to be the most difficult. They also feel hard pressed for time-- there seems to be too much to learn for the time allowed. However, they expect that as they go through medical school, their training will be less difficult. A majority of them find themselves very much involved in the competition among themselves. Their attitudes towards this are rather neutral. They express satisfaction with their faculty members in the given direction in their studies. (b) In the assessment of their performance during their training, a majority of the students classify themselves as average, the reference point of which is largely found in themselves rather than in their fellow students, or in the opinion of the faculty members. (c) With regard to their attitudes and values; students tend to hold the initial values which they had on entering medical school, namely, "people-orientation." No student thinks of himself as a doctor in The first year, in fact, from the beginning he did not expect to establish his professional self-image in the first year. On the other hand, the outline of the image of physician which emerged on entry into medical school remains almost the same at the end of the year with only a slight modification. The image is characterized primarily by personality traits, and a task-oriented emphasis. As the year comes to an end, a substantial proportion of students tend to specify themselves as preferring general practice as their later career. This was not chosen by anyone at the beginning of the year. Their expected income differs little from the actual current income of physicians. They tend to express more satisfaction with their chosen career as they progress through the first year.
title: ÐÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÐ½ÑÐµ Ð´ÐµÑÐµÐ²ÑÐ½Ð½ÑÐµ Ð±Ð°Ð»ÐºÐ¸ ÐºÐ¾ÑÐ¾Ð±ÑÐ°ÑÐ¾Ð³Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ
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 Ð¾Ð¼Ð°Ð½Ð¾Ð², ÐÐ¸ÐºÐ¾Ð»Ð°Ð¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐÐ°Ð»ÐºÐ¸ Ð´ÐµÑÐµÐ²ÑÐ½Ð½ÑÐµ
ÐÐ¾Ð½ÐµÑÐ½ÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð¼ÐµÑÐ¾Ð´
ÐÐ»Ð¸ÑÑ ÑÐµÐ±ÑÐ¸ÑÑÑÐµ
ÐÐ»Ð¸ÑÑ Ð´ÑÐµÐ²ÐµÑÐ½Ð¾-ÑÑÑÑÐ¶ÐµÑÐ½ÑÐµ

description: ÐÐºÑÐ¸Ð²Ð½Ð¾ ÑÐ°Ð·Ð²Ð¸Ð²Ð°ÑÑÐ¸Ð¹ÑÑ ÑÑÐ½Ð¾Ðº Ð´ÐµÑÐµÐ²ÑÐ½Ð½Ð¾Ð³Ð¾ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° ÑÑÐµÐ±ÑÐµÑ Ð¼Ð¾Ð´ÐµÑÐ½Ð¸Ð·Ð°ÑÐ¸Ð¸, Ð¸Ð·Ð¾Ð±ÑÐµÑÐµÐ½Ð¸Ñ Ð¸ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² Ð¸ Ð½Ð¾Ð²ÑÑ ÑÐ¸Ð¿Ð¾Ð² ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹. ÐÐ´Ð½Ð¸Ð¼ Ð¸Ð· Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ð½ÑÑ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð´Ð»Ñ Ð½ÐµÑÑÑÐ¸Ñ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð´ÐµÑÐµÐ²ÑÐ½Ð½ÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ ÑÐ²Ð»ÑÑÑÑÑ Ð´ÐµÑÐµÐ²ÑÐ½Ð½ÑÐµ Ð±Ð°Ð»ÐºÐ¸ Ð´Ð²ÑÑÐ°Ð²ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¸ ÐºÐ¾ÑÐ¾Ð±ÑÐ°ÑÐ¾Ð³Ð¾ ÑÐµÑÐµÐ½Ð¸Ð¹. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¸ÑÑÐ»ÐµÐ´ÑÐµÑÑÑ Ð±Ð°Ð»ÐºÐ° ÐºÐ¾ÑÐ¾Ð±ÑÐ°ÑÐ¾Ð³Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ, Ð¿Ð¾ÑÑÐ° ÐºÐ¾ÑÐ¾ÑÐ¾Ð¹ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ñ Ð¸Ð· ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð´ÑÐµÐ²ÐµÑÐ¸Ð½Ñ, Ð° ÑÑÐµÐ½ÐºÐ¸ Ð¸Ð· Ð¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾-ÑÑÑÑÐ¶ÐµÑÐ½ÑÑ Ð¿Ð»Ð¸Ñ. ÐÑÐ¸Ð²Ð¾Ð´Ð¸ÑÑÑ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ð¹, Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð½ÑÑ Ð¿Ð¾ Ð¾ÑÐµÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾Ð¹ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐµ, Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ Ð¸Ð· Ð¾Ð±ÑÐµÐ¼Ð½Ð¾Ð¹ ÐºÐ¾Ð½ÐµÑÐ½Ð¾-ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ½Ð¾Ð¹ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð² ÐÐ ÐÐ¸ÑÐ° Ð¡ÐÐÐ  Ð¸ Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð½ÑÑ Ð¿Ð¾ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ°Ð¼ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ¾Ð². Ð ÑÐ°ÑÑÐµÑÐµ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° ÑÑÐ¸ÑÑÐ²Ð°ÑÑÑÑ Ð°Ð½Ð¸Ð·Ð¾ÑÑÐ¾Ð¿Ð½ÑÐµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð´ÑÐµÐ²ÐµÑÐ¸Ð½Ñ Ð¸ ÐÐ¡Ð-Ð¿Ð»Ð¸Ñ Ð¿ÑÑÐµÐ¼ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ Ð¾ÑÑÐ¾ÑÑÐ¾Ð¿Ð½ÑÑ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð². ÐÐ¿ÑÐµÐ´ÐµÐ»ÑÑÑÑÑ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ Ð¾Ð¿Ð°ÑÐ½ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ Ð² ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸. Ð Ð·Ð°ÐºÐ»ÑÑÐµÐ½Ð¸Ð¸ Ð´Ð°ÑÑÑÑ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð°ÐºÑÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÑÐµÑÑÐ²ÑÑÑÐµÐ¹ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾Ð¹ Ð±Ð°Ð·Ñ, ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐ°ÑÑÐµÑÑ Ð±Ð°Ð»Ð¾Ðº ÐºÐ¾ÑÐ¾Ð±ÑÐ°ÑÐ¾Ð³Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ. ÐÑÐ¸Ð²Ð¾Ð´Ð¸ÑÑÑ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð´Ð°Ð½Ð½ÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ Ð² ÐºÐ°ÑÐºÐ°ÑÐ½Ð¾Ð¼ Ð´Ð¾Ð¼Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ð¸.
title: ÐÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð»ÐµÑÐµÐ±Ð½Ð¾Ð³Ð¾ Ð±Ð»Ð¾ÐºÐ° Â«Ð¥Ð¾ÑÐ¿Ð¸Ñ (ÐÐµÑÑÐºÐ¸Ð¹)Â»
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ±ÑÑÐ°ÑÐ¼Ð°Ð½Ð¾Ð²Ð°, 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: 2017
Subjects: Ð³ÐµÐ½ÐµÑÐ°Ð»ÑÐ½ÑÐ¹ Ð¿Ð»Ð°Ð½
Ð¾Ð±ÑÐµÐ¼Ð½Ð¾-Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ðµ ÑÐµÑÐµÐ½Ð¸Ðµ
ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½Ð¾Ðµ ÑÐµÑÐµÐ½Ð¸Ðµ
Ð»ÐµÐ½ÑÐ¾ÑÐ½ÑÐ¹ ÑÑÐ½Ð´Ð°Ð¼ÐµÐ½Ñ
ÑÑÐ¾Ð»Ð±ÑÐ°ÑÑÐ¹ ÑÑÐ½Ð´Ð°Ð¼ÐµÐ½Ñ

description: B ÑÐ°Ð¼ÐºÐ°Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð·Ð°Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½ ÐÐµÑÐµÐ±Ð½ÑÐ¹ Ð±Ð»Ð¾Ðº Â«Ð¥Ð¾ÑÐ¿Ð¸Ñ (ÐÐµÑÑÐºÐ¸Ð¹)Â» Ð² Ð³. Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³.ÐÑÑÐ¸ÑÐµÐºÑÑÑÐ½Ð¾-ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ ÑÐ°ÑÑÑ Ð²ÐºÐ»ÑÑÐ°ÐµÑ Ð² ÑÐµÐ±Ñ ÐºÑÐ°ÑÐºÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÑ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÐºÑÐ°, ÐºÑÐ°ÑÐºÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÑ ÑÑÐ»Ð¾Ð²Ð¸Ð¹ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð°, Ð¾Ð±ÑÐµÐ¼Ð½Ð¾-Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ðµ Ð¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½Ð¾Ðµ ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð´Ð°Ð½Ð¸Ñ, ÑÐ°ÑÑÐµÑ Ð³Ð»ÑÐ±Ð¸Ð½Ñ Ð¿ÑÐ¾Ð¼ÐµÑÐ·Ð°Ð½Ð¸Ñ Ð³ÑÑÐ½ÑÐ° Ð¸ Ð³Ð»ÑÐ±Ð¸Ð½Ñ Ð·Ð°Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð¾ÑÐ²Ñ ÑÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÐ¾Ð². B ÑÐ°ÑÑÐµÑÐ½Ð¾-ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½Ð¾Ð¹ ÑÐ°ÑÑÐ¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ ÑÐ±Ð¾Ñ Ð½Ð°Ð³ÑÑÐ·Ð¾Ðº. Ð ÑÐ¾Ð¼ ÑÐ¸ÑÐ»Ðµ ÑÐ°ÑÑÑÑ ÑÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÐ°. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐ°ÑÐ°ÐºÑÐµÑÐ½ÑÐµ ÑÐ·Ð»Ñ.
E… state con INAF
Creators: Francesca Aloisio
Publisher: name: Media Inaf
Year: 2016

Anche in questo 2016 il calendario degli appuntamenti che si terranno presso le sedi INAF sparse su tutto il territorio da nord a sud è ricco e variegato, appuntamenti dedicati al cielo, per avvicinare tutti nel modo più piacevole allo studio e alla passione per l'astronomia. Ce n'è per tutti i gusti, trovate quello più vicino a voi e... godetevi la serata.
Planck-scale Lorentz violation constrained by Ultra-High-Energy Cosmic Rays
Creators: name: Maccione, Luca
name: Taylor, Andrew M.
name: Mattingly, David M.
name: Liberati, Stefano
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We investigate the consequences of higher dimension Lorentz violating, CPT even kinetic operators that couple standard model fields to a non-zero vector field in an Effective Field Theory framework. Comparing the ultra-high energy cosmic ray spectrum reconstructed in the presence of such terms with data from the Pierre Auger observatory allows us to establish two sided bounds on the coefficients of the mass dimension five and six operators for the proton and pion. Our bounds imply that for both protons and pions, the energy scale of Lorentz symmetry breaking must be well above the Planck scale. In particular, the dimension five operators are constrained at the level of $10^{-3} M_{\rm Planck}^{-1}$. The magnitude of the dimension six proton coefficient is bounded at the level of $10^{-6} M_{Planck}^{-2}$ except in a narrow range where the pion and proton coefficients are both negative and nearly equal. In this small area, the magnitude of the dimension six proton coefficient must only be below $10^{-3} M_{\rm Planck}^{-2}$. Constraints on the dimension six pion coefficient are found to be much weaker, but still below $M_{\rm Planck}^{-2}$.
description: v1:21 pages, 5 figures. Submitted to JCAP. v2: Accepted by JCAP. References added. v3: DESY report number added
Dynamics of the TrES-2 system
Creators: name: Freistetter, Florian
name: Süli, Áron
name: Funk, Barbara
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 TrES-2 system harbors one planet which was discovered with the transit technique. In this work we investigate the dynamical behavior of possible additional, lower-mass planets. We identify the regions where such planets can move on stable orbits and show how they depend on the initial eccentricity and inclination. We find, that there are stable regions inside and outside the orbit of TrES-2b where additional, smaller planets can move. We also show that those planets can have a large orbital inclination which makes a detection with the transit technique very difficult.
description: accepted for publication in AN 330 (2009)
title: ÐÐ»Ð°Ð·Ð¼ÐµÐ½Ð½ÑÐµ Ð¿ÑÐ¾ÑÐµÑÑÑ ÑÐ¾ÑÑÐ° Ð¸ ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð½Ð¸ÑÑÐ¸Ð´Ð½ÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð²
title: ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÑ 01.04.08 "Ð¤Ð¸Ð·Ð¸ÐºÐ° Ð¿Ð»Ð°Ð·Ð¼Ñ"
titleType: Subtitle
Creators: name: ÐÐ°ÑÑÑÐºÐ¾Ð², Ð®Ñ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: 2022
Subjects: ÐÐ»Ð°Ð·Ð¼Ð° (ÑÐ¸Ð·.)
ÐÑÐµÐ¼Ð½Ð¸Ð¹, Ð½Ð¸ÑÑÐ¸Ð´Ñ
Ð¢ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð²
ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ
Ð½Ð°Ð½Ð¾ÑÑÑÐ±ÐºÐ¸
Ð¾ÐºÑÐ¸Ð´ ÐºÑÐµÐ¼Ð½Ð¸Ñ
ÑÑÐ¾ÑÐ¾Ð²Ð¾Ð´Ð¾ÑÐ¾Ð´

description: ÐÐ¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐµÐ»ÐµÐºÑÐ¸Ð²Ð½Ð¾Ð¼Ñ Ð¿Ð»Ð°Ð·Ð¼ÐµÐ½Ð½Ð¾Ð¼Ñ ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð½Ð¸ÑÑÐ¸Ð´Ð° Ð¸ Ð²ÑÑÐ¾ÐºÐ¾ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÐ½Ð¾Ð¼Ñ ÑÐ¸Ð½ÑÐµÐ·Ñ Ð½Ð°Ð½Ð¾ÑÑÑÐ±Ð¾Ðº Ð½Ð¸ÑÑÐ¸Ð´Ð° Ð±Ð¾ÑÐ°. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð²Ð¿ÐµÑÐ²ÑÐµ Ð¿Ð¾ÐºÐ°Ð·Ð°Ð½Ð¾, ÑÑÐ¾ ÐºÐ¾Ð»ÐµÐ±Ð°ÑÐµÐ»ÑÐ½Ð¾ Ð²Ð¾Ð·Ð±ÑÐ¶Ð´ÐµÐ½Ð½ÑÐµ Ð¼Ð¾Ð»ÐµÐºÑÐ»Ñ ÑÑÐ¾ÑÐ¾Ð²Ð¾Ð´Ð¾ÑÐ¾Ð´Ð° Ð¸Ð½Ð¸ÑÐ¸Ð¸ÑÑÑÑ ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð½Ð¸ÑÑÐ¸Ð´Ð° ÐºÑÐµÐ¼Ð½Ñ Ð±ÐµÐ· ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾ÐºÑÐ¸Ð´Ð° ÐºÑÐµÐ¼Ð½Ð¸Ñ. ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð° Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¼Ð¾Ð´ÐµÐ»Ñ, Ð¾Ð¿Ð¸ÑÑÐ²Ð°ÑÑÐ°Ñ ÑÐºÐ¾ÑÐ¾ÑÑÑ ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð½Ð¸ÑÑÐ¸Ð´Ð° Ð¸ Ð¾ÐºÑÐ¸Ð´Ð° ÐºÑÐµÐ¼Ð½Ð¸Ñ Ð¾Ñ ÐºÐ¾Ð½ÑÐµÐ½ÑÑÐ°ÑÐ¸Ð¹ ÑÐµÐ°Ð³ÐµÐ½ÑÐ¾Ð², ÑÐ°ÐºÐ¸Ñ ÐºÐ°Ðº HF(v0), HF(v1), H2O, F. ÐÐ¿ÐµÑÐ²ÑÐµ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ Ð¿Ð¾Ð´ÑÐ¾Ð±Ð½ÑÐ¹ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐµÐºÑÑÑÐ¾ÑÐ¾Ð² ÑÐ¾ÑÑÐ° Ð½Ð°Ð½Ð¾ÑÑÑÐ±Ð¾Ðº Ð½Ð¸ÑÑÐ¸Ð´Ð° Ð±Ð¾ÑÐ° Ð¿ÑÐ¸ Ð²ÑÑÐ¾ÐºÐ¾ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÐ½Ð¾Ð¼ ÑÐ¸Ð½ÑÐµÐ·Ðµ Ð² ÑÐ¼ÐµÑÐ¸ B/N2. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ð¾, ÑÑÐ¾ ÑÐ¸ÐºÑÐ°ÑÐ¸Ñ Ð¼Ð¾Ð»ÐµÐºÑÐ»ÑÑÐ½Ð¾Ð³Ð¾ Ð¸ Ð¿Ð¾ÑÑÐµÐ±Ð»ÐµÐ½Ð¸Ðµ Ð±Ð¾ÑÐ° â ÑÑÐ¾ ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÐµ Ð¿ÑÐ¾ÑÐµÑÑÑ, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¿ÑÐ¾ÑÐµÐºÐ°ÑÑ Ð² Ð½ÐµÑÐ°Ð²Ð½Ð¾Ð²ÐµÑÐ½Ð¾Ð¼ ÑÐµÐ¶Ð¸Ð¼Ðµ Ð¿ÑÐ¸ ÑÐ¸Ð¿Ð¸ÑÐ½ÑÑ Ð´Ð»Ñ ÑÐ¸Ð½ÑÐµÐ·Ð° ÑÐºÐ¾ÑÐ¾ÑÑÑÑ Ð¾ÑÐ»Ð°Ð¶Ð´ÐµÐ½Ð¸Ñ Ð³Ð°Ð·Ð°. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ð¾, ÑÑÐ¾ Ð²ÑÑÐ¾ÐºÐ¾Ðµ Ð´Ð°Ð²Ð»ÐµÐ½Ð¸Ðµ, Ð¼ÐµÐ´Ð»ÐµÐ½Ð½Ð°Ñ ÑÐºÐ¾ÑÐ¾ÑÑÑ Ð¾ÑÐ»Ð°Ð¶Ð´ÐµÐ½Ð¸Ñ Ð³Ð°Ð·Ð° Ð¸ Ð½Ð¸Ð·ÐºÐ°Ñ Ð½Ð°ÑÐ°Ð»ÑÐ½Ð°Ñ ÐºÐ¾Ð½ÑÐµÐ½ÑÑÐ°ÑÐ¸Ñ Ð±Ð¾ÑÐ° ÑÐ¼ÐµÑÐ°ÑÑ ÑÐµÐ°ÐºÑÐ¸Ð¸ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐµÐºÑÑÑÐ¾ÑÐ¾Ð² Ð² ÑÑÐ¾ÑÐ¾Ð½Ñ ÑÐ°Ð²Ð½Ð¾Ð²ÐµÑÐ¸Ñ, ÑÑÐ¾ Ð² ÑÐ²Ð¾Ñ Ð¾ÑÐµÑÐµÐ´Ñ ÑÐ²ÐµÐ»Ð¸ÑÐ¸Ð²Ð°ÐµÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¿Ð¾ÑÑÐµÐ±Ð»ÐµÐ½Ð¸Ñ Ð±Ð¾ÑÐ°.
Bell-like inequality for spin-orbit separability of a classical laser beam
Creators: name: Borges, C. V. S.
name: Hor-Meyll, M.
name: Huguenin, J. A. O.
name: Khoury, A. Z.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: In analogy with Bell's inequality for two-qubit quantum states we propose an inequality criterion for the non-separability of the spin-orbit degrees of freedom of a classical laser beam. A definition of separable and non-separable spin-orbit modes is used in consonance with the one presented in Phys. Rev. Lett. 99, 160401 (2007). As the usual Bell's inequality can be violated for entangled two-qubit quantum states, we show both theoretically and experimentally that the proposed spin-orbit inequality criterion can be violated for non-separable modes. A discussion on the classical-quantum transition is also presented.
description: 4 pages, 2 figures
Mayapan PEMY Informe 2008-2009 Seasons
Creators: name: Masson, Marilyn
Year: 2012
Subjects: subject: Yucatan (State / Territory)
valueUri: https://core.tdar.org/browse/geographic-keyword/762/yucatan-state-territory
subject: Mesoamerican Postclassic period
valueUri: https://core.tdar.org/browse/temporal-keyword/5618/mesoamerican-postclassic-period
subject: Postclassic Maya
valueUri: https://core.tdar.org/browse/culture-keyword/8273/postclassic-maya
subject: Urban
valueUri: https://core.tdar.org/browse/site-type/2131/urban
subject: Ceramic
valueUri: https://core.tdar.org/browse/material-type/1/ceramic
subject: Chipped Stone
valueUri: https://core.tdar.org/browse/material-type/2/chipped-stone
subject: Fauna
valueUri: https://core.tdar.org/browse/material-type/4/fauna
subject: Ground Stone
valueUri: https://core.tdar.org/browse/material-type/7/ground-stone
subject: Building Materials
valueUri: https://core.tdar.org/browse/material-type/8/building-materials
subject: sculpture
valueUri: https://core.tdar.org/browse/material-type/3307/sculpture
subject: political capital
valueUri: https://core.tdar.org/browse/other-keyword/166127/political-capital
subject: Household Archaeology
valueUri: https://core.tdar.org/browse/other-keyword/134855/household-archaeology
subject: Archaeological Overview
valueUri: https://core.tdar.org/browse/investigation-type/1/archaeological-overview

description: Report to INAH of 2008-2009 seasons of horizontal excavations in the urban residential zone of Mayapan, including residences, workshops, and a temple and hall at the outlying ceremonial group of Itzmal Ch'en (in Spanish).
The nonlinear saturation of the non-resonant kinetically driven streaming instability
Creators: name: Gargate, L.
name: Fonseca, R. A.
name: Niemiec, J.
name: Pohl, M.
name: Bingham, R.
name: Silva, L. O.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: A non-resonant instability for the amplification of the interstellar magnetic field in young Supernova Remnant (SNR) shocks was predicted by Bell (2004), and is thought to be relevant for the acceleration of cosmic ray (CR) particles. For this instability, the CRs streaming ahead of SNR shock fronts drive electromagnetic waves with wavelengths much shorter than the typical CR Larmor radius, by inducing a current parallel to the background magnetic field. We explore the nonlinear regime of the non-resonant mode using Particle-in-Cell (PIC) hybrid simulations, with kinetic ions and fluid electrons, and analyze the saturation mechanism for realistic CR and background plasma parameters. In the linear regime, the observed growth rates and wavelengths match the theoretical predictions; the nonlinear stage of the instability shows a strong reaction of both the background plasma and the CR particles, with the saturation level of the magnetic field varying with the CR parameters. The simulations with CR-to-background density ratios of n_CR/n_b=10^(-5) reveal the highest magnetic field saturation levels, with energy also being transferred to the background plasma and to the perpendicular velocity components of the CR particles. The results show that amplification factors >10 for the magnetic field can be achieved, and suggest that this instability is important for the generation of magnetic field turbulence, and for the acceleration of CR particles.
Quel vento elettrico su Venere
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2016

C’è un continuo flusso di particelle che abbandona l'atmosfera del pianeta considerato il “gemello bollente” della Terra. Ad alimentarlo, secondo i ricercatori che lo hanno individuato grazie ai dati raccolti dalla missione Venus Express, è l’intenso campo elettrico di Venere. Il commento di Giuseppe Piccioni (INAF)
title: ÐÐµÐ´Ð°Ð³Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ Ð¿ÑÐ°ÐºÑÐ¸ÐºÐ° ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÐ·Ð° ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÑÐ»ÑÑÑÑÑ
title: Pedagogical practice of students of the university of physical culture
Creators: name: Ð¡Ð¼Ð¸ÑÐ½Ð¾Ð²Ð°, 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: Ð½ÐµÐ¿ÑÐµÑÑÐ²Ð½Ð°Ñ Ð¿ÐµÐ´Ð°Ð³Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ Ð¿ÑÐ°ÐºÑÐ¸ÐºÐ°
Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»Ð¸Ð·Ð¼ Ð¿ÐµÐ´Ð°Ð³Ð¾Ð³Ð°
Ð¿ÐµÐ´Ð°Ð³Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¼ÐµÐ»Ð¾ÑÑÑ

description: Ð¡ÑÑÑ Ð½ÐµÐ¿ÑÐµÑÑÐ²Ð½Ð¾Ð¹ Ð¿ÐµÐ´Ð°Ð³Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¿ÑÐ°ÐºÑÐ¸ÐºÐ¸ ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð² ÑÐ¾Ð¼, ÑÑÐ¾Ð±Ñ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¿ÐµÐ´Ð°Ð³Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð±ÑÐ»Ð° ÑÐµÐ³ÑÐ»ÑÑÐ½Ð¾Ð¹, ÑÐ¸ÑÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹, ÐºÐ°Ðº ÑÑÐµÐ±Ð½ÑÐµ Ð·Ð°Ð½ÑÑÐ¸Ñ. ÐÐ½Ð°ÑÐµ Ð³Ð¾Ð²Ð¾ÑÑ, Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÑÑÑÐ´ÐµÐ½ÑÐ° ÑÐ¾Ð»ÑÐºÐ¾ ÑÐ°Ð¼ Ð¸ ÑÐ¾Ð³Ð´Ð° Ð±ÑÐ´ÐµÑ ÑÑÐ¸ÑÐ°ÑÑÑÑ Ð½ÐµÐ¿ÑÐµÑÑÐ²Ð½Ð¾Ð¹ Ð¿ÐµÐ´Ð°Ð³Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¿ÑÐ°ÐºÑÐ¸ÐºÐ¾Ð¹, ÐºÐ¾Ð³Ð´Ð° Ð¸ Ð³Ð´Ðµ Ð¾Ð½: Ð°) Ð¸Ð¼ÐµÐµÑ ÑÐµÐ°Ð»ÑÐ½ÑÑ ÑÑÐµÐ½Ð¸ÐºÐ¾Ð²; Ð±) Ð¾Ð±ÑÑÐ°ÐµÑ, Ð²Ð¾ÑÐ¿Ð¸ÑÑÐ²Ð°ÐµÑ Ð¸ ÑÐ°Ð·Ð²Ð¸Ð²Ð°ÐµÑ Ð¸Ñ; Ð²) Ð¾ÑÑÑÐµÑÑÐ²Ð»ÑÐµÑ Ð¿ÐµÐ´Ð°Ð³Ð¾Ð³Ð¸ÑÐµÑÐºÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð½Ð° Ð¿ÑÐ¾ÑÑÐ¶ÐµÐ½Ð¸Ð¸ Ð²ÑÐµÐ¹ ÑÑÐµÐ±Ñ Ð² Ð²ÑÐ·Ðµ.
description: The essence of continuous pedagogical practice is that studentsâ practical pedagogical activity should be regular and systematic like training sessions. In other words, a studentâs activity only there and then will be considered continuous, when and where the practicant: a) has real students; b) teaches, educates and develops them; c) carries out pedagogical activity throughout his studies at the university.
Verwerfung in der Sozialen Arbeit – Corona als Auslöser?
Creators: name: Meyer, Nikolaus
Publisher: name: Universitäts- und Landesbibliothek Sachsen-Anhalt
Year: 2020
Subjects: subject: Corona
subject: Deprofessionalisierung
subject: 300
subject: 360

description: In dem Artikel werden die mit der Corona-Pandemie einhergehenden Deprofessionalisierungsprozesse in der Sozialen Arbeit zum Thema gemacht.
[APPENDICES] AN ASSESSMENT OF ENERGY EFFICIENCY OBLIGATIONS AS AN ENERGY POLICY INSTRUMENT AND A PERSPECTIVE FOR 2030
Creators: name: Baião, João Pedro Roldão Fernandes
Publisher: name: Zenodo
Year: 2021
Subjects: Energy efficiency obligations, Energy Efficiency Directive, Annual Reports, Energy Savings, Alternative Measures.

description: Appendices of the dissertation in the scope of the Master in Energy for Sustainability, supervised by Professor Dr. Álvaro Filipe Peixoto Cardoso de Oliveira Gomes, and by Professor Dr. António Manuel Oliveira Gomes Martins, and presented to the Department of Mechanical Engineering of the Faculty of Science and Technology, University of Coimbra.
description: {"references": ["EED. (2012). Directive 2012/27/EU of the European Parliament and of the Council of 25 October 2012 on energy efficiency. October 2012, 1\u201356."]}
Pandemic policymaking in European populist and liberal democracies: a comparison between Hungary and Portugal
Creators: name: Kopasz, Marianna
name: Bartha, Attila
name: Takács, Judit
Publisher: name: Taylor & Francis
Year: 2025
Subjects: Medicine
Molecular Biology
Environmental Sciences not elsewhere classified
Cancer
Science Policy
Mental Health
Computational Biology

description: This study compares COVID-19 pandemic policymaking in Hungary and Portugal. These EU member states are similar in most factors that potentially shape the health policy outcome of a pandemic: the level of economic development, the centralization of public administration system and legislature, and the health crisis management preparedness. Yet, the health policy outcome of COVID-19 differs significantly in favour of Portugal. Our expectation is that political factors, in particular distinctive features in pandemic policymaking between populist and liberal democracies may help to explain this difference. To examine the traits of populist pandemic policymaking that may have contributed to worse health policy outcomes in Hungary, we contrast pandemic policymaking in Hungary and Portugal across three dimensions: policy content, policy process, and policy discourse. The empirical analysis covers the period between March 2020 and December 2021, the first four waves of the pandemic in both countries. A main finding is that in Hungary, recurrent polarizing narratives and the lack of collaborative governance may have reduced the government's capacity for policy learning and successful pandemic management.
Fosforo, zinco e zolfo: mai viste stelle così
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2016

Utilizzando il Cosmic Origins Spectrograph, i ricercatori hanno trovato elementi particolari in stelle antichissime della nostra galassia. La scoperta è eccezionale, perché finora (a parte lo zinco) non erano mai stati visti in questo tipo di stelle
From Cavendish to PLANCK: Constraining Newton's Gravitational Constant with CMB Temperature and Polarization Anisotropy
Creators: name: Galli, Silvia
name: Melchiorri, Alessandro
name: Smoot, George F.
name: Zahn, Oliver
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present new constraints on cosmic variations of Newton's gravitational constant by making use of the latest CMB data from WMAP, BOOMERANG, CBI and ACBAR experiments and independent constraints coming from Big Bang Nucleosynthesis. We found that current CMB data provide constraints at the 10% level, that can be improved to 3% by including BBN data. We show that future data expected from the Planck satellite could constrain G at the 1.5% level while an ultimate, cosmic variance limited, CMB experiment could reach a precision of about 0.4%, competitive with current laboratory measurements.
description: 6 pages, 8 figures, corrected typos, added references