cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÐ¾ÑÑÐ¸Ð½Ð¸ÑÐ°. Ð Ð°ÑÑÐµÑ ÐºÐ¾Ð»Ð¾Ð½Ð½Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÑÐ¾Ð²Ð¸Ñ, ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾
Ð¼Ð¾Ð½Ð¾Ð»Ð¸Ñ
ÑÐ°ÑÑÐµÑ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¼ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¼ Ð¿ÑÐ¾ÐµÐºÑÐµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¿ÑÐ¾ÐµÐºÑ ÑÐ°ÑÑÐ¸ÑÐµÐ½Ð¸Ñ Ð³Ð¾ÑÑÐ¸Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° Ð¿ÑÑÐµÐ¼ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð½Ð¾Ð²Ð¾Ð³Ð¾ 2-ÑÑÐ°Ð¶Ð½Ð¾Ð³Ð¾ Ð·Ð´Ð°Ð½Ð¸Ñ Ð³Ð¾ÑÑÐ¸Ð½Ð¸ÑÑ Ñ Ð¼ÐµÐ·Ð¾Ð½Ð¸Ð½Ð¾Ð¼. ÐÐµÑÑÐ¾ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð³Ð¾ÑÑÐ¸Ð½Ð¸ÑÑ - ÐÑÐ±Ð¾ÑÐ³ÑÐºÐ¾Ðµ ÑÐ¾ÑÑÐµ Ð½Ð° Ð¿ÐµÑÐµÑÐµÑÐµÐ½Ð¸Ð¸ Ñ Ð¿Ñ. ÐÑÐ½Ð°ÑÐ°ÑÑÐºÐ¾Ð³Ð¾. ÐÐ»Ð¾ÑÐ°Ð´Ñ Ð·Ð°ÑÑÑÐ¾Ð¹ÐºÐ¸ ÑÐ¾ÑÑÐ°Ð²Ð»ÑÐµÑ 996 Ð¼. Ð Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¼ Ð¿ÑÐ¾ÐµÐºÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð°ÑÑÐ¸ÑÐµÐºÑÑÑÐ½ÑÐµ, Ð¾Ð±ÑÐµÐ¼Ð½Ð¾- Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½ÑÐµ Ð¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð´Ð°Ð½Ð¸Ñ. Ð ÑÐ°Ð·Ð´ÐµÐ»Ðµ Â«Ð Ð°ÑÑÐµÑÐ½Ð°Ñ ÑÐ°ÑÑÑÂ» Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ Ð½ÐµÑÑÑÐµÐ¹ ÐºÐ¾Ð»Ð¾Ð½Ð½Ñ. Ð Ð°ÑÑÐµÑ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾-Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° Base. ÐÑÐ¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ð¸ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÐ°ÐºÐ¶Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð»Ð¸ÑÑ ÑÐ¸ÑÑÐµÐ¼Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, ÑÐ°ÐºÐ¸Ðµ ÐºÐ°Ðº AutoCAD. ÐÐ° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾, ÐºÐ¾Ð¼ÑÐ¾ÑÑÐ½Ð¾Ð³Ð¾ Ð¸ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾Ð³Ð¾ Ð³Ð¾ÑÑÐ¸Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ°.
Se la dinamo solare balla al ritmo dei pianeti
Creators: Paolo Soletta
Publisher: name: Media Inaf
Year: 2019

Il periodico allineamento fra Venere, Terra e Giove potrebbe avere un ruolo nell’inversione del campo magnetico del Sole e, dunque, nel ciclo dell’attività solare. Lo propone uno studio dell’istituto di ricerca tedesco Helmholtz-Zentrum Dresden-Rossendorf, aggiungendo nuovi dettagli a un filone di ricerca che va avanti da anni
Eine Disziplin stellt um: Open-Access-Transformation in der Linguistik
Creators: name: Nordhoff, Sebastian
Publisher: name: Zenodo
Year: 2022
Subjects: Open Access

description: In diesem Vortrag skizziert Dr. Sebastian Nordhoff (Language Science Press, TIB) die Open-Access-Transformation in der Sprachwissenschaft, die als Disziplin in dieser Hinsicht sehr weit fortgeschritten ist, und diskutiert Faktoren, die hier einen positiven Einfluss hatten. Ziel ist, durch klare Identifikation der Faktoren sowie Fallbeispiele anderen Disziplinen ein Instrumentarium an die Hand zu geben, wie eine disziplinäre Open-Access-Transformation gelingen kann. Illustriert wird die Transformation an drei Fallbeispielen: Lingua (Elsevier, closed access) → Glossa (Open Library of Humanities, Diamond Open Access)  Zeitschrift für Sprachwissenschaften (de Gruyter, closed access) → Zeitschrift für Sprachwissenschaften (de Gruyter, Diamond Open Access) Language Science Press (Neugründung, Diamond Open Access) Als Rahmenbedingungen werden die historische Publikationskultur in der Linguistik sowie die linguistische Verlagslandschaft erläutert, die Hinweise liefern, warum hier eine Transformation relativ erfolgreich sein konnte. Ein Vergleich von disziplinär ausgerichteten Plattformen (Language Science Press, SCOAP³) mit regional ausgerichteten Universitätsverlagen rundet den Vortrag ab. Die Präsentation wurde im Rahmen der Webinar-Reihe Open Access Talk des BMBF-geförderten Projektes open-access.network am 25.11.2021 gehalten.
Paspalum dilatatum Poir.
Creators: name: Cardona, Àngel Manuel Hernández
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Paspalum
Paspalum dilatatum

description: Paspalum dilatatum Poir.
(serreig d’arròs). De procedència sud-americana, s’ha naturalitzat a una gran part del món. Es fa en herbassars humits ruderalitzats. Hi és present a les zones baixes.
description: Published as part of Cardona, Àngel Manuel Hernández, 2022, Catàleg actualitzat i claus d'identificació de les gramínies de Sant Llorenç del Munt i l'Obac (Barcelona), pp. 64-86 in Nemus 12 on page 73, DOI: 10.5281/zenodo.12170499
Novae With Long-Lasting Supersoft Emission That Drive a High Accretion Rate
Creators: name: Schaefer, Bradley E.
name: Collazzi, Andrew C.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We identify a new class of novae characterized by the post-eruption quiescent light curve being more than roughly a factor of ten brighter than the pre-eruption light curve. Eight novae (V723 Cas, V1500 Cyg, V1974 Cyg, GQ Mus, CP Pup, T Pyx, V4633 Sgr, and RW UMi) are separated out as being significantly distinct from other novae. This group shares a suite of uncommon properties, characterized by the post-eruption magnitude being much brighter than before eruption, short orbital periods, long-lasting supersoft emission following the eruption, a highly magnetized white dwarf, and secular declines during the post-eruption quiescence. We present a basic physical picture which shows why all five uncommon properties are causally connected. Most novae do not have adequate accretion for continuous hydrogen burning, but some can achieve this if the companion star is nearby (with short orbital period) and a magnetic field channels the matter onto a small area on the white dwarf so as to produce a locally high accretion rate. The resultant supersoft flux irradiates the companion star and drives a higher accretion rate (with a brighter post-eruption phase), which serves to keep the hydrogen burning and the supersoft flux going. The feedback loop cannot be perfectly self-sustaining, so the supersoft flux will decline over time, forcing a decline in the accretion rate and the system brightness. We name this new group after the prototype, V1500 Cyg. V1500 Cyg stars are definitely not progenitors of Type Ia supernovae. The V1500 Cyg stars have similar physical mechanisms and appearances as predicted for nova by the hibernation model, but with this group accounting for only 14% of novae.
description: Astronomical Journal, in press, 39 pages, 10 figures
title: ÐÐµÐ»ÐµÐ·Ð¾Ð±ÐµÑÐ¾Ð½Ð½ÑÐµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸. Ð Ð°ÑÑÐµÑÑ Ð¿Ð¾ Ð½ÐµÑÑÑÐµÐ¹ ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¡ÑÑÐ°ÑÐ¾Ð², ÐÐ¼Ð¸ÑÑÐ¸Ð¹
name: Ð¡Ð¾ÐºÐ¾Ð»Ð¾Ð², ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2009
Subjects: ÐÐµÐ»ÐµÐ·Ð¾Ð±ÐµÑÐ¾Ð½Ð½ÑÐµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸

description: ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾-ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ° Ð²ÑÐµÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ Ð¿ÑÐ¸ Ð¿ÑÐ¾ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ð¸ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¾ÑÐ½Ð¾Ð² Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«ÐÐµÐ»ÐµÐ·Ð¾Ð±ÐµÑÐ¾Ð½Ð½ÑÐµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸Â» Ð¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ð¸ Ð¿Ð¾ ÑÑÐ¾Ð¹ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ ÐºÑÑÑÐ¾Ð²ÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð² Ð¸ ÑÐ°Ð±Ð¾Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐ¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ð¸ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½ÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð² Ð¸ Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ð¸Ð¸ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¸Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¹. ÐÐ·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ñ ÑÐ°ÑÑÐµÑÐ° Ð¶ÐµÐ»ÐµÐ·Ð¾Ð±ÐµÑÐ¾Ð½Ð½ÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð±ÐµÐ· Ð¿ÑÐµÐ´Ð²Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ Ð½ÐµÑÑÑÐµÐ¹ ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ (Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÐ¸ Ð¸ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸). ÐÐ¾Ð´ÑÐ¾Ð±Ð½Ð¾ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÑÐ°Ð´Ð¸Ð¸ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð½Ð¾-Ð´ÐµÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð¿Ð¾ Ð¼ÐµÑÐµ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ ÑÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð½Ð°Ð³ÑÑÐ·ÐºÐ¸, ÑÐ°ÑÑÐµÑÐ½ÑÐµ Ð¿ÑÐµÐ´Ð¿Ð¾ÑÑÐ»ÐºÐ¸ Ð¸ ÑÐ¿ÑÐ¾ÑÐ°ÑÑÐ¸Ðµ Ð´Ð¾Ð¿ÑÑÐµÐ½Ð¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¼ÐµÑÐ¾Ð´Ñ ÑÐ°ÑÑÐµÑÐ° Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐ¸Ð¼Ð¸ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½ÑÐ¼Ð¸ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°Ð¼Ð¸ (Ð¡ÐÐ¸Ð 52-01-2003 Ð¸ Ð¡Ð 52-101-2003). ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¸ Ð¿Ð¾ÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÑÐ°ÑÑÐµÑÐ° Ð¸Ð·Ð³Ð¸Ð±Ð°ÐµÐ¼ÑÑ (Ð¿Ð¾ Ð½Ð¾ÑÐ¼Ð°Ð»ÑÐ½ÑÐ¼ Ð¸ Ð½Ð°ÐºÐ»Ð¾Ð½Ð½ÑÐ¼ ÑÐµÑÐµÐ½Ð¸ÑÐ¼), Ð²Ð½ÐµÑÐµÐ½ÑÑÐµÐ½Ð½Ð¾-ÑÐ¶Ð°ÑÑÑ Ð¸ ÑÐ°ÑÑÑÐ½ÑÑÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð². ÐÐµÐºÐ¾ÑÐ¾ÑÑÐµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð²Ð¿ÐµÑÐ²ÑÐµ. ÐÐ¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾-ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ°, Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ ÐºÐ°Ðº Ð¿Ð¾ Ð´Ð½ÐµÐ²Ð½Ð¾Ð¹ Ð¸ Ð²ÐµÑÐµÑÐ½ÐµÐ¹ ÑÐ¾ÑÐ¼Ð°Ð¼ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ, ÑÐ°Ðº Ð¸ Ð¿Ð¾ ÑÑÐµÐ±Ð½ÑÐ¼ Ð¿Ð»Ð°Ð½Ð°Ð¼ Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð°Ð¼ Ð·Ð°Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð¾ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ñ. ÐÐ¾Ð¶ÐµÑ Ð±ÑÑÑ ÑÐ°ÐºÐ¶Ðµ Ð¿Ð¾Ð»ÐµÐ·Ð½ÑÐ¼ Ð´Ð»Ñ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð² Ð¸ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾-ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ°Ð±Ð¾ÑÐ½Ð¸ÐºÐ¾Ð², Ð·Ð°Ð½Ð¸Ð¼Ð°ÑÑÐ¸ÑÑÑ ÐºÐ¾Ð½ÑÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¸ ÑÐ°ÑÑÐµÑÐ¾Ð¼ Ð¶ÐµÐ»ÐµÐ·Ð¾Ð±ÐµÑÐ¾Ð½Ð½ÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Astro2010 Decadal Survey Whitepaper: Coordinated Science in the Gravitational and Electromagnetic Skies
Creators: name: Bloom, Joshua S.
name: Holz, Daniel E.
name: Hughes, Scott A.
name: Menou, Kristen
name: Adams, Allan
name: Anderson, Scott F.
name: Becker, Andy
name: Bower, Geoffrey C.
name: Brandt, Niel
name: Cobb, Bethany
name: Cook, Kem
name: Corsi, Alessandra
name: Covino, Stefano
name: Fox, Derek
name: Fruchter, Andrew
name: Fryer, Chris
name: Grindlay, Jonathan
name: Hartmann, Dieter
name: Haiman, Zoltan
name: Kocsis, Bence
name: Jones, Lynne
name: Loeb, Abraham
name: Marka, Szabolcs
name: Metzger, Brian
name: Nakar, Ehud
name: Nissanke, Samaya
name: Perley, Daniel A.
name: Piran, Tsvi
name: Poznanski, Dovi
name: Prince, Tom
name: Schnittman, Jeremy
name: Soderberg, Alicia
name: Strauss, Michael
name: Shawhan, Peter S.
name: Shoemaker, David H.
name: Sievers, Jonathan
name: Stubbs, Christopher
name: Tagliaferri, Gianpiero
name: Ubertini, Pietro
name: Wozniak, Przemyslaw
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: It is widely expected that the coming decade will witness the first direct detection of gravitational waves (GWs). The ground-based LIGO and Virgo GW observatories are being upgraded to advanced sensitivity, and are expected to observe a significant binary merger rate. The launch of The Laser Interferometer Space Antenna (LISA) would extend the GW window to low frequencies, opening new vistas on dynamical processes involving massive (M >~ 10^5 M_Sun) black holes. GW events are likely to be accompanied by electromagnetic (EM) counterparts and, since information carried electromagnetically is complementary to that carried gravitationally, a great deal can be learned about an event and its environment if it becomes possible to measure both forms of radiation in concert. Measurements of this kind will mark the dawn of trans-spectral astrophysics, bridging two distinct spectral bands of information. The aim of this whitepaper is to articulate future directions in both theory and observation that are likely to impact broad astrophysical inquiries of general interest. What will EM observations reflect on the nature and diversity of GW sources? Can GW sources be exploited as complementary probes of cosmology? What cross-facility coordination will expand the science returns of gravitational and electromagnetic observations?
description: 7 pages (plus one coverpage), submitted to the US Astro2010 Decadal Survey. This is a living document, with updates expected to be posted to this archive. Those interested in contributing should contact J. S. Bloom
title: Reconstruction of satellite images using partial convolutional neural networks
title: ÐÐ¾ÑÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¿ÑÑÐ½Ð¸ÐºÐ¾Ð²ÑÑ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ°ÑÑÐ¸ÑÐ½ÑÑ ÑÐ²ÐµÑÑÐ¾ÑÐ½ÑÑ Ð½ÐµÐ¹ÑÐ¾Ð½Ð½ÑÑ ÑÐµÑÐµÐ¹
Creators: name: Machuca Mendoza Cristian Rodrigo
name: Markov, Nikolai
name: "ÐÑÐµÐ´Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ° Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÑ  Ð³ÑÐ°Ð¶Ð´Ð°Ð½ Ð² Ð²ÑÐ·Ð°Ñ  Ð Ð¾ÑÑÐ¸Ð¸", Ð¼ÐµÐ¶Ð²ÑÐ·Ð¾Ð²ÑÐºÐ°Ñ Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¾Ð½Ð»Ð°Ð¹Ð½-ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (4; 2022; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2023
Subjects: ÐÐµÐ¹ÑÐ¾Ð½Ð½ÑÐµ ÑÐµÑÐ¸
ÐÐ·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ñ
inpainting
semantic segmentation
Ð·Ð°Ð´Ð°ÑÐ° Ð²Ð¾ÑÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð¸Ñ
ÑÐµÐ¼Ð°Ð½ÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐµÐ³Ð¼ÐµÐ½ÑÐ°ÑÐ¸Ñ

description: In the field of remote sensing, cloud removal from satellite imagery and reconstruction (inpainting) of areas under clouds remain as major challenges. This paper proposes a partial convolutional neural network-based algorithm for reconstructing multispectral satellite images with distant clouds. It is studied the performance of this neural network and the traditional U-Net neural network to solve the inpainting task.
description: Ð Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð´Ð¸ÑÑÐ°Ð½ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð·Ð¾Ð½Ð´Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐÐµÐ¼Ð»Ð¸ ÑÐ´Ð°Ð»ÐµÐ½Ð¸Ðµ Ð¾Ð±Ð»Ð°ÐºÐ¾Ð² ÑÐ¾ ÑÐ¿ÑÑÐ½Ð¸ÐºÐ¾Ð²ÑÑ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹ Ð¸ Ð²Ð¾ÑÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¾Ð±Ð»Ð°ÑÑÐµÐ¹ Ð¿Ð¾Ð´ Ð¾Ð±Ð»Ð°ÐºÐ°Ð¼Ð¸ ÑÐ²Ð»ÑÑÑÑÑ Ð°ÐºÑÑÐ°Ð»ÑÐ½ÑÐ¼Ð¸ Ð·Ð°Ð´Ð°ÑÐ°Ð¼Ð¸. Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ°ÑÑÐ¸ÑÐ½Ð¾Ð¹ ÑÐ²ÐµÑÑÐ¾ÑÐ½Ð¾Ð¹ Ð½ÐµÐ¹ÑÐ¾Ð½Ð½Ð¾Ð¹ ÑÐµÑÐ¸ Ð´Ð»Ñ Ð²Ð¾ÑÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð¼ÑÐ»ÑÑÐ¸ÑÐ¿ÐµÐºÑÑÐ°Ð»ÑÐ½ÑÑ ÑÐ¿ÑÑÐ½Ð¸ÐºÐ¾Ð²ÑÑ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹ Ñ ÑÐ´Ð°Ð»ÐµÐ½Ð½ÑÐ¼Ð¸ Ð¾Ð±Ð»Ð°ÐºÐ°Ð¼Ð¸. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð¹ Ð½ÐµÐ¹ÑÐ¾Ð½Ð½Ð¾Ð¹ ÑÐµÑÐ¸ Ð¸ ÑÑÐ°Ð´Ð¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐµÑÐ¸ U-Net Ð¿ÑÐ¸ ÑÐµÑÐµÐ½Ð¸Ð¸ Ð·Ð°Ð´Ð°ÑÐ¸ Ð²Ð¾ÑÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð¸Ñ.
Muscle and vascular remodelling in inflamed, fibrotic colon of patients with ulcerative colitis
Creators: name: Ippolito, Chiara
name: Segnani, Cristina
name: Dini, Sauro
name: Colucci, Rocchina
name: Fornai, Matteo
name: Errede, Mariella
name: Virgintino, Daniela
name: Buccianti, Piero
name: Chiarugi, Massimo
name: Dolfi, Amelio
name: Bernardini, Nunzia
Publisher: name: Italian Journal of Anatomy and Embryology
Year: 2015
Subjects: Ulcerative colitis; human; fibrosis; tunica muscularis; smooth muscle cells; vascular remodelling

description: Background. Intestinal fibrosis is a common complication of inflammatory bowel diseases, affecting patients with both Crohn’s disease and ulcerative colitis (UC). Of note, the progression of intestinal fibrosis has been recently considered to depend on distinct processes from those involved in inflammation [1]. In this context, angiogen- esis is currently regarded as a good candidate of active gut disease, closely related to fibrogenesis [2]. Therefore, studies on the multifactorial pathways promoting these processes are needed for understanding the pathophysiology of fibrosis, and there- by identifying anti-fibrogenic therapies. Aim. The present study was performed to evaluate the distribution of fibrotic tissue, the behaviour of smooth muscle cells and the presence of neovessels in the colon of UC patients. Patients and Methods. Full- thickness left colonic samples were studied, from patients with established and phar- macologically unresponsive UC for the following parameters: collagen and elastic fib- ers by histochemistry; fibrotic and profibrotic factors [type 1 and 3 collagens, elastin, fibronectin, vimentin, alpha-smooth muscle actin (α-SMA), proliferating nuclear anti- gen (PCNA), RhoA] by immunohistochemistry and western blot; vascular networks [CD31, CD105, nestin] by confocal microscopy immunofluorescence. Results. A sig- nificant increase in collagen fibers and decrease in elastin content were detected in the colon from UC patients as compared with controls. The increment of type 1 and 3 collagens, fibronectin, vimentin, PCNA and RhoA expression was associated with alpha-SMA decrease in the tunica muscularis of UC colon. A relevant rearrangement of vascular networks was observed in the fibrotic tunica muscularis, with neovessels displaying both proliferating CD105+ endothelial cells and activated nestin+ pericytes. Conclusion. The present data show that a significant muscle and vascular remodel- ling occurs in inflamed colonic tissues from UC patients, suggesting that, under these conditions, smooth muscle cells and vascular cells may be involved in fibrogenic pro- cesses by cell transition to mesenchymal phenotype.
description: Italian Journal of Anatomy and Embryology, Vol. 120, No. 1 (Supplement) 2015
Intraorbital arteries studied in pediatric age by high resolution superselective angiography
Creators: name: Bracco, Sandra
name: Venturi, Carlo
name: Leonini, Sara
name: Romano, Daniele
name: Cioni, Samuele
name: Vallone, Ignazio
name: Gennari, Paola
name: Galluzzi, Paolo
name: Bertelli, Eugenio
Publisher: name: Italian Journal of Anatomy and Embryology
Year: 2015
Subjects: Orbit; ophthalmic artery; angiography; angiographic incidence; visibility index

description: Angiography is a powerful tool to identify intraorbital arteries. However, the incidence by which these vessels can be identified is unknown. Our purpose was to determine such incidence and which angiographic approach is best for the identifica- tion of each artery. A retrospective study of 353 angiographic procedures (via oph- thalmic artery and/or external carotid artery) carried out on 79 children affected by intraocular retinoblastoma was made to investigate the arterial anatomy in 87 orbits. For each intraorbital artery two parameters were calculated: the angiographic inci- dence, as the percentage of times a given artery was identified, and the visibility index, as the ratio between the angiographic incidence and the true anatomic inci- dence. All collaterals of the ophthalmic artery could be spotted. Most of them were identified with a high angiographic incidence; some of them were less easily identi- fied because too thin or because frequently shielded. The visibility index paralleled the angiographic incidence of most arteries. However, the lacrimal and meningolac- rimal arteries had a higher visibility index suggesting that their identification was more frequent than the angiographic incidence alone could suggest. Statistical anal- ysis demonstrated that the lacrimal artery and some muscular branches had higher chances to be identified if the angiography of the ophthalmic artery was accompa- nied by the study of the external carotid system. This work provides an objective measure of how powerful angiography is to identify intraorbital arteries as well as useful references for professionals who need to operate in the orbit.
description: Italian Journal of Anatomy and Embryology, Vol. 120, No. 1 (Supplement) 2015
Inverse Problem of Cosmic-Ray Electron/Positron from Dark Matter
Creators: name: Hamaguchi, Koichi
name: Nakaji, Kouhei
name: Nakamura, Eita
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We discuss the possibility of solving the inverse problem of the cosmic-ray electron/positron from decaying/annihilating dark matter, and show simple analytic formulae to reconstruct the source spectrum of the electron/positron from the observed flux. We also illustrate our approach by applying the obtained formula to the just released Fermi data as well as the new HESS data.
description: 16 pages, 6 figures
Molinia caerulea
Creators: name: Cardona, Àngel Manuel Hernández
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Molinia
Molinia caerulea

description: Molinia caerulea (L.) Moench
(molínia, herba molinera). Natural de les zones temperades i fredes d’Europa, Àsia i nord d’Àfrica, i introduïda en altres parts del món. Creix en prats molls, herbassars higròfils, vores de rius, torrents i estanys, deus d’aigua i al peu de balços regalimosos. Ha estat referida del riu Ripoll i dels torrents de les Vendranes i de Rellinars (Pintó, 1994: 198), primeres citacions fetes a Sant Llorenç del Munt i l’Obac.
description: Published as part of Cardona, Àngel Manuel Hernández, 2022, Catàleg actualitzat i claus d'identificació de les gramínies de Sant Llorenç del Munt i l'Obac (Barcelona), pp. 64-86 in Nemus 12 on page 72, DOI: 10.5281/zenodo.12170499
Alcohol, gender and violence in Bougainville
Creators: name: Eves, Richard
Publisher: name: Canberra, ACT : Coral Bell School of Asia Pacific Affairs, College of Asia and the Pacific, The Australian National University
Year: 2016

description: This In Brief reports on research undertaken in Bougainville in October 2015 (Eves and Crawford 2014).1 Unlike previous studies, this research specifically explored the relationship between women’s economic empowerment and violence against women through in-depth qualitative interviews. Interviewees included business women in the urban context of Arawa (Kieta District) and rural women involved in informal marketing and alluvial mining (Panguna District) and in informal marketing and cocoa farming (Tinputz District).2 Preliminary analysis reveals a strong connection between men’s excessive alcohol consumption and violence against their intimate partners.
title: ÐÐ½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¾ÑÐµÐ½ÐºÐ° Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð² ÐµÐµ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾ÑÑÐ¸ÐºÐ¾Ð²Ð°, Ð¢Ð°ÑÑÑÐ½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ
Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÑ
Ð´ÐµÐ»Ð¾Ð²Ð°Ñ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ
Ð¿Ð»Ð°ÑÐµÐ¶ÐµÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ
ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÑ
financial condition
financial stability
liquidity
business activity

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÐºÐ¾ÑÑÑÐ¸ÑÐ¸ÐµÐ½ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð²ÑÐ±ÑÐ°Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÐµÐ³Ð¾ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ Ð¸ ÑÑÐ°Ð±Ð¸Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ. Ð ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð¾Ð±ÑÐµÐºÑÐ° Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²ÑÐ±ÑÐ°Ð½Ð° ÐÐ¾ÑÐ»Ð°ÑÑÐºÐ°Ñ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð°Ñ Ð´Ð¸ÑÑÐ°Ð½ÑÐ¸Ñ Ð¿Ð¾Ð³ÑÑÐ·Ð¾ÑÐ½Ð¾-ÑÐ°Ð·Ð³ÑÑÐ·Ð¾ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð¸ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¸Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹ ÐÐ¸ÑÐµÐºÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐµÑÐ¼Ð¸Ð½Ð°Ð»ÑÐ½Ð¾-ÑÐºÐ»Ð°Ð´ÑÐºÐ¸Ð¼ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ¾Ð¼ Ð¡ÐµÐ²ÐµÑÐ½Ð¾Ð¹ Ð¶ÐµÐ»ÐµÐ·Ð½Ð¾Ð¹ Ð´Ð¾ÑÐ¾Ð³Ð¸ - ÑÐ¸Ð»Ð¸Ð°Ð» ÐÐÐ Â«Ð ÐÐÂ». ÐÑÐµÐ´Ð¼ÐµÑ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð²ÑÐ±ÑÐ°Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð·Ð° 2013-2015 Ð³Ð¾Ð´Ñ.
description: This paper presents the theoretical foundations of the analysis of the financial condition of the organization, held coefficient analysis of the financial position of the selected companies on the basis of its financial statements and has developed a set of measures to improve and stabilize the financial situation.As the object of study selected Kotlas Mechanized handling operations and commercial operations of the Directorate for Management of Terminal and Warehouse Complex Northern Railway - branch of JSC "Russian Railways". The subject of this study - financial and economic activities of the selected companies for the years 2013-2015.
Variational anatomy of the orbitomeningeal foramen
Creators: name: Regoli, Marì
name: Macchi, Veronica
name: Bracco, Sandra
name: Morra, Aldo
name: Porzionato, Andrea
name: De Caro, Raffaele
name: Bertelli, Eugenio
Publisher: name: Italian Journal of Anatomy and Embryology
Year: 2015
Subjects: Orbit; orbitomeningeal foramen; angiography; computed tomography

description: In addition to the optic canal and the superior orbital fissure, orbits are connect- ed with the cranial cavity via inconstant canals including the orbitomeningeal fora- men. Though the orbitomeningeal foramen received considerable attention in the last twenty years, many of its anatomical details relevant for clinical practice still await to be defined.
Almost 1000 skulls and 50 computerized tomographies were examined to deter- mine incidence, number, length and caliber of the orbitomeningeal foramen as well as the topography of their orbital and cranial openings. A retrospective study of angi- ographies performed on more than 100 children was performed to look for arteries candidate for running through the orbitomeningeal foramen.
Orbitomeningeal foramens were detected in 59.5% of skulls and in 54% of indi- viduals by computerized tomography. Orbits with two to five foramina were found. Canals were classified as M-subtype or A-subtype depending on their cranial open- ing into the middle or the anterior cranial fossa. Large foramina, with the caliber ranging between 1 and 3 mm, were found in 12.2% of orbitomeningeal foramen- bearing orbits. By computed tomography the average caliber measured 1.2±0.3 mm and 1.5±0.5 mm (p<0.005) at the orbital and cranial openings respectively (p<0.005). Angiographies showed meningolacrimal and meningoophthalmic arteries, meningeal branches of the lacrimal and supraorbital arteries, and some unidentified arteries that could pass through the orbitomeningeal foramina.
Orbitomeningeal foramina are a common occurrence. When large they may house important arteries that can be the source of severe bleedings during deep dissection of the lateral wall of the orbit. Orbital surgeons should be aware of their existence.
description: Italian Journal of Anatomy and Embryology, Vol. 120, No. 1 (Supplement) 2015
Some reactions of alkyl iodides and perfluoroalkyl iodides with iodides of group V elements
Creators: name: Baig, Mirza Mohammed
Publisher: name: University of British Columbia
Year: 2012

description: The reaction of alkyl iodides with phenyl-iodo-arsines in the presence of mercury has been found to yield arsonium derivatives of triiodomercury (II). Extension of these reactions to other iodides of the Group V elements showed that when reacted with iodomethane and mercury, phosphorus triiodide gave the 1:1 complex of trimethylphosphine and mercuric iodide; antimony triiodide gave tetramethylstibonium triiodomercury (II); diiodophenylstibine reacted only to a limited extent; and bismuth triiodide gave an unstable product. Trifluoroiodomethane failed to react with the Group V iodides in the presence of mercury. Because of the possibility that 1:1 tertiary arsine mercuric iodide complexes are intermediates in the reactions which give rise to arsonium triiodomercury (II) derivatives, the reaction of these complexes with alkyl iodides was investigated. In all cases investigated using iodomethane, direct reaction occurred with the formation of arsonium triiodomercury (II) derivatives. Iodoethane, bromoethane and trifluoroiodomethane were found to react only to a slight extent, if at all, with tertiary arsine mercuric iodide complexes.
title: Comite permanent du droit des marques, des dessins et modeles industriels et des indications geographiques :
title: établi par le Bureau International.
titleType: Subtitle
Creators: name: (:Unas)
Publisher: name: Unknown
Year: 0

description: Le Comité permanent du droit des marques, des dessins et modèles industriels et des indications géographiques (ci-après dénommé “comité permanent”) a tenu sa première session à Genève du 13 au 17 juillet 1998.
Bulk high-Tc superconductors with drilled holes: how to arrange the holes to maximize the trapped magnetic flux ?
Creators: name: Lousberg, Gregory P
name: Ausloos, M
name: Vanderbemden, Ph
name: Vanderheyden, B
Publisher: name: arXiv
Year: 2008
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Drilling holes in a bulk high-Tc superconductor enhances the oxygen annealing and the heat exchange with the cooling liquid. However, drilling holes also reduces the amount of magnetic flux that can be trapped in the sample. In this paper, we use the Bean model to study the magnetization and the current line distribution in drilled samples, as a function of the hole positions. A single hole perturbs the critical current flow over an extended region that is bounded by a discontinuity line, where the direction of the current density changes abruptly. We demonstrate that the trapped magnetic flux is maximized if the center of each hole is positioned on one of the discontinuity lines produced by the neighbouring holes. For a cylindrical sample, we construct a polar triangular hole pattern that exploits this principle; in such a lattice, the trapped field is ~20% higher than in a squared lattice, for which the holes do not lie on discontinuity lines. This result indicates that one can simultaneously enhance the oxygen annealing, the heat transfer, and maximize the trapped field.
title: ÐÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ Ð¸ ÑÐ¸ÑÐºÐ¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸
title: Competitiveness and risks of construction company
Creators: name: ÐÐ¾Ð»Ð¸ÐºÐ¾Ð²Ð°, Ð®Ð»Ð¸Ñ
name: ÐÐµÑÐ½Ð¾ÑÐµÐºÐ¾Ð²Ð°, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
name: "Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸ÑÐºÐ°Ð¼Ð¸: Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸ ÑÐµÑÐµÐ½Ð¸Ñ (Ð ÐÐ¡ÐâÐ­â2022)", Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¼ ÑÑÐ°ÑÑÐ¸ÐµÐ¼ (8; 2022; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2022
Subjects: ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ
Ð½ÐµÐ¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½Ð¾ÑÑÑ
ÑÐ¸ÑÐºÐ¸
ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ
Ð¾ÑÐµÐ½ÐºÐ°
competitiveness
uncertainty
risks
classification
evaluation

description: Ð ÑÑÐ°ÑÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ Ðº Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¸ Ð¾ÑÐµÐ½ÐºÐµ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ñ ÑÑÐµÑÐ¾Ð¼ Ð¾ÑÑÐ°ÑÐ»ÐµÐ²Ð¾Ð¹ ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ¸, ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ ÑÐ¸ÑÐºÐ¾Ð² Ð¿Ð¾ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ Ðº Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÑ Ð²Ð¾Ð·Ð½Ð¸ÐºÐ½Ð¾Ð²ÐµÐ½Ð¸Ñ, Ð¸Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐµÑÑÑ, ÑÑÐµÐ¿ÐµÐ½Ñ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð½Ð° ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð¢Ð°ÐºÐ¸Ðµ ÐºÐ°ÑÐµÐ³Ð¾ÑÐ¸Ð¸, ÐºÐ°Ðº ÑÐ¸ÑÐº Ð¸ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ ÑÑÑÐµÑÑÐ²ÑÑÑ Ð½ÐµÑÐ°Ð·ÑÑÐ²Ð½Ð¾, Ð¿Ð¾ÑÑÐ¾Ð¼Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÑÑÐµÐ¹ Ð·Ð°Ð´Ð°ÑÐµÐ¹ Ð¿ÑÐ¸ Ð¿Ð¾ÑÑÐ°Ð½Ð¾Ð²ÐºÐµ ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐµÐ»ÐµÐ¹ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð²ÑÑÑÐ¿Ð°ÑÑÐµÐ³Ð¾ Ð² ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ½ÑÑ Ð±Ð¾ÑÑÐ±Ñ, ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸ÑÐºÐ°Ð¼Ð¸.
description: The article discusses approaches to determining and evaluating the competitiveness of a construction organization, taking into account industry specifics, the relevance of the chosen topic is indisputable in the conditions of the parallel growth of uncertainty and competition. The article considers the classification of risks in relation to the source of occurrence, their main features, and the degree of influence on the competitiveness of the enterprise. Such categories as risk and competitiveness exist inextricably; therefore, risk management is the defining task when setting strategic goals for any enterprise entering into a competitive struggle.
Aurore a ventaglio nella storia del Giappone
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2019

Un team interdisciplinare di fisici solari e umanisti giapponesi ha studiato le rappresentazioni iconografiche di un particolare tipo di aurore – a forma di ventaglio – in disegni e fotografie dal Settecento a oggi. I risultati sul Journal of Space Weather and Space Climate
Effects of the pesticide Lindane on granulosa cell ultrastructure
Creators: name: Palmerini, Maria Grazia
name: Zhurabekova, Gulmira
name: Balmagambetova, Aru
name: Miglietta, Selenia
name: Maiese, Maria Carmela
name: Bianchi, Serena
name: Cecconi, Sandra
name: Nottola, Stefania Annarita
name: Macchiarelli, Guido
Publisher: name: Italian Journal of Anatomy and Embryology
Year: 2015
Subjects: Lindane; sterility; granulosa cells; ultrastructure; mouse

description: The excessive exposure to pesticides in the Aral Sea area was correlated to the increased reproductive pathologies in those regions [1]. One of the principal chemical employed was the gamma-hexachlorocycloexane herbicide Lindane (L), a persistent organochlorine that may induces alterations in granulosa cell (GCs) survival [2, 3]. However, a comprehensive experimental study on the L-induced dose-effect morpho- logical alterations, has not yet addressed. Therefore, we studied by means of trans- mission and scanning electron microscopy, the morphological changes of mouse GCs, matured in vitro with increasing concentrations of L [4-6].
GCs showed several dose-dependent changes, in respect to controls. In particular, we observed significant reduction of GC microvilli and decrease of cytoplasmic pro- cesses between adjacent GCs. In addition, peripheral aggregation of chromatin under the nuclear membrane, extensive plasma membrane blebbing, abundant GC remnants and cellular debris were also present. Mitochondria, endoplasmic reticula and Golgi apparatuses did not show significant changes. In conclusion, our results showed a dose-dependent toxicity of L on GCs, associated to morphological signs of apoptosis. Alterations of GCs may be associated to impaired oocyte competence and sterility [7].
description: Italian Journal of Anatomy and Embryology, Vol. 120, No. 1 (Supplement) 2015
Concentrated growth factors (CGF): morphological and biochemical characterization
Creators: name: Bonazza, Veronica
name: Dellavia, Claudia
name: Labanca, Mauro
name: Merigo, Davide
name: Borsani, Elisa
Publisher: name: Italian Journal of Anatomy and Embryology
Year: 2015
Subjects: CGF; growth factors release; fibrin matrix; platelets; platelet concentrates

description: Concentrated growth factors (CGF) represents the novel generation of solid plate- let concentrate preparations (1-2). These 100% autologous preparations, obtained from a venous blood sample, not only enhance tissue healing but also improve the clinical outcomes of various surgical procedures, reducing complications like pain, inflammation and morbidity (3). Considering the few data on CGF morphology and its biological properties, the aim of this study was to analyse the CGF structure (blood cell localization and fibrin matrix architecture) and the in vitro cumulative release of seven growth factors (PDGF-AB, VEGF, TNF-α, TGF-β1, IGF-I, BDNF and BMP-2). CGF was obtained from volunteer donors using a specific protocol of cen- trifugation. Blood cell localization and fibrin architecture were evaluated after prop- erly staining and immunostaining protocols. The kinetics of the growth factor release were performed by incubation of the CGF in a free growth factors cell medium, at 37°C for 5 hours, 1, 3, 6, 7 and 8 days. After each incubation period, the medium was collected, centrifuged and stored at −80 °C until analysis. The total quantity of growth factors was checked using ELISA kits. After venous blood centrifugation, the CGF obtained consisted in three parts: the upper white part (PPP), the lower red part (RBC) and the middle “buffy coat” part (interface between white and red part). The results showed that platelets and leukocytes were localized in the buffy coat, where- as the erythrocytes were present only in the red part of CGF. Moreover, in the white part, the fibrin network and architecture changed moving far from the buffy coat becoming less compact. The in vitro cumulative release of growth factors revealed that each of them had a specific kinetic. Considering the mean value obtained for each time point from all volunteers, PDGF-AB, TGF-β1 and IGF-1 had a constant kinetic release, reaching the maximum accumulation at day 3rd and 6th respectively; VEGF and BMP-2 had a slow kinetic release, reaching the maximum accumulation at day 8th; TNF-α and BDNF had a fast kinetic release, reaching the maximum accumu- lation at day 1st and 3rd respectively. These findings support the clinical use of CGF and will allow us to better understand and improve the clinical outcomes.
description: Italian Journal of Anatomy and Embryology, Vol. 120, No. 1 (Supplement) 2015
Paspalum distichum
Creators: name: Cardona, Àngel Manuel Hernández
Publisher: name: Zenodo
Year: 2022
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Paspalum
Paspalum distichum

description: Paspalum distichum L.
(gram d’aigua). D’origen neotropical, es troba naturalitzat al sud d’Europa i en diverses altres zones temperades i càlides. Es fa vora l’aigua i en indrets embassats o molt humits. Es localitza principalment al riu Ripoll.
description: Published as part of Cardona, Àngel Manuel Hernández, 2022, Catàleg actualitzat i claus d'identificació de les gramínies de Sant Llorenç del Munt i l'Obac (Barcelona), pp. 64-86 in Nemus 12 on page 73, DOI: 10.5281/zenodo.12170499
Constraining Star Formation and AGN in z~2 Massive Galaxies using High Resolution MERLIN Radio Observations
Creators: name: Casey, Caitlin M.
name: Chapman, Scott C.
name: Muxlow, Tom W. B.
name: Beswick, Rob J.
name: Alexander, David M.
name: Conselice, Christopher J.
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: We present high spatial resolution MERLIN 1.4GHz radio observations of two high redshift (z~2) sources, RGJ123623 (HDF147) and RGJ123617 (HDF130), selected as the brightest radio sources from a sample of submillimetre-faint radio galaxies. They have starburst classifications from their rest-frame UV spectra. However, their radio morphologies are remarkably compact (<80mas and <65mas respectively), demanding that the radio luminosity be dominated by Active Galactic Nuclei (AGN) rather than starbursts. Near-IR imaging (HST NICMOS F160W) shows large scale sizes (R_(1/2)~0.75", diameters ~12kpc) and SED fitting to photometric points (optical through the mid-IR) reveals massive (~5x10^(11) M_sun), old (a few Gyr) stellar populations. Both sources have low flux densities at observed 24um and are undetected in observed 70um and 850um, suggesting a low mass of interstellar dust. They are also formally undetected in the ultra-deep 2Ms Chandra data, suggesting that any AGN activity is likely intrinsically weak. We suggest both galaxies have evolved stellar populations, low star formation rates, and low accretion rates onto massive black holes (10^(8.6) M_sun) whose radio luminosity is weakly beamed (by factors of a few). A cluster-like environment has been identified near HDF130 by an over-density of galaxies at z=1.99, reinforcing the claim that clusters lead to more rapid evolution in galaxy populations. These observations suggest that high-resolution radio (MERLIN) can be a superb diagnostic tool of AGN in the diverse galaxy populations at z~2.
description: 8 pages, 4 figures; accepted for publication in MNRAS
C’è un “pianeta proibito” nel deserto nettuniano
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2019

Il deserto nettuniano è una regione prossima alle stelle dove si ritiene che non si possano trovare pianeti con dimensioni pari a quelle di Nettuno. In questo caso, però, l'esopianeta Ngts-4b (simile a Nettuno, più grande della Terra e decisamente più caldo di Mercurio) si è fatto strada arrivando proprio lì dove non dovrebbe stare, conservando intatta la sua atmosfera gassosa
Tre regimi per ruotarle e incatenarle
Creators: Maura Sandri
Publisher: name: Media Inaf
Year: 2019

Analizzando i dati dei primi 22 mesi di osservazioni di Gaia, è stato possibile individuare nuove transizioni magnetiche in stelle nane di tipo spettrale avanzato. Tutti i dettagli di questo quadro sorprendente e inaspettato sono riportati su ApJ in uno studio guidato da ricercatori dell’Università e dell’Inaf di Catania
The fluorides of platinum and related compounds
Creators: name: Lohmann, Derek Harry
Publisher: name: University of British Columbia
Year: 2011

description: The fluorides of platinum have been reinvestigated. Attempts to prepare a difluoride were unsuccessful. It is suggested that this is-due to it being unstable towards disproportionation. X-ray Crystallographic evidence is presented as evidence for a trifluoride of platinum although a pure sample has not been isolated. This trifluoride is shown to be isostructural with the rhombohedital trifluorides of palladium, iridium and rhodium. Platinum tetrafluoride has been reinvestigated. It was found to be diamagnetic and to have a lattice of slightly-distorted, tetragonal uranium tetrachloride type. The adducts of platinum tetrafluoride with bromine trifluoride and selenium tetrafluoride were investigated further and found to be diamagnetic. The platinum tetrafluoride, selenium tetrafluoride adduct was shown to be isostructural with the corresponding palladium and germanium compounds. An ionic lattice is suggested for these compounds. Bromine trifluoride adducts do not form a similar-series and this, combined with their physical properties lead to the suggestion that these compounds are more covalent in nature. The previously unknown pentapositive state of platinum has been established. Platinum pentafluoride is a deep-red, reactive solid which readily disproportionates on heating. It gives rise to 1:1 adducts with iodine pentafluoride and chlorine trifluoride. These, like the bromine trifluoride adducts, are low-melting solids. Potassium fluoroplatinate (V) was prepared as a deep-yellow solid, crystallizing with the rhombohedral potassium fluorosmate lattice. A pentapositive oxyfluoride, platinum oxytrifluoride was found, it is suggested that this is polymeric. Platinum hexafluoride has been briefly investigated. A very reactive oxyfluoride, of formula PtO₂F₆, has been prepared and investigated. It is a deep-red solid which can be sublimed at 90° in a vacuum. It melts with decomposition at 219°. It is paramagnetic and crystallizes in a cubic lattice. Many of its chemical properties were studied. It is suggested that this compound is platinum peroxidehexafluoride. The crystal structures of the tetrafluorides of platinum rhodium, tin and lead were investigated. No similarity in structure was found. A brief investigation into the fluorides of rhodium has lead to the suggestion that a pentafluoride, in addition to a tetrafluoride, exists.
L’eclisse di Einstein
Creators: Stefano Giovanardi
Publisher: name: Media Inaf
Year: 2019

Con questo articolo dedicato all'eclisse di Sole che, esattamente un secolo fa – era il 29 maggio 1919 – fornì la prima prova sperimentale della Relatività generale, inauguriamo su Media Inaf una nuova rubrica mensile. A cura di Giangiacomo Gandolfi, Stefano Giovanardi e Gianluca Masi (Planetario e Museo Astronomico di Roma), ripercorrerà episodi in cui gli astri hanno davvero influenzato la storia dell’uomo
Indagine ai confini delle stelle di neutroni
Creators: Eliana Lacorte
Publisher: name: Media Inaf
Year: 2019

A governare le intense e improvvise emissioni di raggi X delle Supergiant Fast X-ray Transients sarebbe la magnetosfera della compagna più compatta del sistema binario. Lo suggerisce uno studio condotto da ricercatori dell’Inaf Iasf di Milano utilizzando il metodo dei “blocchi bayesiani”
Scuola di astronomia a Saint-Barthélemy
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2019

La Scuola estiva 2019 è un’occasione imperdibile di approfondimento sulle ultime novità in tema di astronomia, astrofisica, spazio e non solo, dalla viva voce dei protagonisti del campo, per ricordarci sempre, come recita un antico detto, di guardare la Luna e non il dito
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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°
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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¸Ð½ÑÐµÑÐ½ÐµÑ-Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³
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title: Ð ÐµÐ¼Ð°ÑÑÐµÑÐ¸Ð½Ð³ ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ ÑÐ°Ð¹ÑÐ° ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐÐÐ Â«Ð¡Ð°Ð½ÑÐ°ÑÐ°Â»
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
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Creators: name: ÐÑÐ´Ð°ÐºÐ¾Ð², ÐÑÑÐµÑÐ»Ð°Ð²
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
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