cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Treatment of the Intrinsic Hamiltonian in Particle-Number Nonconserving Theories
Creators: name: Hergert, H.
name: Roth, R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We discuss the implications of using an intrinsic Hamiltonian in theories without particle-number conservation, e.g., the Hartree-Fock-Bogoliubov approximation, where the Hamiltonian's particle-number dependence leads to discrepancies if one naively replaces the particle-number operator by its expectation value. We develop a systematic expansion that fixes this problem and leads to an a posteriori justification of the widely-used one- plus two-body form of the intrinsic kinetic energy in nuclear self-consistent field methods. The expansion's convergence properties as well as its practical applications are discussed for several sample nuclei.
description: 6 pages, 5 figures
Padme all’inseguimento del fotone oscuro
Creators: Ufficio Comunicazione Infn
Publisher: name: Media Inaf
Year: 2018

«Padme entrerà in presa dati nelle prossime settimane e si metterà subito a caccia del fotone oscuro, una particella simile al fotone ordinario», spiega il ricercatore dell’Infn Paolo Valente, «ma contraddistinto dal fatto di avere una piccola massa». Importanti anche i risvolti tecnologici e industriali
Pulse width controlled resistivity switching at room temperature in Bi0.8Sr0.2MnO3
Creators: name: Rebello, A.
name: Mahendiran, R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We report pulsed as well as direct current/voltage induced electroresistance in Bi0.8Sr0.2MnO3 at room temperature. It is shown that bi-level and multi-level resistivity switching can be induced by a sequence of pulses of varying pulse width at fixed voltage amplitude. Resistivity increases abruptly (= 55 % at 300 K) upon reducing pulse width from 100 ms to 25 ms for a fixed electric field (E = 2 V/cm2) of 200 ms pulse period. The resistivity switching is accompanied by a periodic change in temperature which alone can not explain the magnitude of the resistivity change.
description: 12 pages, 3 figures
Voglio una stella spericolata
Creators: Maura Sandri
Publisher: name: Media Inaf
Year: 2018

Il telescopio spaziale Hubble ha immortalato l'enigmatica nebulosa Iras 05437+2502, una piccola regione di formazione stellare che sembrerebbe nascondere una storia drammatica. L'arco luminoso evidente nell'immagine potrebbe essere stato creato dall’interazione di una giovane stella spericolata con la nube di gas e polvere, mentre la sta attraversando
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÐ½ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾Ð² Ð´Ð»Ñ ÐÐÐ Â«Ð¡Ð¸ÑÑÐµÐ¼Ð°Â»
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¯ÑÐµÐ½ÐºÐ¾, 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: 2017
Subjects: Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³
ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¸Ñ
Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸
ÑÐµÐ½Ð¾Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«Ð¡Ð¸ÑÑÐµÐ¼Ð°Â». Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ ÑÐµÐ½ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾Ð² Ð² ÑÐµÐ³Ð¼ÐµÐ½ÑÐµ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð³ÑÐ°Ð¶Ð´Ð°Ð½ÑÐºÐ¾Ð³Ð¾ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð°, Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ Ð´Ð°Ð½Ð½ÑÑ Ð¸ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ðµ Ð¼ÐµÑ Ð¿Ð¾ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð¾ÑÐ½Ð¾ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾ Ð´ÑÑÐ³Ð¸Ñ Ð¿Ð¾ÑÑÐ°Ð²ÑÐ¸ÐºÐ¾Ð² Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð². ÐÑÑÐ²Ð»ÐµÐ½Ð¾, ÑÑÐ¾ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐ¼Ð¸ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ½ÑÐ¼Ð¸ ÑÐ°ÐºÑÐ¾ÑÐ°Ð¼Ð¸, ÑÑÐµÐ±ÑÑÑÐ¸Ð¼Ð¸ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ, ÑÐ²Ð»ÑÑÑÑÑ ÑÑÐ¾Ð²ÐµÐ½Ñ ÑÐµÐ½ Ð¸ ÑÑÐ¾ÐºÐ¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° Ð³Ð¾ÑÐ¾Ð²ÑÑ Ð¸Ð·Ð´ÐµÐ»Ð¸Ð¹. Ð ÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¼ÐµÑ Ð¿Ð¾ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÑ Ðº Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐ¾Ð¹ Ð¿ÑÐ¸Ð±ÑÐ»Ð¸ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸.
A Flaring X-ray Source with an Halpha-bright Counterpart toward the SMC
Creators: name: Laycock, Silas
name: Drake, Jeremy J.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the discovery of a flaring X-ray source with an optical counterpart with Halpha emission and red-excess, in the direction of the SMC. A 100 ksec X-ray observation with Chandra detected a flare lasting 6 ksec in the source CXO J005428.9-723107. The X-ray spectrum during the flare was consistent with a thermal plasma of temperature kT=2.5 keV. In quiescence following the flare the spectrum was softer (kT= 0.4 keV). Timing analysis did not reveal any significant periodicities or QPOs. Optical images taken with the Magellan-Baade 6.5m telescope show a single star in the (0.9") error circle. This star has apparent magnitude V=19.17, exhibits enhanced Halpha emission (Halpha - r = -0.88), and has a large proper motion. Alternative explanations are explored, leading to identification as a relatively nearby (Galactic) coronally active star of the BY Draconis class.
description: 7 pages, 5 figures, submitted to ApJ
title: ÐÐ¾ÑÑÐºÐ¸Ðµ Ð³Ð¸Ð´ÑÐ¾ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð½Ð° ÐÐ°ÑÐµÐ½ÑÐµÐ²Ð¾Ð¼ Ð¼Ð¾ÑÐµ Ð² ÑÐ°Ð¹Ð¾Ð½Ðµ ÐÑÑÐ¼Ð°Ð½ÑÐºÐ°
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ»ÑÐ¸Ð½, ÐÐµÐ¾ÑÐ³Ð¸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: Ð¾Ð³ÑÐ°Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾Ðµ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ðµ
Ð¿ÑÐ¸ÑÐ°Ð»ÑÐ½Ð¾Ðµ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ðµ
Ð¼Ð¾Ð»
Ð²ÑÑÐ¾ÐºÐ¸Ð¹ ÑÐ²Ð°Ð¹Ð½ÑÐ¹ ÑÐ¾ÑÑÐ²ÐµÑÐº
Ð¿ÐµÑÐµÐ´Ð½Ð¸Ð¹ Ð½Ðµ Ð½ÐµÑÑÑÐ¸Ð¹ ÑÐ¿ÑÐ½Ñ

description: Ð Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ Ð¾Ð³ÑÐ°Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾Ðµ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ðµ Ð¸Ð· Ð¼Ð°ÑÑÐ¸Ð²Ð¾Ð²-Ð³Ð¸Ð³Ð°Ð½ÑÐ¾Ð²; Ð¿ÑÐ¸ÑÐ°Ð»ÑÐ½Ð¾Ðµ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ðµ Ñ Ð²ÑÑÐ¾ÐºÐ¸Ð¼ ÑÐ²Ð°Ð¹Ð½ÑÐ¼ ÑÐ¾ÑÑÐ²ÐµÑÐºÐ¾Ð¼ Ð¸ Ð½ÐµÑÑÑÐµÐ¹ Ð¿ÐµÑÐµÐ´Ð½ÐµÐ¹ ÑÐ¿ÑÐ½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÐµÐ½ÐºÐ¾Ð¹; Ð»ÐµÐ´Ð¾Ð²ÑÐµ Ð½Ð°Ð³ÑÑÐ·ÐºÐ¸ Ð½Ð° ÑÐ²Ð°Ð¸.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ Ð²Ð·ÑÑÐºÐ°Ð½Ð¸Ñ Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð² Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸, ÑÐ¿ÑÐ°Ð²Ð»ÑÑÑÐµÐ¹ Ð¶Ð¸Ð»ÑÐ¼ Ð¼Ð½Ð¾Ð³Ð¾ÐºÐ²Ð°ÑÑÐ¸ÑÐ½ÑÐ¼ ÑÐ¾Ð½Ð´Ð¾Ð¼ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ "Ð¡ÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ")
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ½Ð´ÑÐ¸Ð°Ð½Ð¾Ð²Ð°, ÐÐ¸ÐºÑÐ¾ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð±ÑÑ Ð³Ð°Ð»ÑÐµÑÑÐºÐ¾Ð³Ð¾ ÑÑÐµÑÐ°
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð·
Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ°Ñ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÑ
Ð¶Ð¸Ð»Ð¸ÑÐ½Ð¾-ÐºÐ¾Ð¼Ð¼ÑÐ½Ð°Ð»ÑÐ½ÑÐµ ÑÑÐ»ÑÐ³Ð¸

description: ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - ÐÐÐ Â«Ð¡ÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÐ¸ÑÑÐµÐ¼ÑÂ», Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ, Ð¾ÑÑÑÐµÑÑÐ²Ð»ÑÑÑÐ°Ñ ÑÐ²Ð¾Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð² Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ðµ. ÐÐ°Ð½Ð¸Ð¼Ð°ÐµÑÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼ Ð¶Ð¸Ð»ÑÐ¼ Ð¼Ð½Ð¾Ð³Ð¾ÐºÐ²Ð°ÑÑÐ¸ÑÐ½ÑÐ¼ ÑÐ¾Ð½Ð´Ð¾Ð¼. Ð¦ÐµÐ»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°ÑÑ Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÑÑ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÑ Ð² Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð²Ð·ÑÑÐºÐ°Ð½Ð¸Ñ Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÐ¸. ÐÐ½Ð°Ð»Ð¸Ð· Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð²ÑÑÐ²Ð¸Ð», ÑÑÐ¾ Ð² ÑÐ²ÑÐ·Ð¸ Ñ Ð½ÐµÐ¾Ð¿Ð»Ð°ÑÐµÐ½Ð½Ð¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¿Ð¾ Ð¶Ð¸Ð»Ð¸ÑÐ½Ð¾-ÐºÐ¾Ð¼Ð¼ÑÐ½Ð°Ð»ÑÐ½ÑÐ¼ ÑÑÐ»ÑÐ³Ð°Ð¼ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ Ð²Ð¾Ð·ÑÐ°ÑÑÐ°ÐµÑ ÐºÑÐµÐ´Ð¸ÑÐ¾ÑÑÐºÐ°Ñ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÑ. ÐÐ¾ Ð¸ÑÐ¾Ð³Ð°Ð¼ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð¸ Ð²Ð½ÐµÑÐµÐ½Ñ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð²Ð·ÑÑÐºÐ°Ð½Ð¸Ñ Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÐ¸.
BepiColombo corre inesorabile verso il lancio
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2018

I due orbiter scientifici della missione congiunta Esa-Jaxa per lo studio di Mercurio sono stati collegati nella loro configurazione di lancio, ed è stato dato il via libera per il rifornimento di propellente. La prima finestra di lancio è in calendario per le 3:45 del 19 ottobre
Additional file 1 of Immunoprofiling of early, untreated rheumatoid arthritis using mass cytometry reveals an activated basophil subset inversely linked to ACPA status
Creators: name: Koppejan, H.
name: Hameetman, M.
name: Beyrend, G.
name: van Unen, V.
name: Kwekkeboom, J. C.
name: van der Helm-van Mil, A. H.
name: Toes, R. E. M.
name: van Gaalen, F. A.
Publisher: name: figshare
Year: 2021
Subjects: subject: Immunology
subject: FOS: Clinical medicine

description: Additional file 1: Supplementary Table 1: Antibodies used for Mass Cytometry. * in-house conjugated at 100μg scale using a Maxpar© X8 antibody labeling kit (Fluidigm)
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÑÐµÐ¶Ð½Ð°Ñ, ÐÐ½Ð½Ð°
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: Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÑÑÐ´Ð° ÑÑÐºÐ¾Ð²Ð¾Ð´Ð¸ÑÐµÐ»Ñ
ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¸Ð¹ ÑÑÑÐ´
Ð¾ÑÐµÐ½ÐºÐ° Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°
Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ°Ð±Ð¾ÑÑ ÑÑÐºÐ¾Ð²Ð¾Ð´Ð¸ÑÐµÐ»Ñ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«ÐÐ¸ÑÐ¸ÑÐ¸Ð°Ð²ÑÐ¾ÐºÐ¾Ð¼Ð¿Â». Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ Ð² ÐÐÐ Â«ÐÐ¸ÑÐ¸ÑÐ¸Ð°Ð²ÑÐ¾ÐºÐ¾Ð¼Ð¿Â». ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÐºÐ¸ÑÐ¸ÑÑÐºÐ¾Ð¹ Ð°Ð²ÑÐ¾ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐÐÐ Â«ÐÐ¸ÑÐ¸ÑÐ¸Ð°Ð²ÑÐ¾ÐºÐ¾Ð¼Ð¿Â» Ð²ÑÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÑ Ð´Ð»Ñ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸. Ð¡Ð´ÐµÐ»Ð°Ð½ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð· Ð²ÑÑÑÑÐºÐ¸ Ð¸ Ð·Ð°ÑÑÐ°Ñ Ð¾Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¼ÐµÑ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸. Ð ÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¼ÐµÑ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÑ Ðº Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐ¾Ð¹ Ð¿ÑÐ¸Ð±ÑÐ»Ð¸ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸.
title: ÐÑÑÐ¾ÑÐ¸Ñ ÐºÐ¾ÑÐ°Ð±Ð»ÐµÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐºÐ¾Ð»Ñ Ð² ÐÐ¾Ð»Ð¸ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¾Ð¼
Creators: name: Ð¡Ð¼ÐµÐ»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: 2005
Subjects: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ
Ð¡ÑÐ´Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ðµ

description: Ð ÐºÐ½Ð¸Ð³Ðµ ÑÐ°ÑÑÐºÐ°Ð·Ð°Ð½Ð¾ Ð¾ ÐºÐ¾ÑÐ°Ð±Ð»ÐµÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¼ Ð¾ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ð¸ (ÑÐ°ÐºÑÐ»ÑÑÐµÑÐµ) Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸Ð½ÑÑÐ¸ÑÑÑÐ° â Ð¿ÐµÑÐ²Ð¾Ð¹ Ð² Ð Ð¾ÑÑÐ¸Ð¸ Ð²ÑÑÑÐµÐ¹ ÑÐºÐ¾Ð»Ðµ Ð³ÑÐ°Ð¶Ð´Ð°Ð½ÑÐºÐ¾Ð³Ð¾ ÑÑÐ´Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¸ Ð¾Ð´Ð½Ð¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾ Ð¿ÐµÑÐ²Ð¾Ð¹ Ð²ÑÑÑÐµÐ¹ Ð°Ð²Ð¸Ð°ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐºÐ¾Ð»Ðµ, Ð½Ð° Ð±Ð°Ð·Ðµ ÐºÐ¾ÑÐ¾ÑÑÑ Ð² 1930 Ð³Ð¾Ð´Ñ Ð±ÑÐ»Ð¸ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ñ ÐÐ¾ÑÐ°Ð±Ð»ÐµÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð¸Ð½ÑÑÐ¸ÑÑÑ Ð² ÐÐµÐ½Ð¸Ð½Ð³ÑÐ°Ð´Ðµ Ð¸ ÐÐ²Ð¸Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¸Ð½ÑÑÐ¸ÑÑÑ Ð² ÐÐ¾ÑÐºÐ²Ðµ. ÐÐ½Ð¸Ð³Ð° Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ð° Ð½Ð° Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð¾ÑÐ½Ð¾Ð²Ðµ. ÐÑÐ¾Ð±Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ Ð¸ÑÑÐ¾ÑÐ¸Ð¸ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸Ñ Ð¾ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ñ. ÐÑÐµÐ½ÐµÐ½ Ð²ÐºÐ»Ð°Ð´ ÐºÐ¾ÑÐ°Ð±ÐµÐ»Ð¾Ð² Ð¸Ð· ÐÐ¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸Ð½ÑÑÐ¸ÑÑÑÐ° Ð² ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ðµ Ð½Ð°Ð´Ð²Ð¾Ð´Ð½ÑÑ, Ð¿Ð¾Ð´Ð²Ð¾Ð´Ð½ÑÑ Ð¸ Ð²Ð¾Ð·Ð´ÑÑÐ½ÑÑ ÐºÐ¾ÑÐ°Ð±Ð»ÐµÐ¹. ÐÐ»Ñ Ð²ÑÐµÑ Ð¸Ð½ÑÐµÑÐµÑÑÑÑÐ¸ÑÑÑ Ð¸ÑÑÐ¾ÑÐ¸ÐµÐ¹ Ð½ÑÐ½ÐµÑÐ½Ð¸Ñ Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½ÑÑ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸ ÐÐ¾ÑÑÐºÐ¾Ð³Ð¾ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ¾Ð² Ð¸, Ð²Ð¾Ð¾Ð±ÑÐµ, Ð¾ÑÐµÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð²ÑÑÑÐµÐ¹ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐºÐ¾Ð»Ñ
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Statistical properties of spectral fluctuations for a quantum system with infinitely many components
Creators: name: Makino, H.
name: Minami, N.
name: Tasaki, S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Physical sciences

description: Extending the idea formulated in Makino {\it{et al}}[Phys.Rev.E {\bf{67}},066205], that is based on the Berry--Robnik approach [M.V. Berry and M. Robnik, J. Phys. A {\bf{17}}, 2413], we investigate the statistical properties of a two-point spectral correlation for a classically integrable quantum system. The eigenenergy sequence of this system is regarded as a superposition of infinitely many independent components in the semiclassical limit. We derive the level number variance (LNV) in the limit of infinitely many components and discuss its deviations from Poisson statistics. The slope of the limiting LNV is found to be larger than that of Poisson statistics when the individual components have a certain accumulation. This property agrees with the result from the semiclassical periodic-orbit theory that is applied to a system with degenerate torus actions[D. Biswas, M.Azam,and S.V.Lawande, Phys. Rev. A {\bf 43}, 5694].
description: 6 figures, 10 pages
Nubi d’acqua nella Grande macchia rossa
Creators: Sara Venturi
Publisher: name: Media Inaf
Year: 2018

Un nuovo studio condotto da un team di ricerca del Goddard Space Flight Center della Nasa, analizzando dalle Hawaii l’emissione infrarossa nell'area della grande tempesta gioviana, ha condotto a importanti passi avanti nella stima della quantità di acqua presente sul gigante gassoso. I risultati su The Astronomical Journal.
title: ÐÐ°ÑÐ¸Ð°Ð½ÑÑ ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½ÑÑ Ð·Ð°Ð´Ð°Ñ Ð¿Ð¾ ÑÐµÐ¾ÑÐ¸Ð¸ Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÐµÐ¹
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¼Ð¾ÑÐ¾Ð²Ð°, ÐÐ°ÑÐ°Ð»Ð¸Ñ
name: ÐÐ°Ð½ÑÐ¸Ð»Ð¾Ð²Ð°, ÐÐ°Ð´ÐµÐ¶Ð´Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2020
Subjects: ÐÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÐµÐ¹ ÑÐµÐ¾ÑÐ¸Ñ
ÐÑÐ°ÑÑÐ¾Ð½Ð° ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ
ÐÐµÑÐ½ÑÐ»Ð»Ð¸ ÑÐ¸ÑÐ»Ð°
Ð¡Ð»ÑÑÐ°Ð¹Ð½ÑÐµ Ð²ÐµÐ»Ð¸ÑÐ¸Ð½Ñ

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ 30 Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ¾Ð² ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½ÑÑ Ð·Ð°Ð´Ð°Ñ (Ð¿Ð¾ 14 Ð·Ð°Ð´Ð°Ñ Ð² ÐºÐ°Ð¶Ð´Ð¾Ð¼ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐµ) Ð¿Ð¾ ÑÐµÐ¾ÑÐ¸Ð¸ Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÐµÐ¹, Ð¸Ð·ÑÑÐ°ÐµÐ¼Ð¾Ð¹ Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«ÐÑÑÑÐ°Ñ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ°Â». Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð²ÐºÐ»ÑÑÐµÐ½Ñ Ð·Ð°Ð´Ð°ÑÐ¸, Ð¾ÑÐ½Ð¾ÑÑÑÐ¸ÐµÑÑ Ðº Ð±Ð°Ð·Ð¾Ð²ÑÐ¼ ÑÐ°Ð·Ð´ÐµÐ»Ð°Ð¼ ÑÐµÐ¾ÑÐ¸Ð¸ Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÐµÐ¹, ÑÐ°ÐºÐ¸Ð¼ ÐºÐ°Ðº ÐºÐ»Ð°ÑÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¸ Ð³ÐµÐ¾Ð¼ÐµÑÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÐ¸, ÑÐµÐ¾ÑÐµÐ¼Ñ ÑÐ»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¸ ÑÐ¼Ð½Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÐµÐ¹, ÑÐ¾ÑÐ¼ÑÐ»Ñ Ð¿Ð¾Ð»Ð½Ð¾Ð¹ Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÐ¸ Ð¸ ÐÐ°Ð¹ÐµÑÐ°, ÑÑÐµÐ¼Ð° ÐÐµÑÐ½ÑÐ»Ð»Ð¸ Ð¸ Ð¿ÑÐ¸Ð±Ð»Ð¸Ð¶ÐµÐ½Ð½Ð°Ñ ÑÐ¾ÑÐ¼ÑÐ»Ñ ÐÑÐ°ÑÑÐ¾Ð½Ð°, Ð¾Ð´Ð½Ð¾Ð¼ÐµÑÐ½ÑÐµ (Ð´Ð¸ÑÐºÑÐµÑÐ½ÑÐµ Ð¸ Ð½ÐµÐ¿ÑÐµÑÑÐ²Ð½ÑÐµ) ÑÐ»ÑÑÐ°Ð¹Ð½ÑÐµ Ð²ÐµÐ»Ð¸ÑÐ¸Ð½Ñ, Ð½Ð¾ÑÐ¼Ð°Ð»ÑÐ½ÑÐ¹ Ð·Ð°ÐºÐ¾Ð½ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ, ÑÑÐ½ÐºÑÐ¸Ð¸ ÑÐ»ÑÑÐ°Ð¹Ð½ÑÑ Ð²ÐµÐ»Ð¸ÑÐ¸Ð½, Ð´Ð²ÑÐ¼ÐµÑÐ½Ð°Ñ Ð´Ð¸ÑÐºÑÐµÑÐ½Ð°Ñ ÑÐ»ÑÑÐ°Ð¹Ð½Ð°Ñ Ð²ÐµÐ»Ð¸ÑÐ¸Ð½Ð°.
 ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¿ÑÐ¸Ð¼ÐµÑÑ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð·Ð°Ð´Ð°Ñ.
Ð¡ÑÑÑÐºÑÑÑÐ° Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ¾Ð² Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÑ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð´Ð»Ñ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð·Ð½Ð°Ð½Ð¸Ð¹ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÐºÐ°Ðº Ð² ÑÐ¾ÑÐ¼Ðµ Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½ÑÑ Ð´Ð¾Ð¼Ð°ÑÐ½Ð¸Ñ Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹, ÑÐ°Ðº Ð¸ Ð² ÑÐ¾ÑÐ¼Ðµ ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð¸ ÑÐµÑÑÐ¾Ð².
 Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½ÑÐ¼ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ°Ð¼Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð°Ð¼ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¤ÐÐÐÐ£ÐÐ Â«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¸ÐºÐ¾Ð³Ð¾Â» Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² Ð¸ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸Ð½ÑÑÐ¸ÑÑÑÐ¾Ð².
Aurora boreale su Saturno
Creators: Matteo Boni
Publisher: name: Media Inaf
Year: 2018

Osservazioni nell'ultravioletto realizzate dal telescopio spaziale Hubble, fatte nel 2017 nei periodi precedente e successivo il solstizio estivo dell'emisfero nord di Saturno, hanno permesso agli astronomi di conoscere meglio la magnetosfera del Signore degli Anelli. Questo grazie anche alla coordinazione delle osservazioni di Hubble con il Gran Finale della missione Cassini, durante il quale la sonda spaziale ha scandagliato le regioni aurorali di Saturno
title: Ð¯Ð·ÑÐº Ð´ÐµÐ»Ð¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÐ½Ð¸Ñ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¾Ð»Ð¾ÑÐ¸Ð½Ð¾Ð²Ð°, ÐÐ½Ð°ÑÑÐ°ÑÐ¸Ñ
name: ÐÐ¾Ð»Ð¾ÑÐ¸Ð½Ð¾Ð²Ð°, Ð¢Ð°ÑÑÑÐ½Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2017
Subjects: ÑÑÑÑÐºÐ¸Ð¹ ÑÐ·ÑÐº
Ð´ÐµÐ»Ð¾Ð²Ð¾Ðµ Ð¾Ð±ÑÐµÐ½Ð¸Ðµ
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ "Ð¯Ð·ÑÐº Ð´ÐµÐ»Ð¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÐ½Ð¸Ñ" Ð¸ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¾ Ð½Ð° ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð²Ð½ÑÑ ÐºÐ¾Ð¼Ð¿ÐµÑÐµÐ½ÑÐ¸Ð¹. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¾ Ð½Ð° ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ, ÑÐ¸Ð·Ð¸ÐºÐ¾-Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ñ, ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸ Ð³ÑÐ¼Ð°Ð½Ð¸ÑÐ°ÑÐ½ÑÑ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹. ÐÐ¾Ð¶ÐµÑ Ð±ÑÑÑ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð¾Ð²Ð°Ð½Ð¾ ÑÐ°ÐºÐ¶Ðµ ÑÐ¸ÑÐ¾ÐºÐ¾Ð¼Ñ ÐºÑÑÐ³Ñ Ð·Ð°Ð¸Ð½ÑÐµÑÐµÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÑÐ¸ÑÐ°ÑÐµÐ»ÐµÐ¹.
Additional file 2 of Immunoprofiling of early, untreated rheumatoid arthritis using mass cytometry reveals an activated basophil subset inversely linked to ACPA status
Creators: name: Koppejan, H.
name: Hameetman, M.
name: Beyrend, G.
name: van Unen, V.
name: Kwekkeboom, J. C.
name: van der Helm-van Mil, A. H.
name: Toes, R. E. M.
name: van Gaalen, F. A.
Publisher: name: figshare
Year: 2021
Subjects: subject: Immunology
subject: FOS: Clinical medicine

description: Additional file 2: Supplementary Table 2: Antibodies used for Flow Cytometry. Antibodies used in FC experiments to investigate frequencies Cluster 18 (panel 1) and Cluster 24 (panel 2) identified by MC.
title: ÐÐ¸Ð¾Ð¼Ð¾Ð»ÐµÐºÑÐ»ÑÑÐ½Ð°Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ°. ÐÐ²ÐµÐ´ÐµÐ½Ð¸Ðµ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÑÑÐ¸Ñ ÑÑÐµÐ±Ð½ÑÑ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹, Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ñ ÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² Â«Ð¢ÐµÑ Ð½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°Â»
titleType: Subtitle
Creators: name: ÐÐµÐ»Ð¸ÑÐºÐ¾, ÐÐ»ÐµÐ½Ð°
name: Ð¦ÑÐ±Ð¸Ð½, ÐÐ»ÐµÐ³
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2011
Subjects: Ð­Ð»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ°
ÐÐ°Ð½Ð¾ÑÑÑÑÐºÑÑÑÐ½ÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ
Ð±Ð¸Ð¾Ð¼Ð¾Ð»ÐµÐºÑÐ»ÑÑÐ½Ð°Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ°
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ¸Ð·Ð¸ÐºÐ¾-ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ¸; Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ñ, ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ Ð¸ ÑÑÑÐ½Ð¾ÑÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ð¾Ð± Ð¾Ð±ÑÐµÐºÑÐ°Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð² Ð±Ð¸Ð¾Ð¼Ð¾Ð»ÐµÐºÑÐ»ÑÑÐ½Ð¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐµ; ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾-ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð±Ð¸Ð¾Ð¼Ð¾Ð»ÐµÐºÑÐ» Ð¸ Ð¼Ð¾Ð»ÐµÐºÑÐ»ÑÑÐ½ÑÑ ÑÐ¸ÑÑÐµÐ¼. ÐÐ·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð±Ð°Ð·Ð¾Ð²ÑÐµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð±Ð¸Ð¾Ð¼Ð¾Ð»ÐµÐºÑÐ»ÑÑÐ½Ð¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ¸, Ð¾Ð±Ð¾Ð±ÑÐµÐ½Ð½ÑÐ¹ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸Ð¼ÐµÑÑÐ¸ÑÑÑ Ð½Ð°ÑÑÐ½Ð¾-ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð² Ð±Ð¸Ð¾Ð¼Ð¾Ð»ÐµÐºÑÐ»ÑÑÐ½Ð¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐµ Ð¸ Ð¸Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÐ¹ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð».
ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÐ·Ð¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¸Ð¼ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð°Ð¼ Â«Ð¤Ð¸Ð·Ð¸ÐºÐ° Ð±Ð¸Ð¾Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð¸ ÑÐ¸ÑÑÐµÐ¼Â» Ð¸ Â«Ð¤Ð¸Ð·Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ°Â» Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² Â«Ð¢ÐµÑÐ½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°Â». ÐÐ¾Ð¶ÐµÑ Ð±ÑÑÑ ÑÐ°ÐºÐ¶Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð¿ÑÐ¸ Ð¾Ð±ÑÑÐµÐ½Ð¸Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Â«Ð­Ð»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ° Ð¸ Ð½Ð°Ð½Ð¾ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ°Â», Â«Ð¤Ð¸Ð·Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ°Â» Ð¸ Ð² ÑÐ¸ÑÑÐµÐ¼Ð°Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Proton magnetic resonance in paramagnetic and antiferromagnetic single crystals of CoCl₂.6H₂O
Creators: name: Sawatzky, Erich
Publisher: name: University of British Columbia
Year: 2012

description: Standard radio-frequency nuclear resonance spectroscopy techniques have been applied to study the fine structure of the proton magnetic resonance absorption line in single crystals of CoCl₂.6H₂O. Cobaltous Chloride is a paramagnetic crystal at high temperatures and becomes antiferromagnetic at about 2.29°K. The position and number of lines strongly depend on temperature and on the direction of the externally applied magnetic field. Fewer lines than the theoretical number of twenty-four were always observed. At room temperature the proton resonance at 12 Mc/sec. in a field of 2.82 K gauss consists of a single line about six gauss wide. A splitting of this line into a maximum of six components has been observed at liquid helium temperature. The maximum overall separation at 4.2°K is about 110 gauss. For each direction of the externally applied magnetic field the separation between the lines increases with decreasing temperature. The transition temperature is measured and effects due to short-range order above the transition are observed. Theoretical formulae for the positions of the component lines are developed by considering the two-proton spin system within a water molecule of hydration immersed in the homogeneous external field [formula omitted] H and the inhomogeneous time- averaged field of the cobalt ions. Measurements in the antiferromagnetic state have been partially completed.
Testing the Epeak - Eiso relation for GRBs detected by Swift and Suzaku-WAM
Creators: name: Krimm, H. A.
name: Yamaoka, K.
name: Sugita, S.
name: Ohno, M.
name: Sakamoto, T.
name: Barthelmy, S. D.
name: Gehrels, N.
name: Hara, R.
name: Norris, J. P.
name: Ohmori, N.
name: Onda, K.
name: Sato, G.
name: Tanaka, H.
name: Tashiro, M.
name: Yamauchi, M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: One of the most prominent, yet controversial associations derived from the ensemble of prompt-phase observations of gamma-ray bursts (GRBs) is the apparent correlation in the source frame between the peak energy Epeak) of the nu-F(nu) spectrum and the isotropic radiated energy, Eiso. Since most gamma-ray bursts (GRBs) have Epeak above the energy range (15-150 keV) of the Burst Alert Telescope (BAT) on Swift, determining accurate Epeak values for large numbers of Swift bursts has been difficult. However, by combining data from Swift/BAT and the Suzaku Wide-band All-Sky Monitor (WAM), which covers the energy range from 50-5000 keV, for bursts which are simultaneously detected, one can accurately fit Epeak and Eiso and test the relationship between them for the Swift sample. Between the launch of Suzaku in July 2005 and the end of April 2009, there were 48 gamma-ray bursts (GRBs) which triggered both Swift/BAT and WAM and an additional 48 bursts which triggered Swift and were detected by WAM, but did not trigger. A BAT-WAM team has cross-calibrated the two instruments using GRBs, and we are now able to perform joint fits on these bursts to determine their spectral parameters. For those bursts with spectroscopic redshifts, we can also calculate the isotropic energy. Here we present the results of joint Swift/BAT-Suzaku/WAM spectral fits for 91 of the bursts detected by the two instruments. We show that the distribution of spectral fit parameters is consistent with distributions from earlier missions and confirm that Swift bursts are consistent with earlier reported relationships between Epeak and isotropic energy. We show through time-resolved spectroscopy that individual burst pulses are also consistent with this relationship.
description: Accepted for publication in the Astrophysical Journal
Come riaccendere una nana bianca
Creators: Matteo Boni
Publisher: name: Media Inaf
Year: 2018

Un nuovo studio, accettato per la pubblicazione su The Astrophysical Journal, simula le interazioni tra un buco nero non rotante di massa intermedia e una nana bianca che gli passa accanto. Tra i risultati dell'interazione, la riaccensione delle reazioni nucleari all'interno della nana bianca per pochi secondi
Be Star Disk Models in Consistent Vertical Hydrostatic Equilibrium
Creators: name: Sigut, T. A. A.
name: McGill, M. A.
name: Jones, C. E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: A popular model for the circumstellar disks of Be stars is that of a geometrically thin disk with a density in the equatorial plane that drops as a power law of distance from the star. It is usually assumed that the vertical structure of such a disk (in the direction parallel to the stellar rotation axis) is governed by the hydrostatic equilibrium set by the vertical component of the star's gravitational acceleration. Previous radiative equilibrium models for such disks have usually been computed assuming a fixed density structure. This introduces an inconsistency as the gas density is not allowed to respond to temperature changes and the resultant disk model is not in vertical, hydrostatic equilibrium. In this work, we modify the {\sc bedisk} code of \citet{sig07} so that it enforces a hydrostatic equilibrium consistent with the temperature solution. We compare the disk densities, temperatures, H$α$ line profiles, and near-IR excesses predicted by such models with those computed from models with a fixed density structure. We find that the fixed models can differ substantially from the consistent hydrostatic models when the disk density is high enough that the circumstellar disk develops a cool ($T\lesssim10,000 $K) equatorial region close to the parent star. Based on these new hydrostatic disks, we also predict an approximate relation between the (global) density-averaged disk temperature and the $T_{\rm eff}$ of the central star, covering the full range of central Be star spectral types.
description: 25 pages; 11 figures
title: ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ ÐºÑÑÑÐ° "Ð¦Ð¸ÑÑÐ¾Ð²ÑÐµ Ð¸Ð·Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°"
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÐ»ÑÐ½ÑÐµÐ²Ð°, ÐÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐ¸ÑÑÐ¾Ð²ÑÐµ Ð¸Ð·Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°
Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐµÐ±Ð½ÑÑ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¹
Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸Ð½ÑÐµÑÐ½ÐµÑ-ÑÐµÑÑÑÑÐ¾Ð²
ÑÑÑÑÐºÑÑÑÐ° ÐºÑÑÑÐ°

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð° Ð² Ð½Ð°Ð³Ð»ÑÐ´Ð½Ð¾Ð¹ Ð¸ Ð´Ð¾ÑÑÑÐ¿Ð½Ð¾Ð¹ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐ¾ÑÐ¼Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ð° Â«Ð¦Ð¸ÑÑÐ¾Ð²ÑÐµ Ð¸Ð·Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°Â». ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð° Ð¸ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð° ÑÑÑÑÐºÑÑÑÐ° Ð»ÐµÐºÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÐºÑÑÑÐ° Ð¿Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ Ñ Ð¿Ð¾Ð´Ð¾Ð±Ð½ÑÐ¼Ð¸ ÐºÑÑÑÐ°Ð¼Ð¸ Ð´ÑÑÐ³Ð¸Ñ ÐÐ£ÐÐ¾Ð². ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð¾Ð±Ð·Ð¾Ñ ÐÐ½ÑÐµÑÐ½ÐµÑ-ÑÐµÑÑÑÑÐ¾Ð² Ð¸ ÑÑÐ½ÐºÐ° ÑÐ¸ÑÑÐ¾Ð²ÑÑ Ð¸Ð·Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐ¸Ð±Ð¾ÑÐ¾Ð² Ð¸ Ð¸Ñ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð². ÐÑÐ» ÑÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½ Ð½Ð°Ð±Ð¾Ñ Ðº Ð¿ÑÐµÐ·ÐµÐ½ÑÐ°ÑÐ¸ÑÐ¼ ÐºÑÑÑÐ°. ÐÑÐµÐ·ÐµÐ½ÑÐ°ÑÐ¸Ð¸ Ð¾ÑÐ¾ÑÐ¼Ð»ÐµÐ½Ñ Ð² ÐµÐ´Ð¸Ð½Ð¾Ð¼ ÑÑÐ¸Ð»Ðµ.
title: ÐÐµÐ¹ÑÐ¾Ð½Ð½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° ÑÑÐ°Ð½ÑÐ»ÑÑÐ¸Ð¸ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐµÐºÑÑÑÐµÐ½ÑÐ½ÑÑ Ð½ÐµÐ¹ÑÐ¾Ð½Ð½ÑÑ ÑÐµÑÐµÐ¹
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: Ð¢ÑÐ½Ñ Ð§Ð¶Ð°Ð¾Ð»Ð¸Ð½Ñ
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ÐµÐ¹ÑÐ¾Ð½Ð½ÑÐµ ÑÐµÑÐ¸
ÐÑÐºÑÑÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑ
ÐÐµÑÐµÐ²Ð¾Ð´ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ð¹

description: ÐÐ°ÑÐ¸Ð½Ð°Ñ Ñ 2000 Ð³Ð¾Ð´Ð°, Ñ Ð¿Ð¾ÑÑÐ¾ÑÐ½Ð½ÑÐ¼ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐµÐ¾ÑÐ¸Ð¸ Ð² Ð¸ÑÐºÑÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¼ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÐµ, Ð¸ÑÐºÑÑÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð½ÐµÐ¹ÑÐ¾Ð½Ð½ÑÐµ ÑÐµÑÐ¸ ÑÑÐ°Ð»Ð¸ Ð½Ð¾Ð²ÑÐ¼Ð¸ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ°Ð¼Ð¸ Ð¼Ð°ÑÐ¸Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð°. ÐÐ¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ Ñ ÑÑÐ°Ð´Ð¸ÑÐ¸Ð¾Ð½Ð½ÑÐ¼ SMT (ÑÑÐ°ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ð¼ Ð¼Ð°ÑÐ¸Ð½Ð½ÑÐ¼ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð¾Ð¼) Ð½ÐµÐ¹ÑÐ¾Ð½Ð½Ð°Ñ ÑÐµÑÑ NMT (Ð½ÐµÐ¹ÑÐ¾Ð½Ð½ÑÐ¹ Ð¼Ð°ÑÐ¸Ð½Ð½ÑÐ¹ Ð¿ÐµÑÐµÐ²Ð¾Ð´) Ð¿ÑÐµÐ²Ð¾ÑÑÐ¾Ð´Ð¸Ñ SMT Ð²Ð¾ Ð¼Ð½Ð¾Ð³Ð¸Ñ Ð°ÑÐ¿ÐµÐºÑÐ°Ñ, ÑÐ°ÐºÐ¸Ñ ÐºÐ°Ðº ÑÐ¾ÑÐ½Ð¾ÑÑÑ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð°, Ð¿ÐµÑÐµÑÐ¿Ð¾ÑÑÐ´Ð¾ÑÐµÐ½Ð¸Ðµ Ð´Ð»Ð¸Ð½Ð½ÑÑ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹, ÑÐ¸Ð½ÑÐ°ÐºÑÐ¸Ñ, ÑÐ¾Ð»ÐµÑÐ°Ð½ÑÐ½Ð¾ÑÑÑ Ðº ÑÑÐ¼Ð½ÑÐ¼ Ð´Ð°Ð½Ð½ÑÐ¼ Ð¸ Ð´Ñ. Ð 2014 Ð³Ð¾Ð´Ñ, Ñ Ð¿Ð¾ÑÐ²Ð»ÐµÐ½Ð¸ÐµÐ¼ Ð¼Ð¾Ð´ÐµÐ»ÐµÐ¹ Ð¿Ð¾ÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ-Ðº-Ð¿Ð¾ÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ (seq2seq) Ð¸ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð¾Ð² Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ñ, Ð²Ð²ÐµÐ´ÐµÐ½Ð½ÑÑ Ð² Ð¼Ð¾Ð´ÐµÐ»Ñ, NMT Ð±ÑÐ» ÐµÑÐµ Ð±Ð¾Ð»ÐµÐµ ÑÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½, Ð¸ ÐµÐ³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÑÑÐ°Ð½Ð¾Ð²Ð¸Ð»Ð°ÑÑ Ð²ÑÐµ Ð»ÑÑÑÐµ Ð¸ Ð»ÑÑÑÐµ. Ð ÑÑÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÑÑÑ Ð¿Ð¾Ð¿ÑÐ»ÑÑÐ½ÑÐ¹Ð½Ð° Ð´Ð°Ð½Ð½ÑÐ¹ Ð¼Ð¾Ð¼ÐµÐ½Ñ Ð¿Ð¾Ð´ÑÐ¾Ð´ Ð¿Ð¾ÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ-Ðº-Ð¿Ð¾ÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð´Ð»Ñ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð° Ð½ÐµÐ¹ÑÐ¾Ð½Ð½ÑÑ Ð¼Ð°ÑÐ¸Ð½ Ñ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ Ð½Ð° ÐºÐ¸ÑÐ°Ð¹ÑÐºÐ¸Ð¹. ÐÑÐ¾Ð¼Ðµ ÑÐ¾Ð³Ð¾, Ð² ÑÐ°Ð±Ð¾ÑÐµ Ð²Ð¼ÐµÑÑÐ¾ ÑÑÐ°Ð´Ð¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ RNN (ÑÐµÐºÑÑÑÐµÐ½ÑÐ½Ð¾Ð¹ Ð½ÐµÐ¹ÑÐ¾Ð½Ð½Ð¾Ð¹ ÑÐµÑÐ¸) Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÑÑÑ LSTM (Ð´Ð¾Ð»Ð³Ð°Ñ ÐºÑÐ°ÑÐºÐ¾ÑÑÐ¾ÑÐ½Ð°Ñ Ð¿Ð°Ð¼ÑÑÑ) Ð´Ð»Ñ ÑÑÑÑÐ°Ð½ÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ° Ð¸ÑÑÐµÐ·Ð½Ð¾Ð²ÐµÐ½Ð¸Ñ Ð³ÑÐ°Ð´Ð¸ÐµÐ½ÑÐ° Ð¸ Ð³ÑÐ°Ð´Ð¸ÐµÐ½ÑÐ½Ð¾Ð³Ð¾ Ð²Ð·ÑÑÐ²Ð°, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð² ÑÐ²Ð¾Ñ Ð¾ÑÐµÑÐµÐ´Ñ Ð½Ð°ÑÐ¾Ð´ÑÑÑÑ Ð²Ð¾ Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸. Ð ÑÑÑ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ» ÑÐ°ÐºÐ¶Ðµ Ð²ÐºÐ»ÑÑÐµÐ½ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ñ. Ð­ÑÐ¾Ñ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ Ð½ÐµÐ¹ÑÐ¾Ð½Ð½ÑÐ¼ ÑÐµÑÑÐ¼ ÑÐ´ÐµÐ»ÑÑÑ Ð±Ð¾Ð»ÑÑÐµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ñ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑÐ¸Ð¼ ÑÐ°ÑÑÑÐ¼ Ð²ÑÐ¾Ð´Ð½ÑÑ Ð¿Ð¾ÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾ÑÑÐµÐ¹ Ð¸ Ð¼ÐµÐ½ÑÑÐµ Ðº Ð½ÐµÑÐ²ÑÐ·Ð°Ð½Ð½ÑÐ¼ ÑÐ°ÑÑÑÐ¼ Ð¿ÑÐ¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ð¸ Ð·Ð°Ð´Ð°Ñ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. Ð ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð¾Ð¹ ÑÐ°ÑÑÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÑÑÑ TensorFlow Ð´Ð»Ñ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¼Ð¾Ð´ÐµÐ»Ð¸ NMT.
An integrated dynamic weighing system based on SCADA
Creators: name: BAZYDŁO, Piotr
name: SZEWCZYK, Roman
name: URBAŃSKI, Michał
Publisher: name: Wrocław University of Technology, Wrocław University of Economics, Polish Operational and Systems Research Society
Year: 2015
Subjects: SCADA
industrial signal processing
system integration
dynamic weighing

description: OPERATIONS RESEARCH AND DECISIONS; ISSN 2081-8858
Localizing of the atmospheric contamination source  based on the  Kori field tracer experiment data
Creators: name: KOPKA, Piotr
name: WAWRZYNCZAK, Anna
name: BORYSIEWICZ, Mieczysław
Publisher: name: Wrocław University of Technology, Wrocław University of Economics, Polish Operational and Systems Research Society
Year: 2015
Subjects: Sequential Monte Carlo methods
accidental releases into the atmosphere
emergency reaction system

description: OPERATIONS RESEARCH AND DECISIONS; ISSN 2081-8858
Un battito d’ali, ed è subito tempesta magnetica
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2018

Pubblicato su “Chaos” un nuovo metodo di analisi non lineare in grado di render conto del comportamento della magnetosfera considerata come sistema in uno stato lontano dall’equilibrio: potrebbe aiutare a prevedere le tempeste geomagnetiche. Con il commento di Mauro Messerotti, fisico solare all’Inaf di Trieste
Open statistical issues in particle physics
Creators: name: Lyons, Louis
Publisher: name: arXiv
Year: 2008
Subjects: subject: Applications (stat.AP)
subject: FOS: Computer and information sciences

description: Many statistical issues arise in the analysis of Particle Physics experiments. We give a brief introduction to Particle Physics, before describing the techniques used by Particle Physicists for dealing with statistical problems, and also some of the open statistical questions.
description: Published in at http://dx.doi.org/10.1214/08-AOAS163 the Annals of Applied Statistics (http://www.imstat.org/aoas/) by the Institute of Mathematical Statistics (http://www.imstat.org)
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð±Ð°Ð½ÐºÐ¾Ð²ÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«Ð¡Ð±ÐµÑÐ±Ð°Ð½ÐºÂ»)
title: Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ
titleType: Subtitle
Creators: name: ÐÐ¾ÑÐ¾Ð½Ð¸Ð½Ð°, ÐÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÐºÑÐµÐ´Ð¸ÑÐ½Ð°Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ
Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐµÐ¿ÑÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐ¸ÑÐºÐ¸
Ð±Ð°Ð½ÐºÐ¾Ð²ÑÐºÐ°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
credit company
state regulation
reputational risks
banking activity

description: Ð Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¼ÐµÑ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÑÐµÐ´Ð¸ÑÐ½ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¹, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ¸Ñ Ð¼ÐµÑ. ÐÑÐ¾ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð´ÐµÑÐ°Ð»ÑÐ½ÑÐµ Ð¿Ð»Ð°Ð½Ñ Ð¿Ð¾ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð¼ÐµÑ.
description: The research paper analyzes the measures of state regulation of credit institutions, has developed proposals to improve these measures. Worked out detailed plans for the implementation of the proposed measures.
A Game Theoretical Study of Generalised Trust and Reciprocation in Poland: II. A description of the Study Group
Creators: name: RAMSEY, David M.
name: MARKOWSKA-PRZYBYŁA, Urszula
Publisher: name: Wrocław University of Technology, Wrocław University of Economics, Polish Operational and Systems Research Society
Year: 2015
Subjects: Bayesian networks
principal component analysis
social survey
experimental game theory

description: OPERATIONS RESEARCH AND DECISIONS; ISSN 2081-8858
Good open access: minimum requirements vs best practice
Creators: name: Rücknagel, Jesko
name: Schmeja, Stefan
Publisher: name: Zenodo
Year: 2023
Subjects: open access

description: Open Access aims to enable people worldwide to access scholarly information without barriers. To achieve this, various publication channels exist, and the number of possible publication venues continues to grow. The presentation will focus on explaining which selection criteria should be applied when choosing a publication venue in order to best achieve the goals of the Open Access movement. For this purpose, we take a closer look at the myths that still exist regarding Open Access. The following questions will be discussed: What best practices should I follow in publishing open access? What initiatives are there to push forward the publishing system's transformation? Which tools can help me to find a suitable publication venue?
Stelle al ritmo forsennato della “galassia mostro”
Creators: Matteo Boni
Publisher: name: Media Inaf
Year: 2018

Un articolo appena pubblicato su Nature illustra i risultati della più dettagliata cartina di una galassia primordiale mai ottenuta. Grazie ad Alma è stata osservata una mostruosa galassia, distante 12.4 miliardi di anni luce, che presenta un’intensissima formazione stellare lontano dal centro, in regioni piene di gas altamente instabile
Fascia di Kuiper: New Horizons mira al bersaglio
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2018

Lanciata dalla Florida nel 2006 e arrivata attorno a Plutone nel 2015, la sonda della Nasa si sta dirigendo a gran velocità verso il planetoide Ultima Thule, nome che significa “oltre i confini del mondo conosciuto”. Gli scatti giunti ora dalla sonda Nasa sono i più distanti dal Sole che siano mai stati fatti
Hayabusa smaschera quel vecchietto di Itokawa
Creators: Sara Venturi
Publisher: name: Media Inaf
Year: 2018

Uno studio condotto dai ricercatori dell'Università di Osaka, utilizzando i dati raccolti dalla sonda Hayabusa, ha permesso di determinare l'età dell'asteroide Itokawa e altre caratteristiche utili allo studio dell'evoluzione degli asteroidi vicini alla Terra
title: Ð ÐµÐ»ÐµÐ¹Ð½Ð°Ñ Ð·Ð°ÑÐ¸ÑÐ° ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÑÑÐ¸Ñ ÑÑÐµÐ±Ð½ÑÑ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹, Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ñ ÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 220100 âÐ¡Ð¸ÑÑÐµÐ¼Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ"
titleType: Subtitle
Creators: name: ÐÑÐ»ÑÑÐµÐ², ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
name: ÐÐ°Ð½Ð¸Ð½, ÐÐ°Ð»ÐµÑÐ¸Ð¹
name: ÐÐ°Ð²Ð¾Ð»Ð¾ÑÐ½ÑÐ¹, ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
name: ÐÐ¾Ð¿Ð¾Ð², ÐÐ°ÐºÑÐ¸Ð¼
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2008
Subjects: Ð­Ð»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ

description: ÐÑÐ°ÑÐºÐ¾ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐµÐ¾ÑÐ¸Ð¸ Ð·Ð°ÑÐ¸Ñ, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼ÑÑ Ð² ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐµÑÑÑ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸ÐµÐ¼ 6-35 ÐºÐ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ¾ÐºÐ¾Ð²ÑÐµ Ð·Ð°ÑÐ¸ÑÑ, ÑÑÑÐ°Ð½Ð°Ð²Ð»Ð¸Ð²Ð°ÐµÐ¼ÑÐµ Ð½Ð° Ð»Ð¸Ð½Ð¸ÑÑ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸ Ð¸ ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾ÑÐ°Ñ. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð·Ð°Ð´Ð°ÑÐ¸ Ñ ÑÐµÑÐµÐ½Ð¸ÑÐ¼Ð¸ Ð¸ Ð¿ÑÐ¸Ð¼ÐµÑÑ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð·Ð°ÑÐ¸Ñ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 220100 Â«Ð¡Ð¸ÑÑÐµÐ¼Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÂ». ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¼Ð¾Ð¶ÐµÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÑÑÑ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼Ð¸, Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ð¼Ð¸ÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 140200 Â«Ð­Ð»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ° Ð¸ ÑÐ»ÐµÐºÑÑÐ¾ÑÐµÑÐ½Ð¸ÐºÐ°Â».
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Additional file 1 of Can use of pictograms reduce liquid medication administration errors by mothers? An interventional study
Creators: name: Patidar, Pawan
name: Mathur, Aditya
name: Pathak, Ashish
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases

description: Additional file 1: Additional Table 1. Different measuring devices and the corresponding doses used in text only and text plus pictogram measuring session.
Magnetic and magnetoelectric studies in pure and cation doped BiFeO3
Creators: name: Naik, V. B.
name: Mahendiran, R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We report magnetic and magnetoelectric studies on BiFeO3 and divalent cation (A) suvtitute Bi0.7A0.3FeO3 (A = Sr,Ba, and Sr0.5Ba0.5). It is shown that the rapid increase of magnetization at the Neel temperature (TN = 642 K) is suppressed in the co-doped compound A = Sr0.5Ba0.5. All the divalent subtituted compounds show enhanced magnetization and hysteresis loop. Both longitudinal and transverse magnetoelectric coefficients were measured using the dynamical lock-in technique. The co-doped compound shows the highest magnetoelectric coefficient at room temperature although it is not the compound with the highest saturation magnetization. It is found that as the size of the A-site cation increses, the transverse magnetoelectric coeffient increases and exceeds the longitudinal magnetoelectric coefficient. It is suggested that changes in magnetic domain structure and magnetostriction are possible reasons for the observed changes in the magnetoelectric coefficients.
description: 16 pages, 6 figure
Ecco il getto sovraionizzato della Medusa
Creators: Mario Guarcello
Publisher: name: Media Inaf
Year: 2018

Tre risultati in un colpo solo per Emanuele Greco, dottorando all’Inaf di Palermo. Il jet analizzato nel suo studio su Ic 443 è il terzo caso noto di getto in un resto di supernova e il primo di getto sovra-ionizzato. Inoltre, viene identificata con una ragionevole certezza anche la stella di neutroni prodotta dal collasso della stella progenitrice
Gli audio dimenticati dell’Apollo 11
Creators: Redazione Ansa
Publisher: name: Media Inaf
Year: 2018

La Nasa ha reso disponibili in rete, in formato mp3, 19mila ore di audio dalla storica missione di 49 anni fa. Dialoghi che catturano i momenti drammatici poco prima dell’atterraggio sulla Luna, ma anche scambi spensierati e scherzosi
title: ÐÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð²Ð¾ÑÐ¿ÑÐ¸ÑÑÐ¸Ñ ÑÑÐµÐ±Ð½Ð¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ð¸ ÑÑÐ¿ÐµÐ²Ð°ÐµÐ¼Ð¾ÑÑÑ Ð¿Ð¾ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½Ð¾Ð¼Ñ ÑÐ·ÑÐºÑ Ñ Ð¿Ð¾Ð´ÑÐ¾ÑÑÐºÐ¾Ð² Ð¿ÑÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ð¸ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÐ¾ÑÐ¼ Ð¿Ð¾Ð´Ð°ÑÐ¸ ÑÑÐµÐ±Ð½Ð¾Ð³Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°
title: Features of perception of educational information and performance in foreign languages in adolescents while using various forms of presentation of prescribed syllabus
Creators: name: ÐÑÐ¸Ð±ÑÐ»Ð¾Ð²Ð°, ÐÐ°ÑÐ°Ð»ÑÑ
name: Ð¤ÑÐ¾Ð»Ð¾Ð²Ð°, Ð¡Ð²ÐµÑÐ»Ð°Ð½Ð°
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2020
Subjects: ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸
Ð²Ð¾ÑÐ¿ÑÐ¸ÑÑÐ¸Ðµ ÑÑÐµÐ±Ð½Ð¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸
Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÐµ ÑÐ·ÑÐºÐ¸

description: Ð¡ÑÐ°ÑÑÑ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÑÐµÐ´ÑÑÐ² Ð¿Ð¾Ð´Ð°ÑÐ¸ ÑÑÐµÐ±Ð½Ð¾Ð³Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð° Ð¿ÑÐ¸ Ð¾Ð±ÑÑÐµÐ½Ð¸Ð¸ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÐ¼ ÑÐ·ÑÐºÐ°Ð¼, ÑÐ°ÐºÐ¸Ñ ÐºÐ°Ðº ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐ¹ ÑÐµÑÑÑÑ Â«ÐÐ¾ÑÐºÐ¾Ð²ÑÐºÐ°Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð°Ñ ÑÐºÐ¾Ð»Ð°Â» (ÐÐ­Ð¨). Ð ÑÑÐ°ÑÑÐµ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¼Ð¿Ð¸ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ¸ Ð²Ð¾ÑÐ¿ÑÐ¸ÑÑÐ¸Ñ ÑÑÐµÐ±Ð½Ð¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ð¿Ð¾Ð´ÑÐ¾ÑÑÐºÐ°Ð¼Ð¸ Ð² Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ Ð¾Ñ ÑÐ¿Ð¾ÑÐ¾Ð±Ð° Ð¿Ð¾Ð´Ð°ÑÐ¸ ÑÑÐµÐ±Ð½Ð¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸. ÐÐ²ÑÐ¾ÑÑ Ð¾ÑÐ¼ÐµÑÐ°ÑÑ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÑ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ Ð´Ð¾Ð»Ð¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ¸Ð½ÐµÑÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸ Ð°ÑÐ´Ð¸Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÐºÐ°Ð½Ð°Ð»Ð¾Ð² Ð²Ð¾ÑÐ¿ÑÐ¸ÑÑÐ¸Ñ Ð¿ÑÐ¸ Ð¾Ð±ÑÑÐµÐ½Ð¸Ð¸ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÐ¼ ÑÐ·ÑÐºÐ°Ð¼ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ ÑÐµÑÑÑÑÐ¾Ð² ÐÐ­Ð¨.
description: The article is devoted to the issue of using modern means of presenting educational material in teaching foreign languages, such as the electronic resource âMoscow Electronic Schoolâ (MES). The article analyzes the results of an empirical study of the specifics of the perception of educational information by adolescents, depending on the method of presentation of prescribed syllabus. The authors emphasize the need to increase the use of kinesthetic and auditory channels of perception while teaching foreign languages via MES.
Two procedures for robust monitoring of probability distributions of economic data stream induced by depth functions
Creators: name: OSAGIEDE, Augustine A.
name: EKHOSUEHI, Virtue U.
Publisher: name: Wrocław University of Technology, Wrocław University of Economics, Polish Operational and Systems Research Society
Year: 2015
Subjects: data stream
robust procedure
statistical depth function

description: OPERATIONS RESEARCH AND DECISIONS; ISSN 2081-8858
title: Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÑÑÐµÑÑÐ°Ð¼Ð¸ Ð¸ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ½ÑÐ¼Ð¸ ÑÐ¸ÑÑÐ°ÑÐ¸ÑÐ¼Ð¸ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐµÐ»Ð»Ð¼Ð°ÑÑÂ»)
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð»ÐºÐ¾Ð²Ð°, ÐÐ¸Ð´Ð¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐµÐ¾ÑÐ¸ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÑÑÐµÑÑÐ°Ð¼Ð¸ Ð¸ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ°Ð¼Ð¸
ÑÐµÐ¾ÑÐ¸Ð¸ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ¾Ð²
Ð¿Ð¾Ð½ÑÑÐ¸Ðµ Ð¸ ÑÐµÐ¾ÑÐ¸Ð¸ ÑÑÑÐµÑÑÐ°
Ð°Ð½Ð°Ð»Ð¸Ð· Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐµÐ¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐÐÐ Â«ÐÐµÐ»Ð»Ð¼Ð°ÑÑÂ»

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«ÐÐµÐ»Ð»Ð¼Ð°ÑÑ Ð¡ÐÐ±Â». Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÑÑÐµÑÑÐ°Ð¼Ð¸ Ð¸ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ°Ð¼Ð¸ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ ÐÐÐ Â«ÐÐµÐ»Ð»Ð¼Ð°ÑÑ Ð¡ÐÐ±Â». ÐÑÐ»Ð¸ Ð¸Ð·ÑÑÐµÐ½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÑÑÐµÑÑÐ°Ð¼Ð¸ Ð¸ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ°Ð¼Ð¸. ÐÑÐ» Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐµÐ¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐÐÐ Â«ÐÐµÐ»Ð»Ð¼Ð°ÑÑÂ» Ð¸ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ¾Ð² Ð² Ð½ÐµÐ¼. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÑÑÐµÑÑÐ°Ð¼Ð¸ Ð¸ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ°Ð¼Ð¸ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ ÐÐÐ Â«ÐÐµÐ»Ð»Ð¼Ð°ÑÑÂ». ÐÐ¿Ð¸ÑÐ°Ð½ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÑÑÐµÐºÑ Ð¾Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹.
Asteroide Ryugu, ecco dove avverrà l’approdo
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2018

Compromesso ideale fra le esigenze degli scienziati e quelle degli ingegneri della missione, la regione MA-9, situata nell’emisfero meridionale dell’asteroide, sarà il luogo nel quale il prossimo 3 ottobre toccherà il suolo il lander Mascot della sonda Hayabusa-2
Giove adolescente per due milioni di anni
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2018

Un gruppo di ricercatori dell’Eth di Zurigo, in Svizzera, ha dimostrato che il tempo impiegato dal giovane pianeta per crescere da 15 a 50 masse terrestri è stato molto più lungo di quanto si pensasse in precedenza. Lo studio è pubblicato su Nature Astronomy