cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
A high-resolution spectroscopic survey of late-type stars: chromospheric activity, rotation, kinematics, and age
Creators: name: Lopez-Santiago, J.
name: Montes, D.
name: Galvez-Ortiz, M. C.
name: Crespo-Chacon, I.
name: Martinez-Arnaiz, R. M.
name: Fernandez-Figueroa, M. J.
name: De Castro, E.
name: Cornide, M.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Aims: We present a compilation of spectroscopic data from a survey of 144 chromospherically active young stars in the solar neighborhood which may be used to investigate different aspects of the formation and evolution of the solar neighborhood in terms of kinematics and stellar formation history. The data have already been used by us in several studies. With this paper, we make all these data accessible to the scientific community for future studies on different topics. Methods: We performed spectroscopic observations with echelle spectrographs to cover the entirety of the optical spectral range simultaneously. Standard data reduction was performed with the IRAF ECHELLE package. We applied the spectral subtraction technique to reveal chromospheric emission in the stars of the sample. The equivalent width of chromospheric emission lines was measured in the subtracted spectra and then converted to fluxes using equivalent width-flux relationships. Radial and rotational velocities were determined by the cross-correlation technique. Kinematics, equivalent widths of the lithium line 6707.8 angstroms and spectral types were also determined. Results: A catalog of spectroscopic data is compiled: radial and rotational velocities, space motion, equivalent widths of optical chromospheric activity indicators from Ca II H & K to the calcium infrared triplet and the lithium line in 6708 angstroms. Fluxes in the chromospheric emission lines and R'HK are also determined for each observation of star in the sample. We used these data to investigate the emission levels of our stars. The study of the Halpha emission line revealed the presence of two different populations of chromospheric emitters in the sample, clearly separated in the log F(Halpha)/Fbol - (V-J) diagram.
description: Accepted to A&A. 56 pages, 7 pages. Online material: 4 tables and 27 figures
title: ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° MathCAD. Ð§. 1
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐµÑÑÐ°Ñ, ÐÐ¸ÐºÑÐ¾Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ
ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½ÑÐµ

description: Ð ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ Ð¸Ð½ÑÐµÑÑÐµÐ¹Ñ Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ MathCAD.ÐÐ¿Ð¸ÑÐ°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐ°Ð±Ð¾ÑÑ, Ð² ÑÐ¾Ð¼ ÑÐ¸ÑÐ»Ðµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾ÑÑÐµÐ¹ÑÐ¸Ñ Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ð¹. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ°Ð±Ð¾ÑÐ° Ñ Ð²ÐµÐºÑÐ¾ÑÐ°Ð¼Ð¸ Ð¸ Ð¼Ð°ÑÑÐ¸ÑÐ°Ð¼Ð¸, ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ðµ Ð³ÑÐ°ÑÐ¸ÐºÐ¾Ð², ÑÐ¸Ð¼Ð²Ð¾Ð»ÑÐ½ÑÐµ Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ñ Ð¸ ÑÐµÑÐµÐ½Ð¸Ðµ Ð°Ð»Ð³ÐµÐ±ÑÐ°Ð¸ÑÐµÑÐºÐ¸Ñ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ð¹. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿ÑÐ¸Ð¼ÐµÑÑ.ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÐÐ½ÑÑÐ¸ÑÑÑÐ° Ð¼ÐµÑÐ°Ð»Ð»ÑÑÐ³Ð¸Ð¸, Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¸ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ°, Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ°Â» Ð¸ Â«ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ°Â».
title: Ð¢ÐµÐ¾ÑÐ¸Ñ ÑÑÑÐ±Ð¾Ð¼Ð°ÑÐ¸Ð½. ÐÑÐ½Ð¾Ð²Ñ ÑÐµÐ¾ÑÐ¸Ð¸ ÑÑÑÐ±Ð¾ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÐ¾Ð²
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¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² "Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð°ÑÐ¸Ð½Ñ Ð¸ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ"
titleType: Subtitle
Creators: name: ÐÐ°Ð»ÐµÑÐºÐ¸Ð½, Ð®ÑÐ¸Ð¹
name: ÐÐ¾Ð¶ÑÑÐ¾Ð², Ð®ÑÐ¸Ð¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2013
Subjects: Ð¢ÑÑÐ±Ð¾ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÑ
Ð¢ÑÑÐ±Ð¾Ð¼Ð°ÑÐ¸Ð½Ñ

description: Ð¡Ð¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¿Ð¾ Ð¾ÑÐ½Ð¾Ð²Ð°Ð¼ ÑÐµÐ¾ÑÐ¸Ð¸ ÑÑÑÐ±Ð¾Ð¼Ð°ÑÐ¸Ð½. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð¸ÑÑÐ¾ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¾Ð±Ð·Ð¾Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐµÐ¾ÑÐ¸Ð¸ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÐºÐ¸ ÑÑÑÐ±Ð¾Ð¼Ð°ÑÐ¸Ð½, ÑÐµÑÐ¼Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸ Ð³Ð°Ð·Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐµÐ¾ÑÐ¸Ð¸ ÑÑÑÐ±Ð¾Ð¼Ð°ÑÐ¸Ð½, Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐµÐ¾ÑÐ¸Ð¸ ÑÑÑÐ±Ð¾ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÐ°. ÐÐ·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐµÐ¾ÑÐ¸Ð¸ Ð¸ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ñ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð³Ð°Ð·Ð° Ð² ÐºÐ°Ð½Ð°Ð»Ð°Ñ Ð¿ÑÐ¾ÑÑÐ¾Ð¹ ÑÐ¾ÑÐ¼Ñ, Ð² ÐºÐ°Ð½Ð°Ð»Ð°Ñ ÑÑÑÐ±Ð¾Ð¼Ð°ÑÐ¸Ð½. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½ ÑÐ°Ð±Ð¾ÑÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð² ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ°Ñ Ð¿ÑÐ¾ÑÐ¾ÑÐ½Ð¾Ð¹ ÑÐ°ÑÑÐ¸ Ð¾ÑÐµÐ²ÑÑ Ð¸ ÑÐµÐ½ÑÑÐ¾Ð±ÐµÐ¶Ð½ÑÑ ÑÑÑÐ±Ð¾ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÐ¾Ð². Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ 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 Ð¿ÑÐ¾ÑÐ¸Ð»Ñ Â«ÐÐ°ÐºÑÑÐ¼Ð½Ð°Ñ Ð¸ ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÐ½Ð°Ñ ÑÐµÑÂ­Ð½Ð¸ÐºÐ°Â» Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² Â«Ð¢ÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð°ÑÐ¸Ð½Ñ Ð¸ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸ÐµÂ».
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°.
Influence of insole slope on bone joint stress, foot bone stress, and foot pressure distribution
Creators: name: Nattapon Chantarapanich
name: Sunton Wongsiri
name: Kriskrai Sitthiseripratip
Publisher: name: Research and Development Office, Prince of Songkla University
Year: 2019
Subjects: insole slope
bone stress
joint stress
foot pressure

description: Songklanakarin Journal of Science and Technology, 41, 2, 375-382
Le leggi di Keplero diventano virali
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

È il primo video della neonata band de “I Supplenti Italiani”, e in pochi giorni ha fatto il giro del web, raccogliendo consensi e risate anche fra gli astronomi professionisti. «Le nostre canzoni vengono fatte ascoltare in classe dai professori, e questo per noi è un grande onore», dice Lorenzo Baglioni, comico fiorentino, autore dei testi e membro della band
Schwarzschild radius from Monte Carlo calculation of the Wilson loop in supersymmetric matrix quantum mechanics
Creators: name: Hanada, Masanori
name: Miwa, Akitsugu
name: Nishimura, Jun
name: Takeuchi, Shingo
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: In the string/gauge duality it is important to understand how the space-time geometry is encoded in gauge theory observables. We address this issue in the case of the D0-brane system at finite temperature T. Based on the duality, the temporal Wilson loop operator W in gauge theory is expected to contain the information of the Schwarzschild radius R_{Sch} of the dual black hole geometry as log = R_{Sch} / (2 pi alpha' T). This translates to the power-law behavior log = 1.89 (T/lambda^{1/3})^{-3/5}, where lambda is the 't Hooft coupling constant. We calculate the Wilson loop on the gauge theory side in the strongly coupled regime by performing Monte Carlo simulation of supersymmetric matrix quantum mechanics with 16 supercharges. The results reproduce the expected power-law behavior up to a constant shift, which is explainable as alpha' corrections on the gravity side.
description: REVTeX4, 4 pages, 1 figure
Inheritance of pericarp pigment on crossing between black rice and white rice
Creators: name: Kristamtini
name: Taryono
name: Panjisakti Basunanda
name: Murti, Rudi Hari
Publisher: name: Research and Development Office, Prince of Songkla University
Year: 2019
Subjects: pericarp pigment
inheritance
black rice
white rice

description: Songklanakarin Journal of Science and Technology, 41, 2, 383-388
Interplay between shear loading and structural aging in a physical gel
Creators: name: Ronsin, O.
name: Caroli, C.
name: Baumberger, T.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We show that the aging of the mechanical relaxation of a gelatin gel exhibits the same scaling phenomenology as polymer and colloidal glasses. Besides, gelatin is known to exhibit logarithmic structural aging (stiffening). We find that stress accelerates this process. However, this effect is definitely irreducible to a mere age shift with respect to natural aging. We suggest that it is interpretable in terms of elastically-aided elementary (coil$\to$helix) local events whose dynamics gradually slows down as aging increases geometric frustration.
Sasson and Kramer- memory of content that varies in presentation speed and complexity
Creators: name: TAU Experimental Psychology Team
name: Sasson, Gil
name: Kramer, Liron
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Social and Behavioral Sciences
subject: Psychology
subject: FOS: Psychology

description: This is our pre-registration, as part of a research we run in Tel Aviv university.
title: Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÑÑ Ð¢Ð­Ð¦ Ñ 4 Ð±Ð»Ð¾ÐºÐ°Ð¼Ð¸ Ð¼Ð¾ÑÐ½Ð¾ÑÑÑÑ 63 ÐÐÑ
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ÑÐ°ÐºÐ¾Ð²Ð°, 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: 2018
Subjects: ÑÐ»ÐµÐºÑÑÐ¾Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ
ÑÑÑÑÐºÑÑÑÐ½Ð°Ñ ÑÑ ÐµÐ¼Ð°
Ð³Ð»Ð°Ð²Ð½Ð°Ñ ÑÑ ÐµÐ¼Ð°
ÑÑ ÐµÐ¼Ð° ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð½ÑÐ¶Ð´
ÐºÐ¾ÑÐ¾ÑÐºÐ¾Ðµ Ð·Ð°Ð¼ÑÐºÐ°Ð½Ð¸Ðµ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°ÑÑÐ¸ ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¾ÑÐµÐ½ÑÑÐ°Ð»Ð¸. ÐÑÐ±ÑÐ°Ð½Ð° Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ½Ð°Ñ ÑÑÐµÐ¼Ð° Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ðµ ÑÐ»ÐµÐºÑÑÐ¾Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ñ ÑÐ¾ÐºÐ¸ ÐºÐ¾ÑÐ¾ÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð¼ÑÐºÐ°Ð½Ð¸Ñ. ÐÑÐ±ÑÐ°Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÑ Ð¸ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¸. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð³Ð»Ð°Ð²Ð½Ð°Ñ ÑÑÐµÐ¼Ð° ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹ Ð¸ ÑÑÐµÐ¼Ð° ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð½ÑÐ¶Ð´.
title: Ð¡Ð»ÐµÐ´ÑÑÐ¸Ð¹ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´ Ñ Ð½ÐµÐ»Ð¸Ð½ÐµÐ¹Ð½Ð¾Ð¹ ÑÐºÐ¾ÑÐ¾ÑÑÐ½Ð¾Ð¹ Ð¾Ð±ÑÐ°ÑÐ½Ð¾Ð¹ ÑÐ²ÑÐ·ÑÑ
title: Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ
titleType: Subtitle
Creators: name: ÐÐ¾Ð»Ð¾ÑÐ¾Ð², ÐÐ¸ÑÐ°Ð»Ð¸Ð¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÐ»ÐµÐ´ÑÑÐ¸Ð¹ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´
Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð½Ð°Ð»Ð°Ð´ÐºÐ°

description: Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÑÐ»ÐµÐ´ÑÑÐ¸Ð¹ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´ Ñ Ð½ÐµÐ»Ð¸Ð½ÐµÐ¹Ð½Ð¾Ð¹ ÑÐºÐ¾ÑÐ¾ÑÑÐ½Ð¾Ð¹ Ð¾Ð±ÑÐ°ÑÐ½Ð¾Ð¹ ÑÐ²ÑÐ·ÑÑ. Ð Ð°Ð·ÑÐ°Ð±Ð°ÑÑÐ²Ð°ÑÑÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ ÑÐ¸Ð½ÑÐµÐ·Ð° ÑÐ»ÐµÐ´ÑÑÐ¸Ñ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¾Ð², Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð½ÑÑ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÑÑÑÐºÑÑÑ Ñ Ð¼Ð¾Ð´Ð°Ð»ÑÐ½ÑÐ¼ Ð¸ Ð¼Ð¾Ð´Ð°Ð»ÑÐ½Ð¾-Ð¿Ð¾Ð´ÑÐ¸Ð½ÐµÐ½Ð½ÑÐ¼ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÐºÐ¾Ð¾ÑÐ´Ð¸Ð½Ð°Ñ. ÐÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ°ÑÑÑÑ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð½Ð°Ð»Ð°Ð´ÐºÐµ Ð² ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÐµÐ¶Ð¸Ð¼Ð°Ñ ÑÐ°Ð±Ð¾ÑÑ.
Il deserto delle Cefeidi
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2016

Attorno al centro della nostra galassia c’è una vasta regione sorprendentemente vuota di giovani stelle. Lo studio, firmato tra gli altri da Giuseppe Bono dell’Università di Roma Tor Vergata e associato INAF, è pubblicato su MNRAS
The environmental management systems certification in the forestry sector in Italy
Creators: name: Giorgio, Franceschetti
name: Davide, Pettenella
name: Laura, Secco
Publisher: name: Unknown
Year: 1998
Subjects: Environmental Economics and Policy
Resource /Energy Economics and Policy

description: Proceedings of the Sixth Joint Conference on Agriculture, Food, and the Environment, August 31 - September 2, 1998, Minneapolis, Minnesota
Appuntamento in FM prima dell’esplosione
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2016

Si tratta della supernova più celebre del XX secolo, anche perché l'evento si è verificato una trentina di anni fa a soli 160 mila anni luce di distanza. Di recente, dall'Australia, un gruppo di ricercatori è riuscito a sbirciare nel passato della stella milioni di anni prima che esplodesse
FK/Fpi in full QCD
Creators: name: Ramos, A.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We determine the ratio FK/Fpi in QCD with Nf=2+1 flavors of sea quarks, based on a series of lattice calculations with three different couplings, large volumes and a simulated pion mass reaching down to about 190 MeV. We obtain FK/Fpi = 1.192 +- 0.007(stat) +- 0.006(sys) with all the sources of systematic uncertainty under control.
description: 8 pages, 9 figures, 1 table. Presented at the XXVII International Symposium on Lattice Field Theory (2009)
Ecological characterization of local entomopathogenic nematodes Steinernema sp. and its pathogenicity test against termites Macrotermes sp.
Creators: name: Priyantini Widiyaningrum
name: Niken Subekti
name: Bambang Priyono
Publisher: name: Research and Development Office, Prince of Songkla University
Year: 2019
Subjects: ecological characteristics
local EPNs
pathogenicity
Steinernema sp.
Macrotermes sp.

description: Songklanakarin Journal of Science and Technology, 41, 2, 459-464
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð½ÐµÐ²Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð°Ð¼Ð¾ÑÑÐ¸Ð·Ð°ÑÐ¾ÑÐ°, ÑÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð½Ð° ÑÐ¾ÑÐ¾ÑÐµ Ð¸ÑÐ¿ÑÑÐ°ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐµÐ½ÑÑÐ¸ÑÑÐ³Ð¸
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÑÐ¾ÑÐ¼Ð°Ð»Ñ, ÐÐ»Ð°Ð´Ð¸Ñ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: 2017
Subjects: Ð¦ÐµÐ½ÑÑÐ¸ÑÑÐ³Ð¸
Ð Ð¾ÑÐ¾ÑÑ
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description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð¸ÑÐ¿ÑÑÐ°ÑÐµÐ»ÑÐ½ÑÐ¹ ÑÑÐµÐ½Ð´ - ÑÐµÐ½ÑÑÐ¸ÑÑÐ³Ð°, Ð½Ð° ÑÐ¾ÑÐ¾ÑÐµ ÐºÐ¾ÑÐ¾ÑÐ¾Ð³Ð¾ ÑÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ñ Ð¿Ð½ÐµÐ²Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð¼Ð¾ÑÑÐ¸Ð·Ð°ÑÐ¾Ñ ÑÐ¾Ð²Ð¼ÐµÑÑÐ½Ð¾ Ñ Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¸Ð¼ Ð²Ð¸Ð±ÑÐ°ÑÐ¾ÑÐ¾Ð¼. Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð¿Ð½ÐµÐ²Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð°Ð¼Ð¾ÑÑÐ¸Ð·Ð°ÑÐ¾ÑÐ° Ð¿ÑÐ¸ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¸ ÑÐµÐ½ÑÑÐ¾Ð±ÐµÐ¶Ð½Ð¾Ð¹ ÑÐ¸Ð»Ñ Ð¸ Ð²Ð¸Ð±ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÑÐ¸Ð»Ð¸Ð¹. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¾Ð¿Ð¸ÑÐ°Ð½Ñ Ð²Ð¸Ð´Ñ Ð¸ÑÐ¿ÑÑÐ°ÑÐµÐ»ÑÐ½ÑÑ ÑÐµÐ½ÑÑÐ¸ÑÑÐ³, Ð¸Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ, Ð¼ÐµÑÐ¾Ð´Ñ ÐºÐ¾Ð¼Ð¿Ð¾Ð½Ð¾Ð²ÐºÐ¸ ÑÐµÐ½ÑÑÐ¸ÑÑÐ³Ð¸ Ð¸ ÑÐ¾ÑÐ¾ÑÐ°. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ñ ÑÐµÐ°Ð»ÑÐ½ÑÐµ Ð¼Ð¾Ð´ÐµÐ»Ð¸, ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ðµ Ð½Ð° ÑÑÐ½ÐºÐµ. ÐÐ¿Ð¸ÑÐ°Ð½Ñ Ð²Ð¸Ð´Ñ Ð°Ð¼Ð¾ÑÑÐ¸Ð·Ð°ÑÐ¾ÑÐ¾Ð², ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ñ Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð°Ð½Ð°Ð»Ð¾Ð³Ð¸ÑÐ½ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð² ÑÐ°ÑÑÐ½Ð¾ÑÑÐ¸, ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð¸ÑÐ¿ÑÑÐ°ÑÐµÐ»ÑÐ½ÑÑ ÑÐµÐ½ÑÑÐ¸ÑÑÐ³, Ð¾ÑÑÑÐµÑÑÐ²Ð»ÑÑÑÐ¸Ðµ ÑÐ¾Ð²Ð¼ÐµÑÑÐ½Ð¾ Ð»Ð¸Ð½ÐµÐ¹Ð½ÑÐµ Ð¸ Ð²Ð¸Ð±ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÑÐºÐ¾ÑÐµÐ½Ð¸Ñ. Ð¡Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð° ÑÑÑÑÐºÑÑÑÐ½Ð¾-ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð°Ñ ÑÑÐµÐ¼Ð° Ð¸ÑÐ¿ÑÑÐ°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐµÐ½Ð´Ð°, ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð¸ÑÑÐ»ÐµÐ´ÑÐµÑÑÑ. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¾ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ ÑÐ¶Ð°ÑÐ¾Ð³Ð¾ Ð²Ð¾Ð·Ð´ÑÑÐ° Ð²Ð½ÑÑÑÐ¸ ÐºÐ°Ð¼ÐµÑÑ Ð·Ð°ÐºÑÑÑÐ¾Ð³Ð¾ ÑÐ¸Ð»Ð¸Ð½Ð´ÑÐ°, ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð·Ð°ÐºÑÐµÐ¿Ð»ÐµÐ½ Ð½Ð° ÑÐ¾ÑÐ¾ÑÐµ Ð¸ÑÐ¿ÑÑÐ°ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐµÐ½ÑÑÐ¸ÑÑÐ³Ð¸, Ð¿ÑÐ¸ Ð²ÑÐ°ÑÐµÐ½Ð¸Ð¸ ÑÐ¾ÑÐ¾ÑÐ° Ñ Ð¿Ð¾ÑÑÐ¾ÑÐ½Ð½Ð¾Ð¹ ÑÐºÐ¾ÑÐ¾ÑÑÑÑ, Ð³Ð´Ðµ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ñ Ð³ÑÐ°ÑÐ¸ÐºÐ¸ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ð¹ Ð¿ÑÐ¸ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð·Ð½Ð°ÑÐµÐ½Ð¸ÑÑ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² ÑÐ¸ÑÑÐµÐ¼Ñ.
China-New Zealand-Cook Islands Triangular Aid Project on Water Supply
Creators: name: Zhang, Denghua
Publisher: name: Canberra, ACT : Coral Bell School of Asia Pacific Affairs, College of Asia and the Pacific, The Australian National University
Year: 2015

description: Recently, the Pacific region seems to be a testing place for China’s growing triangular aid cooperation. The China–New Zealand–Cook Islands triangular project on water supply (Te Mato Vai) is an interesting case study as it claims to be China’s first triangular aid project with traditional donors. Based on my fieldwork research, this In Brief aims to provide a succinct summary of this project and some early observations to inform future triangular cooperation.
The geometry of the higher dimensional black hole thermodynamics in Einstein-Gauss-Bonnet theory
Creators: name: Biswas, Ritabrata
name: Chakraborty, Subenoy
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: This paper deals with five-dimensional black hole solutions in (a) Einstein-Yang-Mills-Gauss-Bonnet theory and (b)Einstein-Maxwell-Gauss-Bonnet theory with a cosmological constant for spherically symmetric space time. The geometry of the black hole thermodynamics has been studied for both the black holes.
description: 8 pages
Strangeness and charm content of the nucleon
Creators: name: Bali, Gunnar
name: Collins, Sara
name: Schaefer, Andreas
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present results on the scalar strangeness and charm contents of the nucleon and of the disconnected contributions to the nucleon spin. These are obtained on two flavour non-perturbatively improved Sheikholeslami-Wilson configurations at a pseudoscalar mass of 290 MeV. We quote f_{T_s} = m_s/m_N< = 0.070(22) as our preliminary value for the strange quark fraction of the nucleon mass and a modified minimal subtraction scheme value Delta s = -0.015(10), with as yet unknown systematics, for the strangeness contribution to the spin.
description: 7 pages, 5 figures, talk presented at The XXVI International Symposium on Lattice Field Theory (LAT2009), July 26-31 2009, Peking University, Beijing, China
Forest types of the coastal western hemlock zone
Creators: name: Orlóci, László
Publisher: name: University of British Columbia
Year: 2012

description: This thesis contributes analytical and synthetical data on the forest phytocoenoses and proposes a classification. Detailed floristical and environmental descriptions are given, also consideration of succession and life-form distribution. The following ecosystem classification is proposed: I. Dry edaphic and mesic zonal forest types of the dry subzone. 1) Pseudotsugetum menziesii a) subassoc. tsugetosum heterophyllae or the orthic Gaultheria forest type b) subassoc. legosolicum or the legosolic Gaultheria forest type c) subassoc. mahonietosum or the Gaultheria - Mahonia forest type 2) Tsugetum heterophyllae Subassoc. plagiothecietosum undulati a) var. muscosum or the orthic Plagiothecium forest type b) var. mahoniosum or the Plagiothecium - Mahonia forest type II. Dry edaphic and mesic zonal forest types of the wet subzone 3) Tsugeto – Gaultherietum a) subassoc. typicum or the orthic Vaccinium alaskaense - Gaultheria forest type b) subassoc, legosolicum or the legosolic Vaccinium alaskaense - Gaultheria forest type 4) Abieteto - Tsugetum heterophyllae a) vara clintoniosum or the Vaccinium alaskaense - Plagiothecium - Clintonia forest type b) var. acerosum circinati or the Vaccinium alaskaense - Plagiothecium - Acer circinatum forest type III. Seepage forest types 5) Thujeto - Polystichetum or the Polystichum forest type 6) Thujeto – Blechnetum a) subassoc. typicum or the orthic Blechnum forest type b) subassoc. gleysolicum or the gleysolic Blechnum forest c) subassoc. turfosum or the peaty Blechnum forest type d) subassoc. rubetosum vitifolii or the Blechnum - Rubus vitifolius forest type 7) Abieteto - Oplopanacetum or the Oplopanax - Adiantum forest type 8) Piceeto - Lysichitetum or the Vaccinium alaskaense - Lysichitum forest type IV. Moor forest types 9) Pineto - Ledetum or the Ledum forest type 10) Thujeto - Coptetum or the Lysichitum - Coptis forest type V. Flood plain forest types 11) Piceeto - Symphoricarpetum or the Symphoricarpos - Disporum forest type 12) Piceeto – Oplopanacetum a) var. populosum trichocarpae or the Ribes braeteosum - Oplopanax - Populus forest type b) var. abietosum amabilis or the Ribes bracteosum - Oplopanax - Abies amabilis forest type 13) Populeto - Loniceretum or the Lonicera - Rubus spectabilis forest type 14) Alneto - Ribisetum bracteosi or the Ribes bracteosum - Lysichitum forest type 15) Saliceto - Oenanthetum or the Lysichitum - Oenanthe forest type. The floristic structure of the phytocoenoses was studied, described and correlated with factors of the environment. Variations in the floristic and ecotopic characteristics of the units support this classification. These characteristics were used in the key proposed for identification of the forest types. Forest types as basic ecosystem units are offered for practical use. They are uniform in composition and, therefore, potentionally they require different treatments in forest management.
Due pianeti rocciosi scoperti da un team INAF
Creators: Sabrina Masiero
Publisher: name: Media Inaf
Year: 2016

«È il primo risultato che otteniamo dal nostro studio su esopianeti attorno a stelle più piccole e più fredde del Sole», dice Laura Affer dell’Osservatorio astronomico di Palermo. Il pianeta più interno potrebbe rappresentare il tassello mancante nello studio della composizione dei mondi simili alla Terra
Vita sulla Terra: è una “nata prematura”?
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2016

L’epoca nella quale l’emergenza della vita così come la conosciamo ha maggiori chance, stima uno studio di Harvard guidato da Avi Loeb, dovrebbe essere ampiamente spostata nel futuro. Il fatto che sul nostro pianeta sia comparsa così presto rappresenterebbe un’eccezione
Reformulasi Paradigma Dakwah dan Komunikasi di Era Pos-Pandemi Covid-19
Creators: name: Huda, Sokhi
Publisher: name: Zenodo
Year: 2021
Subjects: Paradigma
dakwah
komunikasi
pos-pandemi Covid-19
post-Western world

description: Era pandemi Covid-19 telah mengubah tatanan hidup masyarakat dunia dalam semua aspeknya sampai ke kemunculan ‘Post-Western World’ dan ‘Post-Western Social Sciences and Global Knowledge’. Hal ini menjadi tantangan dinamis bagi dakwah untuk menawarkan formulanya. Kajian ini berusaha menawarkan reformulasi paradigma dakwah dan komunikasi pada era pos-pandemi dengan pendekatan kualitatif dan perspektif teori paradigma Kuhn dan Ritzer. Hasil kajian ini menunjukkan, bahwa dakwah memerlukan redefinisi dan reformulasi paradigma sesuai dengan kondisi era pos-pandemi. Redefinisi dakwah menempatkan kebahagiaan kedalam pengalaman proses dakwah dan pengamalan ajaran agama, bukan dalam tujuan dakwah. Redefinisi ini dikukuhkan dalam formula paradigma baru, yaitu paradigma dakwah bahagia. Tampilannya mengedepankan identitas paradigmanya. Kinerja sistem aktivitasnya diarahkan untuk menawarkan pesan, bukan memaksakannya. Tampilan dan kinerja sistem dikemas kedalam pola-pola komunikasi yang menarik secara kreatif, inovatif, suportif, dan afirmatif dengan pemanfaatan teknologi informasi sebagai media komunikasi yang efisien. Kajian ini berargumen, bahwa dakwah tertantang untuk melakukan otokritik dan menawarkan paradigma baru komunikasinya untuk menunjang pertumbuhan hidup individu dan masyarakat pada era pos-pandemi.
title: ÐÐ¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð²ÑÑÐ¾ÐºÐ¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐ½Ð¾Ð¹ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½Ñ Ð·Ð° ÑÑÐµÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐµÐ°Ð½Ð¸Ð¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¾ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ð¹
title: Increasing the efficiency of high-tech medicine through the specialization of intensive care units
Creators: name: Ð¡ÐµÐ¼Ð¸Ð³Ð¾Ð»Ð¾Ð²ÑÐºÐ¸Ð¹, ÐÐ¸ÐºÐ¸ÑÐ°
name: ÐÐ°Ð»Ð»ÑÐ·ÐµÐº, ÐÐ°ÑÐ¸Ð½Ð°
name: ÐÐ¾ÑÐ¾Ð½Ð¸Ð½, ÐÐ¸ÑÐ°Ð¸Ð»
name: ÐÐ°Ð·ÑÑÐµÐ½ÐºÐ¾, Ð¡ÐµÑÐ³ÐµÐ¹
name: Ð¡ÐµÐ¼Ð¸Ð³Ð¾Ð»Ð¾Ð²ÑÐºÐ¸Ð¹, Ð¡Ð°Ð²Ð²Ð°
name: Ð¨Ð°Ð±Ð°Ð»Ð¸Ð½Ð°, ÐÐ°ÑÐ¸Ð½Ð°
name: ÐÐ»Ñ ÐÑÐ´Ð°Ð» ÐÑÑÑÐ°ÑÐ°, Ð¥Ð°ÑÐ°Ð½
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2022
Subjects: Ð²ÑÑÐ¾ÐºÐ¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐ½Ð°Ñ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ°Ñ Ð¿Ð¾Ð¼Ð¾ÑÑ
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Ð°Ð¾ÑÑÐ¾ÐºÐ¾ÑÐ¾Ð½Ð°ÑÐ½Ð¾Ðµ ÑÑÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÑÑÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÐºÐ¾ÑÐ¾Ð½Ð°ÑÐ½ÑÑ Ð°ÑÑÐµÑÐ¸Ð¹
High-tech medical care
cardiology
resuscitation and intensive care
Health Organization
coronary angiography
coronary artery bypass surgery
coronary artery stenting

description: ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð¾ 3 ÑÑÐ°Ð¿Ð° ÑÐ°Ð±Ð¾ÑÑ ÐºÐ°ÑÐ´Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ»ÑÐ¶Ð±Ñ Ð¼Ð½Ð¾Ð³Ð¾Ð¿ÑÐ¾ÑÐ¸Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°ÑÐ¸Ð¾Ð½Ð°ÑÐ° Ñ ÑÐ¾ÑÐºÐ¸ Ð·ÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½Ð¾Ð¹ ÑÐµÐ¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ð¹ ÑÐµÐ°Ð½Ð¸Ð¼Ð°ÑÐ¸Ð¸ Ð¸ Ð¸Ð½ÑÐµÐ½ÑÐ¸Ð²Ð½Ð¾Ð¹ ÑÐµÑÐ°Ð¿Ð¸Ð¸ ÐºÐ°ÑÐ´Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐ¸Ð»Ñ. Ð ÑÑÐµÐ´Ð½ÐµÐ¼ Ð·Ð° Ð³Ð¾Ð´ Ð¿ÑÐ¾Ð»ÐµÑÐ¸Ð²Ð°Ð»Ð¾ÑÑ Ð¸Ð½ÑÐµÐ½ÑÐ¸Ð²Ð½Ð¾ 2317 Ð¿Ð°ÑÐ¸ÐµÐ½ÑÐ¾Ð², ÑÑÐ¾ Ð½Ð° 25 % Ð²ÑÑÐµ ÐµÐ¶ÐµÐ³Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÐ¼Ð°, Ð´Ð¾ÑÑÐ¸Ð³Ð½ÑÑÐ¾Ð³Ð¾ Ð½Ð° Ð¿ÑÐµÐ´ÑÐ´ÑÑÐµÐ¼ ÑÑÐ°Ð¿Ðµ.
description: The 3 stages of the work of the cardiological service of a multidisciplinary hospital were analyzed from the point of view of the effectiveness of the reorganization of the intensive care units (ICU). On average, 2,317 patients were treated intensively per year, which is 25% higher than the annual volume achieved at the previous stage.
Tutti a caccia delle Perseidi
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2016

Arriva agosto e con esso lo sciame di meteore delle celeberrime 'lacrime di San Lorenzo'. Anche quest'anno, nuvole permettendo, le condizioni per osservare il fenomeno si preannunciano assai favorevoli. I nostri consigli per godervi al meglio questo spettacolo celeste e i principali eventi astronomici del mese
Change-point estimation under adaptive sampling
Creators: name: Lan, Yan
name: Banerjee, Moulinath
name: Michailidis, George
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistics Theory (math.ST)
subject: FOS: Mathematics
subject: 62F12, 62K99 (Primary)

description: We consider the problem of locating a jump discontinuity (change-point) in a smooth parametric regression model with a bounded covariate. It is assumed that one can sample the covariate at different values and measure the corresponding responses. Budget constraints dictate that a total of $n$ such measurements can be obtained. A multistage adaptive procedure is proposed, where at each stage an estimate of the change point is obtained and new points are sampled from its appropriately chosen neighborhood. It is shown that such procedures accelerate the rate of convergence of the least squares estimate of the change-point. Further, the asymptotic distribution of the estimate is derived using empirical processes techniques. The latter result provides guidelines on how to choose the tuning parameters of the multistage procedure in practice. The improved efficiency of the procedure is demonstrated using real and synthetic data. This problem is primarily motivated by applications in engineering systems.
description: Published in at http://dx.doi.org/10.1214/08-AOS602 the Annals of Statistics (http://www.imstat.org/aos/) by the Institute of Mathematical Statistics (http://www.imstat.org)
Juno a un punto di svolta
Creators: Francesca Aloisio
Publisher: name: Media Inaf
Year: 2016

A cinque anni dal lancio alla volta di Giove la sonda NASA Juno, partita con l’obiettivo di aiutarci a svelare i misteri nascosti sotto la coltre di nubi e gas che lo ricopre, è giunta per la prima volta alla massima distanza della sua orbita dal pianeta gigante. Ora inizia la ricaduta in avvicinamento al pianeta, con tutti gli strumenti scientifici pronti per le osservazioni.
Derived Categories of Toric Fano 3-Folds via the Frobenius Morphism
Creators: name: Bernardi, Alessandro
name: Tirabassi, Sofia
Publisher: name: arXiv
Year: 2010
Subjects: subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics
subject: 14F05, 14M25

description: In a work of Costa and Miró-Roig state the following conjecture: Every smooth complete toric Fano variety has a full strongly exceptional collection of line bundles. The goal of this article is to prove it for toric Fano 3-folds.
Niente acqua per i calanchi marziani
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2016

Si tratta di formazioni geomorfologiche che si trovano anche sulla Terra, ma che evidentemente hanno un'origine diversa. Il materiale vulcanico trovato da MRO sembra non aver mai interagito con l'acqua allo stato liquido
Reversible room-temperature magnetocaloric effect with large temperature span in antiperovskite compounds Ga1-xCMn3+x (x=0, 0.06, 0.07, and 0.08)
Creators: name: Wang, B. S.
name: Tong, P.
name: Sun, Y. P.
name: Zhu, X. B.
name: Luo, X.
name: Li, G.
name: Song, W. H.
name: Yang, Z. R.
name: Dai, J. M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The magnetic and magnetocaloric properties of Ga1-xCMn3+x have been investigated. Reversible magnetocaloric effect (MCE) occurs near the Curie temperature TC. The magnetic entropy change decreases with increasing x, though TC and magnetization increases. Meanwhile, the temperature span of vs. T plot becomes well broadened with x. Due to the competition between the broadening temperature span and decreasing, the relative cooling power (RCP) increases initially, and then decreases with increasing x. The largest RCP (2.1 J/cm3, under 45 kOe) observed when x=0.07 (TC = 296.5 K) is comparable to the contemporary magnetic refrigerant materials. Considering the reversible MCE, inexpensive and innoxious raw materials, our result suggests that Ga1-xCMn3+x can be promising candidate for magnetic refrigeration around room temperature.
description: 14 pages, 10 figure
Eine vergessen geglaubte Festung in Afrika kehrt in das Bewusstsein zurück
Creators: name: Heyden, Ulrich Van Der
Publisher: name: Burgen und Schlösser - Zeitschrift für Burgenforschung und Denkmalpflege
Year: 2022

description: Burgen und Schlösser - Zeitschrift für Burgenforschung und Denkmalpflege, Bd. 41 Nr. 2 (2000): Burgen und Schlösser - Zeitschrift für Burgenforschung und Denkmalpflege
Lack of strong completeness for stochastic flows
Creators: name: Li, Xue-Mei
name: Scheutzow, Michael
Publisher: name: arXiv
Year: 2009
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 60H10

description: It is well-known that a stochastic differential equation (SDE) on a Euclidean space driven by a Brownian motion with Lipschitz coefficients generates a stochastic flow of homeomorphisms. When the coefficients are only locally Lipschitz, then a maximal continuous flow still exists but explosion in finite time may occur. If -- in addition -- the coefficients grow at most linearly, then this flow has the property that for each fixed initial condition $x$, the solution exists for all times almost surely. If the exceptional set of measure zero can be chosen independently $x$, then the maximal flow is called {\em strongly complete}. The question, whether an SDE with locally Lipschitz continuous coefficients satisfying a linear growth condition is strongly complete was open for many years. In this paper, we construct a 2-dimensional SDE with coefficients which are even bounded (and smooth) and which is {\em not} strongly complete thus answering the question in the negative.
Effects of invasive Ageratina adenophora on mycelial growth of some important soil fungi
Creators: name: Sujan Balami
name: Thapa, Lal B
name: Jha, Sanjay Kumar
Publisher: name: Research and Development Office, Prince of Songkla University
Year: 2019
Subjects: Crofton weed
extracts
poison food technique
antifungal activity

description: Songklanakarin Journal of Science and Technology, 41, 2, 465-470
title: Ð¢ÐµÑ Ð½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ ÑÐ¿Ð¾ÑÐ¾Ð±Ð¾Ð² Ð±ÐµÑÐ¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ Ð±Ð¸Ð·Ð½ÐµÑ-ÑÐµÐ½ÑÑÐ°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¨Ð°ÑÐ¾ÑÐ½Ð°Ñ, ÐÐ»ÐµÐºÑÐ°Ð½Ð´ÑÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð±ÐµÑÐ¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
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description: Ð Ð Ð°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÑÐ¸ ÑÐ¿Ð¾ÑÐ¾Ð±Ð° Ð±ÐµÑÐ¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð½ÐµÑÑÑÐ¸Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ Ð±Ð¸Ð·Ð½ÐµÑ-ÑÐµÐ½ÑÑÐ°: Ð¾Ð´Ð¸Ð½ Ð²Ð°ÑÐ¸Ð°Ð½Ñ - Ð±Ð°ÑÐµÐ½Ð½ÑÐ¼ ÐºÑÐ°Ð½Ð¾Ð¼, Ð´Ð²Ð° Ð´ÑÑÐ³Ð¸Ñ - Ð°Ð²ÑÐ¾Ð±ÐµÑÐ¾Ð½Ð¾Ð½Ð°ÑÐ¾ÑÐ°Ð¼Ð¸. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð¿Ð¾Ð´Ð±Ð¾Ñ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¼Ð°ÑÐ¸Ð½, ÑÐ°ÑÑÐµÑ Ð¸Ñ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÐµÐ¹. ÐÑÑÐ¾Ð´Ñ Ð¸Ð· ÑÑÐ¾Ð³Ð¾, Ð±ÑÐ»Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ ÑÑÐ¾ÐºÐ¸ Ð¸ ÑÑÐµÐ¼Ñ Ð±ÐµÑÐ¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹, Ð¿Ð¾ÑÐ»Ðµ ÑÐµÐ³Ð¾ ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ð° ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÑ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÑÐ¸Ñ ÑÐ°Ð±Ð¾Ñ. Ð¡Ð´ÐµÐ»Ð°Ð½ Ð²ÑÐ²Ð¾Ð´ Ð¾Ð± ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð°Ð²ÑÐ¾Ð±ÐµÑÐ¾Ð½Ð¾Ð½Ð°ÑÐ¾ÑÐ¾Ð².
Buchi neri fuori dal coro
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2016

Grazie al potere risolutivo del telescopio spaziale per raggi X NuSTAR della NASA, un team internazionale di astrofisici, fra i quali Andrea Comastri e Luca Zappacosta dell’INAF, è riuscito a risolvere circa il 35 percento del fondo cosmico di raggi X ad alta energia
Theory of itinerant magnetic excitations in the SDW phase of iron-based superconductors
Creators: name: Knolle, J.
name: Eremin, I.
name: Chubukov, A. V.
name: Moessner, R.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We argue that salient experimental features of the magnetic excitations in the SDW phase of iron-based superconductors can be understood within an itinerant model. We identify a minimal itinerant model and use a multi-band RPA treatment of the dynamical spin susceptibility. Weakly-damped spin-waves are found near the ordering momentum and it is shown how they dissolve into the particle-hole continuum. We show that ellipticity of the electron bands accounts for the anisotropy of the spin waves along different crystallographic directions and the gap at the momentum conjugated to the ordering one. We argue that our theory agrees well with the neutron scattering data.
description: 6 pages, 3 figures
On fuzzy quasi-prime ideals in near left almost rings
Creators: name: Pairote Yiarayong
Publisher: name: Research and Development Office, Prince of Songkla University
Year: 2019
Subjects: nLA-ring
fuzzy quasi-prime
fuzzy completely prime
weakly fuzzy quasi-prime
weakly fuzzy completely prime

description: Songklanakarin Journal of Science and Technology, 41, 2, 471-482
Dal Brasile allo spazio con le AstrOlimpiadi NASA
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2016

Al via AstrOlympics, un’iniziativa didattica ideata dal team di comunicazione del telescopio spaziale Chandra per mettere a confronto le incredibili acrobazie e prestazioni degli atleti olimpici con i fenomeni più spettacolari osservati nell’Universo.
Physical properties of galaxies and their evolution in the VIMOS VLT Deep Survey. II. Extending the mass-metallicity relation to the range z=0.89-1.24
Creators: name: Perez-Montero, E.
name: Contini, T.
name: Lamareille, F.
name: Brinchmann, J.
name: Walcher, C. J.
name: Charlot, S.
name: Bolzonella, M.
name: Pozzetti, L.
name: Bottini, D.
name: Garilli, B.
name: Brun, V. Le
name: Fevre, O. Le
name: Maccagni, D.
name: Scaramella, R.
name: Scodeggio, M.
name: Tresse, L.
name: Vettolani, G.
name: Zanichelli, A.
name: Adami, C.
name: Arnouts, S.
name: Bardelli, S.
name: Cappi, A.
name: Ciliegi, P.
name: Foucaud, S.
name: Franzetti, P.
name: Gavignaud, I.
name: Guzzo, L.
name: Ilbert, O.
name: Iovino, A.
name: McCracken, H. J.
name: Marano, B.
name: Marinoni, C.
name: Mazure, A.
name: Meneux, B.
name: Merighi, R.
name: Paltani, S.
name: Pello, R.
name: Pollo, A.
name: Radovich, M.
name: Vergani, D.
name: Zamorani, G.
name: Zucca, E.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Aims. We present a continuation of our study about the relation between stellar mass and gas-phase metallicity in the VIMOS VLT Deep Survey (VVDS). In this work we extend the determination of metallicities up to redshift = 1.24 for a sample of 42 star-forming galaxies with a mean redshift value of 0.99. Methods. For a selected sample of emission-line galaxies, we use both diagnostic diagrams and empirical calibrations based on [OII] emission lines along with the empirical relation between the intensities of the [OIII] and [NeIII] emission lines and the theoretical ratios between Balmer recombination emission lines to identify star-forming galaxies and to derive their metallicities. We derive stellar masses by fitting the whole spectral energy distribution with a set of stellar population synthesis models. Results. These new methods allow us to extend the mass-metallicity relation to higher redshift. We show that the metallicity determinations are consistent with more established strong-line methods. Taken together this allows us to study the evolution of the mass-metallicity relation up to z = 1.24 with good control of systematic uncertainties. We find an evolution with redshift of the average metallicity of galaxies very similar to those reported in the literature: for a given stellar mass, galaxies at z = 1 have, on average, a metallicity = 0.3 dex lower than galaxies in the local universe. However we do not see any significant metallicity evolution between redshifts z = 0.7 (Paper I) and z = 1.0 (this paper). We find also the same flattening of the mass-metallicity relation for the most massive galaxies as reported in Paper I at lower redshifts, but again no apparent evolution of the slope is seen between z = 0.7 and z = 1.0.
description: 9 pages and 8 figures. In press in Astronomy & Astrophysics
Distruzione preventiva per scongiurare l’impatto
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2016

Simulando al computer strategie di difesa con testate nucleari, un team di ricercatori russi è giunto a concludere che, se l’asteroide venisse bombardato e disintegrato mentre si sta allontanando dalla Terra, eventuali frammenti radioattivi non rappresenterebbero una minaccia
Rosetta: come nascono le comete
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

Uno studio condotto sui dati raccolti dalla sonda Rosetta e da missioni spaziali precedenti di flyby attorno a nuclei cometari mostra che le comete si formano dall’aggregazione successiva a bassa velocità di grani di materiale primordiale. Marco Fulle (INAF): «L’unico modo per capire una cometa è ripetere una missione complessa almeno quanto Rosetta»
Movement behaviour of the common frog (Rana temporaria) in an anthropized mountain landscape: integrated step selection analysis of GPS tracking data
Creators: name: Boncourt, Etienne
name: Reineking, Björn
name: Chambonnet, Gabriel
name: Gaucherand, Stéphanie
Publisher: name: Brill Online
Year: 2023
Subjects: classificationCode: 310399
subject: Ecology not elsewhere classified

description: Movement is a key aspect of amphibian ecology as the life cycle of many species involves seasonal dispersal and migration. However, there is still a lack of knowledge about how amphibians move across landscapes in relation to landscape structure and resource availability. Modern lightweight GPS loggers and associated statistical tools offer new perspectives to fill this gap. We tracked the movements of 20 adult European common frogs (Rana temporaria) in a human-transformed mountain landscape during summer using GPS tags programmed with a constant 4-hour time interval between fixes. Using integrated step-selection analysis, we demonstrate firstly that frogs strongly selected aquatic habitats over open grassland. Second, ski runs have a negative effect on frogs, indicated by longer movement steps. Weather (air temperature and rain) had no effect on frog movements. These results constitute a promising first step towards studying anuran movement in relation to landscape structure at fine spatial and temporal scales.
Electronic origin of the incommensurate modulation in the structure of phosphorus IV
Creators: name: Degtyareva, Valentina F.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: An incommensurate modulated structure was found recently in a light group V element phosphorous in the phase P-IV stable in the pressure range 107-137 GPa. We consider configurations of the Brillouin zone and Fermi sphere within a nearly-free-electron model in order to analyze the importance of these configurations for the crystal structure energy. For the phase P-IV with the base-centered orthorhombic structure, oC2, we consider a commensurate approximant with an 11-fold supercell along the c-axis and a modulation wave vector equal 3/11 which is close to the experimentally observed value of 0.267. Atomic shifts due to the modulation result in appearance of satellite reflections and hence in a formation of additional Brillouin zone planes. The stability of this structure is attributed to the lowering of the electronic band structure energy due to Brillouin zone - Fermi surface interactions.
title: Ð¡Ð¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð°Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐºÐ¾ÑÐ¾ÑÑÐ½Ð¾Ð¹ Ð²ÑÐ½Ð¾ÑÐ»Ð¸Ð²Ð¾ÑÑÐ¸ Ð²ÑÑÐ¾ÐºÐ¾ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÑÑ ÑÐºÐ²Ð¾Ð½Ð´Ð¸ÑÑÐ¾Ð² Ð½Ð° Ð¿ÑÐµÐ´ÑÐ¾ÑÐµÐ²Ð½Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼ ÑÑÐ°Ð¿Ðµ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸
title: A special technique for the development of high-speed endurance of highly qualified taekwondo athletes at the pre-competition stage of training
Creators: name: Ð¡Ð¸Ð¼Ð°ÐºÐ¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
name: "Ð¡Ð¿Ð¾ÑÑ, ÑÐµÐ»Ð¾Ð²ÐµÐº, Ð·Ð´Ð¾ÑÐ¾Ð²ÑÐµ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð½Ð°ÑÑÐ½ÑÐ¹ ÐºÐ¾Ð½Ð³ÑÐµÑÑ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2023
Subjects: ÑÑ ÑÐºÐ²Ð¾Ð½Ð´Ð¾
ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð°Ñ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ°Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ°
ÑÐºÐ¾ÑÐ¾ÑÑÐ½Ð°Ñ Ð²ÑÐ½Ð¾ÑÐ»Ð¸Ð²Ð¾ÑÑÑ
Ð¿ÑÐµÐ´ÑÐ¾ÑÐµÐ²Ð½Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½ÑÐ¹ ÑÑÐ°Ð¿ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸
taekwondo
special physical training
speed endurance
pre-competitive stage of training

description: Ð Ð½Ð°ÑÑÐ¾ÑÑÐµÐµ Ð²ÑÐµÐ¼Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ° Ð²ÑÑÐ¾ÐºÐ¾ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÑÑÑÐºÐ²Ð¾Ð½Ð´Ð¸ÑÑÐ¾Ð² Ðº Ð¾ÑÐ²ÐµÑÑÑÐ²ÐµÐ½Ð½ÑÐ¼ ÑÐ¾ÑÐµÐ²Ð½Ð¾Ð²Ð°Ð½Ð¸ÑÐ¼ ÑÑÐµÐ±ÑÐµÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¸Ðº, Ð¾ÑÐ²ÐµÑÐ°ÑÑÐ¸Ñ Ð¿Ð¾ÑÐ»ÐµÐ´Ð½Ð¸Ð¼ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸ÑÐ¼ Ð² Ð¿ÑÐ°Ð²Ð¸Ð»Ð°Ñ ÑÐ¾ÑÐµÐ²Ð½Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð¿Ð¾
Ð²Ð¸Ð´Ð°Ð¼ ÑÐ¿Ð¾ÑÑÐ°. ÐÐ°Ð½Ð½ÑÐ¹ ÑÐ°ÐºÑ Ð¿ÑÐµÐ´Ð¿Ð¾Ð»Ð°Ð³Ð°ÐµÑ Ð½Ðµ ÑÐ¾Ð»ÑÐºÐ¾ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÑÐ¾Ð²Ð½Ñ ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¼Ð°ÑÑÐµÑÑÑÐ²Ð° ÑÐ¿Ð¾ÑÑÑÐ¼ÐµÐ½Ð¾Ð², Ð½Ð¾ Ð¸ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ðµ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ Ð²ÑÐ½Ð¾ÑÐ»Ð¸Ð²Ð¾ÑÑÐ¸. ÐÐ¾ÑÑÐ¸ÑÑ ÑÑÐ¾Ð³Ð¾ Ð¼Ð¾Ð¶Ð½Ð¾ Ð·Ð° ÑÑÑÑ Ð³ÑÐ°Ð¼Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐµÐ½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð½Ð° Ð¿ÑÐµÐ´ÑÐ¾ÑÐµÐ²Ð½Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼ ÑÑÐ°Ð¿Ðµ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸.
description: Currently, the preparation of highly qualified taekwondo athletes for responsible competitions requires the development and implementation of special techniques that meet the latest changes in the rules of competitions in sports. This fact implies not only an increase in the level of technical and tactical skills of athletes, but also an increase in special endurance. This can be achieved through competent planning of the training process at the pre-competition stage of preparation.
La scarpa giusta per la Luna
Creators: Francesca Aloisio
Publisher: name: Media Inaf
Year: 2016

Avete presente i poveri astronauti che intabarrati nelle tute spaziali camminano goffamente sul suolo lunare? La loro mobilità con indosso l’attrezzatura è molto limitata e si sono anche verificati dei capitomboli lunari, soprattutto a causa della poca sensibilità che le calzature attualmente in uso consentono. La soluzione è semplice e già in avanzata fase di sperimentazione. D’altra parte si sa, per camminare (ovunque), ci vogliono delle scarpe comode
The proton and deuteron F_2 structure function at low Q^2
Creators: name: Tvaskis, V.
name: Arrington, J.
name: Asaturyan, R.
name: Baker, O. K.
name: Blok, H. P.
name: Bosted, P.
name: Boswell, M.
name: Bruell, A.
name: Christy, M. E.
name: Cochran, A.
name: Ent, R.
name: Filippone, B. W.
name: Gasparian, A.
name: Keppel, C. E.
name: Kinney, E.
name: Lapikás, L.
name: Lorenzon, W.
name: Mack, D. J.
name: Mammei, J.
name: Martin, J. W.
name: Mkrtchyan, H.
name: Niculescu, I.
name: Piercey, R. B.
name: Potterveld, D. H.
name: Smith, G.
name: Spurlock, K.
name: van der Steenhoven, G.
name: Stepanyan, S.
name: Tadevosian, V.
name: Wood, S. A.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Measurements of the proton and deuteron $F_2$ structure functions are presented. The data, taken at Jefferson Lab Hall C, span the four-momentum transfer range $0.06 < Q^2 < 2.8$ GeV$^2$, and Bjorken $x$ values from 0.009 to 0.45, thus extending the knowledge of $F_2$ to low values of $Q^2$ at low $x$. Next-to-next-to-leading order calculations using recent parton distribution functions start to deviate from the data for $Q^2<2$ GeV$^2$ at the low and high $x$-values. Down to the lowest value of $Q^2$, the structure function is in good agreement with a parameterization of $F_2$ based on data that have been taken at much higher values of $Q^2$ or much lower values of $x$, and which is constrained by data at the photon point. The ratio of the deuteron and proton structure functions at low $x$ remains well described by a logarithmic dependence on $Q^2$ at low $Q^2$.
description: 3 figures, submitted paper