cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Ð¤Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½ÑÐ° Ð¸ Ð¾ÑÐµÐ½ÐºÐ° ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¶ÐµÐ½ÑÐºÐ¾Ð¹ ÐºÐ¾Ð¶Ð°Ð½Ð¾Ð¹ Ð¾Ð±ÑÐ²Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÐºÐ¾Ð²Ð°, 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: Ð¶ÐµÐ½ÑÐºÐ°Ñ ÐºÐ¾Ð¶Ð°Ð½Ð°Ñ Ð¾Ð±ÑÐ²Ñ
ÐºÐ°ÑÐµÑÑÐ²Ð¾ Ð¾Ð±ÑÐ²Ð¸
ÑÐ¾ÑÐ³Ð¾Ð²ÑÐ¹ Ð¿ÑÐ¾ÑÐµÑÑ
Ð¿Ð¾ÑÑÐ°Ð²ÑÐ¸ÐºÐ¸

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«ÐÐ¾Ð²ÑÐ¹ ÐÐ¸ÑÂ». Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½ÑÐ° Ð¸ Ð¾ÑÐµÐ½ÐºÐ° ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¶ÐµÐ½ÑÐºÐ¾Ð¹ ÐºÐ¾Ð¶Ð°Ð½Ð¾Ð¹ Ð¾Ð±ÑÐ²Ð¸. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¿Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾Ð¹ ÑÐµÐ»Ð¸ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½ÑÐ¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð´Ð»Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° Ð¾Ð±ÑÐ²Ð¸, Ð¿ÑÐ¾ÑÐµÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°, ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ Ð¸ Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½Ñ, Ð¿Ð¾ÑÑÐµÐ±Ð¸ÑÐµÐ»ÑÑÐºÐ¸Ðµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð¸Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° ÐºÐ¾Ð¶Ð°Ð½Ð¾Ð¹ Ð¾Ð±ÑÐ²Ð¸. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½ Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½Ñ Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¾Ð±ÑÐ²Ð¸, ÑÐµÐ°Ð»Ð¸Ð·ÑÐµÐ¼Ð¾Ð¹ Ð² ÐÐÐ Â«ÐÐ¾Ð²ÑÐ¹ ÐÐ¸ÑÂ» Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð° Ð¾Ð±ÑÐ²Ð¸ Â«FreedomÂ». ÐÑÐ°ÑÐ°ÐºÑÐµÑÐ¸Ð·Ð¾Ð²Ð°Ð½Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸, Ð¸Ð·ÑÑÐµÐ½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð³Ð¾ Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð², Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½ÑÑ ÑÐ²ÑÐ·ÐµÐ¹ Ð¸ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹ Ð¿Ð¾ Ð¿Ð¾ÑÑÐ°Ð²ÐºÐ°Ð¼ ÑÐ¾Ð²Ð°ÑÐ¾Ð². ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾Ð±ÑÐ²Ð¸ Ð² ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¼ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸Ð»Ð¸ÑÑ Ð² Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ. ÐÐ»Ñ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² Ð±ÑÐ»Ð¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ñ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð°Ñ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ñ, ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð°Ñ Ð¸ ÑÑÐµÐ±Ð½Ð°Ñ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ° Ð¿Ð¾ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐµÐ¼Ðµ, Ð° ÑÐ°ÐºÐ¶Ðµ ÐÐ½ÑÐµÑÐ½ÐµÑ-ÑÐµÑÑÑÑÑ.
La natura delle antiche nubi di gas
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2016

Osservazioni profonde realizzate con i maggiori telescopi terrestri hanno permesso di individuare antiche nubi di gas freddo. I risultati di questo studio, riportati su ApJ Letters, forniscono nuovi indizi per la soluzione di un vecchio problema che riguarda la natura dei cosiddetti ‘damped Lyman alpha systems’
Theory of conductivity modulation in semiconductors
Creators: name: Nishi, Ronald Yutaka
Publisher: name: University of British Columbia
Year: 2011

description: The theory of conductivity modulation in semiconductors and the conditions under which negative resistance can be obtained are investigated. The ambipolar transport equation is derived for one-dimensional flow in a two-terminal homogeneous semiconductor with no trapping and no temperature gradients. Charge neutrality is assumed in the majority of the models studied. A phenomenological model is considered first to show how conductivity modulation can lead to negative resistance. Since the general problem of carrier transport with drift and diffusion currents is difficult, the models investigated are mainly concerned with either drift or diffusion as the dominant transport mechanism. For a unipolar space-charge limited drift model, negative resistance in frequency bands is found. For bipolar, neutral drift models, negative resistance is found under special conditions for the case of no recombination and for recombination with a carrier lifetime increasing with carrier density. For recombination with a constant lifetime, the bipolar drift model gives current-voltage characteristics of the form: J α V at low injection levels, J α V² at high injection levels, and J α V³ at very high injection levels. Space charge is important in the cube law case. Models ignoring diffusion are shown to be valid only for extrinsic semiconductors. Bipolar neutral flow with equal carrier densities leads to diffusion solutions of the ambipolar equation. This case applies to extrinsic material at high injection levels as well as to intrinsic material and is found to exhibit negative resistance under certain conditions. The most favourable situation is the case where the carrier lifetime increases with carrier density. The dependence of the lifetime with carrier density determines the possibility of defining completely a negative resistance model. It is found that the properties of the contacts are important in attaining negative resistance. Contacts and their properties are briefly discussed in relation to the carrier density boundary conditions. Avalanche injection and its relation to the conductivity modulation problem is considered. Several outstanding problems, both theoretical and experimental, arising from this thesis are outlined in the last chapter.
title: ÐÐ¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð°
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¡Ð¾ÑÐ¾ÐºÐ¸Ð½, 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: 2018
Subjects: Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½
Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¿Ð»Ð°Ð½
ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð°Ñ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐ¸Ñ
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¹ Ð¿Ð»Ð°Ð½

description: 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° Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð° ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð° Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¸Ð½ÑÐµÑÐ½ÐµÑ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð° Â«Ð¡ÑÐ¸Ð»Ñ Ð¶Ð¸Ð·Ð½Ð¸Â». Ð Ð¿ÑÐ¾ÑÐµÑÑÐµ ÑÐ°Ð±Ð¾ÑÑ Ð½Ð°Ð¼Ð¸ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð°ÑÐ¿ÐµÐºÑÑ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð° ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð¿ÑÐ¸ ÐµÐ³Ð¾ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ð¸, Ð² ÐºÐ¾ÑÐ¾ÑÑÑ Ð±ÑÐ»Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÑÐµÐ¼Ñ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð±Ð¸Ð·Ð½ÐµÑÐ°. ÐÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð°ÑÐ¿ÐµÐºÑÑ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð±Ð¸Ð·Ð½ÐµÑÐ° Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸, Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÐºÐ¾ÑÐ¾ÑÑÑ Ð¼Ñ ÑÐ¼Ð¾Ð³Ð»Ð¸ ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÑÐ¸ÑÐ¾Ð²Ð°ÑÑ Ð½Ð°Ñ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½ Ð½Ð° ÑÑÐ½ÐºÐµ Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð°ÑÐ¿ÐµÐºÑÐ°Ñ, Ð¼Ñ Ð¿ÑÐ¸ÑÑÑÐ¿Ð¸Ð»Ð¸ Ðº ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð°. ÐÐ¿Ð¸ÑÐ°Ð½Ð¸Ðµ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð° ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð¸Ð· ÐºÑÐ°ÑÐºÐ¾Ð¹ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ð¸ ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð¢Ð¾Ð²Ð°ÑÑ Ð¸ ÑÑÐ»ÑÐ³Ð¸, Ð¿Ð¾Ð¼ÐµÑÐµÐ½Ð¸Ðµ Ð¸ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ, ÐºÐ¾ÑÐ¾ÑÑÐµ ÑÑÐ°ÑÑÐ²ÑÑÑ Ð² ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐ²Ð»ÑÑÑÑÑ Ð³Ð»Ð°Ð²Ð½ÑÐ¼ Ð·Ð²ÐµÐ½Ð¾Ð¼ Ð²ÑÐµÐ³Ð¾ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾Ð³Ð¾ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð°. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐ½ÐºÐ° Ð¸ ÑÐ¾Ð·Ð´Ð°Ð½Ð½ÑÐ¹ ÑÐµÐºÐ»Ð°Ð¼Ð½ÑÐ¹ Ð¿Ð»Ð°Ð½ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ Ð´ÐµÑÐ¶Ð°ÑÑÑÑ Ð½Ð°ÑÐµÐ¼Ñ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ñ Ð½Ð° ÑÑÐ½ÐºÐµ. ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¿Ð»Ð°Ð½ Ð¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¹ Ð¿Ð»Ð°Ð½ Ð½Ð°ÑÐµÐ¹ ÑÐ°Ð±Ð¾ÑÑ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ð»Ð¸ ÑÐ±ÐµÐ´Ð¸ÑÑÑÑ Ð² ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸ ÑÐµÐ»ÐµÑÐ¾Ð¾Ð±ÑÐ°Ð·Ð½Ð¾ÑÑÑ Ð½Ð°ÑÐµÐ³Ð¾ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð°. ÐÐ¾Ð·Ð²Ð¾Ð»Ð¸Ð»Ð¸ ÑÐ¾Ð·Ð´Ð°ÑÑ Ð¿Ð¾Ð»Ð½ÑÑ ÐºÐ°ÑÑÐ¸Ð½Ñ Ð½Ð¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
I gemelli di Eta Carinae
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2016

Nel 2015 un team di esperti ha trovato ben due candidati nella galassia M83 e altri tre oggetti candidati nelle galassie NGC 6946, M101 e M51. Questi cinque oggetti imitano le proprietà ottiche e infrarosse di Eta Carinae, indicando che ognuno contiene molto probabilmente una stella molto massiccia sepolta da un alone di gas e polvere 5 o 10 volte la massa del Sole
Conformational phase diagram for polymers adsorbed at ultrathin nanowires
Creators: name: Vogel, Thomas
name: Bachmann, Michael
Publisher: name: arXiv
Year: 2010
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We study the conformational behavior of a polymer adsorbed at an attractive nanostring and construct the complete structural phase diagram in dependence of the binding strength and effective thickness of the string. For this purpose, Monte Carlo optimization techniques are employed to identify lowest-energy structures for a coarse-grained hybrid polymer-wire model. Among the representative conformations in the different phases are, for example, compact droplets attached to the string and also nanotube-like monolayer films wrapping the string in a very ordered way. We here systematically analyze low-energy shapes and structural order parameters to elucidate the transitions between the structural phases.
Buchi neri ad occhio nudo
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

Un team internazionale di scienziati, guidato da ricercatori dell’Università di Kyoto, afferma che i buchi neri possono essere osservati anche nella banda visibile. Lo studio ha riguardato V404 Cygni, un sistema binario che contiene un buco nero, ed è stato condotto da una rete mondiale di telescopi da Terra e satellitari. I risultati sono apparsi oggi sulla rivista Nature
Inclusion4Schools final Glossary
Creators: name: Sípos, Flórián
name: Toth, Tamás
name: Bogdan, Milán
name: Kioupkiolis, Alexandros
name: Pechtelidis, Jannis
name: Hadjar, Andreas
Publisher: name: Zenodo
Year: 2025

description: The uploaded Glossary offers clear and accessible explanations of key concepts related to education, inequality, inclusion, and community engagement in education. It covers the following main themes in everyday language. The document overall promotes understanding that addressing educational inequalities requires systemic change, inclusive practices, and community involvement, emphasising a broader societal impact beyond individual classrooms.
Opportunità dell’ammasso globulare
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2016

Uno studio recente, presentato oggi al 227° meeting dell’American Astronomical Society, suggerisce che gli ammassi globulari, sistemi stellari molto densi e compatti che risalgono all’epoca di formazione della Via Lattea, potrebbero rappresentare luoghi particolarmente speciali dove cercare pianeti potenzialmente abitabili. Lo scopo è quello di individuare la presenza di segnali artificiali generati da qualche civiltà intelligente
Notebook for revealing the interlevel dependence structure of categorical inputs with kernel model selection - application to cyclone-induced wave modelling
Creators: name: Jeremy, Rohmer
Publisher: name: Zenodo
Year: 2022
Subjects: Categorical variables; Computationally intensive simulator; Metamodel; Kriging; Model selection

description: Jupyter Notebook (file named 'notebook_EMS_cycloneApplicationCase.ipynb') to showcase the implementation of Gaussian process models using mixed continuous/categorical inputs variables based on Roustant et al. (2020)'s methodological developments. The supporting test case is based on the modelling study for cyclone-induced waves at Reunion Island (Rohmer et al., 2016 within the ANR-funded project SPICY http://spicy.brgm.fr/fr), and corresponds to application case 1 of Rohmer et al. (2022). To re-use the present data, please contact Jeremy Rohmer, BRGM (j.rohmer@brgm.fr). The design of numerical experiments corresponds to the ascii file named 'scenarios.txt'. The corresponding numerical results correspond to the ascii file named 'Hs_chemin_correc.txt'. The categorical input corresponds to the index assigned to a cyclone track (denoted Traj). Five scalar inputs corresponding to the cyclone chracteristics are taken into account as well (maximum wind speed, distance to the island center, etc.). The variable of interest is the maximum wave height at Sainte Suzanne city located in the NE of the island. Calculations are performed using R package kergp https://cran.r-project.org/web/packages/kergp/index.html. The notebook also provides the R scripts (file named 'utils.R') that can easily be adapted to any other application case. To speed up the calculation, a RData file named 'precalculated_study_cyclone.RData' is provided and contains precalculated results.
description: {"references": ["Rohmer J., Lecacheux S., Pedreros R., Quetelard H., Bonnardot F., and Idier D. (2016). \"Dynamic parameter sensitivity in numerical modelling of cyclone-induced waves: a multi-look approach using advanced meta-modelling techniques\".\u00a0Natural Hazards, 84, 1765\u20131792", "Rohmer J., Roustant, O., Lecacheux S., Manceau J.-C. (2022). \"Revealing the interlevel dependence structure of categorical inputs in numerical environmental simulations with kernel model selection\".\u00a0Environmental modelling and software, under revision", "Roustant, O., Padonou, E., Deville, Y., Cl\u00e9ment, A., Perrin, G., Giorla, J., Wynn, H., 2020. \"Group kernels for Gaussian process metamodels with categorical inputs\". SIAM/ASA Journal on Uncertainty Quantification 8(2), 775-806"]}
Stelle in formazione viste da VLA
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2016

Le immagini di questa ricerca hanno richiesto 264 ore di osservazione nella Nube di Perseo che contiene materiale pari a 10.000 soli. Si tratta di un laboratorio importante per gli astronomi che cercano di capire le fasi di formazione stellare
State diagrams for harmonically trapped bosons in optical lattices
Creators: name: Rigol, Marcos
name: Batrouni, George G.
name: Rousseau, Valery G.
name: Scalettar, Richard T.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: Quantum Gases (cond-mat.quant-gas)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We use quantum Monte Carlo simulations to obtain zero-temperature state diagrams for strongly correlated lattice bosons in one and two dimensions under the influence of a harmonic confining potential. Since harmonic traps generate a coexistence of superfluid and Mott insulating domains, we use local quantities such as the quantum fluctuations of the density and a local compressibility to identify the phases present in the inhomogeneous density profiles. We emphasize the use of the "characteristic density" to produce a state diagram that is relevant to experimental optical lattice systems, regardless of the number of bosons or trap curvature and of the validity of the local-density approximation. We show that the critical value of U/t at which Mott insulating domains appear in the trap depends on the filling in the system, and it is in general greater than the value in the homogeneous system. Recent experimental results by Spielman et al. [Phys. Rev. Lett. 100, 120402 (2008)] are analyzed in the context of our two-dimensional state diagram, and shown to exhibit a value for the critical point in good agreement with simulations. We also study the effects of finite, but low (T
description: 10 pages, 11 figures, published version
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÐºÐ¾Ð´Ð¾Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÐ° ÐºÐ»Ð¸ÐµÐ½ÑÐ° RESTful ÑÐ»ÑÐ¶Ð± Ð´Ð»Ñ Python.
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÐ»ÑÐºÐ¾Ð²Ð°, ÐÐºÐ°ÑÐµÑ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: ÐºÐ¾Ð´Ð¾Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾Ñ
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Andromeda ai raggi X
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2016

Grazie al telescopio spaziale NuSTAR della NASA è stato possibile osservare una frazione importante della galassia gemella Andromeda e in particolare di studiare nel dettaglio binarie X per cercare di comprendere il ruolo da esse svolto nel riscaldamento del gas intergalattico all'alba dell'universo
Mancano stelle attorno al buco nero
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2016

… e venne chiamata Due Cuori: la galassia SDSS J1126 + 2944 presenta una coppia di buchi neri supermassicci al proprio interno, residuo della fusione di due galassie più piccole. Ora si è scoperto che uno dei due “cuori” è stranamente spoglio di stelle circostanti e, magari, non è quel gigante che si credeva
Atom interferometry tests of local Lorentz invariance in gravity and electrodynamics
Creators: name: Chung, Keng-Yeow
name: Chiow, Sheng-wey
name: Herrmann, Sven
name: Chu, Steven
name: Mueller, Holger
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We present atom-interferometer tests of the local Lorentz invariance of post-Newtonian gravity. An experiment probing for anomalous vertical gravity on Earth, which has already been performed by us, uses the highest-resolution atomic gravimeter so far. The influence of Lorentz violation in electrodynamics is also taken into account, resulting in combined bounds on Lorentz violation in gravity and electrodynamics. Expressed within the standard model extension or Nordtvedt's anisotropic universe model, we limit twelve linear combinations of seven coefficients for Lorentz violation at the part per billion level, from which we derive limits on six coefficients (and seven when taking into account additional data from lunar laser ranging). We also discuss the use of horizontal interferometers, including atom-chip or guided-atom devices, which potentially allow the use of longer coherence times in order to achieve higher sensitivity.
description: Reference added; corrected factor of 2 in Tab. IV and V. 12 pages, 4 figures, 6 tables
L’astrosismologia a caccia di campi magnetici
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

Grazie ai dati raccolti dalla missione Kepler, un team internazionale di astronomi è stato in grado di osservare nel dettaglio un esteso set di stelle con masse da 1.5 a 2 volte quella del Sole. Con uno studio di astrosismologia su queste stelle hanno concluso che circa il 60% di loro ospita campi magnetici intensi al loro interno (contro lo 0-5% delle stime precedenti). Importanti le implicazioni sugli studi di evoluzione stellare
КАТТА МЕВАЛИ ПУШТИ РАНГЛИ ПОМИДОР НАВЛАРИ СЕЛЕКЦИЯСИ УЧУН БОШЛАНҒИЧ МАНБА
Creators: name: Алматов, Бахром
name: Арамов, Музаффар
Publisher: name: Zenodo
Year: 2025

description: Мақолада 22 та катта мевали пушти рангли помидор нав намуналарини муҳим хўжалик белгилари бўйича баҳолаш натижалари келтирилган. Қимматли хўжалик белгиларини ўзида мужассамлаштирган, умумий ва эртаги ҳосилдорлиги юқори  NP-7, Вельможа, NA-17, E-50, Дархон, Новичок розовый, F1 Розовый  десертный  навлари ажратилган ва селекция ишлари учун бошланғич манба сифатида тавсия этилган.
Orologio stellare da ricalibrare
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2016

Astronomi del Carniege Institute hanno ricontrollato, grazie ai dati del satellite Kepler, il meccanismo di determinazione dell'età stellare, chiamato girocronologia, il calcolo dell'età stellare sulla base della loro velocità di rotazione, scoprendo che andrebbe ricalibrato
Inhomogeneities in the Universe with exact solutions of General Relativity
Creators: name: Célérier, Marie-Noëlle
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Physics (physics.gen-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: It is commonly stated that we have entered the era of precision cosmology in which a number of important observations have reached a degree of precision, and a level of agreement with theory, that is comparable with many Earth-based physics experiments. One of the consequences is the need to examine at what point our usual, well-worn assumption of homogeneity associated to the use of perturbation theory begins to compromise the accuracy of our models. It is now a widely accepted fact that the effect of the inhomogeneities observed in the Universe cannot be ignored when one wants to construct an accurate cosmological model. Well-established physics can explain several of the observed phenomena without introducing highly speculative elements, like dark matter, dark energy, exponential expansion at densities never attained in any experiment (i.e. inflation), and the like. Two main classes of methods are currently used to deal with these issues. Averaging, sometimes linked to fitting procedures a la Stoegger and Ellis, provide us with one promising way of solving the problem. Another approach is the use of exact inhomogeneous solutions of General Relativity. This will be developed here.
description: 13 pages, 6 figures, to be published in the proceedings of the Invisible Universe International Conference, held in Paris, 29 June - 3 July 2009, eds. J.-M. Alimi, A. Fuzfa and P.-S. Corasaniti
Regional Modelling of the Southern African Geomagnetic Field using Harmonic Splines
Creators: name: Geese, Anne
name: Hayn, Michael
name: Lesur, Vincent
name: Mandea, Mioara
Publisher: name: arXiv
Year: 2010
Subjects: subject: Geophysics (physics.geo-ph)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: FOS: Physical sciences

description: Over the southern African region the geomagnetic field is weak and changes rapidly. For this area series of geomagnetic field measurements exist since the 1950s. We take advantage of the existing repeat station surveys and observatory annual means, and clean these data sets by eliminating jumps and minimising external field contributions in the original time series. This unique data set allows us to obtain a detailed view of the geomagnetic field behaviour in space and time by computing a regional model. For this, we use a system of representation similar to harmonic splines. Initially, the technique is systematically tested on synthetic data. After systematically testing the method on synthetic data, we derive a model for 1961 to 2001 that gives a detailed view of the fast changes of the geomagnetic field in this region.
description: submitted to GJI
Il migliore test per la relatività generale
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2016

Secondo uno studio pubblicato su Physical Review Letters, i brevi, rari lampi radio veloci rappresentano un ottimo test, fino a 100 volte migliore rispetto ai metodi che si basano sui lampi gamma, per verificare i principi che stanno alla base della teoria della relatività generale. L’articolo ha ricevuto una particolare attenzione da parte degli editori grazie alla sua importanza, innovazione e attrattiva
3 Approaches for the Year of Open Science
Creators: name: Clatterbuck, Corey
name: Fenwick, Ileana
name: London, Josh
name: Lopez, Luis
name: Nickles, Cassandra
name: Rios, Adyan
name: Butland, Stefanie
name: Lowndes, Julia Stewart
name: Robinson, Erin
Publisher: name: Zenodo
Year: 2023
Subjects: Open Science
ESIP
NASA
NOAA
Openscapes

description: At the 2023 ESIP Winter Meeting, “Opening Doors to Open Science”, we held a session called “Better Science for Future Us: Openscapes stories and approaches for the Year of Open Science” with speakers from University of North Carolina (UNC), National Oceanic and Atmospheric Administration (NOAA) Fisheries, California Water Boards, NASA’s National Snow and Ice Data Center, and NASA’s Physical Oceanography Distributed Active Archive Center. The goals of this session were to hear from and boost a diverse set of leaders from across the US government and academia to highlight open science in daily work, including peer-teaching, mentoring, and learning. Building from our session at ESIP Winter 2022, we hope to create more channels for inter- and cross-agency learning, and share open science stories across agencies, as part of the 2023 Year of Open Science as recently declared by the US Biden-Harris Administration. Speakers shared stories about open science in government and their experiences with Openscapes. Stories were shared in a “Fishbowl” format, where speakers each shared and then there was a broader discussion with the 50+ participants. This blog is co-authored with the speakers. Link to source blog post: https://www.openscapes.org/blog/2023/03/16/esip-winter-2023/
Spatially Resolved 3 micron Spectroscopy of Elias 1: Origin of Diamonds in Protoplanetary Disks
Creators: name: Goto, M.
name: Henning, Th.
name: Kouchi, A.
name: Takami, H.
name: Hayano, Y.
name: Usuda, T.
name: Takato, N.
name: Terada, H.
name: Oya, S.
name: Jäger, C.
name: Andersen, A. C.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present spatially resolved 3 um spectra of Elias 1 obtained with an adaptive optics system. The central part of the disk is almost devoid of PAH emission at 3.3 um; it shows up only at 30 AU and beyond. The PAH emission extends up to 100 AU, at least to the outer boundary of our observation. The diamond emission, in contrast, is more centrally concentrated, with the column density peaked around 30 AU from the star. There are only three Herbig Ae/Be stars known to date that show diamond emission at 3.53 um. Two of them have low-mass companions likely responsible for the large X-ray flares observed toward the Herbig Ae/Be stars. We speculate on the origin of diamonds in circumstellar disks in terms of the graphitic material being transformed into diamond under the irradiation of highly energetic particles.
description: 7 pages, 4 figures, Accepted for publication in the Astrophysical Journa
title: Ð¤Ð¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÑÑÐµÑÑ ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð±ÑÐ¾ÐºÐ¸Ð½Ð³Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ¸ÑÐ½Ð¸ÐºÐ¾Ð², ÐÐ¸ÑÐ°Ð¸Ð»
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð·
ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½ÑÐ¹ Ð±ÑÐ¾ÐºÐ¸Ð½Ð³
Ð°Ð½Ð°Ð»Ð¸Ð· Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸
Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿Ð»Ð°ÑÐµÐ¶ÐµÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸
Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÐ¸

description: Ð Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÑÐ½ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÑÑÐµÑÑ ÑÐ°Ð¼Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð±ÑÐ¾ÐºÐ¸Ð½Ð³Ð° Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«Ð£ÑÐ°Ð»ÐÑÐ¾ÐºÐ¡ÐµÑÐ²Ð¸Ñ-ÐÐ¾Ð½ÑÑÐ»ÑÑÐ°Ð½ÑÂ», Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸ Ð¸ Ð¿Ð»Ð°ÑÐµÐ¶ÐµÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸, ÑÑÑÑÐºÑÑÑÑ Ð±Ð°Ð»Ð°Ð½ÑÐ°. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ð° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸, Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ Ð´ÐµÐ»Ð¾Ð²Ð¾Ð¹ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ Ð´Ð°Ð½Ð½ÑÑ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÐµ Ð¼ÐµÑÑ Ð¿Ð¾ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸.
Conservation complexities: conservationists’ and local landowners’ different perceptions of development and conservation in Sandaun Province, Papua New Guinea
Creators: name: Pedersen, Marianne
Publisher: name: Canberra, ACT: State, Society and Governance in Melanesia (SSGM) Program, Research School of Pacific and Asian Studies, The Australian National University
Year: 2013
Subjects: Papua New Guinea
land
conservation
environment
development

description: For some people, conservation may be the story of saving the world as we know it. It may be perceived as conservationists’ continuous battles against gigantic forces such as population growth, extractive industries and corrupt governments in an attempt to save the planet’s biodiversity for future generations. For some rural forest dwellers, conservation may be seen as social and economic progress, social change and access to modern commodities. However, a quick look at recent debates of conservation tells the story of rural forest dwellers being dispossessed from their land due to the establishment of protected areas 9cf.Kelly 2011; Li 2011), of local disempowerment, and of unrealised expectations (cf.West 2006). (First paragraph of paper).
title: ÐÑÐ±Ð¾Ñ ÑÐ¿Ð¾ÑÐ¾Ð±Ð° Ð¼Ð¾Ð´ÐµÑÐ½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¶ÐµÐ»ÐµÐ·Ð½Ð¾Ð´Ð¾ÑÐ¾Ð¶Ð½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ° Ð´Ð»Ñ ÐÐ Â«ÐÐ¾ÐºÐ¾Ð¼Ð¾ÑÐ¸Ð²Â»
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÐ¸Ð½Ð°, ÐÐ½Ð°ÑÑÐ°ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¶ÐµÐ»ÐµÐ·Ð½Ð¾Ð´Ð¾ÑÐ¾Ð¶Ð½ÑÐ¹ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑ
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Ð»Ð¾ÐºÐ¾Ð¼Ð¾ÑÐ¸Ð²
ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ°

description: 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 Ð²ÑÐ±Ð¾Ñ ÑÐ¿Ð¾ÑÐ¾Ð±Ð° Ð¼Ð¾Ð´ÐµÑÐ½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¶ÐµÐ»ÐµÐ·Ð½Ð¾Ð´Ð¾ÑÐ¾Ð¶Ð½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ° Ð´Ð»Ñ ÐÐ Â«ÐÐ¾ÐºÐ¾Ð¼Ð¾ÑÐ¸Ð²Â». ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¶ÐµÐ»ÐµÐ·Ð½Ð¾Ð´Ð¾ÑÐ¾Ð¶Ð½Ð¾Ð¹ Ð¸Ð½ÑÑÐ°ÑÑÑÑÐºÑÑÑÑ Ð¸ ÑÐ°Ð±Ð¾ÑÑ ÐÐ Â«ÐÐ¾ÐºÐ¾Ð¼Ð¾ÑÐ¸Ð²Â» Ð±ÑÐ»Ð¾ Ð¿ÑÐ¸Ð½ÑÑÐ¾ ÑÐµÑÐµÐ½Ð¸Ðµ Ð¾ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¼Ð¾Ð´ÐµÑÐ½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¶ÐµÐ»ÐµÐ·Ð½Ð¾Ð´Ð¾ÑÐ¾Ð¶Ð½ÑÑ Ð¿ÑÑÐµÐ¹ Ð¾Ñ ÑÑ. ÐÐ¸Ð³Ð¾Ð²Ð¾ Ð´Ð¾ ÐÐ¾Ð»ÑÐ¾Ð½ÑÐºÐ¾Ð³Ð¾ ÑÐ¾ÑÑÐµ Ð¿ÑÐ¾ÑÑÐ¶ÐµÐ½Ð½Ð¾ÑÑÑÑ Ð² 2,6 ÐºÐ¼.
Atmospheric proton and neutron spectra at energies above 1 GeV
Creators: name: V. A. Naumov
name: T. S. Sinegovskaya
Publisher: name: INFN Open Access Repository
Year: 2001

description: We discuss an effective numerical method for solving the transport equations
for cosmic ray nucleons in the atmosphere. It is demonstrated that the nucleon
attenuation lengths are strongly energy and depth dependent due to the
non-power-law behavior of the primary spectrum, growth of the total inelastic
cross sections with energy, and scaling violation in the nucleon-nucleus
interactions. The numerical results are compared with the available
experimental data.
Time Delay Between Gravitational Waves and Neutrino Burst From a
  Supernova Explosion: a Test for the Neutrino Mass
Creators: name: D. Fargion
Publisher: name: Lett.Nuovo Cim. 31 (1981) 499-500
Year: 2001

description: During Supernova explosions two signals, Gravitational burst wave and
Neutrino Burst, of different nature, originated within 0.1 s from thesuper nova
explosion will be radiated in the outer space. If the neutrinos (as well as the
gravitons) are massless particles, than the original interval (if any) between
the two signals will be freezed forever. On the contrary, if the neutrinos have
a tiny mass, the time delay will increase during the propagation because of the
slower velocity of the neutrinos with respect to the massless gravitons.
Therefore, two signals, of different nature, originated within 0.1 s from the
super nova explosion will be radiated in the outer space. If the neutrinos (as
well as the gravitons) are massless particles, than the original interval (if
any) between the two signals will be freezed forever. If the neutrino has a
mass the time delay will increase during the propagation because of the slower
velocity of the neutrinos with respect to the massless gravitons: the time
delay detection may measure the neutrino mass or its absence may inferr a
severe neutrino mass bound.
Noncompactness and maximum mobility of type III Ricci-flat self-dual neutral Walker four-manifolds
Creators: name: Derdzinski, Andrzej
Publisher: name: arXiv
Year: 2009
Subjects: subject: Differential Geometry (math.DG)
subject: FOS: Mathematics
subject: 53C50, 53C12, 53B30, 53B05

description: It is shown that a self-dual neutral Einstein four-manifold of Petrov type III, admitting a two-dimensional null parallel distribution compatible with the orientation, cannot be compact or locally homogeneous, and its maximum possible degree of mobility is 3. Diaz-Ramos, Garcia-Rio and Vazquez-Lorenzo found a general coordinate form of such manifolds. The present paper also provides a modified version of that coordinate form, valid in a suitably defined generic case and, in a sense, "more canonical" than the usual formulation. Moreover, the local-isometry types of manifolds as above having the degree of mobility equal to 3 are classified. Further results consist in explicit descriptions, first, of the kernel and image of the Killing operator for any torsionfree surface connection with everywhere-nonzero, skew-symmetric Ricci tensor, and, secondly, of a moduli curve for surface connections with the properties just mentioned that are, in addition, locally homogeneous. Finally, hyperbolic plane geometry is used to exhibit examples of codimension-two foliations on compact manifolds of dimensions greater than 2 admitting a transversal torsionfree connection, the Ricci tensor of which is skew-symmetric and nonzero everywhere. No such connection exists on any closed surface, so that there are no analogous examples in dimension 2.
description: 31 pages
Detecting circumbinary planets using eclipse timing of binary stars - numerical simulations
Creators: name: Sybilski, P.
name: Konacki, M.
name: Kozłowski, S.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The presence of a body in an orbit around a close eclipsing binary star manifests itself through the light time effect influencing the observed times of eclipses as the close binary and the circumbinary companion both move around the common centre of mass. This fact combined with the periodicity with which the eclipses occur can be used to detect the companion. Given a sufficient precision of the times of eclipses, the eclipse timing can be employed to detect substellar or even planetary mass companions. The main goal of the paper is to investigate the potential of the photometry based eclipse timing of binary stars as a method of detecting circumbinary planets. In the models we assume that the companion orbits a binary star in a circular Keplerian orbit. We analyze both the space and ground based photometry cases. In particular, we study the usefulness of the on-going COROT and Kepler missions in detecting circumbinary planets. We also explore the relations binding the planet discovery space with the physical parameters of the binaries and the geometrical parameters of their light curves. We carry out detailed numerical simulations of the eclipse timing by employing a relatively realistic model of the light curves of eclipsing binary stars. We study the influence of the white and red photometric noises on the timing precision. We determine the sensitivity of the eclipse timing technique to circumbinary planets for the ground and space based photometric observations. We provide suggestions for the best targets, observing strategies and instruments for the eclipse timing method. Finally, we compare the eclipse timing as a planet detection method with the radial velocities and astrometry.
description: 9 pages, 15 figures, accepted for publication in MNRAS
Constraints on the Primordial Magnetic Field from $σ_8$
Creators: name: Yamazaki, Dai G.
name: Ichiki, Kiyotomo
name: Kajino, Toshitaka
name: Mathews, Grant. J.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: A primordial magnetic field (PMF) can affect the evolution of density field fluctuations in the early universe.In this paper we constrain the PMF amplitude $B_λ$ and power spectral index $n_\mathrm{B}$ by comparing calculated density field fluctuations with observational data, i.e. the number density fluctuation of galaxies.We show that the observational constraints on cosmological density fluctuations, as parameterized by $σ_8$, lead to strong constraints on the amplitude and spectral index of the PMF.
description: 11 pages, 1 figure, accepted for publication as Phys. Rev. D
A new formal solution of the radiative transfer in arbitrary velocity fields
Creators: name: Knop, S.
name: Hauschildt, P. H.
name: Baron, E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present a new formal solution of the Lagrangian equation of radiative transfer that is useful in solving the equation of radiative transfer in the presence of arbitrary velocity fields. Normally a term due to the inclusion of the wavelength derivative in the Lagrangian equation of radiative transfer is associated with a generalised opacity. In non-monotonic velocity fields, this generalised opacity may become negative. To ensure that the opacity remains positive, this term of the derivative is included in the formal solution of the radiative transfer problem. The new definition of the generalised opacity allows for a new solution of the equation of radiative transfer in the presence of velocity fields. It is especially useful for arbitrary velocity fields, where it effectively prevents the occurrences of negative generalised opacities and still allows the explicit construction of the Lambda-operator of the system needed for an accelerated Lambda-iteration. We performed test calculations, where the results of old, established solutions were compared with the new solution. The relative deviations never exceeded 1% and so the new solution is indeed suitable for use in radiative-transfer modelling. Non-monotonic velocity fields along photon paths frequently occur in three-dimensional hydrodynamical models of astrophysical atmospheres. Therefore, the formal solution will be of use for multidimensional radiative transfer and has immediate applications in the modelling of pulsating stars and astrophysical shock fronts.
description: Astronomy & Astrophysics, in press 8 figures
Extended Skyrme interaction (I): spin fluctuations in dense matter
Creators: name: Margueron, Jérôme
name: Sagawa, Hiroyuki
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Most of the Skyrme interactions are known to predict spin or isospin instabilities beyond the saturation density of nuclear matter which contradict predictions based on realistic interactions. A modification of the standard Skyrme interaction is proposed so that the ferromagnetic instability is removed. The new terms are density dependent and modify only the spin p-h interaction in the case of spin-saturated system. Consequences for the nuclear response function and neutrino mean free path are shown. The overall effect of the RPA correlations makes dense matter more transparent for neutrino propagation by a factor of 2 to 10 depending of the density.
description: 6 pages, 5 Figs., 2 Tabs
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾Ð¿ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð·Ð°Ñ Ð¾Ð´Ð° Ð½Ð° Ð¿Ð¾ÑÐ°Ð´ÐºÑ Ð±ÐµÑÐ¿Ð¸Ð»Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð»ÐµÑÐ°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÐ°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ´Ð·Ð°, ÐÐ»ÐµÐºÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð±ÐµÑÐ¿Ð¸Ð»Ð¾ÑÐ½ÑÐ¹ Ð»ÐµÑÐ°ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð¿Ð¿Ð°ÑÐ°Ñ
ÑÐ¸ÑÑÐµÐ¼Ð° Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð·Ð°Ñ Ð¾Ð´Ð° Ð½Ð° Ð¿Ð¾ÑÐ°Ð´ÐºÑ
ÐºÑÑÑÐ¾-Ð³Ð»Ð¸ÑÑÐ°Ð´Ð½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð°
Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¿Ð¾ÑÐ°Ð´ÐºÐ°
unmanned aerial vehicle
system instrumental landing
courses-glide system
automatic landing

description: Ð¦ÐµÐ»ÑÑ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² ÐºÑÑÑÐ¾-Ð³Ð»Ð¸ÑÑÐ°Ð´Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ, Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÑÑÐµÐ¹ Ð²Ð·Ð»ÐµÑ Ð¸ Ð¿Ð¾ÑÐ°Ð´ÐºÑ Ð¼ÑÐ»ÑÑÐ¸ÑÐ¾ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð±ÐµÑÐ¿Ð¸Ð»Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð»ÐµÑÐ°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÐ° Ð² Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð¼ ÑÐµÐ¶Ð¸Ð¼Ðµ Ð±ÐµÐ· ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¾ÑÐ¾Ð¼. Ð ÑÐ¾Ð´Ðµ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ» ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÐºÐ¾Ð½ÑÐµÐ¿Ñ ÑÐ¸ÑÑÐµÐ¼Ñ, Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð° ÐµÐ³Ð¾ ÑÐµÐ»ÐµÑÐ¾Ð¾Ð±ÑÐ°Ð·Ð½Ð¾ÑÑÑ, Ð¿Ð¾Ð´Ð¾Ð±ÑÐ°Ð½Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð´ÑÑÐµÐµ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÐ½Ð¾Ðµ ÑÐµÑÐµÐ½Ð¸Ðµ, Ð½Ð°Ð¹Ð´ÐµÐ½Ð° ÑÐµÑÐºÐ° ÑÐ°ÑÑÐ¾Ñ Ð¸ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ Ð±ÑÑÑÑÐ¾Ð³Ð¾ Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¤ÑÑÑÐµ, ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑÐ¸Ðµ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑÐ¼ Ð²ÑÐ±ÑÐ°Ð½Ð½Ð¾Ð³Ð¾ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ. ÐÑÐ»Ð¾ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ðµ Ð¸Ð¼Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ, Ð¿Ð¾Ð´ÑÐ²ÐµÑÐ´Ð¸Ð²ÑÐµÐµ Ð¿ÑÐ°Ð²Ð¸Ð»ÑÐ½Ð¾ÑÑÑ Ð½Ð°Ð¹Ð´ÐµÐ½Ð½ÑÑ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² Ð¸ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ð²ÑÐµÐµ Ð¾Ð¿ÑÐµÐ´ÐµÐ»Ð¸ÑÑ Ð³ÐµÐ¾Ð¼ÐµÑÑÐ¸Ñ Ð¿Ð¾ÑÐ°Ð´Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÐ°. Ð¢Ð°ÐºÐ¶Ðµ Ð±ÑÐ» Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½ Ð¿ÑÐ¾ÑÐ¾ÑÐ¸Ð¿ Ð°Ð½Ð°Ð»Ð¾Ð³Ð¾Ð²Ð¾Ð¹ ÑÐ°ÑÑÐ¸ ÑÐ¸ÑÑÐµÐ¼Ñ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾Ð´ÑÐ²ÐµÑÐ´Ð¸Ð»Ð° ÑÐ°Ð±Ð¾ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ Ð¸ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ° Ð¸ Ð´Ð°Ð»Ð° Ð½Ð°ÑÐ°Ð»Ð¾ Ð¿Ð¾ÑÐ»ÐµÐ´ÑÑÑÐµÐ¹ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ ÑÐ¸ÑÑÐµÐ¼Ñ.
description: The aim of this work was to develop elements of instrument landing system that provides takeoff and landing of multirotor unmanned aerial vehicles automatically, without operator control. During this work the concept of the system was developed, its expediency was proved. Were found the hardware solution, the frequency grid and parameters of the fast Fourier transform, according to features of the selected hardware. Computer simulations, that confirmed the correctness of the found parameters and helped to find proportions of the beacon were made. Was made the prototype of analogue part of the system. This work confirmed the operability of the developed concept and started the next development phase.
Additional file 2 of Impact of a spatial repellent product on Anopheles and non-Anopheles mosquitoes in Sumba, Indonesia
Creators: name: Permana, Dendi H.
name: Zubaidah, Siti
name: Syahrani, Lepa
name: Asih, Puji B. S.
name: Syafruddin, Din
name: Rozi, Ismail E.
name: Hidayati, Anggi P. N.
name: Kosasih, Sully
name: Dewayanti, Farahana K.
name: Rachmawati, Nia
name: Risandi, Rifqi
name: Bangs, Michael J.
name: Bøgh, Claus
name: Davidson, Jenna R.
name: Hendershot, Allison L.
name: Burton, Timothy A.
name: Grieco, John P.
name: Eugenio, Evercita C.
name: Liu, Fang
name: Achee, Nicole L.
name: Lobo, Neil F.
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Neuroscience
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 2. The relationship between HBR and malaria infection by species for overall infections.
title: Ð¤Ð°ÐºÑÐ¾ÑÐ¸Ð½Ð³ ÐºÐ°Ðº ÑÐ¿Ð¾ÑÐ¾Ð± ÑÐ¸Ð½Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¾Ð±Ð¾ÑÐ¾ÑÐ½ÑÑ ÑÑÐµÐ´ÑÑÐ² Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐÐ¡Â»)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÑÑÑÑÐ¸Ð½Ð°, ÐÐ²Ð³ÐµÐ½Ð¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÐ°ÐºÑÐ¾ÑÐ¸Ð½Ð³
Ð¾Ð±Ð¾ÑÐ¾ÑÐ½ÑÐµ Ð°ÐºÑÐ¸Ð²Ñ
Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ°Ñ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÑ
ÐºÐ»Ð¸Ð½Ð¸Ð½Ð³Ð¾Ð²ÑÐµ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸
factoring
current assets
receivables
cleaning companies

description: Ð Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð¿Ð¾Ð½ÑÑÐ¸Ñ ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÐµ Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¾Ð±Ð¾ÑÐ¾ÑÐ½ÑÑ Ð°ÐºÑÐ¸Ð²Ð¾Ð² Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð·Ð° ÑÑÐµÑ ÑÐ°ÐºÑÐ¾ÑÐ¸Ð½Ð³Ð°, Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð° ÑÐ°Ð±Ð¾ÑÐ° Ñ Ð´Ð°Ð½Ð½ÑÐ¼ Ð²Ð¸Ð´Ð¾Ð¼ ÑÑÐ»ÑÐ³ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÑÐ¸Ð»Ð¸Ð°Ð»Ð° ÐºÐ»Ð¸Ð½Ð¸Ð½Ð³Ð¾Ð²Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐÐÐ¡ Ð³.Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³, ÑÐ´ÐµÐ»Ð°Ð½Ñ Ð²ÑÐ²Ð¾Ð´Ñ, Ð¸ÑÑÐ¾Ð´Ñ Ð¸Ð· Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð½ÑÑ Ð´Ð°Ð½Ð½ÑÑ, Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
description: In the work were analyzed various concepts related to the financing of the current assets, using factoring; analyzed the work with this type of service by the example of the branch of the cleaning company Â«OMCÂ» Ltd. St. Petersburg. Also were made conclusions on the base of represented data, and were suggested tactics to improve the company's financial status.