cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÑÑÑÐµÐ¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð¿Ð°ÐµÐ²ÑÑ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¾Ð½Ð´Ð¾Ð² (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ "Ð£Ð "ÐÑÑÐ°Ð³ÐµÑÐ°")
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð½Ð¾Ð¼Ð°ÑÐµÐ½ÐºÐ¾, ÐÐ½Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¿Ð°ÐµÐ²ÑÐµ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐ¾Ð½Ð´Ñ
ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð·
Ð´Ð¾Ð²ÐµÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ
Ð°Ð½Ð°Ð»Ð¸Ð· Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ "Ð£Ð¿ÑÐ°Ð²Ð»ÑÑÑÐ°Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ñ "ÐÑÑÐ°Ð³ÐµÑÐ°". Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÑÑÑÐµÐ¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸, Ð¾ÑÑÑÐµÑÑÐ²Ð»ÑÑÑÐµÐ¹ Ð´Ð¾Ð²ÐµÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿Ð°ÐµÐ²ÑÐ¼Ð¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐ¼Ð¸ ÑÐ¾Ð½Ð´Ð°Ð¼Ð¸, Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐºÐ¾Ð½ÐºÑÐµÑÐ½Ð¾Ð¹ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸. ÐÐ»Ñ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐÐÐ "Ð£Ð¿ÑÐ°Ð²Ð»ÑÑÑÐ°Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ñ "ÐÑÑÐ°Ð³ÐµÑÐ°" Ð±ÑÐ» Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÑÑÑÐµÐ¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð¿Ð°ÐµÐ²ÑÐ¼Ð¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐ¼Ð¸ ÑÐ¾Ð½Ð´Ð°Ð¼Ð¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð°ÐºÑÐ¸Ð²Ð¾Ð², Ð½Ð°ÑÐ¾Ð´ÑÑÐ¸ÑÑÑ Ð² Ð´Ð¾Ð²ÐµÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ð¼ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÑÑÑÐµÐ¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð¿Ð°ÐµÐ²ÑÐ¼Ð¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐ¼Ð¸ ÑÐ¾Ð½Ð´Ð°Ð¼Ð¸. ÐÑÑÐ²Ð»ÐµÐ½Ñ Ð¿ÑÑÐ¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÑÑÑÐµÐ¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð¿Ð°ÐµÐ²ÑÐ¼Ð¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐ¼Ð¸ ÑÐ¾Ð½Ð´Ð°Ð¼Ð¸.
Quei fiumi di gas? Arrivano dritti dal Big Bang
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2013

Osservati per la prima volta flussi d’idrogeno primordiale scorrere verso una galassia a 11 miliardi di anni luce da noi. A rilevarne la firma, grazie all’allineamento con un quasar retrostante, i telescopi del Keck e il Large Binocular Telescope.
I supervulcani di Marte
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2013

Si è sempre pensato che l'attività vulcanica abbia avuto una grande influenza sulla geologia e il clima del Pianeta rosso, soprattutto nella zona equatoriale, ma i crateri visibili appartengono a vulcani relativamente giovani e piccoli. Due ricercatori del Natural History Museum hanno trovato le prove di antichi vulcani giganti nella regione Arabia Terra, simili a quelli di Yellowstone o dei Campi Flegrei. Lo studio pubblicato su Nature.
title: Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¼ÐµÑ Ð°Ð½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð´ÐµÑÐ°Ð»Ð¸ Â«Ð²ÑÑÐ»ÐºÐ°Â»
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ°ÑÐ½Ð¾Ð², ÐÐ²Ð°Ð½
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ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ
Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð½Ð°Ð»Ð°Ð´ÐºÐ°
Ð±Ð°Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ

description: Ð Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð½Ð° Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÑÑ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÑ Ð²ÑÑÐ»ÐºÐ¸, Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð½Ð¾Ð¹ Ð¸Ð· Ð¡ÑÐ°Ð»Ð¸ 40Ð¥ ÐÐÐ¡Ð¢ 4543-71. ÐÐ°Ð½Ð° ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½Ð¾Ð¹ Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð´ÐµÑÐ°Ð»Ð¸. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð²ÑÐ±Ð¾Ñ Ð¼ÐµÑÐ¾Ð´Ð° Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸, Ð¿Ð¾ÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸, ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ, Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÑÑÐ¸Ðµ Ð¼Ð¸Ð½Ð¸Ð¼Ð°Ð»ÑÐ½ÑÑ ÑÑÑÐ´Ð¾ÐµÐ¼ÐºÐ¾ÑÑÑ Ð¸ ÑÐµÐ±ÐµÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÑ Ð¸Ð·Ð³Ð¾ÑÐ°Ð²Ð»Ð¸Ð²Ð°ÐµÐ¼Ð¾Ð¹ Ð´ÐµÑÐ°Ð»Ð¸ Ð¿ÑÐ¸ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ð¸ Ð·Ð°Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ ÐºÐ°ÑÐµÑÑÐ²Ð°. ÐÑÑÐ¾Ð´Ñ Ð¸Ð· ÑÑÐ¾Ð³Ð¾, ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ñ Ð¿ÑÐ¸Ð¿ÑÑÐºÐ¸ Ð¸ ÑÐµÐ¶Ð¸Ð¼Ñ ÑÐµÐ·Ð°Ð½Ð¸Ñ Ñ Ð½Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹ Ð´Ð»Ñ ÑÑÐ»Ð¾Ð²Ð¸Ð¹ ÑÐµÑÐ¸Ð¹Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ñ Ð¿ÑÐ¸ÑÐ¿Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð´ÐµÑÐ°Ð»Ð¸.
Metti un’elica nella nebulosa
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2013

La splendida nebulosa NGC 7293 in direzione della costellazione dell'Acquario è sopra l'orizzonte dei nostri cieli nelle notti di ottobre. Pur essendo tra le più brillanti, non è però visibile ad occhio nudo. I consigli per osservarla e le spettacolari riprese del telescopio spaziale Hubble nel video su INAF tv.
title: ÐÐ½Ð°Ð»Ð¸Ð· Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸ Ð¸ Ð¿Ð»Ð°ÑÐµÐ¶ÐµÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ñ ÐÐ¾Ð´ÑÐ¸Ð¹Â»)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸ÐºÐ¸ÑÐ¸Ð½Ð°, Ð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: 2017
Subjects: Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸
Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¿Ð»Ð°ÑÐµÐ¶ÐµÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¹ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐµ ÑÐµÑÑÑÑÑ

description: ÐÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÑ Ð²Ð¾Ð¿ÑÐ¾ÑÐ¾Ð² Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸ Ð¸ Ð¿Ð»Ð°ÑÐµÐ¶ÐµÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ Ð²ÑÑÐ¾ÐºÐ° Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÐºÑÐ¸Ð·Ð¸ÑÐ°. ÐÐ¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÑ Ð²ÑÑÑÑÐ¿Ð°ÐµÑ ÐºÐ°Ðº Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾Ðµ Ð¸ Ð¾Ð±ÑÐ·Ð°ÑÐµÐ»ÑÐ½Ð¾Ðµ ÑÑÐ»Ð¾Ð²Ð¸Ðµ Ð¿Ð»Ð°ÑÐµÐ¶ÐµÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸, ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð·Ð° ÑÐ¾Ð±Ð»ÑÐ´ÐµÐ½Ð¸ÐµÐ¼ ÐºÐ¾ÑÐ¾ÑÐ¾Ð¹ ÑÐ²Ð»ÑÐµÑÑÑ Ð²Ð°Ð¶Ð½ÐµÐ¹ÑÐµÐ¹ ÑÑÐ½ÐºÑÐ¸ÐµÐ¹ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. ÐÐ»Ñ ÑÑÐ°Ð±Ð¸Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ Ð¿Ð¾ÑÑÐ¾ÑÐ½Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸ Ð¸ Ð¿Ð»Ð°ÑÐµÐ¶ÐµÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¸ Ð¸Ñ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ. ÐÑÐµ ÑÑÐ¾ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐµÑ Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÑ Ð¸ Ð²Ð°Ð¶Ð½Ð¾ÑÑÑ ÑÐµÐ¼Ñ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ°. ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÑÑÑÑ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÐÐÐ Â«ÐÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ñ ÐÐ¾Ð´ÑÐ¸Ð¹Â». ÐÑÐµÐ´Ð¼ÐµÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿Ð»Ð°ÑÐµÐ¶ÐµÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð¸ Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð¦ÐµÐ»ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¿Ð»Ð°ÑÑÐ¶ÐµÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¿Ð»Ð°ÑÐµÐ¶ÐµÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ ÐºÐ¾Ð½ÐºÑÐµÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐµÐ³Ð¾ ÑÐµÑÐ°ÑÑ ÑÑÐ¾ÑÑÐ¸Ðµ Ð¿ÐµÑÐµÐ´ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸ÐµÐ¼ Ð·Ð°Ð´Ð°ÑÐ¸ Ð¸ ÑÐ²ÐµÑÐµÐ½Ð½Ð¾ ÑÑÑÐ¾Ð¸ÑÑ ÑÐ²Ð¾Ðµ Ð±ÑÐ´ÑÑÐµÐµ. Ð Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ ÑÐµÑÐ°ÑÑÑÑ ÑÐ»ÐµÐ´ÑÑÑÐ¸Ðµ Ð·Ð°Ð´Ð°ÑÐ¸: Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¿Ð»Ð°ÑÑÐ¶ÐµÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸; Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð´Ð¸Ð°Ð³Ð½Ð¾ÑÑÐ¸ÑÑÐµÑÑÑ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð² Ñ.Ñ. Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ Ð¿Ð»Ð°ÑÐµÐ¶ÐµÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸; ÑÐ°Ð·ÑÐ°Ð±Ð°ÑÑÐ²Ð°ÑÑÑÑ ÐºÐ¾Ð½ÐºÑÐµÑÐ½ÑÐµ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÐµ Ð½Ð° Ð±Ð¾Ð»ÐµÐµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐµÑÑÑÑÐ¾Ð² Ð¸ ÑÐºÑÐµÐ¿Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
Enhanced electron correlations, local moments, and Curie temperature in strained MnAs nanocrystals embedded in GaAs
Creators: name: Moreno, M.
name: Cerdá, J. I.
name: Ploog, K. H.
name: Horn, K.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: We have studied the electronic structure of hexagonal MnAs, as epitaxial continuous film on GaAs(001) and as nanocrystals embedded in GaAs, by Mn 2p core-level photoemission spectroscopy. Configuration-interaction analyses based on a cluster model show that the ground state of the embedded MnAs nanocrystals is dominated by a d5 configuration that maximizes the local Mn moment. Nanoscaling and strain significantly alter the properties of MnAs. Internal strain in the nanocrystals results in reduced p-d hybridization and enhanced ionic character of the Mn-As bonding interactions. The spatial confinement and reduced p-d hybridization in the nanocrystals lead to enhanced d-electron localization, triggering d-d electron correlations and enhancing local Mn moments. These changes in the electronic structure of MnAs have an advantageous effect on the Curie temperature of the nanocrystals, which is measured to be remarkably higher than that of bulk MnAs.
description: 4 figures, 2 tables
title: Ð¡ÑÐ¸Ð»ÐµÐ²ÑÐµ Ð´Ð¾Ð¼Ð¸Ð½Ð°Ð½ÑÑ Ð² ÑÐ¾Ð¼Ð°Ð½Ðµ Ð ÑÑ ÐÑÑÐ´Ð±ÐµÑÐ¸ Â«451 Ð³ÑÐ°Ð´ÑÑ Ð¿Ð¾ Ð¤Ð°ÑÐµÐ½Ð³ÐµÐ¹ÑÑÂ»
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÑÑÑÐ½Ð¸ÑÐµÐ²Ð°, 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: 2017
Subjects: Ñ ÑÐ´Ð¾Ð¶ÐµÑÑÐ²ÐµÐ½Ð½ÑÐ¹ ÑÐµÐºÑÑ
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ÑÑÐ¸Ð»ÐµÐ²ÑÐµ Ð´Ð¾Ð¼Ð¸Ð½Ð°Ð½ÑÑ

description: ÐÐ°ÑÑÐ¾ÑÑÐ°Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð° Ð½Ð° ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ°Ñ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð½Ð°Ð¼Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÑÐ¸Ð»Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐ¸ÐµÐ¼Ð¾Ð² Ð² ÑÑÐ´Ð¾Ð¶ÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð¼ ÑÐµÐºÑÑÐµ. ÐÐ°Ð½Ð½ÑÐµ ÑÑÐ¸Ð»Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿ÑÐ¸ÐµÐ¼Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÑÑÑÑÑ Ñ ÑÐ¾ÑÐºÐ¸ Ð·ÑÐµÐ½Ð¸Ñ Ð¸Ñ ÑÐ¿Ð¾ÑÑÐµÐ±Ð»ÐµÐ½Ð¸Ñ Ð½Ð° Ð»ÐµÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¼ Ð¸ ÑÐ¸Ð½ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¼ ÑÑÐ¾Ð²Ð½ÑÑ. Ð¦ÐµÐ»ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ ÑÑÐ¸Ð»ÐµÐ²ÑÑ Ð´Ð¾Ð¼Ð¸Ð½Ð°Ð½Ñ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÑÐ¾Ð¼Ð°Ð½Ð° Ð ÑÑ ÐÑÑÐ´Ð±ÐµÑÐ¸ Â«451 Ð³ÑÐ°Ð´ÑÑ Ð¿Ð¾ Ð¤Ð°ÑÐµÐ½Ð³ÐµÐ¹ÑÑÂ». ÐÑÐ¸ Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ð¸Ð¸ ÑÐ°Ð±Ð¾ÑÑ Ð¼Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð»Ð¸ Ð¼ÐµÑÐ¾Ð´ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð½Ð°ÑÑÐ½Ð¾Ð¹ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ, Ð¼ÐµÑÐ¾Ð´ ÑÐ¿Ð»Ð¾ÑÐ½Ð¾Ð¹ Ð²ÑÐ±Ð¾ÑÐºÐ¸, Ð° ÑÐ°ÐºÐ¶Ðµ ÐºÐ¾Ð½ÑÐµÐºÑÑÑÐ°Ð»ÑÐ½ÑÐ¹, ÑÑÐ¸Ð»Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ð¹, ÑÑÐ°ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ð¹, Ð¸Ð½ÑÐµÑÐ¿ÑÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¼ÐµÑÐ¾Ð´Ñ. ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð¸Ð· Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ñ, Ð´Ð²ÑÑ Ð³Ð»Ð°Ð², ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´Ð°ÐµÐ¼ÑÑ Ð²ÑÐ²Ð¾Ð´Ð°Ð¼Ð¸, Ð·Ð°ÐºÐ»ÑÑÐµÐ½Ð¸Ñ, ÑÐ¿Ð¸ÑÐºÐ° Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ Ð¸ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ. Ð ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°ÑÑÐ¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ²Ð¾ÑÑÐµÑÑÐ²Ð¾ Ð ÑÑ ÐÑÑÐ´Ð±ÐµÑÐ¸, Ð¶Ð°Ð½ÑÐ¾Ð²Ð¾Ðµ ÑÐ²Ð¾ÐµÐ¾Ð±ÑÐ°Ð·Ð¸Ðµ ÐµÐ³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹ Ð¸ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ ÑÐ¾Ð¼Ð°Ð½Ð°. ÐÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÑÑ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ ÑÐ°ÑÑÐ¾ Ð²ÑÑÑÐµÑÐ°ÑÑÐ¸ÑÑÑ ÑÑÐ¸Ð»ÐµÐ²ÑÑ Ð´Ð¾Ð¼Ð¸Ð½Ð°Ð½Ñ Ð² ÑÐ¾Ð¼Ð°Ð½Ðµ.
D1.8.7 Report on extended method and analysis documentation – the extension of the initial simple method documentation
Creators: name: Institute of Food Research
Publisher: name: Zenodo
Year: 2005
Subjects: NoE and NEXUS Projects
The EuroFIR Food Platform
EuroFIR

description: WP1.8 Extended Specification for Method Documentation

WP1.8 has developed an extended specification for method documentation. In addition to the general Method Indicator (linked to the EuroFIR method thesaurus) reported for a compositional value, the Method Specification entity includes details of key method steps and laboratory performance. This report outlines the extended analytical method specification.
Doppler Spread Estimation by Tracking the Delay-Subspace for OFDM Systems in Doubly Selective Fading Channels
Creators: name: Zhao, Xiaochuan
name: Peng, Tao
name: Yang, Ming
name: Wang, Wenbo
Publisher: name: arXiv
Year: 2008
Subjects: subject: Information Theory (cs.IT)
subject: FOS: Computer and information sciences

description: A novel maximum Doppler spread estimation algorithm for OFDM systems with comb-type pilot pattern is presented in this paper. By tracking the drifting delay subspace of time-varying multipath channels, a Doppler dependent parameter can be accurately measured and further expanded and transformed into a non-linear high-order polynomial equation, from which the maximum Doppler spread is readily solved by resorting to the Newton's method. Its performance is demonstrated by simulations.
description: 4 pages, 2 figures, Appear in IEEE Signal Process. Letters
Per la NASA compleanno tra pochi intimi
Creators: Nicola Nosengo
Publisher: name: Media Inaf
Year: 2013

Nel giorno del suo anniversario, l'agenzia spaziale americana fa i conti con il temuto blocco delle operazioni dovuto alla mancata approvazione del budget del governo USA per il nuovo anno fiscale. Il 97 per cento dei dipendenti costretto a rimanere a casa. Proseguono regolarmente solo le attività legate alla ISS.
On some universal sums of generalized polygonal numbers
Creators: name: Ge, Fan
name: Sun, Zhi-Wei
Publisher: name: arXiv
Year: 2009
Subjects: subject: Number Theory (math.NT)
subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: 11E25, 11D85, 11E20, 11P32

description: For $m=3,4,\ldots$ those $p_m(x)=(m-2)x(x-1)/2+x$ with $x\in\mathbb Z$ are called generalized $m$-gonal numbers. Sun [13] studied for what values of positive integers $a,b,c$ the sum $ap_5+bp_5+cp_5$ is universal over $\mathbb Z$ (i.e., any $n\in\mathbb N=\{0,1,2,\ldots\}$ has the form $ap_5(x)+bp_5(y)+cp_5(z)$ with $x,y,z\in\mathbb Z$). We prove that $p_5+bp_5+3p_5\,(b=1,2,3,4,9)$ and $p_5+2p_5+6p_5$ are universal over $\mathbb Z$, as conjectured by Sun. Sun also conjectured that any $n\in\mathbb N$ can be written as $p_3(x)+p_5(y)+p_{11}(z)$ and $3p_3(x)+p_5(y)+p_7(z)$ with $x,y,z\in\mathbb N$; in contrast, we show that $p_3+p_5+p_{11}$ and $3p_3+p_5+p_7$ are universal over $\mathbb Z$. Our proofs are essentially elementary and hence suitable for general readers.
description: Final published version
Una luna di plastica
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2013

Nella bassa atmosfera di Titano ci sono tracce di propilene. A rilevarle, la sonda Cassini della NASA. È la prima volta che la presenza di questa molecola, il cui corrispondente polimero non è altro che il Moplen, viene registrata su una luna o un pianeta che non sia il nostro.
title: ÐÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð²Ð°ÑÐ¸Ð°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐ¸ÑÐ¼Ð° ÑÐµÑÐ´ÑÐ° ÑÑÑÐ±Ð¾Ð»Ð¸ÑÑÐ¾Ð²
title: Features of heart rate variability in football players
Creators: name: ÐÑÐ¾ÑÐ¾ÑÑÐµÐ²Ð°, ÐÐ»ÐµÐºÑÐ°Ð½Ð´ÑÐ°
name: ÐÑÑÐ°Ð¿ÑÑÐº, ÐÐ½Ð°ÑÑÐ°ÑÐ¸Ñ
name: ÐÐ°Ð»Ð¸Ð½Ð¸Ð½Ð°, ÐÑÐ¸Ð½Ð°
name: ÐÐ¾Ð»Ð¾Ð²Ð½Ð¸ÐºÐ¾Ð²Ð°, ÐÐ°ÑÐ¸Ð½Ð°
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: Ð²Ð°ÑÐ¸Ð°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÑ ÑÐ¸ÑÐ¼Ð° ÑÐµÑÐ´ÑÐ°
ÑÑÑÐ±Ð¾Ð»Ð¸ÑÑÑ
Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ Ð½Ð°Ð´ÐµÐ¶Ð½Ð¾ÑÑÑ
Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ñ
ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐµ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸
heart rate variability
football players
biological reliability
adaptation
functionality

description: ÐÑÑÐ¾ÐºÐ°Ñ Ð¸ Ð½ÐµÐºÐ¾Ð½ÑÑÐ¾Ð»Ð¸ÑÑÐµÐ¼Ð°Ñ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ°Ñ Ð½Ð°Ð³ÑÑÐ·ÐºÐ° Ð²Ð¾ Ð²ÑÐµÐ¼Ñ ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½ÑÑ ÑÑÐµÐ½Ð¸ÑÐ¾Ð²Ð¾Ðº Ð¼Ð¾Ð¶ÐµÑ Ð¿ÑÐ¸Ð²ÐµÑÑÐ¸ Ðº Ð¿Ð°ÑÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¼ Ð¼Ð¾ÑÑÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¼ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸ÑÐ¼ Ð² ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ ÑÐµÑÐ´ÐµÑÐ½Ð¾-ÑÐ¾ÑÑÐ´Ð¸ÑÑÐ¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ. ÐÐ¾Ð½Ð¸ÑÐ¾ÑÐ¸Ð½Ð³ Ð²Ð°ÑÐ¸Ð°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐ¸ÑÐ¼Ð° ÑÐµÑÐ´ÑÐ° (ÐÐ Ð¡) ÑÐ¿Ð¾ÑÑÑÐ¼ÐµÐ½Ð¾Ð² Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½ ÐºÐ°Ðº ÑÑÑÐµÐºÑÐ¸Ð²Ð½ÑÐ¹ Ð¼ÐµÑÐ¾Ð´ Ð¾ÑÐµÐ½ÐºÐ¸ Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð½Ð°Ð´ÐµÐ¶Ð½Ð¾ÑÑÐ¸ Ð¸ Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð° ÑÐµÑÐ´ÐµÑÐ½Ð¾-ÑÐ¾ÑÑÐ´Ð¸ÑÑÐ¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð½Ð° Ð²ÑÐµÑ ÑÑÐ°Ð¿Ð°Ñ ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸. ÐÐ³ÑÐ° Ð² ÑÑÑÐ±Ð¾Ð» Ð¸Ð·-Ð·Ð° ÑÐ²Ð¾ÐµÐ¹ Ð²ÑÑÐ¾ÐºÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´ÑÑÐ²Ð»ÑÐµÑ Ð²ÑÑÐ¾ÐºÐ¸Ðµ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ Ðº ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐ¿Ð¾ÑÑÑÐ¼ÐµÐ½Ð°. Ð ÑÐ¾Ð´Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ ÐÐ Ð¡, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¼Ð¾Ð³ÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÑÑÑ Ð² ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÑÑÐ¸Ñ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ¾Ð².
description: High and uncontrolled physical activity during sports training can lead to pathological morphological changes in the functioning of the cardiovascular system. Monitoring of heart rate variability (HRV) of athletes can be used as an effective method for assessing the biological reliability and adaptive potential of the cardiovascular system at all stages of sports activity. The game of football, because of its high dynamism, places high demands on the functional fitness of an athlete. In the course of the study, HRV parameters were identified that can be used as determining components.
The rate of reaction between bromoacetate and thiosulphate ions in dodium chloride and sea water media
Creators: name: Dodimead, Allan John
Publisher: name: University of British Columbia
Year: 2012

description: Rate measurements of the thiosulphate-bromoacetate reaction have been made in sodium chloride and sea water media at 15.3°, 25.2° and 32.0°C and in magnesium chloride at 15.3°C, Rates are more simply dependent on the concentration and kind of cations in the media than upon the ionic strength. The rate constants are approximately 6% higher in neutral solutions of sea water than in sodium chloride media and the higher rate constants are attributed to the presence in sea water of the cations, K⁺, Ca⁺⁺ and Mg⁺⁺. The energy of activation is 16,000±100 cal./mole and the entropy of activation is-6.6 e.u. for the reaction done in both media. The convergence of the rate curves in magnesium and sodium chloride media at high concentrations may be explained by the presence of undissociated species. The magnitude of the correction to the observed rate depends upon the concentration of the cations and the formation constant for the undissociated species. This explanation has been used to account for the decrease in rate in sea water that has been made alkaline.
On the use of X-ray and gamma-ray telescopes for identifying the origin of electrons and positrons observed by ATIC, Fermi, and PAMELA
Creators: name: Calvez, Antoine
name: Essey, Warren
name: Fairbairn, Malcolm
name: Kusenko, Alexander
name: Loewenstein, Michael
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: X-ray and gamma-ray observations can help understand the origin of the electron and positron signals reported by ATIC, PAMELA, PPB-BETS, and Fermi. It remains unclear whether the observed high-energy electrons and positrons are produced by relic particles, or by some astrophysical sources. To distinguish between the two possibilities, one can compare the electron population in the local neighborhood with that in the dwarf spheroidal galaxies, which are not expected to host as many pulsars and other astrophysical sources. This can be accomplished using X-ray and gamma-ray observations of dwarf spheroidal galaxies. Assuming the signal detected by Fermi and ATIC comes from dark matter and using the inferred dark matter profile of the Draco dwarf spheroidal galaxy as an example, we calculate the photon spectrum produced by electrons via inverse Compton scattering. Since little is known about the magnetic fields in dwarf spheroidal galaxies, we consider the propagation of charged particles with and without diffusion. Extending the analysis of Fermi collaboration for Draco, we find that for a halo mass ~ 1 billion Solar masses, even in the absence of diffusion, the gamma-ray signal would be above the upper limits. This conclusion is subject to uncertainties associated with the halo mass. If dwarf spheroidal galaxies host local magnetic fields, the diffusion of the electrons can result in a signal detectable by future X-ray telescopes.
description: 21 pages, 3 figures
Galassie multispin a Capodimonte
Creators: Maria Teresa Fulco
Publisher: name: Media Inaf
Year: 2013

In corso all'Osservatorio dell'INAF a Napoli un congresso su una classe di galassie peculiari, dove una loro componente di gas, stelle o entrambi, ruota in un piano diverso da quello principale della galassia ospitante.  Una sezione del meeting sarà inoltre dedicata al futuro dell'Astronomia, in vista della realizzazione del grande telescopio europeo E-ELT.
Using known zeta-series to derive the Dancs-He series for $\,\ln{2}\,$ and $\,ζ{(2\,n+1)}$
Creators: name: Lima, F. M. S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: History and Overview (math.HO)
subject: FOS: Mathematics
subject: 11M06, 11Y35, 41A30, 65D15

description: In a recent work, Dancs and He found new `Euler-type' formulas for $\,\ln{2}\,$ and $\,ζ{(2\,n+1)}$, $\,n\,$ being a positive integer, each containing a series that apparently can not be evaluated in closed form, distinctly from $\,ζ{(2\,n)}$, for which the Euler's formula allows us to write it as a rational multiple of $\,π^{2n}$. There in that work, however, the formulas are derived through certain series manipulations, by following Tsumura's strategy, which makes it \emph{curious} --- in the words of those authors themselves --- the appearance of the numbers $\,\ln{2}\,$ and $\,ζ{(2\,n+1)}$. In this short paper, I show how some known zeta-series can be used to derive the Dancs-He series in an alternative manner.
description: 7 pages, no figures. Second revision completed. Only small corrections. Submitted to J. T. N. Bordeaux (04/07/2011)
title: ÐÑÐ½Ð¾Ð²Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¸Ð·Ð°ÑÐ¸Ð¸. Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¤Ð¸Ð»Ð¸Ð¿Ð¾Ð²ÑÐºÐ¸Ð¹, ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: 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
ÐÐ»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ°
ÐÐ¾Ð´Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð²ÐµÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð¤ÐÐÐ¡ ÐÐ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 27.03.04 Â«Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð² ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼Ð°ÑÂ» (ÑÑÐ¾Ð²ÐµÐ½Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¸Ð°ÑÐ°). Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ ÐºÑÐ°ÑÐºÐ¸Ðµ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾Ð± Ð­ÐÐ, Ð¼ÐµÑÐ¾Ð´Ñ Ð¸ Ð¿Ð¾ÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¸Ð·Ð°ÑÐ¸Ð¸, ÐºÐ¾Ð´Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¾ÑÐ»Ð°Ð´ÐºÐ¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼. ÐÐ°Ð½Ñ Ð¿ÑÐ¸Ð¼ÐµÑÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÑÐ¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð°Ð´Ð°Ñ Ð½Ð° Ð­ÐÐ Ñ ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ Ð½Ð° Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ·ÑÐºÐ°Ñ. Ð¡Ð¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ðµ Ð½Ð°ÑÑÐ¾ÑÑÐµÐ³Ð¾ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð¾Ð¿Ð¸ÑÐ°ÐµÑÑÑ Ð½Ð° ÑÑÐ°Ð´Ð¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ Ð¸ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐµÑÐ½Ð¸ÐºÐ¸ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÑÑÑÐ¸Ñ ÑÑÑÑÐ¾Ð¹ÑÑÐ² Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ½ÑÑ ÑÑÐµÐ¼ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð². Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ ÐÑÑÑÐµÐ¹ Ð¨ÐºÐ¾Ð»Ñ ÐÐ¸Ð±ÐµÑÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼ Ð¸ Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ (Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Â«Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð² ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼Ð°ÑÂ») Ð² ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð»ÐµÐºÑÐ¸Ð¾Ð½Ð½ÑÑ ÐºÑÑÑÐ¾Ð² Ð¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ð¸ ÐºÑÑÑÐ¾Ð²ÑÑ Ð¸ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ ÐºÑÑÑÐ°Ð¼ "ÐÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ", "ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ°", "ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ°", "ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼" Ð¸ Ð´ÑÑÐ³Ð¸Ñ, ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÑ Ñ ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ Ð´Ð»Ñ Ð­ÐÐ.
Cromosfera ad alta definizione
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2013

Una visione molto ravvicinata e dettagliata della cromosfera solare è quella ottenuta da ricercatori dell'istituto tedesco Max Planck con le osservazioni in ultravioletto del telescopio solare Sunrise della NASA, che lo scorso giugno ha volato per cinque giorni sopra l'Atlantico con un pallone stratosferico.
Higher order energy conservation and global wellposedness of solutions for Gross-Pitaevskii hierarchies
Creators: name: Chen, Thomas
name: Pavlović, Nataša
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mathematical Physics (math-ph)
subject: Analysis of PDEs (math.AP)
subject: FOS: Physical sciences
subject: FOS: Mathematics
subject: 35Q55, 81V70

description: We consider the cubic and quintic Gross-Pitaevskii (GP) hierarchies in $d$ dimensions, for focusing and defocusing interactions. We introduce new higher order energy functionals and prove that they are conserved for solutions of energy subcritical defocusing, and $L^2$ subcritical (de)focusing GP hierarchies, in spaces also used by Erdös, Schlein and Yau in \cite{esy1,esy2}. By use of this tool, we prove a priori $H^1$ bounds for positive semidefinite solutions in those spaces. Moreover, we obtain global well-posedness results for positive semidefinite solutions in the spaces studied in the works of Klainerman and Machedon, \cite{klma}, and in \cite{chpa2}. As part of our analysis, we prove generalizations of Sobolev and Gagliardo-Nirenberg inequalities for density matrices.
description: AMS Latex, 36 pages
Online companion -Technical Impacts of the Deployment of Renewable Energy Community on Electricity Distribution Grids
Creators: name: Julien, Allard
name: Rosseel Arnaud
name: Sadoine Louise
name: Faraji Jamal
name: Brihaye Thomas
name: Capizzi Filippo
name: Nteziyaremye Boniface
name: Bordes François
name: Vallée François
name: De Grève Zacharie,
Publisher: name: Zenodo
Year: 2023

description: Online companion for the article "Technical Impacts of the Deployment of Renewable Energy Community on Electricity Distribution Grids".
title: ÐÐ½ÐµÐ´ÑÐµÐ½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ "ÐÐ¸ÑÑÐ¸ÐºÑ24" Ð² ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ "CustomServ" Ð´Ð»Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ñ ÐºÐ»Ð¸ÐµÐ½ÑÐ°Ð¼Ð¸ Ð¸ Ð¿Ð°ÑÑÐ½ÐµÑÐ°Ð¼Ð¸
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°Ð²ÑÐ¸Ð»Ð¾Ð², ÐÐ¸ÐºÐ¸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: 2018
Subjects: crm
itil
helpdesk
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description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ð¾ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÐ¸ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÐÐ¸ÑÑÐ¸ÐºÑ24 Ð² ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ CustomServ, Ð²Ð¾Ð·Ð½Ð¸ÐºÑÐµÐ¹ Ð½Ð° ÑÑÐ°Ð¿Ðµ ÑÐ¾ÑÑÐ° ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸, ÐºÐ¾Ð³Ð´Ð° Ð¿Ð¾ÑÐµÑÑ Ð²Ð°Ð¶Ð½Ð¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸, ÐµÐµ Ð¿Ð¾Ð¸ÑÐº Ð¸ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ðµ Ñ ÐºÐ»Ð¸ÐµÐ½ÑÐ°Ð¼Ð¸ Ð¸ Ð¿Ð°ÑÑÐ½ÐµÑÐ°Ð¼Ð¸ ÑÐ°ÑÑÐ¾ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¸Ð»Ð¸ Ðº ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¼ Ð¿Ð¾ÑÐµÑÑÐ¼ Ð¸ ÑÑÑÐ´ÑÐµÐ½Ð¸ÑÐ¼ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¹ Ð¼ÐµÐ¶Ð´Ñ ÐºÐ»Ð¸ÐµÐ½ÑÐ°Ð¼Ð¸ Ð¸ Ð¿Ð°ÑÑÐ½ÐµÑÐ°Ð¼Ð¸. ÐÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°ÑÑ ÑÐµÐºÑÑÑÑ ÑÐ°Ð±Ð¾ÑÑ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸, ÑÐ´ÐµÐ»Ð°ÑÑ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´Ð¾ Ð¸ Ð¿Ð¾ÑÐ»Ðµ, Ð´Ð»Ñ ÑÑÐ¿ÐµÑÐ½Ð¾Ð³Ð¾ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ, Ñ. Ðº. Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ð¹ Ð¸Ð´ÐµÐµÐ¹ Ð²ÑÑÑÑÐ¿Ð°ÐµÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ ÐµÐ´Ð¸Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ, ÐºÐ¾ÑÐ¾ÑÐ°Ñ Ð¼Ð°ÐºÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾ ÑÐ¼Ð¾Ð¶ÐµÑ Ð¿Ð¾ÐºÑÑÑÑ Ð²ÑÐµ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ CustomServ.
Ð Ð¾Ð±ÑÐ·Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼ Ð¿Ð¾ÑÑÐ´ÐºÐµ, Ð²ÑÐµ Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð´Ð¾Ð»Ð¶Ð½Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÑÑÑÑÑ ÑÐ¾Ð»ÑÐºÐ¾ Ð² ÑÑÐ¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ðµ, Ð¸ Ð¾ÑÐ¾Ð±Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ Ð½ÑÐ¶Ð½Ð¾ ÑÐ´ÐµÐ»Ð¸ÑÑ Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÐ¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸. ÐÑÐ´ÐµÐ»ÑÐ½ÑÐ¼ Ð·Ð²ÐµÐ½Ð¾Ð¼ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¸ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð¾Ð±Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÑÐ°Ð»Ð¸ Ð¼Ð½Ð¾Ð³Ð¾ÑÐ¸ÑÐ»ÐµÐ½Ð½ÑÐµ Ð½Ð°ÑÑÑÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸. Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÑÐµÑÑ Ð´Ð¾Ð»Ð¶Ð½Ñ Ð¿Ð¾Ð¼Ð¾ÑÑ ÑÐ´ÐµÐ»Ð°ÑÑ Ð²ÑÐ²Ð¾Ð´Ñ Ð¾ ÑÐ¾Ð¼, ÑÑÐ¾ ÑÐµÑÐµÐ½Ð¸Ðµ Ð¾ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ð¸ Ð¸ Ð²ÑÐµ Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð±ÑÐ»Ð¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ñ Ð¿ÑÐ°Ð²Ð¸Ð»ÑÐ½ÑÐ¼ Ð¾Ð±ÑÐ°Ð·Ð¾Ð¼. Ð ÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ÐÐ¸ÑÑÐ¸ÐºÑ24 Ð´Ð¾Ð»Ð¶Ð½Ñ Ð¿ÑÐ¸Ð²ÐµÑÑÐ¸ Ðº ÑÐ»Ð°Ð¶ÐµÐ½Ð½Ð¾Ð¹ Ð¸ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð² ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ CustomServ Ð¸ Ð¿ÑÐ°Ð²Ð¸Ð»ÑÐ½Ð¾Ð¼Ñ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ñ ÐºÐ»Ð¸ÐµÐ½ÑÐ°Ð¼Ð¸ Ð¸ Ð¿Ð°ÑÑÐ½ÐµÑÐ°Ð¼Ð¸. ÐÑÐµ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿ÑÐ¾ÑÐµÑÑÑ Ð²Ð½ÑÑÑÐ¸ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð¿Ð¾ÑÑÐµÐ¿ÐµÐ½Ð½Ð¾ Ð´Ð¾Ð»Ð¶Ð½Ñ Ð±ÑÑÑ Ð½Ð°Ð»Ð°Ð¶ÐµÐ½Ñ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ ÐÐ¸ÑÑÐ¸ÐºÑ24, Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸ÑÑ ÑÐ°Ð·Ð²Ð¸Ð²Ð°ÑÑÑÑ Ð´Ð°Ð»ÑÑÐµ Ð¸ ÐºÑÐµÐ¿ÐºÐ¾ ÑÐ´ÐµÑÐ¶Ð¸Ð²Ð°ÑÑÑÑ Ð½Ð° ÑÑÐ½ÐºÐµ.
A Banach space-valued ergodic theorem and the uniform approximation of the integrated density of states
Creators: name: Lenz, Daniel
name: Schwarzenberger, Fabian
name: Veselić, Ivan
Publisher: name: arXiv
Year: 2010
Subjects: subject: Mathematical Physics (math-ph)
subject: Spectral Theory (math.SP)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: In this paper we consider bounded operators on infinite graphs, in particular Cayley graphs of amenable groups. The operators satisfy an equivariance condition which is formulated in terms of a colouring of the vertex set of the underlying graph. In this setting it is natural to expect that the integrated density of states (IDS), or spectral distribution function, exists. We show that it can be defined as the uniform limit of approximants associated to finite matrices. The proof is based on a Banach space valued ergodic theorem which even allows explicit convergence estimates. Our result applies to a variety of group structures and colouring types, in particular to periodic operators and percolation-type Hamiltonians.
description: corrected version
Problemi dopo il lancio per BRRISON
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2013

Un'anomalia verificatasi circa due ore e mezza dopo il lancio mette in crisi la missione della NASA, destinata a studiare la cometa ISON con un telescopio montato su un pallone stratosferico. Si attendono aggiornamenti.
title: ÐÑÐµÐ½ÐºÐ° ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð½Ð°ÑÑÐ½Ð¾-Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½ÑÑ ÑÑÑÑÐºÑÑÑ
title: Evaluation of the effectiveness of integrated innovative scientific and educational structures
Creators: name: ÐÐ°ÑÐµÑÐºÐ°Ñ, ÐÐ°ÑÐ°Ð»ÑÑ
name: ÐÐ»ÑÑÐ¾Ð², ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
name: ÐÐ»Ð¾ÑÐºÐ¾Ð², Ð®ÑÐ¸Ð¹
name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ¾ÑÑÐ¼ (2018; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³). Ð¡ÐµÐºÑÐ¸Ñ "ÐÐ·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ðµ ÐºÐ°ÑÐµÐ´Ñ Ð®ÐÐÐ¡ÐÐ Ð¿Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÐºÐ°ÑÐµÑÑÐ²Ð¾Ð¼ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð¸Ð½ÑÐµÑÐµÑÐ°Ñ  ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ"
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2018

description: Ð¦ÐµÐ»Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð½Ð°ÑÑÐ½Ð¾-Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÑÑÑÐºÑÑÑÑ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐµÑ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÐµÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸. ÐÑÐµÐ½ÐºÐ° ÑÑÑÑÐºÑÑÑÑ Ð´ÐµÐ»Ð°ÐµÑÑÑ Ð´Ð»Ñ ÑÐ¾Ð³Ð¾, ÑÑÐ¾Ð±Ñ Ð¿Ð¾Ð½ÑÑÑ, Ð½Ð° ÐºÐ°ÐºÐ¾Ð¹ ÑÑÐ°Ð´Ð¸Ð¸ ÑÐ²Ð¾ÐµÐ³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð½Ð°ÑÐ¾Ð´Ð¸ÑÑÑ ÑÑÑÑÐºÑÑÑÐ°, Ð²ÑÐ¿Ð¾Ð»Ð½ÑÐµÑ Ð»Ð¸ Ð¾Ð½Ð° Ð¿Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÑ ÑÐµÐ»Ñ Ð¸ Ð¿Ð¾Ð»ÑÑÐ°ÐµÑ Ð»Ð¸ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ Ð´Ð¾Ð»Ð¶Ð½ÑÐµ Ð´Ð¸Ð²Ð¸Ð´ÐµÐ½Ð´Ñ.
description: The purpose of creating an integrated innovative scientific and educational structure
determines the indicators of its effectiveness. The purpose of the structure assessment is to understand at what stage of its development the structure is, whether it fulfils the set goal and whether the
University receives due dividends.
Effects of quasiparticle ambipolarity on the Nernst effect in underdoped cuprate superconductors
Creators: name: Tewari, Sumanta
name: Zhang, Chuanwei
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We consider the Nernst effect in the normal state of the underdoped cuprate superconductors, where recent quantum oscillation experiments have indicated the existence of Fermi surface pockets and quasiparticle ambipolarity in the excitation spectrum. Using an ambipolar d-density wave model for the pseudogap, we predict a peak in the Nernst coefficient with decreasing temperature below the pseudogap temperature. The existence of the peak and its sign, which we predict to be the same as that due to mobile vortices in a superconductor, result from the dominance of the electron pocket at low temperatures, as has been observed in recent Hall experiments.
description: 4 pages, 2 eps figures; parts rewritten, new references added; version as published in PRL
The synthesis of some secondary amyl and hexyl homologues of dinitro ortho and para cresols
Creators: name: Hillman, Melville Ernest Douglas
Publisher: name: University of British Columbia
Year: 2012

description: Eight new dinitro secondary amyl and hexylphenols of unequivocal structure were synthesized and characterized by their piperidine, morpholine and cyclohexylamine salts. The first step in the syntheses was the esterification of phenol to give phenyl acetate and phenyl propionate. A high temperature Fries rearrangement in the absence of solvent was used to convert the phenyl esters to o- and p-hydroxyaceto- and propiophenones. The alkyl o- and p-hydroxyphenyl ketones were then methylated with dimethylsulphate in an alkaline medium. The resulting methoxyacetophenones and methoxypropiophenones were reacted with Grignard reagents prepared from n- and isopropyl bromides. The tertiary alcohols thus obtained were dehydrated by refluxing in toluene, in the presence of iodine. The water in the water-toluene azeotrope was collected in a Dean and Stark tube. Nitrosyl chloride derivatives of the alkenes were prepared whenever possible, and analyzed for nitrogen. The alkenes were dissolved in ethanol and hydrogenated under 1000 p.s.i. pressure at 50° C. The resulting alkylanisoles were characterized as sulphonamides which were analyzed for both nitrogen and methoxyl content. The para alkylanisoles were demethylated by refluxing with pyridine hydrobromide at 200° C. The ortho alkyl anisoles were demethylated by refluxing with constant boiling hydriodic acid and phenol. The resulting alkylphenols were characterized as 3,5-dinitrobenzoate derivatives which were analyzed for nitrogen. The alkylphenols were nitrated to the dinitro derivativeswith concentrated nitric acid (density 1.50) in glacial acetic acid at -15° C. The piperidine, morpholine and cyclohexylamine salts were prepared by the addition of the amine to a benzene solution of the nitrophenol. The amine salts were analyzed for nitrogen. The alcohols, alkenes and alkylanisoles were analyzed for methoxyl values. Carbon and hydrogen analyses for the alkylphenols were also obtained. The phenols prepared were: 2-(o- and p-hydroxyphenyl)-pentane, 2-(o- and p-hydroxyphenyl)-3-methylbutane, 3-(o-and p-hydroxyphenyl)-hexane, 3-(o- and p-hydroxyphenyl)-2-methylpentane. A sample of "o-sec-amylphenol” obtained from Sharpies Chemicals Inc. was found to consist mainly of 2-(o-hydroxy-phenyl)-pentane. A Fries rearrangement of phenyl trimethyl acetate (phenyl pivalate) gave phenol as the only identifiable product, together with possible degraded and polysubstituted mixtures. o-Hydroxytrimethylacetophenone (o-hydroxypivalophenone) could not be separated or identified in the distillate.
Tenendo accese le stelle …
Creators: Caterina Boccato
Publisher: name: Media Inaf
Year: 2013

E’ iniziata alle cinque del pomeriggio la lunga notte europea dei ricercatori a Padova. Tema di quest’anno il Viaggio. Giochi, spettacoli, conferenze e mostre che hanno richiamato un pubblico attento e curioso. Un pubblico che in questo periodo di profonda crisi ha comunque voglia di credere nel futuro e che, per questo, si rivolge agli scienziati per avere risposte ma, soprattutto, per conoscere perché, a differenza di chi ci governa, sa quanto questo sia importante.
A Perugia è in scena SHARP
Creators: Francesco Rea
Publisher: name: Media Inaf
Year: 2013

Per la prima volta presente al Perugia Science Fest l'Istituto Nazionale di Astrofisica con una mostra allestita a Piazza Matteotti insieme ad un planetario portatile per un viaggio nello spazio destinato a grandi e piccini
Sotto il cielo di Kepler-7b
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2013

Usando il telescopio spaziale Kepler un gruppo di ricerca internazionale ha prodotto la prima mappa delle nuvole di un esopianeta, Kepler-7b. Un ulteriore tassello nella comprensione delle dinamiche atmosferiche esoplanetarie per l'individuazione dei segni distintivi della vita.
Compensation temperature of 3d mixed ferro-ferrimagnetic ternary alloy
Creators: name: Kis-Cam, Ebru
name: Aydiner, Ekrem
Publisher: name: arXiv
Year: 2009
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: In this study, we have considered the three dimensional mixed ferro-ferrimagnetic ternary alloy model of the type AB$_{p}$C$_{1-p}$ where the A and X (X=B or C) ions are alternately connected and have different Ising spins S$^{A}$=3/2, S$^{B}$=1 and S$^{C}$=5/2, respectively. We have investigated the dependence of the critical and compensation temperatures of the model on concentration and interaction parameters by using MC simulation method. We have shown that the behavior of the critical temperature and the existence of compensation points strongly depend on interaction and concentration parameters. In particular, we have found that the critical temperature of the model is independent on concentration of different types of spins at a special interaction value and the model has one or two compensation temperature points in a certain range of values of the concentration of the different spins.
description: To be published in JMMM
‘Barriers and facilitators to refugees, asylum seekers and people experiencing homelessness accessing non hospital based care’: A mixed methods systematic review protocol.
Creators: name: McGowan, Emer
name: Fitzharris, Laura
name: Broderick, Julie
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Medicine and Health Sciences
subject: Trinity College Dublin

description: Context: Social exclusion is characterised by and represents a form of disadvantage and marginalisation of vulnerable groups of people in society, who cannot fully participate in the normal activities of daily living. Socially excluded groups consist of, but are not limited to the following groups: people experiencing homelessness, asylum seekers and refugees. People from socially excluded groups have complex healthcare needs including infectious and non-communicable diseases. People from socially excluded groups tend to present more to the acute hospital setting as emergency presentations. Little is known about barriers and facilitators experienced by these groups to accessing non hospital based care. Objectives: This mixed methods systematic review, will critically examine the concept of ‘barriers’ and ‘facilitators’ for refugees, asylum seekers and people experiencing homelessness, to accessing non hospital based care. Methods: This methodological review will follow the Joanna Briggs Institute guidance for conducting mixed methods reviews. The following databases will be searched: Central Medline, PubMed, Embase, CINAHL, and the Cochrane Library. Relevant grey literature will be included. Title and abstract screening, followed by full-text screening will be undertaken independently by two reviewers. The Joanna Briggs Institute extraction tool will be adapted for data extraction. Discussion: This mixed method review will comprehensively evaluate quantitative and qualitative data, synthesise both barriers and facilitators and follow a systematic approach through establishing use of mixed methods research across a number of marginalised groups, and how they affect accessing non hospital based care. It will explore conceptual models of access to healthcare and how they influence these factors.
title: ÐÐ¸Ð»Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ Ñ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ½ÑÐ¼ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸ÐµÐ¼ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð·Ð¸Ð¼Ð½ÐµÐ³Ð¾ Ð±ÐµÑÐ¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸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ÑÑÑÑ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: 2018
Subjects: Ð¼Ð¾Ð½Ð¾Ð»Ð¸ÑÐ½Ð¾Ðµ Ð´Ð¾Ð¼Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾
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description: Ð¡ÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ Ð¾ÑÑÐ°ÑÐ»Ñ Ð¾ÑÐµÐ½Ñ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐ½Ð¾ ÑÐ°Ð·Ð²Ð¸Ð²Ð°ÐµÑÑÑ. ÐÐ¾Ð·Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð·Ð´Ð°Ð½Ð¸Ð¹ Ð¸ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹ Ð¸Ð· Ð±ÐµÑÐ¾Ð½Ð° Ð²ÑÐµ ÑÐ°ÑÐµ Ð²ÑÑÑÐµÑÐ°ÐµÑÑÑ Ð² Ð¿ÑÐ¾ÐµÐºÑÐ°Ñ Ð·Ð´Ð°Ð½Ð¸Ð¹ Ð¸ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹. Ð¦ÐµÐ»ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÑ ÑÑÐ¾Ð²ÐµÐ½Ñ Ð¾ÑÐµÑÐµÑÑÐ²ÐµÐ½Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð·Ð¸Ð¼Ð½ÐµÐ³Ð¾ Ð±ÐµÑÐ¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. Ð Ð°Ð±Ð¾ÑÐ° ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¾Ð±Ð·Ð¾Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° Ð±ÐµÑÐ¾Ð½Ð½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ñ Ð·Ð´Ð°Ð½Ð¸Ð¹ Ð¸ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹ Ð² Ð·Ð¸Ð¼Ð½ÐµÐµ Ð²ÑÐµÐ¼Ñ Ð¿ÑÐ¸ ÑÑÐµÐ´Ð½Ðµ Ð¾ÑÑÐ¸ÑÐ°ÑÐµÐ»ÑÐ½ÑÑ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÐ°Ñ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¿Ð¾ÑÐ¾Ð±Ð¾Ð² Ð·Ð¸Ð¼Ð½ÐµÐ³Ð¾ Ð±ÐµÑÐ¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, Ð¾Ð¿Ð¸ÑÐ°Ð½Ñ Ð¸Ñ Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ, Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐºÐ¸ Ð¸ Ð¿ÑÐµÐ¸Ð¼ÑÑÐµÑÑÐ²Ð° ÐºÐ°Ð¶Ð´Ð¾Ð³Ð¾ Ð¸Ð· ÑÐ¿Ð¾ÑÐ¾Ð±Ð¾Ð². ÐÐ°Ð½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÐºÐ°Ð¶Ð´Ð¾Ð³Ð¾ Ð¸Ð· ÑÐ¿Ð¾ÑÐ¾Ð±Ð¾Ð² Ð·Ð¸Ð¼Ð½ÐµÐ³Ð¾ Ð±ÐµÑÐ¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð²ÑÐ´ÐµÑÐ¶Ð¸Ð²Ð°Ð½Ð¸Ñ Ð±ÐµÑÐ¾Ð½Ð½Ð¾Ð¹ ÑÐ¼ÐµÑÐ¸ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ ÑÑÐµÐ´Ð½Ð¸Ñ Ð¾ÑÑÐ¸ÑÐ°ÑÐµÐ»ÑÐ½ÑÑ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑ Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´Ñ. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¾ ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ, Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð½Ð¾Ðµ Ð½Ð° Ð¸Ð½ÑÐµÐ½ÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ½ÐµÑÐ³Ð¾Ð·Ð°ÑÑÐ°Ñ Ð¸ ÑÑÑÐ´Ð¾ÐµÐ¼ÐºÐ¾ÑÑÐ¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÑÐµÐ¼ÑÑ ÑÐ°Ð±Ð¾Ñ. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ ÑÑÐ¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ´ÐµÐ»Ð°Ð½ Ð²ÑÐ²Ð¾Ð´ Ð¾ Ð»ÑÑÑÐµÐ¼ Ð¼ÐµÑÐ¾Ð´Ðµ Ð·Ð¸Ð¼Ð½ÐµÐ³Ð¾ Ð±ÐµÑÐ¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ.
title: Representing thunderstorm electrification for lightning forecast evaluation
Creators: name: Courtier, Ben
Publisher: name: University of Reading
Year: 2020

description: Forecasts of lightning in the Met Office’s Unified Model (MetUM) are known to overforecast the total number of lightning flashes in the UK. One of the difficulties in understanding why this happens comes from the dependence of the lightning forecast on the convective forecast. This problem can be mitigated using a more physically representative forecasting method to compare against and by comparing lightning production in modelled thunderstorms to that in observed thunderstorms. In order to provide a more physically representative forecasting method a new, explicit thunderstorm electrification and lightning scheme is implemented within the MetUM. This scheme uses non-inductive collisional charging to represent the charge generated on hydrometeors and produce a charge density distribution. From this, the magnitude of the electric field is calculated, with appropriate thresholds selected to allow initiation of lightning events. It is shown that this scheme accurately represents observed thunderstorm charge magnitude and structure. Results from the new electrification scheme are compared with those from the existing lightning parameterisation within the MetUM, and to natural lightning observations in two case studies. The new electrification scheme performs well in both a scattered, fair weather convection case study in the UK and an organised, deep convection case study in the US. It shows realistic lightning coverage and reproduced the daily lightning flash accumulation relatively accurately. The collision-separation efficiency is found to be a key parameter and therefore a potential source of uncertainty in the scheme. Through comparison with the new scheme, the existing MetUM parameterisation is shown to be producing lightning in a manner that is too closely dependent on the rainfall accumulation, which it is suggested is related to its poor performance in the UK case study. Observations of single cell thunderstorms are used to investigate the production of lightning in thunderstorms in the UK. It is found that prior to the onset of lightning production, single cell thunderstorms show an increase in storm core area. Model simulations of similarly intensifying thunderstorms show that, during these intensifications, the updraft velocity and area both increase, as does the graupel mass in the storm core. It is shown that the new electrification scheme can reproduce the increase in updraft area and graupel mass in intensifying storms, whereas the existing lightning parameterisation does not reproduce any of these parameters. The use of this new electrification scheme, whilst not operationally feasible with existing computer power, provides a research tool with which to further improve lightning forecasting.
La mongolfiera che rincorre la cometa
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2013

Anche un pallone stratosferico per studiare la ISON. Verrà lanciato il 29 settembre per la prima missione di un giorno. Raggiungerà l'altitudine di 37 chilometri sopra la Terra e, a quell'altezza, sarà largo circa 140 metri. A bordo un telescopio da 80 cm per osservazioni nell'infrarosso, nella luce visibile e nel vicino ultravioletto.
Singular integrals on Ahlfors-David regular subsets of the Heisenberg group
Creators: name: Chousionis, Vasilis
name: Mattila, Pertti
Publisher: name: arXiv
Year: 2009
Subjects: subject: Analysis of PDEs (math.AP)
subject: Metric Geometry (math.MG)
subject: FOS: Mathematics

description: We investigate certain singular integral operators with Riesz-type kernels on s-dimensional Ahlfors-David regular subsets of Heisenberg groups. We show that $L^2$-boundedness, and even a little less, implies that $s$ must be an integer and the set can be approximated at some arbitrary small scales by homogeneous subgroups. It follows that the operators cannot be bounded on many self similar fractal subsets of Heisenberg groups.
description: We added a much simpler proof of Lemma 2.11 and one reference
Un viaggio pieno d’energia
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2013

In uno studio pubblicato sulla rivista Science, il più dettagliato resoconto dei processi di conversione dell'energia di origine solare che avvengono nella magnetosfera della Terra. Un importante passo per migliorare le previsioni degli effetti dell'attività della nostra stella sull'ambiente terrestre.