Search results for "SCAE"

showing 6 items of 6 documents

La formula di Mucio Scevola, i nomi delle azioni e l'agere per concepta uerba

2021

The formula Mucii Scaeuolae depicted in the fresco of ‘The Jurist’s Villa’ upon the Aniene river probably does not refer to a specific action of the formulary procedure (agere per formulas). The pratice of naming some actions after the nomen gentilicium of a praetor is in fact attested in our sources only after the so-called codification of the Edictum Perpetuum in the age of Hadrian. The discovery of the fresco leads us to reflect once again on the origins of the formulary procedure, since the Mucius Scaevola of the fresco inscription may well refer to the jurist Quintus Mucius Scaevola. This in turn might suggest both that he was actually owner of the villa and that it was he who introduc…

Civil Roman procedureagere per concepta uerbaRoman jurisprudenceQuintus Mucius Scaeuolathe Jurist’s Villa
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Ruolo dei parassitoidi oofagi nel controllo naturale dei fitofagi del nocciolo responsabili del “cimiciato delle nocciole” nel Parco dei Nebrodi (ME).

2009

Role of oophagous parasitoids in the natural control of hazelnut bugs inducing the “cimiciato seeds” in Nebrodi Park (ME) Oophagous parasitoids of bugs collected on hazelnut cultivations and seasonal parasitism on eggs of Gonocerus acutengulatus (Goeze) were studied from 2004 to 2006 in the Nebrodi Park (ME). Samples of bug eggs were collected in three altitude areas, 300-590, 600-890 and 900-1100 m above sea level, and examined in laboratory. Parasitoid adults obtained from all eggs were identified. Parasitization levels, detected on G. acuteangulatus in all areas showed a similar trend with the most value on August. Significant regression between the total number of eggs and the number of…

Controllo biologico Anastatus bifasciatus Gryon muscaeformis Telenomus viggianiSettore AGR/11 - Entomologia Generale E Applicata
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X-ray emission from MP Muscae: an old classical T Tauri star

2007

We study the properties of X-ray emitting plasma of MP Mus, an old classical T Tauri star. We aim at checking whether an accretion process produces the observed X-ray emission and at deriving the accretion parameters and the characteristics of the shock-heated plasma. We compare the properties of MP Mus with those of younger classical T Tauri stars to test whether age is related to the properties of the X-ray emission plasma. XMM-Newton X-ray spectra allows us to measure plasma temperatures, abundances, and electron density. In particular the density of cool plasma probes whether X-ray emission is produced by plasma heated in the accretion process. X-ray emission from MP Mus originates from…

PhysicsElectron densitystars: abundances stars: circumstellar matter stars: coronae stars: individual: MP Muscae stars: pre-main sequence X-rays: starsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)X-rayHigh densityFOS: Physical sciencesAstronomy and AstrophysicsPlasmaAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsSpectral lineAccretion (astrophysics)Accretion rateT Tauri starSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Galaxy Astrophysics
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A method for anomaly detection in hyperspectral images, using deep convolutional autoencoders

2017

Menetelmä poikkeavuuksien havaitsemiseen hyperspektrikuvista käyttäen syviä konvolutiivisia autoenkoodereita. Poikkeavuuksien havaitseminen kuvista, erityisesti hyperspektraalisista kuvista, on hankalaa. Kun ongelmaan yhdistetään ennalta tuntematon data ja poikkeavuudet, muodostuu ongelma vielä laajemmaksi. Spektraalisten poikkeavuuksien havaitsemiseen on kehitetty useita eri menetelmiä, mutta spatiaalisten poikkeavuuksien havaitseminen on huomattavasti hankalempaa. Tässä työssä esitellään uudenkaltainen menetelmä sekä spatiaalisten että spektraalisten poikkeavuuksien samanaikaiseen havaitsemiseen. Menetelmä on suunniteltu erityisesti spektraaliselle datalle, mutta soveltuu myös perinteisil…

hyperspectral imagesautoencoderautoenkooderithdbscanSCAEconvolutional neural networkdeep learninghavaitseminenneuroverkotanomaly detectionconvolutional autoencodermachine learningkoneoppiminenpoikkeavuuskonvoluutioälytekniikkaCAEhyperspektrikuvatautoenkooderi
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X-ray emission from the old CTTS MP Muscae

2007

We study the properties of X-ray emitting plasma of MP Mus, an old classical T Tauri star. XMM-Newton/RGS spectra allow us to measure the plasma electron density, which probes whether X-ray emission is produced in the accretion process. X-ray emission from MP Mus originates from high density cool plasma but a hot flaring component is also present, suggesting that both coronal magnetic activity and accretion contribute to the observed X-ray emission. From the soft part of the X-ray emission from MP Mus, mostly produced by plasma heated in the accretion shock, we derive the accretion parameters and the characteristics of the shock-heated plasma.

stars: coronaestars: individual: MP MuscaeSettore FIS/05 - Astronomia E Astrofisicastars: abundancesX-rays: starsstars: circumstellar matterstars: pre-main sequence
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X-ray emission from an adolescent classical T Tauri star

2007

stars: coronaestars: individual: MP MuscaeSettore FIS/05 - Astronomia E Astrofisicastars: abundancesX-rays: starsstars: circumstellar matterstars: pre-main sequence
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