Processos de aquecimento na alta atmosfera estelar: emissão coronal em raio-x e emissão cromosférica em CaII

In the present work we study the processes of heating in the high stellar atmosphere, with base in an analysis of behavior of the cromospheric and coronal emission for a sample of single stars classified as giant in the literature. The evolutionary status of the stars of the sample was determined from HIPPARCOS satellite trigonometric parallax measurements and from the Toulouse Genéve code. In this study we show the form of behavior of the CaII emission flux in spectral lines H and K F(CaII) and the X-ray emission flux in function of the rotation, number of Rossby Ro and depth in mass of the convective envelope. In this analysis we show that while the cromospheric activity is dominated clearly by a physical process of heating associated with the rotation, like a magnetic field produced by dynamo effect, the coronal activity seems to be influenced for a mechanism independent of the rotation. We show also that the effective role of the depth in massa of the convective envelope on the stellar activity has an important effect in the responsible physical process for the behavior of the activity in the atmosphere of the stars.

Investigando o campo magnético das estrelas análogas e gêmeas solares através da espectropolarimetria

This study proposes an observing program focused on the investigation of the stellar magnetism and dynamo evolution in cool active solar-like stars. More mainly in the solar analogs and twins. Observations of stars of our base were carried out with two spectropolarimeter (ESPaDOnS@CFHT and NARVAL@TBL). The analyse of stars in stage different allows an understanding of the dependence of magnetic activity on basic stellar parameters such as rotation, mass, age and depth of the convection zone. This study provides measures necessary for testing dynamo theories. The 65 targets for this project are solar type stars with mass spanning from 0:9 M=Mfi 1:075 solar masses and at different evolutionary stages. Our two main science objectives were, (i) To determine how the magnetic field evolved from the ZAMS to the TO (turn off) for stars with 0:9 M=Mfi 1:075; (ii) To determine the impact of convective depth and rotation on magnetic of cool stars of solar type. The main result from this study was the characterization of the dependence of magnetic field intensity as function of age, Rossby number and the convective zone deepening. This context, the availability of ESPaDOnS and NARVAL opens an exceptional possibility to study the magnetic properties of Sun-like stars by means of spectropolarimetric observations

The correlation between thermal comfort in buildings and fashion products

This article is about thermal comfort in the wearable product. The research correlates fashion and architecture, in so far as it elects the brise soleil - an architectural element capable of regulating temperature and ventilation inside buildings - as a study referential, in trying to transpose and adapt its mechanisms to the wearable apparel.

Mineralizações auríferas hospedadas na faixa metavulcano-sedimentar Jacuí-Bom Jesus da Penha - Sudoeste de Minas Gerais

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Leptogenesis via hypermagnetic fields and baryon asymmetry

We study baryon asymmetry generation originated from the leptogenesis in the presence of hypermagnetic fields in the early Universe plasma before the electroweak phase I ransition (EWPT). For the simplest Chern-Simons (CS) wave configuration of hypermagnetic field we find the baryon asymmetry growth when the hypermagnetic field value changes due to alpha(2)-dynamo and the lepton asymmetry rises due to the Abelian anomaly. We solve the corresponding integro-differential equations for the lepton asymmetries describing such selfconsistent dynamics for lepto- and baryogenesis in the two scenarios: (i) when a primordial lepton asymmetry sits in right electrons e(R); and (ii) when, in addition to e(R), a left lepton asyninwtty for e(L) and v(eL) at due to chirality flip reactions provided by in Iiigg,s decays at the temperatures, T < T-RL similar to 10 TeV. We find that the baryon asymmetry of the Universe (BAU) rises very fast through such leptogenesis, especially, in strong hypermagnetic fields. Varying (decreasing) the CS wave number parameter k(0) < 10(-7) T-EW one can recover the observable value of BAU, eta(B) similar to 10(-9), where k(0) = 10(-7) T-EW corresponds to the ataxinittat value for CS wave number surviving ohmic dissipation of hypermagnetic field. In the scenario (ii) one predicts the essential difference of the lepton numbers of right- and left electrons at EWPT time, L-eR - L-eL similar to (mu(eR) / mu(eL))/T-EW = Delta mu/T-EW similar or equal to 10(-5) that can be used as an initial condition for chiral asymmetry after EWPT.

Magnetic flux transport by turbulent reconnection in astrophysical flows

The role of magnetohydrodynamics (MHD) turbulence in astrophysical environments is still highly debated. An important question that permeates this debate is the transport of magnetic flux. This is particularly important, for instance, in the context of star formation. When clouds collapse gravitationally to form stars, there must be some magnetic flux transport. Otherwise, the newborn stars would have magnetic fields several orders of magnitude larger than the observed ones. Also, the magnetic flux that is dragged in the late stages of the formation of a star can remove all the rotational support from the accretion disc that grows around the protostar. The efficiency of the mechanism that is often invoked to allow transport of magnetic fields at different stages of star formation, namely ambipolar diffusion, has recently been put in check. We discuss here an alternative mechanism for magnetic flux transport which is based on turbulent fast magnetic reconnection. We review recent results from three-dimensional MHD numerical simulations that indicate that this mechanism is very efficient in decoupling and transporting magnetic flux from the inner denser regions to the outskirts of collapsing clouds at different stages of star formation. We discuss this mechanism also in the context of dynamo processes and speculate that it can play a role both in solar dynamo and in accretion disc dynamo processes.

Ricerca di criteri analitico-progettuali per la riqualificazione paesaggistica di strutture e infrastrutture in aziende agricole multifunzionali.

Obiettivo generale dello studio è rivolto alla definizione di linee d’indirizzo volte alla riqualificazione paesaggistica, per l’integrazione ed il recupero delle corti e degli edifici moderni dei centri aziendali agricoli a carattere multifunzionale in territorio rurale, attraverso soluzioni appropriate sia sul piano tecnologico-formale che su quello economico-funzionale. Con riferimento ad un’area studio sovracomunale della provincia di Bologna (Regione Emilia-Romagna), si è determinato, quale obiettivo specifico, l’individuazione delle possibili soluzioni di riqualificazione, da realizzarsi in economia, cioè primariamente attraverso i mezzi e le competenze normalmente disponibili in un’azienda agricola di questo tipo. A seguito del riconoscimento dei caratteri specifici e dei tipi edilizi degli edifici rurali tradizionali nella pianura emiliano romagnola, dell’identificazione delle metodologie d’indagine dei caratteri degli edifici rurali in letteratura, nonché dell’analisi della normativa di riferimento in materia di aziende multifunzionali, sono state definite le aziende studio, appartenenti ad aree geografiche differenti. La metodologia d’indagine individuata è stata condotta per la determinazione delle tipologie costruttive, dei materiali utilizzati e dei requisiti delle aziende, in relazione alle diverse specificità, alla definizione funzionale degli spazi costruiti, degli spazi aperti e delle differenti relazioni fra essi e l’identificazione ed analisi dei percorsi delle diverse tipologie di fruitori. L’identificazione delle criticità dei caratteri architettonici riscontrate, sia negli edifici agricoli sia nella corte, ha condotto al riconoscimento degli ambiti di intervento per la progettazione delle soluzioni di riqualificazione funzionale e paesaggistica, attraverso lo studio delle possibili soluzioni per la schermatura o rivalorizzazione sia degli edifici moderni di servizio all’agricoltura (analizzando le potenzialità progettuali offerte dalle pareti verdi, dai brise soleil, dalle facciate ventilate o da intonaci e tinteggiature), sia per la riqualificazione dei percorsi e degli aspetti paesaggistici (intervenendo sulla proposta di materiali da pavimentazione, e delle essenze da utilizzare), da realizzarsi in economia, ma comparati con alternative proposte di tipo commerciale.

1967-1987: l'altra civiltà del testo. Impulsi storici e scrittura nel teatro d'innovazione francese

Lo studio analizza le svolte nel teatro di innovazione francese prodotte dalla rivolta sociale e dalla sua rivoluzione culturale del 1968. La ricerca si è concentrata su tre livelli di analisi: un'analisi – storica, politica, sociale, culturale – dell'anno-tournant; un'analisi delle reazioni nel mondo del teatro contemporanee alla rivolta; un'analisi delle prassi spettacolari di lunga durata originate dall'evento. Sono stati, quindi, esaminati criticamente i testi cardine degli intellettuali ispiratori, protagonisti e interpreti della breccia culturale, per poi rintracciare i valori emersi all'interno del mondo dello spettacolo. La contestazione sociale ha agito sul mondo del teatro producendo delle ripercussioni immediate – l'occupazione dell'Odéon, la contestazione al XXII Festival d'Avignon, la produzione della Déclaration de Villeurbanne – e delle prassi di lunga durata che hanno agito sui processi formativi e creativi delle compagnie francesi che, dalla fine degli anni Sessanta, hanno prodotto creazioni collettive (in particolare il Théâtre du Soleil e il Théâtre de l'Aquarium, ma anche la Nouvelle Compagnie d'Avignon, il Grand Magic Circus e il Théâtre Populaire di Lorraine) e sul corpus drammaturgico e teorico di Michel Vinaver. Sono state, quindi, analizzate le relazioni che si sono instaurate tra i protagonisti appena nominati e i differenziati contesti, sociali e teatrali, facendo emergere nuove istanze creative. Tali istanze hanno saputo rispondere alle spinte etiche ed estetiche del momento storico, le hanno declinate sul piano delle prassi teatrali e rilanciate verso modalità nuove che hanno favorito l'emersione di una nuova civiltà del testuale.

Evidence for distinct modes of solar activity

The Sun shows strong variability in its magnetic activity, from Grand minima to Grand maxima, but the nature of the variability is not fully understood, mostly because of the insufficient length of the directly observed solar activity records and of uncertainties related to long-term reconstructions. Here we present a new adjustment-free reconstruction of solar activity over three millennia and study its different modes. Methods. We present a new adjustment-free, physical reconstruction of solar activity over the past three millennia, using the latest verified carbon cycle, 14C production, and archeomagnetic field models. This great improvement allowed us to study different modes of solar activity at an unprecedented level of details. Results. The distribution of solar activity is clearly bi-modal, implying the existence of distinct modes of activity. The main regular activity mode corresponds to moderate activity that varies in a relatively narrow band between sunspot numbers 20 and 67. The existence of a separate Grand minimum mode with reduced solar activity, which cannot be explained by random fluctuations of the regular mode, is confirmed at a high confidence level. The possible existence of a separate Grand maximum mode is also suggested, but the statistics is too low to reach a confident conclusion. Conclusions. The Sun is shown to operate in distinct modes – a main general mode, a Grand minimum mode corresponding to an inactive Sun, and a possible Grand maximum mode corresponding to an unusually active Sun. These results provide important constraints for both dynamo models of Sun-like stars and investigations of possible solar influence on Earth’s climate.

Ce(III) and Ce(IV) (re)distribution and fractionation in a laterite profile from Madagascar: Insights from in situ XANES spectroscopy at the Ce LIII-edge

The distribution of trivalent and tetravalent cerium, Ce(III) and Ce(IV) respectively, in a lateritic profile from Madagascar, has been characterized by X-ray-absorption near-edge structure (XANES) spectroscopy at the Ce LIII-edge on the LUCIA beamline (SOLEIL synchrotron, France). XANES spectra were acquired on bulk-rock samples as well as on specific lateritic minerals or polymineral zones (in-situ measurements) of the tonalite bedrock and the three overlying weathered horizons (C-, B- and A-horizons). Geochemically, the bedrock, and the A- and C-horizons show similar rare earth element content (REE = 363–405 mg/kg). They also display the same positive Ce-anomaly (CeCN/Ce∗ = 1.12–1.45), which is therefore likely to be inherited from the bedrock. In the B-horizon, the higher REE content (REE = 2194 mg/kg) and the larger Ce-anomaly (CeCN/Ce∗ = 4.26) are consistent with an accumulation zone caused by the evaporation of groundwater during the dry season. There is a good agreement between the Ce(III)/Cetotal ratio (XCe(III)) deduced from the positive Ce-anomaly (bulk-rock geochemical data) and that derived from XANES spectroscopy on the same bulk-rock samples (BR-XCe(III)-XANES) in the bedrock, and the C- and B-horizons. In the A-horizon, XANES measurements on bulk rock and minerals revealed a higher BR-XCe(III)-XANES (up to 100%) compared to the XCe(III) deduced from geochemical data (XCe(III) = 79%). The preservation of a positive Ce-anomaly in the A-horizon suggests that the Ce mobilization and redistribution during weathering occurred with no significant Ce fractionation from other trivalent REE. Remarkably, the only investigated sample where cerianite is observed belongs to the B-horizon. Within this horizon, Ce oxidation state varies depending on the microstructural position (porosity, cracks, clay-rich groundmass). The highest Ce(IV) concentrations are measured in cerianite (and aluminophosphates) localized in pores at the vicinity of Mn-rich domains (XCe(III)-XANES = 30–51%). Therefore, Ce fractionation from other REE is attributed to a Ce oxidation and precipitation potentially assisted by oxyhydroxide scavenging. In the C-horizon, Ce(III) and Ce(IV) are mainly distributed in REE-minerals of the rhabdophane group found in pores and cracks. The similarity between the Ce(III) proportion of rhabdophane grains (XCe(III)-XANES = 74–89%) with that of the bedrock (BR-XCe(III)-XANES = 79%) suggests no significant fractionation of Ce(III) and Ce(IV) between solution and mineral during the successive stages of primary REE-mineral alteration, transport in solution and secondary precipitation in the incipient stages of weathering. Overall, our novel spectroscopic approach shows that Ce is not necessarily oxidized nor fractionated from other REE during weathering in lateritic conditions. This implies that like Ce(III), Ce(IV) can be mobilized in aqueous fluids during weathering, possibly thanks to complexation with organic molecules, and can precipitate together with Ce(III) in secondary REE-bearing minerals. The corollary is that (paleo)redox reconstructions in soils and/or sediments based on Ce-anomaly in weathered rocks or minerals must be interpreted with caution.

El color en el siglo XIX: utilización de fondos de colores oscuros en los revestimientos de paramentos interiores en la arquitectura del siglo XIX

El Color en el Siglo XIX: Utilización de Fondos de Colores Oscuros en los Revestimientos de Paramentos Interiores en la Arquitectura del Siglo XIX De los elementos del pasado el color es el que más rápidamente cambia y se deteriora, por lo que no podemos saber las condiciones originales de color e iluminación en los interiores que han llegado hasta nosotros. Frecuentemente nos enfrentamos a los problemas que plantean los espacios del pasado, proyectando nuestros propios criterios sobre color y luz, que no tienen que coincidir necesariamente con los criterios de épocas anteriores. En las hermosas láminas del libro de Cesar Daly ?Décorations intérieures: peintes? de 1877, observamos que los colores que decoran las paredes son sorprendentemente oscuros. La oscuridad de estos muros es más sorprendente si pensamos en la débil luz de llama que iluminaba las salas en esa época, muy inferior a los niveles de luz que nos proporciona la luz eléctrica hoy en día. No obstante, esta débil iluminación sobre paredes de tonos oscuros puede tener alguna ventaja. Las paredes y las líneas de la habitación se difuminan en las sombras, mientras los objetos brillantes que decoran la habitación, como los cuadros, los barnices de los muebles y de los instrumentos musicales, y sobre todo los trajes y los rostros, reflejan la tenue luz, destacando sobre el fondo oscuro de las paredes, convirtiéndose en el centro de una escenografía. Es lo que Lewis Mumford en su Libro ?Técnica y civilización?, llama la ?ventaja estética? del mundo oscuro de la Revolución Industrial, dominado por el uso del carbón, que contamina el ambiente, transforma el color de los edificios y produce nieblas que atenúan la luz. En este mundo, según este autor, se acrecienta la sensibilidad por la luz, y se valora como un bien preciado la luz tenue que brilla entre la niebla que disuelve los objetos, lo que podemos observar en cuadros como el de ?Lluvia, vapor y velocidad? de Turner, o ?Impressión: soleil levant? de Monet. La importancia de los fondos de color oscuro se hace evidente al comprobar cómo los diseñadores de vanguardia del siglo XX para superar el mundo caduco del XIX deciden pintar de blanco las superficies, lo que se convierte en el signo de la modernidad.

COMUNICAÇAO INTEGRADA DE MARKETING E AÇÕES DE PATROCÍNIO A EVENTOS: O EFEITO SINÉRGICO

Este trabalho enfoca a ação de patrocínio a eventos como ferramenta comunicacional, incorporada ao composto da comunicação de marketing. O principal objetivo é analisar e apresentar como as empresas usam e articulam as ferramentas da comunicação integrada de marketing às ações de patrocínio para se criar um efeito sinérgico de comunicação. A metodologia constitui-se em pesquisa bibliográfica e documental e o estudo de casos envolvendo as empresas Ambev, Petrobras e Bradesco com o patrocínio aos respectivos eventos: Skol Beats; Jogos Pan-americanos 2007 e o Espetáculo Saltimbanco do Cirque du Soleil, verificando como os aspectos teóricos foram apropriados em cada caso. As conclusões apontam, principalmente, que as empresas vêm buscando utilizar o potencial máximo de comunicação dos eventos não só ao promoverem, mas também na condição de patrocinadoras, e que o patrocínio deve ser parte de um plano integrado, no qual as ações estratégicas de comunicação de marketing, através das várias ferramentas que as constituem, podem e devem ser conjugadas para alcançar sinergia e valorizar as ações comunicacionais dos patrocinadores.(AU)

COMUNICAÇAO INTEGRADA DE MARKETING E AÇÕES DE PATROCÍNIO A EVENTOS: O EFEITO SINÉRGICO

Este trabalho enfoca a ação de patrocínio a eventos como ferramenta comunicacional, incorporada ao composto da comunicação de marketing. O principal objetivo é analisar e apresentar como as empresas usam e articulam as ferramentas da comunicação integrada de marketing às ações de patrocínio para se criar um efeito sinérgico de comunicação. A metodologia constitui-se em pesquisa bibliográfica e documental e o estudo de casos envolvendo as empresas Ambev, Petrobras e Bradesco com o patrocínio aos respectivos eventos: Skol Beats; Jogos Pan-americanos 2007 e o Espetáculo Saltimbanco do Cirque du Soleil, verificando como os aspectos teóricos foram apropriados em cada caso. As conclusões apontam, principalmente, que as empresas vêm buscando utilizar o potencial máximo de comunicação dos eventos não só ao promoverem, mas também na condição de patrocinadoras, e que o patrocínio deve ser parte de um plano integrado, no qual as ações estratégicas de comunicação de marketing, através das várias ferramentas que as constituem, podem e devem ser conjugadas para alcançar sinergia e valorizar as ações comunicacionais dos patrocinadores.(AU)

Six duos pour voix égales pouvant être chantés en chœur avec accompagnement de piano.

Cover title.

Journal des observations physiques, mathematiques et botaniques ... /

Contiene con portadilla y sign. propias : Tables des declinaisons du soleil ...