Evoluzione dell’inventario di radioisotopi rilevanti ai fini del trattato CTBT per il bando dei test nucleari, tramite l’utilizzo del codice di calcolo ORIGEN-ARP

L’oggetto di questa tesi è lo studio dei radionuclidi rilevanti che vengono generati dalla detonazione di ordigni nucleari. L’obiettivo principale è la ricerca di parametri legati alle sostanze radioattive derivanti dalla fissione nucleare che permettano di capire se c’è stato un rilascio non autorizzato di radioisotopi legati all’esplosione di una bomba nucleare. Inoltre dall’inventario dei nuclidi rilevati si vuole cercare di capire che tipo di tecnologia è stata utilizzata per la costruzione dell’ordigno facendo riferimento a specifici rapporti isotopici. Per ricavare il probabile inventario dei radionuclidi derivanti da fissione è stato utilizzato il codice di calcolo Origen-Arp, programma utilizzato per l’analisi isotopica delle sostanze derivanti dalla “combustione” di materiale fissile all’interno di un reattore nucleare. Il lavoro svolto quindi ha riguardato una parte prettamente sperimentale in cui è stato utilizzato il codice di calcolo e una parte più teorica grazie alla quale è stato possibile contestualizzare i risultati trovati.

Bill Arp's scrap book; humor and philosophy.

Mode of access: Internet.

Caracterização funcional de dois cDNAs homólogos à ciclofilina e à proteína reprimida por auxina (ARP) identificados em bibliotecas subtrativas a para floração em tomateiro

Flowering is a fundamental process in the life cycle for plant. This process is marked by vegetative to reproductive apical meristem conversion, due to interactions between several factors, both internal and external to plant. Therefore, eight subtractive libraries were constructed using apical meristem induced or not induced for two contrasting species: Solanum lycopersicum cv. Micro-Tom and Solanum pimpinellifolium. Several cDNAs were identified and among these, were selected two cDNAs: one homologous cDNA to cyclophilin (LeCYP1) and the other to Auxin repressed protein (ARP). It has observed that LeCYP1 and ARP genes are important in the developmental process to plants. In silico analysis, were used several databases with the exclusion criterion E-value <1.0x10-15. As a result, conservation was observed for proteins analyzed by means of multiple alignments and the presence of functional domains. Then, overexpression cassettes were constructed for the ARP cDNA in sense and antisense orientations. For this step, it was used the CaMV35S promoter. The cDNA orientation (sense or antisense) in relation to the promoter was determined by restriction enzymes and sequencing. Then, this cassette was transferred to binary vector pZP211 and these cassettes were transferred into Agrobacterium tumefaciens LBA4404. S. lycopersicum cv. Micro-Tom (MT) and MT-Rg1 plants were transformed. In addition, seedlings were subjected to hormone treatments using a synthetic auxin (- naphthalene acetic acid) and cyclosporin A (cyclophilin inhibitor) treatments and it was found that the hormone treatment there were changes in development of lateral roots pattern, probably related to decreases in auxin signaling caused by reduction of LeCYP1 in MT-dgt plants while cyclosporin A treatments, there was a slight delay in flowering in cv. MT plants. Furthermore, assay with real-time PCR (RT-qPCR) were done for expression level analysis from LeCYP1 and ARP in order to functionally characterize these sequences in tomato plants.

Uso de aeronaves remotamente pilotadas (ARP) no planejamento florestal.

O uso da fotogrametria digital a partir de Aeronaves Remotamente Pilotadas (ARP/RPA) surge como uma alternativa viável para realização do planejamento florestal em distintas tipologias de nativa ou em sistemas de plantios florestais, além de ser uma importante ferramenta de monitoramento.

An epidemic of pain in an Australian radiology practice

This paper presents findings from a study of an organisationally mandated assimilation process of an enterprise-wide information system in a radiology practice in Australia. A number of interviews with radiologists, radiographers and administrative staff are used to explore the impact of institutional structures on the assimilation process. The case study develops an argument that culture within and outside the Australian Radiology Practice (ARP), social structures within the ARP and organisational-level management mandates have impacted on the assimilation process. The study develops a theoretical framework that integrates elements of social actor theory (Lamb & Kling, 2003) to provide a more fine-grained analysis concentrating on the relationship among the radiology practitioners, the technology (an enterprise-wide Health Information System) and a larger social milieu surrounding its use. This study offers several theoretical and practical implications for technology assimilation in the health and radiology industry regarding the important roles social interactions, individual self-perceptions, organisational mandates and policies can play in assimilating new ICTs.

Whole-genome sequencing identifies EN1 as a determinant of bone density and fracture

The extent to which low-frequency (minor allele frequency (MAF) between 1-5%) and rare (MAF

A Triggering Mechanism for Enhanced Star-Formation in Colliding Galaxies

We propose a physical mechanism to explain the origin of the intense burst of massive-star formation seen in colliding/merging, gas-rich, field spiral galaxies. We explicitly take account of the different parameters for the two main mass components, H-2 and H I, of the interstellar medium within a galaxy and follow their consequent different evolution during a collision between two galaxies. We also note that, in a typical spiral galaxy-like our galaxy, the Giant Molecular Clouds (GMCs) are in a near-virial equilibrium and form the current sites of massive-star formation, but have a low star formation rate. We show that this star formation rate is increased following a collision between galaxies. During a typical collision between two field spiral galaxies, the H I clouds from the two galaxies undergo collisions at a relative velocity of approximately 300 km s-1. However, the GMCs, with their smaller volume filling factor, do not collide. The collisions among the H I clouds from the two galaxies lead to the formation of a hot, ionized, high-pressure remnant gas. The over-pressure due to this hot gas causes a radiative shock compression of the outer layers of a preexisting GMC in the overlapping wedge region. This makes these layers gravitationally unstable, thus triggering a burst of massive-star formation in the initially barely stable GMCs.The resulting value of the typical IR luminosity from the young, massive stars from a pair of colliding galaxies is estimated to be approximately 2 x 10(11) L., in agreement with the observed values. In our model, the massive-star formation occurs in situ in the overlapping regions of a pair of colliding galaxies. We can thus explain the origin of enhanced star formation over an extended, central area approximately several kiloparsecs in size, as seen in typical colliding galaxies, and also the origin of starbursts in extranuclear regions of disk overlap as seen in Arp 299 (NGC 3690/IC 694) and in Arp 244 (NGC 4038/39). Whether the IR emission from the central region or that from the surrounding extranuclear galactic disk dominates depends on the geometry and the epoch of the collision and on the initial radial gas distribution in the two galaxies. In general, the central starburst would be stronger than that in the disks, due to the higher preexisting gas densities in the central region. The burst of star formation is expected to last over a galactic gas disk crossing time approximately 4 x 10(7) yr. We can also explain the simultaneous existence of nearly normal CO galaxy luminosities and shocked H-2 gas, as seen in colliding field galaxies.This is a minimal model, in that the only necessary condition for it to work is that there should be a sufficient overlap between the spatial gas distributions of the colliding galaxy pair.

Starbursts triggered by cloud compression in interacting galaxies

We propose a physical mechanism for the triggering of starbursts in interacting spiral galaxies by shock compression of the pre-existing disk giant molecular clouds (GMCs). We show that as a disk GMC tumbles into the central region of a galaxy following a galactic tidal encounter, it undergoes a radiative shock compression by the pre-existing high pressure of the central molecular intercloud medium. The shocked outer shell of a GMC becomes gravitationally unstable, which results in a burst of star formation in the initially stable GMC. In the case of colliding galaxies with physical overlap such as Arp 244, the cloud compression is shown to occur due to the hot, high-pressure remnant gas resulting from the collisions of atomic hydrogen gas clouds from the two galaxies. The resulting values of infrared luminosity agree with observations. The main mode of triggered star formation is via clusters of stars, thus we can naturally explain the formation of young, luminous star clusters observed in starburst galaxies.

Luminosity profiles of advanced mergers of galaxies using 2MASS data

A sample of 27 disturbed galaxies that show signs of interaction but have a single nucleus were selected from the Arp and the Arp-Madore catalogues. For these, the Ks band images from the Two Micron All Sky Survey (2MASS) are analysed to obtain their radial luminosity pro�les and other structural parameters. We �nd that in spite of their similar optical appearance, the sample galaxies vary in their dynamical properties, and fall into two distinct classes. The �rst class consists of galaxies which can be described by a single r1=4 law and the second class consists of galaxies that show an outer exponential disk. A few galaxies that have disturbed pro�les cannot be �t into either of the above classes. However, all the galaxies are similar in all other parameters such as the far-infrared colours, the molecular hydrogen content and the central velocity dispersion. Thus, the dynamical parameters of these sets seem to be determined by the ratio of the initial masses of the colliding galaxies. We propose that the galaxies in the �rst class result from a merger of spiral galaxies of equal masses whereas the second class of galaxies results from a merger of unequal mass galaxies. The few objects that do not fall into either category show a disturbed luminosity pro�le and a wandering centre, which is indicative of these being unrelaxed mergers. Of the 27 galaxies in our sample, 9 show elliptical-like pro�les and 13 show an outer exponential. Interestingly, Arp 224, the second oldest merger remnant of the Toomre sequence shows an exponential disk in the outer parts.

Análisis de riesgo de plagas de importancia fitosanitaria para Nicaragua en la importación de semilla de cebolla (Allium cepa L.) procecedente de Canadá

El presente Análisis de riesgo de Plagas (ARP) se realizó en el Centro Nacional de Diagnóstico Fitosanitario (CNDF) y Cuarentena del MAG-FOR en Managua, Nicaragua, e1 cual tuvo por objetivo evaluar el riesgo de introducción, establecimiento y dispersión de plagas de importancia fitosanitaria para Nicaragua en semilla de cebolla (Allium cepa L.) importada de Canadá, así como determinar las medidas adecuadas de protección fitosanitarias para evitar la introducción de las mismas a Nicaragua. De un listado inicial de 18 plagas, sólo 6 plagas son sujetas a evaluación y manejo del riesgo después de pasar por las tres etapas de evaluación de un ARP según la Norma Centroamericana del OIRSA, por considerarse que estas presentan capacidad biológica y de comportamiento, así como rangos óptimos de temperaturas que se asemejan a las condiciones de clima de las zonas productoras de Allium cepa L. del país. (Anexo1). El cuadro 1 contiene la lista de las plagas no sujetas a Evaluación del Riesgo Puccinia allii ( DC) Rudolphi y Urocistis Cepulae. Frost que causan la Roya y el carbón de la cebolla respectivamente son consideradas plagas específicas de los cultivos del género Allium P. allí es considerada plaga de bajo riesgo de introducción al país siendo la limitante para su establecimiento que su óptimo de temperatura ( 1 O" a 15" C), no se asemeja a las condiciones de temperatura de las zonas productoras del país( Anexo l ), mientras que U. cepulae es considerado como un hongo muy peligroso capaz de provocar pérdidas en la producción de hasta 80 por ciento tiene alta probabilidad de establecimiento v diseminación en las zonas productoras del país va que las condiciones de edafoclímaticas (16-22" C y pH 5-8) le favorecen( Anexo 1) Botryotinia squamosa. Viennot-Bourgín es un hongo que causa la pudrición blanda de la cebolla, se considera una plaga especifica de cultivos del género Allium con probabilidad alta de establecimiento v disemmac1ón en las zonas productoras de cebolla del país ya que el rango superior óptimo de temperatura (23" C) se asemeja a las condiciones de temperatura de las mismas (Anexo 11. Sclerotium cepivorum. Berkeley (1841 ). Es un hongo que causa la pudrición blanca de la cebolla y es considerado una plaga general de corto rango de hospedero quien además de atacar a cultivos del género Allium ataca también a lycopersicum esculentum (tomate) puede causar pérdidas en la producción de hasta un 70 por ciento (promedio) Y, con riesgo Alto de establecimiento en el país ya que temperaturas de 1 0"-20" C y baja humedad 40%. (pariona et. al) inclusive 30"- 5"C cuando hay humedad (Agrios 1985) y pH desde 1.4 a 8.8 le favorecen y las condiciones edafoclimáticas de las zonas productoras de cebolla del país se asemejan (Anexo ll). El nemátodo Ditylenchus dipsaci es un endoparásito destructor, y es considerado plaga general de cultivos del género Allium que ataca otros cultivos como cucurbitáceas. Zea mays (Maíz), Solanum tuberosum (Papa) y Nicotiana Tabacum (Tabaco). Es capaz de reducir la producción hasta un 75 por ciento (promedio) y la probabilidad de ingreso al país es media, a pesar de que su óptimo de temperatura (15º C) no se asemejan a la temperatura de las zonas productoras de cebolla del país. se considera de gran importancia sus características como: gran capacidad reproductiva es endoparásito y podemos encontrarlo dentro de cualquier parte de la planta inclusive dentro de la semilla. Aphelenchoides fragariae es un nematodo que tiene por hospedero secundario a Allium cepa. L puede ser capaz de ocasionar pérdidas en la producción de hasta 66.5% (promedio), es considerado plaga general de cultivos del género Allium con baja probabilidad de ingreso al país, va que su hospedero primario es la fresa y no se reportan daños en cebolla (no preferencia por Allium cepa L que es hospedero secundario) Todas estas plagas son consideradas de categoría A 1 1 para Nicaragua (no presentes en el país), lo que justifica plenamente la realización de este ARP a fin de tomar las medidas pertinentes que acompañen la importación de semilla y así evitar la introducción de nuevas plagas de difícil control.

Telekomunikazio-sare eta zerbitzuak: ariketa ebaitziak

Helburuak: Ariketa-bilduma honen helburu nagusia bikoitza da, 'Telekomunikazio-sare eta zerbitzuak' (2001eko ikasketa-planetako Telekomunikazio Ingeniaritza Teknikoetako 2. mailan irakasten zena) eta 'Telekomunikazio-sare eta zerbitzuak I' (1995eko ikasketa-planetako Telekomunikazio Ingeniaritzako 2. mailan irakasten zena) irakasgaietako ikasleentzat (hortaz, ikasketarako) zein irakasleentzat (hots, irakaskuntzarako) lagungarri izatea. Horregatik, teorian ikasitako kontzeptuen aplikazio praktikoa islatzen duten ariketak dira bilduma honetakoak. Aipatutako irakasgaien konplexutasuna dela eta, liburu hau, 'Telekomunikazio-sare eta zerbitzuak: Teoria' testu-liburuaren lagungarri gisa argitaratu dugu. Norentzat izan daiteke baliagarria: 2001eko ikasketa-planetako Telekomunikazio Ingeniaritza Teknikoetako 2. mailan irakasten zen 'Telekomunikazio-sare eta zerbitzuak' eta 1995eko ikasketa-planetako Telekomunikazio Ingeniaritzako 2. mailan irakasten zen 'Telekomunikazio-sare eta zerbitzuak I' irakasgaietako ikasleentzat zein irakasleentzat.

Lurking in ULIRGs: Molecular Gas in local Merging Galaxies

Mergers and interacting galaxies are pivotal to the evolution of galaxies in the universe. They are the sites of prodigious star formation and key to understanding the starburst processes: the physical and chemical properties and the dynamics of the molecular gas. ULIRGs or Ultraluminous Infrared Galaxies are a result of many of these mergers. They host extreme starbursts, AGNs, and mergers. They are the perfect laboratory to probe the connection between starbursts, black hole accretion and mergers and to further our understanding of star formation and merging.

NGC 6240 and Arp 220 can be considered the founding members of this very active class of objects. They are in different stages of merging and hence are excellent case studies to further our understanding about the merging process. We have imaged the dense star-forming regions of these galaxies at sub-arcsec resolution with CARMA C and B Configurations (2" and 0.5 - 0.8"). Multi-band imaging allows excitation analysis of HCN, HCO⁺, HNC, and CS along with CO transitions to constrain the properties of the gas. Our dataset is unique in that we have observed these lines at similar resolutions and high sensitivity which can be used to derive line ratios of faint high excitation lines.

Arp 220 has not had confirmed X-ray AGN detections for either nuclei. However, our observations indicate HCN/HNC ratios consistent with the chemistry of X-ray Dominated Regions (XDRs) -- a likely symptom of AGN. We calculated the molecular Hydrogen densities using each of the molecular species and conclude that assuming abundances of HNC and HCO⁺ similar to those in galactic sources are incorrect in the case of ULIRGs. The physical conditions in the dense molecular gas in ULIRGs alter these abundances. The derived H2 volume densities are ~ 5 x 10⁴ cm^-3 in both Arp 220 nuclei and ~ 10⁴ cm^-3 in NGC 6240.