Argonauta Video Database: Spectography experiment. Scene 3 (Left camera)

Scenes for Spectrography experiment Scenes were recorded following the tasks involved in spectrography experiments, which are carried out in front of "J9" output radiadion channel, the latter in open condition. These tasks may be executed by one or two persons. One person can do the tasks, but requiring him to crouch in front of "J9" to adjust the angular position the experimental appartus (a crystal to bend the neutron radiation to the spectograph), and then to get up to verify data in a computer aside; these movements are repeated until achieving the right operational conditions. Two people may aid one another in such a way one remais crouched while the other remains still in front of the computer. They may also interchange tasks so as to divide received doses. Up to now, there are available two scenes with one person and one scene with two persons. These scenes are described in the sequel: - Scene 3: Comprises the scene with two persons performing spectography experiment. Video file labels: "20140327182906_IPCAM": recorded by the left camera.

D��tection des ��v��nements de "Minimum Bias" et neutrons avec les d��tecteurs ATLAS-MPX par simulations

Un r��seau de seize d��tecteurs ATLAS-MPX a ��t�� mis en op��ration dans le d��tecteur ATLAS au LHC du CERN. Les d��tecteurs ATLAS-MPX sont sensibles au champ mixte de radiation de photons et d�����lectrons dans la caverne d���ATLAS et sont recouverts de convertisseurs de fluorure de lithium et de poly��thyl��ne pour augmenter l���efficacit�� de d��tection des neutrons thermiques et des neutrons rapides respectivement. Les collisions �� haute ��nergie sont domin��es par des interactions partoniques avec petit moment transverse pT , associ��s �� des ��v��nements de ���minimum bias���. Dans notre cas la collision proton-proton se produit avec une ��nergie de 7 TeV dans le centre de masse avec une luminosit�� de 10�����cm�����s����� telle que fix��e dans les simulations. On utilise la simulation des ��v��nements de "minimum bias" g��n��r��s par PYTHIA en utilisant le cadre Athena qui fait une simulation GEANT4 compl��te du d��tecteur ATLAS pour mesurer le nombre de photons, d�����lectrons, des muons qui peuvent atteindre les d��tecteurs ATLASMPX dont les positions de chaque d��tecteur sont incluses dans les algorithmes d���Athena. Nous mesurons les flux de neutrons thermiques et rapides, g��n��r��s par GCALOR, dans les r��gions de fluorure de lithium et de poly��thyl��ne respectivement. Les r��sultats des ��v��nements de ���minimum bias��� et les flux de neutrons thermiques et rapides obtenus des simulations sont compar��s aux mesures r��elles des d��tecteurs ATLAS-MPX.

A finite element-spherical harmonics model for radiative transfer in inhomogeneous clouds. Part II. some applications

EVENT has been used to examine the effects of 3D cloud structure, distribution, and inhomogeneity on the scattering of visible solar radiation and the resulting 3D radiation field. Large eddy simulation and aircraft measurements are used to create realistic cloud fields which are continuous or broken with smooth or uneven tops. The values, patterns and variance in the resulting downwelling and upwelling radiation from incident visible solar radiation at different angles are then examined and compared to measurements. The results from EVENT confirm that 3D cloud structure is important in determining the visible radiation field, and that these results are strongly influenced by the solar zenith angle. The results match those from other models using visible solar radiation, and are supported by aircraft measurements of visible radiation, providing confidence in the new model.

Global and diffuse solar irradiances in urban and rural areas in southeast Brazil

The seasonal evolution of daily and hourly values of global and diffuse solar radiation at the surface are compared for the cities of Sao Paulo and Botucatu, both located in Southeast Brazil and representative of urban and rural areas, respectively. The comparisons are based on measurements of global and diffuse solar irradiance carried out at the surface during a six year simultaneous period in these two cities. Despite the similar latitude and altitude, the seasonal evolution of daily values indicate that Sao Paulo receives, during clear sky days, 7.8% less global irradiance in August and 5.1% less in June than Botucatu. On the other hand, Sao Paulo receives, during clear sky days, 3.6% more diffuse irradiance in August and 15.6% more in June than Botucatu. The seasonal variation of the diurnal cycle confirms these differences and indicates that they are more pronounced during the afternoon. The regional differences are related to the distance from the Atlantic Ocean, systematic penetration of the sea breeze and daytime evolution of the particulate matter in Sao Paulo. An important mechanism controlling the spatial distribution of solar radiation, on a regional scale, is the sea breeze penetration in Sao Paulo, bringing moisture and maritime aerosol that in turn further increases the solar radiation scattering due to pollution and further reduces the intensity of the direct component of solar radiation at the surface. Surprisingly, under clear sky conditions the atmospheric attenuation of solar radiation in Botucatu during winter - the biomass burning period due to the sugar cane harvest - is equivalent to that at Sao Paulo City, indicating that the contamination during sugar cane harvest in Southeast Brazil has a large impact in the solar radiation field at the surface.

An automatic correction method for the heel effect in digitized mammography images

The most significant radiation field nonuniformity is the well-known Heel effect. This nonuniform beam effect has a negative influence on the results of computer-aided diagnosis of mammograms, which is frequently used for early cancer detection. This paper presents a method to correct all pixels in the mammography image according to the excess or lack on radiation to which these have been submitted as a result of the this effect. The current simulation method calculates the intensities at all points of the image plane. In the simulated image, the percentage of radiation received by all the points takes the center of the field as reference. In the digitized mammography, the percentages of the optical density of all the pixels of the analyzed image are also calculated. The Heel effect causes a Gaussian distribution around the anode-cathode axis and a logarithmic distribution parallel to this axis. Those characteristic distributions are used to determine the center of the radiation field as well as the cathode-anode axis, allowing for the automatic determination of the correlation between these two sets of data. The measurements obtained with our proposed method differs on average by 2.49 mm in the direction perpendicular to the anode-cathode axis and 2.02 mm parallel to the anode-cathode axis of commercial equipment. The method eliminates around 94% of the Heel effect in the radiological image and the objects will reflect their x-ray absorption. To evaluate this method, experimental data was taken from known objects, but could also be done with clinical and digital images.

Genesis of quantum nonlocality

We revisit the problem of an otherwise classical particle immersed in the zero-point radiation field, with the purpose of tracing the origin of the nonlocality characteristic of Schrodinger`s equation. The Fokker-Planck-type equation in the particles phase-space leads to an infinite hierarchy of equations in configuration space. In the radiationless limit the first two equations decouple from the rest. The first is the continuity equation: the second one, for the particle flux, contains a nonlocal term due to the momentum fluctuations impressed by the field. These equations are shown to lead to Schrodinger`s equation. Nonlocality (obtained here for the one-particle system) appears thus as a property of the description, not of Nature. (C) 2011 Elsevier B.V. All rights reserved.

An exactly soluble multiatom-multiphoton coupling model

Funda����o de Amparo �� Pesquisa do Estado de S��o Paulo (FAPESP)

Response of L-alanine and 2-methylalanine minidosimeters for K-Band (24 GHz) EPR dosimetry

Minidosimeters of L-alanine and 2-methylalanine (2MA) were prepared and tested as potential candidates for small radiation field dosimetry. To quantify the free radicals created by radiation a K-Band (24 GHz) EPR spectrometer was used. X-rays provided by a 6 MV clinical linear accelerator were used to irradiate the minidosimeters in the dose range of 0.5-30 Gy. The dose-response curves for both radiation sensitive materials displayed a good linear behavior in the dose range indicated with 2MA being more radiation sensitive than L-alanine. Moreover, 2MA showed a smaller LLD (lower limit detection) value. The proposed system minidosimeter/K-Band spectrometer was able to detect 10 Gy EPR spectra with good signal-to-noise ratio (S/N). The overall uncertainty indicates that this system shows a good performance for the detection of dose values of 20 Gy and above, which are dose values typically used in radiosurgery treatments. (c) 2007 Elsevier B.V. All rights reserved.

Study of the effects of exposure to ionizing irradiation on the materials used for dental restoration

A quantitative study was made about the effects caused by ionizing irradiation on materials used for dental restoration (amalgams, compound resins and compomere), aiming to alleviate in bearers of head and neck cancer, the possible harmful effects of radiotherapy perceived when the repaired teething is within the radiation field. Research also encourages further studies for new alternative materials to be used in dental repair of patients submitted to radiotherapy for head and neck cancer. Test samples were submitted to a gamma radiation beam coming from a cobalt-therapy source and analyzed according to the X-ray fluorescence technique, comparing the chemical composition of the samples before and after irradiation. Radiation detectors such as an ionization chamber and a Geiger-Muller were used to measure the rate of residual dose. Gamma spectrometry with Nal detectors was also performed on the same samples. Results showed that there was no significant change in the chemical composition and that at post-irradiation, samples did not exhibit radiation emission, that is to say they had not become radioactive.

Global and diffuse solar irradiances in urban and rural areas in southeast Brazil

The seasonal evolution of daily and hourly values of global and diffuse solar radiation at the surface are compared for the cities of S��o Paulo and Botucatu, both located in Southeast Brazil and representative of urban and rural areas, respectively. The comparisons are based on measurements of global and diffuse solar irradiance carried out at the surface during a six year simultaneous period in these two cities. Despite the similar latitude and altitude, the seasonal evolution of daily values indicate that S��o Paulo receives, during clear sky days, 7.8% less global irradiance in August and 5.1% less in June than Botucatu. on the other hand, S��o Paulo receives, during clear sky days, 3.6% more diffuse irradiance in August and 15.6% more in June than Botucatu. The seasonal variation of the diurnal cycle confirms these differences and indicates that they are more pronounced during the afternoon. The regional differences are related to the distance from the Atlantic Ocean, systematic penetration of the sea breeze and daytime evolution of the particulate matter in S��o Paulo. An important mechanism controlling the spatial distribution of solar radiation, on a regional scale, is the sea breeze penetration in S��o Paulo, bringing moisture and maritime aerosol that in turn further increases the solar radiation scattering due to pollution and further reduces the intensity of the direct component of solar radiation at the surface. Surprisingly, under clear sky conditions the atmospheric attenuation of solar radiation in Botucatu during winter - the biomass burning period due to the sugar cane harvest - is equivalent to that at S��o Paulo City, indicating that the contamination during sugar cane harvest in Southeast Brazil has a large impact in the solar radiation field at the surface.

Deviation from the sech2 superradiant emission law in a two-level atomic system

The atomic superradiant emission is treated in the single-particle mean-field approximation. A single-particle Hamiltonian, which represents a dressed two-level atom in a radiation field, can be obtained and it is verified that it describes the transient regime of the emission process. While the line-shape emission for a bare atom follows the sech2 law, for the dressed atom the line shape deviates appreciably from this law and it is verified that the deviation depends crucially on the ratio of the dynamic frequency shift to the transition frequency. This kind of deviation is observed in experimental results. �� 1990 The American Physical Society.

Avalia����o da dose de radia����o absorvida em exames radiol��gicos durante o planejamento radioter��pico

P��s-gradua����o em Pesquisa e Desenvolvimento (Biotecnologia M��dica) - FMB

Observational effects of stellar rotation on Be stars' disks

Be stars are known to be fast rotators. At high rotation rates a profound modification of the radiation field reaching the circumstellar environment is expected. The origin of this modification is the decrease of the effective gravity on stellar surface leading to the stellar geometrical flattening and the gravity darkening effect predicted by Von Zeipel. Making use of the radiative transfer code HDUST we discuss the consequences of such stellar rotation on the structure of Be star disks based on the Viscous Decretion Disk model. Observational predictions are also made, as SED, IR-excess and Hydrogen line profiles. The modified illumination of the circumstellar disk generates significant changes in these quantities. Ascertaining these changes is useful to set some of the fundamental parameters of the Be system and to unveil the role of stellar rotation over the stellar evolution.

Entwicklung und Evaluierung einer Modellhierarchie zur Simulation der aktinischen Strahlung in aerosolbelasteter und bew��lkter Atmosph��re

Das Verstaendnis der in der Atmosphaere stattfindendenOzonproduktions- und Ozonabbaumechanismen ist eines derwichtigsten Ziele der aktuellen Umweltforschung. Da Ozon inder Atmosphaere ausschliesslich durch photochemischeProzesse gebildet wird, ist die Kenntnis der aktinischenStrahlung eine grundlegende Voraussetzung fuer die Prognosevon Ozonkonzentrationen. Die vorliegende Arbeit befasst sichdaher mit der Modellierung der aktinischen Strahlung alsBasis zur Untersuchung photochemischer Prozesse. Dazu wurde eine Modellhierarchie entwickelt, welcheausgehend von der Berechnung der optischen Eigenschaften deratmosphaerischen Extingenten den Strahlungstransport in derAtmosphaere bestimmt. Dazu wurden verschiedeneStrahlungstransportmodelle verwendet, welche sich durch dieLoesungsmethode der Strahlungstransportgleichung und dieAnzahl der raeumlichen Dimensionen unterscheiden. Zur Ueberpruefung der entwickelten Modellhierarchie und zurUntersuchung des Einflusses der verschiedenen Extingentenauf das atmosphaerische Strahlungsfeld wurden zahlreicheSensitivitaetsstudien durchgefuehrt. Dabei zeigte sich, dasssich der Einfluss von Ozon fast ausschliesslich auf denAnteil der Strahlung mit Wellenlaengen kleiner 340 nmauswirkt. Bei der Untersuchung des Einflusses vonAerosolpartikeln und Wolkentropfen auf die aktinischeStrahlung wurde festgestellt, dass die chemischeZusammensetzung, das Vertikalprofil, die Groesse und dieGroessenverteilung der Partikel einen entscheidendenEinfluss nehmen. Eine Evaluierung des 1-dimensionalenStrahlungstransportmodells an Hand von Vergleichen mit denErgebnissen anderen Strahlungstransportmodelle undverschiedenen Messungen ergab, dass die entwickelteModellhierarchie sehr zuverlaessige Resultate liefert. Die Effekte durchbrochener Bewoelkung konnten mit einer2-dimensionalen Simulation untersucht werden. DieUntersuchungen zeigen, dass die haeufig durchgefuehrteapproximative Betrachtung von partieller Bewoelkung mit1-dimensionalen Strahlungstransportmodellen im Vergleich zuden Ergebnissen der 2-dimensionalen Simulation grosse Fehlerverursacht, da die Effekte an den seitlichen Wolkenraendernvon den 1-dimensionalen Strahlungstransportmodellen nichtberuecksichtigt werden koennen.

Galactic fountain flows in high-resolution hydrodynamical simulations of galaxy disks

Feedback from the most massive components of a young stellar cluster deeply affects the surrounding ISM driving an expanding over-pressured hot gas cavity in it. In spiral galaxies these structures may have sufficient energy to break the disk and eject large amount of material into the halo. The cycling of this gas, which eventually will fall back onto the disk, is known as galactic fountains. We aim at better understanding the dynamics of such fountain flow in a Galactic context, frame the problem in a more dynamic environment possibly learning about its connection and regulation to the local driving mechanism and understand its role as a metal diffusion channel. The interaction of the fountain with a hot corona is hereby analyzed, trying to understand the properties and evolution of the extraplanar material. We perform high resolution hydrodynamical simulations with the moving-mesh code AREPO to model the multi-phase ISM of a Milky Way type galaxy. A non-equilibrium chemical network is included to self consistently follow the evolution of the main coolants of the ISM. Spiral arm perturbations in the potential are considered so that large molecular gas structures are able to dynamically form here, self shielded from the interstellar radiation field. We model the effect of SN feedback from a new-born stellar cluster inside such a giant molecular cloud, as the driving force of the fountain. Passive Lagrangian tracer particles are used in conjunction to the SN energy deposition to model and study diffusion of freshly synthesized metals. We find that both interactions with hot coronal gas and local ISM properties and motions are equally important in shaping the fountain. We notice a bimodal morphology where most of the ejected gas is in a cold $10^4$ K clumpy state while the majority of the affected volume is occupied by a hot diffuse medium. While only about 20\% of the produced metals stay local, most of them quickly diffuse through this hot regime to great scales.