Measurement of the galactic cosmic ray antiproton flux from 0.25 gev to 3.11 gev with the isotope matter antimatter experiment (imax)

The intensities and relative abundances of galactic cosmic ray protons and antiprotons have been measured with the Isotope Matter Antimatter Experiment (IMAX), a balloon-borne magnet spectrometer. The IMAX payload had a successful flight from Lynn Lake, Manitoba, Canada on July 16, 1992. Particles detected by IMAX were identified by mass and charge via the Cherenkov-Rigidity and TOP-Rigidity techniques, with measured rms mass resolution ≤0.2 amu for Z=1 particles.

Cosmic ray antiprotons are of interest because they can be produced by the interactions of high energy protons and heavier nuclei with the interstellar medium as well as by more exotic sources. Previous cosmic ray antiproton experiments have reported an excess of antiprotons over that expected solely from cosmic ray interactions.

Analysis of the flight data has yielded 124405 protons and 3 antiprotons in the energy range 0.19-0.97 GeV at the instrument, 140617 protons and 8 antiprotons in the energy range 0.97-2.58 GeV, and 22524 protons and 5 antiprotons in the energy range 2.58-3.08 GeV. These measurements are a statistical improvement over previous antiproton measurements, and they demonstrate improved separation of antiprotons from the more abundant fluxes of protons, electrons, and other cosmic ray species.

When these results are corrected for instrumental and atmospheric background and losses, the ratios at the top of the atmosphere are p/p=3.21(+3.49, -1.97)x10^(-5) in the energy range 0.25-1.00 GeV, p/p=5.38(+3.48, -2.45) x10^(-5) in the energy range 1.00-2.61 GeV, and p/p=2.05(+1.79, -1.15) x10^(-4) in the energy range 2.61-3.11 GeV. The corresponding antiproton intensities, also corrected to the top of the atmosphere, are 2.3(+2.5, -1.4) x10^(-2) (m^2 s sr GeV)^(-1), 2.1(+1.4, -1.0) x10^(-2) (m^2 s sr GeV)^(-1), and 4.3(+3.7, -2.4) x10^(-2) (m^2 s sr GeV)^(-1) for the same energy ranges.

The IMAX antiproton fluxes and antiproton/proton ratios are compared with recent Standard Leaky Box Model (SLBM) calculations of the cosmic ray antiproton abundance. According to this model, cosmic ray antiprotons are secondary cosmic rays arising solely from the interaction of high energy cosmic rays with the interstellar medium. The effects of solar modulation of protons and antiprotons are also calculated, showing that the antiproton/proton ratio can vary by as much as an order of magnitude over the solar cycle. When solar modulation is taken into account, the IMAX antiproton measurements are found to be consistent with the most recent calculations of the SLBM. No evidence is found in the IMAX data for excess antiprotons arising from the decay of galactic dark matter, which had been suggested as an interpretation of earlier measurements. Furthermore, the consistency of the current results with the SLBM calculations suggests that the mean antiproton lifetime is at least as large as the cosmic ray storage time in the galaxy (~10^7 yr, based on measurements of cosmic ray ^(10)Be). Recent measurements by two other experiments are consistent with this interpretation of the IMAX antiproton results.

I. Reactively sputtered Ti-Si-N thin films for diffusion barrier applications. II. Oxidation, diffusion and crystallization of an amorphous Zr_(60)Al_(15)Ni_(25) alloy.

Films of Ti-Si-N obtained by reactively sputtering a TiSi_2, a Ti_5Si_3, or a Ti_3Si target are either amorphous or nanocrystalline in structure. The atomic density of some films exceeds 10^23 at./cm^3. The room-temperature resistivity of the films increases with the Si and the N content. A thermal treatment in vacuum at 700 °C for 1 hour decreases the resistivity of the Ti-rich films deposited from the Ti_5Si_3 or the Ti_3Si target, but increases that of the Si-rich films deposited from the TiSi_2 target when the nitrogen content exceeds about 30 at. %.

Ti_(34)Si_(23)N_(43) deposited from the Ti_5Si_3 target is an excellent diffusion barrier between Si and Cu. This film is a mixture of nanocrystalline TiN and amorphous SiN_x. Resistivity measurement from 80 K to 1073 K reveals that this film is electrically semiconductor-like as-deposited, and that it becomes metal-like after an hour annealing at 1000 °C in vacuum. A film of about 100 nm thick, with a resistivity of 660 µΩcm, maintains the stability of Si n+p shallow junction diodes with a 400 nm Cu overlayer up to 850 °C upon 30 min vacuum annealing. When used between Si and Al, the maximum temperature of stability is 550 °C for 30 min. This film can be etched in a CF_4/O_2 plasma.

The amorphous ternary metallic alloy Zr_(60)Al_(15)Ni_(25) was oxidized in dry oxygen in the temperature range 310 °C to 410 °C. Rutherford backscattering and cross-sectional transmission electron microscopy studies suggest that during this treatment an amorphous layer of zirconium-aluminum-oxide is formed at the surface. Nickel is depleted from the oxide and enriched in the amorphous alloy below the oxide/alloy interface. The oxide layer thickness grows parabolically with the annealing duration, with a transport constant of 2.8x10^(-5) m^2/s x exp(-1.7 eV/kT). The oxidation rate is most likely controlled by the Ni diffusion in the amorphous alloy.

At later stages of the oxidation process, precipitates of nanocrystalline ZrO_2 appear in the oxide near the interface. Finally, two intermetallic phases nucleate and grow simultaneously in the alloy, one at the interface and one within the alloy.

Chilodonella cyprini (Moroff, 1902) [Translation from: Izv.gos.nauchno-issled.Inst.ozer.i rech.ryb.kh-va 49 25-28, 1959]

The ciliated protozoan Chilodonella cyprini is described. Chilodon parasitizes the body, gills and fins of fishes. The infusoria produce irritation of the integument and strengthened mucous secretion. The sparse knowledsge of the ecology of chilodon is summarised and some advice on the struggle against cholodoniasis in carp given.

The role of infusoria and bacteria as food for Cyclopoida in Rybinsk Reservoir [Translation from: Trudy Instituta Biologii Vnutrennykh Vodnany 22(25), 37-42, 1971]

Despite the fact that it is a long time sinc e the methods of collection and quantitative estimatio n of protozoa were worked out data on the abundance of these animals in freshwaters are not very numerous. Nevertheless, Infusoria and Rhizopoda at high densities are widespread in the water and sediments of lakes and reservoirs. In order to find ou t the importance of infusoria as a food source for cyclopoids we carried out experimental investigations using C14. For this three species of cyclopoids, widely distributed in open regions of Rybinsk reservoir were selected: Cyclops vicinus, Mesocyclops oithonoides and Kesocyclops leuckarti. The data presented give evidence that the species investigated are able as predators to consume infusorian plankton arid bacteria in the form of flocs or small clumps of detritus.

La estratigrafía analítica: 25 años de ensayo y aprendizaje en el análisis e interpretación del registro arqueológico

Homenaje a Georges Laplace, realizado en Vitoria-Gasteiz el 13,14 y 15 de noviembre de 2012. Edición a cargo de Aitor Calvo, Aitor Sánchez, Maite García-Rojas y Mónica Alonso-Eguíluz.

Major ions in 25 frequently sampled tarns in the English Lake District (1954-56, 1974-1976) [Dataset]

This dataset provides raw data of chemical analyses made during studies on seasonal variations of 25 frequently sampled tarns in Cumbria. Measurements of sodium, calcium, potassium, magnesium, pH, chloride ions, alkalinity, sulphite, strong acids and nitrate were taken between 1954 and 1956 and between 1974-1976.

Análise da eficácia do instrumento RECIPROC #25 em atingir o forame apical sem glide path

O presente estudo avaliou a eficáciado instrumento Reciproc#25 em atingir o forame de canais de molares inferiores sem um glide path manual prévio. Para isso, uma amostra geral de 300 molares inferiores foi radiografada e previamente selecionada quanto ao grau de curvatura segundo critério de Schneider sendo divididos em classes I e II. Após a aplicação dos critérios de inclusão e exclusão, uma amostragem total de 502 canais radiculares foi incluída para formar os grupos experimentais: 253 canais no grupo de molares inferiores classe I e 249 no grupo de molares classe II. Todos os canais foram instrumentados diretamente com a lima 25, sem nenhum glide path prévio, seguindo criteriosamente as diretrizes do fabricante. Os dados foram descritos como a frequência da distribuição do número de canais (%) nos quais foi possível chegar ao forame apical sem a necessidade de glide path, assim como o número de fraturas em cada grupo. Os resultados compilados dos 2 grupos experimentais mostraram que em 93,4% do total dos canais instrumentados, o instrumento R25 foi capaz de ir até o forame apical sem a necessidade de glide path. Em 6,4% do total dos canais, o instrumento R25 não chegou até o forame apical e em somente 0,2% dos casos ocorreu fratura da lima (um caso no grupo classe I, enquanto no grupo classe II não houve nenhuma ocorrência de fratura). O teste Qui-quadrado foi realizado para verificar se uma determinada classe de canais encontra-se mais associada ou não a necessidade de glide path quando o sistema Reciproc é usado. No grupo de molares classe II houve maior número de canais (23) que o instrumento R25 não foi capaz de ir até o forame apical do que no grupo de molares classe I (9), sendo essa diferença estatisticamente significante (Qui-quadrado, p=0,020, X2=5,452). Dentro das condições experimentais do presente estudo, pode-se concluir então quea lima R25 mostrou uma alta eficácia em instrumentar toda a extensão dos canais de molares inferiores classe I e II sem a necessidade de glide path prévio. Além disso, o sistema de instrumentação proposto mostrou-se altamente seguro quanto ao índice de fratura.

Campagnes Chalci, Chalci 84-01 (du 17 au 25-01-84) et Chalci 84-02 (du 03 au 11-07-84): resultats des chalutages

This publication gives the results of bottom trawlings made during the cruises CHALCI 84-01 and CHALCI 84-02 by the oceanographic research vessel "Andre NIZERY" sur le plateau continental ivoirien.

Espaço e lugar sagrado na percepção das membros da Assembleia de Deus Jardim 25 de Agosto - ADJ25A: um estudo de geografia da religião em Duque de Caxias - RJ - 2013

Esta dissertação lança o olhar geográfico sobre a igreja Assembléia de Deus, estuda sua gênese, difusão e sua espacialidade no Brasil, através da proposta de estudo de geografia e religião, tendo como base as proposições fé, espaço e tempo: difusão e área de abrangência, e espaço e lugar sagrado: vivência, percepção e simbolismo. Para tanto, o estudo de caso na escala local da Igreja Assembléia de Deus Jardim 25 de Agosto - ADJ25A, no município de Duque de Caxias, no Estado do Rio de Janeiro, torna-se imprescindível. Este estudo privilegia a difusão da mensagem pentecostal e a organização espacial de seus seguidores no país e se propõe a refletir sobre a geograficidade das práticas cotidianas religiosas individuais e de grupo dos membros da ADJ25A. A partir da observação empírica, da aplicação de um questionário individual e da análise dos resultados obtidos, é possível inferir sobre as práticas religiosas do homem religioso assembleiano no seu construir, no seu perceber e na sua vivência no lugar sagrado.