Ratios of Elastic Scattering of Pions from 3H and 3He

We have measured the elastic-scattering ratios of normalized yields for charged pions from 3H and 3He in the backward hemisphere. At 180 MeV, we completed the angular distribution begun with our earlier measurements, adding six data points in the angular range of 119 deg to 169 deg in the pi-nucleus center of mass. We also measured an excitation function with data points at 142, 180, 220, and 256 MeV incident pion energy at the largest achievable angle for each energy between 160 deg and 170 deg in the pi-nucleus center of mass. This excitation function corresponds to the energies of our forward-hemisphere studies. The data, taken as a whole, show an apparent role reversal of the two charge-symmetric ratios r1 and r2 in the backward hemisphere. Also, for data > 100 deg we observe a strong dependence on the four-momentum transfer squared (-t) for all of the ratios regardless of pion energy or scattering angle, and we find that the superratio R data match very well with calculations based on the forward-hemisphere data that predicts the value of the difference between the even-nucleon radii of 3H and 3He. Comparisons are also made with recent calculations incorporating different wave functions and double scattering models.Comment: RevTex 8pages, 12 figure file

Psychology and aggression

Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/68264/2/10.1177_002200275900300301.pd

A single fast radio burst localized to a massive galaxy at cosmological distance

Fast radio bursts (FRBs) are brief radio emissions from distant astronomical sources. Some are known to repeat, but most are single bursts. Nonrepeating FRB observations have had insufficient positional accuracy to localize them to an individual host galaxy. We report the interferometric localization of the single-pulse FRB 180924 to a position 4 kiloparsecs from the center of a luminous galaxy at redshift 0.3214. The burst has not been observed to repeat. The properties of the burst and its host are markedly different from those of the only other accurately localized FRB source. The integrated electron column density along the line of sight closely matches models of the intergalactic medium, indicating that some FRBs are clean probes of the baryonic component of the cosmic web

Measuring ionospheric movements using totally reflected radio waves

It is shown that for radio waves of a particular frequency reflected totally from the ionosphere the effect of refraction as well as reflection can be simulated by an effective reflecting surface. This mirrorlike surface will give the correct angle of arrival and Doppler shift for all radars operating at this frequency. It is theoretically possible for the effective reflecting surface to be folded back on itself, but this is unlikely except for F-region echoes refracted by sporadic E-clouds. If the surface is not folded and exists everywhere, it is always possible to describe its motion and change in terms of wave undulations. Experimental data for F-region echoes show that these wave undulations are very dispersive. However, the matching between the best fitting model and the experimental data is worse than expected for reasons we do not understand

Definição da dimensão do indivíduo solo e determinação do número de amostras simples necessário à sua representação Determination of a soil individual and the number of single samples required to represent it

Uma população é composta por indivíduos, e a amostragem correta dos indivíduos estima adequadamente as características da população. Porém, para avaliar a fertilidade do solo, quem seria o indivíduo solo (unidades de amostra) e qual sua dimensão? Com o objetivo de definir a dimensão do indivíduo solo componente de determinada população, sob plantio direto (PD) ou sob plantio convencional antes (PCAA) ou depois da aração (PCDA), visando avaliar a fertilidade do solo e desenvolver um método de amostragem de solos, determinando o número de amostras simples necessário à formação de uma amostra composta que caracterize o indivíduo solo (unidade de amostra), foram coletadas amostras simples de solo (5,4 cm de diâmetro x 10 cm de profundidade) sobre as semidiagonais de cinco hexágonos delimitados sobre cada uma das áreas selecionadas para amostragem (PD, PCAA e PCDA). Os hexágonos de amostragem apresentavam 2 m de lado e, em cada uma das seis semidiagonais dos mesmos, foram coletadas dez amostras simples de solo (55 por hexágono) nas seguintes distâncias, a partir de uma amostra simples central, medidas até o centro do orifício de coleta: 12,5; 25,0; 37,5; 50,0; 75,0; 100,0; 112,5; 150,0 e 200,0 cm, sendo a amostra simples central comum às seis semidiagonais. Foram determinados o pH (H2O), os teores de P e K disponíveis e de Ca2+ e Mg2+, H + Al, P-rem e a matéria orgânica. As amostras simples foram agrupadas sucessivamente a partir do centro do hexágono, formando nove unidades de amostra: A (até 18,75), B (até 31,25), C (até 43,75), D (até 56,25), E (até 81,25), F (até 106,25), G (até 118,75), H (até 156,25) e I (até 206,25 cm). Foi realizada análise de regressão das médias e dos desvios-padrão das características avaliadas, considerando possíveis dimensões da unidade de amostra de solo. A partir dos resultados obtidos, pôde-se concluir que: para a caracterização do indivíduo solo (unidade de amostra), devem-se coletar 25 amostras simples, necessárias à formação de uma amostra composta representativa, num hexágono de 68,75 cm de lado e área de 1,228 m².<br>A population consists of individuals and a correct sampling of the individuals estimates population characteristics adequately. However, to evaluate soil fertility, what would be the soil individual (sample units), and of what size? The objective of this study was to determine the dimension of the individual soil component of a particular population, in three sampling areas: under no-till or under conventional tillage before or after plowing, and to evaluate soil fertility and develop a soil sampling method, determining the number of single samples required to form a composite sample that would characterize a soil individual (sample unit). Single soil samples (5.4 cm diameter x 10 cm deep) were collected along the semi-diagonals of five hexagons outlined on the selected sampling areas. The sampling hexagons had 2 m long sides and from each of the six semi-diagonals, 10 single soil samples (55 per hexagon) were collected at the distances 12.5; 25.0; 37.5; 50.0; 75.0; 100.0; 112.5; 150.0 and 200.0 cm, measured from a simple central sample, to the center of the sampling spot. The single central sample was the same for the six semi-diagonals. Soil pH (H2O), available P and K, Ca2+ and Mg2+ concentrations and H + Al, equilibrium-P and organic matter were determined. The single samples were grouped successively from the hexagon center and formed nine sampling units: A (up to 18.75), B (up to 31.25), C (up to 43.75), D (up to 56.25), E (up to 81.25), F (up to 106.25), G (up to 118.75), H (up to 156.25) and I (up to 206.25 cm). Regression analysis of the means and standard deviations of the evaluated characteristics was performed considering the possible dimensions of the soil sample unit. Based on the results, the conclusion was drawn that 25 simple samples must be collected to characterize a soil individual (sample unit), for the formation of a representative composite sample in a 68.75 cm-sided hexagon with an area of 1.228 m²