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On the Energy Dependence of Galactic Cosmic Ray Anisotropies in the Very Local Interstellar Medium
We report on the energy dependence of Galactic cosmic rays (GCRs) in the very local interstellar medium (VLISM) as measured by the Low Energy Charged Particle (LECP) instrument on the Voyager 1 spacecraft. The LECP instrument includes a dual-ended solid-state detector particle telescope mechanically scanning through 360° across eight equally spaced angular sectors. As reported previously, LECP measurements showed a dramatic increase in GCR intensities for all sectors of the ≥211 MeV count rate (CH31) at the Voyager 1 heliopause (HP) crossing in 2012; however, since then the count rate data have demonstrated systematic episodes of intensity decrease for particles around 90° pitch angle. To shed light on the energy dependence of these GCR anisotropies over a wide range of energies, we use Voyager 1 LECP count rate and pulse height analyzer (PHA) data from ≥211 MeV channel together with lower-energy LECP channels. Our analysis shows that, while GCR anisotropies are present over a wide range of energies, there is a decreasing trend in the amplitude of second-order anisotropy with increasing energy during anisotropy episodes. A stronger pitch angle scattering at higher velocities is argued as a potential cause for this energy dependence. A possible cause for this velocity dependence arising from weak rigidity dependence of the scattering mean free path and resulting velocity-dominated scattering rate is discussed. This interpretation is consistent with a recently reported lack of corresponding GCR electron anisotropies. © 2022. The Author(s). Published by the American Astronomical Society.Open access journalThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at [email protected]
Genetic parameters estimates for gestation length in beef cattle Componentes de variância para o perÃodo de gestação em bovinos de corte
Variance components were estimated for gestation length fitting the additive direct effect of calf, maternal genetic effect and sire effect as random effects. The statistical models also included the fixed effects of contemporary group, that included the date of breeding (AI), date of birth, and sex of calf, and the covariate age of dam at calving (linear and quadratic). Two different models were used, model 1 considering GL as a trait of the calf, and model 2 considering GL as a trait of the dam. The means of gestation length for the purebred animals were 294.55 days (males) and 293.34 days (females), while for the crossbred animals they were 292.49 days (males) and 292.55 days (females). Variance components for the purebred animals, fitting model 1, were 14.47, 72.78 and 57.31, for the additive genetic (sigma2a), total phenotypic (sigma2p) and residual (sigma2e) effects, respectively, with a heritability estimate of 0.21. For the crossbred animals, variance components for sigma2a, sigma2p, sigma2e were 90.40, 127.35 and 36.95, respectively, with a heritability of 0.71. Fitting model 2, the estimated variance components for the purebred animals were 12.78, 5.01, 74.84 and 57.05 for sigma2a , sire of calf (sigma ²asire), sigma2p, and sigma2e , respectively. The sire effect accounted for 0.07 (c²) of the phenotypic variance and the coefficient of repeatability was 0.17. For the crossbred animals, the variance components were 22.11 (sigma2a ), 22.97 (sigma ²asire ), 127.70 (sigma2p) and 82.61 (sigma2e), while c² was 0.18 and repeatability was 0.17. Therefore, regarding selection of beef cattle, it is suggested to use the heritability estimate obtained by model 1, where GL is considered as a trait of the calf.<br>Estimaram-se os componentes de variância do perÃodo de gestação (PG) considerando-se o efeito direto do bezerro e os efeitos direto da vaca e aleatório do touro (pai do bezerro). Além dos efeitos aleatórios, os modelos estatÃsticos incluÃram os efeitos fixos de grupo de contemporâneos, composto pela data juliana de inseminação, ano de nascimento e sexo do bezerro, e a idade da vaca ao parto (covariável linear e quadrática). As médias de PG para os animais da raça Nelore foram 294,55 dias (machos) e 293,34 dias (fêmeas) e para os animais cruzados, 292,49 dias (machos) e 292,55 dias (fêmeas). Os componentes de variância observados no Nelore, utilizando-se o modelo 1, que considerou o PG como caracterÃstica do bezerro, foram 14,47; 72,78 e 57,31 para os componentes aditivo direto (sigma2a), fenotÃpico total (sigma2p) e residual (sigma2e), respectivamente, e a herdabilidade foi 0,21. Para os animais cruzados, pelo mesmo modelo, os componentes de variância foram 90,40 (sigma2a), 127,35 (sigma2p ) e 36,95 (sigma2e), e a herdabilidade, 0,71. Os componentes de variância do PG do Nelore sob o modelo 2, que considerou o PG como caracterÃstica da vaca, foram 12,78; 5,01; 74,84 e 57,05, para sigma2a; sigma2pb (variância do pai do bezerro); sigma2p e sigma2e, respectivamente. A fração fenotÃpica atribuÃda ao touro (c²) foi 0,07 e a repetibilidade, 0,17. Para os cruzados, estimaram-se 22,11; 22,97; 127,70 e 82,61 para sigma2a; sigma2pb; sigma2p e sigma2e, respectivamente, enquanto o c² foi 0,18 e o coeficiente de repetibilidade, 0,17. Sugere-se, para fins de seleção, que o coeficiente de herdabilidade utilizado seja o obtido na análise em que PG foi considerado como caracterÃstica do bezerro