Cost of energy and mutual shadows in a two-axis tracking PV system

The performance improvement obtained from the use of trackers in a PV system cannot be separated from the higher requirement of land due to the mutual shadows between generators. Thus, the optimal choice of distances between trackers is a compromise between productivity and land use to minimize the cost of the energy produced by the PV system during its lifetime. This paper develops a method for the estimation and optimization of the cost of energy function. It is built upon a set of equations to model the mutual shadows geometry and a procedure for the optimal choice of the wire cross-section. Several examples illustrate the use of the method with a particular PV system under different conditions of land and equipment costs. This method is implemented using free software available as supplementary material

On the algorithmic construction of classifying spaces and the isomorphism problem for biautomatic groups

We show that the isomorphism problem is solvable in the class of central extensions of word-hyperbolic groups, and that the isomorphism problem for biautomatic groups reduces to that for biautomatic groups with finite centre. We describe an algorithm that, given an arbitrary finite presentation of an automatic group $\Gamma$, will construct explicit finite models for the skeleta of $K(\Gamma,1)$ and hence compute the integral homology and cohomology of $\Gamma$.Comment: 21 pages, 4 figure

Relación entre la composición química corporal, la fertilidad y la prolificidad en conejas primíparas.

En este trabajo se ha estudiado el efecto de la composición química corporal, estimada mediante el método de impedancia bioeléctrica (BIA) en la primera y segunda inseminación artificial (IA), sobre la fertilidad y la prolificidad de conejas primíparas. Se utilizaron los datos de 137 conejas procedentes de dos granjas que utilizaban dos genéticas distintas (UPV e Hyplus) y tres ritmos reproductivos (R4: inseminación a los 4 días tras el parto y destete a los 28 días, R11: inseminación a los 11 días postparto y destete a 35 días y R14: inseminación a los 14 días tras el parto y destete a los 42 días). La fertilidad media observada en el segundo parto fue de un 56,2% y el porcentaje de nacidos vivos, sobre los nacidos totales, fue de un 87,5%, no encontrándose diferencias entre los ritmos utilizados. El aumento de la proporción de proteína corporal, grasa y energía en la primera IA tuvieron un efecto positivo (P=0,007; P=0,03 y P<0,001, respectivamente) sobre la fertilidad del segundo parto. Igualmente, un mayor contenido en grasa (P<0,001) y energía (P<0,001) en la segunda IA también incrementaron la fertilidad del segundo parto. El incremento del ratio proteína/energía corporal de las conejas, determinado en las dos IA, tuvo un efecto negativo sobre la fertilidad en el segundo parto (P<0,001), observándose mejores resultados en conejas con 12 g proteína/MJ respecto a otras con valores superiores. El porcentaje de nacidos vivos (P<0,001), sobre los nacidos totales, aumentó con la proporción de proteína de las conejas en el momento de la segunda IA, pero esta última no tuvo efecto sobre la fertilidad. This study evaluated the effect of chemical body composition at first and second artificial inseminations (AI), determined by bioelectric impedance technique (BIA), on fertility and prolificacy of primiparous rabbit does. Data of 137 does from two farms using two different genetics (UPV and Hyplus) and three breeding systems were analyzed. Fertility was 56.2 % and the percentage of kits born alive over total born was 87.5 %. Breeding system had no effect on fertility or the percentage of kits born alive. Higher body protein, fat and energy of the rabbit doe at first artificial insemination (AI) increased the fertility in the second parity (P=0.007, P=0.03 and P<0.001 respectively). Fat and energy content of the doe at the second AI affected positively fertility in the second parity (P<0.001 and P<0.001 respectively), while protein influenced positively only prolificacy (P<0.001). The increase of the ratio protein/energy in both AI moments had a negative influence on fertility in the second parity (P<0.001), rabbit does with 12 g protein/MJ showed a higher fertility than those with higher value

A Nexafs Study of Nitric Oxide Layers Adsorbed from a nitrite Solution onto a Pt(111) Surface

NO molecules adsorbed on a Pt(111) surface from dipping in an acidic nitrite solution are studied by near edge X-ray absorption fine structure spectroscopy (NEXAFS), X-ray photoelectron spectroscopy (XPS), low energy electron diffraction (LEED) and scanning tunnelling microscopy (STM) techniques. LEED patterns and STM images show that no long range ordered structures are formed after NO adsorption on a Pt(111) surface. Although the total NO coverage is very low, spectroscopic features in N K-edge and O K-edge absorption spectra have been singled out and related to the different species induced by this preparation method. From these measurements it is concluded that the NO molecule is adsorbed trough the N atom in an upright conformation. The maximum saturation coverage is about 0.3 monolayers, and although nitric oxide is the major component, nitrite and nitrogen species are slightly co-adsorbed on the surface. The results obtained from this study are compared with those previously reported in the literature for NO adsorbed on Pt(111) under UHV conditions

Efecto de la suplementación con arginina y glutamina sobre la digestiblidad ileal y fecal de gazapos tras el destete

Se estudió el efecto de la suplementación con arginina y glutamina así como su posible interacción sobre la digestibilidad ileal y fecal de los nutrientes en gazapos tras el destete. Para ello se formuló una dieta basal (C) y se fabricaron otros 3 piensos añadiendo un 0,4% de arginina (ARG), un 0,4% de glutamina (GLN) y una mezcla de un 0,4% de arginina y un 0,4% de glutamina (ARG+GLN) a la ración basal. Se observó una interacción ARG×GLN en la digestibilidad fecal de la EB y el N (P = 0,008 y P = 0,001 respectivamente). La suplementación con ARG o GLN mejoró la digestibilidad de estos componentes en comparación con el pienso control, si bien cuando el pienso estuvo suplementado con ambos aminoácidos ARG+GLN mostró valores intermedios entre el grupo control y los suplementados con ARG o GLN (P < 0,001). La digestibilidad fecal de la FND fue superior en los piensos suplementados con GLN (P < 0,001). Los tratamientos no modificaron la digestibilidad ileal de la MS ni del N (P ≥ 0,44). La suplementación con glutamina tendió a incrementar la digestibilidad ileal del ácido glutámico (P = 0,099) respecto a los gazapos no suplementados, mientras que no afectó a la digestibilidad ileal de los demás aminoácidos (P ≥ 0,13). La suplementación con arginina + glutamina aumentó o tendió a aumentar la digestibilidad ileal aparente de la mayor parte de los aminoácidos esenciales y no esenciales de los gazapos de 35 d de edad (P < 0,096) respecto a la suplementación con glutamina

The optical system of the Tenerife Microwave Spectrometer: a window for observing the 10-20 GHz sky spectra

The TMS optical system is based on a decentered dual-reflector system in a Gregorian configuration to observe with an angular resolution of less than $2^\circ$. The primary goal of the present study is to evaluate the final design and verify that it satisfies the design requirements. We aim for low cross-polarization (-30 dB), low sidelobe (-25 dB) levels, and a stable beam in terms of shape (low ellipticity) and size over a full octave bandwidth (10-20 GHz). We performed both ray-tracing and full-wave simulations using the CST Studio software in order to investigate the system behaviour. We gave special attention to the beam frequency variation and polarization leakage. We have characterized the effects on the radiation pattern produced by the cryostat window. We present the final design of the TMS optical system, as well as a complete study of the system's performance in terms of cross-polarization, sidelobes, ellipticity and beamwidth. We discuss the effects of sidelobes and study the need for a baffle.Comment: 30 pages, 15 figures. Accepted for publication in JINS

Near-Infrared Polarimetric Adaptive Optics Observations of NGC 1068: A torus created by a hydromagnetic outflow wind

We present J' and K' imaging linear polarimetric adaptive optics observations of NGC 1068 using MMT-Pol on the 6.5-m MMT. These observations allow us to study the torus from a magnetohydrodynamical (MHD) framework. In a 0.5" (30 pc) aperture at K', we find that polarisation arising from the passage of radiation from the inner edge of the torus through magnetically aligned dust grains in the clumps is the dominant polarisation mechanism, with an intrinsic polarisation of 7.0%$\pm$2.2%. This result yields a torus magnetic field strength in the range of 4$-$82 mG through paramagnetic alignment, and 139$^{+11}_{-20}$ mG through the Chandrasekhar-Fermi method. The measured position angle (P.A.) of polarisation at K$'$ is found to be similar to the P.A. of the obscuring dusty component at few parsec scales using infrared interferometric techniques. We show that the constant component of the magnetic field is responsible for the alignment of the dust grains, and aligned with the torus axis onto the plane of the sky. Adopting this magnetic field configuration and the physical conditions of the clumps in the MHD outflow wind model, we estimate a mass outflow rate $\le$0.17 M$_{\odot}$ yr$^{-1}$ at 0.4 pc from the central engine for those clumps showing near-infrared dichroism. The models used were able to create the torus in a timescale of $\geq$10$^{5}$ yr with a rotational velocity of $\leq$1228 km s$^{-1}$ at 0.4 pc. We conclude that the evolution, morphology and kinematics of the torus in NGC 1068 can be explained within a MHD framework.Comment: 14 pages, 4 figures, Accepted by MNRA

Zone center phonons of the orthorhombic RMnO3 (R = Pr, Eu, Tb, Dy, Ho) perovskites

A short range force constant model (SRFCM) has been applied for the first time to investigate the phonons in RMnO3 (R = Pr, Eu, Tb, Dy, Ho) perovskites in their orthorhombic phase. The calculations with 17 stretching and bending force constants provide good agreement for the observed Raman frequencies. The infrared frequencies have been assigned for the first time. PACS Codes: 36.20.Ng, 33.20.Fb, 34.20.CfComment: 8 pages, 1 figur

Mid-infrared imaging- and spectro-polarimetric subarcsecond observations of NGC 1068

We present sub-arcsecond 7.5$-$13 $\mu$m imaging- and spectro-polarimetric observations of NGC 1068 using CanariCam on the 10.4-m Gran Telescopio CANARIAS. At all wavelengths, we find: (1) A 90 $\times$ 60 pc extended polarized feature in the northern ionization cone, with a uniform $\sim$44$^{\circ}$ polarization angle. Its polarization arises from dust and gas emission in the ionization cone, heated by the active nucleus and jet, and further extinguished by aligned dust grains in the host galaxy. The polarization spectrum of the jet-molecular cloud interaction at $\sim$24 pc from the core is highly polarized, and does not show a silicate feature, suggesting that the dust grains are different from those in the interstellar medium. (2) A southern polarized feature at $\sim$9.6 pc from the core. Its polarization arises from a dust emission component extinguished by a large concentration of dust in the galaxy disc. We cannot distinguish between dust emission from magnetically aligned dust grains directly heated by the jet close to the core, and aligned dust grains in the dusty obscuring material surrounding the central engine. Silicate-like grains reproduce the polarized dust emission in this feature, suggesting different dust compositions in both ionization cones. (3) An upper limit of polarization degree of 0.3 per cent in the core. Based on our polarization model, the expected polarization of the obscuring dusty material is $\lesssim$0.1 per cent in the 8$-$13 $\mu$m wavelength range. This low polarization may be arising from the passage of radiation through aligned dust grains in the shielded edges of the clumps.Comment: 17 pages, 10 figures, accepted for publication at MNRA