Distribución volumétrica, simetría del chorro y diámetro de gotas de las boquillas TF-VS2

El conocimiento de las características de las diferentes boquillas de pulverización tiene una importancia imprescindible para la adecuada y correcta recomendación de su uso. El objetivo de este trabajo fue determinar el espaciamiento máximo en la barra horizontal de pulverización, la simetría del chorro y el diámetro de gotas en boquillas de pulverización TF-VS2. El trabajo fue realizado en mesa de deposición, en donde fueron utilizadas las presiones de 100, 200 y 300 kPa en las alturas de trabajo de 40 y 50 cm. La simetría del chorro fue determinada en función de dos metodologías (empírica y trigonométrica). También se determinó el tamaño de las gotas, utilizando el método de difracción de rayos laser, en función de dos caldos de pulverización constituidos por agua y por agua con adyuvante en las tres presiones de trabajo ya descritas. Los espaciamientos máximos entre las boquillas en la barra de pulverización no pueden rebasar los 70 y 82 cm, admitiéndose el CV de un 10% para las alturas de 40 y de 50 cm respectivamente. La mayor presión proporcionó el menor diámetro mediano volumétrico (DMV) y la peor uniformidad de gotas, además del mayor porcentaje de gotas susceptibles a deriva, así como también aumentó la simetría entre los chorros.The knowledge of spray distribution pattern and analysis of droplets size of spray hydraulic nozzles turbo Floodjet TF-VS2 to adapt the spacing on spray boom are very important for a proper and correct use and recommendations. The aim of this study was to determine the maximum spacing on the horizontal spraying boom held on a patternator to the tips TF-VS2, under pressures of 100, 200 and 300 kPa in heights of work of 40 and 50 cm. Symmetry of spraying fan was determined due empirical and trigonometric methodology. It was also determined the droplets size by means of laser diffraction, with two spray liquids consisting of water and water plus adjuvant under three work pressures, described above. The maximum spacing between nozzles should be 70 and 82cm assuming the coefficient of variation of 10% for the heights of 40 and 50cm respectively. The higher pressure of work provided the lowest volume median diameter (VMD) and the worst uniformity of drops, beyond the higher percentage of drops susceptible to drift and improve the spray symmetry

Euclid: Early Release Observations -- Programme overview and pipeline for compact- and diffuse-emission photometry

International audienceThe Euclid ERO showcase Euclid's capabilities in advance of its main mission, targeting 17 astronomical objects, from galaxy clusters, nearby galaxies, globular clusters, to star-forming regions. A total of 24 hours observing time was allocated in the early months of operation, engaging the scientific community through an early public data release. We describe the development of the ERO pipeline to create visually compelling images while simultaneously meeting the scientific demands within months of launch, leveraging a pragmatic, data-driven development strategy. The pipeline's key requirements are to preserve the image quality and to provide flux calibration and photometry for compact and extended sources. The pipeline's five pillars are: removal of instrumental signatures; astrometric calibration; photometric calibration; image stacking; and the production of science-ready catalogues for both the VIS and NISP instruments. We report a PSF with a full width at half maximum of 0.16" in the optical and 0.49" in the three NIR bands. Our VIS mean absolute flux calibration is accurate to about 1%, and 10% for NISP due to a limited calibration set; both instruments have considerable colour terms. The median depth is 25.3 and 23.2 AB mag with a SNR of 10 for galaxies, and 27.1 and 24.5 AB mag at an SNR of 5 for point sources for VIS and NISP, respectively. Euclid's ability to observe diffuse emission is exceptional due to its extended PSF nearly matching a pure diffraction halo, the best ever achieved by a wide-field, high-resolution imaging telescope. Euclid offers unparalleled capabilities for exploring the LSB Universe across all scales, also opening a new observational window in the NIR. Median surface-brightness levels of 29.9 and 28.3 AB mag per square arcsec are achieved for VIS and NISP, respectively, for detecting a 10 arcsec x 10 arcsec extended feature at the 1 sigma level

Euclid: Early Release Observations -- Programme overview and pipeline for compact- and diffuse-emission photometry

International audienceThe Euclid ERO showcase Euclid's capabilities in advance of its main mission, targeting 17 astronomical objects, from galaxy clusters, nearby galaxies, globular clusters, to star-forming regions. A total of 24 hours observing time was allocated in the early months of operation, engaging the scientific community through an early public data release. We describe the development of the ERO pipeline to create visually compelling images while simultaneously meeting the scientific demands within months of launch, leveraging a pragmatic, data-driven development strategy. The pipeline's key requirements are to preserve the image quality and to provide flux calibration and photometry for compact and extended sources. The pipeline's five pillars are: removal of instrumental signatures; astrometric calibration; photometric calibration; image stacking; and the production of science-ready catalogues for both the VIS and NISP instruments. We report a PSF with a full width at half maximum of 0.16" in the optical and 0.49" in the three NIR bands. Our VIS mean absolute flux calibration is accurate to about 1%, and 10% for NISP due to a limited calibration set; both instruments have considerable colour terms. The median depth is 25.3 and 23.2 AB mag with a SNR of 10 for galaxies, and 27.1 and 24.5 AB mag at an SNR of 5 for point sources for VIS and NISP, respectively. Euclid's ability to observe diffuse emission is exceptional due to its extended PSF nearly matching a pure diffraction halo, the best ever achieved by a wide-field, high-resolution imaging telescope. Euclid offers unparalleled capabilities for exploring the LSB Universe across all scales, also opening a new observational window in the NIR. Median surface-brightness levels of 29.9 and 28.3 AB mag per square arcsec are achieved for VIS and NISP, respectively, for detecting a 10 arcsec x 10 arcsec extended feature at the 1 sigma level

Euclid: Early Release Observations -- Programme overview and pipeline for compact- and diffuse-emission photometry

International audienceThe Euclid ERO showcase Euclid's capabilities in advance of its main mission, targeting 17 astronomical objects, from galaxy clusters, nearby galaxies, globular clusters, to star-forming regions. A total of 24 hours observing time was allocated in the early months of operation, engaging the scientific community through an early public data release. We describe the development of the ERO pipeline to create visually compelling images while simultaneously meeting the scientific demands within months of launch, leveraging a pragmatic, data-driven development strategy. The pipeline's key requirements are to preserve the image quality and to provide flux calibration and photometry for compact and extended sources. The pipeline's five pillars are: removal of instrumental signatures; astrometric calibration; photometric calibration; image stacking; and the production of science-ready catalogues for both the VIS and NISP instruments. We report a PSF with a full width at half maximum of 0.16" in the optical and 0.49" in the three NIR bands. Our VIS mean absolute flux calibration is accurate to about 1%, and 10% for NISP due to a limited calibration set; both instruments have considerable colour terms. The median depth is 25.3 and 23.2 AB mag with a SNR of 10 for galaxies, and 27.1 and 24.5 AB mag at an SNR of 5 for point sources for VIS and NISP, respectively. Euclid's ability to observe diffuse emission is exceptional due to its extended PSF nearly matching a pure diffraction halo, the best ever achieved by a wide-field, high-resolution imaging telescope. Euclid offers unparalleled capabilities for exploring the LSB Universe across all scales, also opening a new observational window in the NIR. Median surface-brightness levels of 29.9 and 28.3 AB mag per square arcsec are achieved for VIS and NISP, respectively, for detecting a 10 arcsec x 10 arcsec extended feature at the 1 sigma level