Uso de poda verde, plásticos refletivos, antitranspirante e potássio na produção de pêssegos Using green pruning, reflective plastics, antitranspirant and potassium in peach production

O objetivo deste trabalho foi avaliar técnicas que viabilizem a produção de pêssegos de melhor qualidade, ao potencializar características externas como a coloração vermelha na epiderme e o tamanho, bem como características químicas relativas ao sabor. Num pomar comercial de pessegueiros da cultivar Maciel, no Município de Pelotas, RS, foram avaliados os efeitos da poda verde, o uso de dois tipos de plástico refletivo sob a copa das plantas, diferentes concentrações de cloreto de potássio (KCl) incorporado ao solo, com ou sem KCl via foliar e antitranspirante. O delineamento experimental utilizado foi o de blocos ao acaso. O uso de 1.200 g de KCl via solo, combinado com 10 g de KCl via foliar e poda verde, produziu coloração vermelha mais intensa na epiderme dos pêssegos. O uso de 1.600 g de KCl no solo, combinado com poda verde, produziu pêssegos com maior peso médio, maior diâmetro e baixa acidez titulável. A cobertura do solo, sob a copa das plantas, com plástico de ráfia, combinado com poda verde, resultou num maior teor de sólidos solúveis totais nos frutos. O uso dessas práticas culturais, realizadas na pré-colheita, influencia positivamente a qualidade final das frutas de pessegueiro da cultivar Maciel.<br>The objective of this work was to evaluate techniques which make possible the production of peaches of high quality by improving external characteristics, percent of red cover color, fruit size, and chemical characteristics that influence flavor, in a field peach of cultivar Maciel, in Pelotas, RS, Brazil. Effects evaluated were: vegetative pruning, the use of two types of reflective plastics under the plant canopy, the different potassium chloride concentrations incorporated to the soil, with and without foliar aplication of KCl, and the use of antitranspirant. The experiment was carried out in a randomized block design. The results showed that the use of 1,200 g of KCl applied to soil, combined with 10 g of KCl as foliar application and vegetative pruning, provided intense red coloration of the peaches epidermis. The use of 1,600 g of KCl in the soil, combined with green pruning, resulted in higher average weight, larger diameter and low titratable acidity. Soil cover with raffia plastic under plant canopy, combined with green pruning, resulted in higher soluble solids content in the fruits. These practics during preharvest influence positively the final quality of cultivar Maciel peaches

Multi-messenger Observations of a Binary Neutron Star Merger

International audienceOn 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of $\sim 1.7\,{\rm{s}}$ with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg(2) at a luminosity distance of ${40}_{-8}^{+8}$ Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 $\,{M}_{\odot }$. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at $\sim 40\,{\rm{Mpc}}$) less than 11 hours after the merger by the One-Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ∼10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position $\sim 9$ and $\sim 16$ days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC 4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta