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Marcelle Michelotti Bettoni,Átila Francisco Mogor,Volnei Pauletti,Nieves Goicoechea 한국원예학회 2017 Horticulture, Environment, and Biotechnology Vol.58 No.5
The combined application of humic substances and mycorrhizal inocula under increased CO2 in the air is apromising horticultural technique for improving the quality of greenhouse-grown onion seedlings. The objective of thisstudy was to evaluate if the development and qualitative characteristics of bulbs from the yellow onion Allium cepaL. Alfa São Francisco improved with the application of the abovementioned agronomic, biotic, and environmentalfactors. The lowest dry matter was achieved in bulbs of onions not inoculated with mycorrhizal fungi, non-amendedwith humic acids (HA), and grown at ambient CO2. Mycorrhizal inoculation significantly increased bulb biomass inplants cultivated at ambient CO2, and not fertilized with HA, which may be a consequence of the enhanced acidphosphatase activity in roots. The application of HA always increased bulb dry matter, which were more evident atelevated rather than ambient CO2 conditions and correlated with improved acid phosphatase activity in the plants atelevated CO2. Mycorrhizal inoculation, HA supplementation, and elevated CO2 in the air had an additive effect ofincreasing the content of soluble sugars, proteins, and phenolics in bulbs. While high levels of sugars and proteinsenhanced the energetic value of onions, the increase in phenolics improved their antioxidant properties. The tripleinteraction between mycorrhization, HA fertilization, and elevated CO2 also increased the ratio between soluble solidsand total titratable acidity, which may enhance the perception of sweetness and make onions more pleasant forconsumption.
GASP. I. Gas Stripping Phenomena in Galaxies with MUSE
Poggianti, Bianca M.,Moretti, Alessia,Gullieuszik, Marco,Fritz, Jacopo,Jaffé,, Yara,Bettoni, Daniela,Fasano, Giovanni,Bellhouse, Callum,Hau, George,Vulcani, Benedetta,Biviano, Andrea,Omizzolo, A American Astronomical Society 2017 The Astrophysical journal Vol.844 No.1
Lutz, M.F.M.,Lange, J.S.,Pennington, M.,Bettoni, D.,Brambilla, N.,Crede, V.,Eidelman, S.,Gillitzer, A.,Gradl, W.,Lang, C.B.,Metag, V.,Nakano, T.,Nieves, J.,Neubert, S.,Oka, M.,Olsen, S.L.,Pappagallo, North Holland Pub. Co 2016 Nuclear physics. A Vol.948 No.-
<P>We report on the EMMI Rapid Reaction Task Force meeting 'Resonances in QCD', which took place at GSI October 12-14,2015. A group of 26 people met to discuss the physics of resonances in QCD. The aim of the meeting was defined by the following three key questions: What is needed to understand the physics of resonances in QCD? Where does QCD lead us to expect resonances with exotic quantum numbers? What experimental efforts are required to arrive at a coherent picture? For light mesons and baryons only those with up, down and strange quark content were considered. For heavy-light and heavy-heavy meson systems, those with charm quarks were the focus. This document summarizes the discussions by the participants, which in turn led to the coherent conclusions we present here. (C) 2016 Elsevier B.V. All rights reserved.</P>
Can a spontaneous smile invalidate facial identification by photo-anthropometry?
Pinto, Paulo Henrique Viana,Rodrigues, Caio Henrique Pinke,Rozatto, Juliana Rodrigues,da Silva, Ana Maria Bettoni Rodrigues,Bruni, Aline Thais,da Silva, Marco Antonio Moreira Rodrigues,da Silva, Ricar Korean Academy of Oral and Maxillofacial Radiology 2021 Imaging Science in Dentistry Vol.51 No.3
Purpose: Using images in the facial image comparison process poses a challenge for forensic experts due to limitations such as the presence of facial expressions. The aims of this study were to analyze how morphometric changes in the face during a spontaneous smile influence the facial image comparison process and to evaluate the reproducibility of measurements obtained by digital stereophotogrammetry in these situations. Materials and Methods: Three examiners used digital stereophotogrammetry to obtain 3-dimensional images of the faces of 10 female participants(aged between 23 and 45 years). Photographs of the participants' faces were captured with their faces at rest (group 1) and with a spontaneous smile (group 2), resulting in a total of 60 3-dimensional images. The digital stereophotogrammetry device obtained the images with a 3.5-ms capture time, which prevented undesirable movements of the participants. Linear measurements between facial landmarks were made, in units of millimeters, and the data were subjected to multivariate and univariate statistical analyses using Pirouette<sup>®</sup> version 4.5 (InfoMetrix Inc., Woodinville, WA, USA) and Microsoft Excel<sup>®</sup> (Microsoft Corp., Redmond, WA, USA), respectively. Results: The measurements that most strongly influenced the separation of the groups were related to the labial/buccal region. In general, the data showed low standard deviations, which differed by less than 10% from the measured mean values, demonstrating that the digital stereophotogrammetry technique was reproducible. Conclusion: The impact of spontaneous smiles on the facial image comparison process should be considered, and digital stereophotogrammetry provided good reproducibility.
Bellhouse, C.,Jaffé,, Y. L.,Hau, G. K. T.,McGee, S. L.,Poggianti, B. M.,Moretti, A.,Gullieuszik, M.,Bettoni, D.,Fasano, G.,D’Onofrio, M.,Fritz, J.,Omizzolo, A.,Sheen, Y.-K.,Vulcani, B. American Astronomical Society 2017 The Astrophysical journal Vol.844 No.1
<P>This paper presents a spatially. resolved kinematic study of the jellyfish galaxy JO201, one of the most spectacular cases of ram-pressure stripping (RPS) in the. GAs Stripping Phenomena in galaxies with MUSE (GASP) survey. By studying the environment of JO201, we find that it is moving through the dense intracluster medium of Abell 85 at supersonic speeds along our line of sight, and that it is likely accompanied by a small group of galaxies. Given the density of the intracluster medium and the galaxy's mass, projected position, and velocity within the cluster, we estimate that JO201 must so far have lost similar to 50% of its gas during infall via RPS. The MUSE data indeed reveal a smooth stellar disk. accompanied by large projected tails of ionized (Ha) gas, composed of kinematically cold (velocity dispersion < 40 km s(-1)) star-forming knots and very warm (> 100 km s(-1)) diffuse emission,. that. extend out to at least similar to 50 kpc from the galaxy center. The ionized H alpha-emitting gas in the disk rotates with the stars out to similar to 6. kpc; but, in the disk outskirts,. it. becomes increasingly redshifted with respect to the (undisturbed) stellar disk. The observed disturbances are consistent with the presence of gas trailing behind the stellar component. resulting from intense face-on RPS. along the line of sight. Our kinematic analysis is consistent with the estimated fraction of lost gas. and reveals that stripping of the disk happens outside-in, causing shock heating and gas compression in the stripped tails.</P>