Coordination des actions impliquees dans le reboisement forestier pour obtenir la maximum de'efficacite et d'economie d'ensembre dans les trabaux

International Union of Forest Research Organizations . World Congress 17o . 1981 . Japon)Depto. de Estadística e Investigación OperativaFac. de Ciencias MatemáticasTRUEpu

Active plasmonic devices and optical metamaterials

We studied active near-infrared metamaterials based on phase transition of vanadium oxide thin films, asymmetrically coupled split-ring resonators for narrowing resonance line-widths , field effect modulation of plasmon propagation and 3D single layer, plasmonic negative-index metamaterials

Global, Diffuse, Direct, and Ultraviolet Solar Irradiance Recorded in Malta and Atmospheric Component Influences

AbstractGlobal and diffuse shortwave (SW) and global erythemal (UVER) irradiances were measured in Malta, in the middle of Mediterranean Sea. The effect of solar zenith angle on these irradiances is studied using the measurements and simulations developed with a radiative transfer model. The role of ozone, scattering by gases, and aerosols is analyzed. Results show that ozone and Rayleigh scattering are the main drivers responsible for the behavior of UVER variations with SZA. In the case of global and diffuse irradiance, the role of aerosols is the principal determinant

Phase diagram and critical properties in the Polyakov--Nambu--Jona-Lasinio model

We investigate the phase diagram of the so-called Polyakov--Nambu--Jona-Lasinio model at finite temperature and nonzero chemical potential with three quark flavours. Chiral and deconfinement phase transitions are discussed, and the relevant order-like parameters are analyzed. The results are compared with simple thermodynamic expectations and lattice data. A special attention is payed to the critical end point: as the strength of the flavour-mixing interaction becomes weaker, the critical end point moves to low temperatures and can even disappear.Comment: Talk given at the 9th International Conference on Quark Confinement and the Hadron Spectrum - QCHS IX, Madrid, Spain, 30 August - September 201

Diagnóstico ambiental do Município de Iguaraci, PE.

O municipio de Iguaraci, com uma area de 770,96 km2, localiza-se na regiao semi-arida de Pernambuco, na Zona do Alto Pajeu. O estudo, na escala 1:100.000, identifica os diversos ambientes do municipio, com suas principais vocacoes, potencialidades e limitacoes. Pode, entao, subsidiar o planejamento de atividades agricolas, pecuarias, florestais ou outros tipos de atividades nao agricolas, incluindo recomendacoes de areas para preservacao ambiental. O municipio foi dividido em 15 segmentos geoambientais em funcao do arranjo e distribuicao dos diferentes solos em topossequencias, do grau xerofitico da caatinga (hiper e hipoxerofila) e, no caso das Serras e Serrotes, tambem foram consideradas suas dimensoes e diferencas geologicas. Estes segmentos geoambientais foram agrupados em 5 subunidades geoambientais em funcao de diferenciacoes geologicas, aspectos morfoestruturais, e de combinacoes de caracteristicas de geologia e relevo. As subunidades geoambientais identificadas foram as seguintes: (1) Tabuleiros Interioranos Dissecados Isolados - TD (com o segmento geoambiental TD1); (2) Superficies Avermelhadas do Cristalino - SA (com o segmento geoambiental SA1); (3) Pediplanos do Alto Pajeu - PD (com os segmentos geoambientais PD1 a PD6); (4) Terracos Aluviais - Baixios - TA (com os segmentos geoambientais TA1 e TA2); e (5) Serras, Serrotes e Elevacoes Residuais - SS (com os segmentos geoambientais SS1 a SS5). Os segmentos geoambientais indicados preferencialmente para lavouras sao TD1, SA1, TA1, TA2, PD1 e PD2, que perfazem uma area de 76,48 km2. Os segmentos indicados para lavouras e/ou pastagens (plantadas ou naturais) sao PD3 e PD4, abrangendo uma area de 206,74 km2. Os segmentos geoambientais recomendados para pecuaria extensiva, pastagem natural e/ou plantada e apicultura, sao PD5 e PD6, perfazendo uma area de 359,56 km2. Os segmentos indicados para preservacao ambiental sao os SS1 a SS5, perfazendo uma area de 18,18 km2.bitstream/CNPS/10851/1/circular_tecnica_07_2000.pd

Detection of optical emission from the supernova remnant G7.7-3.7

We present the first optical study of the supernova remnant (SNR) G7.7-3.7, with the aim of determining its evolutionary phase since it has been suggested to be the remnant of SN 386 AD. We obtained narrow-band images in the filters H$\alpha$ + [NII], H$\beta$, [OIII], [SII] that revealed faint optical emission in the southern region of the SNR consisting of two filaments elongated in the east-west direction aligned with the X-ray emitting region of the remnant. The filaments were seen in H$\alpha$ + [NII], [OIII] images and marginally in the [SII] images, with a non-detection in H$\beta$. Long-slit spectroscopy of three regions along one filament revealed large ratios of [SII] / H$\alpha$ = (1.6-2.5), consistent with that expected for a shock-heated SNR. The [SII] doublet ratio observed in two of the regions implies an upper limit for the electron density of the gas, with estimates falling below 400 cm$^{-3}$ and 600 cm$^{-3}$ in the respective areas. We discuss potential physical mechanisms that formed the observed optical filaments and we suggest that most likely they resulted by a collision of the SNR with a dense circumstellar shell lying at the southern region of the remnant.Comment: 10 pages, 5 figures, accepted in MNRA

Detection of optical emission from the supernova remnant G7.7–3.7

The work of VD is supported by a grant from NWO graduate programme/GRAPPA-PhD programme. VD also acknowledges support from the LKBF, subsidy no. 19.2.027. JVHS acknowledges support from STFC grant ST/R000824/1. PZ acknowledges the support from the NWO Veni Fellowship, grant no. 639.041.647 and NSFC grant 11590781. SA thanks the support under the grant 5077 financed by IAASARS/NOA. AdB thanks the support from the Spanish Government Ministerio de Ciencia e Innovación through grants PGC-2018-091, 3741-B-C22, and SEV 2015-0548, from the Canarian Agency for Research, Innovation and Information Society (ACIISI) of the Canary Islands Government, and from the European Regional Development Fund (ERDF), under grant with reference ProID2017010115.We present the first optical study of the supernova remnant (SNR) G7.7–3.7, with the aim of determining its evolutionary phase since it has been suggested to be the remnant of SN 386 AD. We obtained narrow-band images in the filters H α + [N ii], H β, [O iii], [S ii] that revealed faint optical emission in the southern region of the SNR consisting of two filaments elongated in the east–west direction aligned with the X-ray emitting region of the remnant. The filaments were seen in H α + [N ii], [O iii] images and marginally in the [S ii] images, with a non-detection in H β. Long-slit spectroscopy of the three regions along one filament revealed large ratios of [S ii]/H α = (1.6–2.5), consistent with that expected for a shock-heated SNR. The [S ii] doublet ratio observed in two of the regions implies an upper limit for the electron density of the gas, with estimates falling below 400 cm−3 and 600 cm−3 in the respective areas. We discuss potential physical mechanisms that formed the observed optical filaments and we suggest that most likely they resulted by a collision of the SNR with a dense circumstellar shell lying at the southern region of the remnant.Publisher PDFPeer reviewe

Stars and brown dwarfs in the sigma Orionis cluster IV. IDS/INT and OSIRIS/GTC spectroscopy and Gaia DR2 astrometry

Context. Only a few open clusters are as important for the study of stellar and substellar objects, and their formation and evolution, as the young σ Orionis cluster. However, a complete spectroscopic characterisation of its whole stellar population is still missing. Aims. We filled most of that gap with a large spectroscopic and astrometric survey of targets towards σ Orionis. Eventually, it will be one of the open clusters with the lowest proportion of interlopers and the largest proportion of confirmed cluster members with known uncontrovertible youth features. Methods. We acquired 317 low-resolution optical spectra with the Intermediate Dispersion Spectrograph (IDS) at the 2.5 m Isaac Newton Telescope (INT) and the Optical System for Imaging and low Resolution Integrated Spectroscopy (OSIRIS) at the 10.4 m Gran Telescopio Canarias (GTC). We measured equivalent widths of Li i, Hα, and other key lines from these spectra, and determined spectral types. We complemented this information with Gaia DR2 astrometric data and other features of youth (mid-infrared excess, X-ray emission) compiled with Virtual Observatory tools and from the literature. Results. Of the 168 observed targets, we determined for the first time spectral types of 39 stars and equivalent widths of Li i and Hα of 34 and 12 stars, respectively. We identified 11 close (ρ </≈ 3 arcsec) binaries resolved by Gaia, of which three are new, 14 strong accretors, of which four are new and another four have Hα emission shifted by over 120 km s^(−1) , two juvenile star candidates in the sparse population of the Ori OB1b association, and one spectroscopic binary candidate. Remarkably, we found 51 non-clustermembers, 35 of which were previously considered as σ Orionis members and taken into account in high-impact works on, for example, disc frequency and initial mass function