Status and conservation of old-growth forests and endemic birds in the pine-oak zone of the Sierra Madre occidental Mexico

The pine-oak forests of the Sierra Madre Occidental, a mountain range in NW Mexico, have recently been recognized as an area of high endemism and biodiversity. Selective logging threatens three bird species endemic to this habitat, who depend on standing dead trees (snags). This report is based on an 11 month field survey that aimed to locate oldgrowth remnants and to assess the status of the endemic birds. Old-growth is defined here as a forest that has never been logged mechanically. Old-growth forests were located by ground-truthing of areas predicted by various methods: analyses of topographical maps and satellite images, aerial surveys, interviews with forestry technicians and local inhabitants, and literature studies. None of the prediction methods gives unambiguous results on their own. Only by applying the whole set of techniques could a comprehensive inventory be obtained of old-growth sites. Of the original 93, 560 km² of pine-oak habitat in the Sierra Madre Occidental, 571 km² remained as old-growth in 1995. This is a reduction of 99.4 %. The forests on high mesas, where the largest and most accessible timber stood, have been reduced to 22 km² uncut forest. In logged forests pines greater than 30 cm girth have been extracted and snags have been cut for the production of paper pulp. Small settlements are everywhere. Information on the Imperial Woodpecker Campephilus imperialis was obtained through interviews with 62 elder inhabitants who had known the bird. The extinction peak of this species was between 1946 and 1965, when 60 % of the informants saw their last Imperial Woodpecker. Hunting by settlers and loggers, for fun and for medicinal purposes, quickly decimated populations. Recovery from the shooting became impossible through the ensuing logging of nearly all the pine-oak habitat. Mature pines and pine snags were removed, depriving the Imperial Woodpecker of foraging and nesting sites. Imperial Woodpeckers were often seen in groups. A typical group consisted of seven or eight birds. With an estimated average density of one Imperial Woodpecker per 13 km², the original pine-oak habitat in the whole range of the species may have carried only 8,000 individuals or 1060 groups. Interviews, and workings found in one old-growth area, indicate that very few Imperial Woodpeckers may have survived into the 1990s. Extinction of the species seems nevertheless inevitable since nowhere does any breeding habitat remain. Cutting of snags is the main threat to the Thick-billed Parrot Rhynchopsitta pachyrhyncha. This species only breeds at altitudes above 2300 m, but snags are scarce on the exploited mesa forests in the highest parts of the sierra. The breeding range runs from within 85 km of the US border in northern Chihuahua south to central western Durango, with an apparent gap in southern Chihuahua. Pine seeds for foraging are widely available in young recovering forest. Compared with historical records, encountered groups of wintering Thick-billed Parrots were small, few groups were seen, and the numbers of bathing and drinking parrots at a waterfall in northern Chihuahua were low. This indicates numbers have sharply declined in the course of the 20th century. The status of the Eared Trogon Euptilotis neoxenus is far less critical. Eared Trogons were observed at 55 locations, mainly in canyons. Nests were found in riparian corridors in canyons. Such corridors are hardly accessible to the logging industry. The ability, and probable preference, of the Eared Trogon to breed in canyons likely explains why it is still fairly common. The erroneous notion that the Eared Trogon is a local and rare species must stem from the paucity of field studies in the Sierra Madre Occidental, as well as the wariness of the bird. It is mostly to be detected by its vocalizations. Efforts are being made to ensure the total protection of three priority areas (figures 26 to 28). These areas encompass the main old-growth fragments in the Sierra Madre Occidental. They are also of major importance to the endemic fauna. Protection of snags is required for three breeding areas of the Thick-billed Parrot (figures 29 to 31). Ideally, exploitation of snags should be banned throughout the Sierra Madre Occidental

Modelagem da recomendação de corretivos e fertilizantes para a cultura da soja Modeling lime and fertilizer recommendations for soybean

A recomendação de adubação para as culturas agrícolas, no Brasil, é feita com base em tabelas que relacionam a classe de disponibilidade do nutriente no solo com a dose a ser aplicada. Este trabalho apresenta uma alternativa para recomendar corretivos e fertilizantes para a cultura da soja, o SIRSo (sistema de recomendação de corretivos e fertilizantes para a cultura da soja). O princípio desse sistema é o balanço nutricional, ou seja, a recomendação se faz a partir da diferença entre o requerimento de nutrientes pela planta e o suprimento de nutrientes pelo solo, por resíduos orgânicos, por fertilizantes e pela calagem. O sistema considera ainda o fator sustentabilidade, visando manter uma quantidade de nutriente no solo capaz de garantir produtividade mínima em cultivos subseqüentes. Para recomendar calagem, o sistema considera dois métodos: a neutralização do Al3+ e a elevação dos teores de Ca2+ + Mg2+, ou a saturação por bases. O requerimento de nutrientes varia com a produtividade esperada de grãos, com as características do solo e com a taxa de recuperação pela planta do nutriente aplicado ao solo. O suprimento pelo solo depende da disponibilidade do nutriente, estimada a partir da análise de solo e da taxa de recuperação pelo extrator do nutriente aplicado. As comparações entre as recomendações geradas pelo SIRSo e aquelas oriundas das tabelas em uso no País mostram, em geral, que o SIRSo recomenda maior quantidade de nutrientes, principalmente de P e K quando consideradas as maiores produtividades, fato confirmado pela análise de sensibilidade, que mostrou grande variação da dose a ser recomendada desses nutrientes com a produtividade de grãos. Esse fato pode ser considerado como vantagem do SIRSo em relação às tabelas, muitas das quais apresentam pouca ou nenhuma variabilidade das doses em relação à produtividade.<br>Fertilizer recommendations for agricultural crops in Brazil are based on tables that relate indexes of nutrient availability in the soil with the required dose of the nutrient. This study presents an alternative for lime and fertilizer recommendations for soybean, called SIRSo. This lime and fertilizer recommendation system for soybean considers the nutritional balance, i.e., recommendations are based on the difference between plant nutrient requirement and the nutrient supply from the soil through organic residues, fertilizers and liming. The system further takes a sustainability factor into consideration, aiming at the maintenance of soil nutrient levels that ensure a desired minimum yield in subsequent cultivations. The system considers two methods for liming recommendations: Al3+ neutralization and increased Ca2+ + Mg2+ contents or base saturation. Nutrient requirements vary according to the expected grain yield, the soil characteristics and plant recovery rate of the nutrient applied to the soil. The soil supply depends on the estimated nutrient availability based on the soil analysis, and on the recovery rate of the applied nutrient by the extractor. Comparisons of SIRSo-based recommendations with those of the tables used nationwide show that SIRSo generally recommends higher nutrient quantities, mainly for P and K, when the highest yields are considered. This fact was confirmed by the sensitivity analysis, which detected wide variation of the recommended dose for these nutrients according to the grain yield. This fact is considered an advantage of SIRSo over the tables, where recommendations of doses according to the yield are little or not adjustable at all

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