910 resultados para Wilt, Joshua


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Plant-parasitic nematodes are microscopic worms that feed on plants. Almost every nematode that feeds on corn is capable of feeding on many other plants. These nematode parasites are thought to be native to most Iowa soils and to have fed upon native plants before corn was grown as a cultivated crop. Population densities (numbers) of most species of plant-parasitic nematodes that feed on corn have to increase to damaging levels (called damage thresholds) before yield loss occurs.

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Producers continue to look at different management practices to increase corn and soybean yields. One area of interest is planting corn and soybeans in narrow rows. Traditionally, these crops have been planted in row widths of 30 to 38 in. Planters on the market today have the capability to plant corn and soybeans in 15- and 20-in. rows, as well as in twin rows that are spaced eight inches apart. This study was set up to evaluate the yield impact of planting soybeans in 15-in. rows versus the traditional 30-in. row spacing.

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Growers of organic squash need effective ways to manage insect and disease problems. The squash bug (Anasa tristis) sucks sap, causing leaves to wilt and turn black. The squash vine borer (Melittia cucurbitae) can devastate winter squash plantings. Burrowing by larvae into the base of the stem causes yellowing and wilting. Organic insecticides are expensive, have limited efficacy, require many applications, and some kill beneficial as well as target insects.

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Cucurbit crops, especially muskmelon and cucumber, attract cucumber beetles, which vector bacterial wilt: Erwinia tracheiphila, causing significant crop losses. High beetle densities are associated with high bacterial wilt incidence, which usually occurs during the first stages of plant establishment. Growers of organic muskmelon need effective ways to manage the cucumber beetle/bacterial wilt complex.

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A limiting factor in the accuracy and precision of U/Pb zircon dates is accurate correction for initial disequilibrium in the 238U and 235U decay chains. The longest-lived-and therefore most abundant-intermediate daughter product in the 235U isotopic decay chain is 231Pa (T1/2 = 32.71 ka), and the partitioning behavior of Pa in zircon is not well constrained. Here we report high-precision thermal ionization mass spectrometry (TIMS) U-Pb zircon data from two samples from Ocean Drilling Program (ODP) Hole 735B, which show evidence for incorporation of excess 231Pa during zircon crystallization. The most precise analyses from the two samples have consistent Th-corrected 206Pb/238U dates with weighted means of 11.9325 ± 0.0039 Ma (n = 9) and 11.920 ± 0.011 Ma (n = 4), but distinctly older 207Pb/235U dates that vary from 12.330 ± 0.048 Ma to 12.140 ± 0.044 Ma and 12.03 ± 0.24 to 12.40 ± 0.27 Ma, respectively. If the excess 207Pb is due to variable initial excess 231Pa, calculated initial (231Pa)/(235U) activity ratios for the two samples range from 5.6 ± 1.0 to 9.6 ± 1.1 and 3.5 ± 5.2 to 11.4 ± 5.8. The data from the more precisely dated sample yields estimated DPazircon/DUzircon from 2.2-3.8 and 5.6-9.6, assuming (231Pa)/(235U) of the melt equal to the global average of recently erupted mid-ocean ridge basaltic glasses or secular equilibrium, respectively. High precision ID-TIMS analyses from nine additional samples from Hole 735B and nearby Hole 1105A suggest similar partitioning. The lower range of DPazircon/DUzircon is consistent with ion microprobe measurements of 231Pa in zircons from Holocene and Pleistocene rhyolitic eruptions (Schmitt (2007; doi:10.2138/am.2007.2449) and Schmitt (2011; doi:10.1146/annurev-earth-040610-133330)). The data suggest that 231Pa is preferentially incorporated during zircon crystallization over a range of magmatic compositions, and excess initial 231Pa may be more common in zircons than acknowledged. The degree of initial disequilibrium in the 235U decay chain suggested by the data from this study, and other recent high precision datasets, leads to resolvable discordance in high precision dates of Cenozoic to Mesozoic zircons. Minor discordance in zircons of this age may therefore reflect initial excess 231Pa and does not require either inheritance or Pb loss.

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In an attempt to determine the helium and neon isotopic composition of the lower oceanic crust, we report new noble gas measurements on 11 million year old gabbros from Ocean Drilling Program site 735B in the Indian Ocean. The nine whole rock samples analyzed came from 20 to 500 m depth below the seafloor. Helium contents vary from 3.3*10**-10 to 2.5*10**-7 ccSTP/g by crushing and from 5.4*10**-8 to 2.4*10**-7 ccSTP/g by melting. 3He/4He ratios vary between 2.2 and 8.6 Ra by crushing and between 2.9 and 8.2 by melting. The highest R/Ra ratios are similar to the mean mid-ocean ridge basalt (MORB) ratio of 8+/-1. The lower values are attributed to radiogenic helium from in situ alüha-particle production during uranium and thorium decay. Neon isotopic ratios are similar to atmospheric ratios, reflecting a significant seawater circulation in the upper 500 m of exposed crust at this site. MORB-like neon, with elevated 20Ne/22Ne and 21Ne/22Ne ratios, was found in some high temperature steps of heating experiments, but with very small anomalies compared to air. These first results from the lower oceanic crust indicate that subducted lower oceanic crust has an atmospheric 20Ne/22Ne ratio. Most of this neon must be removed during the subduction process, if the ocean crust is to be recirculated in the upper mantle, otherwise this atmospheric neon will overwhelm the upper mantle neon budget. Similarly, the high (U+Th)/3He ratio of these crustal gabbros will generate very radiogenic 4He/3He ratios on a 100 Ma time scale, so lower oceanic crust cannot be recycled into either MORB or oceanic island basalt without some form of processing.

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Existen pocas publicaciones sobre claves de identificación de larvas de trips. Sin embargo, el tema es de interés básico para detectar el rango de hospedantes de los trips. Algunas especies son capaces de transmitir Tospovirus, agentes causales de la peste negra y otras enfermedades. El insecto adquiere el virus sólo como larva. Una clave de larvas será una herramienta útil para estudios epidemiológicos. La identificación de larvas es difícil porque tienen menos caracteres distintivos que los adultos; además, los individuos crecen constantemente. Las larvas obtenidas para este trabajo se recolectaron del campo sobre varias malezas y algunas plantas nativas y cultivadas. También se criaron en chauchas de poroto o polen y miel diluida a partir de adultos identificados. En este trabajo se presenta una descripción breve del segundo estadío larval de Frankliniella australis Morgan, F. gemina Bagnall, F. occidentalis Pergande, F. schultzei Trybom, F. valdiviana Sakimura et O'Neil y Thrips tabaci Lindeman y una clave para separar estas especies. Estación Experimental Agropecuaria INTA Mendoza.

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En alcauciles (Cynara scolymus L.) de la variedad Bleek cultivados en Coquimbito (Mendoza, Argentina) se observó marcada detención del crecimiento y atraso en la formación de las inflorescencias. Las plantas sanas tenían aprox. 1 m de altura mientras las enfermas no llegaban a 30 cm. Las hojas más externas manifestaban clorosis y leve marchitez con posterior necrosis. Se realizaron aislamientos en APG desarrollándose colonias de aspecto mucoso, sobreelevadas, de color castaño claro. También se sembró en medio Kelman base sin TZ desarrollando colonias de iguales características pero con bordes festoneados típicos del género Erwinia. Pruebas bioquímicas y de patogenicidad en invernáculo resultaron positivas. Se identificó a Erwinia carotovora (Jones) Bergey et al. subsp. carotovora Dye, como agente causal de esta podredumbre radical en alcaucil.

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Ralstonia solanacearum (Rs) produce la enfermedad cuarentenaria denominada marchitez bacteriana en papa. México es un país importador de semilla de Estados Unidos de América y Canadá, aspecto significante para provocar una eventual introducción de esta enfermedad en áreas con amplias extensiones de papa. Sonora es una región importante en relación con la producción de este cultivo. Por lo anteriormente expuesto, se realizó la presente investigación, teniendo como objetivos: a) la producción de antisuero para la bacteria Rs; b) diagnosticar Rs en tubérculos de importación que se utilizan para siembra, y en tubérculos de procedencia mexicana para consumo humano, que son utilizados como semilla; c) la detección de la bacteria durante el desarrollo vegetativo de lotes de papa en Sonora, México. Se analizó tubérculo semilla de importación, de consumo humano, plantas de papa, hojas y tubérculos de producción; los métodos de detección utilizados fueron medios de cultivos específicos, ELISA, antisuero producido y pruebas de patogenicidad. Los resultados mostraron positiva la presencia de Rs en tubérculos de consumo; en tubérculos de importación y en etapas vegetativas fue negativa. Cada prueba de detección por separado no debe ser utilizada como método único; la presencia de Rs representa un riesgo de eventual manifestación de la enfermedad, por lo que es necesario que las áreas productoras realicen actividades de control preventivo fitosanitario.

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El tomate de cáscara (Physalis ixocarpa Brot.) es un cultivo alimenticio de gran importancia económica en México. Sin embargo, es afectado por diversas plagas y enfermedades tales como los Thrips (Thysanoptera: Frankliniella occidentalis) y el virus de la marchitez manchada del tomate (TSWV) que llegan a causar hasta un 80% de pérdidas. El objetivo del presente trabajo fue modelizar la distribución espacial de huevos de Thrips mediante técnicas geoestadísticas y obtener, en consecuencia, mapas de incidencia por medio del Kriging. Se georreferenciaron 121 puntos de muestreo en cada una de las parcelas comerciales de los municipios de Luvianos, Jocotitlán e Ixtlahuaca, a través del método de transectos en tres etapas fenológicas del cultivo. Se contabilizó el número de huevos de Thrips en cada punto de muestreo. Los resultados mostraron que las poblaciones de huevos deThrips presentan una distribución agregada, identificándose varios centros de conglomeración a través de los mapas obtenidos. Los semivariogramas obtenidos de la distribución espacial se ajustaron principalmente a los modelos gaussianos y esféricos. La distribución de huevos de Thrips se presentó en centros de agregación dentro de las parcelas estudiadas, lo cual permitirá establecer estrategias y medidas de control o mitigación en términos de sitios específicos de infestación de huevos de Thrips.

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We characterize the textural and geochemical features of ocean crustal zircon recovered from plagiogranite, evolved gabbro, and metamorphosed ultramafic host-rocks collected along present-day slow and ultraslow spreading mid-ocean ridges (MORs). The geochemistry of 267 zircon grains was measured by sensitive high-resolution ion microprobe-reverse geometry at the USGS-Stanford Ion Microprobe facility. Three types of zircon are recognized based on texture and geochemistry. Most ocean crustal zircons resemble young magmatic zircon from other crustal settings, occurring as pristine, colorless euhedral (Type 1) or subhedral to anhedral (Type 2) grains. In these grains, Hf and most trace elements vary systematically with Ti, typically becoming enriched with falling Ti-in-zircon temperature. Ti-in-zircon temperatures range from 1,040 to 660°C (corrected for a TiO2 ~ 0.7, a SiO2 ~ 1.0, pressure ~ 2 kbar); intra-sample variation is typically ~60-15°C. Decreasing Ti correlates with enrichment in Hf to ~2 wt%, while additional Hf-enrichment occurs at relatively constant temperature. Trends between Ti and U, Y, REE, and Eu/Eu* exhibit a similar inflection, which may denote the onset of eutectic crystallization; the inflection is well-defined by zircons from plagiogranite and implies solidus temperatures of ~680-740°C. A third type of zircon is defined as being porous and colored with chaotic CL zoning, and occurs in ~25% of rock samples studied. These features, along with high measured La, Cl, S, Ca, and Fe, and low (Sm/La)N ratios are suggestive of interaction with aqueous fluids. Non-porous, luminescent CL overgrowth rims on porous grains record uniform temperatures averaging 615 ± 26°C (2SD, n = 7), implying zircon formation below the wet-granite solidus and under water-saturated conditions. Zircon geochemistry reflects, in part, source region; elevated HREE coupled with low U concentrations allow effective discrimination of ~80% of zircon formed at modern MORs from zircon in continental crust. The geochemistry and textural observations reported here serve as an important database for comparison with detrital, xenocrystic, and metamorphosed mafic rock-hosted zircon populations to evaluate provenance.

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We present newly acquired trace element compositions for more than 300 zircon grains in 36 gabbros formed at the slow-spreading Mid-Atlantic and Southwest Indian Ridges. Rare earth element patterns for zircon from modern oceanic crust completely overlap with those for zircon crystallized in continental granitoids. However, plots of U versus Yb and U/Yb versus Hf or Y discriminate zircons crystallized in oceanic crust from continental zircon, and provide a relatively robust method for distinguishing zircons from these environments. Approximately 80% of the modern ocean crust zircons are distinct from the field defined by more than 1700 continental zircons from Archean and Phanerozoic samples. These discrimination diagrams provide a new tool for fingerprinting ocean crust zircons derived from reservoirs like that of modern mid-ocean ridge basalt (MORB) in both modern and ancient detrital zircon populations. Hadean detrital zircons previously reported from the Acasta Gneiss, Canada, and the Narryer Gneiss terrane, Western Australia, plot in the continental granitoid field, supporting hypotheses that at least some Hadean detrital zircons crystallized in continental crust forming magmas and not from a reservoir like modern MORB.

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