5,806 research outputs found

    From Veldt Camp Fires Stories of South Africa

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    https://commons.und.edu/settler-literature/1179/thumbnail.jp

    Trifloxystrobin based seed treatment fungicides control seed rot and pre-emergence damping-off of canola, pulses, and corn

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    Non-Peer ReviewedActive ingredient Trifloxystrobin belongs to the strobilurin class of fungicides which possess improved safety and environmental characteristics. The objective of this research was to evaluate the efficacy of seed treatment fungicides based on Trifloxystrobin to control seed rot and pre-emergence damping off of canola, pulses, and corn crops. In 2004-2006, canola, pulses, and corn trials were conducted in Saskatchewan (Aberdeen, Allan, Indian Head, and Wakaw), Alberta (Vegreville), and Manitoba (High Bluff). The experimental design used was a randomized complete block design with four replications. Seed treatments fungicide tested were Trilex FL (trifloxystrobin [10g]/100 kg of seed); Trilex AL (trifloxystrobin [5g] + Allegiance FL (metalaxyl) [4g]/100 kg of seed); and Trilex FL (trifloxystrobin [5g]/100 kg of seed) tank mixed with Allegiance FL (metalaxyl) [2g]/100 kg of seed) Plants were counted at 14 to 28 days after planting. Data were analyzed using an ANOVA. Trifloxystrobin based seed treatment fungicides possessed excellent efficacy for controlling seed rot and pre-emergence damping-off of canola, pea, lentil, chickpea, and corn crops grown in soils infected with Rhizoctonia solani or Fusarium avenaceum

    Boers and Beasts of the Cape

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    https://commons.und.edu/settler-literature/1178/thumbnail.jp

    Calculation of the aerodynamic characteristics of tapered wings with partial-span flaps

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    Factors derived from wing theory are presented. By means of these factors, the angle of zero lift, the lift-curve slope, the pitching moment, the aerodynamic-center position, and the induced drag of tapered wings with partial-span flaps may be calculated. The factors are given for wings of aspect ratios 6 and 10 , of taper ratios from 0.25 to 1.00, and with flaps of various length. An example is presented of the method of application of the factors. Fair agreement with experimental results is shown for two wings of different taper ratio having plain flaps of various spacing

    Soil treatments and seasonal changes in the sour cherry

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    Publication authorized September 21, 1927.Digitized 2007 AES.Includes bibliographical references

    CORRELATION BETWEEN IMPAIRMENT AND MOTOR PERFORMANCE DURING REACHING TASKS IN SUBJECTS WITH SPASTIC HEMIPARESIS

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    Objective: The main purposes of this study were to examine, in subjects with chronic hemiparesis following a stroke: (i) the correlations between tests of muscle tone, stiffness, spasticity, paresis and co-contraction, and (ii) the correlations of these tests and measurements of impairment to upper extremity motor performance. Design: Prospective, cross-sectional, correlation matrix using sample of convenience. Subjects: Thirteen subjects with chronic hemiparesis secondary to a cerebrovascular accident (stroke) were tested. Methods: Subjects were assessed using the Fugl-Meyer Upper Extremity Motor Assessment, modified Ashworth scale, deep tendon reflexes, and muscle characteristics that included quantification of muscle stiffness, paresis and co-contraction during a voluntary reaching task and during passive movements. Surface electromyographic and myotonometric muscle stiffness data were obtained during movement trials. Results: Biceps and triceps brachii muscle paresis and excess biceps brachii co-contraction during voluntary reaching had the highest correlations to decreased motor performance. Muscle tone measurements did not have significant correlations to upper extremity performance. Conclusion: Paresis of elbow flexors and extensors and excess co-contraction of the biceps brachii during voluntary reaching appear to be most predictive of upper extremity motor performance. Results are discussed in relation to the specific challenges these findings pose for spastic paresis clinical management

    The NASA-UC Eta-Earth Program: III. A Super-Earth orbiting HD 97658 and a Neptune-mass planet orbiting Gl 785

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    We report the discovery of planets orbiting two bright, nearby early K dwarf stars, HD 97658 and Gl 785. These planets were detected by Keplerian modelling of radial velocities measured with Keck-HIRES for the NASA-UC Eta-Earth Survey. HD 97658 b is a close-in super-Earth with minimum mass Msini = 8.2 +/- 1.2 M_Earth, orbital period P = 9.494 +/- 0.005 d, and an orbit that is consistent with circular. Gl 785 b is a Neptune-mass planet with Msini = 21.6 +/- 2.0 M_Earth, P = 74.39 +/- 0.12 d, and orbital eccentricity 0.30 +/- 0.09. Photometric observations with the T12 0.8 m automatic photometric telescope at Fairborn Observatory show that HD 97658 is photometrically constant at the radial velocity period to 0.09 mmag, supporting the existence of the planet.Comment: Submitted to ApJ, 7 pages, 6 figures, 5 table

    Observational constraints on the progenitor metallicities of core-collapse supernovae

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    We present constraints on the progenitor metallicities of core-collapse supernovae. To date, nearly all metallicity constraints have been inferred from indirect methods such as metallicity gradients in host galaxies, luminosities of host galaxies, or derived global galaxy metallicities. Here, progenitor metallicities are derived from optical spectra taken at the sites of nearby supernovae, from the ratio of strong emission lines found in their host HII regions.We present results from the spectra of 74 host HII regions and discuss the implications that these have on the nature of core-collapse supernova progenitors. Overall, while we find that the mean metallicity of type Ibc environments is higher than that of type II events, this difference is smaller than observed in previous studies. There is only a 0.06 dex difference in the mean metallicity values, at a statistical significance of ~1.5 sigma, while using a KS-test we find that the two metallicity distributions are marginally consistent with being drawn from the same parent population (probability >10%). This argues that progenitor metallicity is not a dominant parameter in deciding supernovae type, with progenitor mass and/or binarity playing a much more significant role.Comment: ACCEPTED for publication in MNRA
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