提高生物拮抗菌对果实采后病害的生防效力研究

摘要 　　"随着人们对身体健康和环境污染的日益重视，化学农药作为控制果实采后病害的主要方法受到了很大限制，科学研究者不得不寻求更加安全有效的防治果实采后病害的新方法。生物防治以其对环境和人类健康不造成危害的优点而逐渐受到人们的青睐。然而，由于生物防治是以活菌为基础，有其局限性和时效性，单独使用拮抗菌很难达到化学药剂完全控制果实采后病害的效果，因此，提高拮抗菌的生防效力成为当今生物防治领域的研究重点。本文主要研究了拮抗菌与不同外源物质配合使用的抑病效果及协同抑病机理;拮抗菌对采前田间和采后贮藏环境条件的适应能力;以及采前应用拮抗菌对果实采后贮藏期间病害的生物防治效力。研究结果表明： 　　1、酵母拮抗菌Cryptococcus laurentii与低浓度化学杀菌剂imazalil（25g/ml）和kresoxim-methyl（50g/ml）配合使用可以显著提高对冬枣果实采后黑霉病（Alternaria alternata）和褐腐病（Monilinia fructicola）的防治效果，杀菌剂并不影响拮抗菌在冬枣果实伤口的生长动态。 　　2、酵母拮抗菌Pichia membranefaciens和C. laurentii 与钼酸铵（NH4-Mo，5 mmol/L）和碳酸氢钠（NaHCO3，2%）配合能够显著提高对甜樱桃果实采后褐腐病（M. fructicola）的抑病能力。通过in vitro和扫描电镜观察结果表明，NH4-Mo和NaHCO3能够显著地抑制病原菌M. fructicola在培养基和果实伤口的生长，具有杀菌作用。 　　3、酵母拮抗菌C. laurentii和Rhodotorula glutinis与硅酸钠（Na2SiO3）配合使用对甜樱桃果实采后青霉病（Penicillium expansum）和褐腐病（M. fructicola）以及对冬枣果实青霉病（P. expansum）和黑霉病（A. alternata）的防治效果更好。经in vitro和扫描电镜观察表明，Na2SiO3对病原菌在培养基和果实伤口的生长有明显的抑制作用。同时，Na2SiO3还能诱导果实苯丙氨酸解氨酶（PAL）、多酚氧化酶（PPO）和过氧化物酶（POD）等抗性相关酶活性的提高。 　　4、酵母拮抗菌R. glutinis与水杨酸（SA，0.5mmol/L）配合可显著提高对甜樱桃果实采后青霉病（P. expansum）和黑霉病（A. alternata）的抑病能力。SA不影响拮抗菌在果实伤口的生长，in vitro实验中低浓度的SA对病原菌孢子萌发和芽管伸长也没有抑制作用。SA可能是通过诱导果实产生抗性来协同提高拮抗菌的抑病效果，而不是直接抑制病原菌生长。 　　5、酵母拮抗菌C. laurentii和R. glutinis在气调（Controlled atmospheres, CA）贮藏条件下对樱桃果实采后青霉病（P. expansum）和黑霉病（A. alternata）的防治效果显著提高。气调贮藏不抑制拮抗菌在甜樱桃果实伤口的生长。 　　6、采前应用酵母拮抗菌C. laurentii 和R. glutinis能够显著抑制甜樱桃果实在采后不同贮藏环境下的发病率。拮抗菌能够在田间果实表面生长并一直保持较高的数量。在试验的三种酵母拮抗菌中，C. laurentii的防病效果最好，该菌不仅能在果实表面迅速生长，也能适应低温和CA贮藏环境。"

Distribution, transformation, and long-term accumulation of polychlorinated dibenzo-p-dioxins and dibenzofurans in different tissues of fish and piscivorous birds

The present study monitored 10-year-old fish and piscivorous birds from sites contaminated for many Stars. The data reflected the results of actual, long-term environmental exposures, The results demonstrate that different tissues of fish have quite different concentrations of polychlorinated dibenzo-p-dioxins and dibenzofurans (PCDD/F), The concentration order of PCDD/F within fish is liver congruent to egg congruent to intestines kidney congruent to hearts gill congruent to bladders > muscle > brain. The concentration order of PCDD/F within piscivorous birds was livers egg congruent to hearts muscle congruent to stomachs brain, The results obtained also demonstrate that the accumulation patterns of piscivorous birds and fish are quite different. The tissues of fish and piscivorous birds have different capacities for bioaccumulation and biotransformation of PCDD/F; variable proportions of TEQs were also found throughout their bodies. In fish, toxic equivalency quotient (TEQ): PCDD/F ratios in various tissues ranged from 0.01 to 0.07, whereas in birds the ratios ranged from 0.07 to 0.43. If the concentrations are normalized with lipid content, the results vary less. The effect of different lipid properties is obvious in the case of brain tissue, which is richer in phospholipids. (C) 2000 Academic Press.

Metal alloy and monoelemental nanoclusters in silica formed by sequential ion implantation and annealing in selected atmosphere

The preparation of metal alloy and monoelemental nanoclusters in silica by Ag, Cu ion sequential implantation and annealing in selected oxidizing or reducing atmosphere is studied. The formation of metastable Ag-Cu alloy is verified in the as-implanted samples by optical absorption spectra, selected area electron diffraction and energy dispersive spectrometer spectrum. The alloy is discomposed at elevated annealing temperature in both oxidizing and reducing atmospheres. The different effects of annealing behaviors on the Ag Cu alloy nanoclusters are investigated. (C) 2004 Elsevier B.V. All rights reserved.

Influence of ambient atmosphere on the plasmon resonance absorption of Ag/SiOx(0 <= x <= 2) nanocomposite film

Nanocomposite films consisting of nanosized Ag particles embedded in partially oxidized amorphous Si-containing matrices were prepared by radio frequency magnetron co-sputtering deposition. We studied the influence of ambient atmosphere during the preparation and heat-treatment of Ag/SiOx (0 less than or equal to x less than or equal to 2) nanocompositefilm on its optical absorption properties. We found that the plasmon resonance absorption peak shifts to shorter wavelengths with the increasing oxygen content in the SiOx matrix. The analysis indicates that the potential barrier between Ag nanoparticles and SiOx matrix increases with the increasing x value, which will induce the surface resonance state to shift to higher energy. The electrons in the vicinity of the Fermi level of Ag nanoparticles must absorb more energy to be transferred to the surface resonance state with the increasing x value. It was also found that the plasmon resonance absorption peaks of the samples annealed in different ambient atmospheres are located at about the same position. This is because the oxidation surface layer is dense enough to prevent the oxygen from penetrating into the sample to oxidize the silicon in the inner layer.

Ultra-dry oxygen atmosphere to protect tellurite glass fiber from surface crystallization

In this study we report on surface crystallization phenomena and propose a solution for the fabrication of long and robust tellurite glass fibers. The bulk tellurite glasses of interest were prepared by melting and quenching techniques. Tellurite glass preforms and fibers were fabricated by suction casting and rod-in-tube drawing methods, respectively. The surfaces of the tellurite bulk glass samples and of the drawn fibers prepared under different controlled atmospheres were examined by X-ray diffraction. When the tellurite glass fibers were drawn in ambient air containing water vapor, four primary kinds of small crystals were found to appear on the fiber surface, alpha-TeO(2), gamma-TeO(2), Zn(2)Te(3)O(8) and Na(2)Zn(3)(CO(3))(4)center dot 3H(2)O. A mechanism for this surface crystallization is proposed and a solution described, using an ultra-dry oxygen gas atmosphere to effectively prevent surface crystallization during fiber drawing. (C) 2010 Elsevier B.V. All rights reserved.

Simultaneous multiwavelength observations of sagittarius A

We observed Sgr A* using the Very Large Array (VLA) and the Giant Metrewave Radio Telescope (GMRT) at multiple centimeter and millimeter wavelengths on 2003 June 17. The measured flux densities of Sgr A*, together with those obtained from the Submillimeter Array (SMA) and the Keck II 10 m telescope on the same date, are used to construct a simultaneous spectrum of Sgr A* from 90 cm to 3.8 mu m. The simultaneous spectrum shows a spectral break at about 3.6 cm, a possible signature of synchrotron self-absorption of the strong radio outburst that occurred near epoch 2003 July 17. At 90 cm, the flux density of Sgr A* is 0.22 +/- 0.06 Jy, suggesting a sharp decrease in flux density at wavelengths longer than 47 cm. The spectrum at long cm wavelengths appears to be consistent with free-free absorption by a screen of ionized gas with a cutoff similar to 100 cm. This cutoff wavelength appears to be three times longer than that of similar to 30 cm suggested by Davies, Walsh, & Booth based on observations in 1974 and 1975. Our analysis suggests that the flux densities of Sgr A* at wavelengths longer than 30 cm could be attenuated and modulated by stellar winds from massive stars close to Sgr A*.

Two-component model for the interstellar scattering in direction to the Vela pulsar

This paper discusses a rigorous treatment of the refractive scintillation of pulsar PSR B0833-45 caused by a two-component interstellar scattering medium. It is assumed that the interstellar scattering medium is composed of a thin screen ISM and an extended interstellar medium. We consider that the scattering of the thin screen concentrates in a thin layer presented by a delta function distribution and that the scattering density of the extended irregular medium satisfies the Gaussian distribution. We investigate and develop equations for the flux density structure function corresponding to this two-component ISM geometry in the scattering density distribution and compare our result with that of the Vela pulsar observations. We conclude that the refractive scintillation caused by this two-component ISM scattering gives a more satisfactory explanation for the observed flux density variation of the Vela pulsar than does the single extended medium model. The level of refractive scintillation is strongly sensitive to the distribution of scattering material along the line of sight. The logarithmic slope of the structure function is sensitive to thin screen location and is relatively insensitive to the scattering strength of the thin screen medium. Therefore, the proposed model can be applied to interpret the structure function of flux density observed in pulsar PSR B0833-45. The result suggests that the medium consists of a discontinuous distribution of plasma turbulence embedded in the Vela supernova remnant. Thus our work provides some insight into the distribution of the scattering along the line of sight to the Vela pulsar.

Spatial structure of internal tidal waves generated on weak topographies

The generation of internal gravity waves by barotropic tidal flow passing over a two-dimensional topography is investigated. Rather than calculating the conversion of tidal energy, this study focuses on delineating the geometric characteristics of the spatial structure of the resulting internal wave fields (i.e., the configurations of the internal beams and their horizontal projections) which have usually been ignored. it is found that the various possible wave types can be demarcated by three characteristic frequencies: the tidal frequency, wo; the buoyancy frequency, N; and the vertical component of the Coriolis vector or earth's rotation.f. When different possibilities arising from the sequence of these frequencies are considered, there occur 12 kinds of wave structures in the full 3D space in contrast to the 5 kinds identified by the 2D theory. The constant wave phase lines may form as ellipses or hyperbolic lines on the horizontal plane, provided the buoyancy frequency is greater or less than the tidal frequency. The effect that stems from the consideration of the basic flow is also found, which not only serves as the reason for the occurrence of higtter harmonics but also increases the wave strength in the direction of basic flow. (C) 2009 Elsevier B.V. All rights reserved.