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By means of contrasted immobilization of denitrifying bacterium on several kinds of carbon fibers, the effect of physical and chemical characteristics such as specific surface area, precursor and recycle, especially the surface oxygenic functional group on these carbon fibers was investigated.

通过对比反硝化菌在不同基体碳纤维表面的固着化及碳纤维表面含氧官能团对菌种的固着化实验,研究了碳纤维(基体、比表面积、循环利用性等)特性,尤其表面含氧官能团对反硝化菌固着化的影响。

The results of analysis showed that the DBD was more suitable for oxidizing carbon black than RF. Because carbon black oxidized by DBD had a lot of single oxygenous functional group,carboxyl,which could be used to graft antitumour medicine and could be well dispersed in water.

通过对氧化后炭黑性能的分析测试得出以下结论:DBD 工艺优于RF 工艺,经DBD 氧化改性的纳米炭黑含氧官能团多,官能团单一,在水中的分散稳定性良好,为高选择性地进行药物接枝反应创造了条件。

In order to solve these problems, first, activated carbon which was deashed by hydrochloride was modified through using concentrated sulfuric acid, concentrated nitric acid, hydrogen peroxide and potassium permanganate in the paper, the result showed that the modification of activated carbon is best through using concentrated sulfuric acid under 250℃ through analyzing the desulfurization efficiency and acidic oxygenous group on surface.

对上述问题,本文首先采用浓硫酸、浓硝酸、双氧水和高锰酸钾等氧化剂对盐酸脱灰后的活性炭进行化学改性,通过对改性活性炭的脱硫效果及其表面酸性含氧基团分析,得出在250℃的温度下采用浓硫酸改性活性炭效果最好。

Carbon fiber is very effective in improving the impact strength of copper-graphite composites. The short carbon fiber reinforced cooper-graphite composite can be used to produce pantagraph slider of high performance.

试验证明,短炭纤维对於提高铜-石墨复合材料的冲击值非常有效,短炭纤维增强铜-石黑复合材料可用於制造高性能受电弓滑板。

By 16S rRNA. When it was cultured in MMSW substrate, adding MWFO and SWFO as the carbon source, it could produce crude biodemulsifier of 4 g/L and 3.5 g/L respectively. Compared with biodemulsifier produced by paraffine as the carbon source, both of them could achieve higher demulsification ratio in breaking W/O and O/W model emulsion.

的一株破乳剂产生菌,在以废弃油脂MWFO、SWFO为碳源培养下,得到的生物破乳剂的粗重为4 g/L、3.5 g/L;对于W/O、O/W模型乳状液的破乳效果均可超过以液体石蜡产生的破乳剂,且以SWFO废弃油脂培养得到的生物破乳剂可以同时应用于两种模型乳状液的使用。

The results reveal that transformation from amorphous white carbon black to crystalline occurs at high temperature.And the transformation temperature of the pelleted particles is 80℃ lower than that of the white carbon black powder.

结果表明,白炭黑在高温下发生了非晶向晶态的转变,喷雾造粒白炭黑微球的转变温度比白炭黑粉末低80℃。

Carbon dioxide is 'fixed' by combination with the 5-carbon sugar ribulose bisphosphate,forming two molecu- les of phosphoglyceric acid.

光合作用的暗反应发生在叶绿体基质中,来自于光反应的 ATP和 NADPH被用来将CO2还原成糖类。

In order to improve the electrocatalytic activity of the anode in the Direct Methanol Feul Cell, three kinds of transition metal substituted phosphomolybdic acid modified platinum electrodes were prepared, and the electrochemical behavior in the sulphuric acid solution of transition metal substituted phosphomolybdic acid modified platinum electrodes and their electrocatalytic effects of methanol oxidation were studyed. The anti-poison effect to carbon monoxide of the prepared electrodes were studied by the carbon monoxide adsorbing.

为了提高直接甲醇燃料电池阳极催化活性,本文研究了三种过渡金属取代磷钼酸修饰铂电极在硫酸溶液中的电化学行为及对甲醇的电催化氧化作用,并利用一氧化碳吸附实验评价了三种过渡金属取代磷钼酸修饰铂电极的抗一氧化碳毒化性能。

Because the photospheric temperature of carbon stars are less than 3000K and the temperature of rich-dust envelope formed by the mass loss is lower, and therefore most of the energy from carbon stars are radiated between 1 to 60um range, in which the vibrational and ro-vibrational bands of many molecules also lies, the study of infrared spectra in this wavelength range is very important to reveal chemical compositions, dust formation process, the atmospheric structure and evolutionary status of stars.

碳星光球的有效温度不超过3000K,同时较大的质量损失率形成了富碳的尘埃壳层,以致于它的辐射能量主要集中在1—60μm的红外波段上,并且许多分子的转动振动能谱也集中在红外,因此在红外波段的研究对揭示碳星化学成份及其分布、尘埃形成过程、恒星大气结构和演化状态都有十分重要的意义。

Visual carbon stars whose mid-infrared spectra are mainly dominated by photospheric continuum and show large excesses at 60um, represent a transition phase which follows an interruption of mass loss from the oxygen-rich phase and begins a new phase of the mass loss of carbon-rich material. Excesses at 60um in these stars are the emission from the residual of oxygen-rich material.

光学碳星的中红外能量主要来自光球,在60μm处存在超量发射,人们认为其演化阶段处在抛射富氧物质终止和新的富碳拱星壳层形成之间,其60μm超量发射就是富氧物质的残余效应。

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