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101.
光照强度对海洋微藻脂肪含量及脂肪酸组成影响的研究   总被引:1,自引:0,他引:1  
近年来,海洋微藻脂肪酸组成的研究及其应用越来越受到国内外科学家的重视。高度不饱和脂肪酸(PUFA),特别是长链的n-3 PUFA,如二十碳五烯酸(EPA)和二十二碳六烯酸(DHA)对海洋动物和人类都具有营养学和医学上的价值。在海洋微藻的培养过程中,光照强度是海洋微藻生长的条件之一,光线的明与暗,光度的强与弱,不仅对微藻的生长速率、产量有影响,而且对其脂肪含量和脂肪酸的组成也有影响(Teshima et al.,1983;Thompson et al.,1990; Renaud et al., 1991)。 作者在以往研究的基础上,选择了3种有代表性的海洋微藻:(1)小球藻Chlorella sp-2(李荷芳等,1999),此藻脂肪酸中EPA含量高、且不含DHA;(2)球等鞭金藻(Isochrysis galbana),该藻DHA含量较高,但几乎不含EPA;(3)前沟藻(Amphidinium sp.)的EPA、DHA含量均高。将以上3种微藻作为原料,在不同的光照强度下进行培养,测定并分析藻体中的脂肪含量和脂肪酸组成的变化,从而了解光强对海洋微藻脂肪含量及其脂肪酸组成的影响。  相似文献   
102.
Wave measurement based on light refraction   总被引:2,自引:0,他引:2  
Some authors have developed a few methods of measuring wave slopes based on light refraction, including the measurement method via the distribution of light intensity or color under water. A new method based on light refraction is specified for the measurement of wave surface elevation in wave flume via imaging technology. A plane painted with black and white stripes is put on the flume floor as an indication plane, which can be arranged easily and cheaply. Compared with the previous methods, the present method is less sensitive to the noise and nonlinear effects of optical process, which can be taken as a digital method. The CCD camera is fixed above the flume with its optical axis arranged vertically to grab the images of stripes modulated by the wave surface. The modulated value can be calculated from the Hilbert transform, and then the wave surface elevation can be obtained. The algorithm and experimental procedure are specified in detail, and some experimental results are provided to show the validity of the present method.  相似文献   
103.
礁膜配子放散条件的研究   总被引:2,自引:0,他引:2  
陈昌生 《台湾海峡》1996,15(2):154-158
本文报道了礁膜配子的放散与温度、光照、比重的关系。结果表明,自然海区的礁膜在白天大量放散配子。配子放散的适宜温度为19-21℃;光照为2000-5000lx时能促进配子大量放散出来;配子放散的适宜比重为1.05-1.025;这些研究结果将为礁膜人工育苗提供一些科学依据。  相似文献   
104.
基于夜间灯光数据的南京城镇用地提取   总被引:1,自引:0,他引:1  
针对多时相夜间灯光影像无法直接对比的问题,该文提出了一种基于不变目标进行不同年份不同卫星夜间灯光数据的校正方法。在系统校正多时相夜间灯光数据的基础上,应用支持向量机分类算法提取城镇用地信息,并分析1992—2013年南京城镇扩张动态变化规律。结果表明:该数据校正方法可以有效减少年际夜间灯光影像之间的异常差异,提高不同年份数据间的连续性和可比较性;支持向量机分类算法提取的4个样区城镇用地信息总体精度和Kappa系数平均值分别为88.35%和0.56,能够准确反映区域城镇发展的实际情况;1992—2013年南京城镇经历先缓慢后快速的扩张过程,主城区在1992年城镇基础上往四周扩张,并沿长江及南北交通走廊发展。  相似文献   
105.
The effect of self‐shading and competition for light in the seagrass Enhalus acoroides were investigated with a density reduction experiment in Haad Chao Mai National Park, Trang Province, Thailand. The study was carried out in a monospecific meadow with a natural density of 141.0 ± 8.7 shoots·m?2. The intent was to determine the response of E. acoroides beds to loss of shoots and thinning, which often occur during typhoons and severe storm activity. Permanent quadrats were manipulated by clipping the seagrass shoots to 140, 72, 36 and 16 shoots·m?2, to yield natural, 50%, 25% and 10% densities, respectively. Reducing shoot density in E. acoroides increased underwater light intensity below the canopy, generating increased leaf surface area and shoot weight. Seagrass leaf width, growth rate, and number of leaves per shoot also increased with greater light. The extent of flowering varied among treatments with no consistent trend. Our results demonstrate that increasing the available light to E. acoroides produces an increasing leaf size response as self‐shading in the bed is reduced.  相似文献   
106.
在实验室条件下,对大连蜈蚣藻(Grateloupia dalianensis H.W.Wang et D.Zhao)的孢子早期发育、盘状体的形成和直立枝生长进行了详细研究,对其生活史进行了详细观察,并进行了温度和光照强度对孢子发育影响的研究。结果表明:(1)孢子发育类型为间接盘状体型;(2)生活史由雌、雄配子体、四分孢子体和果孢子体三相世代组成,配子体与孢子体形态相同,属于同型世代交替,与属模蜈蚣藻(G.filicina)一致;(3)温度对盘状体和直立枝生长均有影响,最适温度均为16℃;(4)光照强度对盘状体和直立枝生长均有影响,最适光照强度分别为7 500 lx和10 000 lx。  相似文献   
107.
This paper gives the result of photographic photography of the central star AGK3-0° 695 of the planetary nebula NGC 2346 made from 1981 through 1987. From it we see that after the large-amplitude eclipses which had started at the end of 1981 had continued for several years, the amplitude began to decrease rapidly in 1986 to ˜1.1 mag from ˜4 mag in 1984. In 1987, only irregular fluctuations with amplitudes ˜0.4 mag were present in the light curve and not longer any clear periodicity. A preliminary analysis of this phenomenon is carried out here.  相似文献   
108.
本文分析了南京大学太阳塔1991年10月24日用多波段光谱仪观测到的高时间分辨率(5s)的一个2N/X2.1级白光耀斑光谱.对耀斑谱线轮廓、连续发射强度、X射线和射电爆发资料进行了综合对比,分析表明,该耀斑属Ⅰ类白光耀斑,具有如下特征:(1)在白光耀斑的脉冲相期间,各波段光谱线心强度、连续辐射、谱线半宽以及线翼红不对称性与硬X射线高能波段的爆发同时达到极大;(2)H_a谱线在连续发射极大时半宽达10A,且呈现强烈的线心反转,H_β和H_γ线心亦有反转;(3)所拍摄的5条谱线都有明显的红不对称性,持续时间约为1分钟,根据上述结果,本文用电子束轰击、色球蒸发和色球压缩区对该耀斑能量积聚和释放的动力学机制作了定性的分析和解释。  相似文献   
109.
The effect of light intensity ( 1500 Ix and 5000 Ix) on the total lipid and fatty acid composition of six strains of marine diatoms Cylindrotheca fusiformis (B211 ), Phaeodactylum tricornutum (Bl14, Bl18 and B221) Nitzschia closterium (B222) and Chaetoceros gracilis (B13) was investigated.The total lipids of B13, Bl14, and B211 grown at 5000 Ix were lower than those grown at 1500 Ix. No evident changes were observed in Bl18, B221 and B222. Fatty acid composition changed considerably at different light intensity although no consistent correlation between the relative proportion of a single FA and light intensity. The major fatty acids of the 6 strains were 14:0, 16:0, 16:l(n- 7) and 20:5(n-3) . Cylindrothecafusiformis had high percentage of 20:4n - 6 (9.2 - 10.9% ) . The total polyunsaturated fatty acid /rl all 6 strains decreased with increasing light intensity. The percentage of the highly unsaturated fatty acid eicosapentaenoic acid (EPA) decreased with increasing light intensity in all strains except Chaetoceros gracilis.  相似文献   
110.
About a dozen physical mechanisms and models aspire to explain the negative polarization of light scattered by atmosphereless celestial bodies. This is too large a number for the reliable interpretation of observational data. Through a comparative analysis of the models, our main goal is to answer the question: Does any one model have an advantage over the others? Our analysis is based on new laboratory polarimetric and photometric data as well as on theoretical results. We show that the widely used models due to Hopfield and Wolff cannot realistically explain the phase-angle dependence of the degree of polarization observed at small phase angles. The so-called interference or coherent backscattering mechanism is the most promising model. Models based on that mechanism use well-defined physical parameters to explain both negative polarization and the opposition effect. They are supported by laboratory experiments, particularly those showing enhancement of negative polarization with decreasing particle size down to the wavelength of light. According to the interference mechanism, pronounced negative branches of polarization, like those of C-class asteroids, may indicate a high degree of optical inhomogeneity of light-scattering surfaces at small scales. The mechanism also seems appropriate for treating the negative polarization and opposition effects of cometary dust comae, planetary rings, and the zodiacal light.  相似文献   
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