Retrieving sea-wave spectra using satellite-imagery spectra in a wide range of frequencies

A method to register sea-wave spectra using optical aerospace imagery has been developed. The method is based on the use of retrieval operators both in areas of high and low spatial frequencies, including the areas of spectral maximum. The approach to adjust and validate the method developed using sea truth data obtained by string wave recorders has been suggested. This paper presents the results of using the suggested method to study sea-wave spectra using high-resolution satellite imagery for various water areas under different conditions of wave generation.     

白令海夏季浮游植物的群落结构与时空变化

通过1999年和2010年夏季同期7月在白令海(169°E~166°W,50°N~67°N)获取的94份浮游植物样品分析,获得了近十年的始末两个时间节点的浮游植物群落结构与时空变化,探讨了浮游植物群落动态及其与环境因素的关联。研究结果显示,共鉴定浮游植物(>10μm)5门58属153种,分为3个生态类群。硅藻是浮游植物的主体,种类多丰度高,占总种类数目的66.7%,占总丰度的95.2%。鉴于样品属性和空间范围的不同,物种组成有细微差别,丰度有较大差异且空间分布明显不同,高丰度区受控于上层营养盐供给和表层环流系统。优势种从北方温带大洋性硅藻演变为广温广盐性与冷水性硅藻,1999年以西氏新细齿状藻为第一优势种,柔弱伪菱形藻次之;2010年以丹麦细柱藻为第一优势种,冷水性的诺登海链藻次之并在陆架和陆坡占优。浮游植物群落结构较为稳定,由深水群落和浅水群落组成。深水群落分布于太平洋西北部和白令海盆,种类组成以温带大洋性的西氏新细齿状藻、长海毛藻、大西洋角毛藻和广布性的菱形海线藻、扁面角毛藻、笔尖根管藻为主,丰度低,种间丰度分配均匀,优势种多元化,物种多样性高;浅水群落分布于白令海陆坡和陆架,主要由冷水性的诺登海链藻、叉尖角毛藻、聚生角毛藻和广布性的丹麦细柱藻、旋链角毛藻组成,丰度高,种间丰度分配不均匀,优势种突出,物种多样性低。白令海夏季浮游植物种类组成及丰度变化直接受控于表层环流、营养盐、春季冰缘线等环境因素。     

利用父母本微卫星标记估计大菱鲆(Scophthalmus maximus L.)幼鱼生长性状的遗传参数

The estimation of genetic parameters has played an important role in animal selective breeding for growth traits.Recently studies show that molecular markers can be incorporated into genetic evaluations. In order to improve the performance of an incomplete pedigree(i.e, only parents are known) in the genetic evaluations, 12 microsatellite markers have been applied in the estimation of the genetic parameters for body weight in a farmed population(n=1 890) of juvenile turbot(Scophthalmus maximus L.). A new relatedness called parental molecular relatedness(PMR) is estimated based on results of genotyping of 48 parents(31 males, 17 females) with microsatellites markers. The feasibility of PMR in estimation of genetic parameters is verified by comparison with pedigree related(PR) which is obtained from a complete pedigree. The results demonstrate that a high correlation(0.872) between them is found. Heritabilities are estimated using the PMR(0.52±0.13) and PR(0.55±0.22) with the same animal model. A cross-validation shows that the predictive abilities of models using the PMR and the PR are identical(0.81). From that, a conclusion can be made that PMR and PR predicted genetic values equally well in a population of juvenile turbot. Therefore PMR can be applied as an alternative of the PR when only parents are known. However, for a better performance, more markers and more families should be included in a further study.     

低分子质量褐藻寡糖的高效酶法制备及其抗氧化活性评价

褐藻寡糖具有多种生理活性,本研究通过酶解与分级条件的优化,获得了低分子质量褐藻寡糖的酶法制备工艺,并在体外模型上评价了不同分子质量组分的抗氧化活性。结果表明,优化后的褐藻寡糖制备条件为:底物浓度1.20%,酶底比4.35 U/mg,酶解时间4 h。进一步采用乙醇沉淀和超滤分离后,获得了重均分子质量分别为0.84、1.40、2.25和34.56 k Da的4种组分,其得率分别为50.82%、5.15%、11.48%和12.00%。各组分均具有一定的还原能力,可有效清除DPPH和羟自由基,其中低分子质量组分A的抗氧化活性最为显著,其清除羟自由基的能力与维生素C相近。     

高效液相色谱-离子阱质谱法测定海洋微藻藻粉中的8种脂溶性毒素

建立了利用高效液相色谱-电喷雾离子阱质谱(HPLC-ESI-IT-MS)测定海洋微藻藻粉中8种典型脂溶性毒素的分析方法。藻粉样品经超声细胞破碎后,采用超声波辅助提取法对藻毒素进行提取,用HPLC-ESI-IT-MS多反应离子监测(MRM)模式对各种毒素(包括大田软海绵酸(OA)、鳍藻毒素1(DTX-1)、扇贝毒素2(PTX-2)、虾夷扇贝毒素(YTX)、原多甲藻酸1(AZA1)原多甲藻酸2(AZA2)、罗环内酯毒素(SPX),米氏裸甲藻毒素(GYM))进行测定。8种脂溶性藻毒素均在线性范围内线性关系良好(R2均在0.991以上),检出限均介于0.085～1.315 pg之间,加标回收率在88.5%～111.4%之间,方法重复性相对标准偏差(RSD)在4.82%～10.17%范围。应用该方法对利玛原甲藻干藻粉中的毒素进行了测定,分析结果良好,说明本方法是海洋微藻藻粉中脂溶性藻毒素测定的有效方法。     

杜氏盐藻生长及PSⅡ对不同磷源的响应

在实验室控制条件下,研究了无机磷磷酸二氢钠(NaH_2PO_4)及3种有机磷源三磷酸腺苷二钠盐(adenosine disodium triphosphate,ATP)、β-甘油磷酸二钠(sodiumβ-glycerophosphate,G-P)和D-葡萄糖-6-磷酸(D-Glucose 6-phosphate,D-G-6-P)对杜氏盐藻(Dunaliella salina)生长及PSII系统的影响。结果表明,杜氏盐藻在ATP和NaH_2PO_4的磷环境中生长迅速,最大比生长速率(μ_(max))分别为(0.736±0.0158)/d和(0.667±0.0553)/d;而β-甘油磷酸二钠和D-葡萄糖-6-磷酸培养条件下盐藻生长则具有滞后效应,μ_(max)分别为(0.232±0.0114)/d和(0.31±0.0077)/d。ATP和NaH_2PO_4作为磷源时,盐藻最大电子传递效率(ETR_(max))和最大饱和光强(I_k)显著高于β-甘油磷酸二钠和D-葡萄糖-6-磷酸处理组(P0.05),而NPQ则呈相反。JIP-test参数可知,单位反应中心吸收的光能(ABS/RC)、t=0时单位反应中心捕获的用于还原QA的能量(TR_0/RC)和最大光化学效率(Φ_(P0))在各组间差异不显著(P0.05),但β-甘油磷酸二钠和D-葡萄糖-6-磷酸处理组单位反应中心耗散掉的能量(DI_0/RC)显著增加(P0.05),ψ_0和Φ_(E0)显著降低(P0.05)。表明β-甘油磷酸二钠和D-葡萄糖-6-磷酸作为磷源时盐藻光合系统反应活性中心(RC)部分关闭,反应活性中心的数量(RC/CS_0)减少,PSⅡ受体侧电子传递受到影响,能量耗散效率提高。综上可知,杜氏盐藻均能利用无机磷和有机磷作为磷源供其生长,但ATP作为磷源使得盐藻在最短时间进入对数期,生物量显著提高(P0.05)。     

渤海湾曹妃甸深槽海区地形地貌特征及控制因素

通过研究浅层地震剖面、侧扫声纳和水深地形等数据资料,得出,曹妃甸沙岛的岬角地貌引起深槽海域局部潮流流速增大,甸头前沿深槽区以冲刷为主,最大水深达42 m,刷新了渤海湾最大水深记录,深槽部位的侵蚀量最大,深槽南坡冲刷幅度大于北坡,工程建设后期深槽区侵蚀冲刷程度有变小变缓趋势。早期深槽的形成是由于浅部断层受深部构造影响发生阶梯状错断沉陷,海底地层形成古凹槽,但深槽海底地层沉陷速率略大于沉积速率,使得深槽海域长期保持了渤海湾最大的水深环境。初步得出在历史时期曹妃甸深槽经过2万a以上长期存在,深槽的走向经历了南北向-北东向-北西向的转化过程。认为地质构造、古滦河三角洲演变、海洋水动力作用和人类活动等内外营力作用共同控制了曹妃甸海区地貌体系的发育与演化。达到了研究渤海湾曹妃甸深槽海区地形地貌控制因素和深槽的地质演化的目的,为曹妃甸港的规划、运营期维护和未来发展提供科学依据具有重要意义。     

Zonal REE + Y profiles in garnet and their genetic implications: A case study of metapelites from the northern Ladoga region

The objective of this study is to provide insights into the REE and Y behavior during garnet porphyroblast formation in staurolite-bearing schists as a constituent of Late Paleoproterozoic metapelites of the Ladoga Complex. The MnNCKFMASH P–T pseudosection for a single sample and Grt–Bt thermometry indicate that the garnet core grew at 520°C and under 7.0–7.2 kbar in the Grt–Bt–Pl–Chl–Ms–Zo field, whereas the garnet rim was equilibrated at 590–600°C and under 3.5–4.0 kbar. The measured zoning profiles are strongly depleted in REE + Y in the garnet core containing high Mn and Ca concentrations. The intermediate zone of garnet is enriched in La, Ce, Pr, and Nd (inner LREE + Nd annulus), as well as in Dy, Er, Yb, Lu, and Y (outer HREE + Y + Dy annulus). According to pseudosection analysis, these peaks were probably produced owing to breakdown of epidote-group minerals (allanite, REE-rich epidote) at T < 535°C and P > 6.5 kbar. Towards the rim, the HREE + Y contents gradually decrease, whereas MREE (Sm, Eu, Gd) display an inverse trend. The rim also exhibits a negative Eu anomaly. The former tendency reflects an increase in temperature during garnet crystallization and partitioning of elements between garnet and monazite. It is thought that the latter is linked to oppositely directed change in garnet-monazite partition coefficients for HREE and MREE with increasing temperature.     

Scanning electron microscopy and Raman spectroscopy as combined methods for studying zoning in minerals: The case of spinels from Archean komatiites

Several types of both magmatic and metamorphic spinels have been found in Archean komatiites of the Sovdozero and Kostomuksha greenstone belts in the eastern part of the Fennoscandian Shield. Scanning electron microscopy and Raman spectroscopy revealed relics of cores of primary magmatic chrome-spinels with high Cr and Al contents. In the Sovdozero structure, the relics are better retained than those in the Kostomuksha structure, which is caused by a different degree of metamorphic transformation. The comparable 100 · Cr/(Al + Cr) values of spinel cores from Sovdozero and Kostomuksha reflect similar conditions of partitional melting in the mantle. These data agree with the fact that both komatiite complexes belong to the Al-undepleted petrogenic type. Wide variations in the Cr and Al contents in primary chrome-spinel cores together with a constant Mg/(Fe²⁺ + Mg) ratio correspond to low oxygen fugacity during magma crystallization. In general, the composition of these primary chrome-spinels is similar to that of accessory phases in peridotites from suprasubduction zones and agrees with hypothesis of komatiite complex formation in back-arc basins.     

Suprathermal ions in solar-wind outflows from coronal holes at 1 AU

The energy spectra and relative abundances of ³He, ⁴He, C, O, and Fe ions with energies of ~0.04–2 MeV/nucleon are studied using data from the ULEIS instrument on board the ACE spacecraft obtained during quiescent periods in 2006–2012. During the unique, prolonged minimum between cycles 23 and 24, 35 quiescent periods were distnguished, during which solar-wind flows from near-equatorial coronal holes (CHs) were detected. It is shown that the C/O and Fe/O ratios for suprathermal ions correspond to the relative abundances of the corresponding thermal ions in the fast and slow (Maxwellian) solar wind (SWICS/ACE), while the ⁴He/O ratio exceeds the corresponding ratio in the solar wind by a factor of two. The intensities of the ³He, ⁴He, C, O, and Fe suprathermal ions in outflows from CHs grow with the speed of the solar wind. This indicates that, in periods ofminimumsolar activity, suprathermal ions from CHs represent a high-temperature “tail” of the solar wind. An additional flux of suprathermal helium ions may also be contributed by other external sources.