Contribución de las comunidades bentónicas en la dieta del róbalo (Eleginops maclovinus) en la Ría Deseado (Santa Cruz, Argentina)

Se analiza el aporte de la comunidad bentónica de la ría Deseado a la dieta del róbalo (Eleginops maclovinus), para contribuir al conocimiento de la trama alimentaria costera en la Patagonia austral. Entre la primavera 2005 y otoño 2006 se estudiaron las comunidades bentónicas submareales en áreas de pesca de E. maclovinus y paralelamente, se analizaron los contenidos alimentarios estomacales de róbalos provenientes de la pesca deportiva. La comunidad bentónica de planicies areno-fangosas fue dominada por poliquetos, representados principalmente por las familias Onuphidae, Orbiniidae y Maldanidae. Los crustáceos constituyeron el segundo grupo en importancia y estuvieron representados principalmente por los anfípodos gamáridos Heterophoxus sp. y Ampelisca sp. La comunidad submareal de fondos de rodados estuvo dominada por poliquetos de las familias Nereididae, Cirratulidae y Polynoidae, y los moluscos Perumytilus purpuratus y Margarites violacea. E. maclovinus presentó una dieta bentónica de tipo oportunista y generalista, con una tendencia hacia la ingesta de anfípodos gamáridos y algas clorofíceas. Durante la marea baja, la mayor contribución a su dieta la realizó la comunidad de planicies areno-fangosas submareales. Durante la marea alta, E. maclovinus se alimentó también en el intermareal rocoso, donde preda preferentemente las clorofíceas Enteromorpha spp. ENGLISH: The role of the benthic communities at Ría Deseado in the diet of the Patagonian blenny (Eleginops maclovinus) was analyzed in order to increase the understanding of the coastal food web in southern Patagonia. Subtidal benthic communities were surveyed between spring 2005 and autumn 2006 in areas of E. maclovinus sport fishing. Simultaneously, the stomach contents of patagonian blenny specimens caught during sport fishing were analyzed. The benthic community over flat sandy-muddy bottoms was dominated by polychaetes, mainly from the families Onuphidae, Orbiniidae and Maldanidae, followed by crustaceans, which were mainly represented by the gammarid amphipods Heterophoxus sp. and Ampelisca sp. The subtidal benthic community over pebbly bottoms was dominated by polychaetes from the families Nereididae, Cirratulidae and Polynoidae and the mollusks Perumytilus purpuratus and Margarites violacea. The diet of E. maclovinus was benthic opportunist and generalist, with a preference to feed on gammarid amphipods and chlorophycea algae. During low tide, the main dietary contribution came from the subtidal community over flat sandy-muddy bottoms whereas, during high tide, E. maclovinus also preyed on rocky intertidal species, mainly the Chlorophycea Enteromorpha spp.

El alga invasora Undaria pinnatifida (Harvey) Suringar en la Ría Deseado (Patagonia austral, Argentina): ciclo del esporofito y factores ambientales determinantes de su distribución

Undaria pinnatifida was registered in Ría Deseado (47º45´S, 65º55´W _ southern Patagonia) by the first time in spring 2005, colonizing the intertidal and shallow subtidal. A seasonal survey in 2006 showed that U. pinnatifida was established in a sheltered zone inside the estuary, along a coastal fringe of 8 km between Punta Cascajo and Cañadón del Puerto. This continuous distribution was only interrupted in the mouth of canyons that flow into Ría Deseado, where the bottom is conformed by mud and sand. The sporophytes were mainly found colonizing the rocky bottom in the lower intertidal, bordering the Macrocystis pyrifera population. The highest density and biomass of sporophytes (12.13 ind. m-2; 254.60 g m-2) were registered during spring, when the population was mainly conformed by individuals of medium sizes. The lowest density and biomass (0.33 ind. m-2; 5.69 g m-2) were registered in autumn. Juvenile sporophytes recruited throughout the year, but presented the highest percentage in the population during autumn and winter. First mature sporophytes appeared in spring and attained their maximum size in summer. After this, the sprophytes decayed and disappeared. Environmental factors such as rocky bottoms availability and water transparency may be the main factors determining the sporophytes distribution in Ría Deseado. The field experiment point out that M. pyrifera population is an important factor controlling the dispersion of U. pinnatifida towards the subtidal. SPANISH: Undaria pinnatifida fue registrada en la Ría Deseado (47º45´ S, 65º55´ W _ Patagonia austral) durante la primavera de 2005, colonizando el intermareal y submareal somero. Los relevamientos estacionales realizados durante el 2006, revelaron que U. pinnatifida se encontró establecida en una zona protegida en el interior de la ría, ocupando una franja costera de aproximadamente 8 km de largo entre Punta Cascajo y el Cañadón del Puerto. Esta distribución casi continua sólo presentó algunas interrupciones en la boca de los cañadones que desembocan en la ría, donde el fondo predominante es de tipo areno-fangoso. Los esporofitos de U. pinnatifida ocuparon preferentemente el fondo rocoso del intermareal inferior, limitando con la población de Macrocystis pyrifera. La densidad y biomasa más altas de esporofitos (12,13 ind. m-2; 254,60 g m-2) fueron registradas en primavera, cuando la población se encontró compuesta principalmente por individuos de tallas intermedias. La densidad y biomasa más bajas (0,33 ind. m-2; 5,69 g m-2) fueron registradas durante el otoño. Los esporofitos juveniles se reclutaron a lo largo de todo el año, pero alcanzaron su mayor proporción en la población durante el otoño y el invierno. Los esporofitos reproductivamente maduros aparecieron durante la primavera y alcanzaron su talla máxima durante el verano, luego del cual comenzaron a deteriorarse y a desaparecer. Factores como la disponibilidad de fondos rocosos y la transparencia de las aguas podrían actuar como los principales factores determinantes de su distribución en la ría. El experimento de campo realizado revela que los bosques de M. pyrifera actúan también como un importante factor de control, limitando la dispersión de U. pinnatifida hacia el submareal.

三种兰科植物的保护遗传学研究

本研究在野外调查的基础上，采用随机扩增多态DNA (RAPD)分析和形态学方法，研究了我国三种珍稀濒危兰科植物硬叶兜兰（Paphiopedilummicranthum）、麻栗坡兜兰（P. malipoense）和独花兰（Changnienia amoena）的遗传多样性与群体遗传结构，主要结果如下： 1．采用1 2个引物对分布于我国云贵地区的4个硬叶兜兰群体共161个体进行RAPD扩增和分析，得出物种水平的多态条带百分率（PPB）为71.6%，Nci的基因多样度(h)为0.217，Shannon多样性指数（1)为0.3301;4个群体的平均多样性水平为PPB=45.2%，h=0.1457，1= 0.2204：低于远交兰花的平均水平。分子方差分析(AMOVA)表明，在总遗传变异中，群体间遗传变异占20.31%．群体内占79.69%;POPGENE给出的基因分化系数 （Gst）为0.2958;遗传分化略高于远交物种的平均水平。空间自相关分析表明，所检测的两个群体中存在明显的空间结构，基因型在群体中以不同的小斑块存在。遗传距离和空间距离不存在相关关系。 2．用于麻栗坡兜兰的RAPD引物同上，但取样范围只有贵州的2个群体共10个个体。就所研究的个体柬看，麻栗坡兜兰的遗传多样性明显低于远交兰花物种的平均水平。物种水平上，多态条带百分率(PPB)为49.5%。Nei的基因多样度（h）为0. 1174， Shannon多样性指数(I)为0.1764：在群体水平上，上述三个指标的平均值则分别为12. 75%、0.0486和0.0712，均大大低于硬叶兜兰。然而，尽管作了种种努力，麻栗坡兜兰的取样个体数量仍很少，因此所得结果可能会有误差。 3．用16个引物对分布于河南、湖北、湖南、江西4个省11个独花兰群体共216个体进行了RA PD扩增和分析，独花兰在物种水平PPB=80. 7%，h=0.197．1=0. 3116;在群体水平，上述三个指标的平均值则分别为40. 9%、0.1247和0. 1902，均低于远交兰花的平均水平。AMOVA分析表明，11个独花兰群体间的遗传变异占43.48%，群体内的占56.52%：在神农架和新宁地区内部，群体间的遗传变异分别占13.68%和49.3g%(AMOVA)。POPGENE给出的11个群体的基因分化系数(Gst)为0.3580．神农架和新宁地区内的Gst，值分别为0.1194和0.2597。可见，群体间的遗传分化明显高于远交物种的平均水平。空间自相关分析表明，独花兰的遗传变异在群体内不存在明显的空间结构。群体之间的遗传距离和空间距离不存在相关关系。 4．对独花兰7个群体形态性状的分析发现，12个形态性状在群体内均有较高的变异性，cv值变动于0.022-0.30O。庐山群体(LS)在所有性状上的平均值均为最高。营养性状和花部性状的变异性基本一致。除花葶长和花距直径与某些花部性状之间没有显著的相关关系外，各性状之间均有显著的相关性。对XN4群体的统计没有发现假磷茎数目与其他性状之间存在显著相关性。 根据以上对硬叶兜兰、麻粟坡兜兰和独花兰遗传多样性和群体遗传结构韵研究，结合其他方面的资料;对三种兰花的濒危机制进行了初步的分析。首先，人为采挖和破坏是导致这些兰花物种濒危的直接原因，尤其是麻栗坡兜兰。其次， 适宜兰花生存的生境正在只益萎缩、退化和片段化。这两方面因素的共同作用导致上述兰花群体的数目和规模日益下降，由此引发的遗传多样性降低和遗传结构的改变进一步加剧其濒危状况。对于独花兰而言，较低的繁殖能力又使其生存状态雪上加霜。针对三个物种不同的繁殖特性和遗传学状况，提出如下保护措施。(1)硬叶兜兰由于繁殖能力较强、现存个体尚多，遗传多样性损失不甚严重，因此以保护其所在的生境为基础、实施原位保护，是比较合适的保护策略。(2)麻粟坡兜兰目前受破坏程度非常严重;所剩个体很少，遗传多样性较低，已经很难进行有效的原位保护。因此;应利用迁地保护手段抢救目前尚存的个体。(3)独花兰的繁殖能力较弱，因此在保护生境和严禁采摘的基础上，可采用人工授粉等方式，提高结实率、增加繁殖效率，促使其复壮：在进行迁地保护时，则应注意不同群体间存在较大遗传变异而群体内多样性较低这一现实。

从60MeV/u~(18)O离子辐照过的钍中分离Ra

对以212Pb, 133Ba和224Ra作示踪剂,(NH4)2H2EDTA为淋洗剂,用阳离子交换法从Pb、Ba中分离Ra的工艺条件做了研究。提出了一个从60 MeV/u 18O离子辐照过的ThO2靶中分离Ra的放射化学流程。实验结果表明,该流程对主要反应产物,特别是Ba的去污较好,Ra的产额可达70%以上。

Production cross-section of Ra-230 in the reaction of 60 MeV/u O-18 ions with U-238

A thick natural uranium target was bombarded with a 60 MeV/u O-18 beam. The neutron-rich isotope Ra-230 as the target residue was produced through the multinucleon transfer reaction (U-238-4p-4n). The barium and radium fraction as BaCl2 precipitate were radiochemically separated first from the mixture of uranium and reaction products. Then, the radium fraction was separated from BaCl2 precipitate by using cation exchange technique. The gamma-ray spectra of the Ra fraction were measured using an HPGe detector. The production cross sections of Ra-230 were obtained by a combination of the radiochemical separation technique and off-line gamma-ray spectroscopy. The cross section of Ra-230 has been determined to be 66 +/- 20 mu b.

Cultivar de soja BRS 217 - Flora.

2001

A Cult Film by Proxy: Space is the Place and the Sun Ra Mythos

Sexton, J. (2006). A Cult Film by Proxy: Space is the Place and the Sun Ra Mythos. New Review of Film and Television Studies. 4(3), pp.197-215. RAE2008

Nitrogen uptake of phytoplankton assemblages under contrasting upwelling and downwelling conditions: The Ría de Vigo, NW Iberia

Regenerated production (including organic nitrogen) is shown here to be important in the Ria de Vigo (Galicia, NW Iberia) in supporting both harmful algal bloom communities during the downwelling season, but also (to a lesser extent) diatom communities during stratified periods of weak to moderate upwelling. The Galician Rias, situated in the Iberian upwelling system, are regularly affected by blooms of toxic dinoflagellates, which pose serious threats to the local mussel farming industry. These tend to occur towards the end of summer, during the transition from upwelling to downwelling favourable seasons, when cold bottom shelf waters in the rias are replaced by warm surface shelf waters. Nitrate, ammonium and urea uptake rates were measured in the Ria de Vigo during a downwelling event in September 2006 and during an upwelling event in June 2007. In September the ria was well mixed, with a downwelling front observed towards the middle of the ria and relatively high nutrient concentrations (1.0-2.6 mu mol L-1 nitrate; 1.0-5.6 mu mol L-1 ammonium; 0.1-0.8 mu mol L-1 phosphate; 2.0-9.0 mu mol L-1 silicic acid) were present throughout the water column. Ammonium represented more than 80% of the nitrogenous nutrients, and the phytoplankton assemblage was dominated by dinoflagellates and small flagellates. In June the water column was stratified, with nutrient-rich, upwelled water below the thermocline and warm, nutrient-depleted water in the surface. At this time, nitrate represented more than 80% of the nitrogenous nutrients, and a mixed diatom assemblage was present. Primary phytoplankton production during both events was mainly sustained by regenerated nitrogen, with ammonium uptake rates of 0.035-0.063 mu mol N L-1 h(-1) in September and 0.078-0.188 mu mol N L-1 h(-1) in June. Although f-ratios were generally low (<0.2) in both June and September, a maximum of 0.61 was reached in June due to higher nitrate uptake (0.225 mu mol N L-1 h(-1)). Total nitrogen uptake was also higher during the upwelling event (0.153-0.366 in June and 0.053-0.096 mu mol N L-1 h(-1) in September). Nitrogen uptake kinetics demonstrated a strong preference for ammonium and urea over nitrate in June.

The SuperWASP wide-field exoplanetary transit survey: candidates from fields 23 h <RA <03 h

Photometric transit surveys promise to complement the currently known sample of extra-solar planets (ESPs) by providing additional information on the planets and especially their radii. Here, we present ESP candidates from one such survey called, the Wide Angle Search for Planets (WASP) obtained with the SuperWASP wide-field imaging system. Observations were taken with SuperWASP North located in La Palma during the 2004 April to October observing season. The data cover fields between 23 and 03 h in RA at declinations above +12. This amounts to over ~400000 stars with V magnitudes 8-13.5. For the stars brighter than 12.5, we achieve better than 1 per cent photometric precision. Here, we present 41 sources with low-amplitude variability between ~1 and 10 mmag, from which we select 12 with periods between 1.2 and 4.4 d as the most promising ESP candidates. We discuss the properties of these ESP candidates, the expected fraction of transits recovered for our sample and implications for the frequency and detection of hot-Jupiters.

SuperWASP-N extrasolar planet candidates between 18 <RA <21h

The SuperWASP-I (Wide Angle Search for Planets-I) instrument observed 6.7 million stars between 8 and 15mag from La Palma during the 2004 May-September season. Our transit-hunting algorithm selected 11626 objects from the 184442 stars within the RA (right ascension) range 18-21h. We describe our thorough selection procedure whereby catalogue information is exploited along with careful study of the SuperWASP data to filter out, as far as possible, transit mimics. We have identified 35 candidates which we recommend for follow-up observations.

SuperWASP-North extrasolar planet candidates between 3h <RA <6h

The Wide Angle Search for Planets (WASP) photometrically surveys a large number of nearby stars to uncover candidate extrasolar planet systems by virtue of small-amplitude light curve dips on a