Extracellular polymeric substances of the marine fouling diatom amphora rostrata Wm.Sm

Amphora rostrata was grown under continuous illumination at 27°C in batch cultures using f/2 medium. Cell biomass (measured as chllorophyll a and cell counts) reached a maximum on day 7. Thereafter, cell biomass as chl a showed a small decrease. Planktonic('free') and biofilm extracellular polymeric substances (EPS) from the adherent cells of A. rostrata were studied. Both types of EPS were produced during the logarithmic phase of growth. However, production was higher during the stationary growth phase. Enhanced EPS production was associated with nutrient deficient conditions. Planktonic and biofilm EPS were purified by gel filtration using Sephadex G‐200 and ion exchange chromatography using DEAE‐cellulose. Both polymers showed the presence of a single peak. Capillary gas Chromatographie analysis of both planktonic and biofilm EPS showed that fucose (36.7%) and galactose (27.6%) were the most abundant monosaccharides, with small quantities of rhamnose, xylose, arabinose, mannose and glucose. Other chemical analysis showed the presence of sulphate, uronic acids, hexoamines, pyruvate and proteins in both the planktonic and bio‐film EPS. Uronic acid, pyruvate and sulphate together were found to contribute ～50 to 60% (W/W) to the EPS of A. rostrata. Such a high content of non‐sugar components indicates their importance to the diatom in metal binding, desiccation prevention and flexibility.     

Differences in carbohydrate profiles in batch culture grown planktonic and biofilm cells of Amphora rostrata Wm. Sm

Diatoms are abundant in biofilms developed on surfaces immersed in sunlit waters. In both the planktonic and the biofilm mode of growth, diatoms produce carbohydrate polymers which perform several functions including motility, protection, production of macro-aggregates and detoxification. However, little is known about the differences, if any, in the production and characterization at the molecular level of carbohydrates in planktonic and biofilm cells. In order to identify the differences in these two modes of growth, the concentration of total carbohydrates, carbohydrate fractions, neutral carbohydrates, uronic acids and amino sugars in planktonic and biofilm cells of Amphora rostrata were measured. The results showed that the distribution of carbohydrate fractions, uronic acids and amino sugars was different in biofilm and planktonic cells. Cell normalized concentrations of these components were two to five times greater in planktonic cells compared with biofilm cells. The concentrations of glucose and glucosamine decreased, whereas fucose increased in planktonic cells over the period of cultivation. Conversely, the concentrations of glucose and glucosamine increased while that of fucose decreased in attached cells. The study suggests that marked differences exist between the carbohydrates of the planktonic and the biofilm cells of A. rostrata.     

不同保存条件下Wm84株腮腺炎减毒活疫苗的稳定性

采用留样观察法对Wm84株腮腺炎减毒活疫苗在不同保存条件和不同规格疫苗(1 mL/支21批、0.5mL/支24批)的稳定性进行了比较.结果表明不同规格疫苗的稳定性均较好,疫苗保存温度越低其稳定性越好.     

Hcn and Hnc in Comets C/2000 Wm1 (Linear) and C/2002 C1 (Ikeya-Zhang)

Comets have been suggested as a possibly significant source of organic molecules to the early Earth. Hydrogen cyanide (HCN) is important in models of prebiotic chemistry, but may be difficult to form in the early terrestrial environment, while hydrogen isocyanide (HNC) is a `classical' tracer of interstellar ion-molecule chemistry. We have observed both HCN and HNC in 2 recent comets, bringing the number of comets with published measurements of the HNC/HCN abundance ratio to 6. The HNC/HCN ratio in comet Ikeya-Zhang appears to increase with decreasing heliocentric distance, as was previously observed for comet Hale-Bopp, indicating that the HNC is produced at least in part by processes in the cometary coma (atmosphere) and is not simply a constituent of the nuclear ices. Both comets C/2000 WM1 (Linear) and C/2002 C1 (Ikeya-Zhang) exhibit values of the HNC/HCN ratio that appear to be too large (0.09–0.19) tobe matched by current models of coma chemistry. Cometary HNC maybe a photodissociation product of organic grains or large organic polymers stored in the nucleus. We have also set a limit on the emission from the NO radical in comet WM1.