The Widespread Colonization Island of Actinobacillus actinomycetemcomitans

Genomic islands, such as pathogenicity islands, contribute to the evolution and diversification of microbial life. Here we report on the Widespread Colonization Island, which encompasses the tad (tight adherence) locus for colonization of surfaces and biofilm formation by the human pathogen Actinobacillus actinomycetemcomitans. At least 12 of the 14 genes at the tad locus are required for tenacious biofilm formation and synthesis of bundled Flp pili (fibrils) that mediate adherence. The pilin subunit, Flp1, remains inside the cell in tad-locus mutants, indicating that these genes encode a secretion system for export and assembly of fibrils. We found tad-related regions in a wide variety of Bacterial and Archaeal species, and their sequence characteristics indicate possible horizontal transfer. To test the hypothesis of horizontal transfer, we compared the phylogeny of the tad locus to a robust organismal phylogeny using statistical tests of congruence and tree reconciliation techniques. Our analysis strongly supports a complex history of gene shuffling by recombination and multiple horizontal transfers, duplications and losses. We present evidence for a specific horizontal transfer event leading to the establishment of this region as a determinant of disease.     

Deep winds beneath Saturn's upper clouds from a seasonal long-lived planetary-scale storm

Convective storms occur regularly in Saturn's atmosphere. Huge storms known as Great White Spots, which are ten times larger than the regular storms, are rarer and occur about once per Saturnian year (29.5 Earth years). Current models propose that the outbreak of a Great White Spot is due to moist convection induced by water. However, the generation of the global disturbance and its effect on Saturn's permanent winds have hitherto been unconstrained by data, because there was insufficient spatial resolution and temporal sampling to infer the dynamics of Saturn's weather layer (the layer in the troposphere where the cloud forms). Theoretically, it has been suggested that this phenomenon is seasonally controlled. Here we report observations of a storm at northern latitudes in the peak of a weak westward jet during the beginning of northern springtime, in accord with the seasonal cycle but earlier than expected. The storm head moved faster than the jet, was active during the two-month observation period, and triggered a planetary-scale disturbance that circled Saturn but did not significantly alter the ambient zonal winds. Numerical simulations of the phenomenon show that, as on Jupiter, Saturn's winds extend without decay deep down into the weather layer, at least to the water-cloud base at pressures of 10-12 bar, which is much deeper than solar radiation penetrates.     

断层转折褶皱角度燃系的—种几何学分析方法

通过对断层转折褶皱Suppe模型角度关系的深入分析,提出一种应用圆周和三角形来进行褶皱变形的几何图解方法,论证了该几何作图方法的合理性和准确性。分别就实际应用中4种主要常见情况,即已知半翼间角γ和断层切层角θ、已知半翼间角γ和前翼倾角β、已知断层切层角θ和前翼倾角β以及已知断层切层角θ和断层转折角φ情况下的几何构图方法...