紫茎泽兰精油各馏份对4种仓库害虫的杀虫活性

用紫茎泽兰精油的２０℃￣１５０℃,１５０℃￣２００℃,２００℃￣２３０℃,２３０℃￣３００℃和３００℃以上馏份,分别以４４．４４ｍｇ／Ｌ的熏蒸浓度处理米像、玉米象、绿豆象和蚕豆象,结果表明,在５个馏份中,以１５０℃￣２００℃馏份的杀虫活性最高,其次是２０℃￣１５０℃和２２０℃￣２３０℃馏份,而３００℃以上馏份的杀虫活性最低。进一步的生测结果表明,１５０℃￣２００℃馏份对米象、玉米象、绿豆象和蚕豆象     

Spontaneous formation of macroscopic chiral domains in a fluid smectic phase of achiral molecules

A smectic liquid-crystal phase made from achiral molecules with bent cores was found to have fluid layers that exhibit two spontaneous symmetry-breaking instabilities: polar molecular orientational ordering about the layer normal and molecular tilt. These instabilities combine to form a chiral layer structure with a handedness that depends on the sign of the tilt. The bulk states are either antiferroelectric-racemic, with the layer polar direction and handedness alternating in sign from layer to layer, or antiferroelectric-chiral, which is of uniform layer handedness. Both states exhibit an electric field-induced transition from antiferroelectric to ferroelectric.     

Mercury cratering record viewed from MESSENGER's first flyby

Morphologies and size-frequency distributions of impact craters on Mercury imaged during MESSENGER's first flyby elucidate the planet's geological history. Plains interior to the Caloris basin displaying color and albedo contrasts have comparable crater densities and therefore similar ages. Smooth plains exterior to Caloris exhibit a crater density approximately 40% less than on interior plains and are thus volcanic and not Caloris impact ejecta. The size distribution of smooth-plains craters matches that of lunar craters postdating the Late Heavy Bombardment, implying that the plains formed no earlier than 3.8 billion years ago (Ga). At diameters less than or equal to 8 to 10 kilometers, secondary impact craters on Mercury are more abundant than primaries; this transition diameter is much larger than that on the Moon or Mars. A low density of craters on the peak-ring basin Raditladi implies that it may be younger than 1 Ga.