Thermal Structure of Jupiter's Upper Atmosphere Derived from the Galileo Probe

Temperatures in Jupiter's atmosphere derived from Galileo Probe deceleration data increase from 109 kelvin at the 175-millibar level to 900 ± 40 kelvin at 1 nanobar, consistent with Voyager remote sensing data. Wavelike oscillations are present at all levels. Vertical wavelengths are 10 to 25 kilometers in the deep isothermal layer, which extends from 12 to 0.003 millibars. Above the 0.003-millibar level, only 90- to 270- kilometer vertical wavelengths survive, suggesting dissipation of wave energy as the probable source of upper atmosphere heating.     

Selected Elastic Moduli of Single-Crystal Olivines from Ultrasonic Experiments to Mantle Pressures

Ultrasonic interferometric measurements, developed for polycrystalline samples in a multi-anvil apparatus, were extended to single-crystal samples of San Carlos olivine and forsterite. The elastic moduli, C22 and C55 of San Carlos olivine and C55 of pure forsterite, were measured to about 13 gigapascals. These data on C22 for San Carlos olivine and C55 for forsterite are consistent with earlier measurements and extrapolations. The C55 for San Carlos olivine increases linearly as a function of increasing pressure, unlike the earlier nonlinear behavior observed at high pressure with impulsive stimulated scattering techniques.     

海刺猬和中间球海胆性腺的组织学和组织化学

对海刺猬Glyptocidaris crerularis和中间球海胆Stronylocentrotus intermedius性腺的组织学和组织化学进行了比较研究。结果表明,两者性腺结构均为滤泡型,滤泡由生殖细胞和营养细胞组成,随着生殖细胞的发育成熟,营养细胞中颗粒逐渐减少,当生殖细胞排放后,营养颗粒的数量逐渐增加,且中间球海胆的营养颗粒数量较海刺猬多。观察和分析了海刺猬和中间球海胆的雌、雄生殖细胞、营养颗粒、滤泡细胞的DNA、RNA、多糖、蛋白质和结合脂类的分布、数量及其变化,发现中间球海胆滤泡中营养颗粒的多糖和蛋白质含量比海刺猬高,其它指标两者都很相近。