基板和流速对羟基磷灰石生长的影响

通过共混制备聚二甲基硅氧烷（PDMS）/羟基磷灰石（HAP）和PDMS/生物玻璃复合材料作为生长基板，研究了静止条件下不同基板上HAP的生长.设计了一套流速加载装置，观察模拟体液流速对生物玻璃基板上HAP晶体生长的影响.研究发现在静止条件下，HAP晶体在PDMS复合材料上比在生物玻璃上生长更快，尺寸更大；随着流速的增加，HAP晶体尺寸更大而且无定形沉淀数量减少.      

LiNi0.8Co0.15Al0.05O2(NCA)正极材料的磷酸表面改性

针对新一代空间型号产品对储能电源提出的更高需求,提出采用表面改性的方法提升LiNi0.8Co0.15Al0.05O2（NCA）正极材料在锂离子电池中的循环稳定性。通过采用磷酸（H3PO4）对NCA正极材料进行表面处理,H3PO4会与NCA颗粒表面的含锂碱性物质发生反应,从而在NCA颗粒表面生成稳定且导电性良好的Li3PO4界面层。循环以及阻抗测试结果表明,经H3PO4表面处理的NCA材料组装电池循环50次后电池容量为170.5mA·h/g,容量保持率达到94%以上,界面阻抗得到抑制。H3PO4表面处理有效抑制了NCA颗粒表面碱性残留对电化学性能的不良影响,提升了界面稳定性,获得了更好的循环性能。     

微重力下胶原蛋白纤维化及羟基磷灰石结晶的初步研究

在长期空间飞行过程中, 骨质丢失是一个严重问题. 羟基磷灰石(HAP)晶体是骨骼的主要成分, 骨骼中的胶原蛋白纤维在HAP生长结晶过程中起到关键作用. 研究了胶原蛋白纤维化过程在模拟微重力和常重力条件下的变化, 对以胶原 蛋白纤维作为模板生长出的HAP晶体形貌进行了观察. 结果表明, 不同浓度胶原蛋白溶液中形成的胶原蛋白纤维, 其内部孔隙数量和尺寸在模拟微重力条件下要明显大于常重力条件下, 胶原蛋白纤维内部孔隙的分布也不同于常重力条 件下的结果. 以模拟微重力条件下形成的胶原蛋白纤维为模板生长出的HAP 晶体主要为立方体状, 而以常重力条件下形成的胶原蛋白纤维为模板生长出的 HAP晶体形貌主要为板状. 该结果有助于未来进一步阐明空间骨质丢失的机理.      

Free and membrane-bound calcium in microgravity and microgravity effects at the membrane level.

The changes of [Ca2+]i controlled is known to play a key regulatory role in numerous cellular processes especially associated with membranes. Previous studies from our laboratory have demonstrated an increase in calcium level in root cells of pea seedlings grown aboard orbital station "Salyut 6". These results: 1) indicate that observed Ca(2+)-binding sites of membranes also consist in proteins and phospholipids; 2) suggest that such effects of space flight in membrane Ca-binding might be due to the enhancement of Ca2+ influx through membranes. In model presented, I propose that Ca(2+)-activated channels in plasma membrane in response to microgravity allow the movement of Ca2+ into the root cells, causing a rise in cytoplasmic free Ca2+ levels. The latter, in its turn, may induce the inhibition of a Ca2+ efflux by Ca(2+)-activated ATPases and through a Ca2+/H+ antiport. It is possible that increased cytosolic levels of Ca2+ ions have stimulated hydrolysis and turnover of phosphatidylinositols, with a consequent elevation of cytosolic [Ca2+]i. Plant cell can response to such a Ca2+ rise by an enhancement of membranous Ca(2+)-binding activities to rescue thus a cell from an abundance of a cytotoxin. A Ca(2+)-induced phase separation of membranous lipids assists to appear the structure nonstable zones with high energy level at the boundary of microdomains which are rich by some phospholipid components; there is mixing of molecules of the membranes contacted in these zones, the first stage of membranous fusion, which was found in plants exposed to microgravity. These results support the hypothesis that a target for microgravity effect is the flux mechanism of Ca2+ to plant cell.     

Protein crystal growth aboard the U.S. space shuttle flights STS-31 and STS-32.

The first microgravity protein crystal growth experiments were performed on Spacelab I by Littke and John. These experiments indicated that the space grown crystals, which were obtained using a liquid-liquid diffusion system, were larger than crystals obtained by the same experimental system on earth. Subsequent experiments were performed by other investigators on a series of space shuttle missions from 1985 through 1990. The results from two of these shuttle flights (STS-26 and STS-29) have been described previously. The results from these missions indicated that the microgravity grown crystals for a number of different proteins were larger, displayed more uniform morphologies, and yielded diffraction data to significantly higher resolutions than the best crystals of these proteins grown on earth. This paper presents the results obtained from shuttle flight STS-32 (flown in January, 1990) and preliminary results from the most recent shuttle flight, STS-31 (flown in April, 1990).     

Transport phenomena and crystal growth of the GeSe-Xenon system for different gravitational conditions

Previous chemical vapor transport experiments of the GeSe-GeI₄ system performed under reduced gravity conditions /1/ yielded crystals of considerably improved surface and bulk morphology. In addition, the mass transport rates observed in microgravity environment were significantly greater than predicted. A quantitative thermodynamic analysis of the solid-gas phase reactions of the GeSe-GeI₄ system revealed the multi-component, multi-reaction nature of the vapor phase /2/. Continued transport studies on ground of the GeSe-GeI₄ system in the presence of inert gases provided experimental evidence for the existence of a boundary layer /2/ and its thickness dependence on GeI₄ pressure in closed tube systems. Systematic transport rate measurements for different orientations of the density gradient relative to the gravity vector demonstrated the effects of ampoule inclination on mass flux /3/. Based on a computational model for simultaneous chemical vapor transport, sublimation, and Stefan flow /3/, the excellent agreement of predicted with ground-based experimental mass transport rates over wide pressure ranges /3/ confirmed the validity of the model and the discrepancy between observed and expected transport rates of the GeSe-GeI₄ system in microgravity.     

用国产装置进行的空间蛋白质结晶实验

使用国内研制的管式汽相扩散结晶装置,在我国返回式卫星上,成功地完成了两次空间蛋白质晶体生长实验,10种不同种类的蛋白质配制的48个样品在空间的出晶率分别达52%和80%,其中少数蛋白质生长出了较高质量的蛋白质晶体。结果表明,空间的微重力环境利于改善蛋白质晶体的生长,而且在结晶条件优化足够好的条件下,在空间里能生长出比地面晶体尺寸较大、形态较好和内部有序性较高的蛋白质晶体。本文还就微重力对蛋白质晶体生长的具体作用及其开发利用做了讨论。      

Lithium-induced changes in gravicurvature, statocyte ultrastructure and calcium balance of pea roots.

Calcium signaling has been implicated in plant graviperception. In order to investigate the role of intracellular calcium in the process, I used lithium ions (LiCl), which suppress inositol 1,4,5-trisphosphate (IP3) cycling and signaling by inhibiting inositol-1-phosphatase. After 4 h of gravistimulation, no curvature was observed in 81% of the roots of 5-day Pisum sativum seedlings pretreated with 5 mM LiCl. Structural features of statocyte ultrastructure in these roots were the following: loss of a cellular polarity, appearance of amyloplast clusters, condensed mitochondria, local dilations in a perinuclear space, increases in a relative volume of vacuoles. The intensity of a cytochemical reaction (pyroantimonate staining which detected Ca2+ ions) was moderate: the Ca2+ pyroantimonate deposits were observed in all organelles. There were few granules of this precipitate in a hyaloplasm of the statocytes. Mitochondria and vacuoles were found to contain more granules of the precipitate compared with the controls. Additionally, Ca(2+)-ATPase activity in the statocytes of pea roots pretreated with LiCl was approximately the same as in control roots. Data obtained by using inhibitor of inositol signaling suggest that the observed effects of LiCl on root gravicurvature and ultrastructure of root statocytes were due to effects on Ca2+ homeostasis, particularly on IP3-mediated release of intracellular Ca2+ which can be inhibited by inositol depletion. The work demonstrates the key role played by second messengers (Ca2+ and IP3) in a gravity perception and response.     

The atmosphere of the primitive earth and the prebiotic synthesis of organic compounds.

The prebiotic synthesis of organic compounds using a spark discharge on various simulated prebiotic atmospheres at 25 degrees has been studied. Methane mixtures contained H2 + CH4 + H2O + N2 + NH3 with H2/CH4 molar ratios from 0 to 4 and pNH3 = 0.1 torr. A similar set of experiments without added NH3 was performed. The yields of amino acids (1.2 to 4.7% based on the carbon) are approximately independent of the H2/CH4 ratio and the presence of added NH3, and a wide variety of amino acids are obtained. Mixtures of H2 + CO + H2O + N2 and H2 + CO2 + H2O + N2, with and without added NH3, all give about 2% yields of amino acids at H2/CO and H2/CO2 ratios of 2 to 4. For the H2/CO and H2/CO2 ratios less than 1, the yields fall off drastically to as low as 10(-3)%. Glycine is almost the only amino acid produced from CO and CO2 atmospheres. These results show that the maximum yield is about the same for the three carbon sources at high H2/carbon ratios, but that CH4 is superior at low H2/carbon ratios. In addition, CH4 gives a much greater variety of amino acids than either CO or CO2. If it is assumed that amino acids more complex than glycine were required for the origin of life, then these results indicate the need for CH4 in the primitive atmosphere. The yields of cyanide and formaldehyde parallel the amino acid results, with yields of HCN and H2CO as high as 13% based on the carbon. Ammonia is also produced from N2 in experiments with no added NH3 in yields as high as 4.9%. These results show that large amounts of NH3 would have been synthesized on the primitive earth by electric discharges. The amount of ammonia formed by hydrolysis of HCN and various nitriles may have exceeded that formed directly in electric discharges.     

基于物理光学假设的导体表面电流密度误差分析

用物理光学法计算理想导体雷达散射截面过程中,需要基于无限大切平面假设计算表面电流密度.只有对表面比较光滑的电大尺寸目标,该假设才近似满足,而在一般情况下由该方法求得的表面电流密度存在误差.将二维导体圆柱、方柱以及三角柱等构型在不同入射频率、极化下的物理光学表面电流密度与精确解或矩量法结果进行了对比.分析表明:横磁波照射时物理光学法除在顶点处有较大误差外,基本能够正确反映出表面电流密度分布情况.横电波情形下物理光学法难以如实反映照射面和阴影面电流的谐振变化,与入射方向平行的面上表面电流密度也有较大误差.     

Calcium balance in pea root statocytes under both clinorotation and Ca2+ channel blockers' influence.

We have previously demonstrated that space flight and clinorotation conditions increase cytoplasmic Ca2+ level in pea root statocytes. A rise in [Ca2+]i may be a serious problem for plants in microgravity environment. It is hypothesized that involvement of Ca2+ channel blockers in the growth medium may rescue a plant from abundance of Ca2+ ions. Indeed, combination of clinorotation (2 rpm, 5 days) and any Ca2+ channel blocker (1 micromole D600 or nicardipine, 12 hr) causes decreasing the Ca2+ concentration in pea root statocytes in comparison with clinorotation alone. Redistribution of Ca(2+)-ATPase activities observed under clinorotation comes to normal after D600 application whereas following by nicardipine action the pattern of the cytochemical staining is intermediate between those in stationary control and under clinorotation. Our data support the hypothesis that Ca2+ channel blockers may act as protectors for plants against rise in [Ca2+]i. The role for Ca2+ channels in graviperception and in microgravity effects as well as ways for stabilization of Ca2+ balance in plant cells in space flights are discussed.     

Plant responses to short- and long-term exposures to high carbon dioxide levels in closed environments.

When higher plants are exposed to elevated levels of CO2 for both short- and long-term periods photosynthetic C-gain and photoassimilate export from leaves are generally increased. Water use efficiency is increased on a leaf area basis. During long-term exposures, photosynthesis rates on leaf and whole plants bases are altered in a species specific manner. The most common pattern in C3 plants is an enhanced rate of whole plant photosynthesis in a well irradiated canopy. Nevertheless, in some herbaceous species prolonged exposure to high CO2 results in remobilization of nitrogenous reserves (i.e., leaf protein degradation) and reduced rates of mature leaf photosynthesis when assayed at ambient CO2 and O2 levels. Both short- and long-term exposures to those CO2 levels (i.e., 100 to 2,000 microliter l-1) which modify photosynthesis and export, also modify both endogenous ethylene gas (C2H4) release, and substrate, 1-aminocyclopropane-1-carboxylic acid (ACC), saturated C2H4 release rates from irradiated leaves. Photosynthetically active canopy leaves contribute most of the C2H4 released from the canopy. Prolonged growth at high CO2 results in a persistent increase in the rate of endogenous C2H4 release from leaves which can, only in part, be attributed to the increase of the endogenous pools of C2H4 pathway intermediates (e.g., methionine, M-ACC, and ACC). The capacity for increasing the rate of C2H4 release in response to short-term exposures to varying CO2 levels does not decline after prolonged growth at high CO2. When leaves, whole plants, and model canopies of tomato plants are exposed to exogenous C2H4 a reduction in the rate of photosynthesis can, in each case, be attributed to the classical effects of C2H4 on plant development and morphology. The effect of C2H4 on CO2 gas exchange of plant canopies is shown to be dependent on the canopy leaf area index.     

Coronal activity in F-, G-, and K-type stars; relations between parameters characterizing stellar structures and X-ray emission

A sample of 52 stars containing dwarfs and giants is subjected to a multidimensional factor analysis. The parameters used are the soft X-ray flux at the stellar surface F_x, the Ca II H+K line-core flux F_H+K, the stellar radius and mass. We find a high correlation between F_x and the Ca II H+K excess flux ΔF_H+K obtained by subtracting an observational lower-limit flux from F_H+K. We conclude that the lower-limit Ca II flux is uncorrelated with the stellar X-ray emission. The common-factor analysis shows that, for the present sample, F_x depends only on ΔF_H+K, and not on the stellar radius or mass. All stars included in our analysis follow the relation F_x ∝ Δ^1.4_H+K over almost four decades in F_x.     

EVALUATION OF MORPHOLOGY-STABLE CRITICAL SIZE OF KNbO3 CRYSTALS

Skeletal form of KNbO3 crystals growing in Li2B4O7 solvent was in-situ observed at 900°C and it was found that shallow depression started to develop on the surface of KNbO3 crystals when the crystal size exceeded several micron, typically 7 micron.Based on the quantitative criterion derived by Chernov, the estimated critical size of KNbO3 crystals was 1 micron, which was consistent with the experimental measure ment. The kinetic coefficients, kcorner and kcr, in the criterion were experimentally obtained in the diffusive-convective and diffusive-advective flow states respectively.     

Calcium abundance measurements using the Yohkoh BCS

Soft X-ray observations by SMM and other spacecraft have shown that the abundance of certain elements in solar corona varies from flare to flare. In this study, observations made by the Yohkoh Bragg Crystal Spectrometer (BCS) in helium-like Ca XIX have been analysed, and Ca abundance determined for 177 flares observed during the first four years of the mission (1991–1995). The average abundance of Ca relative to H for all flares is A_Ca = (3.64±0.39) × 10⁻⁶. As with an earlier study of SMM data, the abundance is found to be enhanced compared to the photosphere ((2.24±0.10) × 10⁻⁶), and with only minor variation from flare to flare. However, the absolute value and range of values determined by this study is smaller than in the previous study; these differences are discussed.     

Photolysis of phosphine in the presence of acetylene and propyne, gas mixtures of planetary interest.

Phosphine (PH3) 1 has been observed in the atmospheres of Jupiter and Saturn. We have studied the photochemical reactions of this compound with acetylene (C2H2), an alkyne also detected in these atmospheres. The volatile products formed in these reactions were characterized by H, 31P and 13C NMR. The ethenylphosphine 2 is the first product formed in the photolysis of PH3 in the presence Of C2H2. Photolysis of PH3 in the presence of propyne (C3H4) led to the formation of the Z- and E-prop-1-enylphosphines and traces of 1-methylethenylphosphine. A reaction pathway is proposed. The initial step is the dissociation of PH3 to hydrogen and PH2 radicals. Addition of the phosphinyl radical on alkyne occurs as the next step. Vinylphosphines are then formed by radical combination. This proposed reaction pathway takes into account the nature of the products and studies devoted to the photolysis of germane (GeH4) or hydrogen sulfide (H2S) in the presence of alkyne. Attempts to detect the methylidynephosphine HC triple bond P (the isoelectronic compound of HC triple bond N), in the photolysis products of PH3-C2H2 mixtures were unsuccessful. The application of these findings to Jovian and Saturn atmospheric chemistry is discussed.     

Organic solids produced from simple C/H/O/N ices by charged particles: applications to the outer solar system.

CH4, CO, and CO2 are all potential one-carbon molecular repositories in primitive icy objects. These molecules are all found in the Comet Halley coma, and are probable but, (except for CH4 detected on Triton and Pluto) undetected subsurface constituents in icy outer solar system objects. We have investigated the effects of charged particle irradiation by cold plasma discharge upon surfaces of H2O:CH4 clathrate having a 200:1 ratio, as well as upon ices composed of H2O plus C2H6 or C2H2 (sometimes plus NH3) which are also plausible constituents. These materials color and darken noticeably after a dose 10(9) - 10(10) erg cm-2, which is deposited rapidly (< or = 10(4) yr.) in solar system environments. The chromophore is a yellowish to tan organic material (a tholin) which we have studied by UV-VIS reflection and transmission, and IR transmission spectroscopy. Its yield, -1 C keV-1, implies substantial production of organic solids by the action of cosmic rays and radionuclides in cometary crusts and interiors, as well as rapid production in satellite surfaces. This material shows alkane bands which Chyba and Sagan have shown to well match the Halley infrared emission spectrum near 3.4 microns, and also bands due to aldehyde, alcohol and perhaps alkene/aromatic functional groups. We compare the IR spectral properties of these tholins with the spectra of others produced by irradiation of gases and ices containing simple hydrocarbons.     

THE CONVECTIVE EFFECT ON THE MORPHOLOGICAL INSTABILITY OF KNbO3 CRYSTALS

Experimentally, it was observed that there were various morphologies of KNbO3 crystals in different regions of the melt of Li2B4O7 and KNbO3 mixture in Pt loop heater. Dendrites grew in the central area of the melt, the diffusive-advective region,in which the temperature gradient is negligible; whereas crystals with smooth sur face were observed in the marginal area, the diffusive-convective region, with large temperature gradient. Based on the solute concentration over the KNbO3 crystal surface examined by electronic probe analysis, it was proved that the combinative effect of buoyancy and surface tension convection induced by temperature gradient enhanced the homogeneity of the solute concentration around KNbO3 crystals and thus their morphological stability.     

高强阻尼铝合金的阻尼性能和组织稳定性

采用时效处理实验,研究了快速凝固/粉末冶金工艺制备的X7093/5(Zn-30Al)高强度阻尼铝合金的阻尼性能和组织稳定性.将阻尼铝合金分别在50℃,100℃,120℃保温10?h,50?h,100?h后空冷,采用动态力学热分析仪(DMTA)和透射电镜(TEM)分别测试其阻尼性能和观察微观组织的变化情况.研究结果表明: 阻尼铝合金在时效过程中,组织结构由最初细碎杂乱的晶态结构转变为具有规则晶界的大晶粒结构,晶界对合金阻尼性能的贡献增强.在室温至250℃的温度范围内,合金阻尼值由4×10^-3增至3.0×10^-2.阻尼铝合金在120℃以下、100?h以内的时效处理中,时效温度和时效时间的不同对合金阻尼性能的影响不显著,材料的阻尼性能稳定性良好.     

Complex organics in laboratory simulations of interstellar/cometary ices.

We present the photochemical and thermal evolution of both non-polar and polar ices representative of interstellar and pre-cometary grains. Ultraviolet photolysis of the non-polar ices comprised of O2, N2, and CO produces CO2, N2O, O3, CO3, HCO, H2CO, and possibly NO and NO2. When polar ice analogs (comprised of H2O, CH3OH, CO, and NH3) are exposed to UV radiation, simple molecules are formed including: H2, H2CO, CO2, CO, CH4, and HCO (the formyl radical). Warming produces moderately complex species such as CH3CH2OH (ethanol), HC(=O)NH2 (formamide), CH3C(=O)NH2 (acetamide), R-CN and/or R-NC (nitriles and/or isonitriles). Several of these are already known to be in the interstellar medium, and their presence indicates the importance of grain processing. Infrared spectroscopy, 1H and 13C nuclear magnetic resonance (NMR) spectroscopy, and gas chromatography-mass spectrometry demonstrate that after warming to room temperature what remains is an organic residue composed primarily of hexamethylenetetramine (HMT, C6H12N4) and other complex organics including the amides above and polyoxymethylene (POM) and its derivatives. The formation of these organic species from simple starting mixtures under conditions germane to astrochemistry may have important implications for the organic chemistry of interstellar ice grains, comets and the origins of life.