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11.
AP易吸潮结块而影响其使用性能,需对其进行疏水处理,降低其吸湿性。采用氧化石墨烯( GO)对AP进行一元包覆制备出AP/GO复合物,用氟硅烷( FAS:十二氟庚基丙基三甲氧基硅烷)对AP进行二元包覆制备出AP/GO/FAS复合物。吸湿率测试结果表明,在20℃、相对湿度为85%的条件下,AP粒径越大,吸湿率越小。对AP进行二元包覆后的复合物吸湿率均小于纯AP和一元包覆后的AP复合物的吸湿率,且GO质量分数为0.4%,FAS质量分数为1%时,二元包覆AP后的复合物的吸湿率最小。通过热分析测试结果可知,GO质量分数为0.4%、FAS质量分数为1%的AP/GO/FAS复合物的高温放热分解峰比纯AP提前了约32.9℃。 相似文献
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This paper discusses the generation, stability, and control of artificial equilibrium points for a solar balloon spacecraft in the α Centauri A and B binary star system. The continuous propulsive acceleration provided by a solar balloon is shown to be able to modify the position of the (classical) Lagrangian equilibrium points of the three-body system on a locus whose geometrical form is known analytically. A linear stability analysis reveals that the new generated equilibrium points are usually unstable, but part of them can be stabilized with a simple feedback control logic. 相似文献
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在研究二进制、带符号的二进制(NAF,Non-Adjacent Form)等常见标量乘法算法的基础上,结合椭圆曲线基点的周期特性和预计算倍点序列方式,提出了一种新的标量乘法算法,并给出了新算法的详细步骤.点的周期性和系数决定了直接进行标量乘法运算还是转化为求其逆元,预计算倍点序列方式避免了椭圆曲线密码体制(ECC,Elliptic Curve Cryptosystem)加解密过程中大量的重复运算.为验证算法的正确性,采用密钥长度为192 bit椭圆曲线,给出了一个具体实例.实例结果和算法分析表明:与二进制和NAF算法相比,新算法虽占用了一些存储空间,但省去了倍点运算的时间开销,同时减少了点加的运算次数,极大地提高了标量乘法运算的效率.该算法的提出对完善ECC理论和加快ECC在实际中的应用具有重要意义. 相似文献
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针对高光谱遥感图像中地物识别与分类问题,在对传统二进编码方法的优缺点进行分析的基础上,给出了一种新的二进编码策略,并给出了相应的快速匹配算法。该算法原理简单,易于实现,能够提高不同地物的可分性,试验结果表明,算法可以得到较好的分类效果。 相似文献
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Eugene M. Trunkovsky 《Space Science Reviews》1995,74(3-4):485-488
Photoelectric WBVR observations of Be star HDE 245770=V 725 Tau, the optical counterpart of the transient X-ray pulsar A0535+26, having a pulse period of about 104 s, were conducted for more than 10 years. An irregular long-term optical variability of the star with amplitudes of the order of a few tenths of magnitude was found to be a usual phenomenon. In some cases rapid changes of the star's optical luminosity with a characteristic period of a few tens of minutes or a few hours, and an amplitude of several hundredths of magnitude in all the spectral bands used, which have practically coincided or correlated with the X-ray pulsar outbursts detected by X-ray satellites, were observed.Photoelectric recording of the optical flux from HDE 245770 were made in 1981–1982 with a time resolution of 1 second and 10 s, respectively, in theR spectral band (0 7000 Å) and in the narrowH
-emission-line band (1/2 75 Å) using a 48-cm reflector of High-Mountain Tien-Shan observatory of the Sternberg Astronomical Institute near Alma-Ata. An analysis of autocorrelation functions of the flux changes from object under study and a comparison with the star BD+26° 876 indicated the variability of luminosity of V 725 Tau in theR spectral band on a time scale of a few tens of second; this variability resembles shot noise with a characteristic time of stochastic bursts of about 15–20 s and their amplitudes of about a few tenths of a percent. InH
-emission-line radiation autocorrelation functions and power spectra show quasiperiodic variability of luminosity of HDE 245770 with a characteristic period of about 100–150 s and an amplitude in the neighbour-hood of 0.5%. The latter result is not quite reliable because of not quite fine weather conditions during the observations; independent observations and check-up are required. 相似文献
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