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101.
采用动力学方程,求解了定态情况下磁层中上行离子沿磁力线的分布函数,针对不同的Kp指数,分别对北半球极光带区起源的上行离子O+、H+和He+在子午面内沿磁力线的密度分布及其特性进行了研究.结果表明:1.沿磁力线向外,上行离子密度在近地空间呈急剧下降趋势,在远地空间呈缓慢下降趋势;2.重离子或初始能量较小的离子,其密度沿磁力线向外下降较快;3.Kp指数越大,离子进入磁层的空间范围越大;4.离子的投掷角分布对密度分布的影响甚小;5.离子密度沿磁力线的下降程度随到X轴距离的增大而呈增大趋势;6.在典型参数条件下,求得上行离子O+在等离子体片边界附近的密度为10-3-10-2个cm-3,这与观测结果相一致. 相似文献
102.
彩色合成选择法是根据色度学原理,求出地物之间在各种彩色合成方案中的色差,以选择彩色合成方案。将此方法应用到黄河入海口,提取黄河水、海水、沙滩、陆地等主要地物信息,效果明显。 相似文献
103.
Using the data set of about 1 Hz Lg amplitudes from 80 stations in the six eastern provinces of China, the ratios of horizontal
to vertical amplitude of Lg waves,H/Z are determined. The mean lg(H/Z)-value is equal to 0.13. For the station bases of soft deposit,granite and sedimentary rock, lg(H/Z)-values average 0.55, 0.04 and 0.10, respectively. For the three kinds of station bases, the station terms of horizontal
amplitude,C
h
average 0.65, −0.09 and 0.00; that of vertical amplitude,C
z
average 0.32, −0.04 and 0.00, respectively. There are the relations betweenC
h
,C
z
and lg(H/Z):C
h
=0.01+2.10C
z
andC
h
=−0.15+1.46 lg(H/Z).
The Chinese version of this paper appeared in the Chinese edition ofActa Seismologica Sinica,13, 281–286, 1991.
Project sponsored by the Chinese Joint Seismological Science Foundation. 相似文献
104.
105.
The adsorption of H+, OH– and ARS (Alizarin Red S) onto hydrous fluorapatite surfaces and Ca2+—ARS complexation in solution were studied by means of combined potentiometric and spectrophotometric titrations, as well as zeta potential and FT-IR measurements. Corresponding equilibrium constants of surface and solution reactions are determined. The application in flotation processes is discussed. 相似文献
106.
The peculiar galaxy NGC 4650 A (α=12h 42m. 1; = δ—40° 26′; 1950·0) has been studied by means of direct and spectral observations with the ESO 3·6-m telescope. It is
interpreted as a prolate, elliptical galaxy surrounded by a warped ring of H II regions, dust and stars. The distance is 47
Mpc (H
0=55 km s−1 Mpc−1). The ring is seen nearly edge-on (inclination 85°) and it rotates. It has a diameter of about 21 kpc and is bluer than the
elliptical galaxy for which the (M/L
v) ratio is ∼12 in solar units. The observed configuration may be the result of interaction with the nearby galaxy, NGC 4650. 相似文献
107.
Jiankui?Shi?Email author Zhenxing?Liu Zhang?T.?L. Jianshan?Guo Manlian?Zhang Sheping?Shang Xigui?Luo 《中国科学D辑(英文版)》2003,46(10):986-993
Based on satellite observation data, using dynamics equation, the ionospheric O+ ion’s distribution in the synchronous altitude region for different geomagnetic activity indexK
p is studied by theoretical modeling and numerical analyzing, and semi-empirical models for the O+ ion’s density and flux versus longitude in the synchronous altitude region for differentK
p
are given. The main results show that in the synchronous altitude region: (i) The O+ ion’s density and flux in day-side are larger than those in nightside. (ii) With longitude changing, the higher the geomagnetic
activity indexK
p
is, the higher the O+ ion’s density and flux, and their variation amplitude will be. The O+ ion’s density and flux whenK
p ≥ 6 will be about ten times as great as that whenK
p
= 0. (iii) WhenK
p
= 0 orK
p ≥ 6, the O+ ion’s density reaches maximum at longitudes 120° and 240° respectively, and minimum in the magnetotail. WhenK
p
= 3−5, the O+ ion’s density gets to maximum at longitude 0°, and minimum in the magnetotail. However, the O+ ion’s flux reaches maximum at longitude 120° and 240° respectively, and minimum in the magnetotail for anyK
p
value. 相似文献
108.
Simple straightforward methods are applied to testtheir ability to detect the non-linear response of thesoil. Recordings of the main shock and aftershocks ofthe 1995, Hyogo-ken Nanbu (Kobe) earthquake are used.Non-linear effects are investigated using twodifferent techniques, on a collection of data for 12sites situated on different geological structures inthe Kobe and Osaka areas. The first method used is theso-called receiver functions technique (Langston,1979), which consists of computing the spectral ratiobetween horizontal and vertical components of motion.This ratio has been shown to reveal the fundamentalfrequency of a site (Lachet and Bard, 1994; Lachet etal., 1996; Theodulidis et al., 1995, 1996). For eachsite, recordings of the main shock and a set ofaftershocks are considered. The variation of thisspectral ratio for different values of the maximumacceleration recorded at a site is investigated. Bothvariations of the amplitude of the H/V ratio (due tonon-linear behavior, on the horizontal components inparticular) and of the frequency position of theamplified band-width are observed. The secondtechnique used in this study is related to thevariation of the high frequency content of therecordings during the main-shock and its aftershocks.The high frequency spectral decay of the motion,characterized by parameter, is assumed to berelated mainly to the near-surface attenuation. Itshould then increase with increasing peak velocity, incase of non-linearity. The value of kappa iscalculated for the 12 sites in the Kobe area, fordifferent types of soil conditions, and againdifferent values of peak ground acceleration.Variations of kappa are then related to non-linearbehavior of the soil during the Kobe earthquake. 相似文献
109.
抑制型离子色谱法同时测定水中锂和锶 总被引:2,自引:0,他引:2
对离子色谱法测定水中的锂、锶含量及其影响因素进行了研究。以甲烷磺酸为流动相,用IonPacCS12A阳离子色谱柱分离后,电导检测器同时测定矿泉水中锂和锶,其检出限分别为0.003mg/L和0.006mg/L。对Li^+和Sr^2+的离子色谱条件进行了优化,并对流动相的选择及干扰离子的影响进行了讨论。 相似文献
110.
采用马弗炉将样品与NaOH混合进行熔融煅烧,热去离子水提取、离心、稀释后过OnGuard Ⅱ H柱和过滤膜进行前处理,抑制型电导离子色谱法检测,测定了Ta2O5和Nb2O5的氟离子、氯离子和硫酸根离子。该方法对三种被测阴离子的检测限(s/N=3)在0.15~0.70μg/g(以固体样品实际浓度计)或0.136~0.623μg/L(以溶液浓度计),标准曲线线性范围均在两个数量级以上,方法的精密度(RSD,n=7)小于5.46%,回收率为88%~106%,具有灵敏度高、选择性好、重现性佳、对环境友好等特点,用于实际样品的检测,结果令人满意。 相似文献