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1)  Orthogonal Function Spectrophotometry
正交函数分光光度法
2)  orthogonal function spectrophotometry
正交函数光谱法
3)  orthogonal projection spectrophotometry
正交投影分光光度法
1.
Determinations of SMZ and TMP in Xieliting tablets by orthogonal projection spectrophotometry;
正交投影分光光度法测定泻痢停片中TMP和SMZ的含量
2.
Two ingredients in sulfamethoxazole sulfadiazine and trimethoprim tablets were determined simultaneously by orthogonal projection spectrophotometry.
采用正交投影分光光度法同时测定 3组分复方药物联磺甲氧苄啶片中磺胺甲恶唑 (SMZ)和甲氧苄啶(TMP)二组分的含量。
4)  zero-crossing derivative spectrophotometry
零交导数分光光度法
1.
A zero-crossing derivative spectrophotometry method is established for the determination of ofloxacin in ofloxacin glucose injection.
用零交导数分光光度法测定氧氟沙星葡萄糖注射液中氧氟沙星的含量。
5)  Derivative spectrophotometry
导数分光光度法
1.
Determination of Conjugated Diene in Gasoline by the First Derivative Spectrophotometry;
一阶导数分光光度法测定汽油中共轭二烯烃
2.
In this paper a new method of using first order derivative spectrophotometry to determine the trace aluminium content in the solution of coloring trough for aluminium products has been suggested The results indicate that in the presence of OP emulsifier at pH5 0-7 0 Al with CAS can form a stable complex,the maximum absorbance is at 633.
提出了用一阶导数分光光度法测定铝材着色槽液中微量铝的方法 ,结果表明 ,在 pH5 0~ 7 0之间 ,乳化剂OP存在下 ,Al与铬天青S(CAS)形成稳定络合物 ,测定 6 33 0nm处的导数值 ,选择性大为提高 ,该方法用于铝材着色槽液中微量铝的测定 ,结果令人满意。
3.
By use of the derivative spectrophotometry and computer program, the 0-2 degree derivative curve graph is drawn and measuring parameter is determinated about the ephedrine hydrochloride nasal drops.
应用计算机图形分析技术结合普通(手动式)分光光度计进行导数分光光度法的测定。
6)  luminosity function
光度函数
1.
Inclination-Dependent Luminosity Function of Spiral Galaxies and the Statistic Analysis for Dust Extinction;
旋涡星系光度函数与倾角的关系及尘埃消光的统计分析
2.
On one hand, SAM can match the observations of local galaxy population, which include the luminosity function, the two-point correlation fu.
在引入一系列合理的关于重子物质物理过程的假设,如气体冷却、恒星形成率、超新星能量反馈以后, 结合N体数值模拟,星系形成的半解析模型一方面能较成功地预言许多与观测符合的近邻星系的性质,如光度函数、星系的两点相关函数、Tully-Fisher关系、星系团中椭圆星系的颜色-星等关系等;另一方面还能较成功地预言宇宙的恒星形成历史,以及一部分高红移星系的性质,如Lyman-Break星系的数目随红移的分布。
3.
We have derived the luminosity functions (LFs) of 198 member galaxies in the central region of the nearby cluster of galaxies Abell 2634 in the B,V and R bands.
 我们得到了邻近星系团Abell2634中心区域的198颗成员星系在B、V、R三个波段的光度函数,并且分别用Schechter函数和Gaussian函数及其组合进行了拟合。
补充资料:比色分析法(见紫外—可见分光光度法)


比色分析法(见紫外—可见分光光度法)


  比色分析法见萦外一可见分光光度法。
  
说明:补充资料仅用于学习参考,请勿用于其它任何用途。
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