An NLO hyperbranched polymer （HP1） derived from both ＂H＂-type and star-type chromophores was synthesized successfully for the first time with high yield via one-pot ＂A2 ＋ B3＂ Suzuki polymerization reaction. Iso...An NLO hyperbranched polymer （HP1） derived from both ＂H＂-type and star-type chromophores was synthesized successfully for the first time with high yield via one-pot ＂A2 ＋ B3＂ Suzuki polymerization reaction. Isolation chromophore was also introduced to further improve its performance. Although under the test conditions, the films of HP1 could not be poled completely, it still demonstrated satisfactory macroscopic NLO effect with the second harmonic generation （SHG） coefficient d33 value of 36 pm/V.展开更多
The multiple access fashion is a new resolution for the star-type local area network (LAN) access control and star-type optical fibre LAN. Arguments about this network are discussed, and the results are introduced.
我国正在实施的大型巡天项目(LAMOST项目),急需恒星光谱自动识别与分类系统并给出了一种基于光谱特征的恒星自动识别方法。该方法由以下主要步骤组成:(1)利用谱线小波特征进行恒星谱线整体估计和恒星Balmer线的检测;(2)利用吸收带小波...我国正在实施的大型巡天项目(LAMOST项目),急需恒星光谱自动识别与分类系统并给出了一种基于光谱特征的恒星自动识别方法。该方法由以下主要步骤组成:(1)利用谱线小波特征进行恒星谱线整体估计和恒星Balmer线的检测;(2)利用吸收带小波特征进行吸收带位置和M型星特征频率检测;(3)根据以上检测结果进行发射线星、M型星和早型恒星识别。通过对(sloan digital sky survey,SDSS)(data releasefour,DR4)中的大量真实光谱数据实验表明,方法具有对噪声鲁棒等特点,发射线星识别率达到97.5%,M型星识别率达到98.1%,早型恒星识别率达到96.8%,类星体和星系的误识别率低于2%。该方法可对相对定标的巡天光谱进行自动识别,符合LAMOST数据的要求。展开更多
基金supported by the National Natural Science Foundation of China(No.21034006)
文摘An NLO hyperbranched polymer （HP1） derived from both ＂H＂-type and star-type chromophores was synthesized successfully for the first time with high yield via one-pot ＂A2 ＋ B3＂ Suzuki polymerization reaction. Isolation chromophore was also introduced to further improve its performance. Although under the test conditions, the films of HP1 could not be poled completely, it still demonstrated satisfactory macroscopic NLO effect with the second harmonic generation （SHG） coefficient d33 value of 36 pm/V.
文摘The multiple access fashion is a new resolution for the star-type local area network (LAN) access control and star-type optical fibre LAN. Arguments about this network are discussed, and the results are introduced.
文摘我国正在实施的大型巡天项目(LAMOST项目),急需恒星光谱自动识别与分类系统并给出了一种基于光谱特征的恒星自动识别方法。该方法由以下主要步骤组成:(1)利用谱线小波特征进行恒星谱线整体估计和恒星Balmer线的检测;(2)利用吸收带小波特征进行吸收带位置和M型星特征频率检测;(3)根据以上检测结果进行发射线星、M型星和早型恒星识别。通过对(sloan digital sky survey,SDSS)(data releasefour,DR4)中的大量真实光谱数据实验表明,方法具有对噪声鲁棒等特点,发射线星识别率达到97.5%,M型星识别率达到98.1%,早型恒星识别率达到96.8%,类星体和星系的误识别率低于2%。该方法可对相对定标的巡天光谱进行自动识别,符合LAMOST数据的要求。
