1.
The width,field and phase in temporal and spectral domains are retrieved.
得到了飞秒脉冲的时间宽度及光谱宽度、电场及其相位在时域和频域的详细信息。
2.
Estimating the spectral bandwidth of pulsed Doppler signal with the stationarising method
利用平稳性提高法估计脉冲多普勒信号的频谱宽度
3.
Detection of ribbon objects based on the cross-projection width spectrum
基于正交投影宽度谱的带状目标检测
4.
During unsaturated growth, the width of the spectral profile will decrease.
在非饱和增长期间，谱线轮廓的宽度将减
5.
Measurement of Ion Temperature of Plasma Using Doppler Broadening of Spectral Line
利用谱线的多普勒展宽测定等离子体离子温度
6.
The Correlation Between Broad-band Spectral Index and Luminosity for XBLs and RBLs;
XBLs和RBLs间的光度与宽波段谱指数的相关性分析
7.
Growth of High Precision Anti-Reflectance Multilayers under Broadband Monitoring and Controlling
宽光谱监控法镀制高精度增透膜的研究
8.
The symmetry properties of the optical coherence with respect to the detuning of the light frequency from resonance show up in specific symmetries of the spectra.
研究表明，透射光谱随薄膜厚度的增大而展宽，光谱呈现对称性。
9.
EXTRACTION OF THE DOPPLER VELOCITY SPECTRAL WIDTH FROM CONVENTIONAL INCOHERENT WEATHER ECHOES--AN ANALYSIS OF THE FLUCTUATING SPECTRUM OF ECHO INTENSITY
用非相干的常规天气雷达提取多普勒速度谱宽——回波强度涨落谱分析
10.
In astronomical situations, the natural line width is seldom directly observed.
在天文学研究中，谱线固有宽度很少能直接观测到。
11.
The Detection and Estimation of Carrier Frequency、Chip Width and Amplitude of DS Signal Based on Cyclic Spectrum Theory
基于循环谱理论的直扩信号检测与载频、码片时宽和幅度估计
12.
Influence of Spectrum Width of Optical Source on the Sensitivity of Fabry-Perot Optical Fiber Hydrophone;
光源谱宽对法布里—珀罗光纤水听器灵敏度的影响
13.
High Intensity Light with Wide Spectrum's Primary Research to Acne on Clinical Treatment and Antimicrobial Effect
高强度宽谱红光对痤疮临床治疗及体外抗菌作用的初步研究
14.
Calculation of Electron Density for Lightning Discharge Plasma by NI 493.5 nm Line Stark Broadening
NI 493.5 nm谱线Stark加宽估算闪电放电等离子体电子密度
15.
In signal analysis the Du transform is used to convert signals from the time domain into the gate width domain, thus the characters of signals can usually be represented by their width spectra.
杜氏变换是一种将信号从时域到门宽域的变换,用信号的宽谱密度来描述信号的特征。
16.
Optical System Design of a Star Srnsor with Wide Spectrum and Wide Field of View
宽谱段宽视场星敏感器光学系统设计
17.
The magnitude of the turbulence then follows directly from the observed line with if the nebular gas temperature is known.
如果已知星云气体的温度，则湍流的大小可直接从观测的谱线宽度得出。
18.
Difference in filament and spectrum broadening induced by femtosecond pulses in argon gas with a temperature gradient at different positions
飞秒激光在不同位置温度梯度的惰性气体中成丝及光谱展宽的差异