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991.
We present the high resolution absorption measurements of gaseous HONO at room temperature using continuous-wave cavity ring-down spectroscopy in the near-infrared region between 6017 and 6067 cm−1 at a resolution of 1 pm (0.037 cm−1). For the trans-HONO isomer an extensive analysis of the ν1+2ν3 combination band 6045.8089 cm-1 was performed starting from the results of a previous study for the 11 and 31 vibrational states [Guilmot J-M, Godefroid M, Herman M. Rovibrational parameters for trans-nitrous acid. J Mol Spectrosc 1993;160:387-400]. The present combination band is perturbed because of the existence of several dark states of HONO which could not be identified unambiguously. The rotational constants achieved for the 1132 state deviate slightly from the values which are predicted from the rotational constants achieved in the previous studies for the 11 and 31 vibrational states of trans-HONO.  相似文献   
992.
High precision rotational spectra of isotopic oxygen O2 (with or ) in its electronic ground state have been measured in selected frequency regions between 0.4 and 2.0 THz. The main isotopic species, , was also investigated in its first excited electronic state . The new data, analyzed together with previous measurements, yielded improved spectroscopic parameters.  相似文献   
993.
As a tetrahedral molecule, methane has no permanent dipole moment. Its spectrum, however, displays faint absorption lines in the THz region, due to centrifugal distorsion effects. This is important for planetary applications since this region is used to measure methane concentration in some planetary atmospheres, in particular on Titan. Up to now, all measurements relied either on some old low resolution infrared absorption spectra, or on high resolution Stark measurements for low J values only. Even if these results have been reexamined recently [Wishnow EH, Orton GS, Ozier I, Gush HP. The distorsion dipole rotational spectrum of CH4: a low temperature far-infrared study. J Quant Spectrosc Radiat Transfer 2007;103:102-17], it seemed highly desirable to obtain much more precise laboratory data.The high-intensity synchrotron radiation, combined with a 151.75±0.1 m optical path in a White cell and a Bruker IFS 125 HR FTIR spectrometer at the AILES beamline of SOLEIL, enabled us to record this very weak spectrum at high resolution for the first time. Spectra were obtained in the 50-500 cm−1 wavenumber range at 296 K and 9.91, 20, 50 and 100 mbar with a resolution of 0.00074, 0.00134, 0.0034 and 0.0067 cm−1 (FWHM of the sinc function), respectively. The rotational clusters are fully resolved and the good signal-to-noise ratio has enabled precise measurements of transition intensities (92 cold band lines and 96 Dyad-Dyad hot band lines, with normal abundance intensities in the range 2×10−26-1×10−24 cm−1/(mol cm−2)), yielding an accurate determination of the dipole moment derivatives. Such results should allow a better determination of CH4 concentration in planetary objects.  相似文献   
994.
Optimization of nitroxides as probes for EPR imaging requires detailed understanding of spectral properties. Spin lattice relaxation times, spin packet line widths, nuclear hyperfine splitting, and overall lineshapes were characterized for six low molecular weight nitroxides in dilute deoxygenated aqueous solution at X-band. The nitroxides included 6-member, unsaturated 5-member, or saturated 5-member rings, most of which were isotopically labeled. The spectra are near the fast tumbling limit with T1T2 in the range of 0.50–1.1 μs at ambient temperature. Both spin–lattice relaxation T1 and spin–spin relaxation T2 are longer for 15N- than for 14N-nitroxides. The dominant contributions to T1 are modulation of nitrogen hyperfine anisotropy and spin rotation. Dependence of T1 on nitrogen nuclear spin state mI was observed for both 14N and 15N. Unresolved hydrogen/deuterium hyperfine couplings dominate overall line widths. Lineshapes were simulated by including all nuclear hyperfine couplings and spin packet line widths that agreed with values obtained by electron spin echo. Line widths and relaxation times are predicted to be about the same at 250 MHz as at X-band.  相似文献   
995.
A tunable diode laser spectrometer has been employed to examine the 3rd overtone absorption lines of C2H4 at around 12 000 cm−1 (830 nm). The spectrometer sources are heterostructure AlGaAs tunable diode lasers operating “free-running”. By the aid of the wavelength modulation spectroscopy with the second harmonic detection technique and a Herriott type multipass cell 63 very weak absorption lines have been observed for the first time, with cross sections as low as 2 × 10−26 cm2/mol, equivalent to . The self-broadening coefficient has been measured for one of the most intense lines.  相似文献   
996.
In this paper we described how different line coding techniques vary with values of jitter in soliton transmission system. Then the idea of this soliton transmission system is applied for multiuser structure and effects of initial line phase spacing are examined.  相似文献   
997.
为了提高大靶面交汇测量系统的测量准确度,分析了交汇测量原理,推导出脱靶量坐标公式.根据脱靶量公式分析其各项参量,利用几何关系建立像元坐标与偏移角度之间的映射模型.根据映射模型,利用光栅尺设计了一种针对线阵相机的标定方法,该方法不考虑相机参量,将整个光学系统看作一个整体,基于整体参量直接对像元坐标和它所对应的偏移角进行标定.实验结果表明,标定后的交汇测量系统在1.4m处的平均测量误差为0.4mm,最大测量误差优于0.6mm.该方法简单高效,可提高系统标定的速度,且标定误差满足系统交汇测量准确度的要求.  相似文献   
998.
为了研究储能电容初始电压、电极间距、充气压及灯管内径等条件对脉冲氙灯电流脉冲和发光脉冲的影响,在电极间距100~300mm、充气压13.33~53.32kPa、灯管内径6~12mm、储能电容初始电压1.75~4.25kV的条件下,分别测量了脉冲氙灯的电流脉冲和发光脉冲的变化状况。测量得到脉冲氙灯的电流脉冲宽度和发光脉冲宽度均在15~45μs之间。对比发现:储能电容初始电压较高有助于获得高峰值、窄脉宽且滞后时间短的电流脉冲;具有较高充气压或较长电极间距的脉冲氙灯其电流脉冲与发光脉冲的峰值较小、脉冲宽度较大,且发光脉冲滞后时间较长;较粗灯管内径虽然可以增加电流脉冲的峰值,但电流脉冲的宽度被增宽,发光脉冲峰值减小,发光脉冲宽度展宽,且延长了发光脉冲的滞后时间.  相似文献   
999.
Based on a relativistic quark model approach, the transition properties of the first nucleon resonance △(1232), and the coupling constants gπNN, g△πN are investigated. Tvo different vays to remove the center of mass motion are considered. The results of the relativistic approaches with and without center ofmass correction are compared with those of nonrelativistic constituent quark model. Moreover, pion meson cloud effect on these calculated observables is explicitly addressed. Better results are obtained by taking the pion meson cloud into account.  相似文献   
1000.
用信息熵描述非线性光传输的研究   总被引:2,自引:0,他引:2  
田野  刘承宜  郭旗  胡巍 《光学学报》2002,22(7):13-818
结合光束传输的薛定谔形式理论,基于量子机制的信息熵被用来描述非线性光传输,理论推导和数值模拟结果表明:信息熵及其对光传输方向的变化率可以表征光脉冲的压缩或展宽或光束的聚焦与发散,用信息熵表征非线性光传输优于对用脉(束)宽,二阶矩表征。  相似文献   
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