968 resultados para ZnS-CdS


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研究了光、热和湿气对CdS/Cu2S电池效率及电池成结、结电容、二极管特性和光谱响应特性的影响。结果表明,对未成结电池光加速成结作用;对成结电池光引起电池性能下降。这种衰降是不可逆过程。

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Stable bilayer thin films of indium tin oxide (ITO) on CdS and CdS on ITO were formed for the window material of solar cells by chemical bath and sputtering methods. Scanning electron microscopy and X-ray diffraction studies have shown that both the ITO and CdS films are continuous, homogeneous, with high compactness. Measurement of the CdS film thickness across the 2 x 4 cm(2) reveals the good uniformity of these films. Four-point probe measurements show that the resistivity of a CdS film on an ITO surface is much better than that of the single CdS film The thermal stability of an ITO/CdS bilayer, interfacial reaction and optical transmittance were investigated at different annealing temperatures and environments (air, vacuum and N-2 + H-2). The results showed that the ITO/CdS bilayer film is a good window material for the CuInSe2 and CdTe cells. It is a simple method using a small amount of the cadmium compound.

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介绍了用化学水浴法沉积CdS的方法。SEM、XRD以及透射光谱等分析表明,沉积在玻璃片上的CdS膜,均匀、透明、密实,适合制作太阳电池窗口材料。同时简述了CdS膜生长、生成的化学过程和机理。

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本文着重从仪器本身参数方面和样品方面讨论了由于各参数的不同,对电子结合能的影响。通过半导体CdS膜的研究,探讨了Cd 3d5/2,Cd 3d3/2特征峰结合能的变化规律,分析了这种变化在测试中带来的影响。

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对薄膜CdS/Cu_2S光伏器件稳定性的研究表明,温度对电池寿命的影响是不可忽视的因素。J·Meikin指出,在40℃下对CdS/Cu_2S电池加热5000小时,Ⅰ_(sc)仅下降1%;对于包封电池,K.Boer得出,在60℃下加热两年电池性能没有发生衰变的结论。 我们通过对CdS/Cu_2S太阳电池的加热寿命试验,寻求器件寿命与温度间的关系,并用

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介绍了p-n结电容测量方法。通过测量C-V特性研究了Cds太阳电池的热处理及上栅过程,分析并讨论了p-n结的变化与电池不稳定的关系。初步研究了扩散电位的测定问题。

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本文综述了CdTe/CdS和CuInSe_2/CdS薄膜太阳电池的进展,讨论了这两种电池的发展前景。

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本文报道了CdS薄膜太阳电池制备条件对其性能的影响,并进行了详细讨论,同时提出了制备CdS薄膜太阳电池的最佳条件。

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本文报道了复合胶粘剂的制备和主要性能,介绍了封装技术,给出了用新合成的复合胶粘剂粘接玻璃封装电池的稳定性结果。

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本文报道了Cu、Fe、Zn对CdS晶体半导体参数和Cu_2S/CdS太阳电池性能的影响。随着Cu、Fe、Zn浓度的增加,电阻率也增加,掺Zn使禁带宽度E_g增大,迁移率μ降低,这些参数的变化,直接使电池的I_(sc)、效率和填充因子(F)降低。在本条件下,以上三种杂质都是受主杂质。掺氧能间接增加施主杂质,对受主杂质起补偿作用。

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本文叙述了在各种条件下Cu_2S/CdS太阳电池稳定性的研究,详细提出了氧气和水汽的数量同电池稳定性的关系,提出了温度和真空度对稳定性的影响,同时给出了稳定性与结型、结电容和串联电阻(R_s)的关系.对于上述结果进行了讨论,并提出了关于Cu_2S/CdS太阳电池衰降模型的新观点,最后用这个观点解释了某些衰降现象.

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Simultaneous observations of explosive chromospheric evaporation are presented using data from the Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI) and the Coronal Diagnostic Spectrometer (CDS) on board the Solar and Heliospheric Observatory. For the first time, cospatial imaging and spectroscopy have been used to observe explosive evaporation within a hard X-ray emitting region. RHESSI X-ray images and spectra were used to determine the flux of nonthermal electrons accelerated during the impulsive phase of an M2.2 flare. When we assumed a thick-target model, the injected electron spectrum was found to have a spectral index of similar to 7.3, a low-energy cutoff of similar to 20 keV, and a resulting flux of >= 4 x10(10) ergs cm(-2) s(-1). The dynamic response of the atmosphere was determined using CDS spectra; we found a mean upflow velocity of 230 +/- 38 km s(-1) in Fe (XIX) (592.23 angstrom) and associated downflows of 36 +/- 16 and 43 +/- 22 km s(-1) at chromospheric and transition region temperatures, respectively, relative to an averaged quiet- Sun spectra. The errors represent a 1 j dispersion. The properties of the accelerated electron spectrum and the corresponding evaporative velocities were found to be consistent with the predictions of theory.

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This article examines the impact of pension deficits on default risk as measured by the premia on corporate credit default swaps (CDS). We find highly significant evidence that unfunded pension liabilities raise one- and five-year CDS premia. However, this relation is not homogeneous across countries, with the U.S. CDS market leading its European counterparts in the pricing of defined-benefit pension risk.