1.27μm波段的氧分子近红外气辉是火星大气最重要的气辉辐射之一,该气辉高光谱分辨辐射传输模型的建立对于研制火星探测载荷,反演火星大气的风场温度场与臭氧浓度,以及研究火星空间物理,有重要的科学价值与工程意义.在研究火星大气O_(2)...1.27μm波段的氧分子近红外气辉是火星大气最重要的气辉辐射之一,该气辉高光谱分辨辐射传输模型的建立对于研制火星探测载荷,反演火星大气的风场温度场与臭氧浓度,以及研究火星空间物理,有重要的科学价值与工程意义.在研究火星大气O_(2)(a^(1)Δ_(g))气辉光化学反应模型的基础上,提出了O_(2)(a^(1)Δ_(g))气辉体辐射率的计算方法,并建立了火星大气气辉辐射传输理论;通过与用于研究火星大气特征的光谱学探测仪(Spectroscopy Spectrograph for the Investigation of Characteristics of the Atmosphere of Mars,SPICAM)的实测数据进行对比,验证了所建立的火星O_(2)(a^(1)Δ_(g))气辉高光谱分辨辐射传输模型的准确性;针对火星与地球大气的O_(2)(a^(1)Δ_(g))气辉,在体辐射率、自吸收效应,以及临边辐射光谱特性三个方面进行了系统深入的比较,对比结果表明,火星大气由于密度低、氧气丰度小,其自吸收效应可以忽略不计,但其O_(2)(a^(1)Δ_(g))气辉辐射强度与地球大气相当,可以用于火星大气的风场温度场与臭氧浓度的探测与反演.展开更多
A series of CexPr1-xO2-δ mixed oxides were synthesized by sol-gel met hod and characterized by Raman and XRD techniques. When x value was changed from 1.0 to 0.5, only a cubic phase CeO2 was observed. The samples wer...A series of CexPr1-xO2-δ mixed oxides were synthesized by sol-gel met hod and characterized by Raman and XRD techniques. When x value was changed from 1.0 to 0.5, only a cubic phase CeO2 was observed. The samples were very well cr ystallized on decreasing x from 0.50 to 0.99. For CexPr1-xO2-δ samples 465 cm-1 and 1 150 cm-1 Raman peaks are attributed to the Raman active F2g mode of CeO2. The broad peak at about 570 cm-1 in the region of 0.3 ≤ x ≤ 0.99 can be linke d to lattice defects resulting in oxygen vacancies. The new band at about 195 cm -1 may be attributed to the asymmetric vibration caused by the formation of oxyg en vacancies. Calcination temperatures had great effect on the peak intensity fo r CeO2 but less effect on Ce0.8Pr0.2O2-δ in Raman spectra. It might be due to t he transformation of the colors for the mixed oxides, the insertion of Pr atom i nto the ceria lattice could enhance the sintering resistance and thermal stabili ty of the mixed oxides.展开更多
该研究中一种钌(Ⅱ)基配合物[Ru(phen)_(3)][PF_(6)]_(2)(phen=1,10-phenanthroline)被成功合成,用^(1)H NMR、FTIR和UV-vis表征其结构,并研究其在可见光下催化降解盐酸四环素(TC·HCl)的性能和影响因素。结果表明,该配合物在可见...该研究中一种钌(Ⅱ)基配合物[Ru(phen)_(3)][PF_(6)]_(2)(phen=1,10-phenanthroline)被成功合成,用^(1)H NMR、FTIR和UV-vis表征其结构,并研究其在可见光下催化降解盐酸四环素(TC·HCl)的性能和影响因素。结果表明,该配合物在可见光下能有效催化TC·HCl的降解,影响TC·HCl降解的主要因素是体系的pH值和溶解氧含量。在20℃、辐照强度50 mW/cm^(2)、[Ru(phen)_(3)][PF_(6)]_(2)和TC·HCl浓度分别为6.4 mg/L和20 mg/L的条件下,pH值由4增加到10,5 h TC·HCl降解率由7.8%增至88.9%。pH值为7.5时,去除体系溶解氧,5 h TC·HCl降解率由61.9%降至10.7%。TC·HCl降解过程复杂,主要涉及的活性种为单线态氧。展开更多
文摘1.27μm波段的氧分子近红外气辉是火星大气最重要的气辉辐射之一,该气辉高光谱分辨辐射传输模型的建立对于研制火星探测载荷,反演火星大气的风场温度场与臭氧浓度,以及研究火星空间物理,有重要的科学价值与工程意义.在研究火星大气O_(2)(a^(1)Δ_(g))气辉光化学反应模型的基础上,提出了O_(2)(a^(1)Δ_(g))气辉体辐射率的计算方法,并建立了火星大气气辉辐射传输理论;通过与用于研究火星大气特征的光谱学探测仪(Spectroscopy Spectrograph for the Investigation of Characteristics of the Atmosphere of Mars,SPICAM)的实测数据进行对比,验证了所建立的火星O_(2)(a^(1)Δ_(g))气辉高光谱分辨辐射传输模型的准确性;针对火星与地球大气的O_(2)(a^(1)Δ_(g))气辉,在体辐射率、自吸收效应,以及临边辐射光谱特性三个方面进行了系统深入的比较,对比结果表明,火星大气由于密度低、氧气丰度小,其自吸收效应可以忽略不计,但其O_(2)(a^(1)Δ_(g))气辉辐射强度与地球大气相当,可以用于火星大气的风场温度场与臭氧浓度的探测与反演.
文摘A series of CexPr1-xO2-δ mixed oxides were synthesized by sol-gel met hod and characterized by Raman and XRD techniques. When x value was changed from 1.0 to 0.5, only a cubic phase CeO2 was observed. The samples were very well cr ystallized on decreasing x from 0.50 to 0.99. For CexPr1-xO2-δ samples 465 cm-1 and 1 150 cm-1 Raman peaks are attributed to the Raman active F2g mode of CeO2. The broad peak at about 570 cm-1 in the region of 0.3 ≤ x ≤ 0.99 can be linke d to lattice defects resulting in oxygen vacancies. The new band at about 195 cm -1 may be attributed to the asymmetric vibration caused by the formation of oxyg en vacancies. Calcination temperatures had great effect on the peak intensity fo r CeO2 but less effect on Ce0.8Pr0.2O2-δ in Raman spectra. It might be due to t he transformation of the colors for the mixed oxides, the insertion of Pr atom i nto the ceria lattice could enhance the sintering resistance and thermal stabili ty of the mixed oxides.
文摘该研究中一种钌(Ⅱ)基配合物[Ru(phen)_(3)][PF_(6)]_(2)(phen=1,10-phenanthroline)被成功合成,用^(1)H NMR、FTIR和UV-vis表征其结构,并研究其在可见光下催化降解盐酸四环素(TC·HCl)的性能和影响因素。结果表明,该配合物在可见光下能有效催化TC·HCl的降解,影响TC·HCl降解的主要因素是体系的pH值和溶解氧含量。在20℃、辐照强度50 mW/cm^(2)、[Ru(phen)_(3)][PF_(6)]_(2)和TC·HCl浓度分别为6.4 mg/L和20 mg/L的条件下,pH值由4增加到10,5 h TC·HCl降解率由7.8%增至88.9%。pH值为7.5时,去除体系溶解氧,5 h TC·HCl降解率由61.9%降至10.7%。TC·HCl降解过程复杂,主要涉及的活性种为单线态氧。
