Titan's atmosphere simulation experiment using a continuous-spectrum UV-VUV synchrotron beamline
Titan's atmosphere simulation experiment using a continuous-spectrum UV-VUV synchrotron beamline
复制标题
使用连续光谱 UV-VUV 同步加速器光束线的泰坦大气模拟实验
DOI：
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发表时间：
2012
期刊：
影响因子：
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通讯作者：
G. Cernogora
中科院分区：
文献类型：
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作者：
Zhe Peng;Thomas Gautier;N. Carrasco;Alexandre Giuliani;A. Mahjoub;J. Correia;P. Pernot;A. Buch;Y. Bénilan;C. Szopa;G. Cernogora
We report here a new reactor, named APSIS for Atmospheric Photochemistry SImulated by Synchrotron, where a gas mixture (N2/CH4=90/10) at various pressures in the mbar range in the reactor is irradiated using the continuous-spectrum (60-350 nm) DISCO beam in the SOLEIL Radiation Facility. The photochemical products, in situ detected by quadrupole mass spectrometry, include C2, C3, C4 and probably C5 compounds.We compared the neutral productions in APSIS and other experiments with the INMS measurements.
