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The formation of organic compounds in the atmosphere of Titan is an ongoing process of the generation of complex organics from the simplest hydrocarbon, methane. Solar radiation and magnetosphere electrons are the main energy sources that drive the reactions in Titan's atmosphere. Since energy from solar radiation is 200 times greater than that from magnetosphere electrons, we have investigated the...
Photochemical reaction pathways in Titan's atmosphere were investigated by irradiation of the individual components and the mixture containing nitrogen, methane, hydrogen, acetylene, ethylene, and cyanoacetylene. The quantum yields for the loss of the reactants and the formation of products were determined. Photolysis of ethylene yields mainly saturated compounds (ethane, propane, and butane) while...
Experimental studies were performed to simulate the action of long wavelength solar UV light on Titan’s atmosphere. The experiments were carried out in a photochemical flow reactor using a mixture of gases representative of Titan’s atmosphere at 70° north latitude (Titan’s north pole) in the winter. The solid analog of Titan’s haze formed has optical properties comparable to that determined for Titan’s...
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