Reaction of ammonia and dioxygen in solid neon excited with far-ultraviolet radiation investigated with electronic and vibrational spectra

Author(s):  
Sheng-Lung Chou ◽  
J F Ogilvie ◽  
Jen Iu Lo ◽  
Yu-Chain Peng ◽  
Bing-Ming Cheng

Irradiation of dilute mixtures of NH3 and O2 dispersed in solid Ne at 3.6 K with radiation of wave lengths 200, 192.5, 173 and 143 nm from an electron synchrotron initiated photochemical dissociation of those precursors and the production of N, NH, NH2, O, O3, HO2, NO, NO2, N2O, H2O, HONO in both s-cisoid and s-transoid rotational isomers, and HONO2, detected according to their spectra in mid-infrared absorption from 450 to 4000 cm-1, and in absorption and emission from 200 to 1100 nm. HONO2 was not previously detected in related experiments even though our conditions were much more dilute.

2018 ◽  
Vol 20 (11) ◽  
pp. 7730-7738 ◽  
Author(s):  
Sheng-Lung Chou ◽  
Jen-Iu Lo ◽  
Yu-Chain Peng ◽  
Hsiao-Chi Lu ◽  
Bing-Ming Cheng ◽  
...  

Irradiation of O2 dispersed in solid Ne near 4 K at 173 or 143 nm produced many new spectral lines of O, O2 and O3 in absorption and emission spectra.


2021 ◽  
Vol 13 (8) ◽  
pp. 1454
Author(s):  
Anatoliy A. Nusinov ◽  
Tamara V. Kazachevskaya ◽  
Valeriya V. Katyushina

Modeling the upper atmosphere and ionospheres on the basis of a mathematical description of physical processes requires knowledge of ultraviolet radiation fluxes from the Sun as an integral part of the model. Aeronomic models of variations in the radiation flux in the region of extreme (EUV) and far (FUV) radiation, based mainly on the data of the last TIMED mission measurements of the solar spectrum, are proposed. The EUVT model describes variations in the 5–105 nm spectral region, which are responsible for the ionization of the main components of the earth’s atmosphere. The FUVT model describes the flux changes in the 115–242 nm region, which determines heating of the upper atmosphere and the dissociation of molecular oxygen. Both models use the intensity of the hydrogen Lyman-alpha line as an input parameter, which can currently be considered as one of the main indices of solar activity and can be measured with relatively simpler photometers. A comparison of the results of model calculations with observations shows that the model error does not exceed 1–2% for the FUVT model, and 5.5% for EUVT, which is sufficient for calculating the parameters of the ionosphere and thermosphere.


2006 ◽  
Vol 75 (2) ◽  
pp. 023703 ◽  
Author(s):  
Hidekazu Okamura ◽  
Masato Matsubara ◽  
Koichiro Tanaka ◽  
Kazutoshi Fukui ◽  
Mitsushi Terakami ◽  
...  

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