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Anregung von UV-Strahlung in Stickstoff und Wasserstoff durch einen Elektronenschwarm

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Zeitschrift für Physik

Abstract

The radiation excited in nitrogen and hydrogen by an electron swarm moving in a uniform electric field is investigated. In nitrogen the bands of the 2nd positive group in the region from 3400 to 3800 Å are the dominating part of the radiation. In hydrogen the main part of the radiation is lying in the far ultraviolet (1000 to 1200 Å) due to the excitation of the state 21 II u . The coefficientδ describing the intensity of the radiation is measured with a photomultiplier device as a function of the electric fieldE and the pressurep in the range from about 10 to 100 Torr. Besides the dependence ofδ onE/p a pressure dependence is found which is explained as a quenching process of the excited molecules by collisions. The pressurep 0 for equal probability of radiating and non-radiating decay of the states involved is 60 Torr in N2 and 20 Torr in H2. The theoretical interpretation of the dependence onE/p supports the excitation energy of the state C3 II u of N2 for electron impact to be equal to the spectroscopical value of 11·04 eV and yields 0·9·10−16 cm2 for the maximum of the excitation cross section. The results of the measurements in H2 can be described assuming a cross section of 0·55·10−16 cm2 for the excitation of the state 21 II u by electron impact.

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Herrn Professor Dr. H.Raether danke ich für die Anregung zu dieser Arbeit, die von der Deutschen Forschungsgemeinschaft in dankenswerter Weise durch die Bereitstellung des Spektrographen und eines Monochromators unterstützt wurde.

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Legler, W. Anregung von UV-Strahlung in Stickstoff und Wasserstoff durch einen Elektronenschwarm. Z. Physik 173, 169–183 (1963). https://doi.org/10.1007/BF01377958

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  • DOI: https://doi.org/10.1007/BF01377958

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