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High Temperature Material Processes: An International Quarterly of High-Technology Plasma Processes
SJR: 0.137 SNIP: 0.341 CiteScore™: 0.43

ISSN Imprimir: 1093-3611
ISSN En Línea: 1940-4360

High Temperature Material Processes: An International Quarterly of High-Technology Plasma Processes

DOI: 10.1615/HighTempMatProc.v13.i3-4.100
pages 373-379

PLASMA SOURCE FOR THE EMULATION OF THE ATMOSPHERIC FLUORESCENCE PRODUCED BY THE SECONDARIES OF ULTRA HIGH ENERGY COSMIC RAY PARTICLES

E. Fokitis
National Technical University of Athens, 15780 Zografos, Athens, Greece
V. Gika
National Technical University of Athens, 15780 Zografos, Athens, Greece
P. Fetfatzis
National Technical University of Athens, 15780 Zografos, Athens, Greece
S. Maltezos
National Technical University of Athens, 15780 Zografos, Athens, Greece
I. Kouretis
National Technical University of Athens, 15780 Zografos, Athens, Greece
N. Antonakakis Spyropoulos
National Technical University of Athens, 15780 Zografos, Athens, Greece

SINOPSIS

An application of plasma effect for the emulation of the fluorescence emerging along the Extensive Air Showers created by the nuclear interactions of Ultra High Energy Cosmic ray particles with the atmosphere is presented. We designed and used an appropriate high-resolution spectrograph in order to study the spectral lines of nitrogen atmospheric molecules. We are aiming to achieve adequate signal to noise ratio, in a running period in operating accelerator experiments using electron beams at high energies, so that the main N2 peaks in the UV region as well as their rotational excitations are resolved. The designed spectrograph constitutes a compromise between the sufficient resolution and the required sensitivity demands. For the emulation, a low pressure spectral lamp filled with air is used and typical spectra are presented. Our facility can be of use in studying other plasma spectral features at about 0.05 nm resolution.


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