Shock Wave Generated Megahertz Radiation of Atmosphere

Autor: Sven G. Bilén, A. H. Mkrtchyan, H.F. Khachatryan, Michel Parrot, L.Sh. Grigoryan, A.V. Sargsyan, A. R. Aramyan
Přispěvatelé: Institute of Applied Problems in Physics NAS RA, Department of Electrical and Systems Engineering, University of Pennsylvania [Philadelphia], Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Institute for Physical Research (IPR), National Academy of Sciences of the Republic of Armenia [Yerevan] (NAS RA)
Rok vydání: 2019
Předmět:
Zdroj: IEEE Transactions on Plasma Science
IEEE Transactions on Plasma Science, Institute of Electrical and Electronics Engineers, 2019, 47 (1), pp.118-120. ⟨10.1109/TPS.2018.2870925⟩
ISSN: 1939-9375
0093-3813
Popis: International audience; Based on intuitive reasoning and a simple mathematical model, it is shown that the radio frequency electromagnetic radiation in 1-2-MHz range is generated during the propagation of a directed strong shock wave in air. It is due to the radiation from free electrons (which are produced by the shock wave) in the magnetic field of the earth. The possibility of detection of this radiation is discussed
Databáze: OpenAIRE