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Spectral characteristics of high-latitude raw 40 MHz cosmic noise signals
Cosmic noise at 40 MHz is measured at Ny-Ålesund (79° N, 12° E) using a relative ionospheric opacity meter ("riometer"). A riometer is normally used to determine the degree to which cosmic noise is absorbed by the intervening ionosphere, giving an indication of ionisation of the atmosphere...
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Formato: | Artigo |
Idioma: | Inglês |
Publicado em: |
Copernicus Publications
2016-08-01
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Colecção: | Nonlinear Processes in Geophysics |
Acesso em linha: | http://www.nonlin-processes-geophys.net/23/215/2016/npg-23-215-2016.pdf |
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