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 at altitu...
保存先:
| 第一著者: | |
|---|---|
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
Copernicus Publications
2016-08-01
|
| シリーズ: | Nonlinear Processes in Geophysics |
| オンライン･アクセス: | http://www.nonlin-processes-geophys.net/23/215/2016/npg-23-215-2016.pdf |
| タグ: |
タグなし, このレコードへの初めてのタグを付けませんか!
|