Abstract Transionospheric radio signals may experience fluctuations in their amplitude and phase due to irregularity in the spatial electron density distribution, referred to as scintillation. Ionospheric scintillation is responsible for transionospheric signal degradation that can affect the performance of satellite based navigation systems. Usually, the scintillation activity is measured by means of indices such as the normalised standard deviation of the received intensity S 4 and the standard deviation of the received phase σ ϕ typically calculated over 1min of data. Data from a GPS scintillation monitor based on 50Hz measurements recorded at Dirigibile Italia Station (Ny-Alesund, Svalbard), in the frame of the ISACCO project () are used to investigate possible adoption of an alternative parameter for the estimate of phase fluctuations: i.e., the standard deviation of the phase rate of change S ϕ. This parameter is shown to better correlate with S 4 being much less detrending dependent than σ ϕ. The couple (S 4, S ϕ) should be then considered a more physical proxy of radio scintillation than the couple (S 4, σ ϕ).
Optimum parameter for estimating phase fluctuations on transionospheric signals at high latitudes
Advances in Space Research ; 47 , 12 ; 2188-2193
2010-04-23
6 pages
Article (Journal)
Electronic Resource
English
Optimum parameter for estimating phase fluctuations on transionospheric signals at high latitudes
Online Contents | 2011
|Transionospheric propagation of FM signals
NTRS | 1967
|Effects on transionospheric HF propagation observed by ISIS at middle and auroral latitudes
Online Contents | 2006
|