Cross-correlation functions of spherical waves propagating through a slab containing anisotropic irregularities.
Cross correlation of satellite signals through slab containing small anisotropic irregularities
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Cross correlation of satellite signals through slab containing small anisotropic irregularities
Explorer XX topside sounder observations of ionospheric irregularities in electron density and plasma wave electrostatic resonances
Diurnal variation of ionospheric irregularities, using differential Doppler method for analysis of data transmitted by Beacon satellite
Ionospheric E region irregularities produced by nonlinear coupling of unstable plasma waves
Ionospheric irregularities explained by gravitational field and positive electron density gradient joint effect on ionospheric region below electron distribution peak
F region irregularities studied by scintillation of radio signals from earth satellites
F layer irregularities transverse scale measurements by two-frequency scintillation-ratio technique yielding 600-700 m scales in auroral zone
The rate of TEC index (ROTI) is a measurement that characterizes ionospheric irregularities. It can be obtained from standard GNSS dual-frequency phase data collected using a geodetic type of GNSS receiver. By processing GPS data from ground-based networks of International GNSS Service and Continuously Operating Reference Station (CORS), ROTI maps have been produced to observe global and regional scintillation activities. A major mid-latitude scintillation event in the contiguous United States is reported here that was captured in ROTI maps produced using CORS GPS data collected during a space weather storm. The analyses conducted in this work and previously by another group indicate that ROTI is a good occurrence indicator of both amplitude and phase scintillations of GPS L-band signals, even though the magnitudes of ROTI, S4, and sigma(sub phi) can be different. For example, our analysis indicates that prominent ROTI and the L1 phase scintillation (sigma(sub phi)) are well correlated temporally in the polar region while L1 amplitude scintillation rarely occurs. The differences are partially attributed to physics processes in different latitude regions, such as high-speed plasma convection in the polar region that can suppress the amplitude scintillation. An analysis of the impact of ionospheric scintillation on precise positioning, which requires use of dual-frequency phase data, is also conducted. The results indicate that significant (more than an order of magnitude) positioning errors can occur under phase scintillation conditions.
Diffraction of hf radio waves by ionospheric irregularities - radiation from artificial satellites
Variations in fading period of radio signals from explorer vii satellite used to study electron density irregularities in the ionosphere
Scintillation of radio transmissions from discoverer 38 to determine the existance and nature of diffracting e-region irregularities
Analysis of the amplitude and phase diffraction patterns of radio signals from the transit 4a satellite and their relationship to ionospheric irregularities
Study of the irregularities in the ionospheric electron density, based on variations in the fading period of signals from explorer vii
Angular scattering from irregularly shaped particles with application to astronomy
Dimensions of ionospheric irregular formations by observations on cosmos i, ii, and xi satellites in coherent frequencies
Accurate periods of periodic events observed at irregular intervals of time
Ionized gas in elliptical, SO, spiral, and irregular galaxy nuclei