In this paper, based on the characteristic of incoherent scattering observations of the MU radar, a synthetic data is generated to investigate errors in the wave propagation by using the Fourier analysis.
We present European Incoherent Scatter (EISCAT) observations of spectrally uniform ion line power enhancements (SUIPE), where the up- and downshifted shoulder and the spectral valley between them are enhanced simultaneously and equally.
We examine the performance of the Global Self-Consistent Mofel of Thermosphere, Ionosphere and Protonosphere (GSM TIP) and International Reference Ionosphere-2000 Ionosphere-2000 IRI-2000 IRI-2000ing predictions with the ionosonde and incomparethecatter radar observations over Yakutsk, Irkutsk, modelinge Hill and Arecibo stations.
Incoherent scatter radar observations at Jicamarca (Fejer et al. 2005) indicate daytime westward drifts and stronger nighttime eastward drifts under quiet conditions; nighttime perturbation drifts increase strongly with solar activity.
We have presented the modeling of the ionospheric effects of September 9 14, 2005 geomagnetic storm and the comparison of the GSM TIP results and IRI-2000 predictions with the ionosonde and incoherent scatter radar observations at Yakutsk, Irkutsk, Millstone Hill, and Arecibo.
The ionosphere/plasmasphere electron content (PEC) variations during strong geomagnetic storms in November 2004 were estimated by combining of mid-latitude Kharkov incoherent scatter radar observations and GPS TEC data derived from global TEC maps.
The long-duration continuous Irkutsk incoherent scatter radar observations allowed us to collect 337 electron density vertical profiles obtained almost simultaneously with the radar and the COSMIC in the radar vicinity.
Observations of incoherent scattering echo-power of the MU radar and the corresponding synthetic data on 17 July 2001.
The anti-correlation with solar activity at mid-latitudes had been reported earlier with Incoherent Scatter Radar (ISR) observations (see references in Truhlik et al., 2009a).
The first long-duration incoherent scatter (IS) radar observations over Millstone Hill (42.6°N, 288.5°E) and EISCAT Svalbard radar (ESR, 78.15°N, 16.05°E) from October 4 to November 4, 2002 are compared with the newly updated version of the IRI model (IRI2001).
