Policy on Intellectual Property Right (IPR)
1 Introduction
2 Background
3 Prime degradations due to background ionizations
3.1 TEC
3.1.1 IRI-2012-based method
3.1.2 NeQuick2-based method
3.2 Faraday rotation
3.3 Group delay
3.4 Dispersion
3.5 TEC rate of change
4 Principal degradation due to irregularities
4.1 Scintillation
4.2 Geographic, seasonal
and solar dependence of scintillations
4.3 Ionospheric
scintillation model
4.4 Instantaneous
statistics and spectrum behaviour
4.4.1 Instantaneous
statistics
4.4.2 Spectrum behaviour
4.5 Geometric
consideration
4.5.1 Zenith
angle dependence
4.5.2 Seasonal-longitudinal
dependence
4.6 Cumulative statistics
4.7 Simultaneous occurrence of ionospheric scintillation and rain
fading
4.8 Gigahertz
scintillation model
5 Absorption
5.1 Auroral absorption
5.2 Polar cap absorption
6 Summary