This study correlates ionospheric parameters with the integrated solar radiation for an analysis of the delayed ionospheric response in order to confirm previous studies on the delay and to further specify variations of the delay (seasonal and spatial). Results also indicate the dependence on the geomagnetic activity as well as on the 11-year solar cycle. The results are important for the understanding of ionospheric processes and could be used for the validation of ionospheric models
We analyse solar extreme ultraviolet (EUV) irradiance observed by the Solar EUV Experiment (SEE) onb...
Based on the analysis of electron density Ne profiles (Grahamstown ionosonde), a case study of the h...
The delayed ionospheric response is analyzed for two well‐defined 27‐day solar rotation periods in t...
This study correlates ionospheric parameters with the integrated solar radiation for an analysis of ...
Thermospheric and related ionospheric processes react delayed to the variations of solar UV and EUV ...
Physical and chemical processes in the ionosphere are driven by complex interactions with the solar...
The ionospheric response to solar extreme ultraviolet (EUV) variability during 2011–2014 is shown by...
The ionospheric plasma reacts on solar EUV and UV variations with a time delay of 1-2 days. This del...
Physical and chemical processes in the ionosphere are driven by complex interactions of the neutral ...
Based on the analysis of electron density Ne profiles (Grahamstown ionosonde), a case study of the h...
The ionospheric response to solar EUV variability during 2011 - 2014 is shown by an EUV proxy based ...
Physical and chemical processes in the ionosphere are driven by complex interactions with the solar ...
We investigate the ionospheric response to solar Extreme Ultraviolet (EUV) variations using differe...
The complex interactions in the upper atmosphere, which control the height-dependent ionospheric res...
The delayed ionospheric response is analyzed for two well-defined 27-day solar rotation periods in t...
We analyse solar extreme ultraviolet (EUV) irradiance observed by the Solar EUV Experiment (SEE) onb...
Based on the analysis of electron density Ne profiles (Grahamstown ionosonde), a case study of the h...
The delayed ionospheric response is analyzed for two well‐defined 27‐day solar rotation periods in t...
This study correlates ionospheric parameters with the integrated solar radiation for an analysis of ...
Thermospheric and related ionospheric processes react delayed to the variations of solar UV and EUV ...
Physical and chemical processes in the ionosphere are driven by complex interactions with the solar...
The ionospheric response to solar extreme ultraviolet (EUV) variability during 2011–2014 is shown by...
The ionospheric plasma reacts on solar EUV and UV variations with a time delay of 1-2 days. This del...
Physical and chemical processes in the ionosphere are driven by complex interactions of the neutral ...
Based on the analysis of electron density Ne profiles (Grahamstown ionosonde), a case study of the h...
The ionospheric response to solar EUV variability during 2011 - 2014 is shown by an EUV proxy based ...
Physical and chemical processes in the ionosphere are driven by complex interactions with the solar ...
We investigate the ionospheric response to solar Extreme Ultraviolet (EUV) variations using differe...
The complex interactions in the upper atmosphere, which control the height-dependent ionospheric res...
The delayed ionospheric response is analyzed for two well-defined 27-day solar rotation periods in t...
We analyse solar extreme ultraviolet (EUV) irradiance observed by the Solar EUV Experiment (SEE) onb...
Based on the analysis of electron density Ne profiles (Grahamstown ionosonde), a case study of the h...
The delayed ionospheric response is analyzed for two well‐defined 27‐day solar rotation periods in t...