Abstract
The results of the paper were based upon data on magnetic storms for a five-year period (2008–2012) such as vertical sounding data, magnetometer and riometer data from the Sodankylä station, and satellite data. The main efforts were directed to reveal the relationship between the level of absorption in the ionospheric D-region and magnetic field intensity in a disturbance bay. We detected thresholds in the level of absorption when ionospherically reflected signals were absent in the vertical sounding. Another task of the study was to reveal the relationship between maximum frequencies of Es layers and magnetic field intensity for the magnetic storm period. We established differences between the mentioned regularities for daytime and nighttime periods.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
