Space weather effects on radio propagation: study of the CEDAR, GEM and ISTP storm events

• Published in: Annales Geophysicae
• Main Authors: Blagoveshchensky, D. V., Kalishin, A. S., Sergeyeva, M. A.
• Format: Article in Journal/Newspaper
• Language: English
• Published: Copernicus Publications 2008
• Subjects: article; Verlagsveröffentlichung; North-West Russia
• Online Access: https://doi.org/10.5194/angeo-26-1479-2008; https://noa.gwlb.de/receive/cop_mods_00031395; https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00031349/angeo-26-1479-2008.pdf; https://angeo.copernicus.org/articles/26/1479/2008/angeo-26-1479-2008.pdf

The impact of 14 geomagnetic storms from a list of CEDAR, GEM and ISTP storms, that occurred during 1997–1999, on radio propagation conditions has been investigated. The propagation conditions were estimated through variations of the MOF and LOF (the maximum and lowest operation frequencies) on three high-latitude HF radio paths in north-west Russia. Geophysical data of Dst, Bz, AE as well as some riometer data from Sodankyla observatory, Finland, were used for the analysis. It was shown that the storm impact on the ionosphere and radio propagation for each storm has an individual character. Nevertheless, there are common patterns in variation of the propagation parameters for all storms. Thus, the frequency range Δ=MOF−LOF increases several hours before a storm, then it narrows sharply during the storm, and expands again several hours after the end of the storm. This regular behaviour should be useful for the HF radio propagation predictions and frequency management at high latitudes. On the trans-auroral radio path, the time interval when the signal is lost through a storm (tdes) depends on the local time. For the day-time storms an average value tdes is 6 h, but for night storms tdes is only 2 h. The ionization increase in the F2 layer before storm onset is 3.5 h during the day-time and 2.4 h at night. Mechanisms to explain the observed variations are discussed including some novel possibilities involving energy input through the cusp.