Review of Relationships Between Solar Wind and Ground-Level Atmospheric Electricity: Case Studies from Hornsund, Spitsbergen, and Swider, Poland

• Published in: Surveys in Geophysics
• Main Authors: Michnowski, S., Odzimek, A., Kleimenova, N. G., Kozyreva, O. V., Kubicki, M., Klos, Z., Israelsson, S., Nikiforova, N. N.
• Other Authors: Ministerstwo Nauki i Szkolnictwa Wyższego
• Format: Article in Journal/Newspaper
• Language: English
• Published: Springer Science and Business Media LLC 2021
• Subjects: Geochemistry and Petrology; Geophysics; Arctic; Hornsund; Norway; Svalbard; Spitsbergen
• Online Access: http://dx.doi.org/10.1007/s10712-021-09639-3; https://link.springer.com/content/pdf/10.1007/s10712-021-09639-3.pdf; https://link.springer.com/article/10.1007/s10712-021-09639-3/fulltext.html

Abstract This paper reviews individual cases of the relationships between variations of solar wind parameters and variations of the DC vertical atmospheric electric field, $$E_z$$ E z , and current density, $$J_z$$ J z , measured at ground level in the Arctic, at the S. Siedlecki Polish Polar Station Hornsund, Spitsbergen (Svalbard, Norway), and at the mid-latitude S. Kalinowski Geophysical Observatory in Swider (Poland). A considerable number of events from Hornsund confirmed previous observations of regularity of effects related to the station’s position against the location of the potential bays of ionospheric convection and polar electrojets, observed in other polar locations, as well as effects of other polar cap current systems. This allowed us to conclude that the physical dependence of ground-level $$E_z$$ E z and $$J_z$$ J z on solar wind changes produce measurable effects which do not require statistical analysis to be observed. We can also expect that the dependence does exist, especially in strongly disturbed circumstances, e.g., following solar flares and Earth-directed coronal mass ejections, at middle latitudes. However, further investigations of these physical relationships by this approach are practically almost impossible since a very large number of variable parameters simultaneously affect the recorded lower atmospheric variables. In addition, results of quantitative analysis of predicted and observed effects are not satisfactory. Future research studies require more efficient ways of investigation by theoretical treatment and modelling work using existing and novel observational data besides taking advantage of scientific progress in magnetospheric physics.