Open AccessIonospheric Weather During Five Extreme Geomagnetic Superstorms Since IGY Deduced With the Instantaneous Global Maps GIM‐foF2
Author(s) -
Stanislawska Iwona,
Gulyaeva Tamara L.,
GrynyshynaPoliuga Oksana,
Pustovalova Ljubov V.
Publication year - 2018
Publication title -
space weather
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.254
H-Index - 56
ISSN - 1542-7390
DOI - 10.1029/2018sw001945
Subject(s) - ionosphere , critical frequency , geomagnetic storm , earth's magnetic field , space weather , storm , universal time , meteorology , environmental science , geology , geography , geophysics , physics , quantum mechanics , astronomy , magnetic field
An assessment of the ionosphere perturbations can be made through the construction of the global instantaneous maps of the foF2 critical frequency (GIM‐foF2) and the ionospheric weather index maps GIM‐Wf. These maps can offer a potentially useful tool to provide users with a proper selection of the best radio wave propagation conditions over a certain area and also be used to help mitigate the effects of the disturbances on HF (High Frequency) communication and Global Navigation Satellite System positioning. This paper presents results of reconstruction of the ionospheric weather during five of the most intense superstorms observed since International Geophysical Year, IGY (1957, 1958, 1959, 1989, and 2003) with the instantaneous global maps of the F2 layer critical frequency, GIM‐foF2, and the ionospheric weather index maps, GIM‐Wf. The intensity of the ionospheric superstorm is characterized by the planetary Wfp index derived from GIM‐Wf maps. Superposed epoch analysis of the extreme superstorms is made during 24 hr before the Wfp peak (time zero t 0 = 0 hr) and 48 hr afterwards. Model relationship is established between mean Wfp profile and geomagnetic superstorm profiles demonstrating saturation of the ionospheric storm activity toward the peak of geomagnetic storm. Time lag of Wfp max is found equal to 9 hr after AE max , 6 hr after ap max and aa max , and 2 hr after Dst min , which allows model forecast of ionospheric superstorm when geomagnetic superstorm is captured with one or more of geomagnetic indices.