Title of article
F2 layer response to geomagnetic disturbances in Eastern Asia under the low solar activity Original Research Article
Author/Authors
O.M. Pirog، نويسنده , , N.M. Polekh، نويسنده , , E.B. Romanova، نويسنده , , S.V. Voeykov، نويسنده , , G.A. Zherebtsov، نويسنده , , J.K. Shi، نويسنده , , X. Wang، نويسنده ,
Issue Information
دوهفته نامه با شماره پیاپی سال 2010
Pages
13
From page
921
To page
933
Abstract
In this paper, the peculiarities of ionospheric response to geomagnetic disturbances observed at the decay and minimum of solar activity (SA) in the period 2004–2007 are investigated with respect to different geomagnetic conditions. Data from ionospheric stations and results of total electron content (TEC) measurements made at the network of GPS ground-based receivers located within the latitude–longitude sector (20–70°N, 90–160°Е) are used in this study. Three groups of anomalous ionospheric response to geomagnetic disturbances have been observed during low solar activity. At daytime, the large-scale traveling ionospheric disturbances (LSTIDs) could generally be related to the main phase of magnetic storm. Quasi-two-days wavelike disturbances (WLDs) have been also observed in the main phase independent of the geomagnetic storm intensity. Sharp electron density oscillations of short duration (OSD) occurred in the response to the onset of both main and recovery phases of the magnetic storm in the daytime at middle latitudes. A numerical model for ionosphere–plasmasphere coupling was used to interpret the occurrence of LS TIDs. Results showed that the LSTIDs might be associated with the unexpected lifting of F2 layer to the region with the lower recombination rate by reinforced meridional winds that produces the increase of the electron density in the F2 layer maximum.
Keywords
Ionosphere , Disturbance , Electron density , Traveling ionospheric disturbance , Storm
Journal title
Advances in Space Research
Serial Year
2010
Journal title
Advances in Space Research
Record number
1133133
Link To Document