Day-to-day variability of equatorial anomaly in GPS-TEC during low solar activity period

作者：Aggarwal Malini^*; Joshi H P; Iyer K N; Kwak Y S; Lee J J; Chandra H; Cho K S

来源：Advances in Space Research, 2012, 49(12): 1709-1720.

DOI：10.1016/j.asr.2012.03.005

• GPS-total electron content (TEC)
• Equatorial ionization anomaly (EIA)
• Equatorial electrojet (EEJ)

The ionospheric total electron content (TEC) in the northern hemispheric equatorial ionization anomaly (EIA) crest region is investigated by using dual-frequency signals of the Global Positioning System (GPS) acquired from Rajkot (Geog. Lat. 22.29 degrees N, Geog. Long. 70.74 degrees E; Geom. Lat. 14.21 degrees N, Geom. Long.144.90 degrees E), India. The day-to-day variability of EIA characteristics is examined during low solar activity period (F10.7 similar to 83 sfu). It is found that the daily maximum TEC at EIA crest exhibits a day-to-day and strong semi-annual variability. The seasonal anomaly and equinoctial asymmetry in TEC at EIA is found non-existent and weaker, respectively. We found a moderate and positive correlation of daily magnitude of crest, Ic with daily F10.7 and EUV fluxes with a correlation coefficient of 0.43 and 0.33, respectively indicating an existence of a short-term relation between TEC at EIA and the solar radiation even during low solar activity period. The correlation of daily Ic with Dst index is also moderate (r = -0.35), whereas no correlation is found with the daily Kp index (r = 0.14) respectively. We found that the magnitude of EIA crest is moderately correlated with solar flux in all seasons except winter where it is weakly related (0.27). The magnitude of EIA crest is also found highly related with EEJ strength in spring (r = 0.69) and summer (r = 0.65) than autumn (0.5) and winter (r = 0.47), though EEJ is stronger in autumn than spring.

• 出版日期2012-6-15