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• W2000210934 endingPage "770" @default.
• W2000210934 startingPage "760" @default.
• W2000210934 abstract "During five intense geomagnetic storms with main phases occurring around local dusk sector, equatorial ionosonde and electrojet data, VHF/UHF scintillation data of Calcutta, and several solar wind parameters are investigated to ascertain the polarity of prompt penetration electric field (PPEF). Abrupt increases in AE, ASY-H and/or sharp decreases in Dst/SYM-H with strong southward IMF Bz may symbolize eastward PPEF to equatorial latitude leading to evolution of density irregularities if the period is associated with arrival and sustenance of large magnetospheric shock compression. On the contrary, westward PPEF is more feasible if the shock reduces suddenly or fluctuates with small values." @default.
• W2000210934 created "2016-06-24" @default.
• W2000210934 creator A5038332149 @default.
• W2000210934 creator A5046607346 @default.
• W2000210934 date "2011-05-01" @default.
• W2000210934 modified "2023-09-26" @default.
• W2000210934 title "Equatorial ionospheric responses in relation to the occurrence of main phase of intense geomagnetic storms in the local dusk sector" @default.
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• W2000210934 doi "https://doi.org/10.1016/j.jastp.2011.02.014" @default.
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