Electrodynamical response of the Indian low-mid latitude ionosphere to the very large solar flare of 28 October 2003 ― a case study

• Published in: Annales geophysicae (1988) Vol. 27; no. 10; pp. 3853 - 3860
• Main Authors: MANJU, G, PANT, T. K, DEVASIA, C. V, RAVINDRAN, S, SRIDHARAN, R
• Format: Journal Article
• Language: English
• Published: Göttingen Copernicus 09-10-2009; Copernicus GmbH; Copernicus Publications
• Subjects: Case studies; Earth, ocean, space; Exact sciences and technology; External geophysics; Global Positioning System; Ionosphere; Ionospheric research; Physics of the ionosphere; Physics of the magnetosphere; Upper atmosphere; Delhi; Asia; India; India, Rajasthan, Jodhpur; India, Delhi; Electrodynamics; Mid latitude; Recombination; case studies; Total electron content; Ionosphere (Equatorial ionosphere; Ionospheric disturbances); Magnetospheric physics (Current systems); Solar flare; Global Positioning System; Sunset; Persistence; Equatorial anomaly; Ionization; Ionospheric disturbance; Observation data; Low latitude; Counter electrojet; Equatorial electrojet; Longitudinal variation
• ISSN: 0992-7689; 1432-0576; 1432-0576
• DOI: 10.5194/angeo-27-3853-2009

The electrodynamic effects on the low-mid latitude ionospheric region have been investigated using GPS (global positioning system) data, ionosonde data and ΔH values, during the very large solar flare (X17.2/4B) of 28 October 2003. The results bring out the flare induced unusual behaviour of the equatorial ionosphere on this day just prior to sunset. The important observations are i) Large and prolonged Ne enhancements observed from ionosonde data just after the flare-related peak enhancement in EUV flux. The observed enhancement in Ne is due to the increase in ionization production due to the enhanced EUV flux and the persistence of the enhancement is probably due to the prompt penetration related upliftment of the F layer (just prior to the flare peak phase) to higher altitudes, where recombination rates are lower. ii) A significant enhancement in total electron content (TEC) (~10 TEC units) at regions around the Equatorial Ionization Anomaly (EIA) crest region (Ahmedabad) during the flare in association with the flare related EUV flux enhancement. iii) Similar enhancements seen at stations of Jodhpur and Delhi in the mid latitude sector. iv)The flare related flux enhancements in different longitude sectors in the equatorial electrojet region have been shown to produce positive and negative variations in electrojet strength indicating the presence of current systems having positive and negative polarities in different longitude sectors. Thus the flare effect reveals the longitudinal variation of the counter electrojet events in the Equatorial Electrojet (EEJ) region.