Variabilities observed in the vertical polarization electric field
associated with electrojet current system during solar flare events
Abstract
Using ground based magnetometer data and an in-house developed quasi two
dimensional (QTD) theoretical ionospheric model, we investigate
differential response of the E region ionospheric current system to the
solar flare events which occurred on 20 February 2002, and 24 September
2011. An abrupt increase in $\Delta$H (positive
crochet/Solar Flare Effect (SFE)) was observed at Thirunelveli during 24
September 2011 event, while a decrease in $\Delta$H
(reduced crochet/SFE) was observed during the other event. The reduction
in $\Delta$H was observed on 20 February when there
were no signatures of counter electrojet (CEJ). As per QTD model
simulations, the ratio of integrated Hall to Pedersen conductivity
decreased more on 20 February at EEJ heights. As the conductivity ratio
is directly proportional to the vertical polarization field, a decrease
in conductivity leads to a reduced EEJ strength on 20 February 2002. In
the presence of an additional SFE current system at the boundary between
D and E region, during solar flare, the crochet is the resultant of EEJ
and SFE. On 24 September, both the EEJ and SFE current systems were
strong with the vortex center close to the equator and a positive
crochet was observed. On 20 February, on the other hand, both EEJ and
SFE were weak as the current vortex was away from the magnetic equator.
Hence we surmise that SFE not only depends on the strength of the solar
flare or the background electrojet condition but also the position of
vortex of current systems.