@Article{SivakandanPRTPSNB:2019:MuInTr,
author = "Sivakandan, M. and Paulo, Igo and Ramkumar, T. K. and Taori, A.
and Patra, A. K. and Sripathi, S. and Niranjan, K. and Bilibio,
Anderson Vestena",
affiliation = "{Physical Research Laborator} and {Universidade Federal de Campina
Grande (UFCG)} and National Atmospheric Research Laboratory,
Gadanki and {Regional Remote Sensing Center (RRSC)} and National
Atmospheric Research Laboratory, Gadanki and National Atmospheric
Research Laboratory, Gadanki and {Andhra Universit} and {Instituto
Nacional de Pesquisas Espaciais (INPE)}",
title = "Multi-instrument investigation of troposphere-ionosphere coupling
and the role of gravity waves in the formation of equatorial
plasma bubble",
journal = "Journal of Atmospheric and Solar-Terrestrial Physics",
year = "2019",
volume = "189",
pages = "65--79",
month = "Aug.",
keywords = "Equatorial plasma bubbles, R-T instability, Gravity waves, Ray
tracing.",
abstract = "Present study investigates the role of gravity waves in the
generation of equatorial plasma bubbles (EPBs) during geomagnetic
quiet conditions using co-located observations from Gadanki (13.5
o N, 79.2° E) an all sky airglow imager, Gadanki Ionospheric Radar
Interferometer (GIRI) and Ionosonde observations from Tirunelveli
(8.7° N, 77.8° E). To avoid any changes occurring in the
background ionosphere, four consecutive nights of observation
during 0306 February 2014 is used. Out of these four nights, three
nights (i.e., 03, 05 and 06 February 2014) exhibit occurrence of
EPBs in the OI 630 nm airglow emission and radar plumes and there
is no bubble occurrence during one night, though the ionospheric
peak altitude (h\′F) value is more than 350 km in all these
nights. During these four nights the structures observed in the
E-region drifts and gravity waves noted in the mesospheric OH
emissions are analyzed. It is found that there are common periodic
oscillations in the OH peak emission altitude and E-region in
three nights (03, 04 and 05 February 2014). The mesospheric
gravity wave structures are ray traced to their potential sources
in the lower atmosphere and also for the possibility of their
propagation to the E-region. Our results suggest that apart from
horizontal wavelength and amplitudes, the propagation angle of
gravity wave may also be important for seeding of the
Rayleigh-Taylor (R-T) instability. Thus, it gives an insight about
the role of lower middle and upper atmospheric coupling on the
occurrence of the noted EPBs.",
doi = "10.1016/j.jastp.2019.04.006",
url = "http://dx.doi.org/10.1016/j.jastp.2019.04.006",
issn = "1364-6826",
language = "en",
targetfile = "Sivakandan1-s2.0-S1364682618306497-main.pdf",
urlaccessdate = "03 maio 2024"
}