@InProceedings{MuralikrishnaOdriBati:2015:WaStOb,
author = "Muralikrishna, Polinaya and Odriozola, Siomel Savio and Batista,
Inez Staciarini",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)}",
title = "Wave structures observed in the Equatorial F-region plasma density
and temperature during the sunset period",
year = "2015",
organization = "International Congress of the Brazilian Geophysical Society, 14.",
abstract = "Electron density and temperature measurements were made recently
with rocket-borne Langmuir probes on 2-nd December 2011 using a
Brazilian VS-30 single stage rocket and on 8-th December 2012
using a two stage VS-30/Orion rocket. The first launch was made
from the equatorial rocket launching station CLBI in Natal, Brazil
and the second one from the CLA in Alc{\^a}ntara-MA. Both the
launches were made soon after the local sunset. The ground
equipments operated during the rocket launches clearly showed the
rapid rise of the F-region base indicating probably the pre
reversal enhancement of the F-region vertical plasma drift. At the
time of launch the bubble activity was also at its peak as
indicated by the presence of strong spread-F traces in the
ionograms. The electron density and temperature height profiles
could be estimated from the LP data up to the rocket apogee
altitudes of 139km during the first launch and 428m km during the
second launch. During the first launch the Fregion valley region
showed the presence electron temperatures as high as 2000 ēK while
the temperatures expected from the existing models are around 500
ēK. During the second launch also ground equipments operated at
equatorial stations showed rapid rise in the base of the F-layer
creating ionospheric conditions favorable for the generation of
plasma bubbles. During this launch also electron temperatures as
high as 3500ēK were observed in the valley region both during the
rocket upleg and downleg. These profiles are compared with model
electron density and temperature profiles as well as with electron
density and temperature profiles observed under conditions of no
plasma bubbles. The electron density and temperatures profiles
observed during both the launches showed the presence of
significantly large amplitude waves indicating intense wave
activity in the valley region close to sunset period. These wave
activities are probably related to the electrodynamic processes
that exist in this region during the sunset period.",
conference-location = "Rio de Janeiro, RJ",
conference-year = "3-6 Aug.",
urlaccessdate = "25 abr. 2024"
}