@InProceedings{BatistaAbPaSoMuMe:1994:PlBuEq,
author = "Batista, Inez Staciarini and Abdu, Mangalathayil Ali and Paula,
Eurico Rodrigues de and Sobral, Jos{\'e} Humberto Andrade and
Muralikrishna, Polinaya and Medeiros, R. T.",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {Instituto Nacional de Pesquisas Espaciais (INPE)}",
title = "Plasma bubbles and equatorial sprea F irregularity studies over
Brazil",
booktitle = "Proceedings...",
year = "1994",
editor = "Sakanaka, P. H. and Del Bosco, Edson and Alves, Maria Virginia",
pages = "195--198",
organization = "International Conference on Plasma Physics.",
abstract = "For more 20 years ionospheric studies have been conductecd in
Brazil, in order to understand the plasma bubble and spread F
irregularity phenomena and their influence on radio-wave
propagation. Most of the studies were carried out using
ground-based equipments (ionosondes, polarimeters, scintillation
measurements and photometers), operating in Cachoeira Paulista
(22.5ºS. 45ºW), S{\~a}o Jos{\'e} dos Campos (23ºS, 46ºW) and
Fortaleza (4ºS, 38ºW). In situ measurements carried out using
payloads on board of sounding rockets launched from Natal (5.9ºS,
35.3ºW) have also contributed to the study of the plasma bubble
phenomena over Brazil. The equatorial spread F phenomena are often
associated with plasma depleted magnetic flux tubes, namely,
plasma bubbles. The plasma bubbles are generated over the
equatorial F region through the Rayleigh-Taylor gravitational
instability process. The enhanced post-sunset ExB drift is of
prime importance on the generation of plasma bubbles and
equatorial spread F irregularities. The magnetic declination angle
over Brazil s very high (it attains a global maximum over
Brazilian longitude sector). The observational studies and
theoretical simulations conducted in Brazil have shown that the
very high magnetic declination angle greatly affects the seasonal
distribution of spread F occurrence. In this paper, all these
observational aspects as well as the simulations conducted to
explain them, are reviewed.",
conference-location = "Foz do Igua{\c{c}}u, PR",
conference-year = "31 Oct. - 04 Nov.",
language = "en",
targetfile = "Batista_plasma.pdf",
urlaccessdate = "25 abr. 2024"
}