Numerical simulation of equatorial plasma bubbles over Cachimbo: COPEX campaign

Author(s)

Carrasco, A. J. ^[1] ; Batista, I. S. ^[2] ; Abdu, M. A. ^[2]

Affiliation

^[1] Univ Los Andes, Dept Fis, Merida - Venezuela

^[2] Inst Nacl Pesquisas Espaciais, BR-12201 Sao Jose Dos Campos, SP - Brazil

• Document type: Journal article
• Source: Advances in Space Research; v. 54, n. 3, p. 443-455, AUG 1 2014.
• Web of Science Citations: 1

Abstract

The problem of day-to-day variability in onset of equatorial spread F (ESF) is addressed using data from the 2002 COPEX observational campaign in Brazil and numerical modeling. The observational results show that for values of virtual height of the F layer base less than 355 km at around 18:35 LT, and for the prereversal peak enhancement of the vertical plasma drift (Vp) less than 30 m/s, the spread-F (ESF) was absent on four nights over Cachimbo (9.5 degrees S, 54.8 degrees W, dip latitude = -2.1 degrees). In this work we analyze the geophysical conditions for the generation of the irregularities by comparing the nights with and without the ESF. In the comparison a numerical code is used to simulate plasma irregularity development in an extended altitude range from the bottom of the equatorial F layer. The code uses the flux corrected transport method with Boris Book's flux limiter for the spatial integration and a predictor-corrector method for the direct time integration of the continuity equation for O+ and the SOR (Successive-Over-Relaxation) method for electric potential equation. The code is tested with different evening eastward electric fields (or vertical drifts Vp < 30 m/s and Vp > 30 m/s) in order to study the influence of the prereversal enhancement in the zonal electric field on plasma bubble formation and development. The code also takes into account the zonal wind, the vertical electric field and the collision frequency of ions with neutrals and the amplitude of initial perturbation. The simulation shows a good agreement with the observational results of the ESF. The results of the code suggest that the instability can grow at the F layer bottomside by the Rayleigh-Taylor mechanism only when the Vp > 30 m/s. In the analyzed cases we have considered the competition of other geophysical parameters in the generation of plasma structures. (C) 2013 COSPAR. Published by Elsevier Ltd. All rights reserved. (AU)

• FAPESP's process: 10/05698-8 - Ionospheric irregularities and numerical simulation of plasma bubbles
• Grantee: Inez Staciarini Batista
• Support Opportunities: Research Grants - Visiting Researcher Grant - International