Negative phases at South-American stations during magnetic storms

Main Article Content

X. T. Pincheira
I. S. Batista
M. A. Abdu
P. G. Richards

Abstract

Ionospheric data at three South-American stations (in low, mid and high latitudes) show negative phases in the high latitude location during magnetic storms. The negative phases in foF2 are caused by changes in the ratio between atomic and molecular concentrations of the neutral atmosphere.
We find that at high latitudes the negative phases are well explained by the [O]/[N ] rate changes. As the latitude decreases, as the wind influence on the F2 layer peak is dominant, the propagation of gravity waves can explain short-lived negative phases. In low latitudes, disturbed thermospheric winds can cause time delays in the normal pattern of foF2, creating alternating positive and negative phases.

Article Details

How to Cite
Pincheira, X. T., Batista, I. S., Abdu, M. A., & Richards, P. G. (2000). Negative phases at South-American stations during magnetic storms. Geofisica Internacional, 39(1), 109–115. https://doi.org/10.22201/igeof.00167169p.2000.39.1.305
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Article
Author Biographies

X. T. Pincheira, Universidad del Bio-Bio, Concepción, Chile

 

 

I. S. Batista, Instituto Nacional de Pesquisas Espaciais, São José dos Campos, Brasil

 

 

P. G. Richards, Center of Space Plasma and Aeronomy Research and Computer Sciences Dept., University of Alabama, Huntsville, USA

 

 

References

BORBA, G. L., 1993. Estudo de perturbações propagantesna região F da ionosfera no setor sul-americano. SãoJosé dos Campos, Dissertação (Doutorado em GeofísicaEspacial). Instituto Nacional de Pesquisas Espaciais, 177pp.

PRÖLSS, G. W., 1977. Seasonal variations of atmospheric-ionospheric disturbances. J. Geophys. Res., 82, 1635-1640. DOI: https://doi.org/10.1029/JA082i010p01635

PRÖLSS, G.W., 1995. Ionospheric F-region Storms. In: Valland, H. ed. Handbook of Atmospheric Electrodynamics. Boca Raton: CRC Press, 2, 195-248.

RICHARDS, P. G., 1991. An improved algorithm for determining neutral winds from the height of the F2 peak electron density. J. Geophys. Res., 96, 17839-17849. DOI: https://doi.org/10.1029/91JA01467

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