Model simulations of global change in the ionosphere
Observations of secular trends in the E and Fâ regions of the ionosphere indicate that electron densities have increased, and that the height of the E-region peak has decreased, during the past several decades. Detection of trends in the upper ionosphere through analysis of Fâ-layer parameters has been more complex and controversial. In order to facilitate observational detection of long-term trends in the ionosphere, simulations were performed using a single-column upper atmosphere model. COâ concentrations for the year 2000 and projected for the year 2100 were used to investigate changes of electron densities and the altitudes of ionospheric layers. Results show that increased COâ concentration increases electron density in the lower regions of the ionosphere, but decreases electron density in the upper ionosphere. The transition altitude occurs slightly below the Fâ peak altitude (hmFâ). The proximity of hmFâ to the transition altitude may explain why different analyses of long-term trends in Fâ peak density have shown both positive and negative trends. The altitudes of the E, Fâ and Fâ regions all decrease with increased CO2 concentration.
document
https://n2t.org/ark:/85065/d7v40vd0
eng
geoscientificInformation
Text
publication
2016-01-01T00:00:00Z
publication
2008-04-05T00:00:00Z
An edited version of this paper was published by AGU. Copyright 2008 American Geophysical Union.
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