The non-linear response of the ionosphere to solar activity and the resultant influence on trends.

Details The non-linear response of the ionosphere to solar activity and the resultant influence on trends. The non-linear response of the ionosphere to solar activity and the resultant influence on trends.

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agusmsa34a..05w&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SA34A-05

Physics

7900 Space Weather, 7974 Solar Effects

Scientific paper

The ionosphere exhibits a non-linear response to the solar cycle. This effect can show both a positive and a negative second derivative depending on time of year and time of day. This non-linear response can influence trends, particularly if the response is inappropriately incorporated into a linear statistical model. The influence of the solar cycle on observed trends will be discusses. The results show that linear approximations can result in overestimating and underestimating trends in foF2. The work underlines the importance of choosing statistical models which represent the physics of the ionosphere. Trend results will be shown for five locations.

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