The effect of â¼27 day solar rotation on ionospheric Fâ region peak densities (NmFâ)
Ionospheric F² region peak electron densities (NmF²) observed from 11 ionosonde stations in the East Asian-Australian sector from 1969 to 1986 have been used to investigate the effect of â¼27 day solar rotation on the ionosphere. These stations were located from the magnetically equatorial regions to the middle latitudes in both hemispheres. We found that, averaged over all stations and for 18 years, the normalized standard deviation of the midday â¼27 day variations of NmFâ was 8% and that of the midnight variations was 10%. We applied different data analysis methods, including Fourier transform, band-pass filter, and multiple linear regression analysis, to determine quantitatively the sources of the observed â¼27 day variations of NmFâ and their relative contributions to these variations. Our results show that the â¼27 day variations in solar radiation and geomagnetic activity, caused by solar rotation, are the main drivers of the ionospheric â¼27 day variations. They accounted for more than 85% of the variations seen in the NmFâ â¼27 day variation, and their contributions became about 95% at higher latitudes. At geomagnetically low latitudes, the contribution of the â¼27 day variation in solar EUV radiation was greater than that of the â¼27 day variation in geomagnetic activity. However, the contribution from geomagnetic activity became more significant and was even larger than the contribution of solar radiation at higher latitudes, especially at midnight. At all latitudes the correlation between the â¼27 day variations of NmFâ and solar radiation was evidently positive, whereas that between NmFâ and geomagnetic activity was positive at geomagnetically low latitudes and became negative at higher middle latitudes. We did not found large seasonal or solar cycle changes in the â¼27 day variations of NmFâ. These variations, however, did show significant differences between the two hemispheres.
document
https://n2t.org/ark:/85065/d74t6k1d
eng
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2016-01-01T00:00:00Z
publication
2012-03-06T00:00:00Z
Copyright 2012 American Geophysical Union.
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