Equatorial ionospheric response to the 10.7 cm radio flux over two sunspot cycles (1969-1991)

Hajkowicz, L. A. (1996) Equatorial ionospheric response to the 10.7 cm radio flux over two sunspot cycles (1969-1991). Annales Geophysicae, 14 7: 725-732. doi:10.1007/s00585-996-0725-z


Author Hajkowicz, L. A.
Title Equatorial ionospheric response to the 10.7 cm radio flux over two sunspot cycles (1969-1991)
Journal name Annales Geophysicae   Check publisher's open access policy
ISSN 0992-7689
1432-0576
Publication date 1996
Sub-type Article (original research)
DOI 10.1007/s00585-996-0725-z
Open Access Status Not yet assessed
Volume 14
Issue 7
Start page 725
End page 732
Total pages 8
Place of publication Goettingen, Germany
Publisher Copernicus GmbH
Formatted abstract
It is evident that fluctuations in a standard ionospheric parameter, the minimum (virtual) height (h´F) of the equatorial F-region in the African (Ouagadougou), Asian (Manila) and American (Huancayo) longitudinal sectors, closely resemble changes in solar activity as deduced from the 10.7 cm solar flux index (S), over two solar cycles (1969–91). The monthly median hourly value of h´F, particularly in the post-sunset period (18–20 LT), are positively correlated with the monthly average S. The value of h´F can be deduced from an empirical formula: h´F=0.68S+218.3, with the correlation coefficient (r) between h´F and S being 0.78. The diurnal distribution of r during daytime (06–14 LT) was radically different for the African and Asian longitudinal sectors during 1980-1991, with the most pronounced difference in the post-noon period (12–14 LT) when the correlation coefficients r for the Asian and African sectors are 0.8 and 0.2, respectively. Thus, the daytime F-region in the African sector responded far less to changes in solar activity than the Asian F-region during this cycle. This longitudinal anomaly was however absent in the preceding cycle (1969–1979) when the African and Asian sectors were both characterised by low daytime and pronounced post-sunset correlation coefficient r. The American sector appears to have a high correlation coefficient r in daytime increasing to a small maximum in the post-sunset interval. The post-sunset enhancement in r is a characteristic feature for equatorial stations only (corrected geomagnetic latitude <10°).
Q-Index Code C1
Q-Index Status Provisional Code
Institutional Status Unknown

Document type: Journal Article
Sub-type: Article (original research)
Collection: School of Mathematics and Physics
 
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