Physics
Scientific paper
May 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agusmsa31b..03c&link_type=abstract
American Geophysical Union, Spring Meeting 2009, abstract #SA31B-03
Physics
2435 Ionospheric Disturbances, 2437 Ionospheric Dynamics, 2443 Midlatitude Ionosphere
Scientific paper
This study presents the diurnal, seasonal and solar flux in ionospheric slab thickness (τ), button slab thickness (B0) and the peak height (hmF2) during solar maximum in mid latitudes. The data of foF2, hmF2 and B0 with 15 mimutes interval resolution are measured by the UMLCAR SAO-Explorer at the mid latitude digisonde station Wuhan (30.6oN, 114.4oE). The GPS-derived total electron content (TEC) data are measured at the Wuhan receiver (30.53oN, 114.360E) to study the variations in slab thickness of ionosphere during April, 1999 - March, 2000, corresponding to the solar maximum phase. Meanwhile, the study also make a comparison which are mad with International Reference Ionosphere model (IRI-2001) using both the standard B0 and the Gulyaeva's B0 thickness. This study shows the daily, seasonal, and solar flux variations and comparison with IRI-2000 model during solar maximum phases.
Cheng Wenchi
Chuo Y.
Lee Chaohong
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