Journal
GEOPHYSICAL RESEARCH LETTERS
Volume 35, Issue 15, Pages -Publisher
AMER GEOPHYSICAL UNION
DOI: 10.1029/2008GL034433
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- NSC [96-2628-M-001-018]
- NASA MAP [P480501]
- NSPO
- UCAR CDAAC groups
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[1] We analyze 2 years of the FORMOSAT-3/COSMIC GPS radio occultation data to study the response of the Earth's ionosphere to the solar rotation (27-day) induced solar flux variations. Here we report electron density variations in the ionosphere (similar to 100-500 km) associated with the 27-day solar cycle. The peak-to-peak variation in electron density at low latitudes in the F2 region is about similar to 10(4)-10(5) electrons cm(-3) or 20-40%, and can be as high as 60% depending on altitude, latitude, and season. The half and double periods of the 27-day are also observed at an amplitude comparable to that of the 27-day. The results place useful constraints for modeling chemical and dynamical processes in the ionosphere.
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