Journal
GEOPHYSICAL RESEARCH LETTERS
Volume 38, Issue -, Pages -Publisher
AMER GEOPHYSICAL UNION
DOI: 10.1029/2011GL049173
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Funding
- NSF [ATM-0720396]
- AFOSR [FA9550-10-C-0004]
- JSPS Foundation
- Grants-in-Aid for Scientific Research [22403011, 10F00336] Funding Source: KAKEN
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Understanding the day-to-day variability in occurrence of equatorial spread F (ESF) remains as a high-priority objective in space weather research. A major difficulty has been an inability to resolve the roles being played by large-scale wave structure (LSWS) and the post-sunset rise (PSSR) of the equatorial F layer, in the production of ESF. In this paper, we show conclusively that total electron content (TEC), measured as a function of latitude and longitude, provides clear, routine descriptions of LSWS. Then, together with ionosonde data, we show, for the first time, that while a seed for LSWS can occur in the late afternoon, its amplification takes place mostly during the PSSR. Implications of these findings are discussed in light of existing theories. Citation: Tsunoda, R. T., M. Yamamoto, T. Tsugawa, T. L. Hoang, S. Tulasi Ram, S. V. Thampi, H. D. Chau, and T. Nagatsuma (2011), On seeding, large-scale wave structure, equatorial spread F, and scintillations over Vietnam, Geophys. Res. Lett., 38, L20102, doi:10.1029/2011GL049173.
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