dc.contributor.author |
Tsunoda, Roland T. |
|
dc.contributor.author |
Yamamoto, Mamoru |
|
dc.contributor.author |
Tsugawa, Takuya |
|
dc.contributor.author |
Hoang, Thai Lan |
|
dc.contributor.author |
Tulasiram, S. |
|
dc.contributor.author |
Thampi, Smitha V. |
|
dc.contributor.author |
Chau, Ha Duyen |
|
dc.contributor.author |
Nagatsuma, Tsutomu |
|
dc.date.accessioned |
2016-06-30T06:29:35Z |
|
dc.date.accessioned |
2021-02-12T09:54:51Z |
|
dc.date.available |
2016-06-30T06:29:35Z |
|
dc.date.available |
2021-02-12T09:54:51Z |
|
dc.date.issued |
2011 |
|
dc.identifier.citation |
GRL, v.38/20, 2011, doi: 10.1029/2011GL049173 |
en_US |
dc.identifier.uri |
http://localhost:8080/xmlui/handle/123456789/905 |
|
dc.description.abstract |
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. |
en_US |
dc.language.iso |
en |
en_US |
dc.subject |
Equatorial spread F |
en_US |
dc.subject |
Large-scale wave structure |
en_US |
dc.subject |
Total electron content |
en_US |
dc.subject |
LSWS |
en_US |
dc.title |
On seeding, large-scale wave structure, equatorial spread F, and scintillations over Vietnam |
en_US |
dc.type |
Article |
en_US |
dc.identifier.accession |
091223 |
|