dc.contributor.author |
Ramesh, K. B |
|
dc.contributor.author |
Sastri, J. H |
|
dc.date.accessioned |
2008-08-05T07:53:14Z |
|
dc.date.available |
2008-08-05T07:53:14Z |
|
dc.date.issued |
1995-06 |
|
dc.identifier.citation |
Annales Geophysicae-Atmospheres Hydrospheres and Space Sciences, Vol. 13, No. 6, pp. 633 - 640 |
en |
dc.identifier.issn |
0992-7689 |
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dc.identifier.uri |
http://hdl.handle.net/2248/3025 |
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dc.description.abstract |
Measurements of the changes in phase path of F-region reflections at normal incidence at Kodaikanal (77°28'E, 10°14'N, dip 3°N) from February 1991 to February 1993 are used to determine the variation of the equatorial evening F-region vertical drifts (Vz) with season, solar and magnetic activity. It is found that on average, at Kodaikanal, the post-sunset peak in Vz (Vzp) is higher in equinox and local winter months than in local summer. The day-to-day variability in Vzp is highest in summer and lowest in winter. This seasonal trend persists even on magnetically quiet days (Ap≤14). Vzp is found to increase with 10.7 cm solar flux in all three seasons but tends to saturate for large flux values (>230 units) during local summer and winter months. Magnetic activity [represented by Ap as well as the time-weighted accumulations of ap and ap(τ)] does not seem to have any statistically significant effect on Vzp, except during equinoctial months of moderate solar activity, when Vzp decreases as magnetic activity increases. |
en |
dc.format.extent |
3894 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
European Geophysical Society |
en |
dc.subject |
Equatorial Ionosphere |
en |
dc.subject |
Ionospheric of Region |
en |
dc.subject |
Vertical Drift |
en |
dc.subject |
Solar Cycle |
en |
dc.subject |
Seasonal Variation |
en |
dc.subject |
Geomagnetic Activity |
en |
dc.subject |
India |
en |
dc.subject |
Asia |
en |
dc.title |
Solar cycle and seasonal variations in F-region vertical drifts over Kodaikanal, India |
en |
dc.type |
Article |
en |