dc.contributor.author |
Kishore, P. |
|
dc.contributor.author |
Namboothiri, S.P. |
|
dc.contributor.author |
Igarashi, K. |
|
dc.contributor.author |
Gurubaran, S. |
|
dc.contributor.author |
Sridharan, S. |
|
dc.contributor.author |
Rajaram, R. |
|
dc.contributor.author |
Ratnam, M. Venkat |
|
dc.date.accessioned |
2015-08-27T06:42:06Z |
|
dc.date.accessioned |
2021-02-12T09:27:37Z |
|
dc.date.available |
2015-08-27T06:42:06Z |
|
dc.date.available |
2021-02-12T09:27:37Z |
|
dc.date.issued |
2004 |
|
dc.identifier.citation |
JASTP, v.66/6-9, p.507-515, 2004, doi: 10.1016/j.jastp.2004.01.026 |
en_US |
dc.identifier.uri |
http://localhost:8080/xmlui/handle/123456789/293 |
|
dc.description.abstract |
Wind measurements made during January 1995 through December 1997 using Partial Reflection Radar located at Tirunelveli (8.7°N, 77.8°E), a tropical station in India, have been used to monitor the long-period planetary wave activity in mesosphere and lower thermosphere. Lomb-scargle periodogram analysis and wavelet techniques are used to study the temporal development of these oscillations and their vertical structure. The observed amplitude and power spectrum show a broad peak near 5–7 days, which corresponds to 6.5-day wave reported earlier. The 6.5-day wave is observed to be an equinoctial phenomenon when background wind is westward, being strong during April/May and September/October months. This shows possible effect of semi annual oscillation on this wave. The 6.5-day oscillation is particularly strong in the zonal wind component, and seems to be present almost continuously in the 84–Full-size image (<1 K) height region. The wave activity is found to maximize during the weak-quasi biennial oscillation year. However, this observed feature need to be examined with a much longer dataset and we have initiated some efforts towards this direction. Mean climatology of these variations observed during three years (1995–1997) has been presented and found that there exists a strong interannual variability. The observed wave activity and its possible source mechanisms are compared and discussed with the available literature. |
en_US |
dc.language.iso |
en |
en_US |
dc.subject |
Equatorial dynamics |
en_US |
dc.subject |
Planetary waves |
en_US |
dc.subject |
Nonlinear interaction |
en_US |
dc.subject |
Mesosphere |
en_US |
dc.subject |
MF radar |
en_US |
dc.subject |
Equatorial mesosphere |
en_US |
dc.title |
MF radar observations of 6.5-day wave in the equatorial mesosphere and lower thermosphere |
en_US |
dc.type |
Article |
en_US |
dc.identifier.accession |
090782 |
|