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scostep 2010 (stp12) - Leibniz-Institut für Atmosphärenphysik an der ...

scostep 2010 (stp12) - Leibniz-Institut für Atmosphärenphysik an der ...

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STP12 Abstracts<br />

Berlin, 12 - 16 July <strong>2010</strong><br />

SCOSTEP Symposium <strong>2010</strong><br />

Simult<strong>an</strong>eous observation of quasi 16-day wave in the mesospheric winds <strong>an</strong>d<br />

temperature over low-latitude with SKiYMET radar<br />

Das Siddarth Sh<strong>an</strong>kar<br />

Space Physics Laboratory, VSSC, Triv<strong>an</strong>drum<br />

This paper presents for the first time the seasonal characteristics of 16 day pl<strong>an</strong>etary<br />

wave on mesospheric temperature <strong>an</strong>d winds simult<strong>an</strong>eously over a low-latitude station<br />

Thumba (8.5 o N, 76.5 o E) using meteor radar. Four-years (2005-2008) of meteor winds <strong>an</strong>d<br />

temperature data are used for the present study. It is observed that the amplitude of 16-day<br />

wave in zonal component is more th<strong>an</strong> that of meridional. Further <strong>an</strong>alysis shows that<br />

westerly phase of zonal wind is more favorable for the 16-day waves. The maximum<br />

amplitude in mesospheric temperature is observed during J<strong>an</strong>uary-February <strong>an</strong>d August-<br />

September. Climatology of 16-day wave shows the variability of semi-<strong>an</strong>nual oscillation<br />

(SAO) on mesospheric temperature but not on winds. The vertical amplitude structure of<br />

zonal component shows the maximum amplitude at ~ 88-92 km with const<strong>an</strong>t phase. It is also<br />

noticed that zonal <strong>an</strong>d meridional wind are in phase, whereas as temperature leads zonal wind<br />

by 5±1 days. The signific<strong>an</strong>t of the present result shows the wave characteristics, effect of<br />

background wind <strong>an</strong>d m<strong>an</strong>ifestation of SAO on their propagation behavior. It is envisaged<br />

that the present result will contribute to our un<strong>der</strong>st<strong>an</strong>ding of the dynamics of the MLT region<br />

at low latitude in the northern hemisphere. The detail results will be discussed in the<br />

upcoming symposium.

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