INERTIO-GRAVITY WAVES AND SUBTROPICAL MULTIPLE TROPOPAUSES - VERTICALWAVE-NUMBER SPECTRA OF WIND AND TEMPERATURE OBSERVED BY THE MU-RADAR,RADIOSONDES AND OPERATIONAL RAWINSONDE NETWORK
Md. Yamanaka et al., INERTIO-GRAVITY WAVES AND SUBTROPICAL MULTIPLE TROPOPAUSES - VERTICALWAVE-NUMBER SPECTRA OF WIND AND TEMPERATURE OBSERVED BY THE MU-RADAR,RADIOSONDES AND OPERATIONAL RAWINSONDE NETWORK, Journal of atmospheric and terrestrial physics, 58(6), 1996, pp. 785-805
We have carried out continuous observations of the tropopause region o
ver Japan for three weeks during the Baiu (early summer rain ''in Japa
n'') season in 1991, by using a VHF Doppler radar (the MU radar), radi
osondes launched at the radar site and operational rawinsondes at five
meteorological stations. Based on these observations, we try to exami
ne the hypothesis that the multiple tropopauses and the dominant inert
io-gravity waves are one and the same feature, and obtain some interes
ting results that are not inconsistent with this hypothesis. First, ve
rtical wavenumber spectra and hodographs analyzed from the radar wind
data in the tropopause region suggest that inertio-gravity waves with
vertical wavelengths of similar to 2 km are quasi-monochromatically do
minant (with 2-3 day scale variabilities of 10-20%), and are in accord
ance with activities of the subtropical jet stream and mesoscale cyclo
ne-front system activities observed by the operational network. Second
, striking (potential) temperature fluctuations are detected simultane
ously by the radiosondes and rawinsondes, which appear as multiple tro
popauses in meridional cross-section analysis. Third, vertical wavenum
ber spectra analyzed from the radiosonde temperature data are consiste
nt with the radar wind spectrum, if we assume that both wind and tempe
rature fluctuations are mainly induced by the dominant inertio-gravity
waves. Finally, we confirm that the dominant inertio-gravity waves ca
n be barely detected also from routine rawinsonde (1.5-km running-mean
) wind data if the amplitude is larger than 1.5 m/s. However, the mono
chromatic wave structures are generally quite localized in space and t
ime.