October1966 Stratospheric Notes and Correspondence Wave Disturbances over the Equatorial 291 Propagating Pacific* M. Yanai and T. Maruyama GeophysicalInstitute, Tokyo University, Tokyo (Manuscript received 19 July 1966) 1. Introduction Since the exciting discovery of quasi-annual wind reversal (Ebdon,1960 ; McCreary, 1961; Reed et al, 1961), extensive works have been made on the long-period zonal wind oscillation in the equatorial stratosphere. The 26-month (or quasi-biennial) oscillation has been fully documented (see Reed, 1965). Several authors have suggested to relate the time change of the stratospheric mean zonal wind to the horizontal convergence of the eddy transport of momentum into the equatorial belt (Reed, 1962; Tucker, 1964). However, one still lacks observational evidence of large-scale eddies in the tropical stratosphere, although Riehl and Higgs (1960) noted a large shear line moving across the Caribbean Sea area during January 1960 at 110,000 f t (33.5 km) height. From March to July 1958, a dense upperair observation network in the central tropical Pacific was in operation in support of nuclear tests (see Fig. 1). The present authors have started to look into the data taken during the test period (Joint Task Force Seven Meteoro- Fig. * 1. Upper-air Pacific during Division stations in the central March-July 1958. of Meteorology , Contribution equatorial No. 149. logical Center, 1958) to detect eddy disturbancs in the lower stratospheric winds and have indeed found interesting facts. The following is a short tentative report of our findings. 2. Short-period wind oscillation In March 1958, the general winds in the concerned area were from the west at the heights between 60, 000 ft (18.3 km) and 70, 000 f t (21.3 km). Overlying above, strong easterly winds were blowing. Towards the end of the special observation (July 1958), the depth of the layer of westerly winds gradually became thin. The horizontal width of the belt of the westerly winds gradually became narrow. The westerly winds were seen only at 60, 000 ft height and only above several stations very close to the equator at the end of the observation period. Within this gradually weakening westerly flow, we find rather regular shortperiod oscillation at stations located close to the equator. Fig. 2a shows the 70, 000 f t wind data at Kapingamarangi (1*N, 155*E) during April 1958. One may recognize repeating changes of wind direction between 240* and 300*. Average period of this wind oscillation is somewhere around 5 days. Wind data at Ponape (7*N, 158*E) during the same period show very similar wind oscillation (Fig. 2b). The observed phases of the wind oscillation at these two stations are nearly identical. The existence of wind oscillation of this nature in other areas and other periods have been confirmed. Figs. 2c and 2d respectively illustrate similar wind oscillation at Canton Island (3*S, 172*W) and Balboa, Canal Zone (9*N, 80*W) for February and early March 1958. A detailed vertical time section at Canton Island for later half of April 1958 is reproduced in Fig. 3 to show the vertical extent of the 292 Journal Fig. 2. Fig. 3. Vertical Winds with of the Meteorological Society of Japan Vol.44,No.5 Short-period wind oscillation found at (a) Kapingamarangi, April 1958 (70, 000 ft), (b) Ponape, April 1958 (70, 000 ft), (c) Canton. Island, February-March 1958 (21 km), (d) Balboa, Canal Zone, February-March 1958 (70, 000 ft). time section of the southerly components lower are stratospheric shaded. winds at Canton Island for 15-30 April 1958. October1966 Notes and Correspondence 293 short-period wind oscillation. At around 20 km height southerly and northerly wind components appear alternatively. The wind shift first occurs at about 23 km height and progresses downward at a speed of roughly day to the tropopause level. 3. Westward propagation 1 km/ of the disturbance After several preliminary analyses, we have further found that the observed wind oscillation is, in fact, a reflection of retrogressive waves moving against the general westerly flow. In Fig. 4, the stations Kapingamarangi, Nauru (1*S, 167*E), Tarawa (1*N, 173*E) and Canton Island are placed along the abscissa which is nearly equal to the equator. The date is taken as the ordinate. When we plot 12 hourly wind observations taken at 70, 000 f t height (21 km for Canton), one can recognize large-scale waves propagating westward. Because of the limitted east-west coverage of the stations along the equator, we can estimate the phase velocity of the waves only crudely from the slope of the lines dividing southerly wind components and northerly components. The estimated propagation speed is about -2, 000 km/day or -23 m/sec . When we use the relationship L (wave length) =c (phase velocity) x T (period) and put T=5 days, we get L= 10, 000 km. Although we cannot conclude the existence of waves around the global equatorial belt at this stage, the wind oscillation found at Balboa is very indicative. It may be noteworthy that the estimated phase velocity is not too apart from the figure simply expected from the formula c= U- *L2/4 *2=13 m/sec -58 m/sec = - 45 m/sec . Similar rapid propagation of large-scale vortices has been observed in the upper troposphere in the same area (Yanai, 1963). Further extensive study of the disturbance is now in progress and will be reported in the near future. Acknowledgments The authors wish to express their thanks to Mr. Y. Fujiki and Miss Masako Onozuka for their assistance. This research has been partially supported through a grant from the Japan Society for the Promotion of Science as part of the Japan-U. S. Cooperative Science Fig. 4. Time series of 70, 000 ft (or 21 km) winds at Kapingamarangi, Nauru, Tarawa and Canton Island for 15-30 April 1958. Winds with southerly components are shaded. 294 Journal of the Meteorological Program. References Ebdon, R.A., 1960: Notes on the wind flow at 50mb in tropical and sub-tropical regions in January 1957 and January 1958. Quart. J. Roy. meteor. Soc., 86, 540-542. Joint Task Force Seven Meteorological Center, 1958: Meteorological Report on Operation Hardtack, 1958. JTFMC TP-8, Vols. 1-6. McCreary, F. E., 1961: Variation of the zonal winds in the equatorial stratosphere. Joint Task Force Seven Meteorological Center, JTFMC TP-20, 15pp. Reed, R. J., 1962: On the cause of the 26-month periodicity in the equatorial stratospheric winds. Meteor. Abhandlungen, Freien Universitat Berlin, 36, 245-257. Society of Japan 1965: The present status of the 26-month oscillation. Bull. Amer. meteor. Soc., 46, 374387. Reed, R. J., W. J. Campbell, L. A. Rasmussen and D. G. Rogers, 1961: Evidence of a downward-propagating annual wind reversal in the equatorial stratosphere. J. geophys. Res., 66, 813-818. Riehl, H., and R. Higgs, 1960: Unrest in the upper stratosphere over the Caribbean Sea during January 1960. J. Meteor., 17, 555-561. Tucker, G. B., 1964: Zonal winds over the equator. Quart. J. Roy, meteor. Soc., 90, 405-423. Yanai, M., 1963: A preliminary survey of largescale disturbances over the tropical Pacific region. Geofisica Internacional (Mexico), 3, 7384. 赤道 太平 洋上 を伝 播す る成 層圏 の波 動 柳 井 迫 Vol .44,No.5 雄・丸 山 健 東京大学理学部地球物理学教室 人
© Copyright 2025 Paperzz