Mesospheric wind observations derived from Super Dual Auroral Radar Network (SuperDARN) HF radar meteor echoes at Halley, Antarctica: Preliminary results

The implementation of a technique to derive mesospheric winds from HF radar observations of meteor echoes at Halley (76°S, 27°W), Antarctica, is described. The meteor echoes are observed at near ranges (less than 400 km) and have characteristics distinctly different from echoes backscattered from plasma irregularities in the E and F regions of the ionosphere. A Lorentzian model is used to fit the echo spectrum. The echo occurrence rate has the diurnal variation expected of meteors with a minimum in the afternoon. There also appears to be an annual variation which may be related to seasonal changes in the atmosphere. At present, results are confined to a single beam; that directed toward the south geographic pole is presented here, as this will give the meridional component of the wind and can be compared with other studies. The meridional wind is found to be dominated by the semidiurnal tide most of the year, with maxima in spring and autumn. Data for May 1996 show that the semidiurnal tide is dominant, but there are significant contributions from the 24-hour and 8-hour tides. A moving window spectral analysis technique allows the temporal behavior of the waves over a 10-day period to be studied. A quasi 2-day wave is observed during this interval, and slight changes of period with time can be observed. Planetary waves with periods of 5 and 10 days are observed during the winter of 1996. The radar has been operating since 1988, and so these data form a substantial and valuable database of mesospheric observations in the high-latitude southern hemisphere.

[1]  H. Teitelbaum,et al.  Non-linear interaction between the diurnal and semidiurnal tides: terdiurnal and diurnal secondary waves , 1989 .

[2]  H. Roscoe,et al.  Midwinter Start to Antarctic Ozone Depletion: Evidence from Observations and Models , 1997 .

[3]  J. Forbes,et al.  First results from the meteor radar at South Pole: A large 12‐hour oscillation with zonal wavenumber one , 1995 .

[4]  A. Manson,et al.  Dynamics of the middle atmosphere at Saskatoon (52°N, 107°W): a spectral study during 1981, 1982 , 1986 .

[5]  Farzad Kamalabadi,et al.  Evidence for nonlinear coupling of planetary waves and tides in the Antarctic mesopause , 1997 .

[6]  R. Greenwald,et al.  An HF phased‐array radar for studying small‐scale structure in the high‐latitude ionosphere , 1985 .

[7]  M. Jarvis,et al.  First mesospheric observations using an imaging Doppler interferometer adaptation of the dynasonde at Halley, Antarctica , 1997 .

[8]  A. Hedin Extension of the MSIS Thermosphere Model into the middle and lower atmosphere , 1991 .

[9]  T. B. Jones,et al.  DARN/SuperDARN , 1995 .

[10]  J. Forbes,et al.  Dynamics of the Antarctic and Arctic mesosphere and lower thermosphere regions—II. The semidiurnal tide , 1993 .

[11]  J. Forbes,et al.  Dynamics of the Antarctic and Arctic mesosphere and lower thermosphere regions—I. The prevailing wind , 1993 .

[12]  J. Forbes,et al.  Diurnal tide in the Antarctic and Arctic mesosphere/lower thermosphere regions , 1995 .

[13]  John W. MacDougall,et al.  Super Dual Auroral Radar Network observations of meteor echoes , 1997 .

[14]  R. Greenwald,et al.  Polar Anglo‐American Conjugate Experiment , 1989 .

[15]  T. Thayaparan The terdiurnal tide in the mesosphere and lower thermosphere over London, Canada (43°N, 81°W) , 1997 .

[16]  J. Forbes,et al.  Dynamics of the antarctic and arctic mesosphere/lower thermosphere regions , 1992 .