Abstract

This study presents a new method for determining a neutral wind velocity vector. The basis of the method is measurement of the group velocities of internal gravity waves. Using the case of the Boussinesq dispersion relation, we demonstrated the ability to measure a neutral wind velocity vector using the group velocity and wave vector data. An algorithm for obtaining the group velocity vector from the wave vector spectrum is proposed. The new method was tested by comparing the obtained winter wind pattern with wind data from other sources. Testing the new method showed that it is in quantitative agreement with the Fabry–Pérot interferometer wind measurements for zonal and vertical wind velocities. The differences in meridional wind velocities are also discussed here. Of particular interest were the results related to the measurement of vertical wind velocities. We demonstrated that two independent methods gave the presence of vertical wind velocities with amplitude of ~20 m/s. Estimation of vertical wind contribution to plasma drift velocity indicated the importance of vertical wind measurements and the need to take them into account in physical and empirical models of the ionosphere and thermosphere.

Highlights

  • Internal gravity waves (IGWs) contribute significantly to general atmospheric circulation, providing a coupling between the lower, middle, and upper atmosphere

  • We propose a new method for determining the neutral wind velocity vector, based on IGW group velocity measurements

  • We compared the neutral wind obtained from measurements of IGWs group and phase velocities with the HWM2007 model, results of our previously developed method [6,7], and Fabry–Pérot interferometer (FPI)

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Summary

Introduction

Internal gravity waves (IGWs) contribute significantly to general atmospheric circulation, providing a coupling between the lower, middle, and upper atmosphere. Sufficient statistics obtained from IGW parameters (including a full 3D velocity vector) help to parameterize and account for the effects of these waves in global and local models. Incoherent Scatter Radar (IISR) [1,2] have been arranged to form a triangle with sides ~100 km, which is convenient for investigating medium- and large-scale traveling ionospheric disturbances (TIDs). The vertical sounding ionosonde DPS-4 is located in Irkutsk, while the Incoherent Scatter Radar is 98 km to the north-west of Irkutsk. In the mode of detecting dynamic TID parameters, the radar measures the vertical profiles of scattered signals at two frequencies. Methods for determining the TID space–time structure and propagation parameters have been developed using the cross-correlation and phase difference analysis of the IISR and DPS-4 ionosonde data [3,4]

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