parameters of internal gravity waves in the mesosphere-lower thermosphere region derived from meteor radar wind measurements

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ID: 200956
2005
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Abstract
A procedure of revealing parameters of internal gravity waves from meteor radar wind measurements is presented. The method is based on dividing the measuring volume into different parts and, using wavelet analysis, calculating the phase progression of frequency peaks in the vertical and horizontal direction. Thus, the distribution of vertical and horizontal wavelengths and directions of IGW energy propagation, using meteor radar data, has been obtained. The method was applied to a 4-month data set obtained in July and August, 1998 and 1999. As expected, the majority of waves have been found to propagate upwards, although a considerable number seem to propagate downwards as well. High-frequency (intrinsic periods T* of less than 2 h) waves are dominating. The distribution of waves over the course of an average day is only weakly structured, with weak maxima in the morning and evening.
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oleynikov2005annalesparameters Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors ;A. N. Oleynikov;Ch. Jacobi;D. M. Sosnovchik
Journal journal of food measurement and characterization
Year 2005
DOI
10.5194/angeo-23-3431-2005
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