Wind gradients at meteor heights over mid-latitude stations

Details Wind gradients at meteor heights over mid-latitude stations Wind gradients at meteor heights over mid-latitude stations

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ineps..95..427d&link_type=abstract

Proceedings of the Indian Academy of Sciences - Earth and Planetary Sciences, Volume 95, Issue 3, pp.427-434

Computer Science

Meteor Winds, Amplitude And Phase Gradients, Diurnal And Semidiurnal Components, Mid-Latitudes

Scientific paper

The gradients of amplitude and phase of diurnal and semidiurnal components of zonal and meridional winds in the height intervals of 80-90 km and 90-100 km are studied using the meteor wind radar data collected at Atlanta (34°N, 84°W) during the period August 1974-March 1978. The results are compared with those at Adelaide (35°S, 139°E). It is found that the gradients vary in an opposite manner between the two height intervals.

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