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Fig. 7 | Earth, Planets and Space

Fig. 7

From: Frequency spectra of horizontal winds in the mesosphere and lower thermosphere region from multistatic specular meteor radar observations during the SIMONe 2018 campaign

Fig. 7

Plots a–c illustrate the frequency spectra of horizontal velocities obtained from the WCFI and MWE methods around three altitudes, i.e., 84(±3), 90(±3), 96(±3) km. The solid black line in plots illustrate the spectra obtained from the WCFI method, and the blue dashed lines show the MWE spectra. The solid and transparent shades of black lines and blue lines in the plots show power-law slopes of the WCFI and MWE spectra, respectively. Slope values with standard error are inscribed in the plots in black and blue fonts, which corresponds to WCFI and MWE spectra, respectively

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