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Recently, the horizontal and vertical cross wind at 225‐ to 295‐km altitude were derived from linear acceleration measurements of the Gravity field and steady‐state Ocean Circulation Explorer satellite. The vertical component of these wind data is compared to wind data derived from the mass spectrometers of the Atmosphere Explorer C and E and Dynamics Explorer 2 satellites. From a statistical analysis of the 120‐s moving‐window standard deviation of the vertical wind (σ(V_z)), no consistent discrepancy is found between the accelerometer‐derived and the mass spectrometer‐derived data. The validated Gravity field and steady‐state Ocean Circulation Explorer data are then used to investigate the influence of several parameters and indices on the vertical wind activity. To this end, the probability distribution of σ(V_z) is plotted after distributing the data over bins of the parameter under investigation. The vertical …