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Since there are no remarkable zonal phase structures in the SABER temperature data during this period (not shown here), it is difficult to infer that this local poleward wind disturbance is due to any modulation of planetary waves or enhanced meridional circulation.
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In this study, a nonlinear time-varying dynamic model is proposed to predict modulation sidebands of planetary gear sets.
In this paper, a simplified mathematical model is proposed to describe the mechanisms leading to modulation sidebands of planetary gear sets.
At the end, based on results of the parametric studies and experiments, general rules on modulation sidebands of planetary gear sets are proposed.
In addition to earlier found variations of the Martian magnetotail thickness as a function of the solar wind ram pressure, succeeding analysis of the magnetotail boundary crossings by Phobos 2 orbiter revealed modulation of magnetopause positions by planetary crustal magnetization.
On the basis of the relationships just explained above, the planetary wave modulation of the PRE vertical drift that was observed by Abdu et al. (2006b) was interpreted as caused by the PW-induced oscillations in the E region zonal wind that in turn modified the longitudinal/local time gradient in the E layer integrated conductivity.
In order to overcome the problem of finding the subband that contains the most fault-related modulation components, this paper proposed a new optimal demodulation subband selection method (ODSSM) for fault diagnosis of planetary gearbox.
Hundreds of planetary systems are known.
This is a sight of planetary strangeness.
"This is it: the Super Bowl of planetary exploration.
This lends support to current theories of planetary formation.
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