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The modulation process is identified as a tidally-induced change of the background buoyancy frequency.
We estimate how these particles affect the modulation process in the heliosphere.
The effectiveness of this new modulation process was studied using a Design of Experiments.
At the transmitter, the channel-encoding process is coupled with the modulation process, producing a system known as trellis-coded modulation.
And again, during the 1960's there was an attempt by Voelcker to look at the modulation process using a unified approach.
In coded modulation, error-correcting codes form an integral part of the modulation process, making the signal less susceptible to noise.
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The assumption of a specific coupling between the two modulation processes is investigated.
The physical underpinnings of these solar changes need to be understood and their effect on GCR modulation processes clarified.
Implications of these observations for our understanding of different modulation processes in the inner three-dimensional heliosphere are presented.
Galactic cosmic rays entering the heliosphere are subjected to four modulation processes: diffusion, convection, adiabatic deceleration in the expanding solar wind, gradient, curvature and current sheet drifts.
This is done with a well-established numerical model which includes all four major modulation processes, also the solar wind termination shock (TS) and the heliosheath.
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