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In the present paper, we showed the design and performance of the prototype of the sensor probe, which is dedicated to measure plasma waves in the view point of the measurement of electric field components.
Consequently, sensor probes are expected to be a new way to measure plasma waves at multiple points in space.
The Plasma Wave Experiment (PWE) is one of instruments on board the Arase satellite to measure plasma waves and DC electric field.
Each sensor probe has the ability to measure plasma waves and transfer observation data to a central station, such as a satellite or a rocket (Kojima et al. 2010; Yagitani et al. 2011).
We succeed in developing the prototype model of the small sensor probe that had enough sensitivity for electric field to measure plasma waves and the ability to transfer observation data through wireless communication.
We expect to measure plasma waves such as chorus and EMIC propagating from their generation regions near the equatorial plane and derive their plasma wave properties (e.g., wave normal direction and Poynting flux) that could be also important key parameters to clarify the wave particle interaction along their propagation paths in the off-equatorial region.
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The WFC and OFA are dedicated to measuring plasma waves between 10 Hz and 100 kHz for the two electric field components and between 10 Hz and 20 kHz for the three magnetic field components.
The VLF instrument is one of the instruments on board Akebono used to measure VLF plasma waves, and the Poynting flux analyzer (PFX) is a subsystem of the VLF instrument (Kimura et al. 1990).
These probes can then be used to measure the plasma wave turbulence in a high spatial distribution.
Additionally, SWAVES will measure in situ plasma waves to provide an independent estimate of the local plasma density and temperature.
As shown in these figures, the sensitivity and frequency coverage of the PWE allow it to measure all expected plasma waves and radio waves in the inner magnetosphere.
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