DESCRIPTION |
Instrument Overview
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Fluctuating electric fields are detected in three
pairs of orthogonal antennas, one aligned with the
spacecraft spin axis and the other two in the
equatorial plane (Fig. 6). The antenna voltages
are preamplified and then analyzed by a radiometer
consisting of four superheterodyne receivers, which
step through the frequency range from 30 kHz to 2
MHz. Two channels are narrow-band with a filter
bandwidth of 3 kHz, and two have a filter bandwidth
of 10 kHz. The narrow-band filters sweep between
30 kHz and 1 MHz in 12 steps, while the broadband
filters cover frequencies between 40 kHz and 2 MHz,
also in 12 steps. The frequencies are scanned in a
nonlinear manner so that the highest frequencies
are sampled 12 times as often as the low
frequencies. The complete scan sequence consists
of 72 steps; 56 s are required to read out all
channels at 1024 bit/s.
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REFERENCES |
Reinhard, R and B. Battrick (eds), 'Space Missions to Halley's Comet', European
Space Agency ESA SP-1066, ESA Pub Div, Moordwijk, Netherlands, 1986.
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