DESCRIPTION |
Instrument Overview
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This instrument detects the electric charges
contained in the plasma cloud generated by a solid
particle impacting on a gold target. The principle
of this technique is similar to that adopted for
the impact plasma detectors of SP-2. The magnitude
of the positive and negative charges is
proportional to the mass of the particle Q=Am,
where A= 10**3C/s for an impact velocity of 78
km/s. The SP-1 system includes two similar
detectors. Each unit is made up of a base plate
(1) covered by a gold target (2) at zero potential,
perpendicular to the dust flow, and an array of
strip collectors (4). The collectors are parallel
to the dust flow; they are mounted on an insulator
(3) and their edge is protected from impacts by a
shield (5) connected electrically to the structure.
Adjacent collectors are biased at potentials of 30
V, with opposite polarities. The two sets of
electrodes in each detector detect a positive and a
negative current pulse, which are analysed and
recorded by the electronics unit. The entrance to
one detector is covered by a plastic foil, to
obtain additional information on density and/or
calibration factor. The characteristic parameters
of SP-1 are given in Table 8.
Table 8. Dust Particle Impact Plasma Detector
characteristics
Target material Gold (0.1 mm)
Toil sensor area 160 cm**2, one sensor covered with 0.6
and 2 micro m thick plastic foil
on Vegas-1 and 2, resp.
Impact charge range 3x10**-14 -10**-8 C
Estimated mass range 3x10**-17 -10**-11 g
Integration time 2 s (high data rate)
2.5 min (low data rate)
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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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