ASPERA-3: Neutral Particle Imager
The Neutral Particle Imager head is a replica of the NPI - MCP sensor
developed for the ASPERA - C experiment on the Mars - 96 mission and
successfully flown on the Swedish micro satellite Astrid launched in
In the NPI the charged particles, electrons and ions, are removed by the electrostatic deflection system which consists of two disks separated by a 3 mm gap. The 5 kV potential sweeps away all charged particles with energies up to 60 keV. Since the integral ENA flux substantially exceeds the charged particle flux for energies greater than 60 keV, this rejection energy is sufficient for satisfactory performance. The disks also collimate the incoming beam in the elevation angle. Apart from being ON or OFF the deflection system can be operated in two other modes, alternative mode and sweeping mode. The deflection system also collimates the beam into 32 sectors.
Neutrals passing through the deflection system hit a 32 sided cone target with a grazing (20°) angle of incidence. A MCP stack in the Z configuration detects the particles leaving the target block with 32 anodes. The signal from the MCP gives the direction of the primary incoming neutral. The MCP operates in ion mode with a negative bias of -3.0 kV and thus detects (a) sputtered ions of the target material, (b) ions resulting from stripping of the primary neutrals, and (c) neutrals reflected from the target surface. In order to improve the angular resolution and collimate the particles leaving the interaction surface, 32 separating walls are attached to the target forming a star-like structure. NPI covers 4p in one instrument scan and produces an image of the ENA distribution in the form of an azimuth x elevation matrix. To suppress the UV flux he NPI target uses the same coating as in the PIPPI and ASPERA-C experiments, namely, DAG 213, a resin - based graphite dispersion.
|© 2006, Max Planck Institute for
Solar System Research, Lindau