CDA: Cosmic Dust Analyzer
The Cosmic Dust Analyser (CDA) instrument will provide direct observations of dust and ice particles in interplanetary space and in the Jupiter and Saturn systems. It will investigate the physical, chemical, and dynamic properties of these particles matter as functions of the distances to the Sun, to Jupiter, to Saturn, and to Saturn's satellites and rings. Finally, it will study the interaction of the particles with the Saturnian rings, satellites, and magnetosphere.
CDA Scientific Objectives
- To extend studies of interplanetary dust (sizes and orbits) to the orbit of Saturn
- To define dust and meteoroid distribution (sizes, orbits, composition) near the rings
- To map the size distribution of ring material in and near the known rings
- To analyse the chemical compositions of ring particles
- To study processes (erosional and electromagnetic) responsible for E ring structure
- To search for ring particles beyond the known E ring
- To study the effect of Titan on the Saturn dust complex
- To study the chemical composition of icy satellites from studies of ejecta particles
- To determine the role of icy satellites as a source for ring particles
- To determine the role that dust plays as a magnetospheric charged particle source/sink
CDA Instrument Description
The Cosmic Dust Analyser Subsystem (CDA) will provide direct observations of dust and ice particles in interplanetary space and in the Jupiter and Saturn systems. It will investigate the physical, chemical, and dynamical properties of these particles matter as functions of the distances to the Sun, to Jupiter, to Saturn, and to Saturn's satellites and rings. Finally, it will study the interaction of the particles with the Saturnian rings, satellites, and magnetosphere.
The four major functional elements of the CDA are:
- Dust analyser
- Main electronics
- Articulation mechanism
- High-rate detector assembly
The dust analyser (DA) consists of the following components: four charge pick-up grids; a hemispherical target, an ion collector, an electron multiplier, and the sensor electronics.
The charge pick-up grids collect the initial impact particles. They are mounted at the entrance of the sensor.
The hemispherical target is divided into two parts - a ring-shaped impact ionisation target and a chemical analyser target in the middle of the ionisation target. The chemical analyser target has an acceleration grid mounted 3 mm in front of it.
The ion collector has a grid that is negatively biased in order to collect the positively charged plasma ions produced at the impact ionisation target.
The electron multiplier is located in the centre of the hemispherical ion collector target. It amplifies the signal produced by ions capable of penetrating the ion collector grid. These ions originate from plasma produced by particle impact either on the impact ionisation target or the chemical analyser target. The output signal from the multiplier differs depending upon the target from which impacts are being measured.
The sensor electronics are contained in an electronics box attached to the DA sensor chassis. Among other components, this box contains charge-sensitive amplifiers (CSAs) that measure the signals from all of the grids in the DA.
The CDA main electronics includes amplifiers and transient recorders, a control and timing unit, a microprocessor unit, a bus interface unit, a power input circuit, a low-voltage converter, and a housekeeping system.
All CSA and electron multiplier signals are separately amplified by logarithmic amplifiers and then digitised by an analog-to-digital converter. The data are stored on transient recorders. Only the recorder connected to the pick-up grids is operated continuously. All others are activated only by a signal detected at a target or the acceleration grid. The control and timing unit stores and decodes information received from the microprocessor and produces all timing and synchronisation signals required for instrument operation.
The microprocessor samples and collects the buffered measurement data, coordinates the subsystem measurement cycle, controls the instrument operating modes, processes the data according to a program loaded in its memory, and outputs data to the spacecraft upon request through the bus interface unit (BIU). The BIU is the interface circuit between the spacecraft and the microprocessor and is powered by the CDA instrument. The power input circuit is the interface with the spacecraft Power and Pyrotechnics Subsystem (PPS) and contains a filter circuit and a regulator to produce a DC voltage to feed the low-voltage converter.
The low-voltage converter is a DC/DC converter that provides different regulated low voltages for the electronics circuits and the supply voltage for the high-voltage converters. The converters are synchronised to the 100 kHz clock provided through the BIU from the Command and Data Subsystem (CDS).
The CDA housekeeping system is a data system that multiplexes, digitises, and stores information on the instrument current, the low voltages, the high voltages, and temperature measurements.
The articulation mechanism (AM) allows the entire CDA instrument, including the high-rate detectors, the dust analyser, the main electronics, and the articulation mechanism electronics, to be rotated or repositioned with respect to the spacecraft coordinate system.
High-Rate Detector Assembly
The high-rate detectors (HRDs) are two redundant independent sensors. The electronics for the sensors are contained in the HRD electronics box, and each sensor has its own electronics, independent of the other sensor. The HRD will be operated in two modes: normal and calibrate. In normal mode, the operational HRD continuously collects dust particle data. In calibrate mode, a calibration cycle is initiated, which consists of a sequence of pulses sent to the HRD by the in-flight calibrator (IFC) to verify the stability of the electronics.
||CAPS: Cassini Plasma Spectrometer
||CIRS: Composite Infrared Spectrometer
Last Update: 25 Feb 2005