DESCRIPTION |
Instrument Overview
===================
The ROMAP sensors (fluxgate magnetometer, electrostatic
analyser and Faraday cup) measure the magnetic field from
0 to 32Hz, ions up to 8.0 keV and electrons up to 4.2 keV.
High integration level of sensors and electronics is the basic
for a combined field/plasma measurement instrument with less
than 1 Watt power consumption and 1 kg mass.
Additional two pressure sensors are included in the ROMAP
sensor arrangement.
The sensors are moved from COSAC to ROMAP to optimise long
term operation of pressure sensors. Data of both pressure
sensors are transmitted within the housekeeping frame and
are handled / archived as housekeeping values.
Scientific Objectives
=====================
Main scientific goals of ROMAP are
(1) long term measurements on the surface to study the
cometary activity as function of the distance from the Sun
and
(2) magnetic measurements during the descent phase of the
Lander to investigate the structure of the remnant
magnetization of the nucleus.
Calibration
===========
MAG : Data are precalibrated by nominal scaling. Offsets can
not be corrected automatically. This will be done by
sequence specific cal files (L3).
Finally corrected data (includes the removal of
spacecraft disturbances) are only available for selected
data of scientific interest (L5).
SPM : Instrument calibration will be done preliminary (L3) and
finally for derived data products (L5).
Operational Considerations
==========================
Main measurement sequences are:
- During Flybys
- During Descent
- On cometary Surface
Common operation with Instruments generating magnetic
interferences shall be avoided.
Common operation with RPC-MAG onboard the orbiter is highly
desirable
Electronics
===========
The ROMAP electronics consists of two boards placed inside the
common electronics box. The central part of the near sensor
electronics on the first board is a FPGA which controls AD and
DA-converters. The 16-bit AD converters are digitising science
and housekeeping data from all three sensors. Typical analogue
parts of fluxgate magnetometers like filters or phase-sensitive
integrators are substituted by fast digitalization of the sensor
AC-signal and the following data processing in FPGA's (which
overtakes the functions of the former analogue parts). In this
way mass is saved without any loss of accuracy. The resolution
is still restricted by sensor noise (less than 5pT/sqrt(Hz)
at 1Hz), not by electronics. Compensation fields for the magnetometer
and high voltage steps for electrostatic analyser and Faraday cup
are controlled via DA-converters (dashed lines). The near sensor
electronics is developed by Magson GmbH Berlin The high voltage
generator (developed by the KFKI) is in a separate shielded box
on the front panel of the common electronics box. The controller
is located on the second ROMAP board.
It controls MAG and SPM, stores their data output and implements
the interface to the Lander Command and Data Management System
(CDMS). It triggers the measurement cycle of the magnetometer,
implements the digital magnetometer algorithm, controls the
magnetometer feedback and generates data frames. For the SPM
sensors the controller has implemented the counting logic for
electrons and ions, samples Faraday cup data, generates SPM data
frames, controls the high voltage parameters (energy,
elevation), controls the channeltron HV-supply and computes the
plasma parameters. In the parameter mode only the sums of the
rows and columns of the sampled ion and ion-current arrays are
transmitted.
The controller is based on a RTX2010. Address decoder, reset
logic, clock generators, control signals generator, watchdog
logic and CDMS interface are integrated within a FPGA. Hard- and
software are developed by the IWF Graz.
Sensor / Sensor Location
========================
The magnetometer sensor consists of two ringcores (crossed in to
each other) as well as pick-up coils and Helmholtz coils for
each sensor axis. The coil system design without mechanical
support allows the compensation of the external field on the
ringcore position with high homogeneity and low weight (the
overall sensor weight is 30g). Dynamic feedback fields as well
as offset fields up to 2000nT can be generated in order to
compensate Lander and/or Orbiter DC stray fields. The main part
of the SPM-sensor is a hemispherical electrostatic analyzer with
two channeltrons (CEM's) for ions measurement and one for
electrons measurement. The entry of the ion channels is equipped
with deflection plates to realize the spatial resolution.
Despite the small size of the sensor, the sensitivity and
resolution of the instrument are high and its field of view wide
(appr. 100 degree).
The E/q-range extends from 0 to 8 kV. Using CEMs in counting
mode the electrostatic analyzer measures electron and ion
distribution in a wide energy range. Hemisherical deflection
plates analyze the energy in 32 or 64 steps. All major plasma
parameters as bulk velocity, density and isotropic temperature
of protons and electrons can be derived.
A retarding-grid Faraday cup sensor is implemented to measure
currents due to fluxes of low energy charged particles on a
collector plate. The Faraday cup measures the 'reduced' velocity
distribution of the plasma due to its inherent integration over
velocities contained in a plane of differential thickness
perpendicular to the axis of the sensor. The combined
magnetometer / SPM sensor is mounted on a 60 cm boom which is
fixed with a hinge on the upper edge of the Lander structure
and with a launch lock on the Lander balcony. After opening the
launch lock, the boom will be deployed by two springs inside
the hinge.
Two pressure sensors are selected to cover the whole pressure
range from 10^-8 mbar to 10 mbar. For the range from 10^-8 mbar
to 10^-3 mbar an ionising system (Penning) is deployed while for
the range from 10^-3 mbar to 10 mbar a heat conduction sensor
(Minipirani) is available.
Operational Modes
=================
ROMAP can be basically operated in 3 modes:
- Slow Mode
- Fast Mode
- Surface Mode
Subsystems
==========
The sub-systems are described in Auster et al, 2005.
Measured Parameters
===================
Magnetic field; resolution 10 pT
Electrons: 0.35 ... 4200 eV
Ions: 40 ... 8000 eV
Pressure; 10^-8 mbar to 10 mbar.
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