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EMFISIS

An instrument suite on the Van Allen Probes


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INSTRUMENT DESCRIPTION


EMFISIS INSTRUMENT DESCRIPTION

The EMFISIS instrumentation suite provides measurements of wave electric and
magnetic fields as well as DC magnetic fields for the Van Allen Probes mission .
EMFISIS provides a comprehensive set of wave electric and magnetic field
measurements covering the frequency range from 10 Hz up to 400 kHz. EMFISIS
comprises two sensors: a tri-axial fluxgate magnetometer (MAG) and a trixaxial
AC magnetic search coil magnetometer (MSC). Additionally, to measure AC signals
the Waves experiment which includes AC electric fields (from the EFW) experiment
and a tri-axial search coil magnetometer. These instruments are welded into one
integrated whole by a Main Electronics Box (MEB) which ties all measurements
together for maximum impact on the Van Allen Probes.

 The majority of the electronics are contained within the Main Electronics box
comprised of seven printed circuit boards. From bottom to top, is first the Low
Voltage Power Supply (LVPS) which converts primary spacecraft power to voltages
used by the rest of the suite, followed by the Central Data Processing Unit
which controls the suite and handles data transfer to and from the central
spacecraft systems. Above this are the four boards of the Waves component of the
EMFISIS system: two FFT engine boards and the AC electric field and AC magnetic
field receivers. Completing the stack is the MAG drive, sampling, and heater
control board.


MAGNETOMETER

The EMFISIS magnetometer is the latest in a series of magnetic field
investigations developed by the research group at GSFC. This magnetometry group
has a long and successful track record of development and implementation of
complex magnetic field investigations for planetary exploration, earth
observing, and space physics missions. The sensors and analog electronics are
"off-the-shelf" designs which have been or are being flown on numerous NASA
missions including Juno, Messenger, and STEREO.

The STEREO instruments were themselves based on more than fifty magnetometers
previously developed for space missions, from Voyager (still operational after
more than 28 years in space), ISPM, GIOTTO, WIND, ACE, CLUSTER I & II (more than
10 instruments), DMSP (11 instruments) to the more recent Lunar Prospector, and
Mars Global Surveyor instruments. They represent state‑of‑the‑art instruments
with unparalleled performance.

The EMFISIS fluxgate magnetometer is a wide-range, high performance triaxial
fluxgate magnetometer system. The signal processing, analog to digital converter
(A/D) and interface electronics are implemented on a single electronics card
integrated MEB as discussed above. A block diagram is illustrated in Figure 12.
This configuration makes optimal use of limited spacecraft resources and has
been used successfully on several prior missions (Lunar Prospector, STEREO,
Messenger). It takes full advantage of miniaturization made possible by
contemporary technology and the maturity of the magnetometer design. The wide
dynamic range of the instrument covers ambient fields from <0.02 nT to 65,536 nT
in three ranges selected automatically by the CDPU or ground command. The upper
limit measurement capability is designed to make possible operation in the
Earth’s surface field which provides the appropriate range for Van Allen Probes
perigee measurements. 

The magnetometer electronics include three 16-bit sigma-delta high resolution
A/D converters to easily resolve small amplitude fluctuations of the field. The
control and CDPU interface electronics are implemented in a radiation hardened
field programmable gate array (FPGA) and total power consumption is less than
0.5W when fully operational. High reliability and radiation tolerance is
obtained by the use of extremely conservative designs. The intrinsic zero drift
of the sensors is expected to be below 0.2 nT over periods of up to 6 months.
The principal instrument characteristics are summarized Table 1.

Magnetometer Specifications

(Three dynamic ranges)

Data Rate

~3 kbs, depending on compression

Sampling Cadence

64 vectors/s

Ranges

0 - +/-65536 nT

0-4096 nT

0-256 nT

Resolution

2 nT  (65536 nT range)
0.16 nT (4096 nT range)
.001 nT (256 nT range)

Accuracy

0.1 nT (sensor alone, with spacecraft 5 nT)

Frequency Range

0-30Hz

 

Table 1 Magnetometer (MAG) Specifications

 

The MAG instrumentation on the Van Allen Probes is nearly identical to the
instruments built for the IMPACT investigation aboard the STEREO mission. The
only modifications are the mechanical, power and data interfaces for
compatibility with the EMFISIS suite and Van Allen Probes spacecraft designs as
well as added radiation tolerance through parts selection and shielding.

The sensor assembly consists of an orthogonal triaxial arrangement of ring‑core
fluxgate sensors plus additional elements required for thermal control. The
fluxgate sensors are the latest in a series developed for space magnetic field
measurements by Acuña et. al. [1974; 2002] and which have been extensively used
in many space missions due to their superior performance and low power
consumption. The detailed principles of operation of fluxgate magnetometers are
well known and will not be repeated here. For additional information the reader
is referred to Ness, [1970] and Acuña, [1974; 2002].

The fluxgate sensors are driven cyclically to saturation by a 15 KHz signal
derived from the CDPU master clock. The sensor drive signals are derived from an
efficient high energy storage system which is capable of driving the ring core
sensors to peak excitations which are more than 100 times the coercive
saturation force of the cores. This type of excitation eliminates from
consideration many "perming" problems which have been attrib­uted to fluxgate
sensors in the past. In the absence of an external magnetic field, the fluxgate
sensors are "balanced" and no signal appears at the output terminals.

When an external field is applied, the sensor balance is disturbed and a signal
containing only even harmonics of the drive frequency appears at the output of
the sensors. After amplification and filtering, this signal is fed to a
synchronous detector and high gain integrating amplifier used to generate a
current proportional to the magni­tude of the applied field. This signal is
fed‑back to the sensor to null the effective magnetic field. The output of a
single axis magnetometer is then a voltage proportional to the magnitude,
direction and polarity of the ambient magnetic field with respect to the sensor
axis orientation. A triaxial magnetometer is created when three single-axis
sensors are arranged orthogonally and three sets of signal processing
electronics are used to produce three output voltages proportional to the
orthogonal components of the ambient magnetic field.


WAVES INSTRUMENT AND THE MAGNETIC SEARCH COIL (MSC)

The primary objective of the Waves instrument is to provide sufficient
information on plasma waves in the radiation belts to quantitatively determine
the effect of these waves on radiation belt particles. Specifically, the Waves
investigation measures all 3 components of the electric and all 3 components of
the magnetic field for waves in the frequency range between 10 Hz and 12 kHz.
The Waves system in concert with the CDPU also includes the ability to measure
the wave-normal angle and Poynting flux for electromagnetic waves such as
whistler-mode hiss and chorus within the constraints of limited telemetry.
Measuring both the electric and magnetic components of the waves also allows one
to distinguish between electromagnetic and electrostatic waves, especially
important below the electron cyclotron frequency.

The instrument also provides a single electric field component of waves from 10
kHz to 400 kHz in order to measure the spectrum of electron cyclotron harmonic
emissions and to measure the frequency of the upper hybrid resonance band,
thereby providing an accurate determination of the electron density. Figure 15
and Figure 16 show the frequency range and amplitudes for the wave phenomena
relevant to the Van Allen Probes objectives. The Waves instrument will have
suitable dynamic range to cover all of these wave phenomena of relevance to
radiation belt physics.



The electric field signals for the Waves instrument are provided to the EMFISIS
instrumentation from the EFW experiment. These signals consist of differential
voltages from opposing EFW spherical sensors. Two of these signals are derived
from long wire booms in the spin-plane of the spacecraft. The third signal is
provided by rigid booms mounted along the spacecraft axis

 



The Waves magnetic sensors consist of three identical search coil antennas
mounted in a tri-axial configuration with each antenna oriented parallel to one
of the spacecraft scientific (UVW coordinates) axes. Two are parallel to the two
spin-plane EFW electric field double probes and the third is parallel to the
spin axis double probe. The search coils are mounted on the boom opposite from
the magnetometer boom to reduce any interference from the spacecraft. The
spacecraft systems and other instruments have been designed and built with sound
engineering practices that minimize electromagnetic interference.

 


ABOUT MENU

 * EMFISIS Science
 * Instrument Description
 * UVW Spacecraft Coordinate System
 * Team
 * EMFISIS @ rtems.org
 * Current Location of the Van Allen Probes
 * Van Allen Probes Publications


SCIENCE

 * Science Introduction
 * Science Goals
 * Magnetometer Release Notes