Ørsted Satellite Project


Ørsted CPD Particle Experiment

Basic description of the CPD experiment

The high-energy Charged-Particle Detector (CPD) experiment on the Ørsted satellite launched into in a Low-Earth Orbit (LEO) aims at detecting high-energy radiation of particles of the following kinds and energies:

- Electrons : 50 keV - 1 MeV
- Protons : 250 keV - 30 MeV
- Alfa particles: 1-100 MeV

The experiment uses an array of 6 solid-state silicon detectors with different shieldings and depletion depths. The amplified signals from particles entering the detectors are connected to pulse-height analyzers to provide energy resolution of the detected radiation. Four of the analyzer units have 8 discriminator level; two have 4 levels only. The counts in the total of 40 different channels are collected by the experiment computer, that communicate the data and status to and receives commands from the satellite Central Data Handling (CDH) computer.

The detectors with their high-voltage power supplies, pulse amplifiers, pulse-height analyzers, and counter circuits and the experiment computer are all built into a box that may function as a stand-alone unit. It needs standard supply voltages and communicates data and commands with an external computer system via a RS485 signal line.

The experiment has been calibrated at NASA's Goddard Space Flight Center electron- og ion-accelerator facility which can generate radiation of electrons and ions at energies up to 2 MeV. A "flight-unit" of the CPD particle experiment is now orbiting on the Ørsted satellite while an identical "spare flight-unit" is kept for possible tests of performance or post-flight calibration.

The Ørsted satellite was launched on 23 February 1999 into a near polar, slightly elliptical orbit. Inclination is 96 deg, the altitude varies between 640 and 860 km. At launch the ascending node was at 14:11 LT, but drifts toward morning at 0.88 min/day. The satellite is gravity- gradient stabilized such that the 8-m boom is always pointing vertically upward. The rotation around the boom axis is controlled such that the SIM star imager co-located with the CSC vector magnetometer in the gondola look away from the sun.

Four of the CPD particle detectors look vertically upward along the 8-m boom while the remaining two look horizontally to the side. The orientation is seen in the photo to the left. The detectors look out through cut-aways in the top and side solar panels. The pitch angle for each detector can be determined from the vector magnetometer measurements combined with the rotation of the boom-mounted gondola with respect to the satellite body. In near-polar regions (above some 60 deg in latitude) with the high inclination of the geomagnetic field the 4 upward-looking detectors will all look into the loss cone which at the altitude of the satellite (around 700 km) is at 60 deg pitch angle. The 2 horizontally-looking detectors, correspondingly, will always look at the radiation outside the loss cone within polar regions.

Technical specifications

The overall main characteristics of the CPD instrument is shown in Table 1:

Physical parameters
Overall max. dimensions260 x 199 x 113 mm
Total mass 2.3 kg
Total power consumption1.0 Watt
Energy ranges
Electrons50 keV - 1 MeV
Protons250 keV - 30 MeV
Alpha particles1 - 100 MeV
Analyzer levels
4 detectors8 energy levels, logarithmically spaced
2 detectors4 energy levels, log. spaced
Temporal resolution
Very high speed5 samples/sec (selected locations)
High speed1 sample/sec (auroral latitudes)
Moderate speed0.5 sample/sec (polar cap)
Low speed0.1 sample/sec (*)
(*) Low speed sampling is not used. Moderate speed is default.

Table 1. Summary technical specifications for CPD experiment.

The CPD housing and the detector designations and view directions with respect to satellite axes (z1 is along the boom) are shown in the figure below

Figure 1. Schematic CPD box lay-out and detector view directions.

The CPD instrument uses two types of solid-state Silicon detectors. Their characteristics are shown in Table 2.

Detector modelEG&G Ortec ULTRA
TU-011-050-300
EG&G Ortec type B
TB-016-050-1000
Detector typeIon-implantedTotally depleted
Sensitive area50 mm250 mm2
Depletion depth300 um1000 um
Noise width3.2 keV (FWHM)9 keV (FWHM)
Alpha resolution11 keV (FWHM)16 keV (FWHM)
Operating bias100 volts200 volts

Table 2. Basic detector characteristics.

The energy thresholds for the detectors are determined by the entrance windows. The P1, P2 and E1, E2 detector units are shielded by 1.25 micron Nickel foils (in addition to the detectors own gold window). The P3 detector has a 1 mm thick Aluminium shield at its entrance window and the P4 detector a 1 mm Copper shield. The amplified pulses from detected particles penetrating into the depletion layer are fed to pulse height analyzer units with 8, resp. 4 threshold levels. The pulses for each detector unit and each energy level are counted. These counts are sampled by the instrument computer at the rates given in Table 1 and then temporally stored. Controlled by interrupt signals from the CDH main computer the data (and status information) are transferred to the CDH-controlled satellite data memory.
The properties of the detector units and their detection ranges are shown in Table 3.

PropertyP1 and P2P3P4E1 and E2
Sight angle (degree)90 / 0909090 / 0
F.O.V. half angle (degree)20.533.533.520.5
Aperture (cm2)0.1960.2830.2830.196
Geometric factor (cm2 sr)0.0530.250.250.053
Entrance window (um/compound)1.25/Ni1000/Al1000/Cu1.25/Ni
Detector typeTUTUTUTB
Threshold Energies (MeV)
alphas (>1%).5151.989.9.51
alphas (>50%).5352.090.1.53
alphas (>99%).7152.590.7.71
protons.2312.922.3.23
protons.2413.022.5.24
protons.2913.222.8.29
electrons.02.681.75.02
electrons.02.782.2.02
electrons.072.33>60.07
Peak (penetration) energy (MeV)
alphas24.59.95.48.
protons6.15.24.12.
electrons.371.002.1.88
Mean energy lost in Si at
peak (penetration) energy (MeV)
alphas22.822.822.848.
protons5.65.65.612.
electrons.3.3.3.8
Energy bin limits (keV)
142020921247
263574175272
398021802150111
4149077407610168
52150237
63240358
75015553
87610840

Further details

The photo to the left shows the CPD box seen from below. In the large compartment one may observe the lowermost of 4 PC boards. This board holds the CPD experiment computer system based on an Intel 80186 processor. The other PC boards further up in the box hold the charge-sensitive preamplifiers and pulse amplifiers, the analyzer level detector circuits and the counter and read-out circuits. The uppermost of the smaller compartments to the right houses the two side-looking detector units. In the lower small compartment are housed the low-voltage regulators and the high-voltage converters used to provide the detector bias voltages.

This photo shows one of the six solid-state Si-detector elements. The detector is a reverse biased silicon diode with a depleted junction region only covered by thin gold layer which also provides the electrical contact for the diode.
High-energy particles may penetrate the gold layer and enter the reverse-biased depleted junction layer. Here they produce an ionized trail until they are stopped and come to rest. The electrons and holes drift to either side in the applied electric field to be collected by the electrodes at sides of the junction. The total charge collected is a measure of the energy deposited by the incoming high-energy particle. Until the primary particle penetrates the detector this energy amounts to the total energy of the incident particle less the losses in the gold window and the dead-layer just beneath it. For penetrating particles at still higher energies the energy deposited in the detector decrease. The detection process is sketched in the figure to the left.


For further information or questions regarding the CPD experiment please forward e-mail to:

pst@dmi.dk Peter Stauning (PI for the CPD particle experiment)
or
pd@terma.com Peter Davidsen (CoI for the CPD experiment)
or
cyam@fynu.ucl.ac.be Mathias Cyamukungu (CoI for the CPD experiment)


DMI Updated 21. September 2000. PSt