Successful Test of a Geiger-Müller Counter in Vacuum

For a Weatherballoon mission lead by the Ricarda-Huch-Schule we prepared and tested a Geiger-Müller Counter module. The challenge is to operate the high voltage supply of the tube in the partial vacuum of the stratosphere. We may encounter a Corona discharge, which may destroy the electronics or at least impact the measurements. We are all happy to leave Corona behind us. The second issue is the internal pressure of the tube. We passed all tests. Down to 1mbar pressure the unit worked flawlessly.

First, the tube was tested individually. It survived low pressure. The HV was calibrated to 400V as prescribed in the manual. Then we removed the calibration connecter and a power connector that were too close to the HV electrode of the tube. The board was coated twice with a space grade 2-component silicone encapsulant, in particular the HV supply and the area close to the HV end of the tube. We obtained an insulation distance of about 4cm.

The Paschen Curve tells us that we should be good down to a few mbar.

First, we tested in a glas chamber, to visually observe the test. But that pump could not go below 60mbar. Then we used our regular thermal vacuum test stand for balloon missions, shown above. The test was performed at room temperature. We used only the rough vacuum pump, which took the chamber pressure down to 1mbar. The output of the module was monitored with an oscilloscope. A ²⁰⁷Bi souce was place inside the chamber to increase the counting activity. It worked well. Unfortunately, we did not take any pictures.

Vio did the coating, see the log sheet above. Ronja soldered the feedthrough harness and performed the Vaccum tests. Sönke observed radiation safety. Matti provided the counter module.

Now we are waiting for the flight forecasts to predict a landing site on land.

Gluing large BGOs

Last week the big BGOs have arrived. One alone weighs over 1kg. Currently, two BGOs are covered with photodiodes. One with two on opposite sides and one with three each at an angle of 120 degrees. Subsequently, the dependence of the light output (sum of the diode signals) on the number and arrangement of the diodes is to be determined experimentally.

Completion of the sensor head for CHAOSjunior

After performing a calibration measurement for the two HET-B detectors, the BGO was now also integrated into the sensor head and the two glued-on diodes were connected to the two free slots on the preamplifier board. The gain was changed to 3 in advance. Additionally two temperature sensors were connected. One measures the temperature directly at the BGO mount, the other is intended to look out of the box during flight and measure the environmental temperature.

Trigger thresholds for each channel were set to 5mV. In coincidence, the two BGO diodes trigger from even 3mV.
First measurements are running and results will follow shortly right here.

Submission of Letter of Intent to BEXUS

Today we have submitted our letter of intent to the BEXUS program marking our first steps to a possible participation in the next BEXUS-cycle

Our instrument CHAOS (Cherenkov Atmospheric Observation System) represents a scaled-down version of the ATHENA High Energy Particle Monitor (AHEPaM), which is designed to measure the background radiation of the ATHENA mission.

Preampfilters for CHAOSjunior

The preamplifier boards for CHAOSJunior were soldered according to slightly modified scematics of the High Energy Telescop (HET) experiment. For the detector setup of the balloon flight in September 2023, only four preamplifers are necessary and only those four were assembled for now. Since the HET preamp board has room for twelve preamps in total, more can be added at a later time for the detector setup of CHAOS. The assembled preamplifier board was tested for any short circuits and function of the operating points. The boards are working as desired and can now be tested further with attached detectors.

Solid State Detectors for Chaos-Jr

Today Myrdin and Stephan started to put together the sensor head of Chaos-Jr. Two spare Solo-EPD-HET-B detectors were put into a spare HET housing. The wires were soldered to the preamplifier board that was assembled by Sophie. The sensor is now connected to a RPiRENA on a Raspberry Pi1 and is taking data. Next we will put a ²⁰⁷Bi Source next to the sensor to perform a calibration with gamma and X-rays.

Observe how two preamplifiers are still unconnected. That is where the photodiodes from the BGO scintillator will be connected.

First Steps for CHAOSJunior Balloon Experiment

From September 25 to 30, 2023, the science festival “Highlights der Physik” will come to Kiel. As part of this event, we plan to fly a weather balloon with a CHAOSJunior experiment. This consists of a small hexagonal bismuth germanium oxide scintillator (BGO) with two photodiodes glued on opposite sides and two segmented solid state detectors (SSDs), which were adopted from the High Energy Telescop (HET) experiment. These HET-B detectors are placed in front of and behind the BGO and are used for coincidence measurements. In the past weeks, two photodiodes were glued to the BGO on opposite sides. The so prepared BGO was wrapped today in such a way that the light generated in the BGO is reflected on all inner sides and reaches the diodes. This BGO with diodes will be first tested in an already existing test can the following days. In the meantime, a pre-amplifier board for the flight is soldered and connected to the BGO diodes and the HET-B detectors. Then this setup will be tested.

BGO wrapped in teflon tape and put into old casing from HET
BGO with case and other BGO in testbox

Revival of an old Detector

The proposed CHAOS instrument needs a fairly large area Solid State Detector (SSD). All Detectors that we can use are spare parts from earlier space missions. For this large area SSD we put our eyes on a couple of recently rediscovered Soho Costep EPHIN F-Detectors, manufactured in the 1980ies.

A quick test revealed that all but one of them have excessive bias currents. The one good detector, unit F2, was subject of a C-V measurement, Capacitance versus bias Voltage. That kind of measurement tells about the impurity concentrations (dopands) and thickness of the detector.

The results confirm that the detector is about 700µm thick, and needs about 150V bias to be fully depleted, which is in range with the expectations. The diameter of the SSD is about 8cm.

This EPHIN F2 detector may become the anticoincidence counter of CHAOS. Currently it is tested in operation with cosmic muons and a gamma ray source.

Chaos Server

Welcome to the internet presence of the Chaos project. For the next two years you will find updates of the project in this place. The server is a virtual maschine provided by netcup.de.

First Team Meeting

2023-04-14_first-meeting

We don’t have a name for our new team yet, but we have a lot of motivated students and ideas for the next BEXUS project proposal from Kiel University.

With our project we want to do preliminary development work for the ATHENA High Energy Particle Monitor (AHEPaM), which will measure the non-photonic background radiation for the space X-ray telescope ATHENA.

In addition, we want to launch a light junior version beforehand using our own weather balloon as part of the Science Festival “Highlights of Physics” in Kiel.