Purpose of the flight and payload description
In this flight were transported two instruments: a large area phoswich array provided by the Imperial College Group and a large area proportional counter developed by the University of Tasmania. The goal of the flight was to investigate hard cosmic X-ray sources from the southern hemisphere.
The large area phoswich array consisted of 12 identical modules totalling 1600 cm2. Each module had a primary 2 mm thick NaI crystal backed by a 14 mm thick CsI crystal, and a 2° FWHM field of view produced by a tantalum honeycomb collimator; passive shielding was used to block background radiation through the sides. Photons were detected in 31 energy channels over the range 16-200 keV.
The other instrument was a multilayer, multianode proportional counter with an area of 5200 cm2 and 21 cm active depth, filled with Xenon at 1 atmosphere. Its 10-100 keV range was spanned by 20 energy channels. A thin alloy honeycomb collimator defined the 2° FWHM field of view, while the rear and sides were screened by a graded shield. Background due to charged particles was also removed by active screening.
Details of the balloon flight
Balloon launched on: 11/25/1980 at
Launch site: Australian Balloon Launching Station, Alice Springs, Australia
Balloon launched by: National Scientific Balloon Facility (NSBF)
Balloon manufacturer/size/composition: Zero Pressure Balloon
Flight identification number:
End of flight (L for landing time, W for last contact, otherwise termination time): 11/25/1980 at ??
Balloon flight duration (d:days / h:hours / m:minutes): 1 h
Landing site: Balloon brst at 60.000 ft
- X-ray and optical studies of binary x-ray pulsars PhD thesis by D.J. Watts, University of Tasmania, 1984
After running StratoCat in an "advertising free" basis for 16 years, I've joined "Ko-Fi" to get funding for the research I do. If you find this website interesting or useful, you can help me to keep it up and running.