Purpose of the flight and payload description
The BUSS experiment was designed to perform spectrophotometric measurements of the stars in the UV domain. The telescope was mounted on a biaxial pointer, and was controlled in elevation and azimuth by a boresighted startracker. Both the telescope-spectrometer and the pointer were designed and built . The telescope has a focal length of 300 cm and a diameter of 40 cm. It consisted of an f/3 primary mirror and a secondary mirror with magnification m = 2.5. By means of image motion compensation an ultimate tracking precision of a few seconds of arc is achieved. The secondary mirror is mounted in a biaxial flex-pivot gimbal system, and can be tilted by means of two small torque motors.
Near the focal plane a dichroic mirror reflects the ultraviolet radiation towards the spectrometer, and transmits the visible light towards a star position sensor, which provides the control signals for the torque motors.
The original payload was designed and built by Ball Brothers Research Corporation of Boulder, Colorado, in 1971. The payload is about 3.5 m in diameter by 2.5 m high and weighs 540 kg, excluding ballast. Crush pads are attached to the four legs of the lower section or gondola, and the roll cage supplies additional protection to the telescope.
Details of the balloon flight
Balloon launched on: 10/9/1974
Launch site: Columbia Scientific Balloon Facility, Palestine, Texas, US
Balloon launched by: National Scientific Balloon Facility (NSBF)
Balloon manufacturer/size/composition: Zero Pressure Balloon Winzen 437.341 m3 (12.70 microns - Stratofilm)
Flight identification number: 855P
Balloon flight duration (F: time at float only, otherwise total flight time in d:days / h:hours or m:minutes - ): F 6 h 15 m
Payload weight: 796 kgs.
- Chromospheric models for ALTAIR (A7 IV-V) The Astrophysical Journal, Part 1, vol. 439, no. 2, p. 1011
- Mass loss observed in the ultraviolet spectrum of the A2 supergiant, alpha Cygni Astrophysical Journal, vol. 198, May 15, 1975, pt. 2, p. L37-L39
- National Scientific Balloon Facility Annual Report FY 1975 National Center for Atmospheric Research, November 1975
- The MG II doublet emissions near 2800 A observed in alpha Tauri, alpha Orionis, and epsilon Pegasi Astrophysical Journal, vol. 196, Mar. 15, 1975, pt. 2, p. L125-L128
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