Purpose of the flight and payload description

A balloon-borne instrument to make measurements of the cosmic microwave background (CMBCMB (Cosmic Microwave Background)The oldest light in the universe, representing the thermal afterglow left over from the Big Bang. As the universe expanded and cooled over 13.8 billion years, this primordial radiation was stretched into the microwave region of the electromagnetic spectrum, filling all of space with a faint, uniform glow) anisotropy on angular scales between 0.5 and 3 degrees. The experiment uses a one meter, off-axis Cassegrian telescope, coupled with a four spectral band radiometerRadiometerAn instrument that measures electromagnetic radiation, typically infrared, visible light, ultraviolet, or a combination of these. It quantifies radiometric properties such as radiant flux (total emitted power), irradiance (power received per unit area), or radiance (power emitted in a given direction per unit area). Radiometers are widely used in fields ranging from astronomy and climate science to industrial sensing and remote sensing satellites.. The pointing for the experiment is controlled by a platform which was originally built in the early 1980's by a group at GSFC to map the Galactic plane (FIRS instrument).
Details of the balloon flight
Balloon launched on: 6/5/1992 at 00:59 utc
Launch site: National Scientific Balloon Facility (NSBF), Palestine, Texas, US
Balloon launched by: National Scientific Balloon Facility (NSBF)
Balloon manufacturer/size/composition: Zero Pressure Balloon SF3-480.10-080-NSCH-04-ST
Balloon serial number: W39.96-3-11
Flight identification number: 1510P
End of flight (L for landing time, W for last contact, otherwise termination time): 6/5/1992 at 12:32 utc
Balloon flight duration (F: time at float only, otherwise total flight time in d:days / h:hours or m:minutes - ): F 6 h 39 m
Landing site: 30 miles N of Brownwood, Texas, US
After a succesfull launch using dynamic method and assisted by launch vehicle (Tiny Tim) at 00:59 utc of June 5, 1992.
The balloon ascent was nominal abd float altitude of 38 km was achieved at 05:07 utc.
After normal flight the balloon was terminated with sunrise at 10:56 utc.
This first flight of the instrument returned outstanding results, and detected anisotropy in several points.
External references
- MSAM website (Archived) NASA Goddard Space Flight Center
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- A Balloon-borne Millimeter-Wave Telescope for Cosmic Microwave Background Anisotropy Measurements Astrophysical Journal v.470, p.63
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- A Measurement of the Cosmic Microwave Background Radiation (CMBR) Anisotropy at the Half Degree Angular Scale Thesis by Inman, Casey Ann (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 1996
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- A measurement of the medium-scale anisotropy in the cosmic microwave background radiation Astrophysical Journal, Part 2 - Letters vol. 422, no. 2, p. L37-L40
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- Measuring cosmic microwave background radiation anisotropy on medium angular scales Thesis by Puchalla, Jason Lee (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 1995
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- Microwave Mappers Sweat Details SCIENCE - 25 Mar 1994 - Vol 263, Issue 5154 - pp. 1682-1684
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- Mysterious Radiation Sources Add to Riddle of Early Universe Goddard News Vol. 40 Nº 8, August 1993, p. 4
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- NASA Balloon Flights (19891998) in NASA Historical Data Book, Vol. VII: NASA Launch Systems, Space Transportation, Human Spaceflight, and Space Science, 1989-1998
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- Preliminary Results from the Goddard-Mit Medium-Scale Anisotropy Experiment Proceedings of an International Symposium; held in Milano; Italy; 21-25 September 1992; p.497
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- The MSAM/TopHat Program of Anisotropy Measurements Astrophysical Letters and Communications, Vol. 32, p.273
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Images of the mission
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