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STS-3 Snowflake studyVideotape recordings were made of particles observed being released from the orbiter and image processing techniques were used to reduce the data in order to obtain sources and sizes. Results show that a significant number of 1 mm to 1 cm diameter particles were in the vicinity of STS-3. Their origin may be near the aft end of the orbiter; however, 19 of the 33 examined trajectories show that the origin was definitely forward of the aft end of the bay. There may be larger particles near the aft end of the orbiter. Most particles move generally rearward with respect to the orbiter (+X direction).
Document ID
19830014041
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Barengoltz, J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Maag, C.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Kuykendall, F.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 11, 2013
Publication Date
February 1, 1983
Publication Information
Publication: Systematics General Corp. The Shuttle Environ. Workshop
Subject Category
Astronautics (General)
Accession Number
83N22312
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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