1991
DOI: 10.1029/91jd01713
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Space shuttle exhausted aluminum oxide: A measured particle size distribution

Abstract: Aluminum oxide (A2O3) particles were collected from the space shuttle exhaust plume immediately following the launch of STS‐34 on October 18, 1989. A2O3 samples were obtained at 2.4, 3.0, 3.2, and 7.4 km in altitude. The samples were analyzed using scanning electron microscopy to develop particle size distributions. There were no indications that the particle size distribution changed as a function of altitude. The particle number concentrations per cubic meter of air sampled (Nc) for the four collections was … Show more

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Cited by 17 publications
(10 citation statements)
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“…Scenario "F", which assumes all of the alumina particles are in the small size distribution, is an upper limit computation within the assumptions going into our trimodal size distribution. There is no reason to believe that all the particles are in the smallest size distribution, since the alumina particles do coalesce and there are very good measurements of large particles in SRM exhaust plumes [Cofer et al 1987[Cofer et al , 1991.…”
Section: Introductionmentioning
confidence: 99%
“…Scenario "F", which assumes all of the alumina particles are in the small size distribution, is an upper limit computation within the assumptions going into our trimodal size distribution. There is no reason to believe that all the particles are in the smallest size distribution, since the alumina particles do coalesce and there are very good measurements of large particles in SRM exhaust plumes [Cofer et al 1987[Cofer et al , 1991.…”
Section: Introductionmentioning
confidence: 99%
“…Although the value determined here, 37 ± 11%, initially appears to support Beiting, we note the following caveats. Beiting and BM derived size distributions by combining measurements of different limited portions of the size distribution, obtained in the plumes of different rockets, encountered under different atmospheric conditions [ Strand et al , 1981; Zolensky et al , 1989; Cofer et al , 1991]. Hence skepticism must be acknowledged regarding the degree to which the Beiting and BM distributions are representative of any particular SRM under stratospheric conditions.…”
Section: Discussionmentioning
confidence: 99%
“…However, literature on particles emitted by rockets is sparse (e.g., Zolensky et al, 1989), and there areto the best of our knowledge -no studies available on carbonaceous particles by electron microscopy. According to Ross and Sheaffer (2014) (Strand et al, 1981;Zolensky et al, 1989;Cofer III et al, 1991) and can, thus, be excluded as the source of the carbonaceous particles encountered in the present study. Hydrocarbon-fired rockets are powered by kerosene or syntin and can be expected to emit soot.…”
Section: Rocket Exhaustmentioning
confidence: 99%