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Can molecular diffusion explain Space Shuttle plume spreading?
Author(s) -
Meier R. R.,
Plane John M. C.,
Stevens Michael H.,
Paxton L. J.,
Christensen A. B.,
Crowley G.
Publication year - 2010
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/2010gl042868
Subject(s) - thermosphere , plume , advection , diffusion , space shuttle , turbulence , turbulent diffusion , meteorology , satellite , environmental science , atmospheric sciences , exosphere , physics , mechanics , computational physics , geophysics , astronomy , ionosphere , thermodynamics , ion , quantum mechanics
The satellite‐borne Global Ultraviolet Imager (GUVI) has produced more than 20 images of NASA Space Shuttle main engine plumes in the lower thermosphere. These reveal atomic hydrogen and, by inference, water vapor transport over hemispherical‐scale distances with speeds much faster than expected from models of thermospheric wind motions. Furthermore, the hydrogen plumes expand rapidly. We find rates that exceed the horizontal diffusion speed at nominal plume altitudes of 104‐112 km. Kelley et al. (2009) have proposed a 2‐D turbulence mechanism to explain the observed spreading rates (and rapid advection) of the plumes. But upon further investigation, we conclude that H atom diffusion can indeed account for the observed expansion rates by recognizing that vertical diffusion quickly conveys atoms to higher altitudes where horizontal diffusion is much more rapid. We also find evidence for H atom production directly during the Shuttle's main engine burn.