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A study of space shuttle plumes in the lower thermosphere

During the space shuttle main engine burn, some 350 t of water vapor are deposited at between 100 and 115 km. Subsequent photodissociation of water produces large plumes of atomic hydrogen that can expand rapidly and extend for thousands of kilometers. From 2002 to 2007, the Global Ultraviolet Image...

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Published in:Journal of Geophysical Research: Space Physics 2011-12, Vol.116 (A12), p.n/a
Main Authors: Meier, R. R., Stevens, Michael H., Plane, John M. C., Emmert, J. T., Crowley, G., Azeem, I., Paxton, L. J., Christensen, A. B.
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container_issue A12
container_start_page
container_title Journal of Geophysical Research: Space Physics
container_volume 116
creator Meier, R. R.
Stevens, Michael H.
Plane, John M. C.
Emmert, J. T.
Crowley, G.
Azeem, I.
Paxton, L. J.
Christensen, A. B.
description During the space shuttle main engine burn, some 350 t of water vapor are deposited at between 100 and 115 km. Subsequent photodissociation of water produces large plumes of atomic hydrogen that can expand rapidly and extend for thousands of kilometers. From 2002 to 2007, the Global Ultraviolet Imager (GUVI) on NASA's Thermosphere Ionosphere, Mesosphere, Energetics and Dynamics (TIMED) satellite imaged many of these hydrogen plumes at Lyman α (121.567 nm) while viewing in the nadir. The images reveal rapid plume expansion and occasional very fast transport to both north and south polar regions. Some plumes persist for up to 6 d. Near‐simultaneous direct detections of water vapor were made with the Sounding of the Atmosphere with Broadband Emission Radiometry (SABER) instrument, also on TIMED. We compare the spreading of the hydrogen plume with a two‐dimensional model that includes photodissociation as well as both vertical and horizontal diffusion. Molecular diffusion appears to be sufficient to account for the horizontal expansion, although wind shears and turbulent mixing may also contribute. We compare the bulk motion of the observed plumes with wind climatologies derived from satellite observations. The plumes can move much faster than predictions of wind climatologies. But dynamical processes not contained in wind climatologies, such as the quasi‐two‐day wave, can account for at least some of the high speed observations. The plume phenomena raise a number of important questions about lower thermospheric and mesospheric processes, ranging from dynamics and chemistry to polar mesospheric cloud formation and climatology. Key Points Huge exhaust plumes from shuttle launches are observed in the lower thermosphere Atomic hydrogen from shuttle plumes diffuses very rapidly Shuttle plumes can move to polar regions much faster than wind models predict
doi_str_mv 10.1029/2011JA016987
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identifier ISSN: 0148-0227
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source Wiley-Blackwell Read & Publish Collection; Wiley-Blackwell AGU Digital Archive
subjects Atmospheric sciences
Auroras
Climatology
diffusion
Hydrogen
Ionosphere
Meteorology
Plumes
PMC
Polar environments
Radiation
shuttle plume
Space shuttles
thermosphere
Water vapor
Wind
Wind shear
winds
title A study of space shuttle plumes in the lower thermosphere
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