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Infrasound as upper atmospheric monitor (Paperback)
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Discovery Miles 10 910
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Infrasound as upper atmospheric monitor (Paperback)
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Understanding and specification of the higher altitudes of the
atmosphere with global coverage over all local times is hampered by
the challenges of obtaining direct measurements in the upper
atmosphere. Methods to measure the properties of the atmosphere
above the stratopause is an active area of scientific research. In
this thesis, we revisit the use of infrasound as a passive remote
sensing technique for the upper atmosphere. Signals from the
Tungurahua volcano in Ecuador are used to investigate the behavior
of the upper atmosphere. Depending on the atmospheric conditions,
stratospheric, mesospheric and thermospheric arrivals are observed
during intervals of explosive volcanic activity. It is found that
the travel times and dominant frequencies of the thermospheric
arrivals exhibit a coherent variability with periods equal to those
of the tidal harmonics. Theoretical predictions using atmospheric
specifications show that the stratospheric arrivals are predicted
within 1 percent of the observed value. For thermospheric arrivals,
this error can be as high as 10 percent. The error in thermospheric
celerities is found to be in accord with the typical uncertainty in
upper atmospheric winds. Given the observed response of the
infrasound celerities to upper atmospheric tidal variability, it is
suggested that infrasound observations may be used as an additional
source of information to constrain the atmospheric specifications
in the upper atmosphere. We present corrected wind profiles that
have been obtained by minimizing misfits in traveltime and source
location using a Bayesian statistics grid search algorithm.
Additionally, a new numerical method has been developed to solve
the problem of infrasound propagation in a stratified medium with
background flow, based on a modal expansion.
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