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        <identifier>oai:www.ideals.illinois.edu:2142/26160</identifier>
        <datestamp>2023-07-10</datestamp>
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        <thesis xmlns="http://www.ndltd.org/standards/metadata/etdms/1.1/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:dc="http://purl.org/dc/elements/1.1/" xsi:schemaLocation="http://www.ndltd.org/standards/metadata/etdms/1.1/ http://www.ndltd.org/standards/metadata/etdms/1.1/etdms11.xsd http://purl.org/dc/elements/1.1/ http://www.ndltd.org/standards/metadata/etdms/1.1/etdmsdc.xsd">
          <dc:contributor>Liu, Alan Z.</dc:contributor>
          <dc:contributor>Liu, Alan Z.</dc:contributor>
          <dc:contributor>Swenson, Gary R.</dc:contributor>
          <dc:contributor>Rauber, Robert M.</dc:contributor>
          <dc:contributor>Mak, Mankin</dc:contributor>
          <dc:creator>Li, Zhenhua</dc:creator>
          <dc:date>2011-08-25T22:16:44Z</dc:date>
          <dc:date>2011-08-25T22:16:44Z</dc:date>
          <dc:date>2011-08-25T22:16:44Z</dc:date>
          <dc:date>2011-08</dc:date>
          <dc:description>In this thesis, investigations on gravity waves are conducted in two
regions of the middle atmosphere: the lower stratosphere using
high-resolution radiosonde at South Pole and the mesopause region
using OH airglow imager at Maui, Hawaii and Cerro Pachon, Chile. Wave
characteristics at these regions are deduced and the seasonal
variation of wave activity, wave sources, and propagation effect are
studied.
 
The study of gravity waves in the lower stratosphere at South Pole
reveals that sources other than topography are important even for the
lower part of middle atmosphere. Horizontal propagation must be
included in parameterization schemes to reflect the fact that waves
derived from radiosondes have slant propagation paths. They travel
long distance horizontally before they reach higher altitudes.
Long term gravity wave characteristics over Maui from 2002 to 2007 are
deduced from OH airglow imager. Wave parameters from the long term
imager observation provide robust statistics of high-frequency gravity
wave in the midlatitudes. Poleward wave propagation preference during
summer and equatorward wave propagation preference during winter are
observed over Maui. They are also opposite to the seasonal mean
meridional wind direction which are always pointing toward winter
pole. Momentum fluxes deduced from OH imager are also highly
anti-correlated with background winds. At least for the part of
spectrum observed by airglow imager, gravity waves act as damping
mechanism for diurnal tide. Gravity wave occurrence frequency does not
follow the variation of local convective sources and convective
sources in a large domain when ducted waves are considered. In fact,
with a constant wave source and monthly mean background atmospheric
condition, the simulated wave transmission resembles the wave
occurrence frequency observed by OH airglow imager at Maui. Thus, at
Maui the propagation effect dominates the seasonal variation in wave
activity.
Gravity wave momentum fluxes deduced from airglow imager provide
important observation constraint for gravity wave parameterization for
the mesopause region. To explain the cause of seasonal change on
meridional propagation preference, three mechanisms are investigated:
critical-layer filtering, wave ducting, and Doppler-shifting by local
mean wind. Critical-layer filtering failed to explain the propagation
preference. Observed gravity wave propagation directions are largely
related to the background wind in the airglow layer. This is caused by
Doppler-shifting of gravity waves by background wind. Background wind
Doppler shifts gravity waves propagating against (along) background
wind to higher (lower) frequency and larger (smaller) vertical
wavelength. Thus, the observed gravity waves tend to propagate against
background wind. The apparent against background wind propagation is
largely caused by the contrast in cancellation factor for waves
propagate in different direction. To a lesser degree, the difference
in dissipation for waves propagate in different direction also
contributes to the observed against background wind propagation.
The results from this work show gravity wave's propagation in middle
atmosphere is strongly affected by atmospheric field. For low
frequency waves, their propagation paths are slant and can travel
hundreds of kilometers before they reach the middle atmosphere. For
high frequency gravity waves, though their propagation paths are
mostly vertical, they are subject to ducting and reflection. Due to
the large contribution of momentum flux in the Mesosphere and Lower
Thermosphere (MLT) by high-frequency, short-horizontal-scale waves,
these propagation effects must be included in gravity wave
parameterizations.</dc:description>
          <dc:description>Item withdrawn by Rebecca Bryant (rabryant@illinois.edu) on 2011-07-14T19:55:36Z
Item was in collections:
University of Illinois Theses &amp; Dissertations (ID: 1)
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          <dc:identifier>http://hdl.handle.net/2142/26160</dc:identifier>
          <dc:language>en</dc:language>
          <dc:rights>Copyright 2011 Zhenhua Li</dc:rights>
          <dc:subject>Gravity Wave</dc:subject>
          <dc:subject>Atmospheric Dynamics</dc:subject>
          <dc:subject>Airglow Imager</dc:subject>
          <dc:title>An Observational Investigation on Gravity Wave Characteristics   and Propagation in the Lower   Stratosphere and Mesopause</dc:title>
          <degree>
            <department>Atmospheric Sciences</department>
            <departmentCode>1253</departmentCode>
            <discipline>Atmospheric Sciences</discipline>
            <disciplineCode>0334</disciplineCode>
            <grantor>University of Illinois at Urbana-Champaign</grantor>
            <level>Dissertation</level>
            <name>Ph.D.</name>
            <program>PHD:Atmospheric Sciences -UIUC</program>
            <programCode>10KS0334PHD</programCode>
          </degree>
        </thesis>
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