Behavior of the atomic oxygen 5577 Ångström emission intensity at mid-latitudes: a climatological view

dc.contributor.authorDeutsch, Kerry Annen_US
dc.date.accessioned2009-10-06T16:41:58Z
dc.date.available2009-10-06T16:41:58Z
dc.date.issued2000en_US
dc.descriptionThesis (Ph. D.)--University of Washington, 2000en_US
dc.description.abstractA global mid-latitude study of the atomic oxygen green line emission intensity at 5577 A has been undertaken with the goal of developing a climatological understanding of the emission behavior and its usefulness as a tracer for the atmosphere near 97 km. Long-term observations have been analysed at nine stations covering periods of ∼8--12 years, for a total of over 90 years of measurements. The results of this investigation show that the emission typically exhibits a maximum near the summer solstice and again near the fall equinox, before falling to a low winter-time level that persists into the middle of spring. Importantly, the oft-reported maximum at the spring equinox is not a statistically significant feature on the climatological time scale. This finding has implications on our understanding of the dominant processes operating in the region. Specifically, the role of seasonally varying vertical diffusion caused by breaking gravity waves must be readdressed in light of the absence of a strong maximum at the spring equinox.This work also addresses the relationship between the green line emission intensity and geomagnetic and solar activity. Results show that failing to exclude observations taken under high geomagnetic activity conditions leads to increased springtime emission levels and may be one explanation for this feature as has been reported by others. The influence of solar activity on the green line emission over the long term is shown to exhibit a hysteresis effect within a given solar cycle, confirming that there is not a simple linear relationship between the two processes.Finally, a critical examination is made of how long of a data series is necessary to fully achieve a climatological understanding of this emission and how this understanding may reasonably be used to advance our understanding of the upper middle atmosphere region. After ∼10 years, features with periods less than one year become stable (or achieve climatology), but the data examined here show unresolved power at periods approaching the series length which need longer data coverage to fully characterize.en_US
dc.format.extentvii, 98 p.en_US
dc.identifier.otherb45450729en_US
dc.identifier.other46966258en_US
dc.identifier.otherThesis 49870en_US
dc.identifier.urihttp://hdl.handle.net/1773/6803
dc.language.isoen_USen_US
dc.rightsCopyright is held by the individual authors.en_US
dc.rights.urien_US
dc.subject.otherTheses--Geophysicsen_US
dc.titleBehavior of the atomic oxygen 5577 Ångström emission intensity at mid-latitudes: a climatological viewen_US
dc.typeThesisen_US

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