Investigations of the cascade of Langmuir wave turbulence over HAARP Observatory in Gakona, Alaska
Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2007. === Includes bibliographical references (leaf 49). === This thesis investigates the cascade lines from Langmuir wave turbulence as a result of Parametric Decay Instability (PDI) in the ionosphere. This effect is studied us...
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ndltd-MIT-oai-dspace.mit.edu-1721.1-409072019-05-02T16:30:43Z Investigations of the cascade of Langmuir wave turbulence over HAARP Observatory in Gakona, Alaska Burton, Laura M Min-Chang Lee and Richard Temkin. Massachusetts Institute of Technology. Dept. of Physics. Massachusetts Institute of Technology. Dept. of Physics. Physics. Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2007. Includes bibliographical references (leaf 49). This thesis investigates the cascade lines from Langmuir wave turbulence as a result of Parametric Decay Instability (PDI) in the ionosphere. This effect is studied using a high-frequency (HF) heater located at the NSF/DoD High Frequency Active Auroral Research Program (HAARP) Observatory in Gakona, Alaska. Measurements were taken remotely in February 2005 and March 2006 in order to focus study on the altitude variation and number of cascade lines. This data was cross-checked with a recently developed theory by Kuo and Lee [2005] citing two processes possible in PDI: resonant decay and non-resonant decay. The non-resonant cascade of Langmuir waves proceeds at the same location and is severely hampered by frequency mismatch effect, because the decay wave is a driven ion mode oscillating at considerably lower frequency than that of the ion acoustic wave. In contrast, the resonant cascade, which takes place at different resonant locations to minimize the frequency mismatch effect, has to overcome the propagation loss of the mother Langmuir wave in each cascade step. It is known, in general, that the resonant cascade process requires less thresholds than those of the non-resonant cascade process. Thorough analysis concludes that resonant decay is the most probably process due to observed altitude variation and number of cascade lines observed. by Laura M. Burton. S.B. 2008-03-27T18:22:02Z 2008-03-27T18:22:02Z 2007 2007 Thesis http://hdl.handle.net/1721.1/40907 212374799 eng M.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission. http://dspace.mit.edu/handle/1721.1/7582 49 leaves application/pdf n-us-ak Massachusetts Institute of Technology |
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Physics. Burton, Laura M Investigations of the cascade of Langmuir wave turbulence over HAARP Observatory in Gakona, Alaska |
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Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2007. === Includes bibliographical references (leaf 49). === This thesis investigates the cascade lines from Langmuir wave turbulence as a result of Parametric Decay Instability (PDI) in the ionosphere. This effect is studied using a high-frequency (HF) heater located at the NSF/DoD High Frequency Active Auroral Research Program (HAARP) Observatory in Gakona, Alaska. Measurements were taken remotely in February 2005 and March 2006 in order to focus study on the altitude variation and number of cascade lines. This data was cross-checked with a recently developed theory by Kuo and Lee [2005] citing two processes possible in PDI: resonant decay and non-resonant decay. The non-resonant cascade of Langmuir waves proceeds at the same location and is severely hampered by frequency mismatch effect, because the decay wave is a driven ion mode oscillating at considerably lower frequency than that of the ion acoustic wave. In contrast, the resonant cascade, which takes place at different resonant locations to minimize the frequency mismatch effect, has to overcome the propagation loss of the mother Langmuir wave in each cascade step. It is known, in general, that the resonant cascade process requires less thresholds than those of the non-resonant cascade process. Thorough analysis concludes that resonant decay is the most probably process due to observed altitude variation and number of cascade lines observed. === by Laura M. Burton. === S.B. |
author2 |
Min-Chang Lee and Richard Temkin. |
author_facet |
Min-Chang Lee and Richard Temkin. Burton, Laura M |
author |
Burton, Laura M |
author_sort |
Burton, Laura M |
title |
Investigations of the cascade of Langmuir wave turbulence over HAARP Observatory in Gakona, Alaska |
title_short |
Investigations of the cascade of Langmuir wave turbulence over HAARP Observatory in Gakona, Alaska |
title_full |
Investigations of the cascade of Langmuir wave turbulence over HAARP Observatory in Gakona, Alaska |
title_fullStr |
Investigations of the cascade of Langmuir wave turbulence over HAARP Observatory in Gakona, Alaska |
title_full_unstemmed |
Investigations of the cascade of Langmuir wave turbulence over HAARP Observatory in Gakona, Alaska |
title_sort |
investigations of the cascade of langmuir wave turbulence over haarp observatory in gakona, alaska |
publisher |
Massachusetts Institute of Technology |
publishDate |
2008 |
url |
http://hdl.handle.net/1721.1/40907 |
work_keys_str_mv |
AT burtonlauram investigationsofthecascadeoflangmuirwaveturbulenceoverhaarpobservatoryingakonaalaska |
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1719041877841281024 |