A multi-platform investigation of midlatitude sporadic <i>E</i> and its ties to <i>E</i>–<i>F</i> coupling and meteor activity

This paper describes the results of a multi-platform observing campaign aimed at studying midlatitude sporadic <i>E</i> (<i>E</i><sub>s</sub>) and associated ionospheric phenomena. The assets used were the digisonde in Boulder, Colorado; the first station of th...

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Main Author: J. Helmboldt
Format: Article
Language:English
Published: Copernicus Publications 2016-05-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/34/529/2016/angeo-34-529-2016.pdf
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spelling doaj-6843aa97079b4ca0ba32e8ab895c714d2020-11-24T22:30:08ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762016-05-013452954110.5194/angeo-34-529-2016A multi-platform investigation of midlatitude sporadic <i>E</i> and its ties to <i>E</i>–<i>F</i> coupling and meteor activityJ. Helmboldt0US Naval Research Laboratory, Code 7213, 4555 Overlook Ave. SW, Washington, DC 20375, USAThis paper describes the results of a multi-platform observing campaign aimed at studying midlatitude sporadic <i>E</i> (<i>E</i><sub>s</sub>) and associated ionospheric phenomena. The assets used were the digisonde in Boulder, Colorado; the first station of the Long Wavelength Array, LWA1, in New Mexico; the transmitters of the radio station WWV in Colorado; and 61 continuously operating GPS receivers between LWA1 and WWV. The results show that southwestward-directed medium-scale traveling ionospheric disturbances (MSTIDs) were substantially more prevalent when <i>E</i><sub>s</sub> was detected. The amplitudes of these correlate with a plasma frequency up to about 4.5 MHz. For <i>f</i><sub>p</sub> ≳ 5 MHz, the MSTIDs become significantly weaker and basically vanish above  ∼ 6.5 MHz. The prevalence of meteor trail reflections observed with LWA1 also correlates with <i>f</i><sub>p</sub> up to about 4.5 MHz; above this limit, the relationship exhibits a significant turnover. The observed intensity of coherent backscatter from <i>E</i><sub>s</sub> field-aligned irregularities (FAIs) also correlates with inferred plasma frequency. However, this trend continues to higher frequencies with a peak near 6 MHz, followed by a much more subtle turnover. The reflected power from <i>E</i><sub>s</sub> structures observed with LWA1 is significantly more correlated on spatial scales between 10 and 40 km. The magnitude of this correlation increases with <i>f</i><sub>p</sub> up to  ∼  6 MHz, above which it drops. These results are consistent with the following: (1) southwestward-directed MSTIDs are produced via <i>E</i>–<i>F</i> coupling; (2) this coupling is stronger when the <i>E</i><sub>s</sub> layer, seeded by meteor ablation, is more dense; (3) the coupling is substantially diminished for <i>E</i><sub>s</sub> layers harboring extremely dense structures (<i>f</i><sub>p</sub> ≳ 5 MHz).https://www.ann-geophys.net/34/529/2016/angeo-34-529-2016.pdf
collection DOAJ
language English
format Article
sources DOAJ
author J. Helmboldt
spellingShingle J. Helmboldt
A multi-platform investigation of midlatitude sporadic <i>E</i> and its ties to <i>E</i>–<i>F</i> coupling and meteor activity
Annales Geophysicae
author_facet J. Helmboldt
author_sort J. Helmboldt
title A multi-platform investigation of midlatitude sporadic <i>E</i> and its ties to <i>E</i>–<i>F</i> coupling and meteor activity
title_short A multi-platform investigation of midlatitude sporadic <i>E</i> and its ties to <i>E</i>–<i>F</i> coupling and meteor activity
title_full A multi-platform investigation of midlatitude sporadic <i>E</i> and its ties to <i>E</i>–<i>F</i> coupling and meteor activity
title_fullStr A multi-platform investigation of midlatitude sporadic <i>E</i> and its ties to <i>E</i>–<i>F</i> coupling and meteor activity
title_full_unstemmed A multi-platform investigation of midlatitude sporadic <i>E</i> and its ties to <i>E</i>–<i>F</i> coupling and meteor activity
title_sort multi-platform investigation of midlatitude sporadic <i>e</i> and its ties to <i>e</i>–<i>f</i> coupling and meteor activity
publisher Copernicus Publications
series Annales Geophysicae
issn 0992-7689
1432-0576
publishDate 2016-05-01
description This paper describes the results of a multi-platform observing campaign aimed at studying midlatitude sporadic <i>E</i> (<i>E</i><sub>s</sub>) and associated ionospheric phenomena. The assets used were the digisonde in Boulder, Colorado; the first station of the Long Wavelength Array, LWA1, in New Mexico; the transmitters of the radio station WWV in Colorado; and 61 continuously operating GPS receivers between LWA1 and WWV. The results show that southwestward-directed medium-scale traveling ionospheric disturbances (MSTIDs) were substantially more prevalent when <i>E</i><sub>s</sub> was detected. The amplitudes of these correlate with a plasma frequency up to about 4.5 MHz. For <i>f</i><sub>p</sub> ≳ 5 MHz, the MSTIDs become significantly weaker and basically vanish above  ∼ 6.5 MHz. The prevalence of meteor trail reflections observed with LWA1 also correlates with <i>f</i><sub>p</sub> up to about 4.5 MHz; above this limit, the relationship exhibits a significant turnover. The observed intensity of coherent backscatter from <i>E</i><sub>s</sub> field-aligned irregularities (FAIs) also correlates with inferred plasma frequency. However, this trend continues to higher frequencies with a peak near 6 MHz, followed by a much more subtle turnover. The reflected power from <i>E</i><sub>s</sub> structures observed with LWA1 is significantly more correlated on spatial scales between 10 and 40 km. The magnitude of this correlation increases with <i>f</i><sub>p</sub> up to  ∼  6 MHz, above which it drops. These results are consistent with the following: (1) southwestward-directed MSTIDs are produced via <i>E</i>–<i>F</i> coupling; (2) this coupling is stronger when the <i>E</i><sub>s</sub> layer, seeded by meteor ablation, is more dense; (3) the coupling is substantially diminished for <i>E</i><sub>s</sub> layers harboring extremely dense structures (<i>f</i><sub>p</sub> ≳ 5 MHz).
url https://www.ann-geophys.net/34/529/2016/angeo-34-529-2016.pdf
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