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...
Main Author: | |
---|---|
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 |
id |
doaj-6843aa97079b4ca0ba32e8ab895c714d |
---|---|
record_format |
Article |
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 |
work_keys_str_mv |
AT jhelmboldt amultiplatforminvestigationofmidlatitudesporadicieianditstiestoieiificouplingandmeteoractivity AT jhelmboldt multiplatforminvestigationofmidlatitudesporadicieianditstiestoieiificouplingandmeteoractivity |
_version_ |
1725741718000631808 |