@Article{LeeKiKwPaZhGaBa:2014:EqBrPl,
author = "Lee, Woo Kyoung and Kil, Hyosub and Kwak, Young-Sil and Paxton,
Larry J. and Zhang, Yongliang and Galkin, Ivan and Batista, Inez
Staciarini",
affiliation = "Johns Hopkins University Applied Physics Laboratory, 11100 Johns
Hopkins Road, Laurel, MD 20723, United States; Korea Astronomy and
Space Science Institute, Daejeon, South Korea and Johns Hopkins
University Applied Physics Laboratory, 11100 Johns Hopkins Road,
Laurel, MD 20723, United States and Korea Astronomy and Space
Science Institute, Daejeon, South Korea and Johns Hopkins
University Applied Physics Laboratory, 11100 Johns Hopkins Road,
Laurel, MD 20723, United States and Johns Hopkins University
Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD
20723, United States and University of Massachusetts Lowell,
Lowell, MA, United States and {Instituto Nacional de Pesquisas
Espaciais (INPE)}",
title = "Equatorial broad plasma depletions associated with the enhanced
fountain effect",
journal = "Journal of Geophysical Research: Space Physics",
year = "2014",
volume = "119",
number = "1",
pages = "402--410",
keywords = "broad plasma depletions.",
abstract = "Broad plasma depletions (BPDs), plasma depletions whose
longitudinal width is over several hundred kilometers, have been
detected in the equatorial F region by low-earth-orbit satellites
during both magnetically quiet and magnetically disturbed periods.
A few hypotheses were suggested to explain the creation of BPDs,
but the underlying mechanism of this phenomenon is still under
debate. We investigate the origin of BPDs by analyzing the
simultaneous in situ and optical observations of the ionosphere on
30 May 2003 (Kp = 8+), 24 April 2012 (Kp = 7-), and 31 October
2012 (Kp = 0+). BPDs on 30 May 2003 were detected by the Republic
of China Satellite-1 at an altitude of 600 km, and BPDs on the
other days were detected by the Communication/Navigation Outage
Forecasting System satellite near an altitude of 400 km. Our
results show that the detection of BPDs is closely associated with
background ionospheric morphology; BPDs are detected on the days
when the equatorial ionization anomaly (EIA) is intense and the
crests of the EIA have moved poleward. Measurements of upward
plasma motion support the existence of ionospheric uplift at BPD
locations. These observations and the detection of BPDs near the
magnetic equator lead to the interpretation that the satellite
detection of BPDs during those 3 days is likely related to the
uplift of the F peak height above the satellite orbits. Key Points
Broad plasma depletions (BPDs) appear when the EIA is
strengthened. BPDs are associated with the uplift of the F region.
Bubbles are not a pre-requisite for BPDs. ©2013. American
Geophysical Union. All Rights Reserved.",
doi = "10.1002/2013JA019137",
url = "http://dx.doi.org/10.1002/2013JA019137",
issn = "2169-9402",
label = "scopus 2014-05 LeeKiKwPaZhGaBa:2014:EqBrPl",
language = "en",
targetfile = "bpd.pdf",
urlaccessdate = "27 abr. 2024"
}