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Han, Shin-Chan, Kil, Hyosub, Ray, Richard, Lemoine, Frank, and Waters, Colin, 2024. Detection of Extensive Equatorial Plasma Depletions After the 2022 Tongan Volcanic Eruption From Multiple Geodetic Satellite Ranging Systems. Journal of Geophysical Research (Space Physics), 129(11):2024JA032690, doi:10.1029/2024JA032690.
• from the NASA Astrophysics Data System • by the DOI System •
@ARTICLE{2024JGRA..12932690H,
author = {{Han}, Shin-Chan and {Kil}, Hyosub and {Ray}, Richard and {Lemoine}, Frank and {Waters}, Colin},
title = "{Detection of Extensive Equatorial Plasma Depletions After the 2022 Tongan Volcanic Eruption From Multiple Geodetic Satellite Ranging Systems}",
journal = {Journal of Geophysical Research (Space Physics)},
keywords = {electron density, geodetic satellites, total electron content, Tonga volcano},
year = 2024,
month = nov,
volume = {129},
number = {11},
pages = {2024JA032690},
abstract = "{We present a number of unique observations of ionospheric anomalies
following the Hunga-Tonga Hunga-Ha'apai (HTHH) volcanic eruption
on 15 January 2022. All are based on non-dedicated geodetic
satellite systems: Global Positioning System tracking of Low
Earth Orbit (LEO) CubeSats, intersatellite tracking between two
GRACE Follow-On satellites, satellite radar altimeters to the
ocean surface, and Doppler radio beacons from ground stations to
LEO geodetic satellites. Their observations revealed the
development of anomalously large trough-like plasma depletions,
along with plasma bubbles, in the equatorial regions of the
Pacific and East Asian sectors. Trough-like plasma depletions
appeared to be confined within approximately
{\ensuremath{\pm}}20{\textdegree} magnetic latitude, accompanied
by density enhancements just outside this latitude range. These
plasma depletions and enhancements were aligned with the
magnetic equator and occurred across broad longitudes. They were
detected in regions where atmospheric waves from the HTHH
eruption passed through around the time of the sunset
terminator. We interpret these phenomena in terms of the E
dynamo electric fields driven by atmospheric waves from the
eruption. The uplift of the ionosphere beyond satellite
altitudes, followed by subsequent plasma diffusion to higher
latitudes along magnetic field lines, results in the formation
of trough-like plasma depletions around the magnetic equator and
density enhancement at higher latitudes. The detection of plasma
bubbles in the Asian sector during the non-bubble season
(January) is likely associated with the uplift of the ionosphere
at the sunset terminator.}",
doi = {10.1029/2024JA032690},
adsurl = {https://ui.adsabs.harvard.edu/abs/2024JGRA..12932690H},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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