@Article{VadasBeFiBoHaGa:2023:MoCoIC,
author = "Vadas, Sharon L. and Becker, Erich and Figueiredo, Cosme Alexandre
Oliveira Barros and Bossert, Katrina and Harding, Brian J. and
Gasque, L. Claire",
affiliation = "{Northwest Research Associates} and {Northwest Research
Associates} and {Instituto Nacional de Pesquisas Espaciais (INPE)}
and {Arizona State University} and {University of California} and
{University of California}",
title = "Primary and secondary gravity waves and large-scale wind changes
generated by the Tonga volcanic eruption on 15 January 2022:
modeling and comparison with ICON-MIGHTI winds",
journal = "Journal of Geophysical Research: Space Physics",
year = "2023",
volume = "128",
number = "2",
pages = "e2022JA031138",
month = "Feb.",
keywords = "gravity waves, ICON-MIGHTI wind, thermosphere, Tonga eruption.",
abstract = "We simulate the primary and secondary atmospheric gravity waves
(GWs) excited by the upward movement of air generated by the Hunga
Tonga-Hunga Ha'apai (hereafter Tonga) volcanic eruption on 15
January 2022. The Model for gravity wavE SOurce, Ray trAcing and
reConstruction (MESORAC) is used to calculate the primary GWs and
the local body forces/heatings generated where they dissipate. We
add these forces/heatings to the HIgh Altitude Mechanistic general
Circulation Model (HIAMCM) to determine the secondary GWs and
large-scale wind changes that result. We find that a wide range of
medium to large-scale secondary GWs with concentric ring structure
are created having horizontal wind amplitudes of u\′,
v\′ \∼ 100200 m/s, ground-based periods of \τr
\∼ 20 min to 7 hr, horizontal phase speeds of cH \∼
100600 m/s, and horizontal wavelengths of \λH \∼
4007,500 km. The fastest secondary GWs with cH \∼ 500600
m/s are large-scale GWs with \λH \∼ 3,0007,500 km and
\τr \∼ 1.57 hr. They reach the antipode over Africa
\∼9 hr after creation. Large-scale temporally and spatially
varying wind changes of \∼80120 m/s are created where the
secondary GWs dissipate. We analyze the Tonga waves measured by
the Michelson Interferometer for Global High-resolution
Thermospheric Imaging (MIGHTI) on the National Aeronautics and
Space Administration Ionospheric Connection Explorer (ICON), and
find that the observed GWs were medium to large-scale with cH
\∼ 100600 m/s and \λH \∼ 8007,500 km, in good
agreement with the simulated secondary GWs. We also find good
agreement between ICON-MIGHTI and HIAMCM for the timing,
amplitudes, locations, and wavelengths of the Tonga waves,
provided we increase the GW amplitudes by \∼2 and sample
them \∼30 min later than ICON.",
doi = "10.1029/2022JA031138",
url = "http://dx.doi.org/10.1029/2022JA031138",
issn = "2169-9402",
language = "en",
targetfile = "JGR Space Physics - 2023 - Vadas - Primary and Secondary Gravity
Waves and Large\‐Scale Wind Changes Generated by the
Tonga.pdf",
urlaccessdate = "12 maio 2024"
}