2019
DOI: 10.1029/2019ja026635
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Geographical and Seasonal Variability of Mesospheric Bores Observed from the International Space Station

Abstract: Geographical and seasonal variations of mesospheric bores were derived from mesospheric airglow observations by the Visible and near Infrared Spectral Imager (VISI) of Ionosphere, Mesosphere, upper Atmosphere and Plasmasphere (IMAP) mission onboard the International Space Station. In the three‐year data set spanning September 2012 to August 2015, 306 mesospheric bore events were found between 55ºS and 55ºN in the O2(0‐0) airglow whose peak height is around 95 km. The distribution of the bore events showed a hi… Show more

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Cited by 18 publications
(17 citation statements)
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“…The monochromatic wavelength of 45 km is consistent with mesospheric bores. Further, the mesospheric bore occurrence rate is largest around equinoxes (Su et al, 2018) and during evening hours (Hozumi et al, 2019).…”
Section: Agu Advancesmentioning
confidence: 97%
“…The monochromatic wavelength of 45 km is consistent with mesospheric bores. Further, the mesospheric bore occurrence rate is largest around equinoxes (Su et al, 2018) and during evening hours (Hozumi et al, 2019).…”
Section: Agu Advancesmentioning
confidence: 97%
“…The monochromatic wavelength of 45 km is consistent with mesospheric bores. Further, the mesospheric bore occurrence rate is largest around equinoxes (Su et al, ) and during evening hours (Hozumi et al, ).…”
Section: Interpretation and Conclusionmentioning
confidence: 99%
“…The VISI OH* channel was contaminated with background city lights and reflected moonlight from clouds, similar to DNB. Since these signals are largely absorbed by O 2 in the lower atmosphere, only the O 2 emission at~95 km has been used to study global AGWs including mesospheric bores so far [53][54][55][56][57]. VISI data have a horizontal resolution of 14-16 km and a 600 km swath width for the O 2 emission.…”
Section: Instrumentationmentioning
confidence: 99%