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ORIGINAL RESEARCH article

Front. Astron. Space Sci.
Sec. Space Physics
Volume 11 - 2024 | doi: 10.3389/fspas.2024.1308198

Low latitude mesosphere and lower thermosphere (MLT) response to the recent stratospheric warming during 2017-18 and 2018-19 Provisionally Accepted

 S SATHISHKUMAR1* S Sridharan2 K Krishnapriya1 P T. Patil1
  • 1Indian Institute of Geomagnetism (IIG), India
  • 2National Atmospheric Research Laboratory, India

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Upper mesospheric wind data acquired by the medium frequency radar at Kolhapur (16.7 o N, 74.2 o E) and MERRA-2 temperature and wind reanalysis datasets are used to investigate the dynamical response of the low-latitude middle atmosphere to the sudden stratospheric warming (SSW) events occurred during the 2017-18 and 2018-19 winters. When the amplitude of high latitude stratospheric planetary wave (PW) of zonal wavenumber 1 reduces considerably with the onset of the SSW, the low-latitude mesospheric PW over Kolhapur also shows considerable reduction in the PW activity. It is noteworthy 2 that the upper mesospheric winds are eastward for about three weeks after the onset of the SSW. The reduced PW activity is associated with the enhanced gravity wave activity in the meridional wind during the SSW 2018-19. The plane of propagation of gravity waves obtained from the perturbation ellipse method suggests that their predominant plane of propagation is in the north-south direction.The persistence of the eastward winds is suggested to be due to the interaction of the northward propagating gravity waves with the mean flow leading to the eastward acceleration due to Coriolis force.

Keywords: Planetary waves, Gravity wave, mesosphere and lower thermosphere, sudden stratospheric warming, wave number, polar vortex

Received: 06 Oct 2023; Accepted: 26 Mar 2024.

Copyright: © 2024 SATHISHKUMAR, Sridharan, Krishnapriya and Patil. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) or licensor are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.

* Correspondence: Prof. S SATHISHKUMAR, Indian Institute of Geomagnetism (IIG), Mumbai, India