Abstract

We apply the Entire Atmosphere GLobal (EAGLE) model to investigate the upper atmosphere response to the January 2009 sudden stratospheric warming (SSW) event. The model successfully reproduces neutral temperature and total electron content (TEC) observations. Using both model and observational data, we identify a cooling in the tropical lower thermosphere caused by the SSW. This cooling affects the zonal electric field close to the equator, leading to an enhanced vertical plasma drift. We demonstrate that along with a SSW-related wind disturbance, which is the main source to form a dynamo electric field in the ionosphere, perturbations of the ionospheric conductivity also make a significant contribution to the formation of the electric field response to SSW. The post-sunset TEC enhancement and pre-sunrise electron content reduction are revealed as a response to the 2009 SSW. We show that at post-sunset hours the SSW affects low-latitude TEC via a disturbance of the meridional electric field. We also show that the phase change of the semidiurnal migrating solar tide (SW2) in the neutral wind caused by the 2009 SSW at the altitude of the dynamo electric field generation has a crucial importance for the SW2 phase change in the zonal electric field. Such changes lead to the appearance of anomalous diurnal variability of the equatorial electromagnetic plasma drift and subsequent low-latitudinal TEC disturbances in agreement with available observations.Plain Language Summary– Entire Atmosphere GLobal model (EAGLE) interactively calculates the troposphere, stratosphere, mesosphere, thermosphere, and plasmasphere–ionosphere system states and their response to various natural and anthropogenic forcing. In this paper, we study the upper atmosphere response to the major sudden stratospheric warming that occurred in January 2009. Our results agree well with the observed evolution of the neutral temperature in the upper atmosphere and with low-latitude ionospheric disturbances over America. For the first time, we identify an SSW-related cooling in the tropical lower thermosphere that, in turn, could provide additional information for understanding the mechanisms for the generation of electric field disturbances observed at low latitudes. We show that the SSW-related vertical electromagnetic drift due to electric field disturbances is a key mechanism for interpretation of an observed anomalous diurnal development of the equatorial ionization anomaly during the 2009 SSW event. We demonstrate that the link between thermospheric winds and the ionospheric dynamo electric field during the SSW is attained through the modulation of the semidiurnal migrating solar tide.

Highlights

  • The Earth’s ionosphere is a complex system where dynamical, radiative, and chemical processes act together

  • Our modeling results reproduce the following previously observed and explained phenomena during the 2009 stratospheric warming (SSW) event: (1) mesospheric cooling, lower thermospheric warming, and thermospheric cooling over high latitudes of the Northern Hemisphere; (2) stratospheric cooling and mesospheric warming over the tropics; (3) pre-noon Equatorial Ionization Anomaly (EIA) enhancement formed by the eastward electric field intensification; (4) afternoon EIA weakening and total electron content (TEC) decrease at low-latitudes explained by westward electric field intensification

  • The presented results confirm that the vertical plasma drift plays a major role in the daytime low-latitude TEC variability during the 2009 SSW event

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Summary

Introduction

The Earth’s ionosphere is a complex system where dynamical, radiative, and chemical processes act together. Several authors exploited different models and simulation techniques (e.g., assimilation of data or dynamical nudging) to reproduce the observed equatorial electromagnetic drift disturbances during the 2009 SSW event (Fuller-Rowell et al, 2011a; Jin et al, 2012; Pedatella et al, 2016) Most of these attempts were not fully successful and there are still open questions on the generation mechanism of such zonal electric field disturbances during SSW events and for the requirement of atmosphere–ionosphere system models that aim to properly simulate such processes. The model performance was evaluated by comparing simulations with neutral temperature observed by the MIPAS/Envisat instrument and global positioning system total electron content (GPS TEC) measurements

The EAGLE model
MIPAS data
GPS TEC data
Simulation results and comparison with observations
Daily and zonal mean anomalies in the middle and upper atmosphere
Analysis of tidal variations in the lower thermosphere and the electric field
Conclusions
Full Text
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