TY - JOUR
T1 - Ionospheric effects of sudden stratospheric warming during moderate-to-high solar activity
T2 - Case study of January 2013
AU - Goncharenko, L.
AU - Chau, J. L.
AU - Condor, P.
AU - Coster, A.
AU - Benkevitch, L.
N1 - Copyright:
Copyright 2013 Elsevier B.V., All rights reserved.
PY - 2013/10/16
Y1 - 2013/10/16
N2 - A major sudden stratospheric warming (SSW) occurred in January 2013 during moderate-to-high solar activity conditions. Observations during the winter of 2012/2013 reveal strong ionospheric disturbances associated with this event. Anomalous variations in vertical ion drift measured at the geomagnetic equator at Jicamarca (12°S, 77°W) are observed for over 40 days. We report strong perturbations in the total electron content (TEC) that maximize in the crests of equatorial ionization anomaly, reach 100% of the background value, exhibit significant longitudinal and hemispheric asymmetry, and last for over 40 days. The magnitude of ionospheric anomalies in both vertical drifts and TEC is comparable to the anomalies observed during the record-strong SSW of January 2009 that coincided with the extreme solar minimum. This observation contrasts with results of numerical simulations that predict weaker ionospheric response to the tidal forcing during high solar activity. Key Points Ionospheric anomalies due to stratospheric warming of 2013 are long, > 40 days Ionospheric anomalies due to SSW are strong, up to 80-100% of the background This contrasts with numerical simulations
AB - A major sudden stratospheric warming (SSW) occurred in January 2013 during moderate-to-high solar activity conditions. Observations during the winter of 2012/2013 reveal strong ionospheric disturbances associated with this event. Anomalous variations in vertical ion drift measured at the geomagnetic equator at Jicamarca (12°S, 77°W) are observed for over 40 days. We report strong perturbations in the total electron content (TEC) that maximize in the crests of equatorial ionization anomaly, reach 100% of the background value, exhibit significant longitudinal and hemispheric asymmetry, and last for over 40 days. The magnitude of ionospheric anomalies in both vertical drifts and TEC is comparable to the anomalies observed during the record-strong SSW of January 2009 that coincided with the extreme solar minimum. This observation contrasts with results of numerical simulations that predict weaker ionospheric response to the tidal forcing during high solar activity. Key Points Ionospheric anomalies due to stratospheric warming of 2013 are long, > 40 days Ionospheric anomalies due to SSW are strong, up to 80-100% of the background This contrasts with numerical simulations
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U2 - 10.1002/grl.50980
DO - 10.1002/grl.50980
M3 - Article
AN - SCOPUS:84885005232
SN - 0094-8276
VL - 40
SP - 4982
EP - 4986
JO - Geophysical Research Letters
JF - Geophysical Research Letters
IS - 19
ER -