The ionosphere response resulting from minimum solar activity during cycle 23/24 was unusual and offered unique opportunities for investigating space weather in the near-Earth environment. We report ultra low frequency electric field signatures related to the ionospheric Alfvén resonator detected by the Communications/Navigation Outage Forecasting System (C/NOFS) satellite in the equatorial region. These signatures are used to constrain ionospheric empirical models and offer a new approach for monitoring ionosphere dynamics and space weather phenomena, namely aeronomy processes, Alfvén wave propagation, and troposphere-ionosphere-magnetosphere coupling mechanisms. © 2012 American Geophysical Union. All Rights Reserved.
CITATION STYLE
Simões, F., Klenzing, J., Ivanov, S., Pfaff, R., Freudenreich, H., Bilitza, D., … Yokoyama, T. (2012). Detection of ionospheric Alfvén resonator signatures in the equatorial ionosphere. Journal of Geophysical Research: Space Physics, 117(11). https://doi.org/10.1029/2012JA017709
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