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Statistical survey of nighttime midlatitude magnetic fluctuations: Their source location and Poynting flux as derived from the Swarm constellation
Author(s) -
Park Jaeheung,
Lühr Hermann,
Stolle Claudia,
RodriguezZuluaga Juan,
Knudsen David J.,
Burchill Johnathan K.,
Kwak YoungSil
Publication year - 2016
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
eISSN - 2169-9402
pISSN - 2169-9380
DOI - 10.1002/2016ja023408
Subject(s) - poynting vector , middle latitudes , ionosphere , physics , flux (metallurgy) , geophysics , electric field , magnetic field , plasma , context (archaeology) , atmospheric sciences , earth's magnetic field , computational physics , geology , paleontology , materials science , quantum mechanics , metallurgy
Abstract This is the first statistical survey of field fluctuations related with medium‐scale traveling ionospheric disturbances (MSTIDs), which considers magnetic field, electric field, and plasma density variations at the same time. Midlatitude electric fluctuations (MEFs) and midlatitude magnetic fluctuations (MMFs) observed in the nighttime topside ionosphere have generally been attributed to MSTIDs. Although the topic has been studied for several decades, statistical studies of the Poynting flux related with MEF/MMF/MSTID have not yet been conducted. In this study we make use of electric/magnetic field and plasma density observations by the European Space Agency's Swarm constellation to address the statistical behavior of the Poynting flux. We have found that (1) the Poynting flux is directed mainly from the summer to winter hemisphere, (2) its magnitude is larger before midnight than thereafter, and (3) the magnitude is not well correlated with fluctuation level of in situ plasma density. These results are discussed in the context of previous studies.