Investigating Spatial and Temporal Structuring of E-Region Coherent Scattering Regions Over Northern Norway

Abstract Recently, it has been shown that the Spread Spectrum Interferometric Multistatic meteor radar Observing Network radar system located in northern Norway is capable of measuring ionospheric E‐region coherent scatter with spatial and temporal resolutions on the order of 1.5 km and 2 s, respect...

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Bibliographic Details
Published in:Journal of Geophysical Research: Space Physics
Main Authors: Huyghebaert, Devin Ray, Chau, Jorge L., Spicher, Andres, Ivarsen, Magnus Fagernes, Clahsen, Matthias, Latteck, Ralph, Vierinen, Juha-Pekka
Format: Article in Journal/Newspaper
Language:English
Published: 2023
Subjects:
Online Access:http://hdl.handle.net/10852/106288
https://doi.org/10.1029/2023JA031682
Description
Summary:Abstract Recently, it has been shown that the Spread Spectrum Interferometric Multistatic meteor radar Observing Network radar system located in northern Norway is capable of measuring ionospheric E‐region coherent scatter with spatial and temporal resolutions on the order of 1.5 km and 2 s, respectively. Four different events from June and July of 2022 are examined in the present study, where the coherent scatter measurements are used as a tracer for large‐scale ionospheric phenomena such as plasma density enhancements and ionospheric electric fields. By applying a two‐dimensional Fourier analysis to range‐time‐intensity data, we perform a multi‐scale spatial and temporal investigation to determine the change in range over time of large‐scale ionospheric structures (>3 km) which are compared with line‐of‐sight velocities of the small scale structures (∼5 m) determined from the Doppler shift of the coherent scatter. The spectral characteristics of the large‐scale structures are also investigated and logarithmic spectral slopes for scale sizes of 100–10 km were found to be between −3.0 and −1.5. This agrees with much of the previous work on the spatial spectra scaling for ionospheric electric fields. This analysis aids in characterizing the source of the plasma turbulence and provides crucial information about how energy is redistributed from large to small scales in the E‐region ionosphere.