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May 13, 2026Bulletin of the Russian Academy of Sciences Physics0 citations

Analysis of Auroral Kilometric Radiation Detected by WIND Satellite

Features of Auroral Kilometric Radiation in the Solar Wind

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Authors

ВКВ. И. КолпакMMM. M. MogilevskyDCD. V. Chugunin

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Overview

Randomized trial analyzes auroral kilometric radiation in solar wind, indicating its varying nature during the solar cycle.

Key Points

  • This research aims to analyze auroral kilometric radiation (AKR) detected by the WIND satellite and understand its characteristics and behavior in the solar wind.
  • Employed analysis of electromagnetic radiation frequencies from 20 to 1040 kHz detected on the WIND satellite from 2004 to 2021.
  • Conducted a statistical analysis comparing measurements with near-Earth spacecraft data to confirm AKR origins.
  • Examined the spatial distribution and occurrence rate of radiation in relation to the solar cycle.
  • Up to 70% of AKR reaches the L1 libration point where the WIND satellite is located.
  • The AKR spectrum transforms noticeably, reflecting changes during different solar cycle phases.
  • Radiation occurrence rate is nonuniform, varying significantly over time.
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Cite This Study

Колпак et al. (2026) studied this question.

synapsesocial.com/papers/6a04147679e20c90b44446d9https://doi.org/10.1134/s1062873825715429
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