Abstract
Results are presented from observing auroral kilometric radition (AKR) from sources in the auroral regions of the northern and southern hemispheres. The emissions are recorded and analyzed simultaneously using data from the ERG (Arase) satellite. Differences between the AKRs in the northern and southern hemispheres are noted. It is shown that northern and southern sources of AKRs predominate at different times.
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ACKNOWLEDGMENTS
The authors are grateful to A. Kumamoto, J. Kasahara, and F. Tsuchiya for providing the PWE/HFA instrument data used in this work. The ERG (Arase) satellite data and the characteristics of scientific instruments were obtained from the ERG Science Center of ISAS/JAXA and ISEE/Nagoya University, https://ergsc.isee.nagoya-u.ac.jp/ [11, 12]. Data from the PWE HFA-L2 v01.01 device in [14, 15] was analyzed.
Funding
A.A. Chernyshov and V.I. Kolpak acknowledge the support of the Foundation for the Advancement of Theoretical Physics and Mathematics “BASIS.” The work of M.M. Mogilevsky was supported by the RF Ministry of Science and Higher Education, grant no. 075-15-2020-780 (N13.1902.21.0039). The work of A.A. Chernyshov and D.V. Chugunin was supported by the Russian Foundation for Basic Research, project no. 18-29-21037.
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Translated by T. Sokolova
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Chernyshov, A.A., Mogilevsky, M.M., Chugunin, D.V. et al. Simultaneous Observation of Auroral Kilometric Radiation from Northern and Southern Sources. Bull. Russ. Acad. Sci. Phys. 86, 295–299 (2022). https://doi.org/10.3103/S1062873822030078
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DOI: https://doi.org/10.3103/S1062873822030078