Answers are grounded in this paper and cite their sources.
Quasi-periodic variations in the Doppler shift of the HF range frequency at a vertical path and critical frequency of the F 2 layer caused by wave disturbances in the ionosphere on the day of the partial (the magnitude was about 0.42) solar eclipse and on background days are analyzed. For the spectral analysis, the window Fourier transform, adaptive Fourier transform, and wavelet analysis were jointly used. It is shown that on the day of the eclipse and the background day, spectral characteristics of wave disturbances within the 150–200 km height range differed substantially. The changes in the spectral composition began approximately 30–35 min after the solar eclipse beginning and lasted more than 1.5 h.
No takes yet. Share an insight, caveat, or question.
Leonid F. Chernogor (2010) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: