SOLAR ULTRAVIOLET RADIATION AS A POSSIBLE CAUSE OF LONG-PERIOD PREFLARE FLUCTUATIONS OF THE HORIZONTAL COMPONENT OF THE GEOMAGNETIC FIELD |
| 6 | |
| 2013 |
| scientific article | 523.9-739:550.380.25:523.985-125 | ||
| 88-93 | solar ultraviolet emission, H component of the geomagnetic field, proton flares, preflare situations, wavelet analysis |
| Wavelet spectra of solar ultraviolet radiation before proton flares are studied and a comparison is carried out of the preflare behavior of long-period solar UV radiation spectral components and the H component of the geomagnetic field. Long-period (30–60 minutes) pulsations of the H component of the geomagnetic field according to ground-based measurements have been found to be in compliance with those of solar UV radiation spectral components 3–1 days before a proton flare. |
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