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This paper presents an updated concept for the ARKA solar observatory, designed for fundamental research into solar physics and space weather forecasting. The project is envisioned as a ground–space complex, comprising a space observatory deployed near the L1 point of the Sun–Earth system and a ground-based long-wavelength radio telescope for observing interplanetary scintillations and tracking the propagation of coronal mass ejections. This unique approach, which combines high-angular-resolution space observations of the solar atmosphere with ground-based radio observations and measurements of solar wind parameters, will enable the study of solar activity mechanisms and improve the accuracy and lead time of forecasting geoeffective events.
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Rudnitsky et al. (2026) studied this question.
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