Since this introduction to the physics of the Sun first appeared in 1989, significant progress has been made in solar research. New insights grew especially from the results of space missions, above all SOHO, the Solar and Heliospheric Observatory, which in 1996 reached its orbit around the Lagrangian point L1 between the Earth and the Sun. Refined theoretical models have been advanced as well, but clearly, in my view, the lead was on the observational side.
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