On the solar white-light high resolution observations from space

摘要: Abstract Absolutely calibrated telescopic observations of the Sun in white-light with a sufficiently high space–time resolution from space have not been regularly performed. They are needed to resolve several important problems solar physics. Contributions different morphological features total irradiance variations broad range time scales seconds up many years can be definitely established this manner for first time. The quantitative role emission overall energy balance flares and eruptions on evaluated. More adequate theoretical models corresponding processes constructed using new data.