Abstract
Solar flare observations in the sub-mm and IR spectral band are essentially unexistent. They could provide crucial tests to flare models and particle acceleration mechanisms in hot solar plasmas. There are evidences that certain solar bursts exhibit a spectral component extending towards wavelengths shorter than 3 mm. On the other hand, the spectral features of white light flares are unknown in the infra-red range of frequencies. Space and ground-based experiments are proposed for solar flux measurements in that band with high time resolution.
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