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The Atacama Large Millimeter/submillimeter Array (ALMA) will be a valuabletool for observing the chromosphere of our Sun at (sub-)millimeter wavelengthsat high spatial, temporal and spectral resolution and as such has greatpotential to address long-standing scientific questions in solar physics. Inorder to make the best use of this scientific opportunity, the SolarSimulations for the Atacama Large Millimeter Observatory Network has beeninitiated. A key goal of this international collaboration is to support thepreparation and interpretation of future observations of the Sun with ALMA.

Solar Simulations for the Atacama Large Millimeter Observatory Network