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Extracting magnetic and thermodynamic information from spectropolarimetricobservations is a difficult and time consuming task. The amount ofscience-ready data that will be generated by the new family of large solartelescopes is so large that we will be forced to modify the present approach toinference. In this contribution, I propose several possible ways that might beuseful for extracting the thermodynamic and magnetic properties of solarplasmas from such observations quickly.

Extracting information from the data flood of new solar telescopes. Brainstorming