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The extreme ultraviolet portion of the solar spectrum contains a wealth ofdiagnostic tools for probing the lower solar atmosphere in response to aninjection of energy, particularly during the impulsive phase of solar flares.These include temperature and density sensitive line ratios, Doppler shiftedemission lines and nonthermal broadening, abundance measurements, differentialemission measure profiles, and continuum temperatures and energetics, amongothers. In this paper I shall review some of the advances made in recent yearsusing these techniques, focusing primarily on studies that have utilized datafrom Hinode/EIS and SDO/EVE, while also providing some historical backgroundand a summary of future spectroscopic instrumentation.

Extreme Ultra-Violet Spectroscopy of the Lower Solar Atmosphere During Solar Flares