  We describe a new algorithm for reconstruction of Differential Emission
Measures (DEMs) in the solar corona. Although a number of such algorithms
currently exist, they can have difficulty converging for some cases, and can be
complex, slow, or idiosyncratic in their output (i.e., their inversions can
have features that are a result of the inversion code and instrument response,
not of the solar source); we will document some of these issues in this paper.
The new algorithm described here significantly reduces these drawbacks and is
particularly notable for its simplicity; it is reproduced here, in full, on a
single page. After we describe the algorithm, we compare its performance and
fidelity with some prevalent methods. Although presented here for extreme
ultraviolet (EUV) data, the algorithm is robust and extensible to any other
wavelengths (e.g., X-rays) where the DEM treatment is valid.
