SCIENCE GOALS: PROVIDE A STANDARDIZED SET OF TOOLS FOR COMPUTING VIEWING AND ANALYZING THE THERMAL STRUCTURE OF CORONAL PLASMAS EMISSION FROM THE SOLAR CORONA IS CHARACTERIZED BY A `DIFFERENTIAL EMISSION MEASURE' (DEM) WHICH IS A DISTRIBUTION OF SQUARED DENSITY ALONG THE LINE OF SIGHT AS A FUNCTION OF TEMPERATURE. THE INTENSITY OF MOST CORONAL SPECTRAL LINES ARE COMPLETELY DETERMINED BY THESE FUNCTIONS SO THEY ENCOMPASSES EVERYTHING THESE LINE INTENSITIES CAN TELL US FROM A SINGLE POINT OF VIEW. THIS PROJECT