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The Far Ultraviolet (FUV: hereafter 900-1150 A) is a spectral range whichcontains many of the ground state transitions of common elements but has hadlimited observational capabilities due to the unique technological requirementsto operate in this waveband. Conceptual designs are presented, for highresolution (R > 50,000) echelle spectrographs for CubeSat, SMEX and MIDEXmissions, along with comparisons of their performance to past instruments.

Aberration corrected ultraviolet echelle spectrographs: straw man designs and performance