  Future prospects for solar spectroscopy missions operating in the extreme
ultraviolet (EUV) and soft X-ray (SXR) wavelength ranges, 1.2-1600 Angstroms,
are discussed. NASA is the major funder of Solar Physics missions, and brief
summaries of the opportunities for mission development under NASA are given.
Upcoming major solar missions from other nations are also described. The
methods of observing the Sun in the two wavelength ranges are summarized with a
discussion of spectrometer types, imaging techniques and detector options. The
major spectral features in the EUV and SXR regions are identified, and then the
upcoming instruments and concepts are summarized. The instruments range from
large spectrometers on dedicated missions, to tiny, low-cost CubeSats launched
through rideshare opportunities.
