With the Solar Ultraviolet Measurements of Emitted Radiation instrument—a high-resolution normal-incidence telescope and spectrometer on board the Solar and Heliospheric Observatory—heliumlike transitions in the highly ionized species and were observed. The spectral lines were emitted by high-temperature solar flare plasmas. In this paper, we report on wavelength measurements of the He-like lines identified in the recorded spectra. The wavelength uncertainties we obtained from the solar measurements are and in one case This is comparable to or better than the best determinations so far achieved for these heliumlike transitions with instrumentation in the laboratory. For the transition we report what is to our knowledge the first wavelength measurement. The knowledge of the accurate wavelengths can provide important checks on atomic structure calculations.