From December 1987 to February 1988 using the UTR-2 radiotelescope, we recorded the emissions of PSR 0823+26 and PSR 0943+10 at 25 and 16.7 MHz. Both pulsars are of considerable interest; PSR 0943+10 is one of several pulsars having two emission modes (Suleymanova and Izvekova 1984), and PSR 0823+26 has interpulse emission (Backer, Boriakoff, and Manchester 1973, Downs 1979) and dispersion measure, 19.466 pc cm–3. It is known that using the Arecibo telescope at 25 MHz one could succeed in recording only PSR 0919+06 with DM = 27.25 pc cm–3 (Phillips and Wolszczan 1989, 1990). In these papers, the presence of the two modes of PSR 0943+10 emission was confirmed.