The Interhelioprobe (IHP) is a perspective space solar mission developed by the Russian Space Agency together with the Russian Academy of Sciences. The mission aims to provide long-term remote observations of the Sun and in-situ measurements of the heliospheric magnetic fields and plasma from the out-of-ecliptic heliocentric orbit with the perihelion of about 60 solar radii. The Interhelioprobe spacecraft is equipped with an ensemble of imaging instruments at least two of which are specially dedicated for observations of solar eruptive phenomena and CME. The first one is a white-field coronagraph named "Oka" which will observe the outer solar corona from the distance of 2˚ to 10˚ from the Sun's center. The second one is a white-field heliospheric imager "Heliosphera" with the field of view of 10˚ – 30˚. We describe in detail both these instruments and present our scientific program for observation of CME and eruptive phenomena during the IHP mission.