[en] Celestial sphere distribution of gamma bursts ( approximately 70 events) relative to the plane of the solar equator is considered. The following main peculiarities of the bursts have been revealed: concentration in the direction of heliographical latitudes +-12, +-34, +-56, -79 deg and their pair production. Heliolatitude, besides nearness in time (subsequence) of events, is indication of the pair. The above peculiarities of gamma bursts can be understood in the approximation of their genetic relation to the Sun. The presence of a current layer in the heliosphere discovered with the Pioneer 11 satellite at one of the latitudes of gamma burst concentration permits to suggest that the latitudinal zonality in burst distribution reflects the heliomagnetosphere structure and large-scale magnetic field of the Sun. General features of burst and some solar phenomena behaviour in the latitudinal dependences is noted. Suggested heliospheric origin of bursts results in sequences which can be observed: 1) close origin of bursts restricted with the heliosphere size; 2) relation of gamma-bursts with the magnetic structure of a nearsolar space and the Sun; 3) dependence of the number of bursts on the phase of the solar activity