A model for ion-acoustic waves in the solar atmosphere is presented. I
n the limit of strongly magnetized plasma this model leads to the Zakh
arov-Kuznetsov equation which possesses a flat solitary wave solution.
An initial-value problem for this equation is solved numerically to s
how a transition of the flat solitary waves into spherical solitary wa
ves. The paper suggests further developments of an ion-acoustic wave t
heory that may improve our knowledge of ion-acoustic waves and lead to
the possibility of their being detected in the solar atmosphere.