The
m/n = 1/1 helical ion density “snake” located near the
q = 1 magnetic surface in a toroidal, magnetically confined plasma arises naturally in resistive MHD, when the plasma density evolves separately from pressure. Nonlinear numerical simulations show that a helical density perturbation applied around
q = 1 can form a quasi-steady state over
q≳1 with

of opposite average sign to

. Two principal outcomes depend on the magnitude of
/n and the underlying stability of the 1/1 internal kink mode. For a small
q<1 central region, a moderate helical density drives a new, slowly growing type of nonlinear 1/1 internal kink inside
q<1, with small

and
∇
≃ ∇(n
). The hot kink core moves away from, or perpendicular to, the high density region near
q ≃ 1, preserving the snake density during a sawtooth crash. The mode resembles the early stage of heavy-impurity-ion snakes in ohmic discharges, including recent observations in Alcator C-Mod. For a larger, more unstable
q<1 region, the helical density perturbation drives a conventional 1/1 kink where

aligns with

, leading to a rapid sawtooth crash. The crash redistributes the density to a localized helical concentration inside
q≲1, similar to experimentally observed snakes that are initiated by a sawtooth crash.