  Self-annihilating dark matter gravitationally captured by the Sun could yield
observable neutrino signals at current and next generation neutrino detectors.
By exploiting such signals, neutrino detectors can probe the spin-dependent
scattering of weakly interacting massive particles (WIMPs) with nucleons in the
Sun. We describe a method how to convert constraints on neutrino fluxes to a
limit on the WIMP-nucleon scattering cross section. In this method all neutrino
flavors can be treated in a very similar way. We study the sensitivity of
neutrino telescopes for Solar WIMP signals using vertex contained events and
find that this detection channel is of particular importance in the search for
low mass WIMPs. We obtain highly competitive sensitivities with all neutrino
flavor channels for a Megaton sized detector through the application of basic
spectral selection criteria. Best results are obtained with the electron
neutrino channel. We discuss associated uncertainties and provide a procedure
how to treat them for analyses in a consistent way.
