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Motivated by IceCube solar searches, we investigate neutralino dark matter in supersymmetric SU(5) with nonuniversal gaugino masses. Combining micrOMEGAs relic abundances with DarkSUSY calculations, we develop a consistent picture of solar neutrino and muon signals from thermal neutralino subcomponents. We identify how local abundance, neutralino composition, and capture-annihilation equilibrium shape these signals beyond simple scaling with the dark matter fraction. Integrated fluxes and representative benchmarks connect these predictions to published IceCube reference limits. Our results provide a framework for interpreting solar searches and assessing the signals of subdominant neutralino dark matter.

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