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The purpose of this white paper is to put together a coherent vision for therole of helioseismic monitoring of magnetic activity in the Sun's farhemisphere that will contribute to improving space weather forecasting as wellas fundamental research in the coming decade. Our goal fits into the broadercontext of helioseismology in solar research for any number of endeavors whenhelioseismic monitors may be the sole synoptic view of the Sun's farhemisphere. It is intended to foster a growing understanding of solar activity,as realistically monitored in both hemispheres, and its relationship to allknown aspects of the near-Earth and terrestrial environment. Some of thequestions and goals that can be fruitfully pursued through seismic monitoringof farside solar activity in the coming decade include: What is therelationship between helioseismic signatures and their associated magneticconfigurations, and how is this relationship connected to the solar EUVirradiance over the period of a solar rotation?; How can helioseismicmonitoring contribute to data-driven global magnetic-field models for precisespace weather forecasting?; What can helioseismic monitors tell us aboutprospects of a flare, CME or high-speed stream that impacts the terrestrialenvironment over the period of a solar rotation?; How does the inclusion offarside information contribute to forecasts of interplanetary space weather andthe environments to be encountered by human crews in interplanetary space?Thus, it is crucial for the development of farside monitoring of the Sun becontinued into the next decade either through ground-based or space-borneobservations.

Seismic Monitoring of the Sun's Far Hemisphere: A Crucial Component in  Future Space Weather Forecasting (A White Paper Submitted to the Decadal  Survey for Solar and Space Physics (Heliophysics) -- SSPH 2024-2033)