||Short note: Three dimensional deconvolution of helioseismic data||
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This is a short note on helioseismic deconvolution. Herein results are presented by deconvolving helioseismic data with a calculated impulse response in 3D to help determine source information in the shallow solar interior. Tentatively it can be concluded that there the solar acoustic energy is close to uniformaly distributed throughout the convective envelope.