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We study how gravitational focusing (GF) of dark matter by the Sun affectsthe annual and biannual modulation of the expected signal in non-directionaldirect dark matter searches, in the presence of dark matter substructure in thelocal dark halo. We consider the Sagittarius stream and a possible dark disk,and show that GF suppresses some, but not all, of the distinguishing featuresthat would characterize substructure of the dark halo were GF neglected.

Gravitational Focusing and Substructure Effects on the Rate Modulation in Direct Dark Matter Searches