We review our current understanding of the solar sources of interplane tary structures that result in geomagnetic disturbances, especially storms. These sources have been broadly classified as: 1) transient or sporadic, or 2) recurrent, although we now know that these categories are not exclu sive. Transients usually refer to coronal mass ejections (CMEs). Recurrence refers to disturbances that repeat with the 27-day synodic rotation period of the Sun. CMEs are expulsions of large quantities of plasma and magnetic field from the Sun's corona. The occurrence rate of CMEs approximately follows that of the solar (sunspot) activity cycle. Recurrent sources are usu ally attributed to high-speed solar wind streams emanating from coronal holes. However, compression at the leading edge of the stream as it runs into the higher-density slow flow surrounding the heliospheric current sheet leads to a corotating interaction region (CIR), and it is passage of the CIR, not the high speed flow, that results in enhanced recurrent geomagnetic dis turbances. Moreover, the largest recurrent geomagnetic storms are actually caused by CMEs caught up in the CIRs.