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We compare dependences between the storm development rate $|Dst_{min}|/\DeltaT$ ($\Delta T$ is the durations of main phase) and the duration of recoveryphase of magnetic storms generated by three various types of interplanetarydrivers: (1, 2) compression regions CIR and Sheath, and (3) body ofinterplanetary CME (magnetic clouds and Ejecta). Our analyze shows that theduration of recovery phase correlates with the storm development rate for CIR-and Sheath-induced storms, and does not correlate for ICME- induced storms.

Whether duration of the recovery phase of magnetic storm depends on the development rate of storm at its main phase?