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[1] In the paper “Application of the GPS network to estimate the effect of the terrestrial ionosphere on the radio occultation measurements of planetary ionospheres” by K. Noguchi, T. Imamura, K.-I. Oyama, and A. Saito (Radio Science, 36(6), 1607–1613, 2001), an incorrect version of Figure 2 was published. The correct Figure 2 and its caption appear below.

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Figure 2. Probability of detection of the Martian nightside ionosphere versus local time and month. The primary noise source is assumed to be the TEC fluctuation in the terrestrial ionosphere.

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