Fig. 10From: Sub-ion-gyro scale magnetic field compressions generated by the solar wind interaction with the moonDistribution of short-period magnetic enhancements detected by Kaguya. Position of Kaguya at the detection of short-period magnetic enhancements projected on the a \(x - y\), \(x - z\), and \(y - z\) planes of the SSE coordinate system. Red dots (#1 and #2) are limb compressions found in the constant solar wind magnetic field, and black dots are those found at interplanetary magnetic discontinuities. Event numbers are the same as those in Table 1Back to article page