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High-beta plasma blobs in the morningside plasma sheet

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Fig. 1. Large-amplitude ¯uctuations of magnetic ®eld strength and orientation near the apogee of Equator-S during early morning hours
Fig. 2. Plasma and magnetic-®eld measurements plus derived quan- quan-tities on an outbound orbit of Equator-S on 18 March 1998
Fig. 4. Same as Fig. 2, but without total pressure, for 3 April and 9 April 1998
Fig. 6. An example of the detailed variation of magnitude (B), polar angle (theta), and azimuth (phi) of the magnetic ®eld in one of the ®eld depressions (plasma blobs) observed on 9 March 1998
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