Skip to main content
Fig. 4 | Earth, Planets and Space

Fig. 4

From: Relationship between large-scale ionospheric field-aligned currents and electron/ion precipitations: DMSP observations

Fig. 4Fig. 4

a. The MLAT versus MLT distribution of FACs derived from the DMSP satellites for the northern hemisphere. The subpanels are arranged by the intensity of IMF By and Bz components: from left to right, the By component varies from 10 to – 10 nT, and from top to bottom, the Bz varies from 10 to – 10 nT, both with a step of 5 nT. b As the same as Fig. 4a, but for the FACs distribution in the southern hemisphere

Back to article page