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. 2021 Jun 1;48(11):e2021GL092700. doi: 10.1029/2021GL092700

Figure 2.

Figure 2

(a–d) Vector magnetic field measurements from ACE, DSCOVR, Wind, and ARTEMIS in the upstream solar wind. (e) Spacecraft locations in GSE coordinates at 18 UT on November 6. (f and h) B total and B z as well as (g and i) ion density at Wind and ARTEMIS, respectively. (j) Sym‐H, with vertical dashed lines marking the peaks of the six positive excursions.