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Magnetic Connectivity in the Time-dependent Corona and Heliosphere

  • Authors: Roberto Lionello, Cooper Downs, Emily I. Mason, Jon A. Linker, Pete Riley, Mathew J. Owens

Roberto Lionello et al 2026 The Astrophysical Journal Letters 1001 .

  • Provider: AAS Journals

Caption: Figure 2.

Connectivity maps for the runs of Table 1. Color codes: navy, open negative flux; maroon, open positive flux; green, closed flux; sky blue, disconnected flux; and white dashed line, Br = 0. (a) Mercator projection at 1 au for SMTD; (b) cut at 0 longitude for SMTD. (c) Same as (a) for SMSS. (d) Same as (b) for SMSS. (e), (f) Same as (a) and (b), respectively, for E24TD. (g), (h) Same as (c) and (d), respectively, for E24SS.

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