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Turbulence-coupled Electrodynamics of the Martian Year 34 Global Dust Storm on Mars

  • Authors: Chali Idosa Uga, Gary P. Zank, Dennis L. Gallagher

Chali Idosa Uga et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 2.

Latitude–solar longitude (Ls) distribution of column dust optical depth (τ) during MY 34 from MCD v.6.1. Filled contours show τ, and the blue curve denotes the global-mean column dust optical depth (right axis). The blue and green shaded regions indicate the quiescent period (Ls = 20°–60°) and the MY 34 dust-storm interval (Ls = 185°–270°), respectively.

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