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Estimates of Magnetic Field Strength in the Solar Corona Using Observations of Thermal Radio Emission at Low Frequencies

  • Authors: Sayuf Shaik, C. Kathiravan, R. Ramesh

Sayuf Shaik et al 2026 The Astrophysical Journal 1011 .

  • Provider: AAS Journals

Caption: Figure 1.

Layout of the augmented GRAPH array (not to scale). Each blue line in the EW arm represents a group of eight LPDAs in 90° orientation (w.r.t. the celestial north). In the NS arm, each blue line represents groups of eight LPDAs in 90° orientation, and each orange line represent groups of eight LPDAs in 0° orientation (w.r.t. the celestial north). The photograph of a small section of the south arm of the augmented GRAPH is shown in the upper right.

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