Estimates of magnetic field strength in the solar corona using observations of thermal radio emission at low frequencies

arXiv:2609.29602 · astro-ph.SR · Submitted 2026-09-24 · Read on arXiv

astro-ph.SR

Submitted: 2026-09-24

Updated: 2026-09-24

Terminology

• Calibration — 3× in this paper · explained in 7 episodes
• Astronomical Image Processing System — 2× in this paper
• Gauribidanur Radio Observatory — 2× in this paper
• Trace — 2× in this paper · explained in 2 episodes
• Active Regions — 1× in this paper · explained in 1 episode

Sources

• Augmentation of the Gauribidanur radioheliograph for observations of circularly polarized emission from the solar corona at low radio frequencies

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