A Time-of-Arrival Technique to Estimate the Source of a Type III Solar Radio Burst

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Authors

Julia Kirkey · University of Michigan

Jamie Hendrickson · University of Michigan

Saul Roman-Ramirez · University of Michigan

Mojtaba Akhavan-Tafti · University of Michigan

Jason I. Kooi · United States Naval Research Laboratory

Brian Hicks · United States Naval Research Laboratory

T. E. Clarke

Abstract

Type III solar radio bursts (SRBs) are the most common type of low-frequency emission caused by energized electrons coming from the Sun. They are frequently linked to solar flares that can lead to severe geomagnetic storms; consequently, one of the ke

Topics & Keywords

Ionosphere and magnetosphere dynamics Solar and Space Plasma Dynamics Earthquake Detection and Analysis

UN Sustainable Development Goals

Climate action

Publication Details

DOI: 10.22541/essoar.176840689.90354930/v1

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