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PSP/FIELDS Observations of Circularly Polarized Interplanetary Radio Bursts

Date: 2026-02-27 00:00:00

Time: 3:30–4:30 PM

Location: 3853 Slichter Hall

Presented By:
Marc Pulupa – UC Berkeley Space Sciences Lab

Abstract:

Solar radio bursts are signatures of nonthermal electron acceleration by energetic events such as flares and coronal mass ejections. The launches of Parker Solar Probe in 2018 and Solar Orbiter in 2020 have enabled new views of radio bursts from the vantage point of the inner heliosphere. In this talk, I will briefly discuss some of the top radio burst discoveries of the Parker-Orbiter era, with a focus on circular polarization observations made by Parker Solar Probe. I will describe the measurement of polarization using spacecraft antennas, show examples of circularly polarized Type II and Type III radio bursts, and discuss how polarization can serve as a remote diagnostic of radio burst source regions.