Year: 2025
Type: article
Abstract: Introduction The only reliable method to remotely obtain magnetic field information across large swaths of interplanetary/interstellar plasma is with the measurement of Faraday rotation of polarized radio signals. Methods Focusing on the high frequency regime of magnetized plasmas, this paper discusses the most difficult first step toward obtaining these measurements. Transitioning from raw voltage samples to plane of polarization measurements requires both simulated signal tests and qualitative inspections of the behavior of the resulting measurements. Results To demonstrate how this calibration approach works, we show examples collected from the STEREO A and B spacecraft and the Mars Reconnaissance Orbiter spacecraft. Discussion While astronomical radio sources have their own challenges to data processing, we show that spacecraft data have their own unique characteristics that can benefit and hinder the data processing.
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: gold
Estimated APC paid: $2,353
Awards: G1880079534, G2938431867
OpenAlex ID: W4417114963