Solar Flare Observations with the RNO-G Detector

Although designed for detection of cosmic ray neutrinos, the RNO-G detector serendipitously registered signals on Sept. 29, 2022 (approximately 48 hours before illumination of the solar panels fell below threshold to power the array) which were ultimately traced to a solar flare event on that day. Closer examination of the 2022 and 2023 RNO-G data revealed almost 100 solar flare events, each of which produced anywhere from tens to hundreds of triggers in the RNO-G stations. We detail, in this contribution, how those events were identified and subsequently used to calibrate the positions of the in-ice antennas on centimeter scales.

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Publication Details

Published
2024-11-07
DOI
https://doi.org/10.22323/1.470.0004
Primary Topic
Solar and Space Plasma Dynamics
Type
article
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article

Solar Flare Observations with the RNO-G Detector

Sam Hallman, Masha Mikhailova, D. Besson
Solar and Space Plasma Dynamics
article

Solar Flare Observations with the RNO-G Detector

Sam Hallman, Masha Mikhailova, D. Besson
article en

Abstract

Although designed for detection of cosmic ray neutrinos, the RNO-G detector serendipitously registered signals on Sept. 29, 2022 (approximately 48 hours before illumination of the solar panels fell below threshold to power the array) which were ultimately traced to a solar flare event on that day. Closer examination of the 2022 and 2023 RNO-G data revealed almost 100 solar flare events, each of which produced anywhere from tens to hundreds of triggers in the RNO-G stations. We detail, in this contribution, how those events were identified and subsequently used to calibrate the positions of the in-ice antennas on centimeter scales.

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