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.
Authors
- Sam Hallman
- Masha Mikhailova
- D. Besson (ORCID: https://orcid.org/0000-0001-6733-963X)
Publication Details
- Published
- 2024-11-07
- DOI
- https://doi.org/10.22323/1.470.0004
- Primary Topic
- Solar and Space Plasma Dynamics
- Type
- article
- Field-Weighted Citation Impact
- 0.00