Bruce T. Tsurutani, Rajkumar Hajra, and Gurbax S. Lakhina
We discuss the history of quasiperiodic ~27-day recurrent geomagnetic activity and the origin of the names "interaction region", "corotating interaction region" and "stream interaction region". The latter three names have an identical meaning. We recommend the most commonly used name "corotating interaction region" or CIR for sole usage in the literature to avoid confusion.
Received: 01 Jan 2026 – Discussion started: 30 Jan 2026
Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.
Bruce T. Tsurutani, Rajkumar Hajra, and Gurbax S. Lakhina
Metrics will be available soon.
Latest update: 30 Jan 2026
I understand the authors’ concern on the terminology confusions, as some authors use these two terms interchangeably (Waugh and Jardine, 2025). However, I’m not convinced with the authors’ current narratives. According to the modern studies, CIRs (coronating interacting regions) are used as subsets of SIRs (stream interacting regions). Allen et al. (2020) stated, “After a complete solar rotation, the SIR is classified as a corotating interaction region (CIR)”. Richardson (2018) uses “the general term “stream interaction region”, while being aware that some authors (e.g., Jian et al. 2006) use this term to distinguish a stream that is observed on only one solar rotation from a “corotating” interaction region that is seen on more than one rotation.” If the scientific community stops using the term of SIR, how would we call the CIRs that did not persist as long as one solar rotation? It’s straightforward to understand CIRs as a subset of SIRs.