The intensity and evolution of the extreme storms in January 1938

• Published in: arXiv.org
• Main Authors: Hayakawa, Hisashi, Hattori, Kentaro, Pevtsov, Alexei A, Ebihara, Yusuke, Shea, Margaret A, McCracken, Ken G, Daglis, Ioannis A, Bhaskar, Ankush, Ribeiro, Paulo, Knipp, Delores J
• Format: Paper Journal Article
• Language: English
• Published: Ithaca Cornell University Library, arXiv.org 29.10.2020
• Subjects: Auroras; Coronal mass ejection; Cosmic rays; Geomagnetism; Ground level; Ionization chambers; Latitude; Magnetic storms; Physics - Solar and Stellar Astrophysics; Physics - Space Physics; Solar corona; Solar protons; Solar storms; Storms; Sudden storm commencements
• ISSN: 2331-8422
• DOI: 10.48550/arxiv.2010.15762

Major solar eruptions occasionally direct interplanetary coronal mass ejections (ICMEs) to Earth and cause significant geomagnetic storms and low-latitude aurorae. While single extreme storms are of significant threats to the modern civilization, storms occasionally appear in sequence and, acting synergistically, cause 'perfect storms' at Earth. The stormy interval in January 1938 was one of such cases. Here, we analyze the contemporary records to reveal its time series on their source active regions, solar eruptions, ICMEs, geomagnetic storms, low-latitude aurorae, and cosmic-ray (CR) variations. Geomagnetic records show that three storms occurred successively on 17/18 January (Dcx ~ -171 nT) on 21/22 January (Dcx ~ -328 nT) and on 25/26 January (Dcx ~ -336 nT). The amplitudes of the cosmic-ray variations and sudden storm commencements show the impact of the first ICME as the largest (~ 6% decrease in CR and 72 nT in SSC) and the ICME associated with the storms that followed as more moderate (~ 3% decrease in CR and 63 nT in SSC; ~ 2% decrease in CR and 63 nT in SSC). Interestingly, a significant solar proton event occurred on 16/17 January and the Cheltenham ionization chamber showed a possible ground level enhancement. During the first storm, aurorae were less visible at mid-latitudes, whereas during the second and third storms, the equatorward boundaries of the auroral oval were extended down to 40.3{\deg} and 40.0{\deg} in invariant latitude. This contrast shows that the initial ICME was probably faster, with a higher total magnitude but a smaller southward component.