The 1859 space weather event revisited: limits of extreme activity

• Published in: Journal of space weather and space climate Vol. 3; p. A31
• Main Authors: Cliver, Edward W., Dietrich, William F.
• Format: Journal Article
• Language: English
• Published: les Ulis EDP Sciences 01.01.2013
• Subjects: Classification; Cosmic rays; Energy; extreme events; Geomagnetic storms; Geomagnetism; historical records; Magnetic storms; Needlework; Soft x rays; solar activity; Solar flares; Space weather; Storm index; Storms; Terrestrial environments; Weather
• ISSN: 2115-7251; 2115-7251
• DOI: 10.1051/swsc/2013053

The solar flare on 1 September 1859 and its associated geomagnetic storm remain the standard for an extreme solar-terrestrial event. The most recent estimates of the flare soft X-ray (SXR) peak intensity and Dst magnetic storm index for this event are: SXR class = X45 (±5) (vs. X35 (±5) for the 4 November 2003 flare) and minimum Dst = −900 (+50, −150) nT (vs. −825 to −900 nT for the great storm of May 1921). We have no direct evidence of an associated solar energetic proton (SEP) event but a correlation between >30 MeV SEP fluence (F30) and flare size based on modern data yields a best guess F30 value of ~1.1 × 1010 pr cm−2 (with the ±1σ uncertainty spanning a range from ~109–1011 pr cm−2) for a composite (multi-flare plus shock) 1859 event. This value is approximately twice that of estimates/measurements – ranging from ~5–7 × 109 pr cm−2 – for the largest SEP episodes (July 1959, November 1960, August 1972) in the modern era.