May 1921 geomagnetic storm

May 1921 geomagnetic storm

Artist's depiction of solar wind striking Earth's magnetosphere (size and distance not to scale)
Geomagnetic storm
Initial onset	13 May 1921 (1921-05-13)
Dissipated	15 May 1921 (1921-05-15)
Peak Dst	−907±132 nT
Impacts	Substantial damage to overhead and underwater telegraph equipment; electrical fires; localized electric grid interruptions
Part of solar cycle 15

The three-day May 1921 geomagnetic storm, also known as the New York Railroad Storm, was caused by the impact of an extraordinarily powerful coronal mass ejection on Earth's magnetosphere. It occurred on 13–15 May as part of solar cycle 15, and was the most intense geomagnetic storm of the 20th century.^[1]

Since it occurred before the extensive interconnectivity of electrical systems and the general electrical dependence of infrastructure in the developed world, its effect was restricted; however, its ground currents were up to an order of magnitude greater than those of the March 1989 geomagnetic storm which interrupted electrical service to large parts of northeastern North America.^[2]

Effects

The storm's electrical current sparked a number of fires worldwide, including one near Grand Central Terminal which made it known as the "New York Railroad Storm".^[1] Contemporary scientists estimated the size of the sunspot (AR1842)^[1] which began on May 10—and caused the storm—as 151,000 by 34,000 km (94,000 by 21,000 miles).^[3][4]

The storm was extensively reported in New York City, which was a center of telegraph activity as a railroad hub.^[5] Auroras ("northern lights") appeared throughout the eastern United States, creating brightly lit night skies. Telegraph service in the U.S. first slowed and then virtually stopped at about midnight on 14 May due to blown fuses and damaged equipment.^[6] Radio propagation was enhanced during the storm due to ionosphere involvement, however, enabling unusually good long-distance reception. Electric lights were not noticeably affected.^[7]

Undersea telegraph cables were affected by the storm. Damage to telegraph systems was also reported in Europe^[8] and the Southern Hemisphere.^[9]

Comparison to other geomagnetic storms

In space weather, the disturbance storm time index (Dst index) is a measure often used for determining the intensity of solar storms. A negative Dst index means that Earth's magnetic field is weakened—particularly the case during solar storms—with a more negative Dst index indicating a stronger solar storm.

A paper in 2019 estimated that the May 1921 geomagnetic storm had a peak Dst of −907±132 nT.^[10]

For comparison, the Carrington Event of 1859 had a peak Dst estimated to be between −800 nT and −1750 nT.^[11] The March 1989 geomagnetic storm had a peak Dst index of −589 nT.^[12]

See also

• Active region
• Geomagnetic storm
• List of solar storms

References

Footnotes

Bibliography

• The Aurora Borealis of May 14, 1921 JSTOR 40710695
• "May 13, 1921 – The New York Railroad Storm". Solarstorms.org. Retrieved February 9, 2019. A bibliography of newspaper and journal articles.
• "Northern Lights Are Busy" (PDF). New York Times. May 14, 1921. p. 10. Archived from the original (PDF) on March 3, 2016. Retrieved December 19, 2012.
• "Aurora Borealis Halts Telegraph Service to City" (PDF). The Atlanta Constitution. May 15, 1921. p. 1. Archived from the original (PDF) on March 3, 2016. Retrieved December 19, 2012.
• Henry K. Bunn (May 15, 1921). "The Story The Week Has Told" (PDF). The Atlanta Constitution. p. 8. Archived from the original (PDF) on March 4, 2016. Retrieved December 19, 2012.
• "Tricky Aurora Snarls Up Wires" (PDF). Chicago Daily Tribune. May 15, 1921. p. 1. Archived from the original (PDF) on March 3, 2016. Retrieved December 19, 2012.
• "Aurora is Disturber" (PDF). The Los Angeles Times. May 15, 1921. pp. 1 & 2. Archived from the original (PDF) on March 3, 2016. Retrieved December 19, 2012.
• "The Aurora Borealis" (PDF). The Los Angeles Times. May 16, 1921. p. 14. Archived from the original (PDF) on March 3, 2016. Retrieved December 19, 2012.
• "Aurora Borealis Effect on Wires Laid to Sun Spot" (PDF). The Atlanta Constitution. May 16, 1921. p. 3. Archived from the original (PDF) on March 3, 2016. Retrieved December 19, 2012.
• "Sunspot Credited with Rail Tie-Up" (PDF). New York Times. May 16, 1921. p. 2. Archived from the original (PDF) on March 4, 2016. Retrieved December 19, 2012.
• "Magnetic Tremors Expected to Pass Within 48 Hours" (PDF). New York Times. May 16, 1921. p. 1. Archived from the original (PDF) on March 4, 2016. Retrieved December 19, 2012.
• "Cables Still Show Effects of Aurora" (PDF). New York Times. May 18, 1921. p. 12. Archived from the original (PDF) on March 3, 2016. Retrieved December 19, 2012.
• "Electric Disturbances Affect French Wires: Aurora Not Visible, Its Absence Being Attributed to Atmospheric Conditions" (PDF). New York Times. May 18, 1921. p. 12. Archived from the original (PDF) on March 4, 2016. Retrieved December 19, 2012.
• "Magnetic Storms Don't Affect Radio" (PDF). New York Times. May 26, 1921. p. 23. Retrieved December 19, 2012.^{[permanent dead link]}
• S.M. Silverman; E.W.Cliver (March 2001). "Low-latitude auroras: the magnetic storm of 14–15 May 1921". Journal of Atmospheric and Solar-Terrestrial Physics. 63 (5): 523–525. Bibcode:2001JASTP..63..523S. doi:10.1016/S1364-6826(00)00174-7. Retrieved December 18, 2012.

This page was last edited on 23 June 2024, at 05:35