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May 1921 geomagnetic storm

From Wikipedia, the free encyclopedia
Exceptionally powerful geomagnetic storm

May 1921 geomagnetic storm
Aurorae from the geomagnetic storm imaged by theLowell Observatory
Geomagnetic storm
Initial onset13 May 1921 (1921-05-13)
Dissipated15 May 1921 (1921-05-15)
LowestDst−907±132 nT
ImpactsSubstantial damage to overhead and underwatertelegraph equipment;electrical fires; localizedelectric grid interruptions

Part ofsolar cycle 15

The three-dayMay 1921 geomagnetic storm, also known as theNew York Railroad Storm, was caused by the impact of an extraordinarily powerfulcoronal mass ejection onEarth'smagnetosphere. It occurred on 13–15 May as part ofsolar 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 theMarch 1989 geomagnetic storm which interrupted electrical service to large parts of northeastern North America.[2]

Effects

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The storm's electrical current sparked a number of fires worldwide, including one nearGrand Central Terminal which made it known as the "New York Railroad Storm".[1] Contemporary scientists estimated the size of thesunspot (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 inNew York City, which was a center of telegraph activity as a railroad hub.[5]Auroras ("northern lights") appeared throughout the easternUnited 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 theSouthern Hemisphere.[9]

Comparison to other geomagnetic storms

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In space weather, thedisturbance storm time index (Dst index) is a measure often used for determining the intensity of solar storms. A negative Dst index means thatEarth'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, theCarrington Event of 1859 had a peak Dst estimated to be between−800 nT and−1750 nT.[11] TheMarch 1989 geomagnetic storm had a peak Dst index of −589 nT.[12]

See also

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References

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Footnotes

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  1. ^abcPhillips, Tony (May 12, 2020)."The Great Geomagnetic Storm of May 1921".spaceweather.com. RetrievedJune 1, 2020.
  2. ^Dr Tony Phillips (January 21, 2009)."Severe Space Weather - Social and Economic Impacts".NASA. RetrievedDecember 18, 2012.
  3. ^"Borealis Cause, Sun Spots, Will Diminish Today"(PDF).Chicago Daily Tribune. May 16, 1921. p. 4. Archived fromthe original(PDF) on August 12, 2014. RetrievedDecember 19, 2012.
  4. ^"Sun Spots Vanishing"(PDF).The Los Angeles Times. May 16, 1921. pp. 1 & 2. Archived fromthe original(PDF) on August 12, 2014. RetrievedDecember 19, 2012.
  5. ^"May 13, 1921 – The New York Railroad Storm".SolarStorms.org.Archived from the original on September 28, 2006. RetrievedMay 31, 2020.
  6. ^M. Hapgood (2019)."The great storm of May 1921: An exemplar of a dangerous space weather event".Space Weather.17 (7):950–975.Bibcode:2019SpWea..17..950H.doi:10.1029/2019SW002195.
  7. ^"Sunspot Aurora Paralyses Wires"(PDF).New York Times. May 15, 1921. pp. 1 & 3. Archived fromthe original(PDF) on October 22, 2013. RetrievedDecember 19, 2012.
  8. ^"Cables Damaged by Sunspot Aurora"(PDF).New York Times. May 17, 1921. pp. 1 & 4. Archived fromthe original(PDF) on August 12, 2014. RetrievedDecember 19, 2012.
  9. ^"Aurora Borealis".Hawera & Normanby Star. May 16, 1921. p. 8. RetrievedDecember 18, 2012.
  10. ^Jeffrey J. Love; Hisashi Hayakawa; Edward W. Cliver (2019)."Intensity and Impact of the New York Railroad Superstorm of May 1921".Space Weather.17 (8):1281–1292.Bibcode:2019SpWea..17.1281L.doi:10.1029/2019SW002250.
  11. ^"Near Miss: The Solar Superstorm of July 2012".NASA Science.Archived from the original on May 11, 2024. RetrievedMay 11, 2024.
  12. ^Boteler, D. H. (October 10, 2019)."A 21st Century View of the March 1989 Magnetic Storm".Space Weather.17 (10):1427–1441.Bibcode:2019SpWea..17.1427B.doi:10.1029/2019SW002278.ISSN 1542-7390.

Bibliography

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Solar atmosphere
Interplanetary space
Magnetosphere
Planetary atmosphere
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