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2003 Halloween solar storms

From Wikipedia, the free encyclopedia
Series of intense solar storms in 2003

Halloween solar storms, 2003
Composite image showing aurorae over northern Europe, taken byDMSP on October 30, 2003
Associated solar active region
NOAA regionno.10486
Largest SXR flaresX40+
G5 "Extreme" geomagnetic storm
G-scale (NOAA/SWPC)
Initial onsetOctober 2003 (2003-10)
DissipatedNovember 2003 (2003-11)
PeakKp-index9
PeakAp-index204
PeakDst−383 nT
ImpactsElectrical faults and wear to various satellites; satellitecommunications blackouts; localizedpower outage inSweden

Part ofsolar cycle 23

TheHalloween solar storms were a series ofsolar storms involvingsolar flares andcoronal mass ejections that occurred from mid-October to early November 2003, peaking around October 28–29.[1][2][3] This series of storms generated the largest solar flare ever recorded by theGOES system, modeled as strong as X45 (initially estimated at X28 due to saturation of GOES' detectors).[4][5]

Effects

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On Earth

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Satellite-based systems and communications were affected, aircraft were advised to avoid high altitudes near thepolar regions,[6] and a one-hour-long power outage occurred inSweden as a result of the solar activity.[2]Aurorae were observed at latitudes as far south asTexas[2] and theMediterranean countries ofEurope.[6] Twelve transformers inSouth Africa were disabled and had to be replaced, despite the country's lowgeomagnetic latitude.[7]

On satellites and spacecraft

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TheSOHO satellite failed temporarily and theAdvanced Composition Explorer (ACE) was damaged by the solar activity.[2] Numerous other spacecraft were damaged or experienced downtime due to various issues. Some of them were intentionally put into safe mode in order to protect sensitive equipment.[6] Astronauts aboard theInternational Space Station (ISS) had to stay inside the more shielded parts of theRussian Orbital Segment to protect themselves against the increased radiation levels.[8]

Emissions from the CME were later observed by theMars Odyssey spacecraft orbitingMars,Ulysses spacecraft nearJupiter, and theCassini spacecraft en route toSaturn. In April 2004,Voyager 2 was also able to detect them as they reached the spacecraft.[8]

Analysis

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Various data recorded during the Halloween solar storms

One of the solar storms was compared by some scientists in its intensity to theCarrington Event of 1859.[9]

These events occurred duringsolar cycle 23, approximately three years after its peak in 2000, which was marked by another occurrence of solar activity known as theBastille Day event.

See also

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References

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  1. ^"The Magnetic Storm of Halloween 2003".United States Geological Survey: Science Features. October 15, 2013. RetrievedMay 15, 2014.
  2. ^abcd"NASA - Halloween Storms of 2003 Still the Scariest".NASA/SOHO. October 27, 2008. RetrievedMay 15, 2014.
  3. ^Balch, Christopher; et al. (2004).Service Assessment: Intense Space Weather Storms October 19 – November 07, 2003(PDF). NOAA Technical Memorandum. Silver Spring, MD: Department of Commerce.
  4. ^"2003 Halloween solar storms, sunspot region 2192". SpaceWeatherLive.com. October 28, 2014. RetrievedAugust 9, 2017.
  5. ^"Biggest ever solar flare was even bigger than thought".SpaceRef.com.American Geophysical Union. March 15, 2004. RetrievedAugust 9, 2017.
  6. ^abcNOAA Technical Memorandum OAR SEC-88: HALLOWEEN SPACE WEATHER STORMS OF 2003(PDF). Boulder, Colorado: NOAA Office of Oceanic and Atmospheric Research. June 2004. Archived fromthe original(PDF) on July 28, 2011.
  7. ^Solar storm risk to the north American electric grid(PDF). Lloyd's of London and Atmospheric and Environmental Research. Lloyd's of London. 2013. Archived fromthe original(PDF) on December 5, 2016. RetrievedJuly 31, 2019.
  8. ^abLevin, Eric (January 2, 2005)."2003 Halloween Storms Still Rock Solar System".Discover. RetrievedMay 15, 2014.
  9. ^Cid, Consuelo; E. Saiz; A. Guerrero; J. Palacios; Y. Cerrato (2015). "A Carrington-like Geomagnetic Storm Observed in the 21st Century".J. Space Weather Space Clim.5 (A16): A16.arXiv:1505.07028.Bibcode:2015JSWSC...5A..16C.doi:10.1051/swsc/2015017.S2CID 59019585.
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