Bastille Day solar storm explained

Bastille Day solar storm
G-Impacts:Minor satellite and terrestrial power transformer damage
Solar-Cycle:23
Dst:−301 nT
K-Index:9
A-Index:164
G-Scale:5
Ar-Sxr-Flares:X5.7
Noaa:9077

The Bastille Day solar storm was a powerful solar storm on 14–16 July 2000 during the solar maximum of solar cycle 23. The storm began on the national day of France, Bastille Day. It involved a solar flare, a solar particle event, and a coronal mass ejection which caused a severe geomagnetic storm.[1]

Overview

Solar flare and particle event

On 14 July 2000 from about 10:03 to 10:43 UTC, GOES satellites detected a very strong, X5.7-class, solar flare which peaked in soft X-ray intensity at around 10:24 UTC. This flare originated from the solar active region AR9077 which was located near the center of the Sun's disk (N22 W02) at the time of the flare.[2]

Starting at around 10:41 UTC, GOES satellites began detecting a strong, S3, solar particle event associated with the ongoing X5.7-class flare.[3] This resulted in high energy protons penetrating and ionizing parts of the Earth's ionosphere and creating noise in various satellite imaging systems such as in the EIT and LASCO instruments.[4] Some of these particles had sufficient energy to generate effects measured on Earth's surface, an event referred to as a ground level enhancement. Although the flare was not extremely large, the associated solar particle event was the fourth largest since 1967.[5]

Geomagnetic storm

The detection of the solar flare was also followed by the detection of a halo, or Earth-directed, coronal mass ejection (CME) in coronagraph data starting at 10:54 UTC. This CME reached Earth on 15 July causing a geomagnetic storm on 15–16 July which would reach a peak Kp index of 9+ in the late hours of 15 July corresponding to an extreme-level, or G5, geomagnetic storm and register a peak Dst of −301 nT. The storm caused minor damage to power transformers and satellites.[6] It was also one of only three solar storms having registered a maximum Kp of 9+ since the March 1989 geomagnetic storm, the others being the 2003 Halloween solar storms and the May 2024 solar storms.[7]

Aftermath

Due to being the first major solar storm since the launch of various solar-monitoring satellites, the Bastille Day event proved important towards helping scientists piece together a general theory of how eruptions on the sun occur as well as protecting the Earth from a larger event, such as a Carrington-class event, some day in the future.[8]

Despite their great distance from the Sun, the Bastille Day event was observed by Voyager 1 and Voyager 2.[9]

See also

External links

Notes and References

  1. News: NASA Says Solar Flare Caused Radio Blackouts . Associated Press . . 2000-07-14 . 2007-03-09 .
  2. Reiner . M.J. . Kaiser . M.L. . Karlický . M. . Jiřička . K. . Bougeret . J.-L. . Bastille Day Event: A Radio Perspective . Solar Physics . 2001 . 204 . 121–137 . 10.1023/A:1014225323289. 2001SoPh..204..121R . 133879595 .
  3. News: Space Radiation Storm . 2004-07-14 . NASA . https://web.archive.org/web/20000815063350/http://science.nasa.gov/headlines/y2000/ast14jul_2m.htm . dead . 2000-08-15 . 2007-03-09 .
  4. Andrews . M.D. . Lasco and eit Observations of the Bastille day 2000 Solar Storm . Solar Physics . 2001 . 204 . 179–196 . 10.1023/A:1014215923912. 2001SoPh..204..179A . 118618198 .
  5. The Bastille Day (14 July 2000) event in historical large sun-earth connection events . January 2001 . 10.1023/A:1014273227639 . 2 January 2021. Watari . Shinichi . Kunitake . Manabu . Watanabe . Takashi . Solar Physics . 204 . 425–438 . 2001SoPh..204..425W . 117394988 .
  6. Web site: Minor Damage Reported from Geomagnetic Storm. 2 January 2021.
  7. Web site: Top 50 Geomagnetic Storms . 2 January 2021.
  8. News: Moskowitz . Clara . Bastille Day Solar Storm: Anatomy of a Gargantuan Sun Tempest . 2 January 2021 . 14 July 2011.
  9. Webber . W. R. . McDonald . F. B. . Lockwood . J. A. . Heikkila . B. . The effect of the July 14, 2000 "Bastille Day" solar flare event on >70 MeV galactic cosmic rays observed at V1 and V2 in the distant heliosphere . Geophysical Research Letters . 15 May 2002 . 29 . 10 . 15–1–15-3 . 10.1029/2002GL014729 . 115950366 . free . 2002GeoRL..29.1377W .