Solar Physics

, Volume 265, Issue 1, pp 49–127

From the Sun to the Earth: The 13 May 2005 Coronal Mass Ejection

  • M. M. Bisi
  • A. R. Breen
  • B. V. Jackson
  • R. A. Fallows
  • A. P. Walsh
  • Z. Mikić
  • P. Riley
  • C. J. Owen
  • A. Gonzalez-Esparza
  • E. Aguilar-Rodriguez
  • H. Morgan
  • E. A. Jensen
  • A. G. Wood
  • M. J. Owens
  • M. Tokumaru
  • P. K. Manoharan
  • I. V. Chashei
  • A. S. Giunta
  • J. A. Linker
  • V. I. Shishov
  • S. A. Tyul’bashev
  • G. Agalya
  • S. K. Glubokova
  • M. S. Hamilton
  • K. Fujiki
  • P. P. Hick
  • J. M. Clover
  • B. Pintér
Open AccessRemote Sensing of the Inner Heliosphere

DOI: 10.1007/s11207-010-9602-8

Cite this article as:
Bisi, M.M., Breen, A.R., Jackson, B.V. et al. Sol Phys (2010) 265: 49. doi:10.1007/s11207-010-9602-8

Abstract

We report the results of a multi-instrument, multi-technique, coordinated study of the solar eruptive event of 13 May 2005. We discuss the resultant Earth-directed (halo) coronal mass ejection (CME), and the effects on the terrestrial space environment and upper Earth atmosphere. The interplanetary CME (ICME) impacted the Earth’s magnetosphere and caused the most-intense geomagnetic storm of 2005 with a Disturbed Storm Time (Dst) index reaching −263 nT at its peak. The terrestrial environment responded to the storm on a global scale. We have combined observations and measurements from coronal and interplanetary remote-sensing instruments, interplanetary and near-Earth in-situ measurements, remote-sensing observations and in-situ measurements of the terrestrial magnetosphere and ionosphere, along with coronal and heliospheric modelling. These analyses are used to trace the origin, development, propagation, terrestrial impact, and subsequent consequences of this event to obtain the most comprehensive view of a geo-effective solar eruption to date. This particular event is also part of a NASA-sponsored Living With a Star (LWS) study and an on-going US NSF-sponsored Solar, Heliospheric, and INterplanetary Environment (SHINE) community investigation.

Keywords

Active regions, magnetic fieldsCorona, modelsCorona, radio emissionCoronal mass ejections, initiation and propagationCoronal mass ejections, interplanetaryMagnetic fields, interplanetaryMagnetic fields, modelsRadio bursts, association with flaresRadio scintillationSolar wind, disturbancesSunspots, magnetic fieldsVelocity fields, solar windX-ray bursts, association with flares
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Copyright information

© The Author(s) 2010

Authors and Affiliations

  • M. M. Bisi
    • 1
    • 2
  • A. R. Breen
    • 2
  • B. V. Jackson
    • 1
  • R. A. Fallows
    • 2
  • A. P. Walsh
    • 4
  • Z. Mikić
    • 5
  • P. Riley
    • 5
  • C. J. Owen
    • 4
  • A. Gonzalez-Esparza
    • 6
  • E. Aguilar-Rodriguez
    • 6
  • H. Morgan
    • 7
  • E. A. Jensen
    • 8
    • 9
  • A. G. Wood
    • 2
  • M. J. Owens
    • 2
    • 3
  • M. Tokumaru
    • 10
  • P. K. Manoharan
    • 11
  • I. V. Chashei
    • 12
  • A. S. Giunta
    • 13
    • 14
  • J. A. Linker
    • 5
  • V. I. Shishov
    • 12
  • S. A. Tyul’bashev
    • 12
  • G. Agalya
    • 11
  • S. K. Glubokova
    • 12
    • 15
  • M. S. Hamilton
    • 1
  • K. Fujiki
    • 10
  • P. P. Hick
    • 1
    • 16
  • J. M. Clover
    • 1
  • B. Pintér
    • 2
  1. 1.Center for Astrophysics and Space SciencesUniversity of California, San DiegoLa JollaUSA
  2. 2.Institute of Mathematics and PhysicsAberystwyth UniversityAberystwythWales, UK
  3. 3.Space Environment Physics Group, Department of MeteorologyUniversity of ReadingReadingEngland, UK
  4. 4.Mullard Space Science LaboratoryUniversity College LondonDorkingEngland, UK
  5. 5.Predictive Science, Inc.San DiegoUSA
  6. 6.MEXART, Instituto de Geofisica, Unidad MichoacánUniversidad Nacional Autonoma de MexicoMoreliaMexico
  7. 7.Institute for AstronomyUniversity of HawaiiHonoluluUSA
  8. 8.ACS ConsultingHoustonUSA
  9. 9.MMT ObservatoryAmadoUSA
  10. 10.Solar-Terrestrial Environment Laboratory (STELab)Nagoya UniversityNagoyaJapan
  11. 11.Radio Astronomy Centre, National Centre for Radio AstrophysicsTata Institute of Fundamental ResearchUdhagamandalam (Ooty)India
  12. 12.Pushchino Radio Astronomy Observatory, Astrospace CenterLebedev Physical InstitutePushchinoRussia
  13. 13.Department of PhysicsUniversity of StrathclydeGlasgowScotland, UK
  14. 14.Space Science and Technology DepartmentRutherford Appleton LaboratoryDidcotEngland, UK
  15. 15.Pushchino State UniversityPushchinoRussia
  16. 16.San Diego Supercomputer CenterUniversity of California, San DiegoLa JollaUSA