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

doi:10.1007/s11207-010-9602-8

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. ShishovS. A. Tyul'Bashev, G. Agalya, S. K. Glubokova, M. S. Hamilton, K. Fujiki, P. P. Hick, J. M. Clover, B. Pintér

Department of Physics

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67 Citations (Scopus)

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 ageo-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 USNSF-sponsored Solar, Heliospheric, and Interplanetary Environment(SHINE) community investigation.

Original language	English
Pages (from-to)	49-127
Number of pages	79
Journal	Solar Physics
Volume	265
Issue number	1-2
DOIs	https://doi.org/10.1007/s11207-010-9602-8
Publication status	Published - 01 Aug 2010

Keywords

Active regions, magnetic fields
Corona, models
Corona, radio emission
Coronal mass ejections, initiation and propagation
Coronal mass ejections, interplanetary
Magnetic fields, interplanetary
Magnetic fields, models
Radio bursts, association with flares
Radio scintillation
Solar wind, disturbances
Sunspots, magnetic fields
Velocity fields, solar wind
X-ray bursts, association with flares

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http://adsabs.harvard.edu/abs/2010SoPh..265...49B

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Bisi, M. M., Breen, A. R., Jackson, B. V., Fallows, R. A., Walsh, A. P., Mikić, Z., Riley, P., Owen, C. J., Gonzalez-Esparza, A., Aguilar-Rodriguez, E., Morgan, H., Jensen, E. A., Wood, A. G., Owens, M. J., Tokumaru, M., Manoharan, P. K., Chashei, I. V., Giunta, A. S., Linker, J. A., ... Pintér, B. (2010). From the Sun to the Earth: The 13 May 2005 Coronal Mass Ejection. Solar Physics, 265(1-2), 49-127. https://doi.org/10.1007/s11207-010-9602-8

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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 ageo-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 USNSF-sponsored Solar, Heliospheric, and Interplanetary Environment(SHINE) community investigation.",

keywords = "Active regions, magnetic fields, Corona, models, Corona, radio emission, Coronal mass ejections, initiation and propagation, Coronal mass ejections, interplanetary, Magnetic fields, interplanetary, Magnetic fields, models, Radio bursts, association with flares, Radio scintillation, Solar wind, disturbances, Sunspots, magnetic fields, Velocity fields, solar wind, X-ray bursts, association with flares",

author = "Bisi, {M. M.} and Breen, {A. R.} and Jackson, {B. V.} and Fallows, {R. A.} and Walsh, {A. P.} and Z. Miki{\'c} and P. Riley and Owen, {C. J.} and A. Gonzalez-Esparza and E. Aguilar-Rodriguez and H. Morgan and Jensen, {E. A.} and Wood, {A. G.} and Owens, {M. J.} and M. Tokumaru and Manoharan, {P. K.} and Chashei, {I. V.} and Giunta, {A. S.} and Linker, {J. A.} and Shishov, {V. I.} and Tyul'Bashev, {S. A.} and G. Agalya and Glubokova, {S. K.} and Hamilton, {M. S.} and K. Fujiki and Hick, {P. P.} and Clover, {J. M.} and B. Pint{\'e}r",

year = "2010",

month = aug,

day = "1",

doi = "10.1007/s11207-010-9602-8",

language = "English",

volume = "265",

pages = "49--127",

journal = "Solar Physics",

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Bisi, MM, Breen, AR, Jackson, BV, Fallows, RA, Walsh, AP, Mikić, Z, Riley, P, Owen, CJ, Gonzalez-Esparza, A, Aguilar-Rodriguez, E, Morgan, H, Jensen, EA, Wood, AG, Owens, MJ, Tokumaru, M, Manoharan, PK, Chashei, IV, Giunta, AS, Linker, JA, Shishov, VI, Tyul'Bashev, SA, Agalya, G, Glubokova, SK, Hamilton, MS, Fujiki, K, Hick, PP, Clover, JM & Pintér, B 2010, 'From the Sun to the Earth: The 13 May 2005 Coronal Mass Ejection', Solar Physics, vol. 265, no. 1-2, pp. 49-127. https://doi.org/10.1007/s11207-010-9602-8

TY - JOUR

T1 - From the Sun to the Earth: The 13 May 2005 Coronal Mass Ejection

AU - Bisi, M. M.

AU - Breen, A. R.

AU - Jackson, B. V.

AU - Fallows, R. A.

AU - Walsh, A. P.

AU - Mikić, Z.

AU - Riley, P.

AU - Owen, C. J.

AU - Gonzalez-Esparza, A.

AU - Aguilar-Rodriguez, E.

AU - Morgan, H.

AU - Jensen, E. A.

AU - Wood, A. G.

AU - Owens, M. J.

AU - Tokumaru, M.

AU - Manoharan, P. K.

AU - Chashei, I. V.

AU - Giunta, A. S.

AU - Linker, J. A.

AU - Shishov, V. I.

AU - Tyul'Bashev, S. A.

AU - Agalya, G.

AU - Glubokova, S. K.

AU - Hamilton, M. S.

AU - Fujiki, K.

AU - Hick, P. P.

AU - Clover, J. M.

AU - Pintér, B.

PY - 2010/8/1

Y1 - 2010/8/1

N2 - 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 ageo-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 USNSF-sponsored Solar, Heliospheric, and Interplanetary Environment(SHINE) community investigation.

AB - 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 ageo-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 USNSF-sponsored Solar, Heliospheric, and Interplanetary Environment(SHINE) community investigation.

KW - Active regions, magnetic fields

KW - Corona, models

KW - Corona, radio emission

KW - Coronal mass ejections, initiation and propagation

KW - Coronal mass ejections, interplanetary

KW - Magnetic fields, interplanetary

KW - Magnetic fields, models

KW - Radio bursts, association with flares

KW - Radio scintillation

KW - Solar wind, disturbances

KW - Sunspots, magnetic fields

KW - Velocity fields, solar wind

KW - X-ray bursts, association with flares

UR - http://hdl.handle.net/2160/8311

U2 - 10.1007/s11207-010-9602-8

DO - 10.1007/s11207-010-9602-8

M3 - Article

SN - 0038-0938

VL - 265

SP - 49

EP - 127

JO - Solar Physics

JF - Solar Physics

IS - 1-2

ER -

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

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Keywords

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