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High-speed solar-wind streams and geospace interactions

Research output: Contribution to Journal/Magazine › Journal article › peer-review

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High-speed solar-wind streams and geospace interactions. / Kavanagh, Andrew; Denton, Michael.
In: Astronomy and Geophysics, Vol. 48, No. 6, 14.11.2007, p. 6.24-6.26.

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Harvard

Kavanagh, A & Denton, M 2007, 'High-speed solar-wind streams and geospace interactions', Astronomy and Geophysics, vol. 48, no. 6, pp. 6.24-6.26. https://doi.org/10.1111/j.1468-4004.2007.48624.x

APA

Kavanagh, A., & Denton, M. (2007). High-speed solar-wind streams and geospace interactions. Astronomy and Geophysics, 48(6), 6.24-6.26. https://doi.org/10.1111/j.1468-4004.2007.48624.x

Vancouver

Kavanagh A, Denton M. High-speed solar-wind streams and geospace interactions. Astronomy and Geophysics. 2007 Nov 14;48(6):6.24-6.26. doi: 10.1111/j.1468-4004.2007.48624.x

Author

Kavanagh, Andrew ; Denton, Michael. / High-speed solar-wind streams and geospace interactions. In: Astronomy and Geophysics. 2007 ; Vol. 48, No. 6. pp. 6.24-6.26.

Bibtex

@article{f172a998dd514255bf22d3c976b04e8d,
title = "High-speed solar-wind streams and geospace interactions",
abstract = "High-speed solar-wind streams emanate from solar coronal holes; the fast wind interacts with upstream slow streams producing regions of enhanced magnetic field strength and particle density that are known as co-rotating interaction regions. Due to the recurring nature of coronal holes near solar minimum, this results in periodic driving of the magnetosphere that can last for several days and input as much energy as a storm driven by a coronal mass ejection.",
author = "Andrew Kavanagh and Michael Denton",
year = "2007",
month = nov,
day = "14",
doi = "10.1111/j.1468-4004.2007.48624.x",
language = "English",
volume = "48",
pages = "6.24--6.26",
journal = "Astronomy and Geophysics",
issn = "1366-8781",
publisher = "Oxford University Press",
number = "6",

}

RIS

TY - JOUR

T1 - High-speed solar-wind streams and geospace interactions

AU - Kavanagh, Andrew

AU - Denton, Michael

PY - 2007/11/14

Y1 - 2007/11/14

N2 - High-speed solar-wind streams emanate from solar coronal holes; the fast wind interacts with upstream slow streams producing regions of enhanced magnetic field strength and particle density that are known as co-rotating interaction regions. Due to the recurring nature of coronal holes near solar minimum, this results in periodic driving of the magnetosphere that can last for several days and input as much energy as a storm driven by a coronal mass ejection.

AB - High-speed solar-wind streams emanate from solar coronal holes; the fast wind interacts with upstream slow streams producing regions of enhanced magnetic field strength and particle density that are known as co-rotating interaction regions. Due to the recurring nature of coronal holes near solar minimum, this results in periodic driving of the magnetosphere that can last for several days and input as much energy as a storm driven by a coronal mass ejection.

U2 - 10.1111/j.1468-4004.2007.48624.x

DO - 10.1111/j.1468-4004.2007.48624.x

M3 - Journal article

VL - 48

SP - 6.24-6.26

JO - Astronomy and Geophysics

JF - Astronomy and Geophysics

SN - 1366-8781

IS - 6

ER -