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Equatorwards expansion of unperturbed, high-latitude fast solar wind

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Equatorwards expansion of unperturbed, high-latitude fast solar wind. / Dorrian, Gareth; Breen, Andy; Fallows, Richard; Bisi, Mario.

In: Solar Physics, Vol. 285, No. 1-2, 07.2013, p. 97-110.

Research output: Contribution to journalJournal articlepeer-review

Harvard

Dorrian, G, Breen, A, Fallows, R & Bisi, M 2013, 'Equatorwards expansion of unperturbed, high-latitude fast solar wind', Solar Physics, vol. 285, no. 1-2, pp. 97-110. https://doi.org/10.1007/s11207-012-0081-y

APA

Dorrian, G., Breen, A., Fallows, R., & Bisi, M. (2013). Equatorwards expansion of unperturbed, high-latitude fast solar wind. Solar Physics, 285(1-2), 97-110. https://doi.org/10.1007/s11207-012-0081-y

Vancouver

Author

Dorrian, Gareth ; Breen, Andy ; Fallows, Richard ; Bisi, Mario. / Equatorwards expansion of unperturbed, high-latitude fast solar wind. In: Solar Physics. 2013 ; Vol. 285, No. 1-2. pp. 97-110.

Bibtex

@article{3fdde909c6ba4aa19f9419d9f77a89fb,
title = "Equatorwards expansion of unperturbed, high-latitude fast solar wind",
abstract = "We use dual-site radio observations of interplanetary scintillation (IPS) with ex- tremely long baselines (ELB) to examine meridional flow characteristics of the ambient fast solar wind at plane-of-sky heliocentric distances of 24–85 solar radii (R⊙). Our results demonstrate an equatorwards deviation of 3 – 4◦ in the bulk fast solar wind flow direction over both northern and southern solar hemispheres during different times in the declining phase of Solar Cycle 23.",
author = "Gareth Dorrian and Andy Breen and Richard Fallows and Mario Bisi",
year = "2013",
month = jul,
doi = "10.1007/s11207-012-0081-y",
language = "English",
volume = "285",
pages = "97--110",
journal = "Solar Physics",
issn = "0038-0938",
publisher = "Springer Netherlands",
number = "1-2",

}

RIS

TY - JOUR

T1 - Equatorwards expansion of unperturbed, high-latitude fast solar wind

AU - Dorrian, Gareth

AU - Breen, Andy

AU - Fallows, Richard

AU - Bisi, Mario

PY - 2013/7

Y1 - 2013/7

N2 - We use dual-site radio observations of interplanetary scintillation (IPS) with ex- tremely long baselines (ELB) to examine meridional flow characteristics of the ambient fast solar wind at plane-of-sky heliocentric distances of 24–85 solar radii (R⊙). Our results demonstrate an equatorwards deviation of 3 – 4◦ in the bulk fast solar wind flow direction over both northern and southern solar hemispheres during different times in the declining phase of Solar Cycle 23.

AB - We use dual-site radio observations of interplanetary scintillation (IPS) with ex- tremely long baselines (ELB) to examine meridional flow characteristics of the ambient fast solar wind at plane-of-sky heliocentric distances of 24–85 solar radii (R⊙). Our results demonstrate an equatorwards deviation of 3 – 4◦ in the bulk fast solar wind flow direction over both northern and southern solar hemispheres during different times in the declining phase of Solar Cycle 23.

U2 - 10.1007/s11207-012-0081-y

DO - 10.1007/s11207-012-0081-y

M3 - Journal article

VL - 285

SP - 97

EP - 110

JO - Solar Physics

JF - Solar Physics

SN - 0038-0938

IS - 1-2

ER -