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Space- and ground-based investigations of solar wind-magnetosphere-ionosphere coupling

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

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Space- and ground-based investigations of solar wind-magnetosphere-ionosphere coupling. / Milan, S. E.; Wild, J. A.; Grocott, A. et al.
In: Advances in Space Research, Vol. 38, No. 8, 2006, p. 1671-1677.

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

Harvard

Milan, SE, Wild, JA, Grocott, A & Draper, NC 2006, 'Space- and ground-based investigations of solar wind-magnetosphere-ionosphere coupling', Advances in Space Research, vol. 38, no. 8, pp. 1671-1677. https://doi.org/10.1016/j.asr.2005.08.009

APA

Milan, S. E., Wild, J. A., Grocott, A., & Draper, N. C. (2006). Space- and ground-based investigations of solar wind-magnetosphere-ionosphere coupling. Advances in Space Research, 38(8), 1671-1677. https://doi.org/10.1016/j.asr.2005.08.009

Vancouver

Milan SE, Wild JA, Grocott A, Draper NC. Space- and ground-based investigations of solar wind-magnetosphere-ionosphere coupling. Advances in Space Research. 2006;38(8):1671-1677. doi: 10.1016/j.asr.2005.08.009

Author

Milan, S. E. ; Wild, J. A. ; Grocott, A. et al. / Space- and ground-based investigations of solar wind-magnetosphere-ionosphere coupling. In: Advances in Space Research. 2006 ; Vol. 38, No. 8. pp. 1671-1677.

Bibtex

@article{1833f4ad02244708b65366499971d57e,
title = "Space- and ground-based investigations of solar wind-magnetosphere-ionosphere coupling",
abstract = "This paper provides a brief review of the understanding of the coupled solar wind–magnetosphere–ionosphere system that can be attained from observations of the size of the ionospheric polar caps from space and the ground. These measurements allow the occurrence and rate of dayside and nightside reconnection to be deduced. The former can be correlated with upstream interplanetary magnetic field observations to give an estimate of the effective length of the dayside reconnection X-line. The latter allows a preli- minary statistical study of flux closure during substorms and other, smaller nightside reconnection events.",
keywords = "Solar wind–magnetosphere–ionosphere coupling, Magnetic reconnection, Substorms",
author = "Milan, {S. E.} and Wild, {J. A.} and A. Grocott and Draper, {N. C.}",
note = "The final, definitive version of this article has been published in the Journal, Advances in Space Research 38 (8), 2006, {\textcopyright} ELSEVIER.",
year = "2006",
doi = "10.1016/j.asr.2005.08.009",
language = "English",
volume = "38",
pages = "1671--1677",
journal = "Advances in Space Research",
issn = "0273-1177",
publisher = "Elsevier Ltd",
number = "8",

}

RIS

TY - JOUR

T1 - Space- and ground-based investigations of solar wind-magnetosphere-ionosphere coupling

AU - Milan, S. E.

AU - Wild, J. A.

AU - Grocott, A.

AU - Draper, N. C.

N1 - The final, definitive version of this article has been published in the Journal, Advances in Space Research 38 (8), 2006, © ELSEVIER.

PY - 2006

Y1 - 2006

N2 - This paper provides a brief review of the understanding of the coupled solar wind–magnetosphere–ionosphere system that can be attained from observations of the size of the ionospheric polar caps from space and the ground. These measurements allow the occurrence and rate of dayside and nightside reconnection to be deduced. The former can be correlated with upstream interplanetary magnetic field observations to give an estimate of the effective length of the dayside reconnection X-line. The latter allows a preli- minary statistical study of flux closure during substorms and other, smaller nightside reconnection events.

AB - This paper provides a brief review of the understanding of the coupled solar wind–magnetosphere–ionosphere system that can be attained from observations of the size of the ionospheric polar caps from space and the ground. These measurements allow the occurrence and rate of dayside and nightside reconnection to be deduced. The former can be correlated with upstream interplanetary magnetic field observations to give an estimate of the effective length of the dayside reconnection X-line. The latter allows a preli- minary statistical study of flux closure during substorms and other, smaller nightside reconnection events.

KW - Solar wind–magnetosphere–ionosphere coupling

KW - Magnetic reconnection

KW - Substorms

U2 - 10.1016/j.asr.2005.08.009

DO - 10.1016/j.asr.2005.08.009

M3 - Journal article

VL - 38

SP - 1671

EP - 1677

JO - Advances in Space Research

JF - Advances in Space Research

SN - 0273-1177

IS - 8

ER -