Reconstruction of geomagnetic activity and near-Earth interplanetary conditions over the past 167 yr – Part 2: A new reconstruction of the interplanetary magnetic field

Lockwood, M. ORCID: https://orcid.org/0000-0002-7397-2172, Barnard, L., Nevanlinna, H., Owens, M.J. ORCID: https://orcid.org/0000-0003-2061-2453, Harrison, R.G. ORCID: https://orcid.org/0000-0003-0693-347X, Rouillard, A. P. and Davis, C. J. ORCID: https://orcid.org/0000-0001-6411-5649 (2013) Reconstruction of geomagnetic activity and near-Earth interplanetary conditions over the past 167 yr – Part 2: A new reconstruction of the interplanetary magnetic field. Annales Geophysicae, 31 (11). pp. 1979-1992. ISSN 0992-7689 doi: 10.5194/angeo-31-1979-2013

Abstract/Summary

We present a new reconstruction of the interplanetary magnetic field (IMF, B) for 1846–2012 with a full analysis of errors, based on the homogeneously constructed IDV(1d)composite of geomagnetic activity presented in Part 1 (Lockwood et al., 2013a). Analysis of the dependence of the commonly used geomagnetic indices on solar wind parameters is presented which helps explain why annual means of interdiurnal range data, such as the new composite, depend only on the IMF with only a very weak influence of the solar wind flow speed. The best results are obtained using a polynomial (rather than a linear) fit of the form B = χ · (IDV(1d) − β)α with best-fit coefficients χ = 3.469, β = 1.393 nT, and α = 0.420. The results are contrasted with the reconstruction of the IMF since 1835 by Svalgaard and Cliver (2010).

Item Type	Article
URI	https://reading-clone.eprints-hosting.org/id/eprint/35446
Item Type	Article
Refereed	Yes
Divisions	Science > School of Mathematical, Physical and Computational Sciences > Department of Meteorology
Publisher	Copernicus Publications
Publisher Statement	gold open access paper
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