Space climate and space weather over the past 400 years: 1. The power input to the magnetosphere

@article{Lockwood2017SpaceCA,
  title={Space climate and space weather over the past 400 years: 1. The power input to the magnetosphere},
  author={Mike Lockwood and Mathew J. Owens and Luke A. Barnard and Chris J. Scott and Clare E. J. Watt},
  journal={Journal of Space Weather and Space Climate},
  year={2017},
  volume={7}
}
Using information on geomagnetic activity, sunspot numbers and cosmogenic isotopes, supported by historic eclipse images and in conjunction with models, it has been possible to reconstruct annual means of solar wind speed and number density and heliospheric magnetic field (HMF) intensity since 1611, when telescopic observations of sunspots began. These models are developed and tuned using data recorded by near-Earth interplanetary spacecraft and by solar magnetograms over the past 53 years. In… 
Space climate and space weather over the past 400 years: 2. Proxy indicators of geomagnetic storm and substorm occurrence
Using the reconstruction of power input to the magnetosphere presented in Paper 1 Lockwood  et al. [J Space Weather Space Clim 7 (2017a)], we reconstruct annual means of the geomagnetic Ap and AE
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The Development of a Space Climatology: 2. The Distribution of Power Input Into the Magnetosphere on a 3‐Hourly Timescale
Paper 1 in this series (Lockwood et al., 2018a, https://doi.org/10.1029/2018SW001856) showed that the power input into the magnetosphere Pα is an ideal coupling function for predicting geomagnetic
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