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Reconstructing Sunspot Number by Forward-Modelling Open Solar Flux
Mathew J. Owens, Mike Lockwood, Luke A. Barnard, Ilya Usoskin, Hisashi Hayakawa, Benjamin J. S. Pope and Ken McCracken Solar Physics 299(1) (2024) https://doi.org/10.1007/s11207-023-02241-3
Annual Variations in the Near-Earth Solar Wind
Mathew J. Owens, Mike Lockwood, Luke A. Barnard, Stephanie L. Yardley, Heli Hietala, Adrian T. LaMoury and Laura Vuorinen Solar Physics 298(9) (2023) https://doi.org/10.1007/s11207-023-02193-8
Application of historic datasets to understanding open solar flux and the 20th-century grand solar maximum. 1. Geomagnetic, ionospheric, and sunspot observations
The Development of a Space Climatology: 3. Models of the Evolution of Distributions of Space Weather Variables With Timescale
Mike Lockwood, Sarah N. Bentley, Mathew J. Owens, Luke A. Barnard, Chris J. Scott, Clare E. Watt, Oliver Allanson and Mervyn P. Freeman Space Weather 17(1) 180 (2019) https://doi.org/10.1029/2018SW002017
Revisiting Kunitomo’s Sunspot Drawings During 1835 – 1836 in Japan
The Development of a Space Climatology: 2. The Distribution of Power Input Into the Magnetosphere on a 3‐Hourly Timescale
Mike Lockwood, Sarah N. Bentley, Mathew J. Owens, Luke A. Barnard, Chris J. Scott, Clare E. Watt, Oliver Allanson and Mervyn P. Freeman Space Weather 17(1) 157 (2019) https://doi.org/10.1029/2018SW002016
Hourly weather observations from the Scottish Highlands (1883–1904) rescued by volunteer citizen scientists
Ed Hawkins, Stephen Burt, Philip Brohan, Michael Lockwood, Harriett Richardson, Marjory Roy and Simon Thomas Geoscience Data Journal 6(2) 160 (2019) https://doi.org/10.1002/gdj3.79
The Development of a Space Climatology: 1. Solar Wind Magnetosphere Coupling as a Function of Timescale and the Effect of Data Gaps
Mike Lockwood, Sarah N. Bentley, Mathew J. Owens, Luke A. Barnard, Chris J. Scott, Clare E. Watt and Oliver Allanson Space Weather 17(1) 133 (2019) https://doi.org/10.1029/2018SW001856
Ion Charge States and Potential Geoeffectiveness: The Role of Coronal Spectroscopy for Space‐Weather Forecasting