The development of reconstructions of annual means of near-Earth space conditions from observations of geomagnetic activity and from models using sunspot number observations as input
|From geomagnetic data||Modelled using sunspot data|
|Open Solar Flux (OSF), FS||Lockwood et al. (1999)||Solanki et al. (2000)|
|Owens and Lockwood (2012)|
|Photospheric flux||Solanki et al. (2002)|
|Vieira and Solanki (2010)|
|IMF field strength, B and Solar wind speed VSW||Svalgaard and Cliver (2005)|
|Rouillard et al. (2007)|
|Lockwood and Owens (2011)|
|Lockwood et al. (2014a)|
|Streamer Belt Width and OSF||Lockwood and Owens (2014)|
|IMF field strength, B||Owens et al. (2016a)||Owens et al. (2017)|
|Rahmanifard et al. (2017)|
|IMF field strength, B and||Owens et al. (2017)|
|Solar wind speed VSW|
|Solar wind number density, NSW|
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