The Development of a Space Climatology: 1. Solar Wind Magnetosphere Coupling as a Function of Timescale and the Effect of Data Gaps

Abstract

AbstractDifferent terrestrial space weather indicators (such as geomagnetic indices, transpolar voltage, and ring current particle content) depend on different coupling functions (combinations of near‐Earth solar wind parameters), and previous studies also reported a dependence on the averaging timescale, τ. We study the relationships of the am and SME geomagnetic indices to the power input into the magnetosphere Pα, estimated using the optimum coupling exponent α, for a range of τ between 1 min and 1 year. The effect of missing data is investigated by introducing synthetic gaps into near‐continuous data, and the best method for dealing with them when deriving the coupling function is formally defined. Using Pα, we show that gaps in data recorded before 1995 have introduced considerable errors into coupling functions. From the near‐continuous solar wind data for 1996–2016, we find that α = 0.44 ± 0.02 and no significant evidence that α depends on τ, yielding Pα∝B0.88Vsw1.90(mswNsw)0.23sin4(θ/2), where B is the interplanetary magnetic field, Nsw the solar wind number density, msw its mean ion mass, Vsw its velocity, and θ the interplanetary magnetic field clock angle in the geocentric solar magnetospheric reference frame. Values of Pα that are accurate to within ±5% for 1996–2016 have an availability of 83.8%, and the correlation between Pα and am for these data is shown to be 0.990 (between 0.972 and 0.997 at the 2σ uncertainty level), 0.897 ± 0.004, and 0.790 ± 0.03, for τ of 1 year, 1 day, and 3 hr, respectively, and that between Pα and SME at τ of 1 min is 0.7046 ± 0.0004.