Table 1

Dipole contribution to the yearly change in auroral zone surface area. The first column indicates which dipolar coefficient each row refers to. SV coefficients β̇lm$ {\stackrel{\dot }{\beta }}_l^m$ are calculated as the yearly average over the 2015–2020 AD period from the IGRF-13 model, as in formula (4). The sensitivities Ai/βlm$ \partial {A}_i/\partial {\beta }_l^m$ are the same values as reported in Figure 3 (left panels). The temporal change contributions ∂Ai/∂t are obtained by multiplying Ai/βlm$ \partial {A}_i/\partial {\beta }_l^m$ with the corresponding β̇lm$ {\stackrel{\dot }{\beta }}_l^m$. The column-wise sum of the ∂Ai/∂t values agrees with the l = 1 value reported in Figure 4 (left panel).

β l m $ {\beta }_l^m$ β̇lm$ {\stackrel{\dot }{\beta }}_l^m$ [nT/year] AN/βlm$ \partial {A}_N/\partial {\beta }_l^m$ [km2/nT] AS/βlm$ \partial {A}_S/\partial {\beta }_l^m$ [km2/nT] AN/t$ \partial {A}_N/{\partial t}$ [km2/year] AS/t$ \partial {A}_S/{\partial t}$ [km2/year]
g 1 0 $ {g}_1^0$ 7.340 −1.339 −29.25 −9.825 −214.7
g 1 1 $ {g}_1^1$ 10.18 −26.67 226.2 −271.5 2303
h 1 1 $ {h}_1^1$ −28.70 37.86 −80.12 −1087 2299

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