[Retracted] On the Geoeffectiveness Structure of Solar Wind-Magnetosphere Coupling Functions during Intense Storms

Figure 4

Regression plots of 𝐵 with some commonly used coupling functions for the Solar Wind-Magnetosphere Interaction (according to [1] and the references therein) for the intense storms under investigation: (a) 𝑉𝐵_𝑇, (b) 𝐵_𝑧𝑉², (c) 𝐵_𝑧×𝑉, and (d) 𝐵_𝑧2𝑉.

(a)

(b)

(c)

(d)