She and William were on a low pair of lounge chairs at a distance from his.
It is more complicated than simply using only the low pair vector differences to make models since the complementary data set (the low pair vector sums) is needed in order to resolve other field constituents.
Equation (B.17) holds when the Swarm satellite low pair positions are aligned in an approximately east-west orientation, which is true for low-mid latitudes.
In the statistical SW correlative study, this is manifested as generally low paired correlation coefficient values (CC < ~0.5) with individual solar wind parameters, showing comparable statistical contributions of dayside merging electric field E kl and solar wind dynamic pressure.
If the positions of the Swarm satellite low pair differ only in longitude by Δϕ, then the difference in potentials at (r, θ, ϕ) is given by (B.14 where is the set of modified coefficients.
Similarly, the Swarm low pair vector sums in Eq. (B.17) become exclusive functions of ΣVA in their and uDIF components since the second term has no contribution in these directions.
Let the Swarm low pair, denoted "A" and "B", be at positions (r, θ, ϕ) and (r, θ, ϕ + ϕ), respectively, where r, Ϙ, and ϕ are the radius, colatitude and longitude, respectively, and Δø is a longitude increment.
The Swarm constellation offers the ability of taking differences between the vector magnetometer measurements of the satellite low pair, which effectively eliminates most of the broad-scale external contamination, thus leading to a high SNR of the crustal field signal.
The matching index quantifies the overlap in afferent and efferent connections between two areas, and previous studies have suggested that areas with low pair-wise similarity in their patterns of afferents and efferents tend to have different functional properties [18].
