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Rearrangement rates are larger, by a factor of about four, and occur over a wider range of conditions, if the proppant has migrated into a central sheet than if the solids distribution remains homogeneous.
In HadA, the helical axis is almost perpendicular to the vertical axis of the β-strands forming the central sheet.
A central sheet composed of five strands (β1 β5) is twisted to form a concave cavity at the center.
Notably, the length of all five β strands constituting the central sheet of HadA is longer than that of HadB.
Further, the loop connecting αHD with β2 of the central sheet in HadA (residue 76 84) is longer than that in HadB (residue 75 80) (Fig. 3C).
Within the structural framework of Cass2, a distinct loop feature extending from helix α2 edging the central sheet (residues 41 46) is proposed to undergo structural rearrangement so as to facilitate ligand entry.
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In this alignment the central β-sheets are closer in space, even though an alignment that simultaneously superimposes both the central sheets and the binding sites is not possible due to the above-mentioned permutation.
From the magnetic field B x and B z variations in Fig. 16, we can identify that Geotail transiently entered the central plasma sheet region because of plasma sheet oscillations.
The plasma in this cavity had characteristics similar to that of the central plasma sheet, possibly implying that the central plasma sheet had expanded over and subsequently receded back over the spacecraft.
Different from the classical Rossmann fold that has α-helices flanking the central β-sheet, the β-sheet in the N-lobe is flanked by α-helices (α1 4) at one side but the β-barrel at the other side.
BBF and dipolarization fronts in the central plasma sheet (CPS) produce transient ion beams accompanied by magnetic field disturbances in the near-Earth plasma sheet boundary layer (PSBL) (Zhou et al. 2012).
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