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For field lines to return from the nightside, they must first disconnect from the solar wind.
The cross-tail structure with different flow bursts is demonstrated by Fig. 6, which shows the entropy integral S (color), defined by (1), for field lines crossing the z=0 plane at t=155 and t=185, together with velocity vectors and B z contours (solid black lines).
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The iterative process is illustrated in Table 1 for field line F6.
In this paper the SOAP technology is explained and is illustrated with a new service for field line tracing.
According to IMAGE data, Pc5 polarization pattern along a meridian does not correspond to that expected for field line resonance model.
A magnetic flux rope can be thought of as a locally cylindrical bundle of field lines that have a helical structure except for the axial field line.
For open field lines with A
There are no isolated poles to provide, as electric charges do, sources for the field lines.
The integral (1) was taken from one foot point at the left boundary to the other for closed field lines.
Fig. 1 a Analytic results for magnetic field lines of F t in the x y plane and pressure anisotropy α in color.
The twist T n was calculated for all field lines according to Eq. (56), and the result is shown in Fig. 7 c.
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