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Moreover, ground Pi2 onsets recur under low IMF clock angle conditions.
The dependence of LLBL thickness on IMF clock angle is discussed.
Thus, we also investigated the IMF clock angle dependence of properties of the airglow patches and related fast flows.
Fig. 5 IMF clock angle dependence of a maximum density, b density width, c flow width and d maximum velocity.
Figure 5a d shows the IMF clock angle dependence of the maximum density, flow channel width and maximum flow speed associated with the polar cap patches.
Most of the time interplanetary magnetic field (IMF) clock angle was less than 90°, rotating to more than 270° at the end of the interval, IMF Bx being positive and dominating.
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In these figures, clock angles are from 0° to 180° clockwise from top to bottom.
Angular coordinates of the MIPM reference frame (zenith and clock angles) correspond to those used in the geocentric interplanetary medium (GIPM) frame.
In particular, a square solar sail with a side length of 20m at 1au distance from the Sun is analyzed for different values of incidence and clock angles.
Taking into account the local time of but different, clock angles, and make a preliminary test of model predictions, using records from two ground magnetometer chains, both on the dayside.
Statistical study of beamlet occurrence frequency and their spatial distribution over the Neutral Sheet performed for different interplanetary conditions reveals that these distributions strongly depend on interplanetary magnetic field clock-angle.
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