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Fig. 5. | Earth, Planets and Space

Fig. 5.

From: Solar wind electron interaction with the dayside lunar surface and crustal magnetic fields: Evidence for precursor effects

Fig. 5.

Selenographic map of the foot-point locations of electron observations (same data set as Figs. 13). Blue points indicate observations with no upward-going flux enhancement, green points indicate observations with apparent upward-going conics, and red points indicate observations with upward-going beams. Black contours show 10 nT, 20 nT, and 50 nT levels of surface crustal magnetic field magnitude.

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