Fig. 14
All-sky maps of the thermal emission from the interplanetary dust predicted by two meteoroid engineering models, assuming that their constituent particles are composed of iron. The reference frame is as in Fig. 12. The brightness is provided in units of MJy sterad-1 for the COBE waveband centered at 240 μm, and in units of μK for the Planck and WMAP wavebands.
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