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Earth, Planets and Space
Fig. 17 | Earth, Planets and Space

Fig. 17

From: Heliocentric distance dependence of zodiacal light observed by Hayabusa2#

Fig. 17

Field-variance correction. Left: ZL model brightness of the fields observed by Hayabusa2# (black) and toward the antisolar direction in the ecliptic plane (red) based on the Kelsall model (Kelsall et al. 1998) at 1.25 \(\mu\)m. A radial power-law profile with \(\alpha = 1.34\) is also shown. Right: Observed ZL brightness after subtracting the background components (black) and the corrected ZL brightness toward the antisolar direction in the ecliptic plane (red)

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