Fig. 14
From: Heliocentric distance dependence of zodiacal light observed by Hayabusa2#
Diffuse Galactic Light. Left: DGL image for the field of 2021–08-23 based on the SFD map at \(\lambda =\)100 \(\mu\)m (Schlegel et al. 1998). Center: DGL image for the same field based on the AKARI Wide-S map at \(\lambda =\)90 \(\mu\)m (Doi et al. 2015; Takita et al. 2015) after masking the point sources. Right: Comparison of the intensities from the SFD map and the AKARI Wide-S map of our observation fields. The red line shows the best fit to this correlation