Instrument calibration of the Hayabusa near-infrared spectrometer

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Figure 8: Representative NIRS spectra obtained from in-flgith measurements: (a) Antares, (b)Jupiter, (c) Moon. The spectra used for comparison were taken by the ground-basedtelescopes (Lancon and Wood, 2000; Clark and McCord, 1979).Figure 9: The image of Moon taken by the AMICA shows the relative position of theindividual observation of NIRS. The number in NIRS FOV frames corresponds to that inFigure 8 respectively.20
Figure 10: Comparison of the derived geometric albedo of Itokawa between the NIRS andAMICA. The value at V-band (0.55 μm) has been estimated by AMICA (Ishiguro et al.,2007). As an intermediary the visible to near-infrared spectra of Itokawa obtained from theground-based observations by Binzel et al. (2001) and Tholen (2006) are plotted withnormalized at the value of AMICA’s V-band.21
Page 1 and 2: Instrument calibration of the Hayab
Page 3 and 4: AbstractThe Hayabusa Near-Infrared
Page 5 and 6: spacecraft chassis in such a way th
Page 7 and 8: (Figure 3), dark current characteri
Page 9 and 10: instruments slightly. Coalignment b
Page 11 and 12: Once spectra and images are calibra
Page 13 and 14: ReferencesAbe, M., Takagi, Y., Kita
Page 15 and 16: Table 1: NIRS SpecificationsCharact
Page 17 and 18: Figure 3: Spectral responsivity of
Page 19: Figure 7: Time series plots for (a)

Instrument calibration of the Hayabusa near-infrared spectrometer

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