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Technical Note: Time-dependent limb-darkening calibration for solar occultation instruments

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Fig. 1. The time history of sunrise SAGE event at a single wave- wave-length (1020 nm in this example)
Fig. 2. A schematic of how the Sun appears to a SAGE instrument including to-scale representations of the field of view (FOV) for SAGE II and SAGE III
Fig. 4. An 865-nm image of the solar photosphere from the Gas and Aerosol Measurement Sensor, which flew aboard the NASA DC-8 aircraft during the SOLVE II campaign on 21 January 2003
Fig. 6. Transmission, calculated by normalizing the SAGE II mea- mea-surements against the exoatmospheric meamea-surements, and then  re-normalized for this experiment by dividing by an average  transmis-sion profile, is shown as a function of scan number
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