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Solar Zenith Angle (SZA)When observing a given point on the Earth's surface from a satellite-based instrument, the Solar Zenith Angle (SZA) is the angle between the local zenith (i.e. directly above the point on the ground) and the line of sight from that point to the sun. This means that the higher the Sun is in the sky, to lower the SZA is. The other angle in the graph, the angle between the local zenith and the line of sight to the satellite, is called the Viewing Zenith Angle.
The time SCIAMACHY passes a place overhead is always the same local time, as the satellite orbits the Earth in a so-called sun-synchronus orbit. If a satellite in a polar orbit flies over the pole into the sunlight, the SZA can be well above 100 degrees. The minimum SZA along the centre of an orbit is about 24 degrees. While orbiting on the sun-lit side of the Earth from North to South, SCIAMACHY scans from East to West, with on the East (West) side an SZA that is a little smaller (larger) than in the centre of the orbit.
Note that ENVISAT, the satellite that carries SCIAMACHY, passes the equator at 10:00 a.m. local solar time. For a given logitude the time in UTC is: UTC_time = local_solar_time - longitude/15For example the Galapagos Islands are at about the Equator at 90 degrees West. With local_solar_time of 10:00 this gives a UTC_time for the overpass of about 16:00.
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