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Table 2

Observation geometry of Saturn for the various epochs at mid-observation.

Window 1: July 2011

Date θ λobs φobs λ φ NP LS

2011-07-12 13:25:00 17.06 83.95 9.43 78.43 12.57 356.79 23.41

Window 2: February 2012

Date θ λobs φobs λ φ NP LS

2012-02-02 00:32:00 17.62 245.72 18.41 251.20 15.85 358.57 30.05
2012-02-02 22:01:00 17.65 251.56 18.41 257.02 15.86 358.57 30.08

Window 3: July–August 2012

Date θ λobs φobs λ φ NP LS

2012-07-29 17:25:00 16.73 60.70 15.84 55.10 18.51 357.96 35.79
2012-08-10 18:17:00 16.42 97.90 16.25 92.64 18.68 358.03 36.18

Window 4: January–February 2013

Date θ λobs φobs λ φ NP LS

2013-01-30 03:47:00 17.02 180.70 23.25 186.49 21.05 359.86 41.63
2013-02-02 06:37:00 17.11 188.94 23.27 194.74 21.09 359.87 41.76

Notes. Saturn’s equatorial angular diameter, given in arcsec as seen from Herschel, is represented by θ. λobs and φobs are the longitude and latitude (respectively) of the sub-observer point. λ and φ are the longitude and latitude (respectively) of the sub-solar point. NP is the North Polar angle in degrees, and LS is Saturn’s solar longitude in degrees. The different values are extracted from JPL/Horizons.

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