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    Re: Lunars: Jupiter above the Moon
    From: Frank Reed CT
    Date: 2006 Jul 7, 16:53 -0500

    "How did you calculate and apply the flattening  of the sun?"
    
    You get the refraction for the altitude of the Sun's center  and then the
    refraction for that altitude plus the semi-diameter. The difference  tells you
    how much the Sun's semi-diameter will be shortened in the vertical  direction.
    Let's suppose it's 0.3'. Now if If the arc of the lunar distance was  vertical
    --Moon directly above the Sun-- that's the correction. If th arc is 45
    degrees away from vertical, the correction is half of this or 0.15'. In general,
    you multiply the vertical SD correction by the square of the cosine of the angle
     away from vertical. In practice, it is not even necessary to calculate that
    angle. You can estimate it when you take the sights to sufficient accuracy.
    Some  19th century tables included a simple look-up for this correction based
    on that  estimated angle. Since the Sun and Moon have nearly the same apparent
    diameter,  only one table is needed.
    
    -FER
    42.0N 87.7W, or 41.4N  72.1W.
    www.HistoricalAtlas.com/lunars
    
    
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