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Parhelic
Circle at the South Pole imaged
by Marko Riikonen 11th January 1999 at 0500hrs. The parhelic
circle swings through the 22° high sun, brightens outside the
sundogs and hugs the flat horizon everywhere at the same height. Image ©Marko
Riikonen. |
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Parhelic Circle
for 22° high sun
Sweeping around the horizon, the circle is not uniformly
bright. It is fainter through the sun and inside the sundogs where
it relies primarily on rays reflected externally.
The halo also becomes faint beyond the 120°
parhelia. At these
angles, internal reflections become less efficient.
HaloSim ray
tracing. Fisheye view centered on the zenith, 40% randomly oriented
columns to produce the 22° halo and 60% plate crystals with c/a=0.05. |
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Very low sun
Here the sun is only 5° above the horizon. Again, the parhelic
circle is faint beyond the 120° parhelia - then it brightens
again..
The two bright regions 150
to 160° from the sun are Liljequist parhelia first observed in
Antarctica by the Swedish meteorologist G.H. Liljequist. Almost perfect
hexagonal plate crystals are needed to form them. Their ray paths
involve two internal reflections. An example is a ray entering face
3, reflecting off faces 7 then 6 to exit through face 8 (path 3768
see face
number key). There is net refraction in this ray path and the
Liljequist parhelia are slightly coloured. |
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40° high sun
Contrast the parhelic circle as the sun climbs higher. The rays strike
internal vertical faces more obliquely and are more efficiently reflected.
The circle becomes more uniform. |
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