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   3rd & 4th Order Rainbows 

 

3rd & 4th order rainbows.
  

This BowSim simulation, made by tracing several hundred million rays through a raindrop, looks towards the sun.

On the left is an unfiltered view and all that can be seen is the white glare of the zero order glow surrounding the sun.

The filtered view at right shows only the rays making the 3rd order (inner) and 4th order (outer) rainbows.

   


Rays leaving raindrops after three reflections produce a tertiary rainbow. Unlike the primary and secondary bows which are opposite the sun and centered on the antisolar point, the tertiary appears sunwards and centered on the sun. With a nominal radius of 42.5º it is similar in size to, but very much broader than, the primary bow.

Why can we not see it?*   Its total brightness is 24% of the primary bow and we might think that it ought to be easily visible. There are two snags, its light is swamped by that of rays that pass through raindrops without any internal reflection. These generate an intense glare around the sun, the zero order glow that masks the tertiary. Another factor is that the tertiary is much broader than the primary and secondary, thus its luminosity per unit solid angle of sky is correspondingly less.

But perhaps not enough people have looked hard enough.**  Next time there is a rainbow, shield both your eyes very carefully from the sun and look for a 3rd order bow - of course, rain must be falling in that direction.

The 4th order bow (four internal reflections) is close to the 3rd order but with reversed colours. Its brightness is only 15% of that of the primary.
 

The 3rd and 4th order bows have never been photographed outdoors. 3rd and much higher order bows have been made visible in the laboratory by selectively illuminating a single suspended water drop with laser light.
** . There is a report of a sighting of the 3rd order bow made in Nairobi by D. E. Pegley and described in Weather 41, 401 (1986) and in John Naylor's book. "Whilst in Nairobi recently I had the good fortune to see a tertiary rainbow. On 21st May 1986 at 17.55 a new shower cloud had just started to rain out over my hotel in dense curtains of medium sized drops brilliantly lit by the low sun. From the balcony of my fourth floor room I could see not only a bright primary, accompanied by a moderate secondary, but also a weak bow in the direction of the sun, which was conveniently shielded by the side of the building. The bow was scintillating but distinct for two or three minutes. It was about the same size as the primary bow, with red on the outside and green on the inside."