UK halo display 9th February 2001 | |||
Photographs | HALO site |
HALO3 simulation of
the rare UK display. The sun is below centre inside the bright
circular 22° halo.
30
million virtual light rays were traced through mathematical representations of
the cloud ice crystals to
make this view
as would be photographed by a wide angle camera.
Halos, produced by hexagonal shaped ice crystals in
clouds, are visible once or twice a week on
average.
These are usually sundogs and fragments of a
22° radius circular halo around the sun. In complex
displays
a whole variety of bright and colourful arcs
spread across the sky including ones rarely seen. In the
UK
these displays are few and far between but one was
visible over the Midlands and Northern England
on
Friday 9th February .
The sightings of common and rare halo arcs were:
Observer | Location | Time | Arcs visible | ||
Malcolm Garland | Sheffield | 12.40 - 13.10 | 1 2 4 5 6 7 8 | ||
Malcolm Goldsmith | Prestwich, Manchester | 10.30 &13.30 | 2 10 | ||
Gill Smith | Ashberry near Rievaulx Abbey, Yorkshire | 13.30 - 14.00 | 1 2 3 4 5 7 9 | ||
Ant Veal et.al. | Birmingham | 11.45 - 12.40 | 1 2 3 4 5 9 10 | ||
Tony Young | Derby | 12.00 - 13.15 | 1 2 4 5 6 7 |
The halos:
Key | Name | Cloud crystals | ||||
1 |
22° halo |
poorly oriented crystals |
Weak in display |
|||
2 | 22° sundogs (parhelia) | hexagonal plates |
||||
3 | Circumzenithal arc | plates |
||||
4 | Upper tangent arc | horizontal columns |
Extremely bright and coloured | |||
5 | Parhelic circle | plates
& columns |
||||
6 | Sun pillar | plates & columns | Not often seen when the sun is so high.
Probably made by the large numbers of column crystals. |
|||
7 | 46° halo | poorly oriented | Rare and colourful halo - see supralateral
arc. |
|||
8 | 120° parhelia | plates | Produced by multiple reflections inside plate
crystals. |
|||
9 | Parry arc | Parry columns | Rare halo first seen by Parry in 1820 while
icebound in the Arctic. |
|||
10 | Supralateral arc | columns | The sun was 18 to 22° high and these altitudes
it can be difficult to distinguish between partial supralateral arcs and 46° halo fragments. Crystals capable of generating each were present but the hexagonal columns which generate supralateral arcs were most abundant. |