Thursday, 15 January 2026

Review of the Rovaniemi 2023-11-11 Display and further research on the MS halos in the Borlänge and Naapurinvaara Displays

 

©Marko Riikonen


The Rovaniemi Display of November 11, 2023 – possibly one of the greatest and most bizarre Super Displays ever – a sentiment Marko and I both share. I was deeply fascinated by it when Marko first posted it.

 

https://www.taivaanvahti.fi/observations/show/119911
https://x.com/RiikonenMarko/status/1871867455959707898

 

Above are the original publication, along with additional photos and simulations uploaded by Marko at the end of 2024. In private correspondence with me, Marko mentioned that the identification of the 24d Column Arcs came from a suggestion by Nicolas Lefaudeux. The previous work of Nicolas and Marko has already addressed the simulation for most of the halos observed in this event.

 

However, previous simulations failed to match some halos in the photographs – for instance, the peculiar '35d Spot'. Some of the mysterious puzzles revealed in this event still require further exploration by halo experts and enthusiasts.





'35d Spot' is not at 35 degrees !

 

Ice crystals that produce 24d Column/Plate Arcs theoretically also produce 35d Column/Plate Arcs. But the problem is that the so-called '35d Spot' observed in this event does not align with the theoretical positions of 35d Column/Plate Arcs – it is clearly much closer to the light source.

 

Precise measurements show that the inner edge (closer side from the light source) of the '35d Spot' is about 32°, and the outer edge (farther side from the light source) is about 38°. Obviously, based on measurement result, they are not 35d Column/Plate/Parry Arcs. Some other types of halo must be present and is the main contributor to this strange bright paire of spots.



I also tried exotic pyramid crystals (Miller indices: 3 0 -3 2, 1 0 -1 2, 2 0 -2 1, 2 0 -2 3, 3 0 -3 4, 2 0 -2 5, and 1 0 -1 3), but none provided the correct answer. Perhaps the approach using exotic pyramid crystals was wrong from the start, because even if some special crystals that haven't been found in atmospheric samples can form 32° radius halos, it would be difficult for us to ignore the other halos that would accompany them.

 

Despite many failures, I have recently found a better answer – The 22° Parhelia of the 22° Column Arc.






 

 

The first record of '22° Parhelia of the 22° Column Arc' ?

 

Multiple Scattering(MS) halos from 3-5 ray paths will be closer to the light source than 35d Column/Plate/Parry Arcs. However, differences in the order of 'the first/second type of crystals'  can lead to different halo manifestations. I tested various combinations, and ultimately concluded that only the '22° Parhelia of the 22° Column Arc' provided the best match. The '22° Column Arcs of the 22° Parhelia' were ruled out due to unsatisfactory position and shape. MS halos related to the Parry arcs were eliminated because they were too sharp and also ill-positioned.





 

The second scene taken by Marko also supports this conclusion. In this scene the camera pointed towards the zenith, and Marko had stacked the images, which is more conducive to revealing the ideal morphological characteristics of halos than a single image. 





Precise alignment work showed that the '22° Parhelia of the 22° Column Arc' once again performed very well. This time, even without the contribution of 35d Column Arcs, the '22° Parhelia of the 22° Column Arc' alone aligned the shape/position of the '35d spots' in the stack-image very well.


 




So, did Marko capture another Borlänge Arc? No. I suggest that the situation in Rovaniemi on 2023-11-11 was completely different from the Borlänge Display, Sweden, 2018-12-14.

 

Previously, on Taivaanvahti or TheHaloVault, the Borlänge Arcs were defined as a combination of both the '22° Parhelia of the 22° Column Arc' and '22° Column Arcs of the 22° Parhelia'. This conclusion is likely based on simlations in Halopoint. However, this might be incorrect.

 

https://www.taivaanvahti.fi/observations/show/79745
https://thehalovault.blogspot.com/2018/12/complex-halo-display-borlange-sweden.html

 

After using Zhang Jia Jie's program for further research, we can see the differences – the position and shape of the MS halos in Borlänge and Rovaniemi Displays are not the same. In the Borlänge Display, people likely only observed the '22° Column Arcs of the 22° Parhelia', with the '22° Parhelia of the 22° Column Arc' either not being a major contributor or not appearing at all.




 

A similar conclusion applies to the Naapurinvaara Display in Sotkamo, Finland, on November 25, 2020. Simulation results suggest that the main contributor among the MS halos were the '22° Parhelia of the 22° Column/Parry Arc', not the 22° Column/Parry Arcs of the 22° Parhelia. The situation in Kuopio, Finland, on November 20, 2022, was the same.

 

https://www.taivaanvahti.fi/observations/show/95033
https://thehalovault.blogspot.com/2020/12/two-years-ago-halo-community-got-its.html?m=1

 





I'm unsure if there are other records of Borlänge Arcs around the world. The halo community can help verify this. If there has been no prior confirmed record of the '22° Parhelia of the 22° Column Arc', what Marko captured may very well be the first record of this phenomenon.

 




 

A proposal to redefine the Borlänge arc

 

It was previously widely believed that both of the '22° Column Arcs of the 22° Parhelia' and the '22° Parhelia of the 22° Column Arc' should appear together, which if why the Borlänge Arcs were defined as a mixture of two halo phenomena. But now, should we consider the case of 'only one of them appears alone' – in such cases, they no longer fit the name 'Borlänge Arcs'. Jokingly speaking: a rock band typically has 3, 4 or 5 members; when one member appears alone, they cannot be fully equated with the entire band.

 

To me, instead of creating two new names for the '22° Parhelia of the 22° Column Arc' and the '22° Column Arcs of the 22° Parhelia', it might be better to redefine Borlänge Arcs to apply only to the '22° Column Arcs of the 22° Parhelia'. This way, we only need one new name – a dedicated name for the '22° Parhelia of the 22° Column Arc'. Similar work also applies to redefine the Naapurinvaara Arc.

 

So, what should the new name be? Riikonen Arc? - that name has already been used for another halo. Perhaps Rovaniemi Arc is a name worth considering, or perhaps we should strictly name these MS halos according to their ray paths? In any case, Marko told me he has an article on halo nomenclature ready for publication, perhaps we will find better solutions for above discussions in his article.

 




8 comments:

  1. nicolas lefaudeux19 January 2026 at 14:05

    that is very interesting. i must say that i am not fully convinced about MS halo for the 35deg spot. there are 2 reasons:
    - the order of magnitude of the brightness of the spot does not seem to fit the MS. for instance, if the halo is parhelia of tanarc, the ratio between the brightness of tanarc and 35d spot should be roughly similar as the ratio between the brightness of parhelia vs lamp. here, although the tanarc is bright, it is nowhere as blinding as the lamp compared to the 35d spot.
    - divergence of the lamp beam is not negligible. for instance, parhelia and tanarc have both notable extensions toward lamp. the same would happen with 35d column of plate arcs. so the fact that the 35d plate/column arcs are too far could be just an illusion due to the "toward lamp" extension of divergent halos.

    considering this, 35d column looks like a good match to me. also, some of the outer extensions of the column arc could be masked using small aperture pyramidal faces. especially, the odd radii seems more diffuse, which i would interpret as small pyramidal faces diffracting light and broadening halos.

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    1. Divergence was an option I considered before, but the 24d Plate Arcs did not seem to show divergence, which made me give up explaining ‘35d spots’ with divergence. Perhaps I threw the truth into the trash can.

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  2. nicolas lefaudeux19 January 2026 at 16:55

    the 24d column arcs are pretty large. and from your simulations, 35d column arc would be a better match than 35d plate arc i believe

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    1. Thanks. Hope that one day we can fully simulate these divergent and interference effects (Perhaps you have already achieved a perfect simulation), so that the simulation exactly matches Marko's wonderful photo record.

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  3. It is nice to have these ideas of Parry pyramid and MS anyway. I will take star field photos and do some measurements of that 35° arc. I had floated also an idea of it being one of the counter-24° arcs: https://x.com/RiikonenMarko/status/1871867450716803415

    The thin pyramid ends remove nicely the counterparhelia, which I can't see in the display.

    (As to the terminology, I have been experimenting with both "counter" and "flip" for the basal reflection counterparts in my posts).

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    1. Yes, Marko, I've noticed your contra-24P proposal, but perhaps it can only match this one photo? To other sences which photos taken at different times, it seems that the intensity and shape of '35d spots' cannot be explained by contra-24P.

      Of course, I don't think contra-24P is wrong, because the halo landscape might be changes rapidly during this event. Maybe we need different solutions to adapt to your halo image at different times.

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  4. That's right, I should have specified that contra-24P prospect really concerns only that side view stack. Well, let's see how those measurements turn out once I get the starry sky photos.

    So I see you are experimenting with contra. I have concerns about flip. It's flippant. Maybe the choice, if this the system I propose would get adopted, is between contra and counter.

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    1. In my English dictionary book, the meaning of "flip" seems to be very diverse, but its advantage is that it is short. Contra is more Latinized than counter - if prefixes like 'pseudo' are retained in the future, then contra might be another good latin prefix for halo's name.

      But the real reason why I use contra is very naive - when I was a child, there was a very popular FC-game named 'contra'. (emm, perhaps I shouldn't chat about this things on a website that talks about science.)

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