Sunday, 1 November 2020

One more case of sub-Kern companion arcs

Sometimes a sub-Kern arc "bleeds": it is accompanied by thin arcs below the brightest parts. The first case we photographed on the night of 6/7 January 2016 and second on 28/29 November 2016, both in Rovaniemi. Here is a third display with these arcs in Rovaniemi, photographed on the night of 4/5 January 2017. The lamp is somewhere between 5 and 10 degrees below the horizon. The temperature at this roadside field was -38 C, the lowest I experienced that winter. Earlier that night, at another location, I had photographed odd radius sub-plate arcs.

 

Below are three more photos from that location, taken before the the sub-Kern company arcs appeared.



Thursday, 29 October 2020

Possible Tape arc fragment with other sub-par Parry arcs?


 
 On the 27th of October a quick and interesting halo display took place in Ostrava, Czech Republic. I had little time to observe and the cirrus cloud shield was moving quickly. I was stacking frames with a camera only holding it in my hand. Meanwhile, I took some mobile phone pictures, but the quality is sub-par for any post-processing.

Before the clouds moved to a left-side position of the Sun, a rather weak uppercave Parry was observed.

  
 
 I was almost 100 % sure I saw Lowitz arcs as well, but there are no traces of them on single and stacked frames.

Below is a composite of stacked frames with colour, B-R processing, a simulation and its superimposition over the B-R processed stack.


Let me know, what you think.



Sunday, 20 September 2020

Mysterious sunvex 28° arcs in Yunnan, China

On August 26 2020, Zhang Yibing from Pu'er, Yunnan captured a sunset odd-radius display, in which a bright 28° arc dominates the show. 

Stacked and sharpened. © ZHANG Yibing, shown with permission.

Evolvement of the display. No sharpening. © ZHANG Yibing, shown with permission.

The arc’s brightness is almost on par with the 20° plate arc, while other plate arcs such as the 24° and 35° ones are exceptionally weak and barely show up in stacked photos. What’s more interesting about the 28° arc is its shape. What we are seeing in this display is a gently sun-vex arc which doesn’t quite follow the 28° sun-centric circle.

Stacked and background subtracted photos reveal a left 28° sun-vex arc as well. Note how both arcs curve away from, instead of follow, the 28° circle.


Such appearance contradicts current theories. In the 30-32 pyramid and cubic ice models ( http://www.thehalovault.org/2018/09/28-plate-arc-captured-in-haikou-china.html ), the predicted 28° arcs do not appear sun-vex like the 24° plate arcs do. Quite the opposite, when the crystals are wobbly, the arcs should look more sun-cave and follow the 28° sun-centric ring.


The puzzling shape can still be achieved by tweaking the available theories though. JI Yun and I did some experiments in ZHANG Jiajie’s simulation program and came up with a bizarre solution.

First is to tilt a triangular 30-32 upper pyramid by 109.5° until one of its pyramidal faces goes horizontal. Then, apply a loose ( 15° wobble or more) sun-ward azimuthal lock on both tilted 30-32 crystal and cubic ice.


The revised models produce identical sun-vex 28° arcs which closely match the ones seen in the display.


The idea of az-locking crystals in the air is certainly outlandish and should hardly be taken seriously unless concrete evidence is found in real world. That being said, there’s only so much we can do with available theories. New ideas/experiments are much needed.

This display marks the 11th record of 28° arcs in China since 2016, and more importantly, the 1st record revealing the arcs' real shape. Is it possible that what we're seeing in this display are actually new halos, different from the previous 10 Chinese records and the legendary Lascar arcs? Or is it that all these Chinese 28° arcs are a same new breed different from the Lascar ones? We'll need many more similar displays to draw a conclusion. Looking forward to the next summer.

Update:

Nicolas Lefaudeux proposed another possibility for the arc's peculiar appearance:

"On my side, the sunvex shape is still not so obvious to me. I see more a vertical elongation of the 28° arc + some patch of 28° halo. 

Effects like diffraction by "vertically narrow" crystal faces would create such vertical elongation (like a plate crystal with exotic faces instead of regular prism faces). Unfortunately, such effects cannot be simulated with our current softwares. The appearance of the halos (smooth and rather undefined) make me think of diffraction-affected halos (small crystal faces), like most of the odd radius halos. We would need cases with sharper arcs in order to be more conclusive."

Friday, 18 September 2020

Long subparhelic arcs in Rovaniemi spotlight display

 

Diamond dust season is about to begin, the hissing of guns at the Ruka resort may be heard already at the end of September. To get in the spirit, let's reach into the drawer and grab this display which appeared on the night of 7/8 February 2017 in Rovaniemi. At first it was bog-standard plate with CNA, sub-120, and sub-Lilje / subparhelic circle patch opposite to the lamp, but then it changed, giving these long subparhelic arcs. The lamp sits at the usual ~5 degrees below the horizon. The location is Sieriaapa bog some 6 km east from the ski center. This is the direction where the diamond dust most often heads to, guided by the prevailing wind and topography.

 


Friday, 4 September 2020

August halos from Moravia, Czech Republic

Jiří Kaňovský from Černotín, Czech Republic observed three separate halo complexes this August.


August 2nd, 2020 – bright odd radius halos


I (Jiří Kaňovský) was visiting my aunt when I’ve noticed a halo making cirrostratus cloud shield. It was obvious that what I saw were not classical halos, but odd radii ones. I was able to observe 9°, 18°, 20°, 22°, 23°, 24° and 35° halos. Near the end of the observation, a bright 23° parhelion joined the party.





 

 

August 10th, 2020 – classic halos with a twist

These halos were observed due to an extensive cirrus/cirrostratus cumulonimbogenitus shield from a previous thunderstorm activity. At the evening hours, some of the cirrus clouds began to sublimate. Among the classic halos like 22° halo, UTA, CZA, SLA and 22° parhelion, later image stacking revealed a bright spot near supposed 9° column arcs and a 24° halo or a 24° column arc as well.






August 24th, 2020 – almost invisible uppercave Parry

There was a surprise 14 days later in the form of a weak but nice halo complex. A 22° halo, parhelions, weak UTA and CZA were observed. Later image processing revealed a weak uppercave Parry and a hint of a supralateral arc.







All these observations are a part of an endeavour to bring an old project back to life – the Czech HOP (Halo Observation Project). After 10 years of inactivity, multiple people are joining again to work on the project so it could be a place for amateurs and “professionals” alike where they can share their photos of observed complexes.

Saturday, 27 June 2020

A fine reflection subsun in northern Finland



Heikki Kainulainen uploaded this reflection subsun a couple of days ago to the Finnish observation site Taivaanvahti. It was seen in the Muonio region of northern Finland on May 29. The photo was taken through window at 04:41 when the sun was 6.9 degrees above the horizon. In the direction of the sun there is, starting at 11 km distance from the observation site, a 3 km transect of water. This is lake Pallasjärvi, and could be the source of the reflection. It is the only large water body for 140 km in the sun direction. 




However, according to Kainulainen, Pallasjärvi was still frozen. So maybe the reflection was from the lake ice, or, as Kainulainen suggest as one possiblity, from the possible flood waters in the bog areas. 

As reflection subsuns go, this is a beautiful specimen which shows also the mysterious effects of vertical striation and larger-than-sun width. Below is an usmed close up of the photo above to highlight these features.


 
Yet one more image is shown, in which a separate photo of the sun has been superposed with the pillar. The width of the brightest part of the pillar is about equal with the sun disk, so this part most likely was located on the solar vertical. The sun reference photo was taken with the smallest aperture of the lens and shortest exposure time, but it may still be overexposed slightly.



Wednesday, 17 June 2020

High Quality 28° Arcs in Ji'an, China

Moments before sunset on June 17 2020, a high quality odd-radius plate display with bright and vivid 28° arcs was documented by multiple observers in Ji'an, Jiangxi Province, China.

© HUANG Qian, shown with permission. Single exposure.

© ZHOU Ling, shown with permission. Single exposure.

Annotated version as follows:



The intensity of the display rivals the 2016 Chengdu display as the 28° arcs stand out even in smartphone photos above. 20°, 24° and 35° plate arcs in the photos are also quite well defined.

Unfortunately, like previous displays, no other exotic arcs are found in the photos we received from the community.

Now that we have a great and early start of the season, let's hope for more great stuff to come.

Monday, 15 June 2020

Odd radius sub-plate arcs

Odd radius plate arcs have copies on the other side of the horizon, grouped around the subsun. People have been aware of the possibility of such arcs I call them unofficially here as sub-plate arcs at least from the 1990's, but no observations have surfaced.

Here I show three odd radius sub-plate arc displays that I photographed in Rovaniemi in the winter 2016/2017. The first display was seen on the night of 12/13 December 2016. Only one odd radius sub-plate arc was visible, the 18 sub-plate arc. Below are photos and animations of its appearance.


Flashing two stacked images from a continuous photo series, the other half which had subparhelia and the other which had 18 sub-plate arcs dominating.


Versions of a stack with a slightly different set of photos than above and a simulation. Also other odd radius halos are visible: 18 plate arc and 18 halo, 35 plate arcs and faint 35 halo.


An animation of transformation from subparhelia to 18 sub-plate arc.


A stack of photos from another stage in the display. We see here three halos flanking the subsun: 18 sub-plate arc, subparhelia and a mysterious arc outside the subparhelia. The last one seems to be part of a longer arc that extend faintly to normal parhelion and reminds me of the arc in the 28/29 December 2016 display in Rovaniemi. 


An animation showing the changing display.

_ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _


Next I got odd radius plate arcs on the night 4/5 January 2017. This was the winter's coldest night in Rovaniemi. At the location which was the same as above, the Oikarainen gravel pits the temperature was around -35 C. This also was the night with the best sub odd radius stuff: in addition to 18 sub-plate arc there was an upper 23 sub-plate arc. Both were easily visible to the naked eye.


The best odd radius stage did not last long, here are shown three and five images stacks. The display is all but straighforward case. Like in the first display, there are three halos flanking the subsun: 18 sub-plate arc, subparhelia and, well, something. The vertical feature at the horizon should, according to the shown simulation, contain both 35 plate arcs and 35 sub-plate arcs, and while there may be both or either one, that is likely not the full explanation. See again the 28/29 November 2016 display, which is not an odd radius display, but which nevertheless contains a similar kind of thing. Yet another detail to pay attention is 20 sub-plate arc, which is in the simulation, but absent from the display. It was difficult to avoid it in simulation, it should have been in the display. Concerning the lack of normal parhelia and 18 plate arcs in the display, that may be explained by the lamp not being centered exactly on the camera, but shooting slightly over it. I am not sure, this is something to pay attention to in the future (hopefully the nightly diamond dust halo chase is not dead, as it seems now).


This single photo has the 23 sub-plate arc (arrow) somewhat better than in the stacks above. I turned camera here to try catching one of the distant, unobserved odd radius arcs that I had seen in simulations. Alas, no success. After this photo the odd radius stuff deteriorated quickly, so there was no getting a stack that might have actually gleamed out something novel.


Even though the odd radius halos deteriorated, and the display started turning into a normal plate display, here 18 sub-plate arc is still visible inside subparhelia.


Another photo from another place that night with odd radius stuff. We see odd radius parhelia and circular halos at 18, 20, 24, 35 and a possible odd radius helic arc. No odd radius sub-plate arcs here.


And an animation showing the transformation from conventional display to an odd radius display.

_ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _


The third and the last odd radius sub-plate arc occurrence was in the display on the night of 9/10 February 2017. Only a weak 18 sub-plate arcs were found from photos, as shown below. Again, the location is the Oikarainen gravel pits. It is a good place, with plenty of possibility to play with lamp elevation. It is quite far from the ski center, though, 12 km as the crow flies, so the diamond dust can reach there only on the coldest nights.




_ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _ _


Taken that odd radius sub-plate arcs were found in three displays in one winter, they can't be regarded much of a rarity just get to the right place, switch on the spotlight, and you got them bagged. With spotlight it is in general much more easier to catch subhorizon halos (well, any halos, really) than in solar displays. In case of the odd radius sub-plate arcs, the subhorizon spotlight method has also the advantage that, because of how pyramid crystals orient to keep the larger basal face as the upper face, these halos are easier to form than in sun light, the latter way of which requires the inner reflection to take place from the smaller, and thus less effective, down facing basal face.

For the last, I add here a collection of photos from first two of these displays, and the 28/29 December display (the bottom row), to more easily compare the features in them:


All simulations in this post are made with HaloPoint2.

Friday, 12 June 2020

Surface halos from uniformly oriented crystals


I was searching for surface halos on ice plates for two years without luck because of unfavorable weather in my area (Romania and Hungary). On 18 January 2020 I finally observed my first subparhelia and 120 degree subparhelia complete with the colored nadir spot on a small icy patch near a lake in Romania. In February I continued my search for these kind of halos in northeastern Hungary. Clear weather after a rainy period with minimum temperatures between -5 and -10 degrees ºC promised me a good opportunity, so I went out to a nearby field with plenty of frozen puddles, many of which had air below the ice. Since most of them formed in shady hollows I broke off pieces of ice and placed them in the sunlight to produce the halos. To my surprise these halos appeared more vividly when I held the pieces upside-down (relative to their original position on the ground) indicating more and/or better quality ice prisms on the underside, so I used them in this way. On the plates there were large patches of uniformly oriented prisms, this feature made itself noticable as a break in the observed halos. I tried to take pictures of the crystals, but it was difficult because of their very small size (to the naked eye the surface seemed completely smooth). The only usable image I could get is shown above depicting crystals pointing away from the plate surface in the same orientation rather than being parallel with it.
Below I present the most interesting halo elements with screenshots grabbed from my videos made on 8 and 13 February.  Some of them were previously observed (in Hungary and Finland), others are new. The surface is defocused because I held the camera lens only a few centimeters from the ice plates. Since pictures are not showing the nature of these phenomena well, I recommend watching  my videos  available on Youtube (links can be found at the end of the post).
1. Subparhelia and other spotlike features on the pieces: bright subparhelia always accompanied the subsun on the ice plates. Sometimes a ,,duplication’’of the subparhelia appeared when I held the plate in an almost horizontal position and watched it in a flat angle. When holding the plates in the opposite direction of the Sun, white and colored spots could be observed.kukk
From left to right: colored spot (looking away from the Sun), white spot (probably related to the white arcs), a ,,duplication’’ of the subparhelion on its right side
2. Spots made by the underside crystals of the ice sheet left in its original place: one of the puddles had crystals only on the underside of its ice. The situation was the same on both days, despite of the melting and re-freezing of the ice in the meantime. From here I could not break off pieces for further investigation because there was water only a few centimetres below the ice that instantly destroyed the crystals if I tried to do anything.
Clipboard02
From left to right: orange spot (looking in the direction of the Sun), orange spot (looking away from the Sun), colored spots (the Sun is at the left), white spot in the place of the 120 deg. subparhelion.


3.  Arcs crossing at the subsun with a white spot on them: these arcs change their configuration as one rotates the ice plate. Sometimes a faint subparhelic circle is also visible. The white spot is usually located at the intersection of the subparhelic circle and a white arc, but with changing the angle of the plate it can appear elsewhere.

Clipboard01

White arcs with a spot visible on the right one at the intersection (top) and above the intersection (bottom) with the subparhelic circle.
4. Faint parhelia-like spots near the bright spots of the white arcs, in the direction opposite to the Sun: if one follows the white arcs pointing away from the Sun, the white spots can be found there as well, accompanied by two faint spots on both sides which look as if they were parhelia of the white spot. Also there is a subtle brightening on the arcs above the white spot. Clipboard01d
Parts of the white arcs with the bright spots pointing away from the Sun, the arrows mark the faint ,,parhelia’’ on the sides.
5. The colored nadir spot: sometimes the nadir spot was present, situated on one of the white arcs.  For this feature one must look at the plate from above in a steep angle.  
lulu
The nadir spot is visible on the ,,vertical’’ arc
6. Looking through the ice plate: when looking at the Sun through an ice plate (holding it perpendicular to the Sun-observer axis), a regular six pointed star became visible ending in parhelia-like spots 25 degrees from the Sun (measured by Marko Riikonen using a starfield photo as reference). As I changed the angle and position of the plate, white and colored spots moved away from these parhelia. 
vlcsnap-2020-05-16-12h23m44s501
The six pointed star with parhelia on the ends

kk
Changing the angle of the plate and looking through it to the side and below the Sun gave another set of white and colored spots
7. White star on the opposite side: holding the plate away from the Sun another six pointed star appeared with the reflection of the Sun at its center. In my opinion the arcs that make up this star are strongly related to the white arcs discussed at (3.). 
vlcsnap-2020-06-08-17h06m28s913
The opposite-side star with the Sun’s reflection at its center
Links to my videos (montages created using the best parts of the original material):