I had been troubled by my own remarks I had made in another topic:
(...) From my own experience I can say that any plane within the smaller circle (20km radius from my location) is great. And any plane outside the bigger circle (40km radius) is usually invisible or very weak because it's very low above the horizon, so there is lots of air in the way. (...)
(...) The visibility was great and the range at which I could clearly see a plane's contrails was remarkable. There were 2 cases when I was really surprised that I could clearly see the contrails of a plane that was AT LEAST 60km away. At such distance a plane is only (around) 10 degrees above the horizon (the precise angle depends also on its altitude), so there is lots of air in the way. (...)
I had been somewhat troubled by these (relatively small) distances because I had known that some people claimed that they spotted contrails of planes that were over 300 km away! How could that be, when I was impressed already by distance a little more than 60 km? Here's what I found.
I will describe things in this order (more or less in the order of importance):
1. Air clarity/transparency.
2. Plane's altitude.
3. Observer's (eye) altitude.
4. Atmospheric refraction.
5. Clear view to the horizon.
1. Air clarity/transparency.
The proper info in a table form, based on the STCW (International Convention on Standards of Training, Certification and Watchkeeping for Seafarers) was easy to find on the Polish Wikipedia site for visibility (widzialność) – it was described as “horizontal visibility scale”. On the English Wikipedia site for visibility there was nothing concrete (no table/scale) but I did find something similar, described as “Meteorological optical range table”, here:
Both scales use the unit nautical mile, which is equal to 1.852 km (for comparison a mile on land is equal to 1.609 km). I combined the last/best 3 levels of visibility on both scales (when there was a slight difference I used the higher value):
Visibility / Weather (Meteorological Optical Range):
7) Good / Clear – from 10km to 20km.
8) Very good / Very clear – from 20km to 52km.
9) Exceptional / Exceptionally clear – over 52km.
To me it was quite surprising that good visibility is already at ONLY 10 km! Very good visibility is at only 20 km and any visibility over 52 km is exceptional! So my value of 60 km doesn't look so bad after all.
I have to point out that Meteorological Optical Range (MOR) is “the length of path in the atmosphere required to reduce the luminous flux in a collimated beam from an incandescent lamp to 5% of its original value”. I think it means that a very bright object can “beat” the distances given above and it probably happens with sunlit contrails of a distant plane around sunset (or sunrise), when the sky/background is relatively dark.
I have to also point out that on some Internet sites you can find some things that are clearly wrong, for example the (wrong) info that the atmospheric visibility is less than 300 km, which is misleading without any additional info. The Wikipedia site for visibility states that “AT SEA LEVEL (…) in the cleanest possible atmosphere, visibility is limited to about 296 km.”, so this is purely theoretical number because AT SEA LEVEL you can't see anything at such a huge distance. Some Internet sites repeat this value without any explanation/additional info, as if this number could be used for any practical purpose. No, it can't.
2. Plane's altitude.
Plane's altitude is usually much higher than observer's (eye) altitude, so it's much more important by definition. In order not to confuse things I will keep all the calculations in the present point for the observer's altitude of 2 meters. Please notice that this (small) observer's altitude is “local” (it's NOT altitude above the sea level), because I assume that the terrain all around the observer is roughly at the same level.
Max visible distance in km = 3.57 * square root(observer's altitude in meters) + 3.57 * square root(plane altitude in meters).
The observer's (eye) altitude of 2 meters alone gives distance (to horizon) of (only) 5 km:
3.57 * square root (2) = 5.0
I prepared a cheat sheet with different plane's altitudes (with a bonus of the highest mountain on the Earth):
I marked with the red color the most important thing – there are diminishing results when increasing a plane's altitude, because of the Earth's curvature. Subsequent increases of plane's altitude by 2000 meters result in smaller and smaller increases of the max visible distance (in km).
There is a catch, however – if there were no atmosphere, all these planes would “visible” right at the horizon, so it would be actually impossible to see them because an object has to stick out above the horizon in order to be visible/discernible.
Obviously the max visible distance works both ways – when an observer can see a plane (or a mountain) then the plane (or the mountain) can “see” the observer. It's remarkable that from the highest mountain on the Earth (Everest) you can see a 2-meter-high object/person that is “only” 341 km away!
3. Observer's altitude.
Observer's (eye) altitude adds to the effect of plane's altitude, but it's usually much smaller than plane's altitude, so it's much less important by definition.
I prepared a cheat sheet with different observer's altitudes (with a bonus of the longest photographed line of sight between two mountains):
I marked with the red color the most important thing – there are diminishing results when increasing an observer's altitude, because of the Earth's curvature. Subsequent increases of observer's altitude by 500 meters result in smaller and smaller increases of the max visible distance (in km).
The catch is the same – if there were no atmosphere, all these planes would “visible” right at the horizon, so it would be actually impossible to see them because an object has to stick out above the horizon in order to be visible/discernible.
It's worth to note that the longest photographed line of sight on surface of the Earth is “only” 483.5km. That photographed line of sight was between two very high mountains (Aconcagua photographed from Champaqui) that were “spaced” perfectly – just below the max visible distance! You can see the photograph (and also a video) here:
https://dalekiewidok...cord-andes.html
4. Atmospheric refraction.
All the values for atmospheric refraction were given for bearable temperature of 0 degrees Celsius and max (best) available air pressure, according the online calculator at this site: http://www.jgiesen.d...ract/index.html
Atmospheric refraction may give some impressive results very close to the horizon, “lifting” an object from below to above the horizon like this:
By the way: this visual calculator shows perfectly why the sun appears flattened close to the horizon – it’s because there are significant differences in the atmospheric refraction very close to the horizon.
The higher above the horizon the weaker the effect of atmospheric refraction. When an object is just 2.0 degrees above the horizon the difference is only 0.304 degree (the object appears higher by that much, so at. 2.304 degrees above the horizon):
Such a small difference is hard to notice with the naked eye – here’s how it looks in broader scale:
I prepared a cheat sheet for atmospheric refraction at different angles above the horizon:
I can't post any more pictures here, so I will continue in the next post.