Distant view

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Example of good visibility: View from the blender towards the Zugspitze . The air line between the two points is approx. 67 kilometers. Kempten (Allgäu) is covered by the early morning mist .
Exceptionally good distant view over the Danube valley near Regensburg to the approx. 140 km distant alpine chain
222 km of distant view from the Vosges to Mont Blanc

A clear, far-reaching view into the distance , which usually also allows an overview of the structure of the landscape , is referred to as a distance view or good distance view .

Conditions for good visibility

Good visibility has several requirements of a geographical, meteorological and physiological nature:

  1. A suitable location , for example on a tall building (town or church tower , observation tower ), on a mountain top or on a prominent step in the terrain , such as the mountain station of a cable car. The view from a commercial aircraft offers a particularly wide view (distance view at approx. 12,000 m altitude up to 300 km).
  2. The broadest possible viewing angle ("free horizon "), which is ideally between 180 ° and 360 °, but must be at least 20 ° for a visual impression of the room (for example on a path between trees or rocks).
  3. Good meteorological visibility conditions with little water vapor , dust or haze in the earth's atmosphere .
  4. Good and relaxed eyes, whose well-being can be contributed to by blinking several times. Exerted staring into the distance does the opposite.

Maximum values ​​of visibility

- for calculation see article Visibility -

On earth, good visibility is usually around 50 to 100 km away, but close to a large city 30 km can appear extraordinary. The greatest possible visibility in the high mountains and favorable climatic zones (e.g. western Cordilleras ) or weather conditions (e.g. foehn ) is around 150 to 300 km. The fewer aerosols the air contains, the better its transparency . B. in aviation  - there are special definitions and measuring instruments .

Good visibility is also advantageous for nautical and geodesy purposes. With coastal or visual navigation one reckons with a few km to 20 km, in which area u. a. the visibility of the beacon is. Due to the mostly moist oceanic air, the visibility is less than on the continent. With a telescope , on the other hand, the view is hardly better than with open eyes because the contrast decreases. Nevertheless, sight lengths of 30 to 60 km are possible for large-scale geodetic angle and distance measurements . Good weather conditions or the lighting of the target points are necessary for this. B. Gauss invented the heliotrope to reflect the sun.

In the mountains and on the edge of industrial areas , there is often the best visibility just after heavy rain , when the air z. B. is particularly dust-free and dry for a short time when the weather is on the rear Really clear air is usually only given when the peplopause is exceeded , an approximately 2 km high boundary layer under which there is little mixing. On the other hand, the best viewing conditions on the earth's surface are from a low orbit .

Alpine panorama taken from the Roßberg Tower (Swabian Alb)

Distant view from space

As early as 1960, the first photos from the beginning of space travel showed that the steep (especially vertical ) view through the earth's atmosphere is clearer than originally expected (see literature below). Again and again, even experienced astronauts report their surprise at the fine details they can see from the spaceships . According to some space medics , the change in optokinetic nystagmus (unconscious eye tremors) in weightlessness also contributes to this.

The greatest possible distance is a view of the starry night sky . Occasionally falling stars are about 100 km away, aurora borealis a few 1000 km, the planets with many millions of kilometers 10 to 100,000 times further away, and the next fixed stars with 4½ - 10 light years again at a million times further distance. The most distant, freely visible object is the Andromeda Nebula (astronomically the galaxy M31 ) at a distance of about 2.5 million light years.

See also

literature

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