magellan force
O2 Force comparatives
By Henryk Szubinski
TELESCOPIC RECTICLES: ON THE HOWL RESPONSE OF A DRAWN OUT AND MINIMALISED FORMAT FOR A 3 LEVEL :the closest to audiality on a format for the audio visual interactives on a process by which to localise dark matter:
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The Magellanic Clouds have been known since the earliest times by the ancient Middle Eastern peoples. The first preserved mention of the Large Magellanic Cloud was by Persian astronomer Al Sufi, who in 964, in his Book of Fixed Stars, calls it al-Bakr, meaning “the White Ox”, of the southern Arabs, and points out that while invisible from Northern Arabia and Baghdad, this object is visible from the strait of Bab el Mandeb, at 12°15′ Northern latitude.[1]
In Europe, the Clouds were first observed by Italian Peter Martyr and Andreas Corsali at the end of the 15 century. Subsequently, they were reported by Antonio Pigafetta for the expedition of Ferdinand Magellan during the circumnavigation in 1519–1522.[1] However, naming the clouds after Magellan did not become widespread until much later. In Bayer’s Uranometria they are designated as NVBECVLA MAIOR[4] and NVBECVLA MINOR[4]; even in French astronomer Lacaille‘s 1756 star map, they are designated as le Grand Nuage[5] and le Petit Nuage.[5] (i.e. the “Large Cloud” and the “Small Cloud”, in Latin or French).
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A BASIC TELESCOPIC RANGE IN WHICH THE PROCESS OF TURBULENCE BEING INVOLVED IN THE DATA ON THE BASE LEVEL OF APPROACHES TO THE DEFINITIONS OF WHAT IS LOCALISED DOES NOT EQUATE TO THE FORMATS OF THE BASICS IN TIME
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AS A PHOTON CERTAINTY IN THE CALCULATIONS OF FORCE:
Telescopic sights are usually designed for the specific application for which they are intended. Those different designs create certain optical parameters. Those parameters are:
Magnification — The ratio of the focal length of the eyepiece divided into the focal length of the objective gives the linear magnifying power of telescopes. A magnification of factor 10, for example, produces an image as if one were 10 times closer to the object. The amount of magnification depends upon the application the telescopic sight is designed for. Lower magnifications lead to less susceptibility to shaking. A larger magnification leads to a smaller field of view.
Objective lens diameter – The diameter of the objective lens determines how much light can be gathered to form an image. It is usually expressed in millimeters.
Field of view — The field of view of a telescopic sight is determined by its optical design. It is usually notated in a linear value, such as how many meters (feet) in width will be seen at 100 m (or 100 yd), or in an angular value of how many degrees can be viewed.
Exit pupil — Telescopic sights concentrate the light gathered by the objective into a beam, the exit pupil, whose diameter is the objective diameter divided by the magnifying power. For maximum effective light-gathering and brightest image, the exit pupil should equal the diameter of the fully dilated iris of the human eye — about 7 mm, reducing with age. If the cone of light streaming out of the eyepiece is larger than the pupil it is going into, any light larger than the pupil is wasted in terms of providing information to the eye.
However, a larger exit pupil makes it easier to put the eye where it can receive the light: anywhere in the large exit pupil cone of light will do. This ease of placement helps avoid vignetting, which is a darkened or obscured view that occurs when the light path is partially blocked. And, it means that the image can be quickly found which is important when aiming at game animals that move rapidly. A narrow exit pupil telescopic sight may also be fatiguing because the instrument must be held exactly in place in front of the eyes to provide a useful image. Finally, many people in Europe use their telescopic sights at dusk, dawn and at night, when their pupils are larger. Thus the daytime exit pupil of about 3 to 4 mm is not a universally desirable standard. For comfort, ease of use, and flexibility in applications, larger telescopic sights with larger exit pupils are satisfying choices even if their capability is not fully used by day.