These attributes combined with adequate eye relief for glasses wearers are an outstanding (and recent) optical achievement, but for hand-held binoculars they are of no practical value.
The fovea of the human eye, where highest visual acuity for 20/20 vision is achieved only has a visual field of 1° and outside this, visual acuity degrades more rapidly than the off-axis resolution of a binocular.
If we wanted to view the field edge of a typical binocular with 60° AFoV we would have to redirect our eyes by about 29°. However, the eye's pupil is at about 11 mm radius from the centre of the eyeball, so a 29° redirection is accompanied by rotation and about 5 mm lateral movement, sufficient to result in a complete blackout in most binoculars!
Of course we just don't do this and simply redirect the binocular to place an object of interest in the field centre.
Should there be any doubts about this, I suggest placing a binocular on a tripod and viewing a detailed plane surface (or bookshelf). To see detail in the left field it is necessary to move one's head to the right and vice versa. This technique is often used by amateur astronomers, whose telescopes are always tripod mounted and where eyepieces with up to 110° AFoV are sometimes used.
It is often asserted that for daylight viewing one does not need more than 2,5-3 mm exit pupils but they result in a loss of viewing comfort.
The complaints of veiling glare in some modern designs can perhaps be attributed to their complexity and the "poor" edge performance of Ultravids, SLCs and FLs, particularly those of lower magnification and large exit pupils is in practice more advantage than detriment.
John
The fovea of the human eye, where highest visual acuity for 20/20 vision is achieved only has a visual field of 1° and outside this, visual acuity degrades more rapidly than the off-axis resolution of a binocular.
If we wanted to view the field edge of a typical binocular with 60° AFoV we would have to redirect our eyes by about 29°. However, the eye's pupil is at about 11 mm radius from the centre of the eyeball, so a 29° redirection is accompanied by rotation and about 5 mm lateral movement, sufficient to result in a complete blackout in most binoculars!
Of course we just don't do this and simply redirect the binocular to place an object of interest in the field centre.
Should there be any doubts about this, I suggest placing a binocular on a tripod and viewing a detailed plane surface (or bookshelf). To see detail in the left field it is necessary to move one's head to the right and vice versa. This technique is often used by amateur astronomers, whose telescopes are always tripod mounted and where eyepieces with up to 110° AFoV are sometimes used.
It is often asserted that for daylight viewing one does not need more than 2,5-3 mm exit pupils but they result in a loss of viewing comfort.
The complaints of veiling glare in some modern designs can perhaps be attributed to their complexity and the "poor" edge performance of Ultravids, SLCs and FLs, particularly those of lower magnification and large exit pupils is in practice more advantage than detriment.
John