lipadj46 said:
Leupold makes some tasty kool-aid don't they
benzy2 said:
Again I will ask if you are so big that index matching makes things better do you have resolution chart results and light transmission results from even one Leupold scope to another to state if there is potentially any truth to these trade mark terms or are you just going based on the marketing that a cool term must be good?
So why is it that high-end astronomical telescopes rely heavily on index matching of lenses? All you have to do is read about index matching on astronomy related sights where noise is a BIG problem to realize the benefits of index matching.
Multi-coating all of the lenses and then stacking them up in the scope is not the same as taking the time to match the lenses either by selecting specific refractive indices or coating lenses to obtain specific refractive indices. These matching systems are proprietary and there's no doubt that Nightforce, Schmidt & Bender, US Optics, Leupold etc do it in slightly different ways, but their objectives are the same ...
lipadj46, what scopes do you currently own? How about scopes that you've owned in the past. I've made no secret of the fact that I have a number of Mark 4 scopes and I've owned quite few low-end scopes over the years.
This might help to shed some light on the benefit of index matching.
"When light is focussed by passing it through a lens made from ordinary glass, such as crown glass, each wavelength of light bends a different amount. This is the reason, we are able to see light separated into its spectrum when it passes through a glass prism. This different bending leads to a problem, because each wavelength focusses at a different point. The result is a focal zone rather than a focal point. When a bright object is viewed through such a lens, it is blurry and has a fringe of false colour. Technically, this is referred to as
chromatic aberration. Reflectors don't suffer from this effect because their light rays don't pass through any glass. A second problem, called
spherical aberration, occurs when optical surfaces of lenses or mirrors are not properly figured or shaped. As with chromatic aberration, the focal point becomes a focal zone ...
... a second approach is to
add another matching lens of a glass having a different refractive index. For example, when positive, low-index, BK7 crown glass is matched with negative, high-index, F2 flint glass, the light rays are bent again so that all wavelengths focus near the same point. The result is called an achromatic refractor and the
matched lenses may either be cemented together, or air-spaced by mounting them in a cell which holds them in their correct positions. The two-element lenses used in today's achromats greatly reduce the chromatic aberration. For example, it has been brought to low levels in Sky-Watcher 1201EQ5 and 15012EQ6.
In the ongoing search for the perfect telescope, lens makers produced other lens element combinations and special types of glass, in order to remove all of the false colour. These developments have resulted in semi-apochromatic (almost without colour) and apochromatic (corrected in three colours) refractors but these are very expensive compared to achromatic refractors."