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UVFS Simple Telescope Kit
146-1008
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1848 $
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UVFS Simple Telescope Kit
146-1008
Available: 0
1848 $

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UVFS Simple Telescope Kit

UVFS Simple Telescope Kit

UVFS Simple Telescope Kit includes opto-mechanics, uncoated and coated lenses for 266 nm R<0.2%, 266+355 nm R<0.6%, 210-400 nm R<1.5%, 355 nm R<0.25%, 532+1064 nm R<0.5%, 350-900 nm R<1.5%, 650-950 nm R<1%.

from 1287 $
delivery Estimated delivery time: Request
Qty discount: 5-9 pcs. of the same item - 5% OFF! 10+ pcs. 10% OFF!
Products
List of Lenses in UV FS Lens Kit
Brochures
Description
UVFS
Code Material Coating Price Delivery Add to cart
140-1008 UVFS uncoated 1287 $ Request
144-1008 UVFS 266 nm, R<0.4% 1617 $ Request
149-1008 UVFS 266 nm + 355 nm, R<0.6% 1628 $ Request
146-1008 UVFS 210-400 nm, R<1.5% 1848 $ Request
143-1008 UVFS 355 nm, R<0.25% 1612 $ Request
141-1008 UVFS 532 nm + 1064 nm, R<0.5% 1634 $ Request
145-1008 UVFS 350-900 nm, R<1.5% 1854 $ Request
148-1008 UVFS 650-950 nm, R<1% 1810 $ Request
Any other antireflection coating wavelength region is available on request.

Each kit includes: 8 lenses (3 pcs. of lens 1 and 5 pcs. of lens 2), Aluminium Optical Rail 810-0005-02, two Aluminium Rail Carriers 810-0007-06, Self- Centering Lens Mounts 830-0010 and 830-0020, two Rod Holders 820-0050-02 and two Starndard Rods 820-0010-02

Lens 1 Focal
length f1, mm
Lens 2 Focal length
f2, mm
Distance between
lenses d=F1+F2, mm
Magnification, M
UVFS bi/cv Ø12.7mm   UVFS pl/cx Ø50.8mm      
114-1104  -12.7 110-1505 +75 62 5.9
    110-1509 +100 87 7.7
    110-1511 +150 137 11.8
    110-1515 +200 187 15.7
    110-1517 +250 237 19.7
UVFS bi/cv Ø25.4mm   UVFS pl/cx Ø50.8mm      
114-1204  -25 110-1505 +75 50 3
    110-1509 +100 75 4
    110-1511 +150 125 6
    110-1515 +200 175 8
    110-1517 +250 225 10
UVFS pl/cv Ø25.4mm    UVFS pl/cx Ø50.8mm      
112-1205 -50  110-1505 +75  25 1.5
    110-1509 +100 50 2
    110-1511 +150 100 3
    110-1515 +200 150 4
    110-1517 +250 200 5
Note that distance between lenses d is the distance between focal planes of the lenses and is given theoretically (the thickness of lenses is not included into calculation). It, also, depends on wavelength. The distance should be adjusted ±10 mm in each particular case.

EKSMA Optics Simple Telescope Kit
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Simple lenses are subject to optical aberrations. In many cases these aberrations can be compensated for to a great extent by using a combination of simple lenses with complementary aberrations. A compound lens is a collection of simple lenses of different shapes and made of materials of different refractive indices, arranged one after the other with a common axis.

If two thin lenses are separated in air by some distance d (where d is smaller than the focal length of the first lens), the focal length for the combined system is given by

 

The distance from the second lens to the focal point of the combined lenses is called the back focal length (BFL). If the separation distance is equal to the sum of the focal lengths (d = f1 + f2), the combined focal length and BFL are infinite.

If the separation distance is equal to the sum of the focal lengths (d=f1+f2), the combined focal length and BFL are infinite. This corresponds to a pair of lenses that transform a parallel (collimated) beam into another collimated beam. This type of system is called an afocal system, since it produces no net convergence or divergence of the beam. Two lenses at this separation form the simplest type of optical telescope. Although the system does not alter the divergence of a collimated beam, it does alter the width of the beam. The magnification of such a telescope is given by  

 

which is the ratio of the input beam width to the output beam width. Note the sign convention: a telescope with two convex lenses (f1 > 0, f2 > 0) produces a negative magnification, indicating an inverted image. A concave plus a convex lens (f1 < 0 < f2) produces a positive magnification and the image is upright.