Preview of “ZEISS Microscopy Online ...Opy Basics | Objectives”

Total Page:16

File Type:pdf, Size:1020Kb

Preview of “ZEISS Microscopy Online ...Opy Basics | Objectives” 12/17/12 ZEISS Microscopy Online Campus | Microscopy Basics | Objectives Contact Us | Carl Zeiss Education in Microscopy and Digital Imaging ZEISS Home ¦ Products ¦ Solutions ¦ Support ¦ Online Shop ¦ ZEISS International ZEISS Campus Home Interactive Tutorials Basic Microscopy Spectral Imaging Spinning Disk Microscopy Optical Sectioning Superresolution Introduction Article Quick Links Introduction Live-Cell Imaging The most important imaging component in the optical microscope is the Resolution Fluorescent Proteins objective, a complex multi-lens assembly that focuses light waves Correction originating from the specimen and forms an intermediate image that is Microscope Light Sources Coverslips subsequently magnified by the eyepieces. Objectives are responsible for Digital Image Galleries primary image formation and play a central role in establishing the quality of Specifications Applications Library images that the microscope is capable of producing. Furthermore, the Antireflection magnification of a particular specimen and the resolution under which fine Print Version Reference Library specimen detail also heavily depends on microscope objectives. The most difficult component of an optical microscope to design and assemble, the objective is the first element that light encounters as it passes from the specimen to the image Search plane. Objectives received name from the fact that they are, by proximity, the closest component to the object, or specimen, being imaged. Introduction Image Formation Microscope Resolution Major microscope manufacturers offer a wide range of objective designs that feature excellent optical characteristics under a wide spectrum of illumination conditions and provide various Point-Spread Function degrees of correction for the primary optical aberrations. The objective illustrated in Figure 1 is a Microscope Optical Train 20x multi-immersion media plan-apochromat, which contains 9 optical elements that are Köhler Illumination cemented together into two groups of lens doublets, a movable lens triplet group, and two individual internal single-element lenses. The objective also has a hemispherical front lens and Optical Systems a meniscus second lens, which work synchronously to assist in capturing light rays at high Microscope Objectives numerical aperture with a minimum of spherical aberration. Many high magnification objectives Enhancing Contrast are equipped with a spring-loaded retractable nosecone assembly that protects the front lens elements and the specimen from collision damage. Internal lens elements are carefully oriented Fluorescence Microscopy and tightly packed into a tubular brass housing that is encapsulated by the decorative objective Reflected Light Microscopy barrel. Specific objective parameters such as numerical aperture, magnification, optical tube Reflected Light Contrast length, degree of aberration correction, and other important characteristics are imprinted or engraved on the external portion of the barrel. The objective featured in Figure 1 is designed to zeiss-campus.magnet.fsu.edu/articles/basics/objectives.html 1/7 12/17/12 ZEISS Microscopy Online Campus | Microscopy Basics | Objectives Digital Imaging Basics operate utilizing water, glycerin, or a specialized hydrocarbon-based oil as the imaging medium. Microscope Practical Use In the past 100 years, construction techniques and materials used to manufacture objectives Microscope Ergonomics have greatly improved. Composed up of numerous internal glass lens elements, modern Microscope Care objectives have reached a high state of quality and performance considering the extent of History of the Microscope correction for aberrations and flatness of field. Objectives are currently designed with the assistance of Computer-Aided-Design (CAD) systems, which use advanced rare-element glass formulations of uniform composition and quality characterized by highly specific refractive indices. These advanced techniques have allowed manufacturers to produce objectives that are Microscope Lightpaths very low in dispersion and corrected for most of the common optical artifacts such as coma, astigmatism, geometrical distortion, field curvature, spherical and chromatic aberration. Not only Objective Specifications are microscope objectives now corrected for more aberrations over wider fields, but image flare Optical Pathways has been dramatically reduced thanks to modern coating technologies, with a substantial Microscope Alignment increase in light transmission, yielding images that are remarkably bright, sharp, and crisp. Concept of Magnification Resolution is Determined by the Objective back to top ^ Conjugate Planes Fixed Tube Microscope There are three vital design characteristics of the objective that set the ultimate resolution limit of Infinity Corrected Optics the microscope: The wavelength of light used to illuminate the specimen, the angular aperture of Infinity Optical System the light cone captured by the objective, and the refractive index in the object space between the objective front lens and the specimen. Resolution for a diffraction-limited optical microscope can Field Iris Diaphragm be described as the minimum visible distance between two closely spaced specimen points: Numerical Aperture Airy Disk Formation Resolution = λ/2n(sin(θ)) (1) Spatial Frequency Conoscopic Images where Resolution is the minimum separation distance between two point objects that are clearly Image Resolution resolved, λ is the illumination wavelength, n is the imaging medium refractive index, and θ is equal to one-half of the objective angular aperture. With this in mind, it is apparent that resolution Airy Disk Basics is directly proportional to the illumination wavelength. The human eye responds to the Oil Immersion wavelength region between 400 and 700 nanometers, which represents the visible light Substage Condenser spectrum that is utilized for a majority of microscope observations. Resolution is also dependent upon the refractive index of the imaging medium and the objective angular aperture. Objectives Condenser Aperture are intended to image specimens either through air or a medium of higher refractive index Condenser Light Cones between the front lens and the specimen. The field of view is often highly restricted, and the front Coverslip Thickness lens element of the objective is placed close to the specimen with which it must lie in optical contact. A gain in resolution by a factor of about 1.5 is attained when immersion oil is substituted Focus Depth for air as the imaging medium. Reflected Light Pathways Finally, the last but perhaps most important factor in determining the resolution of an objective is the angular aperture, which has a practical upper limit of about 72 degrees (with a sine value of 0.95). When combined with refractive index, the product: Basic Principles Optical Systems n(sin(θ)) (2) Specimen Contrast Phase Contrast is known as the numerical aperture (NA), and provides an important indicator of the resolution for DIC Microscopy any particular objective. Other than magnification, numerical aperture is generally the most Fluorescence Microscopy important design criteria when considering which microscope objective to choose. Values range from 0.025 for very low magnification objectives (1x to 4x) to as much as 1.6 for high- Polarized Light performance objectives that employ specialized immersion oils. As numerical aperture values Microscope Ergonomics increase for a series of objectives of the same magnification, a greater light-gathering ability and increase in resolution occurs. Under the best circumstances, detail that is just resolved should be enlarged sufficiently to be viewed with comfort, but not to the point that empty magnification obstructs observation of fine specimen detail. The microscopist should carefully choose the numerical aperture of an objective to match the magnification produced in the final image. Magnifications higher than this value will yield no additional useful information (or finer resolution of image detail), and will lead to image degradation. Exceeding the limit of useful magnification causes the image to suffer from empty magnification, where increasing magnification will simply cause the image to become more magnified with no corresponding increase in resolution. Just as the brightness of illumination in a microscope is directed by the square of the working numerical aperture of the condenser, the brightness of an image produced by the objective is determined by the square of its numerical aperture. Additionally, objective magnification also zeiss-campus.magnet.fsu.edu/articles/basics/objectives.html 2/7 12/17/12 ZEISS Microscopy Online Campus | Microscopy Basics | Objectives plays a role in determining image brightness, which is inversely proportional to the square of the lateral magnification. The square of the numerical aperture/magnification ratio expresses the light-gathering power of the objective when used with transmitted illumination. High numerical aperture objectives collect more light and produce a brighter, more corrected image that is highly resolved because they also are often better corrected for aberration. In cases where the light level is a limiting factor (image brightness decreases rapidly as the magnification increases), choose an objective with the highest numerical aperture with the lowest magnification factor capable of producing sufficient resolution. When the objective is assembled, spherical aberration is corrected by selecting the best set of spacers
Recommended publications
  • Sky & Telescope
    S&T Test Report by Rod Mollise Meade’s 115-Millimeter ED Triplet This 4.5-inch apochromat packs a lot of bang for the buck. 115mm Series 6000 THIS IS A GREAT TIME to be in the ice and was eager to see how others market for a premium refracting tele- performed. So when I was approached ED Triplet APO scope. The price for high-quality refrac- about evaluating Meade’s 115mm Series U.S. Price: $1,899 tors has fallen dramatically in recent 6000 ED Triplet APO, I was certainly up meade.com years, and you can now purchase a for the task. 4- to-5-inch extra-low dispersion (ED) First impressions are important, and What We Like apochromatic (APO) telescope that’s when I unboxed the scope on the day Sharp, well-corrected optics almost entirely free of the false color it arrived, I lit up when I saw it. This is Color-free views that plagues achromats for a fraction of Attractive fi nish the cost commonly seen a decade ago. I’ve had a ball with my own recently q The Meade 115mm Series 6000 ED Triplet What We Don’t Like purchased apochromat after using APO ready for a night’s activity, shown with an optional 2-inch mirror diagonal. The scope Visual back locking almost nothing but Schmidt-Cassegrain also accepts fi nderscopes that attach using a system can be awkward telescopes for many years. However, I standardized dovetail system commonly found Focuser backlash still consider myself a refractor nov- on small refractors.
    [Show full text]
  • 31 the Superachromat
    Lesson 31: The Superachromat This lesson will explore a unique feature of SYNOPSYS that can be helpful when you need exceptional color correction, better even than an apochromat. Lesson 8 in this Online Tutorial showed how to select three glass types that make it possible to correct axial color at three wavelengths. For many tasks, that is as good as you will need. But not always. Suppose you are designing a lens to be used over the range 0.4 to 0.9 um. Can you do it with an apochromat? Let’s find out. Here is the RLE file for a starting system, where all surfaces are flat except for the last, which will give us an F/8 telescope objective of 6-inch aperture. (Copy these lines and paste them into the MACro editor.) RLE ID WIDE SPECTRAL RANGE EXAMPLE OBB 0 .25 3 UNITS INCH 1 GLM 1.6 50 3 GLM 1.6 50 5 GLM 1.6 50 6 UMC -0.0625 YMT 7 1 TH .6 2 TH .1 3 TH .6 4 TH .1 5 TH .6 END We did not specify the wavelengths yet, so we get the default CdF lines. We need to change this. Open the Spectrum Wizard (MSW), and change the points indicated. 1 After clicking the Get Spectrum button, click the Apply to lens button. Our lens now has a wider spectrum. Here is our starting lens, in the SketchPad display Uggh! Yes, it’s really awful. Let’s optimize it, varying the glass models. Make a MACro: LOG STO 9 PANT VLIST RAD 1 2 3 4 5 VLIST TH ALL AIR VLIST GLM ALL END AANT END SNAP SYNOPSYS 50 Now put the cursor on the blank line after the AANT command, and click the button .
    [Show full text]
  • A New Refracting Telescope Optical Design in This Article
    THE MELIOR A NePw ROefracCtingH TeleRscopOe OMptical ADesT ign By Joseph Bietry Refracting telescopes have de - veloped over centuries, from the humble beginnings of the Galilean telescope to the modern apochromats of today. Advances in astronomical refractors often came about through improvements to optical materials that offered better control of color er - rors (chromatic aberration). Occa - sionally, a different optical design offered improvements as well. This article will describe a new optical-de - sign form that offers improvements to chromatic aberration, as well as field of view beyond that of current refracting apochromatic telescopes. The name, the Melior Apochro - mat, was chosen for two reasons. First, the English translation for the Latin “melior” is “better” or “im - Figure 1: A simple lens with spherical aberration. proved,” and this is indeed a per - formance improvement over current apochromats. But of more impor - tance to me is that “Meliora” is the motto of my alma mater, the Univer - sity of Rochester. I was lucky enough to have studied lens design at the UR’s Institute of Optics under such greats as Rudolf Kingslake and Robert Hopkins. By using the root of the motto for the naming of this de - sign, I am honoring the University Figure 2: The upper half of a simple lens with spherical aberration. The plot at the right shows and the professors who gave me the the focus error with respect to the position of the ray within the aperture. Astronomy TECHNOLOGY TODAY 69 THE MELIOR APOCHROMAT parallel rays of light entering from the left of the lens represent an infinitely distant point of light (i.e.
    [Show full text]
  • CCAM Objectives.Pdf
    CCAM’s Selection of Zeiss Microscope Objectives Things to consider when selecting an objective 1. Magnification Image scale 2. Resolution The minimum separation distance between two points that are clearly resolved. The resolution of an objective is limited due to diffraction and the nature of light Defined by Abbe’s formula d= l /2NA (l = wavelength of light used, NA = the numerical aperture of the objective) Things to consider when selecting an objective 3. Numerical Aperture (NA) Objective’s ability to collect light and resolve specimen detail at a fixed distance. n = refractive index of medium between front lens element and cover slip. m = ½ the angular aperture (A) (https://micro.magnet.fsu.edu/primer/anatomy/numaperture.html) Things to consider when selecting an objective 3. Numerical Aperture/Refractive index (cont.) • The refractive index is the limiting factor in achieving numerical apertures greater than 1.0. • To obtain a higher numerical aperture, a medium with a higher refractive index must be used. • Highly corrected lenses are designed with higher numerical apertures. Things to consider when selecting an objective 4. Working Distance Distance between the front lens of the objective and the cover glass of the specimen. Note the working distance is reduced with the increase in numerical aperture and magnification. Things to consider when selecting an objective 4. Flatness of Field Correction of field curvature Objectives provide a common focus through the field of view. Such objectives are traditionally named as “plan” Edges in focus Entire field in focus Center in focus https://micro.magnet.fsu.edu/primer/anatomy/fieldcurvature.html Things to consider when selecting an objective 6.
    [Show full text]
  • Chapter 7 Lenses
    Chapter 7 Lenses Chapter 7 Lenses © C. Robert Bagnell, Jr., Ph.D., 2012 Lenses are the microscope’s jewels. Understanding their properties is critical in understanding the microscope. Objective, condenser, and eyepiece lenses have information about their properties inscribed on their housings. Table 7.1 is an example from objective lenses. This chapter will unfold the meaning and significance of these symbols. The three main categories of information are Numerical Aperture, Magnification / Tube Length, and Aberration Corrections. Zeiss Leitz Plan-Apochromat 170/0.17 63X/1.40 Oil Pl 40 / 0.65 ∞/0.17 Nikon Olympus Fluor 20 Ph3 ULWD CDPlan 40PL 0.75 0.50 160/0.17 160/0-2 Table 7.1 – Common Objective Lens Inscriptions Numerical Aperture & Resolution Figure 7.1 Inscribed on every objective lens and most 3 X condenser lenses is a number that indicates the lenses N.A. 0.12 resolving power – its numerical aperture or NA. For the Zeiss lens in table 7.1 it is 1.40. The larger the NA the better the resolving power. Ernst Abbe invented the concept of numerical aperture in 1873. However, prior to Abbe’s quantitative formulation of resolving power other people, such as Charles Spencer, intuitively understood the underlying principles and had used them to produce 1 4˚ superior lenses. Spencer and Angular Aperture 95 X So, here is a bit about Charles Spencer. In the mid N.A. 1.25 1850's microscopists debated the relationship of angular aperture to resolution. Angular aperture is illustrated in 110˚ Pathology 464 Light Microscopy 1 Chapter 7 Lenses figure 7.1.
    [Show full text]
  • Microscope Objectives for Biomed Applications
    Microscopy from Carl Zeiss LSM 5 Family Objectives for Your Biomedical Applications Whether your research subject is in cell biology, developmental biology, neuro- biology or physiology, Zeiss offers you a wide range of objectives to fit the special properties of your specimen and the LSM. This brochure presents a selection of the best Zeiss objectives for LSM use, sorted by type of usage and correction properties. It is intended as a help for choosing the right objectives for your LSM, in order to guarantee the best possible image results. Confocal Laser Scanning Microscopy Multiphoton Laser Scanning Microscopy Fluorescence Correlation Spectroscopy Why Special Objectives for Confocal Microscopy ? In confocal microscopy, the requirements for objective design and quality are much higher than in conven- tional light microscopy. Due to the ability to obtain optical sections in Z and to collect high resolution data of one point in the specimen at various wavelengths Maximum quality of point spread func- tions (PSF) in conventional (wide field) simultaneously, confocal microscope objectives need a microscopy and in confocal microscopy. perfect correction of longitudinal chromatic and spherical The almost ideal PSF in confocal microscopy is only available, of course, errors over the full wavelength range. if perfectly corrected (”diffraction limited“) objectives are used. conventional confocal 10 10 0 0 lateral position,lateral normalized [µm] lateral position,lateral normalized [µm] 10 10 200 20 200 20 axial position, normalized [µm] axial position, normalized [µm] Specimen matching objectives regarding coverslip, media correction and working distances Subject optical dry water oil water property immersion immersion dipping Cell Biology covered, Pl-Neofluar, C-Apochromat Pl-Apochromat, Microbiology thin Fluar, Plan LD Neofluar, Fluar Developmental covered, Plan LD 40x C-Apochromat Pl-Neofluar 25x Biology in dish etc.
    [Show full text]
  • Measuring Chromatic Aberrations in Imaging Systems Using Plasmonic Nano‐Particles
    Measuring chromatic aberrations in imaging systems using plasmonic nano‐particles Sylvain D. Gennaro, Tyler R. Roschuk, Stefan A. Maier, and Rupert F. Oulton* Department of Physics, The Blackett Laboratory, Imperial College London, SW7 2AZ, London UK *Corresponding author: [email protected] Chromatic aberration in optical systems arises from the wavelength dependence of a glass’s refractive index. Polychromatic rays incident upon an optical surface are refracted at slightly different angles and in traversing an optical system follow distinct paths creating images displaced according to color. Although arising from dispersion, it manifests as a spatial distortion correctable only with compound lenses with multiple glasses and accumulates in complicated imaging systems. While chromatic aberration is measured with interferometry1,2 simple methods are attractive for their ease of use and low cost3,4. In this letter we retrieve the longitudinal chromatic focal shift of high numerical aperture (NA) microscope objectives from the extinction spectra of metallic nanoparticles5 within the focal plane. The method is accurate for high NA objectives with apochromatic correction, and enables rapid assessment of the chromatic aberration of any complete microscopy systems, since it is straightforward to implement. A straightforward approach for measuring the longitudinal chromatic aberration of an imaging system involves scanning a pin‐hole3 or the confocal image of an optical fibre4 through a lens’s focal plane so that colours in focus record a stronger transmission. The accuracy of these aperture‐based measurements requires spatially filtering colors that are out of focus. Therefore, a smaller aperture should increase the sensitivity of these methods as it acts as a point‐spread function for the measurement.
    [Show full text]
  • Objective Lenses for Material Science
    Objective Lenses for Material Science This is a series of objective lenses designed for metallurgical microscopes. The user can choose any of the lenses according to the observation method or application specific to chromatic aberration, flatness, etc. 1) MPLAPON This is a Plan Apochromat objective lens series for bright field observation with chromatic aberration corrected at the highest level. This series guarantees optical performance (Wavefront Aberration Correction) at a Strehl ratio of 95% or more and is also compatible with the AF unit (Olympus U-AFA2M). Plan Apochromat 2) MPLN This is a Plan Achromat objective lens series that has attained excellent flatness up to a field number of 22. Plan Achromat 3) MPLN-BD This is a Plan Achromat objective lens series for bright field and dark field observations that has attained excellent flatness up to a field number of 22. Brightfield/Darkfield Plan Achromat 4) MPLFLN This is a universal objective lens series of a semi-apochromat design with chromatic aberration corrected at a high level. This series provides excellent performance not only in bright field, but also in fluorescence, differential interference contrast, and simple polarized observations. Plan Semi-Apochromat 5) MPLFLN-BD This is a universal bright field/dark field objective lens series of a semi-apochromat design with chromatic aberration corrected at a high level. This series provides excellent performance not only in bright field and dark field, but also in fluorescence, differential interference contrast, and simple polarized observations. Brightfield/Darkfield Plan Semi-Apochromat 6) MPLFLN-BDP This is a universal objective lens series that provides high optical performance particularly in polarized, differential interference contrast observations.
    [Show full text]
  • Microscope Objectives Our Objectives Help You Focus on Yours
    Microscope objectives Our objectives help you focus on yours Nikon is a leader in the development and manufacture of optical and digital imaging technology for advanced science and clinical research. With over a 100-year history of optical excellence, Nikon is committed to accelerating innovation in science and clinical imaging to improve healthcare and provide a better quality of life. Nikon’s first microscope, released in 1925 2 The switch from traditional film photography to digital imaging was a major milestone in the field of microscopy, opening up new possibilities in both application and technology. Introduction of digital imaging spurred significant technological changes including the development of objectives with enhanced optical quality and functionality to meet the new demands. Objective lenses are arguably the most important element in the microscope and Nikon continues to invest heavily in the development of objectives to meet the changing demands of science. Explore some of Nikon's newest developments in high-performance objectives in this brochure. 3 In tireless pursuit of the highest quality Each Nikon microscope objective is precision-crafted to provide the highest level of clarity and overall optical performance. World-class Nikon objectives, including the renowned CFI60 infinity optical system, deliver brilliant images of breathtaking sharpness and clarity, from ultralow to the highest magnifications. The initial melting process after blending glass raw materials 4 It Starts with the Glass Nikon has been developing optical glass since its inception in 1917, and to this day, wholly owns and formulates all of its glass. Optical glass starts as an ingot (shown on right) which is formed by blending rare earth elements and repeated melting, shaping and slow cooling to achieve a target refractive index.
    [Show full text]
  • Case File Copy
    H . PREPRINTS OF THE STEWARD OBSERVATORY THE UNIVERSITY OF ARIZONA TUCSON, ARIZONA CASE FILE A 1:1 APOCHROMAT TRANSFER LENS SYSTECOPM Y W. G. Tifft R. A. Buchroeder December 1, 1971 T 71-20 A 1:1 APOCHROMAT TRANSFER LENS SYSTEM by W. G. Tifft R. A. Buchroeder Steward Observatory University of Arizona Tucson, Arizona December 1, 1971 T 71-20 INTRODUCTION Work on the IDCADS project (Image Dissector Control and Data System) has been conducted by the Space Astronomy group of Steward Observatory under NASA Contract NSR 03-002-163 and NASA Grant NCR 03-002-153. One of the tasks has been the development of a remote control instrumentation system for use with large telescopes, with emphasis on future application to space telescopes. A prototype system has been constructed for use with the University of Arizona 90-Inch Telescope on Kitt Peak. The system uses image dissector tubes, a conventional photocell, and photographic plates as detectors for images formed at the Cassegrain focus of the 90-inch telescope. It proved to be impossible to physically locate all of the detector devices directly at the focal plane in the developmental instrument; therefore, it was decided to use an image relay system to transfer selected portions of the image plane to image dissectors and the photographic plate. This report describes the design of a 1:1 relay system for use with the IDCADS. Design considerations are discussed, alternate designs are outlined, and the "optimum" design is discussed in detail. The design was a joint effort between the Space Astronomy group and the Optical Design group of the Optical Sciences Center of the University of Arizona.
    [Show full text]
  • The Magazine from Carl Zeiss in Memory of Ernst Abbe
    INNO_TS/RS_E_15.qxd 15.08.2005 10:35 Uhr Seite III InnovationThe Magazine from Carl Zeiss ISSN 1431-8059 15 In Memory of Ernst Abbe Inhalt_01_Editorial_E.qxd 15.08.2005 9:07 Uhr Seite 2 Contents Editorial Formulas for Success. ❚ Dieter Brocksch 3 In Memory of Ernst Abbe Ernst Abbe 4 Microscope Lenses 8 Numerical Aperture, Immersion and Useful Magnification ❚ Rainer Danz 12 Highlights from the History of Immersion Objectives 16 From the History of Microscopy: Abbe’s Diffraction Experiments ❚ Heinz Gundlach 18 The Science of Light 24 Stazione Zoologica Anton Dohrn, Naples, Italy 26 Felix Anton Dohrn 29 The Hall of Frescoes ❚ Christiane Groeben 30 Bella Napoli 31 From Users The Zebra Fish as a Model Organism for Developmental Biology 32 SPIM – A New Microscope Procedure 34 The Scourge of Back Pain – Treatment Methods and Innovations 38 ZEISS in the Center for Book Preservation ❚ Manfred Schindler 42 Across the Globe Carl Zeiss Archive Aids Ghanaian Project ❚ Peter Gluchi 46 Prizes and Awards 100 Years of Brock & Michelsen 48 Award for NaT Working Project 49 Product Report Digital Pathology: MIRAX SCAN 50 UHRTEM 50 Superlux™ Eye Xenon Illumination 50 Carl Zeiss Optics in Nokia Mobile Phones 51 Masthead 51 2 Innovation 15, Carl Zeiss AG, 2005 Inhalt_01_Editorial_E.qxd 15.08.2005 9:07 Uhr Seite 3 Editorial Formulas for Success... Formulas describe the functions and processes of what It clearly and concisely describes the resolution of optical happens in the world and our lives. It is often the small, instruments using the visible spectrum of light and con- insignificant formulas in particular that play a decisive tributed to the improvement of optical devices.
    [Show full text]
  • Half a Year with Baader 95/560Mm Apochromat
    Half a year with Baader 95/560mm apochromat For about half year, I was enjoying 95mm gether in binoviewers. As a result, unlike Baader apochromat. I admit, I'm hopeless the majority of observers, I prefer single eye refractor lover. It went that far that I have viewing. This is how I was using the tele- designed even my own lens. It is long 82mm scope most of the time. f/20 oil doublet based on short flint, not un- like the first apochromats made by Zeiss still Optical performance in 19th century1. After some time, I was contacted by I'm not really a person that makes system- equally enthusiastic observer from Ger- atic evaluation of telescopes or eyepieces. I many. He was interested in my oil doublet rather like to use the equipment for observ- and in exchange for it he made generous of- ing, as my time under the night skies is quite fer - I could play for couple of months with limited. At least, I keep a habit of star test- his Baader 95mm apochromat. I heard ru- ing new telescope as the test is quick and mors about this oil fluorite triplet before quite informative. I could not see any opti- and I could not resist the offer. After all, cal aberration worth to be mentioned. Sim- with this refractor, Baader was building on ply perfect. Zeiss experiences with their now legendary To further evaluate the performance, I APQ lenses. checked several double stars. I was pleased, I have never looked through a fluorite lens to see the very first night not only E com- and I was curious about its performance.
    [Show full text]