DOCSLIB.ORG

Optical Engineering 2.6 Magnifying Glass and Basic Microscope 2.7 Modern Microscopes 2.8 Beam Expansion 2.9 Telescopes Martina Gerken 15.11.2007 2.10 Optic Design 2

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
Optical Engineering 2.6 Magnifying Glass and Basic Microscope 2.7 Modern Microscopes 2.8 Beam Expansion 2.9 Telescopes Martina Gerken 15.11.2007 2.10 Optic Design 2 3.2 Course outline 1. Imaging optics 2.1 Light propagation across interfaces 2.2 Photography and optical lenses 2.3 Aberrations 2.4 Plane parallel plates and reflective prisms 2.5 Depth of focus Optical Engineering 2.6 Magnifying glass and basic microscope 2.7 Modern microscopes 2.8 Beam expansion 2.9 Telescopes Martina Gerken 15.11.2007 2.10 Optic design 2. Optical sensors 3. Optics in data storage 4. Introduction to displays 5. Fourier optics 6. Diffractive optics and holograms 7. Integrated optics Universität Karlsruhe (TH) 8. Computerized imaging 3.3 3.4 Exercise Magnification • Evaluate the following optical systems to obtain an upright, magnified image • Generation of upright, magnified image of an LED chip at a given distance! Object Magnifi- Group Lens 1 Lens distance Lens 2 distance cation Lens 1 Lens 2 20 mm 40 mm 1 25 mm 117 mm 6x B2 (planoconvex) (planoconvex) 15 mm 60 mm 2 25 mm 155 mm 2.5x G1 (planoconvex) (biconvex) 16 mm 60 mm B1 3 30 mm (combined 165 mm (combined 2.5x convex) convex) f1 f2 10 mm 60 mm b 4 16 mm 125 mm 5x g1 b1 g2 2 (biconvex) (planoconvex) 25 mm 60 mm 5 26 mm 177 mm 5x (convex) (convex) • Suggest an improved system! 3.5 3.6 2-stage imaging with scattering screen 2-stage imaging with field lens • For 2-stage imaging with only two lenses second lens needs to be large to • For 2-stage imaging with only two lenses second lens needs to be large to capture light from all object points capture light from all object points • Solution 1: Include scattering screen • Solution 2: Include field lens at position of intermediate image – Image of entire object – Entire object visible in bright image – Image dark as light scattered in all directions – Disadvantage: dirt on field lens is also imaged Object Intermediate image Image Losses Object Intermediate image + field lens Image Object Intermediate image Image + scattering screen Source: Schröder/Treiber, Technische Optik Source: Schröder/Treiber, Technische Optik 3.7 3.8 Magnifying glass – Calculation of magnification Microscope – Calculation of magnification • For unstrained viewing, eye adapted to infinity and intermediate image at focal • For unstrained viewing, object at single focal length and eye adapted to infinity length of ocular • Tube length is distance between focal plane of objective and focal plane of ocular (typical value 20 cm) Objective Ocular G Lens Lens α0 a G’ s a G α G Intermediate Α α f a image M = M = = s G f f t („Tube length“) f f α0 f Objective Objective Ocular Ocular Lens as G' t + fObj ⎛ 1 1 ⎞ t G M = = = t + f ⎜ − ⎟ = obj ()Obj ⎜ ⎟ G a fObj t + fObj fObj αΑ ⎝ ⎠ Object t as M tot = M obj M ocu = f f fObj fOcu 3.9 3.10 Oculars Course outline • Ocular combines field lens and eye lens 1. Imaging optics • Modern microscopes mostly use positive oculars, i.e., oculars forming real 2.1 Light propagation across interfaces image 2.2 Photography and optical lenses – For negative oculars with virtual image it is not possible to include markers 2.3 Aberrations and image is not delimited well 2.4 Plane parallel plates and reflective prisms 2.5 Depth of focus 2.6 Magnifying glass and basic microscope 2.7 Modern microscopes 2.8 Beam expansion 2.9 Telescopes 2.10 Optic design 2. Optical sensors 3. Optics in data storage 4. Introduction to displays 5. Fourier optics 6. Diffractive optics and holograms 7. Integrated optics 8. Computerized imaging Source: Schröder/Treiber, Technische Optik 3.11 3.12 Exercise: Beam expansion Basic beam expansion systems • To achieve high resolution many imaging systems employ beam expansion • Beam expansion systems are telescopes! – Minimum resolvable angle: • Two basic principles λ ∆φmin = 1.22 [rad] Galilei-telescope D • Principle: Collimated beam is transformed to collimated beam with larger diameter • Design the optics for a 2-lens beam expansion system! • Build your beam expansion system! Objective Optical axis Beam path • Characterize your beam expansion system! – Focal lengths and diameter of lenses – Distance between lenses – Final beam diameter D – Losses – Expansion ratio • Calculate the minimum resolvable angle! Kepler-telescope –2π rad = 360°; 1° = 60′ (Arc minutes); 1′ = 60″ (Arc seconds) Source: http://de.wikipedia.org/ 3.13 3.14 Course outline Kepler-Telescope 1. Imaging optics • Goal: Magnicifaction of distant objects 2.1 Light propagation across interfaces • Most telescopes are afocal systems: Object at negative infinity is imaged to positive infinity 2.2 Photography and optical lenses • Focal points of objective and ocular at same position 2.3 Aberrations 2.4 Plane parallel plates and reflective prisms 2.5 Depth of focus 2.6 Magnifying glass and basic microscope 2.7 Modern microscopes 2.8 Beam expansion 2.9 Telescopes 2.10 Optic design 2. Optical sensors f f 3. Optics in data storage Objective Ocular 4. Introduction to displays Source: http://de.wikipedia.org/ 5. Fourier optics 6. Diffractive optics and holograms fObjektiv 7. Integrated optics • Magnification given by: M = 8. Computerized imaging fOkular 3.15 3.16 Telescope: Refractor Telescope: Reflector • Kepler telescope • Newton-telescope – Combination of two convex lenses – Parabolic main mirror to correct for spherical aberration – Correction of chromatic aberration: Use of additional concave lens – Limited field of view due to aberrations for oblique incidence angles (achromatic objective) – Second mirror reduces resolution due to diffraction Convex lens Secondary mirror Concave lens Ocular Primary mirror 3.17 3.18 Terrestrial telescopes Which Christmas present? • BRASKO 60700 telescope • For observation of terrestrial objects often upright image is desired • “High quality refractor-telescope with many extras” – May be obtained by additional lens or prism system Includes equipment for terrestrial observation (Umkehrlinse), moon filter, Barlow-lens, stable mount with tray, holder of oculars and much more. – Focal length 700 mm – Objective-diameter 60 mm – Maximum resolution 525x – Price: EUR 99,95 Source: http://www.amazon.de 3.19 3.20 Which Christmas present? Compilation of questions • Bresser telescope Pluto 114/500 • Lay out a 2-stage magnification system with an upright image! • “Large Newton reflector telescope in compact layout. For observations • What is the function of a field lens? within and outside our solar system” • Where is the field lens placed in an optical system? – Focal length 500 mm • Calculate the magnification of a magnifying glass with a 62,5 mm focal length – Objective / Mirror ø114 mm lens! – Maximum magnification 25x - 250x • Sketch an optical system to achieve beam expansion! – Price: 134,00 € • Derive the magnification of a Kepler telescope! • Decide until next Thursday which telescope you buy and list your arguments! Source: http://www.das-fernglas.de.
Load more

Recommended publications
  • Ira Sprague Bowen Papers, 1940-1973
    http://oac.cdlib.org/findaid/ark:/13030/tf2p300278 No online items Inventory of the Ira Sprague Bowen Papers, 1940-1973 Processed by Ronald S. Brashear; machine-readable finding aid created by Gabriela A. Montoya Manuscripts Department The Huntington Library 1151 Oxford Road San Marino, California 91108 Phone: (626) 405-2203 Fax: (626) 449-5720 Email: [email protected] URL: http://www.huntington.org/huntingtonlibrary.aspx?id=554 © 1998 The Huntington Library. All rights reserved. Observatories of the Carnegie Institution of Washington Collection Inventory of the Ira Sprague 1 Bowen Papers, 1940-1973 Observatories of the Carnegie Institution of Washington Collection Inventory of the Ira Sprague Bowen Paper, 1940-1973 The Huntington Library San Marino, California Contact Information Manuscripts Department The Huntington Library 1151 Oxford Road San Marino, California 91108 Phone: (626) 405-2203 Fax: (626) 449-5720 Email: [email protected] URL: http://www.huntington.org/huntingtonlibrary.aspx?id=554 Processed by: Ronald S. Brashear Encoded by: Gabriela A. Montoya © 1998 The Huntington Library. All rights reserved. Descriptive Summary Title: Ira Sprague Bowen Papers, Date (inclusive): 1940-1973 Creator: Bowen, Ira Sprague Extent: Approximately 29,000 pieces in 88 boxes Repository: The Huntington Library San Marino, California 91108 Language: English. Provenance Placed on permanent deposit in the Huntington Library by the Observatories of the Carnegie Institution of Washington Collection. This was done in 1989 as part of a letter of agreement (dated November 5, 1987) between the Huntington and the Carnegie Observatories. The papers have yet to be officially accessioned. Cataloging of the papers was completed in 1989 prior to their transfer to the Huntington.
    [Show full text]
  • The Celestron Edgehd a Flexible Imaging Platform at an Affordable Price
    A FLEXIBLE IMAGING PLATFORM AT AN AFFORDABLE PRICE Superior flat-field, coma-free imaging by the Celestron Engineering Team Ver. 04-2013, For release in April 2013. The Celestron EdgeHD A Flexible Imaging Platform at an Affordable Price By the Celestron Engineering Team ABSTRACT: The Celestron EdgeHD is an advanced, flat-field, aplanatic A skilled optician in a well-equipped optical shop can reliably series of telescopes designed for visual observation and imaging produce near-perfect spherical surfaces. Furthermore, by with astronomical CCD cameras and full-frame digital SLR comparing an optical surface against a matchplate—a precision cameras. This paper describes the development goals and reference surface—departures in both the radius and sphericity design decisions behind EdgeHD technology and their practical can be quickly assessed. realization in 8-, 9.25-, 11-, and 14-inch apertures. We include In forty years of manufacturing its classic Schmidt-Cassegrain cross-sections of the EdgeHD series, a table with visual and telescope, Celestron had fully mastered the art of making imaging specifications, and comparative spot diagrams for large numbers of essentially perfect spherical primary and the EdgeHD and competing “coma-free” Schmidt-Cassegrain secondary mirrors. designs. We also outline the construction and testing process for EdgeHD telescopes and provide instructions for placing sensors In addition, Celestron’s strengths included the production of at the optimum back-focus distance for astroimaging. Schmidt corrector plates. In the early 1970s, Tom Johnson, Celestron’s founder, perfected the necessary techniques. Before Johnson, corrector plates like that on the 48-inch 1. INTRODUCTION Schmidt camera on Palomar Mountain required many long The classic Schmidt-Cassegrain telescope (SCT) manufactured hours of skilled work by master opticians.
    [Show full text]
  • A Guide to Smartphone Astrophotography National Aeronautics and Space Administration
    National Aeronautics and Space Administration A Guide to Smartphone Astrophotography National Aeronautics and Space Administration A Guide to Smartphone Astrophotography A Guide to Smartphone Astrophotography Dr. Sten Odenwald NASA Space Science Education Consortium Goddard Space Flight Center Greenbelt, Maryland Cover designs and editing by Abbey Interrante Cover illustrations Front: Aurora (Elizabeth Macdonald), moon (Spencer Collins), star trails (Donald Noor), Orion nebula (Christian Harris), solar eclipse (Christopher Jones), Milky Way (Shun-Chia Yang), satellite streaks (Stanislav Kaniansky),sunspot (Michael Seeboerger-Weichselbaum),sun dogs (Billy Heather). Back: Milky Way (Gabriel Clark) Two front cover designs are provided with this book. To conserve toner, begin document printing with the second cover. This product is supported by NASA under cooperative agreement number NNH15ZDA004C. [1] Table of Contents Introduction.................................................................................................................................................... 5 How to use this book ..................................................................................................................................... 9 1.0 Light Pollution ....................................................................................................................................... 12 2.0 Cameras ................................................................................................................................................
    [Show full text]
  • To Photographing the Planets, Stars, Nebulae, & Galaxies
    Astrophotography Primer Your FREE Guide to photographing the planets, stars, nebulae, & galaxies. eeBook.inddBook.indd 1 33/30/11/30/11 33:01:01 PPMM Astrophotography Primer Akira Fujii Everyone loves to look at pictures of the universe beyond our planet — Astronomy Picture of the Day (apod.nasa.gov) is one of the most popular websites ever. And many people have probably wondered what it would take to capture photos like that with their own cameras. The good news is that astrophotography can be incredibly easy and inexpensive. Even point-and- shoot cameras and cell phones can capture breathtaking skyscapes, as long as you pick appropriate subjects. On the other hand, astrophotography can also be incredibly demanding. Close-ups of tiny, faint nebulae, and galaxies require expensive equipment and lots of time, patience, and skill. Between those extremes, there’s a huge amount that you can do with a digital SLR or a simple webcam. The key to astrophotography is to have realistic expectations, and to pick subjects that are appropriate to your equipment — and vice versa. To help you do that, we’ve collected four articles from the 2010 issue of SkyWatch, Sky & Telescope’s annual magazine. Every issue of SkyWatch includes a how-to guide to astrophotography and visual observing as well as a summary of the year’s best astronomical events. You can order the latest issue at SkyandTelescope.com/skywatch. In the last analysis, astrophotography is an art form. It requires the same skills as regular photography: visualization, planning, framing, experimentation, and a bit of luck.
    [Show full text]
  • Historyofthetelescope
    HISTORY OF THE TELESCOPE Pedro Ré http://pedroreastrophotography.com/ Contents Joseph von Fraunhofer (1787 - 1826) and the Great Dorpat refractor .................................................. 3 Alvan Clark (1804-1887), George Bassett Clark (1827-1891) and Alvan Graham Clark (1832-1897): American makers of telescope optics. .................................................................................................. 13 William Parsons (1800-1867) e o Leviatã de Parsonstown (in Portuguese) ......................................... 21 O Telescópio de Craig (1852) (in Portuguese) ...................................................................................... 29 The 25-inch Newall Refractor ............................................................................................................... 37 The Kew Photoheliograph ..................................................................................................................... 43 O Grande Telescópio de Melbourne (in Portuguese) ........................................................................... 51 O Grande Refractor da Exposição de Paris (1900) (in Portuguese) ...................................................... 61 William Lassell’s (1799-1880) Telescopes and the discovery of Triton ................................................ 71 James Nasmyth’s (1808-1890) telescopes ............................................................................................ 77 The 36-inch Crosley Reflector ..............................................................................................................
    [Show full text]
  • A Barlow Lens Increases the Focal Length of a Telescope Without Increasing the Physical Length Correspondingly
    A Barlow lens increases the focal length of a telescope without increasing the physical length correspondingly. It is a useful way of obtaining higher magnifications without using very short focal length eyepieces. Barlow lenses used to be sold with a specified focal length. The lens was fitted into a cell, within a tube that could be slid into the drawtube. The increase in the focal length could be varied by altering the separation between the Barlow lens and eyepiece. Now, because telescope focusers tend not to have drawtubes, they are sold with a specified, and usually fixed, amplification. Spacer tubes may be supplied to change the amplification. The Barlow lens is negative, and needs to be achromatized, to maintain the spherical and chromatic correction of the telescope objective. The change in the focal length is given by the universal lens formula: 1 1 1 = − f u v where f is the lens focal length v is the object distance u is the image distance € Defining Barlow lens parameters as the negative focal length B, distance inside the prime focus D, and separation between Barlow lens and effective focus S, 1 1 1 = − B S D € and when the negative focal length B is known, can be rearranged in terms of D: SB D = S + B S Image amplification is given by A = D € from which S = B(A −1) The increase in telescope€ tube length is S − D. The Barlow lens cannot be€ placed inside the prime focus by more than its focal length. If placed at its focal length inside prime focus the effective focus becomes infinite.
    [Show full text]
  • Telescope Instruction Manual
    Telescope Instruction Manual 78-9500 60mm RefraCtor Lit. #: 91-0264/08-01 Never Look Directly At The Sun With Your Telescope Permanent Damage To Your Eyes May Occur 2. WHERE DO I START? Your Bushnell telescope can bring the wonders of the universe to your eyes. While this manual is intended to assist you in the set-up and basic use of this instrument, it does not cover everything you might like to know about astronomy. Although Northstar will give a respectable tour of the night sky, it is recommended you obtain a very simple star chart and a flashlight with a red bulb or red cellophane over the end. For objects other than stars and constellations, a basic guide to astronomy is a must. Some recommended sources appear on our website at www.bushnell.com. Also on our website will be current events in the sky for suggested viewing. But, some of the standbys that you can see are: The Moon—A wonderful view of our lunar neighbor can be enjoyed with any magnification. Try viewing at different phases of the moon. Lunar highlands, lunar maria (lowlands called "seas" for their dark coloration), craters, ridges and mountains will astound you. Saturn—Even at the lowest power you should be able to see Saturn’s rings and moons. This is one of the most satisfying objects in the sky to see simply because it looks like it does in pictures. Imagine seeing what you’ve seen in textbooks or NASA images from your backyard! Jupiter—The largest planet in our solar system is spectacular.
    [Show full text]
  • The Barlow Lens
    No. 508 Registered Charity 271313 May 2015 OASI News The newsletter of the Orwell Astronomical Society The extended corona Photo by Paul Whiting FRAS Trustees: Mr Roy Adams Mr David Brown Mr David Payne Honorary President: Dr Allan Chapman D.Phil MA FRAS 1505OASINews Page 1 of 28 oasi.org.uk The UK Partial Solar Eclipse Neil J Short A mosaic from the recent Partial Solar Eclipse – no tracked mount so it was a simple manual camera mount, a very old EOS300 camera The Partial Solar Eclipse 20th March 2015 and an 80mm Leicester Forest Service Station 80mm Refractor with Solar Filter; Canon EOS300 Camera refractor with a glass solar filter. Then it was into Photoshop for the mosaic. I was journeying north up the M1 (with telescope just in case) and finally hit sunshine at just south of Leicester – so this was taken in the car park of the Leicester North Services on the M1. I had missed first contact – first picture was just before 9:00 a.m. but carried on until last contact. Page 2 of 28 1505OASINews oasi.org.uk Contents ! Cover picture: Total Solar Eclipse!...............................................................................1 ! Inside cover pics: The UK Partial Solar Eclipse!..........................................................2 Society Contact details!...............................................................................................4 Access into the School Grounds and Observatory Tower! 4 Articles for OASI News!...............................................................................................4 Ipswich
    [Show full text]
  • Orion Barlow Lenses
    INSTRUCTION MANUAL ORION® BARLOW LENSES Francais ➊Pour obtenir le manuel d'utilisation complet, veuillez vous rendre sur le site Web OrionTelescopes.eu/fr et saisir la référence du produit dans la barre de recherche. ➋Cliquez ensuite sur le lien du manuel d’utilisation du produit sur la page de de- scription du produit. Deutsche ➊Wenn Sie das vollständige Handbuch einsehen möchten, wechseln Sie zu OrionTelescopes.de, und geben Sie in der Suchleiste die Artikelnummer der Orion-Kamera ein. ➋Klicken Sie anschließend auf der Seite mit den Produktdetails auf den Link des entspre- chenden Produkthandbuches. Español ➊ Para ver el manual completo, visite Orion- An Orion barlow lens is a simple concave (negative) lens that amplifies the magnifying power of Telescopes.eu y escriba el número de artí- culo del producto en la barra de búsqueda. any telescope eyepiece it’s used with. It works by reducing the convergence of the light cone heading into the eyepiece. In this way it increases the focal length of the telescope. Since mag- nification is determined by dividing the telescope’s focal length by the eyepiece’s focal length, you can see that by doubling the telescope’s focal length, a 2x barlow lens doubles the magni- ➋A continuación, haga clic en el enlace al manual del producto de la página de detalle fication of the system for a given eyepiece. del producto. In this way, a 2x barlow can effectively double the number of magnifications available to you from a set of eyepieces. For example, if you have eyepieces with focal lengths of 26mm, 18mm, and 10mm, using a 2x barlow will give you the equivalent of 13mm, 9mm, and 5mm eyepieces—like getting three more eyepieces for the price of one barlow! Corporate Offices: 89 Hangar Way, Watsonville CA 95076 - USA Toll Free USA & Canada: (800) 447-1001 International: +1(831) 763-7000 Customer Support: [email protected] AN EMPLOYEE-OWNED COMPANY Copyright © 2020 Orion Telescopes & Binoculars.
    [Show full text]
  • Telescope Eyepieces
    Telescope Eyepieces Mike Swanson Eyepiece Basics • The main purpose of the • For example, a scope with eyepiece is to magnify the 1000mm focal length is used image produced by the with a 10mm eyepiece, objective of the telescope. resulting in a magnification • Eyepieces come in various of 100x (1000/10). focal lengths measured in • Prices range from about $20 millimeters (mm). to several hundred dollars. • The magnification provided • Good quality eyepieces are by an eyepiece is determined “multicoated”, better quality by dividing the focal length eyepieces are “fully of the telescope (also multicoated”. measured in mm) by the • Some eyepiece sets are focal length of the eyepiece. parfocal - very little refocusing required when Scope Calculator switching from one eyepiece to another. Eyepiece Basics • Eyepieces come in three • Some eyepieces are heavy sizes: .965”, 1.25” and 2”, and unbalance small scopes. which indicates the size of • The eye relief of an eyepiece the barrel that fits into the indicates the farthest focuser tube (part of the distance your eye can be scope itself). from the first lens and still • The .965 variety is only take in the entire field of available in low quality view (FOV). eyepieces and must be • With most eyepiece designs, avoided. the shorter the focal length, • The majority of eyepieces the shorter the eye relief. are 1.25”. • If you must wear glasses • The 2” models are to allow when using a scope for a wider field of view on (necessary if you have low power eyepieces. astigmatism), a long eye relief will be required. Field of View (FOV) • The amount of sky we can • Eyepieces have a see through a telescope (or characteristic known as binoculars) is measured in Apparent FOV (AFOV).
    [Show full text]
  • Introduction to Telescopes
    Name(s): _____________________________ _____________________________ _____________________________ _____________________________ Date: __________________ Course/Section: __________________ Grade: __________________ Introduction to Telescopes Objectives: Students will study telescope optics and assemble a simple telescope. Students will also learn how to set up and properly align a tripod-mounted telescope for nighttime viewing. Checklist: □ Complete the pre-lab quiz with your team (if required). □ Compile a list of resources you expect to use in the lab. □ Work with your team to complete the lab exercises and activities. □ Record your results and mark which resources you used. □ Share and discuss your results with the rest of the class. □ Determine if your team’s answers are reasonable. □ Submit an observation request for next week (if required). Pre-Lab Quiz Record your Group's answers to each question, alonG with your reasoninG. These concepts will be relevant later in this lab exercise. 1. 2. 3. 4. Part 1: The Galileoscope 1. What are some of the differences between refractinG and reflectinG telescopes? (DrawinG a diagram may be helpful.) 2. Is the Galileoscope a refractinG or reflectinG telescope? What kinds of celestial objects would you be able to see with it? What kinds of objects would not be ideal for observinG with the Galileoscope? 3. What is an example of a reflectinG telescope? 4. Why does the objective lens of the Galileoscope consist of two separate lenses fused toGether? You may need to research this answer. 5. Find and explain your method for determininG the focal lenGth of the objective lens. (You will need this answer for later.) 6. Describe the view usinG the Galilean eyepiece.
    [Show full text]
  • Instruction Manual for 707Az2
    INSTRUCTION MANUAL FOR 707AZ2 Optical Tube: 70mm/700mm Alt-Azimuth Mount: AZ2 Finderscope Telescope Main Tube Finderscope Bracket Objective Lens Finderscope Alignment Dew Cap / Sun Shade Screws Focus Locking Screw Dust Cap / Mask (Remove before Viewing) Eyepiece Yoke Locking Knob Altitude Lock Knob Yoke Mount Diagonal Focus Tube Focus Knob Altitude Fine-adjustment Control Azimuth Lock Knob Accessory Tray Tripod Leg Height Adjustment Clamp TABLE OF CONTENTS Assembling Your Telescope 3 Tripod Set up 3 Telescope Assembly 3 Finderscope Assembly 4 Eyepiece Assembly 4 Alligning the Finderscope 4 Operating Your Telescope 5 Operating the AZ2 Mount 5 Using the Barlow Lens 5 Focusing 5 Pointing Your Telescope 6 Calculating the Magnification (power) 7 Calculating the Field of View 7 Calculating the Exit Pupil 7 Observing the Sky 8 Sky Conditions 8 Selecting an Observing Site 8 Choosing the Best Time to Observe 8 Chooling the Telescope 8 Using Your Eyes 8 Suggested Reading 9 Before you begin Caution! Read the entire instructions carefully before Never use your telescope to look directly at the beginning. Your telesope should be assembled sun. Permanent eye damage will result. Use during daylight hours. Choose a large, open a proper solar filter for viewing the sun. When area to work to allow room for all parts to be observing the sun, place a dust cap over your unpackaged. finderscope to protect it from exposure. Never use an eyepiece-type solar filter and never use your telescope to project sunlight onto another surface, the internal heat build-up will damage the telescope optical elements. TRIPOD SET UP Fig.1 ASSEMBLING TRIPOD LEGS (Fig.1) 1) Gently push middle section of each tripod leg at the top so that the pointed foot protrudes below the tripod clamp.
    [Show full text]