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OBSERVING THE SKY

 

Sky  conditions  are  usually  defined  by  two  atmospheric  characteristics,  seeing,  or  the  steadiness  of  the  air,  and 

transparency,  light  scattering  due  to  the  amount  of  water  vapour  and  particulate  material  in  the  air. When  you 

observe the Moon and the planets, and they appear as though water is running over them, you probably have bad 

"seeing" because you are observing through turbulent air. In conditions of good "seeing", the stars appear steady, 

without twinkling, when you look at them with unassisted eyes (without a telescope). Ideal "transparency" is when 

the sky is inky black and the air is unpolluted.

Travel to the best site that is reasonably accessible. It should be away from city lights, and upwind from any source 

of  air  pollution.  Always  choose  as  high  an  elevation  as  possible;  this  will  get  you  above  some  of  the  lights  and 

pollution and will ensure that you aren't in any ground fog. Sometimes low fog banks help to block light pollution 

if you get above them. Try to have a dark, unobstructed view of the horizon, especially the southern horizon if you 

are in the Northern Hemisphere and vice versa. However, remember that the darkest sky is usually at the "Zenith", 

directly above your head. It is the shortest path through the atmosphere. Do not try to observe any object when 

the  light  path  passes  near  any  protrusion  on  the  ground.  Even  extremely  light  winds  can  cause  major  air 

turbulence as they flow over the top of a building or wall. If you try to observe on any structure, or even a sidewalk, 

movements you make may cause the telescope to vibrate. Pavement and concrete can also radiate stored  heat 

which will affect observing. 

Observing through a window is not recommended because the window glass will distort images considerably. And 

an open window can be even worse, because warmer indoor air will escape out the window, causing turbulence 

which also affects images. Astronomy is an outdoor activity.

The  best  conditions  will  have  still  air,  and  obviously,  a  clear  view  of  the  sky.  It  is  not  necessary  that  the  sky  be 

cloud-free. Often broken cloud conditions provide excellent seeing. Do not view immediately after sunset. After the 

sun goes down, the Earth is still cooling, causing air turbulence. As the night goes on, not only will seeing improve, 

but air pollution and ground lights will often diminish. Some of the best observing time is often in the early morning 

hours. Objects are best observed as they cross the meridian, which is an imaginary line that runs through the Zenith, 

due  North-South. This  is  the  point  at  which  objects  reach  their  highest  points  in  the  sky.  Observing  at  this  time 

reduces bad atmospheric effects. When observing near the horizon, you look through lots of atmosphere, complete 

with turbulence, dust particles and increased light pollution.

Telescopes require at least 10 to 30 minutes to cool down to outside air temperature. This may take longer if there 

is  a  big  difference  between  the  temperature  of  the  telescope  and  the  outside  air.  This  minimizes  heat  wave 

distortion inside telescope tube (tube currents). Allow a longer cooling time for larger optics. If you are using an 

equatorial mount, use this time for polar alignment.

Do not expose your eyes to anything except red light for 30 minutes prior to observing. This allows your pupils to 

expand to their maximum diameter and build up the levels of optical pigments, which are rapidly lost if exposed to 

bright light. It is important to observe with both eyes open. This avoids fatigue at the eyepiece. If you find this too 

distracting, cover the non-used eye with your hand or an eye patch. Use averted vision on faint objects: The center 

of your eye is the least sensitive to low light levels. When viewing a faint object, don't look directly at it. Instead, 

look slightly to the side, and the object will appear brighter.

S

ky conditions

S

electing an observing site

C

hoosing the best time to observe

C

ooling the telescope

A

dapting your eyes

Содержание Reflector AZ1

Страница 1: ...INSTRUCTION MANUAL REFRACTORS REFLECTORS WITH ALT AZIMUTH MOUNT 090103V2...

Страница 2: ...ripod Leg Height Adjustment Clamp AZ1 AZ2 MOUNTS a b c Accessory Tray Tripod Leg Height Adjustment Clamp A B C D E F G H I J K L Dust Cap Mask Remove before Viewing Dew Cap Sun Shade Objective Lens Te...

Страница 3: ...Finderscope Finderscope Bracket Alignment Screws Focus Tube Eyepiece Diagonal Focus Knob 1 2 3 4 Azimuth Flexible Control Cable Altitude Flexible Control Cable Azimuth Adjustment Knob Tube Rings a b...

Страница 4: ...5 9 5 5 6 6 9 9 10 10 10 10 11 11 12 12 12 13 13 13 13 13 14 15 7 7 8 8 13 14 TABLE OF CONTENTS Before you begin Caution This instruction manual is applicable to all the models listed on the cover Ta...

Страница 5: ...ngth when the equatorial mount is level ATTACHING THE ACCESSORY TRAY Fig 2 1 Place the accessory tray on top of the bracket and secure with the locking knob from underneath Fig 5 Fig 6 Fig 5 Fig 6 ATT...

Страница 6: ...p 2 Insert diagonal and re tighten thumbscrews to hold diagonal in place 3 Loosen the thumbscrews on the diagonal 4 Insert the desired eyepiece into diagonal and secure by re tightening thumbscrews AT...

Страница 7: ...be rings from telescope by releasing their thumb nuts and opening their hinges 2 Fasten the tube rings to the mount using the wench provided ATTACHING THE TELESCOPE MAIN TUBE TO TUBE RINGS Fig 4 1 Fin...

Страница 8: ...nder Small finderscope ATTACHING THE FINDERSCOPE BRACKET RED DOT FINDER Fig 6 1 For finderscope only Locate the finderscope bracket and carefully remove the rubber o ring from it Position the o ring i...

Страница 9: ...tool that uses a coated glass window to superimpose the image of a small red dot onto the night sky The Red Dot Finder is equipped with a variable brightness control azimuth adjustment control and alt...

Страница 10: ...e diagonal can become 3X when placed in front of the diagonal In addition to increasing magnification the benefits of using a Barlow lens include improved eye relief and reduced spherical aberration i...

Страница 11: ...T adapter ring for your camera optional onto the T threads on the other end of the camera adapter tube Fig l This makes the telescope into a lens which you then attach to your camera as you would any...

Страница 12: ...average person has a fully dilated pupil diameter of about 7mm This value varies a bit from person to person is less until your eyes become fully dark adapted and decreases as you get older To determi...

Страница 13: ...ich also affects images Astronomy is an outdoor activity The best conditions will have still air and obviously a clear view of the sky It is not necessary that the sky be cloud free Often broken cloud...

Страница 14: ...and works like this Pull off the lens cap which covers the front of the telescope and look down the optical tube At the bottom you will see the primary mirror held in place by three clips 120 apart a...

Страница 15: ...by stopping at the point where the reflected image of the secondary mirror is closest to the primary mirrors edge Fig s When you get to that point stop and keep your hand there while looking at the b...

Страница 16: ...OF THE TELESCOPE FOR VIEWING THE SUN WHEN OBSERVING THE SUN PLACE A DUST CAP OVER YOUR FINDERSCOPE OR REMOVE IT TO PROTECT YOU FROM ACCIDENTAL EXPOSURE NEVER USE AN EYEPIECE TYPE SOLAR FILTER AND NEVE...

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