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Adv anced ls fea tures, Index, Ls tips – Meade Instruments 6" LS-6 ACF User Manual

Page 32

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INDEX

Terrestrial Observing

The LS is an excellent high-resolution, terrestrial (land)

telescopes. Viewing terrestrial objects requires looking

along the Earth’s surface through heat waves. These

heat waves often cause degradation of image quality.

Lower power eyepieces, like the Super Plössl 26mm

eyepiece, magnify these heat waves less than higher

power eyepieces. Therefore, lower power eyepieces

provide a steadier, higher quality image. If the image is

fuzzy or ill-defi ned, reduce to a lower power eyepiece,

where the heat waves do not have such an effect on

image quality. Observing in early morning hours, before

the ground has built up internal heat, produces better

viewing conditions than during late afternoon hours.

If you wish to observe a distant land object, such as a

mountain top or a bird, you want to use your telescope

in its Terrestrial Observing mode. To start up the

telescope in Terrestrial mode:

1. Turn on the telescope.

2. When you hear the introductory audio, press the

“MODE” key. The telescope will move to the

home position, and when it has stopped “Select

Item” will show on the Handbox screen. Use

the SCROLL keys to move through the menu

to “Align”. Press the “ENTER” key again to set-

up the “Align” menu. Use the SCROLL keys to

move to “Terrestrial” and hit “ENTER”.

3. Move your telescope using the direction arrows

on the handbox while looking through the Red-

Dot Finder to put your target in the eyepiece.

4. Focus on the target with the focus knob (pg. 12,

Fig. 2, 9).

ADV

ANCED LS FEA

TURES

Too Much Power?

Can you ever have too much power? If the

type of power you’re referring to is eyepiece

magnifi

cation, yes, you can! The most

common mistake of the beginning observer

is to “overpower” a telescope by using high

magnifi cations which the telescope’s aperture

and atmospheric conditions cannot reasonably

support. Keep in mind that a smaller, but bright

and well-resolved image is far superior to one

that is larger, but dim and poorly resolved (see

Figs. 7a and 7b to the left). Powers above 400X

should be employed only under the steadiest

atmospheric conditions.

Most observers should have three or four

additional eyepieces to achieve the full range of

reasonable magnifi cations possible with the LS

telescopes. See OPTIONAL ACCESSORIES,

page 16.

LS TIPS

Figs. 7a & 7b: Jupiter; examples of the right amount of
magnifi cation and too much magnifi cation.

32

Capitol Reef, Utah

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