10new_english, Perating the az1/az2 mount, Perating the az3 mount – Sky-Watcher AZ3 MOUNT User Manual

Page 10: Sing the barlow lens, Ocusing

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10

O

perating the AZ3 mount

Azimuth fine adjustment

Altitude fine adjustment

Azimuth locking knob

Fig.g

U

sing the Barlow lens

F

ocusing

Fig.k

This mount has controls for movement in altitude (up-down) and

azimuth (left-right). Coarse azimuth movement is controlled by a

locking knob located near the tripod head for left-right rotation.

Loosen the knob to make large direction changes then lock it for

fine adjustments. Coarse Altitude movement is controlled by a

friction bolt. Use the micro-adjustment control cables to make small

altitude and azimuth movements such as centreing objects in view.

The micro-adjustment controls have limited travel so it is best to

centre them on their threads before making a coarse adjustment

(Fig.i).

A Barlow is a negative lens which increases the magnifying power

of an eyepiece, while reducing the field of view. It expands the

cone of the focussed light before it reaches the focal point, so that

the telescope's focal length appears longer to the eyepiece.

The Barlow is inserted between the focuser and the eyepiece in a

reflector, and usually between the diagonal and the eyepiece in a

refractor or a catadioptric (Fig.j). With some telescopes, it can also

be inserted between the focuser and the diagonal, and in this

position it gives even greater magnification. For example, a 2X

Barlow when inserted after the 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 in the eyepiece. For this reason, a Barlow plus a lens

often outperform a single lens producing the same

magnification. However, it is greatest value may be that a Barlow

can potentially double the number of eyepiece in your collection.

Slowly turn the focus knobs (Fig.k), one way or the other, until the

image in the eyepiece is sharp. The image usually has to be finely

refocused over time, due to small variations caused by

temperature changes, flexures, etc. This often happens with short

focal ratio telescopes, particularly when they haven't yet reached

outside temperature. Refocusing is almost always necessary when

you change an eyepiece or add or remove a Barlow lens.

Fig.j

Barlow

Diagonal

Eyepiece

(Refracting Telescopes)

(Reflecting Telescopes)

Barlow

Eyepiece

Altitude adjustment

Azimuth adjustment

Altitude fine

adjustment

O

perating the AZ1/AZ2 mount

Azimuth adjustment

Altitude fine

adjustment

Altitude adjustment

Fig.h

Fig.i

This telescope has an altitude(up-down)-azimuth(left-right) mount

to control telescope movements. Loosen the azimuth lock knob to

make left-right direction movements then tighten to lock. Loosen

the altitude lock knob to make course up-down changes. Altitude

fine adjustments can be made by rotating the knurled wheel on

the altitude fine adjustment rod after tightening the altitude lock

knob. (AZ1: Fig.g, AZ2: Fig.h)

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