Meade LX200R Manual de instrucciones Pagina 17

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MODE FUNCTIONS
To view the separate modes within the LX200 system, press
the MODE key ( it is located between the ENTER and GO TO
keys at the top of the hand controller). You can customize the
operation of your LX200 to perform virtually any of your
observing requirements by entering and editing information in
the various modes of the system. All the critical information,
such as time, location, alignment type, and many other
functions, are kept in memory—even with the LX200 turned off.
You can set the following through the five modes of the LX200
computerized hand controller:
Type of alignment
Objects that you see
Location from which you observe
Tracking speeds of the drives
Clock and timing functions
Position information
Brightness of the backlit keypad
Once you have selected the desired mode, you can select the
individual file within the mode by pressing the PREV or NEXT
key (up or down arrow key), as shown in Fig. 7. This scrolls the
arrow up or down next to the file description. Although you will
be able to see only two menu selections at a time on the
keypad display, you will see more as you continue to press the
PREV and NEXT keys.
When you select the file, press the ENTER key to view the file
menu. To choose an individual menu, again use the PREV or
NEXT key to move the arrow up or down the file menu. To
explore a menu selection, again press the ENTER key. Some
modes offer options for a file menu selection; others are only for
entering data.
Whenever you wish to return to the main file heading in a
mode, press the MODE key; it will behave as an exit key.
Mode One:
TELESCOPE/ OBJECT LIBRARY
TELESCOPE/OBJECT LIBRARY is the mode to which the
LX200 defaults after the instrument completes its power-on
diagnostic self-test. The T E L E S C O P E / O B J E C T L I B R A R Y
mode is command central. It is where you select the way that
you want the LX200 to perform mechanically and where you
explore and select from its extensive library of stored objects.
To explore either the TELESCOPE menu file or the OBJECT
LIBRARY menu file, move the LCD arrow to the appropriate
selection by using the PREV or the NEXT key and press the
ENTER key.
1. TELESCOPE Menu File
Below are the various selections of the TELESCOPE menu file,
with illustrations of the individual menu files and file options.
a. SITE: The SITE menu option lets you enter up to four of your
favorite viewing locations in latitude and longitude. To
calculate celestial coordinates, the LX200 computer
compares the llatitude and ongitude that you entered to your
local time, GMToffset, and calendar date. Once entered, the
information is stored in the telescope’s internal memory; you
need not re-enter it. To enter new site information or to
change old information, see
QUICKSTART
, page 9.
You can choose any one of the four site options (or the
UNKNOWN site) at your convenience, without entering
latitude and longitude every time you use the LX200. Once
you have chosen the site, exit the SITE menu by pressing
the MODE key.
b. ALIGN: The Align menu selection of the TELESCOPE file
demonstrates the unique ability to transform the LX200 into
an altazimuth, celestial-tracking telescope, a polar-
equatorial celestial-tracking telescope, or a land spotting
scope with electric altazimuth movements within three
options. These options are ALTAZ, POLAR, and LAND.
When you enter correct local time, latitude, and longitude
(see
QUICKSTART
, page 9), you are ready to choose a type
of alignment. Do this by pressing the PREV or NEXT key to
move the arrow beside the desired option of ALTAZ, POLAR,
or LAND, and then pressing the ENTER key. The display
gives you instructions to walk you through the chosen
alignment type.
1. ALTAZ: ALTAZ (altazimuth) requires that you mount the
LX200 directly to the top of the field tripod (with the
power panel facing North) and adjust the leg extensions
of the tripod until the instrument is level. Then align on
one or two of the bright stars in the look-up table of 33
alignment stars.
This allows your LX200 to track in altitude and azimuth
simultaneously for visual observations, very brief (under
five minutes) exposure astrophotography, or CCD
imaging (longer exposures require the field de-rotator).
ALTAZ lets you access the object library as well as all
other telescope functions, including the Smart Drive. Full
instructions for using ALTAZ are in the
QUICKSTART
guide (page 9).
2. POLAR: POLAR allows you to use the 16” LX200
(mounted on a permanent pier set to your latitude) as an
equatorial telescope. With the LX200 powered up, the
POLAR file option selected, and the field tripod leveled,
the telescope should be adjusted so that the Dec. setting
circle (3, Fig. 1) is set to 90° (see Fig. 13), and the
telescope is rotated to the 00 hour angle (H.A.) position
in R.A. In this position, the viewfinder (Fig. 1) is upside
down, and the following all line up:
R.A. pointer (4, Fig. 5)
00 line of the R.A. setting circle (3, Fig. 5)
H.A. pointer (5, Fig. 5)
(If you do not start at the 00 H.A. position, the telescope
will point to the ground instead of the sky when the
keypad display chooses its second star.)
Press the ENTER key; the LX200 slews to the precise
offset of the Polar star in Dec. and R.A.
Aim the telescope at the Pole Star (Polaris, see
APPENDIX B
if the Pole Star is not visible). Center the
Pole Star in the eyepiece field using only the altitude and
azimuth adjustments on the pier. Press the ENTER key
again; the LX200 chooses, and slews to, a very bright
star that is overhead and can usually be seen in the field
of view of the viewfinder. Center the bright star using
only the R.A. and Dec. adjustments of the telescope
(either manually by loosening the locks only or
electrically); press ENTER. You can now access every
function of the LX200.
3. Refined Polar Alignment:Astrophotographers routinely
require polar alignments of the highest accuracy for the
finest guiding characteristics. Refine your initial polar
alignment by using the LX
2 0 0’s electronics with a slightly
d i fferent method in the POLAR menu option. Perform the
following steps at two or three 15-minute intervals. A t
each interval the telescope slews to the area where the
Pole Star should be centered in the optics. The Pole Star
may be somewhat off-center in the eyepiece.
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