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Subject: PE Series LNT Summary
Sent: Tuesday, May 17, 2005 14:38:48
From: mhogansr@comcast.net (mhogansr@comcast.net)
The following is rather lengthy, as it covers the results of my
non-observing activities over the last five months. Many of the
items have been addressed at one time or another on your site,
but I've tried to sort of consolidate them. Some are obvious,
others are not. Do with it as you wish and I hope it is useful.
Nearly five months after ordering and paying for it, I finally
have an ETX125PE that works almost as advertised. It took an
update of the AutoStar software, one replacement AutoStar, and
two LNT/SmartFinder replacements.
During all the "downtime", I had some questions and, thanks to
your informative site and some research, found some answers.
Here's my Q&A.
What is the LNT?
It is an electronic module that provides several related
functions intended to reduce required user input during AutoStar
initialization and `scope alignment:
1) A crystal controlled, battery powered clock to provide
time/date, similar to an internal PC clock;
2) A sensor to automatically detect Level and North;
3) An LED and optical fiber to project a dot onto the
SmartFinder lens.
It is securely attached to a bracket that is mounted on the OTA,
and has an adjustable cover holding the SmartFinder lens.
How does the LNT work?
The module has a serial data interface with the AutoStar via the
`scope wiring and the HBX port, and is powered by the `scope
power source. The clock has its own battery and maintains time
when the power is turned off. The sensor is an array of
magnetic sensors that can determine its orientation with respect
to the local magnetic field.
When power is applied, the AutoStar goes through its own
initialization, including checking whether or not an LNT is
present. If so, the AutoStar will:
1) Initialize the magnetic sensor array;
2) Download and store the current time/date from the clock. Note
that once the initial time is loaded into the AutoStar, it
maintains its own clock and no longer uses the LNT clock;
3) Drive the OTA until data from the sensors indicate it is
aligned with the local magnetic field in both the vertical and
horizontal planes, relative to the center of rotation of the
array. In the absence of other influences, this would be
Level and Magnetic North relative to the Earth's magnetic
field;
4) Correct the data for True Level and True North using
previously stored values and save the results for the current
session;
5) Drive the OTA in the AZ axis while monitoring any variation of
Level and calculate a Tilt coefficient, then save the result
for the current session;
6) Determine the position of the AZ full CCW stop, set by the
user, relative to North; this is used to determine which way
to slew without hitting a stop during GOTO's;
7) Turn on the SmartFinder dot and proceed with a standard
alignment with star positions calculated using parameters from
the preceding steps and stored site information;
8) When alignment is completed successfully, turn off the Dot.
Any corrections obtained will be temporarily saved in the
AutoStar for the current session.
From this point on the LNT serves no purpose except to turn the
Dot on and off via the AutoStar "0" (Light) key. Note that any
corrections determined during the process are only saved for the
current session. When power is turned off, they are lost unless
a Park Scope is used. The only semi-permanent corrections are
those obtained during Calibrate Sensors, which are saved until
the AutoStar is Reset, or the Calibration is performed again.
What are the advantages of the LNT?
1) The user only has to set the internal clock once, the first
time the system is used. After that, the AutoStar will have
the correct time whenever power is applied. It should be
remembered that the internal clock will have some drift,
similar to a PC clock, and should be checked/reset
periodically for really accurate time;
2) Physical setup of the telescope is much less critical. Since
the LNT will determine Tilt, the mounting surface or tripod
head does not have to be perfectly level. Also, orientation
of the base and OTA can be arbitrary since the LNT determines
the "home" position for beginning a star alignment. The AT
series required the user to orient the base with the power
panel pointing West and the OTA level as the "home" position;
3) The SmartFinder provides a much larger FOV so star alignment
is simplified.
Does the LNT have any disadvantages?
Although the concept of the LNT is good, its implementation
leaves a lot to be desired, especially the SmartFinder.
1) In the original version of the LNT, the optical fiber that
projects the Dot onto the lens was not always oriented
properly so the Dot wasn't visible. In a subsequent
modification, the fiber is anchored with an adhesive but its
position is still not very precise and there may not be
enough adjustment to center the Dot during Finder alignment;
2) Also in the early version, the Lens could be easily inserted
the wrong way, so again no Dot was visible. This also was
corrected in the later version but the position of the fiber
can still cause problems;
3) The SmartFinder Lens mounting is very susceptible to external
forces. A small bump can disturb the alignment and I
understand it will not fit into a standard Meade hard case
without modification of the insulating foam;
4) The SmartFinder requires an on-axis eye position as opposed
to the right-angle view finder on the AT series, and there is
some parallax shift;
5) The LNT mounting bracket interferes with proper installation
of the LPI camera so it can only be inserted +/- 90 deg. or a
full 180 deg. from the normal position. The resulting image
on a PC screen can be confusing;
6) A shortcoming, rather than a disadvantage, is that the
Instruction Manual for the PE gives no comprehensive
instruction as to the prerequisites for using the LNT for the
first time, and there are several:
a) The local time/date/daylight saving must be set as
accurately as possible;
b) The observing site lat/lon/time zone must be set;
c) A Motor Calibration and Drive training should be
performed;
d) The Dec circle must be set to "0" when the OTA is level,
if not already there. This should be done using a bubble
level or similar method;
e) Calibrate Sensors must be performed. The previous steps
should be completed first, since they all affect the
accuracy of values obtained during the procedure. These
values will become the correction coefficients used after
the LNT determines local magnetic Level/North.
Any corrections and/or additional info on this subject will be
welcome and appreciated.
Regards to all,
Mike Hogan
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