The LPI is easier to get use to then
the Meade DSI and delivers a great color image. Fast and easy
makes the LPI a perfect candidate for planetary and lunar
imaging. The software is also very easy to use. It will
take someone a long time to run out of objects to image with the
LPI. I have got some pretty great images, even with fair seeing
conditions using the LPI. I have also used it with my 4.5"
Newington and was able to get good results. If you are just
getting into imaging purchasing a Meade’s LPI is a great place to
start. I believe every telescope accessory case should have
one of these in it.
Manufacture By = Meade
Cost = @ $ 149 US Dollars
Vendor/Supplier = www.telescopes.com ( below is the
description available at the time of my purchase 2/2005 which outlines
Meade's exciting new LPI (Lunar Planetary Imager) can be used on any
telescope that uses .965" or 1.25" eyepieces for making images. The VGA
resolution (640x480) color CMOS chip is capable of creating
high-quality lunar and planetary images, as well as daytime terrestrial
images. And because the exposure times can be extended to 15 seconds,
even bright deep-sky objects can be captured. The effective
magnification of the camera is similar to a 6mm eyepiece, and it is
often used with a barlow lens for making images of planets.
Autoguiding with the LPI requires an Autostar-equipped Meade telescope.
Cables are included with the Autostar Suite for linking the PC to the
"RS232" port on these telescopes so that the software can make
corrections to the telescope as the LPI tracks on a star. Autoguiding
with the LPI is as easy as making an image. An initial image is
downloaded, and one only has to draw a box with the computer's mouse
over the star to be tracked. When used in tandem with the LX200GPS with
Smart Drive activated, stars as faint as 10th magnitude may be used.
Making lunar and planetary images with the LPI is
fun and simple. A beginner will find that they only have to do the
following to make images that they will be proud of:
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Install the Autostar Suite software in your PC.
Connect the USB cable to the camera and the PC. Windows will
recognize the new device and a dialog box will appear asking if you
want to install the new drivers. With the Autostar Suite CD disk still
inserted in the computer, click "OK".
Open Autostar Suite, click the "Image" drop-down menu at the
top of the program and select "LPI Imaging". The camera's dim red
L.E.D. "on" light will glow indicating you are connected.
Click the drop down menu under "Object" and select the type
of object that you will image, use "Moon" for taking images of the Moon
Center up the planet or region of the Moon that you wish to
image with an eyepiece. Remove the eyepiece from the telescope's
focuser, and slide in the LPI camera.
The image will appear on the "Live" box on your computer at
this time. You can now focus the telescope to get the sharpest image.
Use the "Magic Eye" tool of the program to determine best focus.
Hold down the left mouse button and draw a box around a
region of interest, and let go. The LPI will "track" on that region
during the exposures.
When you are ready, just click the "Start" button and you
will start tracking and stacking images. You can take and stack as many
images as you like.
Click "Stop" to finish. The LPI software will automatically
name and save your final image. It is that easy!
As your familiarity of using the LPI software
improves, you can over-ride all of the automatic settings and take
control of nearly every aspect of the imaging process to further
improve your imaging skill. For example, the exposure settings can be
user-controlled from .001 to 15 seconds.
The LPI software automatically aligns multiple images and
combines them into one superior image. Since atmospheric seeing will
dictate the quality any single image taken, the LPI software's "Min
Quality" setting can be set to discard poor quality images and only
combine images at or above the setting chosen.
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Other features include taking dark frames with the LPI, or
saving every image taken instead of just the final stacked image. Below
are most of the primary features of the LPI software interface for
controlling the camera:
Live - Displays what the imager sees in the "Live"
tab in the display area.
Exposure - This is the exposure time in seconds (from
.001 to 16 seconds), the up and down spin buttons adjust the exposure
up and down by .5 f/stop.
Gain and Offset - Are like contrast and brightness on
a TV. These controls are sent directly to the camera.
Histogram - Displays a histogram of the image in the
Live tab. It uses a monochrome converted image which is an average of
the RGB of each pixel.
Stretch Controls - The sliders below the histogram
control the stretch of the image. The top one is black and the bottom
one is white. The numbers below the sliders are the stretch values. The
left one is black the right one is white.
LOG Checkbox - This makes the histogram response log.
ROI Checkbox - Makes a histogram in the region of
interest (ROI) of the red rectangle in the Live display area drawn by
Magic Eye Focus - This displays a graphical
representation of the focus. The two orange triangles grow together to
indicate better focus. The red lines indicate the maximum obtained.
Avg Checkbox - This will average the last 5 focus
values to smooth out the noise in the image.
Reset - This will reset the red max indicators of the
Magic Eye Focus tool.
Start - This will start co-adding images and
continuously display the current image in the Live tab and the co-added
image in a new tab with the filename as the tab. The Min Quality,
Evaluation Count, Object Name, and filter selection will be used for
this image. The start button will be relabeled "Stop". When Stop is
pressed the co-added image will be saved as the file type selected and
in the "Image Folder" under the Object Name. If there is already a file
with this name then a number will be suffixed to the name.
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Min Quality - This selects the minimum quality that
is acceptable to co-add an image.
Evaluation Count - This is the number of images
skipped when Start is pressed to determine a quality range.
Object Name - This is the filename that will be used
when the Stop button is pressed.
Kernel Filter - This will insert the selected kernel
filter in the image stream. When co-adding the image, the filter is
applied after the co-add but is only used for display. It is applied
again when the image is saved such that it is only applied once to the
Images Status - This displays the number of co added images.
Quality Status - This displays the quality of the
last camera image.
Centroid - When you draw a rectangle around a bright
object in the Live display area, two crossed lines represent the
centroid of the rectangle (ROI). The rectangle will move with the
centroid to keep it in the middle. This way it will track the bright
spot any where on the image. The centroid is used by the shift and
combine algorithm to determine how much to shift the image by.
*Recommended Minimum System For Installing
PC running Windows 98SE with 64 MB and 100 MB free disk space.