Orion PARSEC 10100C Manual Download Page 8

14

15

arrow button next to the preset name to 
manage your presets, including Update 
Current Preset, and Save As New 
Preset. See MaxIm DL’s 

Help Topics 

for more detailed information.

readout Mode

In the 

Expose Tab

,

 select 

Normal for 

the best image quality, and 

Fast for a 

quicker image download.

Frame type

Choose, 

Light  (Raw or Color for the 

8300C), 

Bias

,

 Dark, and Flat

.

 Please 

read section 5, “Astronomical Imaging” 
to determine when and why to take a 
dark or flat.

Fan Speed

Select 

Camera Settings in the Expose tab (Figure 14.1) to access the fan speed, 

HighMedium, or Low (Figure 14.2). High is recommended for the best cooling 
performance.
There are a large slew of settings in the 

Camera Control Window’s Expose tab. 

Please read MaxIm DL’s 

Help Topics which covers all the settings in greater detail.

3.2. the Screen Stretch Window

The function of the 

Screen Stretch Window (Figure 13) is to properly map the 

image brightness levels captured by the camera into corresponding image bright-
ness levels on the computer screen. A typical camera image has each pixel (light 
detecting site, over eight million pixels form a single Parsec image) represented 
as a number (from 1 to 65535) depending on brightness. This has to be mapped 
into the video monitor’s brightness range (from 1 to 255). It is important to set the 
screen stretch appropriately, or a great image may look terrible!
When an image is displayed, you will notice a graph in the 

Screen Stretch 

Window. This is called the “histogram” of the currently displayed image. A histo-
gram is a simple bar graph that shows the range of brightness in an image. Each 
bar in the graph represents a level of brightness; the bar to the far left in the histo-
gram represents the dimmest pixels, and the bar to the far right is for the brightest 
pixels. The height of the bar is the total number of pixels at that brightness level 
in the image. Every image has a different histogram depending on how much of 
the image is bright or dark. Directly viewing the histogram of your image in the 
Screen Stretch Window provides an easy interface for making decisions on how 
the screen stretch should be set.
In Maxim DL, the two parameters entered in the 

Screen Stretch Window are 

Minimum and Maximum. A pixel that is at the Minimum value is set to zero (black), 
and a pixel at the 

Maximum value is set to 255 (white). An easy way to adjust the 

Maximum and Minimum values is to 
move the slider arrows located directly 
under the histogram of the image in the 
Screen Stretch Window. The red slider 
arrow corresponds to the 

Minimum 

value and the green arrow corresponds 
to the 

Maximum value. Simply left-click 

and then drag each arrow to adjust it 
to the desired level. The best results 
are obtained by adjusting the arrows 
(numbers) until the most pleasing dis-
play appears.
There are also seven automatic settings in the 

Screen Stretch Window. Typically, 

Medium will give good results for deep sky objects, so the default screen stretch 
setting is 

Medium.

Instead of using the 

Screen Stretch Window, it is faster to use the Quick Stretch 

facility. This allows you to modify the image appearance instantly with small up/
down and left/right movements of the mouse. To do this, hold down the Shift key, 
then left-click and drag the mouse on the image. You’ll find this feature to be a 
great convenience when fine adjusting the screen stretch to get an image to look 
its best.
The trick with stretching is determining exactly how to stretch the image for best 
effect. Often there are several different possibilities for the same image. Trial-and-
error will be the best way to judge what the best screen stretch setting is. Try 

Figure 14.1. 

The 

Camera Settings is found in the Expose tab.

Figure 14.2. 

Adjust the 

Fan Speed in 

the 

Parsec Settings.

Figure 13. 

The 

Screen Stretch 

Window is a histogram that allows you to 
adjust the apparent brightness levels of an 
image on your screen.

Number of pix

els at 

br

ightness le

vel

Range of brightness levels

Summary of Contents for PARSEC 10100C

Page 1: ...ec 10100C Color 52078 instruction Manual Providing Exceptional Consumer Optical Products Since 1975 OrionTelescopes com Customer Support 800 676 1343 E mail support telescope com Corporate Offices 831...

Page 2: ...eep Sky Objects 20 5 Image Processing 26 5 1 Image Calibration 26 5 2 Convert Raw to Color For Parsec 8300C and 10100 27 5 3 Stacking Combining Images 28 5 4 Filter 32 5 5 Color Balance 32 6 Multiple...

Page 3: ...ludes 1x1 full resolution 2x2 3x3 and 4x4 This CCD chip offers the unique ability to image in color at 1x1 mode as well as 2x2 mode This is advantageous when imaging with different focal lengths In ge...

Page 4: ...edge darkening may occur Caution Be sure to always firmly tighten the thumbscrew s that secure the Parsec in the telescope focuser or it could fall out and onto the ground If your telescope has T thr...

Page 5: ...plorer 4 or higher required to display on line help High speed USB 2 0 port Power The Parsec requires 12 volts DC 12VDC with approximately 2 amperes of cur rent Power to the entire camera including th...

Page 6: ...he following section of the manual will walk you through the basic features mostly found in the Camera Control Window The Parsec includes a free 60 day trial of MaxIm DL 5 Pro Start by opening MaxIm D...

Page 7: ...it a few seconds for the image to appear It may be over exposed or grossly out of focus Adjust the telescope s focus and adjust the exposure time as needed to get a focused image 4 Look at the Pixel v...

Page 8: ...image has a different histogram depending on how much of the image is bright or dark Directly viewing the histogram of your image in the Screen Stretch Window provides an easy interface for making de...

Page 9: ...se The camera will only download the area you previously selected which makes each image download significantly faster than the whole frame Note If the Parsec is grossly out of focus no object will ap...

Page 10: ...quality of your focus Caution Once you have achieved focus be sure to click the Reset but ton in the Subframe box otherwise the camera will crop all your images into a small square 4 2 Setting the Coo...

Page 11: ...eep sky object into the field of view of your eyepiece If you are using a mount with an accurate computerized go to system you can keep the camera installed in your telescope s focuser without using t...

Page 12: ...iminate most of the camera noise you can take several dark frames average them then subtract them from your astro images also called light images Note Make sure the cooler set point and CCD temperatur...

Page 13: ...flat frames it s a good idea to assign a preset such as F to better organize your different images 4 Set the Seconds to 0 1 for now and click OK then Expose You want the Max Pixel to read somewhere ar...

Page 14: ...s appear in the window 3 Select the Source Folder where you saved your dark frames Figure 23 4 Click Auto Generate and MaxIm DL will automatically find all of your calibration images such as darks and...

Page 15: ...ged into groups according to their FITS header You can open the groups to view the files by clicking on the sign If you would like to view an individual file right click it and select Display Image Al...

Page 16: ...e Add Folder option calibration files are automatically ignored the other methods for adding files will include them Usually you don t want to stack the calibration files automatically since the Set C...

Page 17: ...re a background level adjustment This is accomplished by bringing the background level or bias in each color plane down to zero Each of the Background Level values is subtracted from every image pixel...

Page 18: ...ting of 10 means that the Parsec attempts to track out 100 of the motion whereas a setting of 1 means that the Parsec only tracks out 10 of the motion Usually a setting of around 8 or 9 provides the b...

Page 19: ...mpensation in the mount is turned off On most telescopes the Right Ascension drive likes to have some load pushing against sidereal tracking If the mount is balanced such that it is pulling the mount...

Page 20: ...drift and correct by moving the mount in the appropriate direction To perform the drift method of polar alignment 1 Do a rough polar alignment by pointing the R A axis of the mount at Polaris the Nor...

Page 21: ...ng images of wide field deep sky objects such as the Andromeda Galaxy or the Pleadies star cluster Focal reducers will usually thread onto the nosepiece of the Parsec Barlow lenses increase the focal...

Page 22: ...ith anti reflection coatings Backfocus Distance from T threads 29 24mm 1 15 Weight 900g 32 oz Autoguider capability Yes Mounting 2 nosepiece or T thread Parsec 10100C CCD Sensor Kodak KAI 10100 CXC CC...

Page 23: ...wing two conditions 1 this device may not cause harmful interference and 2 this device must accept any interference received including interference that may cause undesired operation Changes of modifi...

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