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detail finer than the pixel size of 
the frames being combined. The 
technique is described at http://
xxx.lanl.gov/abs/astro-ph/9808087.

5.4. Filter

Filtering an image is an operation that 
emphasizes certain characteristics of 
an image while suppressing others. 
MaxIm DL supports several kinds of 
Filters, such as: 

Unsharp Mask, Kernal 

Filters, and Digital Development, 
available from the 

Filter menu.

Please read MaxIm DL’s 

Help Topics 

for the most detailed information about 
the various image processing filters 
available. The following are just some 
of the many processing filters available 
in MaxIm DL.
Unsharp Mask is a method of sharpening or high-pass filtering an image. It 
amounts to subtracting a low-pass filtered version of an image from itself. The 
low-pass filtered version is called the mask.
KernalHigh-Pass Filter can be set to More or Less for different effect. The High-
Pass Filter can be useful for accentuating fine details in an image.
Kernal, Gaussian Blur is a method of blurring an image. It can be used to sup-
press noise in an image at the expense of sharpness. The 

Radius setting controls 

the amount of blurring applied to the image. Increasing the radius increases the 
amount of blur applied.
For best results, turn on the 

Auto Full Screen preview button, and adjust the set-

tings. This allows you to rapidly adjust the settings until you are satisfied with the 
results. Then, click 

OK to actually apply the filter settings to the image.

It is best to use a light touch with this command, to avoid over-processing the 
image. Over-processing can create artifacts; i.e. features in the image that are not 
real. It also amplifies the noise in the image.

5.5. Color Balance

The sensitivity of most CCD cameras as a function of wavelength (color) is differ-
ent from the response of the human eye. The filters used for creating color com-
posites also have their own characteristics, as do the telescope optics. Although 
“perfect” color rendition is an elusive if not impossible goal (all individuals see col-
ors slightly differently), it is straightforward to get “good” color balance with simple 
weightings. This is where the 

Color Balance command (in the Process menu, 

Figure 31) comes in handy to touch up the resultant colors in your images. Use 

the 

Preview Image to see how altering these parameters will affect your image 

(or click the 

Full Screen button to see the changes applied to your full image).

Note for the Parsec 8300M: Before any color balance adjustment can be made, 
you must first Combine Color to each individual LRGB or RGB images.
Color images from CCD cameras typically require 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 in its color plane. Any pixel values that become negative are forced to 
zero. The 

Auto button automatically determines the settings necessary to equal-

ize the image background in all three color planes. The 

Reset button resets the 

background level subtraction to zero on all planes.
Scaling adjustment (entered as a percentage) allows you to compensate for 
transmittance differences between the filters used to acquire the three color 
planes. Values of 100% result in no change. The scaling percentages can be typed 
in or adjusted using the “spin” controls (small up and down click arrows to the right 
of the scaling numbers). The 

Preview Image is particularly helpful in monitoring 

the results when using the spin controls. The 

Reset Scaling button resets to 100% 

on all three planes.
The 

Click On White Area to Set Scaling check box enables the operation of the 

mouse to set the scaling. Set the 

Background Level first (you can use Auto), then 

click on a white object (e.g. a neutral-colored star) in the image (not the 

Preview 

Image) with the mouse. The Scaling settings will automatically be adjusted to 
make the selected point appear white. If an area of the image is known to be white 
(or gray), this is an easier way to determine the scaling factors, and can be used 
to instantly color balance the image.

note on File Format

When saving individual images that were not taking during a sequence (using 
Save or Save As in the File menu), you have a choice of file formats. The default 
produces .fit files, but .tif, .jpg, .png, and .bmp file formats can also be selected. 
Having a choice of output file formats is useful, especially if images will be 
exported to other software programs for additional image processing (like Adobe 
Photoshop, for instance).
If you save to a file format other than .fit, you will need to check the 

Auto Stretch 

box, or otherwise 

Stretch the image to change the Output Range (in the Stretch 

command window) to match the 

Size Format (in the Save As window). Otherwise, 

the 

Output Range will likely exceed the Size Format, and the saved image will 

be ruined (will turn all white).
For example, say the 

Output Range is set to create image brightness values in 

16-bit format, while the 

Size Format of a specific file format (.jpg, for example) 

may only support 8-bits. Since the 16-bit format sees 65535 brightness levels, 
and the 8-bit format can only support 255 levels, all of the levels above 255 in the 
16-bit image (i.e. the vast majority of the 16-bit brightness levels) will be saved at 
the maximum 8-bit value of 255. So the saved .jpg will have very little brightness 

Figure 31. 

The 

Color Balance 

Window.

Содержание PARSEC 10100C

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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...

Страница 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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