background image

26

27

Each individual deep sky image is faint and has a noticeable amount of noise. 
Combining the individual deep sky images eliminates the noise and enhances the 
detail in the deep sky object by improving the signal to noise ratio. The more imag-
es you combine, the better the resulting image will look. (Figures 22.1 and 22.2).
Read section 5 “Image Processing” to utilize MaxIm DL’s 

Stack function.

5.  Image Processing

After you have captured and combined individual images (with or without dark 
frame subtraction) into a single resultant image, you may want to perform some 
additional image processing to bring out subtle details or to make the image 
appear more pleasing overall. MaxIm DL contains several image processing func-
tions which will further enhance your image once your individual images have 
been calibrated and combined. The image processing functions are found in the 
Process menu.

5.1. Image Calibration

The darks and flats you previously saved will be subtracted from your “light” 
images.
1.  Select 

Setup Calibrate from the Process menu.

2.  Click 

Clear All Groups if any filenames 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 flats. The selected dark frames will 
now appear in the pop-up window.

5.  Click 

OK.

6.  With your astro-image open in MaxIm DL, select 

Calibrate from the Process 

menu (or click the 

Calibrate icon in MaxIm DL) You should see a significant 

amount of noise disappear. This process can be automated for all of your 
light images, see “Stacking – Combining Images”.

5.2. Convert raw to Color (For Parsec 8300C and 10100)

Once you have calibrated your images, you need to convert them to color:
1.  Open the raw images you wish to convert to color. If you need to convert 

more than 5 images or so, please refer to “Batch Processing” as this method 
allows you to combine an unlimited number of images without consuming 
more memory from your computer.

2.  Select 

Convert Color in the Process menu.

Figure 22.1. 

Before your images are 

combined, an individual deep space image 
will have more noise and less detail.

Figure 22.2. 

Combining multiple deep 

space images greatly increases the detail 
in the resulting combined image

Figure 23. 

The 

Set Calibration window lets you automatically select all of your 

calibration images.

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...

Отзывы: