Presentation is loading. Please wait.

Presentation is loading. Please wait.

Announcements After lecture, adjourn to the observatory to start set-up for Dark Sky Observing night Forecast for Thursday doesn’t look good (60% chance.

Similar presentations


Presentation on theme: "Announcements After lecture, adjourn to the observatory to start set-up for Dark Sky Observing night Forecast for Thursday doesn’t look good (60% chance."— Presentation transcript:

1 Announcements After lecture, adjourn to the observatory to start set-up for Dark Sky Observing night Forecast for Thursday doesn’t look good (60% chance of rain during day falling to 20% chance in the evening) SO meet here to start doing basic image processing. I have canned images we can use.

2 Digital Imaging

3 Basics: The Photoelectric Effect

4 Photoelectric Effect: The Theory

5 The MOS works on the photoelectric effect By “catching” the liberated electrons in the MOS device you lose the frequency information. Thus, the MOS simply measure the intensity (# of photons), not the color.

6 CCD Versus CMOS The difference is in the on- pixel amplifier

7 Each pixel is an MOS photodiode The liberated electrons are held in the potential well until they are read out

8 CMOS includes amplifiers on each pixel while CCD’s do not As a result, not all the area on a CMOS pixel is available to collect light. The amplifiers also tend to be nonlinear so they aren’t useful for photometry

9 A CCD array has millions of individual devices The smaller the pixel, the higher the resolution. But, the smaller the pixel, the fewer the number of electrons that can be stored before it fills up

10 Downloading the array is like running a series of conveyor belts

11 Downloading the array

12 If a pixel gets overfilled (saturated), it “blooms” into pixels down the line

13 Anti-blooming Architecture helps eliminate booming

14 The download a numerical array of how many photons hit each pixel Number of electrons in each pixel is proportional to the number of photons that hit that pixel. The result is a spreadsheet that is easy to mathematically manipulate.

15 The numbers in the array can be translated to a grayscale

16 Once pixel is assigned a shade of gray, a black & white image is created from the spreadsheet

17 Color imaging requires filters For pretty pictures we use red, green, blue and luminance. For photometry we use ubvri (Johnson set) or ugriz (SDSS set). Other systems extend into the UV or IR ends of the spectrum

18 It is possible to put filters directly on the CCD chip All color digital cameras use microfilters. Notice there are more greens than reds or blues. Different chips have different wavelength sensitivity.

19 A color chip has a lower resolution since each “pixel” is actually four Silicon chips are most sensitive in infrared and red and least sensitive in blue. An infrared filter will cover the entire chip. The “white balance” adjusts the amplification of each of the colors.

20 A color image download has to account for the colors


Download ppt "Announcements After lecture, adjourn to the observatory to start set-up for Dark Sky Observing night Forecast for Thursday doesn’t look good (60% chance."

Similar presentations


Ads by Google