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I've read some information about sensor sizes here

http://en.wikipedia.org/wiki/Image_sensor_format

according to this, the 35mm ff-CMOS is the sensor with the largest dimensions used in digital cameras. It has a lot of advantages to smaller sensors, caused by its size.

Why are there not even bigger sensors available to force these advantages? 1,5 FF e.g.?

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    \$\begingroup\$ That page is outdated. Hasselblad launched a medium format CMOS sensor in March. \$\endgroup\$
    – Philip Kendall
    Commented Aug 27, 2014 at 10:01
  • \$\begingroup\$ The article specifically mentions different medium format chips that are larger than so-called "full frame" (a misnomer). en.wikipedia.org/wiki/… \$\endgroup\$
    – his
    Commented Aug 27, 2014 at 10:48
  • \$\begingroup\$ @his Which CMOS sensors which are larger than full frame does it mention? \$\endgroup\$
    – Philip Kendall
    Commented Aug 27, 2014 at 11:03
  • \$\begingroup\$ @fubo Are you specifically interested in CMOS sensors (as opposed to CCD sensors) or do you really mean "what limits the size of digital imaging sensors?" \$\endgroup\$
    – Philip Kendall
    Commented Aug 27, 2014 at 11:17
  • \$\begingroup\$ @PhilipKendall updated \$\endgroup\$
    – fubo
    Commented Aug 27, 2014 at 11:23

4 Answers 4

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You can make some very large CCDs. An older press release talks of a CCD that was made for the US Naval Observatory that is 4" × 4" and 10,560 pixels × 10,560 pixels. That's 111 megapixels on one sensor. That's kind of not small.

A 111 megapixel sensor

(From above press release)

The first restriction that the sensor has is that it must be a single wafer of silicon, and that's a fixed price. You can create CCDs that are designed with a three-edge CCD (the remaining edge is where you can read the data out) such as:

mosaic CCD

(From http://loel.ucolick.org/manual/deimos_ccd/science/overview/EL3160.html)

These are often used in telescopes to get a larger imaging area with only a smaller increase in price. Note that there is the issue that each CCD needs to be calibrated separately from the others (no two image sensors have exactly the same response) - this is a significant concern for scientific uses (calibration information for one such CCD array).

The mosaic CCD can be scaled up quite significantly. PanSTARRS has a 1.4 gigapixel sensor array that is made up of a massive array of 600×600 pixel CCDs:

8x8 CCD array from PanSTARRS

Above is an 8×8 array of CCDs - each one quite small. This then is part of a larger array of 8×8 of these segments giving an overall 64×64 array of sensors. This was done because of cost savings, speed (it's faster to read out four thousand 600×600 pixel CCDs simultaneously than it is to read out one larger CCD), isolation of saturated pixels, and an easier replacement in the case of defects.

The LSST uses more conventional three edge CCDs to reach its goal of 3.2 gigapixels. Each segment there is an 8×2 array of 500×200 pixel sensors. All the same factors mentioned for PanSTARRs is also in place here. It is expected to take 2 seconds to read out 3.2 billion pixels (which is actually quite fast). Going to fewer, larger CCDs would mean it's slower - not faster.

LSST sensors

So, while it's possible to use multiple sensors in aggregate, they are still composed of rather small individual sensors rather than a large single sensor (as was done with the USNO's 4×4" sensor). In some cases, the CCDs are much smaller than even those used in point and shoot cameras.

Look back to that first image of the 4×4" sensor and then consider the size of regular sensors on there:

sensors on a wafer

This has some additional information on there to consider. There's the maximum yield of how many you can put on a wafer (you just can't fit more on) and the waste. In order to make that 4"×4" sensor they needed an extremely high quality wafer of silicon. On a regular full frame the flaws in the crystal are there no matter how many sensors you put on the wafer. With an 8" silicon wafer (same size as the one on the top - notice that half the diameter is at the 'edge'), there are flaws scattered throughout the wafer. The fewer sensors on the wafer and the higher the chance that there will be a flaw in the sensor making it unusable (the 36% waste on a full frame sensor wafer vs. 12.6% waste on the 13.2mm × 8.8mm sensor). This is part of the reason there's often more research done on increasing the density of the chip rather than making it larger (and that density research has other applications like making CPUs go faster).

With a sensor that is intended for a 60mm × 60mm frame, you can only fit about 8 sensors on the wafer and the waste goes up. You can see the economy of scale at work there.

Consider that the 15 or 16 working sensors off of the full frame wafer cost the same to make as the 213 or so smaller sensors... and are priced accordingly. The following image shows the issue with the flaws located in the same places on the wafer for various sized dies.

Sensor yield

(From http://commons.wikimedia.org/wiki/File:Wafer_die%27s_yield_model_(10-20-40mm)_-_Version_2_-_EN.png)

If you are willing to step away from the 'an image in one go' you can get a single array (well, three - one for each color) of sensors that move across the image. These are often found as scanning backs for large format cameras. There, the issue is the precision of the equipment rather than the size of the sensor (memory, data storage, fast I/O become significant). There are some cameras that have this as an integrated unit such as the Seitz 6x17 digital.

Further reading:

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  • \$\begingroup\$ 111 megapixels is small compared to the planned LSST (3.2 gigapixel). I think the current largest operating telescope (in terms of pixels) is PanSTARRS, at 1.4 gigapixel. \$\endgroup\$
    – Joe
    Commented Aug 28, 2014 at 13:07
  • \$\begingroup\$ @Joe the key there is one sensor that is 4" x 4". if you scroll down to the "LSST Focal Plane" section in the link provided you will see explanation of "189 3x3 rafts" where each part of that is a 3 edge mosaic CCD. The mosaic approach can be scaled quite large as you've linked... but its not a single sensor. PanSTARRS uses a similar approach - image-sensors-world.blogspot.com/2007/09/… with an array of CCDs ( pan-starrs.ifa.hawaii.edu/public/design-features/images/… ). For both of those, the sensors are rather small. \$\endgroup\$
    – user13451
    Commented Aug 28, 2014 at 16:28
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The largest CMOS sensors available commercially for photography are "medium format" and measure about 44mm x 33mm. CCDs exist in slightly larger sizes up to 54mm x 40mm. Larger sensors for scientific applications may have been produced.

Sensors are produced by projecting a mask onto a large wafer of silicon using UV light. The wafer is then cut into individual sensors. The absolute size limit of a sensor that could be produced with this method is determined by the size of the image circle produced by the projector (though there may be other concerns with very large sensors, such as power usage and heat dissipation which present a hard limit on size).

The practical limit of sensor size is reached much earlier as it is determined by the yield, that is how many sensors have to be discarded during fabrication due to defects. When making many small sensors on a single wafer a single defect will lead to one sensor being discarded but many more being viable, if one sensor takes up the entire wafer then a single defect will mean no sensors are produced. The yield thus decreases with the square of the sensor size, which makes larger sensors uneconomical.

Economies of scale also apply, 36mm x 24mm "full frame" sensors would be more expensive if produced in the same volume as medium format sensors.

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    \$\begingroup\$ Good answer - I appreciate bringing in the realities of both engineering and business \$\endgroup\$
    – B Shaw
    Commented Aug 27, 2014 at 11:59
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There are even bigger sensors. If you look closely to the image in the top-right corner of that page you'll see that the biggest sensor there is 'Medium Format Kodak KAF' sensor.

Ok, I understand that it isn't quite easy to figure this out because one can easily take that the background of that image is gray while in reality the image has a white background.

See it better here.

Besides that sensor there are another sensors bigger than FF. On the same page scroll to the Table of sensor formats and sizes, click on the 'Crop Factor' column to sort the table and look at the formats with a crop factor smaller than 1. Get out the film formats and you will end up with the following sensors in this order:

  • Phase One P 65+, IQ160, IQ180
  • Leaf AFi 10
  • Medium-format (Hasselblad H5D-60)
  • Kodak KAF 39000 CCD
  • Pentax 645D
  • Leica S

But beware: there are also disadvantages for such sensors: big, heavy cameras and lenses. Much more difficult to build a lens for such a sensor (bigger image circle) and... ...of course... ...price.

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  • \$\begingroup\$ But the Kodak sensor is CCD, not CMOS. \$\endgroup\$
    – Philip Kendall
    Commented Aug 27, 2014 at 11:02
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Some more things that can limit what's practical to below what can be manufactured:

  1. weight (of the resulting system). A very large sensor needs a very large image circle, which means large lenses, and a large camera.
  2. power consumption. A large sensor needs more power than a small one, thus battery life is decreased (unless you again increase the size and weight of the camera to house a larger battery).
  3. speed. It takes longer to read out a larger sensor than it does to read out a smaller one with the same sensor element density. So your "shutter speed" goes down.
  4. cost (hinted at, but comes into play at several levels). A larger sensor of course costs more than a small one, not only because it needs more raw materials but also the amount of discarded products goes up, the cost of which all has to be recapped from the smaller number that are sold.
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  • \$\begingroup\$ I'm surprised no one else mentioned the speed issue. It's also worth mentioning that the larger you get (in inches or cm), the more distortion you get at the edges. There are astronomy papers describing how to describe the projection of the image so that others can understand how the image is distorted so they can re-project it to co-align multiple images. Scaling up in pixels without scaling up in physical size is also a speed issue, as it requires longer exposures for sufficient signal to noise. \$\endgroup\$
    – Joe
    Commented Aug 28, 2014 at 13:15
  • \$\begingroup\$ @Joe that's a side effect of the lens you put in front of the sensor not generating perfectly parallel rays all across the sensor face, not a problem with the sensor itself. You could get around that by making your lenses (and your image circle) that much wider, increasing weight, size, and thus cost of your system even more. \$\endgroup\$
    – jwenting
    Commented Aug 28, 2014 at 14:02

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