Dynamic Range, Mid Tones, Metering and ETTR

Dynamic Range, Mid Tones, Metering and ETTR

I recently uploaded a video to my YouTube channel showing you an easy way to find the ‘usable dynamic range’ of you dSLR:

 

The other day I was out with Paul Atkins for a landscape session in the awesome Dinorwic Quarry in Llanberis, Snowdonia.  Highly dynamic clouds and moody light made the place look more like Mordor!

dynamic range

Looking towards the top of the Llanberis Pass from the middle level of Dinorwic Quarry and Electric Mountain.

Here are the 6 unedited shots that make this finished panoramic view:

dynamic range

As you can see, the images are are shot in a vertical aspect ratio.  Shooting at 200mm on the D800E this yields an assembled pano that is 16,000 x 7000 pixels; the advantages for both digital sales and print should be obvious to you!

As you can see, the bright parts of the sky are a lot brighter in the captures than they are in the finished image, but they are not ‘blown’.  Also the shadows in the foreground are not choked or blocked.

In other words the captures are shot ETTR.

Meter – in camera or external.

Any light meter basically looks at a scene (or part thereof) and AVERAGES the tones that it sees.  This average value value is then classed by the meter is MID GREY and the exposure is calculated in terms of the 3 variables you set – Time, Intensity and Applied Gain, or shutter, aperture and ISO.

But this leads to all sorts of problems.

All meters are calibrated to an ANSI Standard of 12% grey (though this gets a bit ambiguous between manufactures and testers).  But you can get a good idea of what ‘light meter mid grey/mid tone” looks like by mentally assigning an RGB value of 118,118,118 to it.

However, we – humans – find 18% grey a more acceptable ‘mid tone grey’ both in print and on our modern monitors.

NOTE: 18% grey refers to the level of REFLECTANCE – it reflects 18% of the light falling on it.  It can also be reproduced in Photoshop using a grey with 128,128.128 RGB values.

So problem number 1 is that of mid tone perception and the difference between what you ‘see’ and what the camera sees and then does in terms of exposure (if you let the camera make a decision for you).

dynamic range

128RGB grey versus 118RGB meter mid grey

Click on the pano image from Dinorwic to view it bigger, then try to FIND a mid grey that you could point your camera meter at – you can’t.

Remember, the grey you try to measure MUST be exactly mid-grey – try it, it’ll drive you nuts trying to find it!

This leads us to problem number 2.

Take your camera outside, find a white wall.  Fill your frame with it and take a shot using ZERO exposure compensation – the wall will look GREY in the resulting shot not WHITE.

Next, find something matte black or near to it.  Fill your frame with it and take another shot – the black will look grey in the shot not black(ish).

Problem number 3 is this – and it’s a bit of a two-headed serpent.  An exposure meter of any kind is COLOUR BLIND but YOU can SEE colours but are tonally blinded to them to some degree or other:

Simple primary red, green and blue translate to vastly different grey tones which comes as a big surprise to a lot of folk, especially how tonally light green is.

Scene or Subject Brightness Range

Any scene in front of you and your camera has a range of tones from brightest to darkest, and this tonal range is the subject brightness range or SBR for short.  Some folk even refer to it as the scene dynamic range.

If you put your camera meter into spot mode you can meter around your chosen scene and make note of the different exposure values for the brightest and darkest areas of your potential shot.

You camera spot meter isn’t the most accurate of spot meters because its ‘spot’ is just too big, typically between 4mm and 5mm, but it will serve to give you a pretty good idea of your potential SBR.

A 1 degree spot meter will, with correct usage, yield a somewhat more accurate picture (pun intended) of the precise SBR of the scene in front of you.

Right about now some of you will be thinking I’m hair-splitting and talking about unnecessary things in todays modern world of post-processing shadow and highlight recovery.

Photography today is full of folk who are prepared to forego the CRAFT of the expert photographer in favour of getting it half-right in camera and then using the crutch of software recovery to correct their mistakes.

Here’s the news – recovery of popped highlights is IMPOSSIBLE and recovery of shadows to anymore than a small degree results in pixel artifacting.  Get this, two WRONGS do NOT make a RIGHT!

If the Mercedes F1 team went racing with the same attitude as the majority of camera users take pictures with, then F1 would be banned because drivers would die at an alarming rate and no car would ever make the finish line!

So, one way or another we can quantify our potential scene SBR.

“But Andy I don’t need to do that because my camera meter does that for me…….”

Oh no it does NOT, it just averages it to what IT THINKS is a correct mid tone grey – which it invariably isn’t!

This whole mid tone/mid grey ‘thing’ is a complete waste of time because:

  • It’s near impossible to find a true mid tone in your scene to take a reading off.
  • What you want as a mid tone will be at odds with your camera meter by at least 1/2stop.
  • If you are shooting wildlife or landscapes you can’t introduce a ‘grey card’.
  • Because of the above, your shot WILL BE UNDER EXPOSED.

“Yeah, but I can always bracket my shots and do an exposure blend Andy so you’re still talking crap….”

Two answers to that one:

  1. You can’t bracket shots and blend if your MAIN subject is moving – de-ghosting is only effective on small parts of a scene with minimal movement between frames.
  2. The popular “shoot and bracket two each end” makes you look like total dickhead and illustrates that you know less than zero about exposure.  Try doing that on a paying job in front of the client and see how long you last in a commercial environment.

By far the BEST way of calculating exposure is the ETTR method.

ETTR, Expose to the Right.

If you meter for a highlight, your camera will treat that as a mid tone because your camera ASSUMES it’s a mid tone.

Your camera meter is a robot programmed to react to anything it sees in EXACTLY the same way.  It doesn’t matter if your subject is a black cat in the coal house or a snow man in a snow storm, the result will be the same 118,118,118 grey sludge.

Mid tones are as we’ve already ascertained, difficult to pin down and full of ambiguity but highlights are not.  So let’s meter the brightest area of the image and expose it hard over to the right of the histogram.

The simplest way to achieve this is to use your live view histogram with the camera in full manual mode.

Unlike the post-shot review histogram, the live-view histogram is not subject to jpeg compression, and can be thought of as something of a direct readout of scene tonality/brightness.

Using your exposure controls (usually shutter speed for landscape photography) you can increase your exposure to push the highlight peak of the histogram to the right as far as you can go before ‘hitting the wall’ on the right hand side of the histogram axis – in other words the camera sensor highlight clipping point.

Of course, this has the added benefit of shifting ALL the other tones ( mids and shadows) to the right as well,resulting in far less clipping potential in your shadow areas.

So back to Dinorwic again and here’s a shot that has been exposed ETTR on the live view histogram using spot metering over what I deemed to be the brightest area of the sky:

The red square indicates the approximate size of the spot meter area.

I was a naughty boy not recording this on video for you but I forgot to pack the HDMI lead for the video recorder – I’ll do one shortly!

The problem with using the Live View Histogram is that it can be a bit of a struggle to see it.  your live view screen itself can be hard to see in certain light conditions outside, and the live view histogram itself is usually a bit on the small side – no where near as big as the image review histogram you can see here.

But looking at the review histogram above you can see that there’s a ‘little bit more juice’ to be had in terms of exposure of the highlights because of that tiny gap between the right end of the histogram and the ‘wall’ at the end of the axis.

Going back to the video the maximum ETTR ‘tipping point’ was centered around these three shots:

Clipped

Not Clipped (the one we allocated the star rating to). Exposure is -1/3rd stop below clipped.

Safe, but -2/3rd stop below Clipped.

The review histogram puts the Dinorwic shot highlights firmly in the same exposure bracket as ‘Safe, but -2/3rd stop below Clipped, and tells us there is another 1/3rd stop ‘more juice’ to be had!

So lengthening the exposure by 1/3rd stop and changing from 160th sec to 1/50th sec gives us this:

The red square indicates the approximate size of the spot meter area.

Live View Histogram ETTR

Live View Histogram plus 1/3 stop more juice! Highlights STILL below Clipping Point and shadows get 1/3rd stop more exposure.

That’s what it’s all about baby – MORE JUICE!

And you will not be in a position to confidently acquire more juice unless you find the USABLE DYNAMIC RANGE of your camera sensor.

The whole purpose of finding that usable DR is to discover where your highlight and shadow clipping points are – and they are very different between camera models.

For instance, the highlight clipping point value of the Nikon D850 is different from that of the Nikon D800E, but the shadow clipping point is pretty similar.

There is an awful lot more use to discovering your cameras usable dynamic range than a lot of folk imagine.

And if you do it the precise way then you can acquire a separate meter that will accept camera profiling:

dynamic range

You can create a dynamic range profile for your camera (and lens combo*) and then load it into the meter:

and then have your cameras usable dynamic range as part of the metering scale – so then you have NO EXCUSE for producing a less than optimum exposure.

(*)Note: yes, the lens does have an effect on dynamic range due to micro-contrast and light transmission variables – if you want to be super-picky!

AND THEY SAY HANDHELD METERS ARE DEAD, OLD TECH and of NO USE!!!

Anyone who says or even thinks that is a total KNOB.

Your camera dynamic range, the truthful one – FIND IT, KNOW IT, USE IT.

And don’t listen to the idiots and know-nothings, just listen and heed the advice of those of us who actually know what we’re doing.

NOTE:  The value of grey (gray) cards and how to use them for accurate measurement is a subject in its own right and provides the curious with some really interesting reading.  Believe me it’s far more expansive than the info I’ve given here.  But adopting an ETTR approach when exposing to sensor that you KNOW the physical behavior of (dynamic response to light/dynamic range) can alleviate you of all critical mid-tone concerns.

This article has taken me over 8 hours to produce in total, and is yours to view for FREE.  If you feel I deserve some support for doing this then please consider joining my membership site over on Patreon by using the link below.

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ETTR High Contrast Scene Processing.

ETTR High Contrast Scene Processing.

When faced with a high contrast scene like this most photographers would automatically resort to bracketing shots.

Sometimes you will be in a situation where shooting a bracketed sequence is difficult or impossible.

But a single image exposed to the right of the histogram – ETTR – where highlights are recorded at their maximum level of exposure can allow the camera sensor to capture far more detail in the darker areas than Lightroom will allow you to see at first glance.

Exposing to the right (of the in-camera histogram) correctly means that you expose the brightest scene highlights AS HIGHLIGHTS.

But it’s a balancing act between exposing them fully, and ‘blowing’ them.

Getting the ETTR exposure correct invariably means that the sensor receives MORE exposure across all tonal ranges, so you end up with more usefully recoverable shadow detail too.

In this video I show you a full Lightroom and Photoshop workflow to produce a noise-free image from a raw file exposed in just such a way.

Members of my Patreon site can download the all the workflow steps together with the raw file so that they can follow my processing, and perhaps come up with their own versions too!

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Lumenzia Plugin for Photoshop: https://getdpd.com/cart/hoplink/21529?referrer=c0vpzfhvq7ks8cw8c

Lumenzia + Comprehensive Training: https://getdpd.com/cart/hoplink/21529?referrer=c0vpzfhvq7ks8cw8c&p=165704

Just to keep you up to speed on my video channel, here’s my previous video from last week which illustrates how I do my dust-spot and blemish removal in Photoshop:

Exposure Value – What does it mean?

Exposure Value (Ev) – what does Ev mean?

I get asked this question every now and again because I frequently use it in the description annotations of image shot data here on the blog.

And I have to say from the outset the Exposure Value comes in two flavours – relative and absolute – and here I’m only talking mainly about the former.

So, let’s start with basic exposure.

Exposure can be thought of as Intensity x Time.

Intensity is controlled by our aperture, and time is controlled by our shutter speed.

This image was shot at 0.5sec (time), f11 (intensity) and ISO 100.

exposure value

We can think of the f11 intensity of light striking the sensor for 0.5sec as a ‘DOSAGE’ – and if that dosage results in the desired scene exposure then that dosage can be classed as the exposure value.

Let’s consider two exposure settings – 0.5sec at f11 ISO100 and 1sec at f16 ISO 100.

Technically speaking they are two different exposures, but BOTH result in the same light dosage at the sensor.  The second exposure is TWICE the length of time but HALF the intensity.

So both exposures have the same Exposure Value or Ev.

The following exposure of the same scene is 1sec at f11 ISO 100:

exposure value

The image was shot at the same intensity (f11) but the shutter speed (time) was twice as long, and so the dosage was doubled.  Double the dose = +1Ev!

And in this version the exposure was 0.25sec at f11 ISO 100:

exposure value

Here the light dosage at the sensor is HALF that of the correct/desired exposure because the time factor was halved while using the same intensity.

So half the dose = -1Ev!

Now some of you will be thinking that -1Ev is 1 stop under exposure – and you’d be right!

But Ev, or exposure value, is just a cleaner way of thinking about exposure because it doesn’t tie you to any specific camera setting – and it’s more easily transferable between cameras.

What Do I Mean by that?

Example – If I use say a 50mm prime lens on my Nikon D800E with the metering in matrix mode, ISO 100 and f14 I might get a metered exposure shutter speed of 1/10th of a second.

But if I replace the D800E with a D4 set at 100 ISO, matrix and f14 I’ll guarantee the metered shutter speed requirement will be either 1/13 or 1/15th of a second.

The D4 meters between -1/3Ev and -2/3Ev (in other words 1/2 stop) faster/brighter than the D800E when fitted with the same lens and set to the same aperture and ISO, and shooting exactly the same framing/composition.

Yet the ‘as metered’ shots from both cameras look pretty much the same with respect to light dosage – exposure value.

Exposure Settings Don’t Transfer between camera models very well, because the meter in a camera is calibrated to the response curve of the sensor.

A Canon 1DX Mk2 will usually generate a evaluative metered shutter speed 1/3rd of a stop faster than a matrix metered Nikon D4S for the same given focal length, aperture and ISO setting.

Both setups ‘as metered’ shots will look pretty much the same, but transposing the Canon settings to the Nikon will result in -1/3 stop under exposure – which on a digital camera is definitely NOT the way to go!

‘As Metered’ can be regarded as +/-0Ev for any camera (Note: this does NOT mean Ev=0!)

Any exposure compensation you use in order to achieve the ‘desired’ exposure on the other hand can be thought of as ‘metered + or – xEv’.

exposure compensation

Shot with the D4 plus 70-200 f2.8@70mm in manual exposure mode, 1/2000th sec, f8 and ISO 400 using +2/3Ev compensation.

The matrix metered exposure indicated by the camera before the exposure value compensation was 1/3200th – this would have made the Parasitic Jaeger (posh name for an Arctic Skua!) too dark.

A 1DXMk2 using the corresponding lens and focal length, f8, ISO 400 and evaluative metering would have wanted to generate a shutter speed of at least 1/4000th sec without any exposure compensation, and 1/2500th with +2/3Ev exposure compensation.

And if shot at those settings the Canon image would look pretty much like the above.

But if the Nikon D4 settings had been fully replicated on the Canon then the shot would be between 1/3 and 1/2 stop over exposed, risking ‘blowing’ of some of the under-wing and tail highlights.

So the simple lesson here is don’t use other photographers settings – they never work unless you’re on identical gear! 

But if you are out with me and I tell you “matrix/evaluative plus 1Ev” then your exposure will have pretty much the same ‘light dosage’ as mine irrespective of you using the right shutter speed, aperture or ISO for the job or not!

I was brought up to think in terms of exposure value and Ev units, and to use light meters that had Ev scales on them – hell, the good ones still have ’em!

If you look up the ‘tech-specs’ for your camera you’ll find that metering sensitivity is normally quoted as an Ev range.  And that’s not all – your auto focus may well have a low light Ev limited quoted too!

To all intents and purposes Ev units and your more familiar ‘f-stops’ amount to one and the same thing.

As we’ve seen before, different exposures in terms of intensity and time can have the same exposure value, and all Ev is concerned with is the cumulative outcome of our shutter speed, aperture and ISO choices.

Most of you will take exposures at ‘what the camera meter says’ settings, or you will use the meter indicated exposure as a baseline and modify the exposure settings with either positive or negative ‘weighting’ via your exposure compensation dial.

That’s Ev compensation relative to your meters baseline.

But have you ever asked yourself just how accurate your camera meter is?

So I’ve just stepped outside my front door and taken these two frames:

exposure value

EV=15/Sunny 16 Rule 1/100th sec, f16, 100 ISO – click to view large.

exposure value

Matrix Metering, no exposure compensation 1/200th sec, f16, ISO 100 – click to view large

These two raw files have been brought into Lightroom and THE ONLY adjustment has been to change the profile from Adobe Color to Camera Neutral.

Members of my subscription site can download the raw files and see for themselves.

Look at the histogram in both images!

The exposure for xxx164.NEF (the top image) is perfection personified while xxx162.NEF is under exposed by ONE WHOLE STOP – why?

Because the bottom image has been shot at the camera-specified matrix metered exposure, while the top image has been shot using the good old ‘Sunny 16 Rule’ that’s been around since God knows when!

“Yeah, but I could just use the shadow recovery slider on the bottom shot Andy….”  Yes, you could, if you wanted to be an idle tit, and even then the top image would still be better because there’s no ‘recovery’ being used on it in the first place.  Remember, more work at the camera means less work in processing!

Recovery of either shadows or highlights is ‘poor form’ and no substitute for correct exposure in the first place. Digital photography is just like shooting colour transparency film – you need to ‘peg the highlights’ as highlights BUT without over exposing them and causing them to ‘blow’.

In other words – ETTR, expose to the right!

And seeing as your camera meter wants to turn everything into midtone grey shite it’s the very last thing you should ever allow to dictate your final exposure settings – as the two images above prove beyond argument.

And herein lies the problem.

Even if you use the spot metering function the meter will read the brightness of what is covered by the ‘spot’ and then calculate the exposure required to expose that tonal brightness AS A MID TONE GREY.

That’s all fine ‘n dandy – if the metered area is actually an exact mid tone.  But what if you were metering a highlight?

Then the metered exposure would want to expose said highlight as a midtone and the overall highlight exposure would be far too dark.  And you can guess what would happen if you trusted your meter to spot-read a shadow.

A proper hand-held spot meter has an angle of view or AoV of 1 degree.

Your camera spot meter angle of view is dictated by the focal length of the lens you have fitted.

On my D800E for example, I need to have a lens AoV of around 130mm focal length equivalent for my spot to cover 1 degree, because the ‘spot’ is 4mm in diameter – total stupidity.

But it does function fairly well with wider angle lenses and exposure calculations when used in conjunction with the live view histogram.  And that will be subject of my next blog post – or perhaps I’ll do a video for YouTube!

So I doubt this blog post about relative exposure compensation is going to light your world on fire – it began as an explanation to a recurring question about my exif annotation habits and snowballed somewhat from there!

But I’ll leave you with this little guide to the aforementioned Sunny 16 Rule, which has been around since Noah took up boat-building:

To use this table just set your ISO to 100.

Your shutter speed needs to be the reciprocal of your ISO – in other words 1/100 sec for use with the stated aperture values:

Aperture Lighting conditions Shadow PROPERTIES
f/22* Snow/sand Dark with sharp edges
f/16 Sunny Distinct
f/11 Slight overcast Soft around edges
f/8 Overcast Barely visible
f/5.6** Heavy overcast No shadows
f/4 Open shade/sunset No shadows

* – I would not shoot at f22 because of diffraction – try 1/200th f16

** – let’s try some cumulative Ev thinking here and go for more depth of field using f11 and sticking with 100 ISO. -2Ev intensity (f5.6 to f11) requires +2Ev on time, so 1/100th sec becomes 1/25th sec.

Over the years I’ve taken many people out on photo training days, and a lot of them seem to think I’m some sort of magician when I turn their camera on, switch it manual, dial in a couple of settings and produce a half decent image without ever looking at the meter on their camera.

It ain’t magic – I just had this table burnt into the back of my eyeballs years ago.

Works a charm – if you can do the mental calculations in your head, and that’s easy with practice.  The skill is in evaluating your shooting conditions and relating them to the lighting and shadow descriptions.

And here’s a question for you; we know our camera meter wants to ‘peg’ what it’s measuring as a midtone irrespective of whether it’s measuring a midtone or not.  But what do you think the Sunny 16 Rule is ‘pegging’ and where is it pegging it on the exposure curve?

If you can answer that question correctly then the other flavour of exposure value – absolute – might well be of distinct interest to you!

Give it a try, and if you use it correctly you’ll never be more than 1/3rd of a stop out, if that.  Then you can go and unsubscribe from all those twats on YouTube who told you it was out-dated and defunct or never told you about it in the first place!

I hope you’ve found the information in this post useful.

I don’t monetize my YouTube videos or fill my blog posts with masses of affiliate links, and I rely solely on my patrons to help cover my time and server costs. If you would like to help me to produce more content please visit my Patreon page on the button above.

Many thanks and best light to you all.

Camera ISO Settings

The Truth About ISO

Andy Astbury,noise,iso

The effect of increased ISO – in camera “push processing” automatically lift the exposure value to where the camera thinks it is supposed to be.

Back in the days of ‘wet photography’, we had rolls and sheets of film that carried various ISO/ASA/DIN numbers.

ISO stands for International Standards Organisation

ASA stands for American Standards Association

DIN – well, that’s ‘Deutsches Institut für Normung’ or German Institute for Standardisation

ISO and ASA were basically identical values, and DIN = (log10)ISO x10 +1, so ASA/ISO 100 equated to DIN 21….nope, I’m not going to say anything!

These numbers were the film ‘speed’ values.  Film speed was critical to exposure metering as it specified the film sensitivity to light.  Metering a scene properly at the correct ISO/ASA/DIN gave us an overall exposure value that ensured the film got the correct ‘dose’ of light from the shutter speed and aperture combination.

Low ISO/ASA/DIN values meant the film was LESS sensitive to light (SLOW FILM) and high values meant MORE sensitivity to light (FAST FILM).

Ilford Pan F was a very slow mono negative film at ASA 50, while Ilford HP5 was a fast 400 ASA mono negative film.

The other characteristic of film speed was ‘grain’.  Correctly exposed, Pan F was extremely fine grained, whereas correctly exposed HP5 was ‘visibly grainy’ on an 8×10 print.

Another Ilford mono negative film I used a lot was FP4.  The stated ASA for this film was 125ASA/ISO, but I always rated it (set the meter ASA speed dial) to 100ASA on my 35mm Canon A1 and F1 (yup, you read that right!) because they both slightly over-metered most scenes.

If we needed to shoot at 1/1000th and f8 but 100ASA only gave us 1/250th at f8 we would switch to 400ASA film – two stops greater sensitivity to light means we can take a shutter speed two stops shorter for the same aperture and thus get our required 1/1000th sec.

But, what if we were already set up with 400ASA film, but the meter (set at 400ASA) was only giving us 1/250th?

Prior to the release of films like Delta 1600/3200 we would put a fresh roll of 400ASA film in the camera and set the meter to a whopping 1600ASA! We would deliberately UNDER EXPOSE Ilford HP5 or Kodak Tri-X by 2 stops to give us our required 1/1000th at f8.

The two stops underexposed film would then be ‘push processed’, which basically meant it was given a longer time in the developer.  This ‘push processing’ always gave us a grainy image, because of the manner in which photographic chemistry worked.

And just to confuse you even more, very occasionally a situation might arise where we would over expose film and ‘pull process’ it – but that’s another story.

We are not here for a history lesson, but the point you need to understand is this – we had a camera body into which we inserted various sensitivities of film, and that sometimes those sensitivities were chemically manipulated in processing.

That Was Then, This Is Now!

ISO/ASA/DIN was SENSITIVITY of FILM.

It is NOT SENSITIVITY of your DSLR SENSOR….!!! Understand that once and for all!

The sensitivity of your sensor IS FIXED.

It is set in Silicon when the sensor is manufactured.  Just like the sensitivity of Kodak Tri-X Pan was ‘fixed’ at 400ASA/ISO when it was made at the factory.

How is the sensitivity of a digital sensor fixed?  By the SIZE of the individual PHOTOSITES on the sensor.

Larger photosites will gather more photons from a given exposure than small ones – it’s that simple.

The greater the number of photons captured means that the output signal from a larger photosite is GREATER than the output signal from a smaller photosite for the same exposure value (EV being a combination shutter speed and aperture/f number).

All sensors have a base level of noise – we can refer to this as the sensor ‘noise floor’.

This noise floor is an amalgamation of the noise floors of each photosite on the sensor.

But the noise floor of each photosite on the sensor is masked/obscured by the photosite signal output; therefore the greater the signal, the larger the signal to noise (S/N) ratio is said to be.

In general, larger photosites yield a higher S/N ratio than smaller ones given the same exposure.

This is why the Nikon D3 had such success being full frame but just over 12 megapixels, and it’s the reason that some of us don’t get overly excited about seeing more megapixels being crammed into our 36mm x 24mm sensors.

Anyway, the total output from a photosite contains both signal and noise floor, and the signal component can be thought of as ‘gain’ over the noise floor – natural gain.

As manufacturers put more megapixels on our sensors this natural gain DECREASES because the photosites get SMALLER – they have to in order to fit more of them into the finite sensor area.

Natural gain CAN be brought back in certain sensor designs by manipulating the design of the micro lenses that sit on top of the individual photosites. Re-design of these micro lenses to ‘suck in’ more tangential photons – rather like putting a funnel in a bottle to make filling it easier and more efficient.

There is a brilliantly simple illustration of how a sensor fits into the general scheme of things, courtesy of digital camera world:

Camera ISO Settings

The main item of note in this image is perhaps not quite so obvious, but it’s the boundary between the analogue and digital parts of the system.

We have 3 component arrays forward of this boundary:

  1. Mosaic Filter including Micro Lenses & Moire filter if fitted.
  2. Sensor Array of Photosites – these suck in photons and release proportional electrons/charge.
  3. Analogue Electronics – this holds the charge record of the photosite output.

Everything forward of the Analogue/Digital Converter – ADC – is just that, analogue! And the variety of attributes that a manufacturer puts on the sensor forward of this boundary can be thought of mostly as modifying/enhancing natural gain.

So What About My ISO Control Settings Andy?

All sensors have a BASE ISO. In other words they have an ISO sensitivity/speed rating just like film!  And as I said before THIS IS A FIXED VALUE.

The base ISO of a sensor photosite array can be defined as that ISO setting that yields the best dynamic range across the whole array, and it is the ISO setting that carries NO internal amplification.

Your chosen ISO setting has absolutely ZERO effect on what happens forward of the Analogue/Digital boundary – NONE.

So, all those idiots who tell you that ISO effects/governs exposure are WRONG – it has nothing to do with it for the simple reason that ISO effecting sensor sensitivity is a total misconception….end of!

Now I’ll bet that’s going to set off a whole raft of negative comments and arguments – and they will all be wrong, because they don’t know what they’re talking about!

The ‘digital side’ of the boundary is where all the ‘voodoo’ happens, and it’s where your ISO settings come into play.

At the end of an exposure the Analogue Digital Converter, or ADC, comes along and makes a ‘count’ of the contents of the ‘analogue electronics’ mosaic (as Digital Camera World like to call it – nice and unambiguous!).

Remember, it’s counting/measuring TOTAL OUTPUT from each photosite – and that comprises both signal and noise floor outputs.

Camera ISO Settings

If the exposure has been carried out at ‘base ISO’ then we have the maximum S/N ratio, as in column 1.

However, if we increase our ISO setting above ‘base’ then the total sensor array output looks like column 2.  We have in effect UNDER EXPOSED the shot, resulting in a reduced signal.  But we have the same value for the noise floor, so we have a lower S/N ratio.

In principal, the ADC cannot discriminate between noise floor and signal outputs, and so all it sees in one output value for each photosite.

At base ISO this isn’t a problem, but once we begin to shoot at ISO settings above base, under exposing in other words, the cameras internal image processors apply gain to boost the output values handed to it by the ADC.

Yes, this boosts the signal output, but it also amplifies the noise floor component of the signal at the same time – hence that perennial problem we all like to call ‘high ISO noise’.

So your ISO control behaves in exactly the same way as the ‘gain switch’ on a CB or long wave radio, or indeed the db gain on a microphone – ISO is just applied gain.

Things You Should Know

My first digital camera had a CCD (charge coupled device) sensor, it was made by Fuji and it cost a bloody fortune.

Cameras today for the most part use CMOS (complimentary metal oxide semi-conductor) sensors.

  • CCD sensors create high-quality, low-noise images.
  • CMOS sensors, traditionally, are more susceptible to noise.
  • Because each photosite on a CMOS sensor has a series of transistors located next to it, the light sensitivity of a CMOS chip tends to be lower. Many of the photons striking the sensory photosite array hit the transistors instead of the photosites.  This is where the newer micro lens designs come in handy.
  • A CMOS sensor consumes less power. CCD sensors can consume up to 100 times more power than an equivalent CMOS sensor.
  • CMOS chips can be produced easily, making them cheaper to manufacture than CCD sensors.

Basic CMOS tech has changed very little over the years – by that I’m referring to the actual ‘sensing’ bit of the sensor.  Yes, the individual photosites are now manufactured with more precision and consistency, but the basic methodology is pretty much ‘same as it ever was’.

But what HAS changed are the bits they stick in front of it – most notably micro-lens design; and the stuff that goes behind it, the ADC and image processors (IPs).

The ADC used to be 12 bit, now they are 14 bit on most digital cameras, and even 16 bit on some.  Increasing the bit depth accuracy in the ADC means it can detect smaller variations in output signal values between adjacent photosites.

As long as the ‘bits’ that come after the ADC can handle these extended values then the result can extend the cameras dynamic range.

But the ADC and IPs are firmware based in their operation, and so when you turn your ISO above base you are relying on a set of algorithms to handle the business of compensating for your under exposure.

All this takes place AFTER the shutter has closed – so again, ISO settings have less than nothing to do with the exposure of the image; said exposure has been made and finished with before any ISO applied gain occurs.

For a camera to be revolutionary in terms of high ISO image quality it must deliver a lower noise floor than its predecessor whilst maintaining or bettering its predecessors low ISO performance in terms of noise and dynamic range.

This where Nikon have screwed their own pooch with the D5. At ISOs below 3200 it has poorer IQ and narrower dynamic range than either the D4 or 4S.  Perhaps some of this problem could be due to the sensor photosite pitch (diameter) of 6.45 microns compared to the D4/4S of 7.30 microns – but I think it’s mostly due to poor ADC and S/N firmware; which of course can be corrected in the future.

Can I Get More Photons Onto My Sensor Andy?

You can get more photons onto your sensor by changing to a lens that lets in more light.

You might now by thinking that I mean switching glass based on a lower f-number or f-stop.

If so you’re half right.  I’m actually talking about t-stops.

The f-number of a lens is basically an expression of the relationship between maximum aperture diameter and focal length, and is an indication of the amount of light the lens lets in.

T-stops are slightly different. They are a direct indicator of how much light is transmitted by the lens – in other words how much light is actually being allowed to leave the rear element.

We could have two lenses of identical focal length and f-number, but one contains 17 lens elements and the other only 13. Assuming the glass and any coatings are of equal quality then the lens with fewer elements will have a higher transmission value and therefore lower T-number.

As an example, the Canon 85mm f1.2 actually has a t-number of 1.4, and so it’s letting in pretty much HALF a stop less light than you might think it is.

In Conclusion

I’ve deliberately not embellished this post with lots of images taken at high ISO – I’ve posted and published enough of those in the past.

I’ve given you this information so that you can digest it and hopefully understand more about how your camera works and what’s going on.  Only by understanding how something works can you deploy or use it to your best advantage.

I regularly take, market and sell images taken at ISO speeds that a lot of folk wouldn’t go anywhere near – even when they are using the same camera as me.

The sole reason I opt for high ISO settings is to obtain very fast shutter speeds with big glass in order to freeze action, especially of subjects close to the camera.  You can freeze very little action with a 500mm lens using speeds in the hundredths of a second.

Picture buyers love frozen high speed action and they don’t mind some noise if the shot is a bit special. Noise doesn’t look anywhere near as severe in a print as it does on your monitor either, so high ISO values are nothing to shy away from – especially if to do so would be at the expense of the ‘shot of a lifetime’.

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The ND Filter

Long Exposure & ND Filters

long exposure,slow shutter speed,ND filter,CMOS sensor,noise

A view of the stunning rock formations at Porth Y Post on the Welsh island of Anglesey. The image is a long exposure of very rough sea, giving the impression of smoke and fog.  30 seconds @f13 ISO 100. B&W 10stop ND – unfiltered exposure would have been 1/30th.

The reason for this particular post began last week when I was “cruising” a forum on a PoD site I’m a member of, and I came across a thread started by someone about heavy ND filters and very long exposures.

Then, a couple of days later a Facebook conversation cropped up where someone I know rather well seemed to be losing the plot over things totally by purchasing a 16 stop ND.

The poor bugger got a right mauling from “yours truly” for the simple reason that he doesn’t understand the SCIENCE behind the art of photography.  This is what pisses me off about digital photography – it readily provides “instant gratification” to folk who know bugger all about what they are doing with their equipment.  They then spend money on “pushing the envelope” only to find their ivory tower comes tumbling down around them because they THOUGHT they knew what they were doing………..stop ranting Andy before you have a coronary!

OK, I’ll stop “ranting”, but seriously folks, it doesn’t matter if you are on a 5DMkIII or a D800E, a D4 or a 1Dx – you have to realise that your camera works within a certain set of fixed parameters; and if you wander outside these boundaries for reasons of either stupidity or ignorance, then you’ll soon be up to your ass in Alligators!

Avid readers of this blog of mine (seemingly there are a few) will know that I’ve gone to great lengths in the past to explain how sensors are limited in different ways by things such as diffraction and that certain lens/sensor combinations are said to be “diffraction limited; well here’s something new to run up your flag pole – sensors can be thought of as being “photon limited” too!

I’ll explain what I mean in a minute…..

SENSOR TYPE

Most folk who own a camera of modern design by Nikon or Canon FAIL at the first hurdle by not understanding their sensor type.

Sensors generally fall into two basic types – CCD and CMOS.

Most of us use cameras fitted with CMOS sensors, because we demand accurate fast phase detection AF AND we demand high levels of ADC/BUFFER speed.  In VERY simplistic terms, CCD sensors cannot operate at the levels of speed and efficiency demanded by the general camera-buying public.

So, it’s CMOS to the rescue.  But CMOS sensors are generally noisier than CCDs.

When I say “noise” I’m NOT referring to the normal under exposure luminance noise that a some of you might be thinking of. I’m talking about the “background noise” of the sensor itself – see post HERE .

Now I’m going to over simplify things for you here – I need to because there are a lot of variables to take into account.

  • A Sensor is an ARRAY of PHOTOSITES or PHOTODIODES
  • A photodiode exists to do one thing – react to being struck by PHOTONS of light by producing electrons.
  • To produce electrons PROPORTIONAL to the number of photons that strike it.

Now in theory, a photodiode that sees ZERO photons during the exposure should release NO ELECTRONS.

At the end of the exposure the ADC comes along and counts the electrons for each photodiode – an ANALOGUE VALUE – and converts it to a DIGITAL VALUE and stores that digital value as a point of information in the RAW file.

A RAW converter such as Lightroom then reads all these individual points of information and using its own in-built algorithms it normalises and demosaics them into an RGB image that we can see on our monitor.

Sounds simple doesn’t it, and theoretically it is.  But in practice there’s a lot of places in the process where things can go sideways rapidly……..!

We make a lot of assumptions about our pride and joy – our newly purchased DSLR – and most of these assumptions are just plain wrong.  One that most folk get wrong is presuming ALL the photodiodes on their shiny new sensor BEHAVE IN THE SAME WAY and are 100% identical in response.  WRONG – even though, in theory, it should be true.

Some sensors are built to a budget, some to a standard of quality and bugger the budget.

Think of the above statement as a scale running left to right with crap sensors like a 7D or D5000 on the left, and the staggering Phase IQ260 on the right.  There isn’t, despite what sales bumph says, any 35mm format sensor that can come even close to residing on the right hand end of the scale, but perhaps a D800E might sit somewhere between 65 and 70%.

The thing I’m trying to get at here is that “quality control” and “budget” are opposites in the manufacturing process, and that linearity and uniformity of photodiode performance costs MONEY – and lots of it.

All our 35mm format sensors suffer from a lack of that expensive quality control in some form or other, but what manufacturers try to do is place the resulting poor performance “outside the envelope of normal expected operation” as a Nikon technician once told me.

In other words, during normal exposures and camera usage (is there such a thing?) the errors don’t show themselves – so you are oblivious to them. But move outside of that “envelope of normal expected operation” and as I said before, the Alligators are soon chomping on your butt cheeks.

REALITY

Long exposures in low light levels – those longer than 30 to 90 seconds – present us with one of those “outside the envelope” situations that can highlight some major discrepancies in individual photodiode performance and sensor uniformity.

Earlier, I said that a photodiode, in a perfect world, would always react proportionally to the number of photons striking it, and that if it had no photon strikes during the exposure then it would have ZERO output in terms of electrons produced.

Think of the “perfect” photodiode/photosite as being a child brought up by nuns, well mannered and perfectly behaved.

Then think of a child brought up in the Gallagher household a la “Shameless” – zero patience, no sense of right or wrong, rebellious and down right misbehaved.  We can compare this kid with some of the photodiodes on our sensor.

These odd photodiodes usually show a random distribution across the sensor surface, but you only ever see evidence of their existence when you shoot in the dark, or when executing very long exposures from behind a heavy ND filter.

These “naughty” photodiodes behave badly in numerous ways:

  • They can release a larger number of electrons than is proportional to their photon count.
  • They can go to the extreme of releasing electrons when the have a ZERO photon count.
  • They can mimic the output of their nearest neighbors.
  • They can be clustered together and produce random spurious specks of colour.

And the list goes on!

It’s a Question of Time

These errant little buggers basically misbehave because the combination of low photon count and overly long exposure time allow them to, if you like, run out of patience and start misbehaving.

It is quite common for a single photodiode or cluster of them to behave in a perfect manner for any shutter speed up to between 30 seconds and 2 minutes. But if we expose that same photodiode or cluster for 3 minutes it can show abnormal behavior in its electron output.  Expose it for 5 minutes and its output could be the same, or amplified, or even totally different.

IMPORTANT – do not confuse these with so-called “hot pixels” which show up in all exposures irrespective of shutter duration.

Putting an ND filter in front of your lens is the same as shooting under less light.  Its effect is even-handed across all exposure values in the scenes brightness range, and therein lies the problem.  Cutting 10 stops worth of photons from the highlights in the scene will still leave plenty to make the sensor work effectively in those areas of the image.

But cutting 10 stops worth of photons from the shadow areas – where there was perhaps 12 stops less to begin with – might well leave an insufficient number of photons in the very darkest areas to make those particular photodiodes function correctly.

Exposure is basically a function of Intensity and Time, back in my college days we used to say that Ex = I x T !

Our ND filter CUTS intensity across the board, so Time has to increase to avoid under exposure in general.  But because we are working with far fewer photons as a whole, we have to curb the length of the Time component BECAUSE OF the level of intensity reduction – we become caught in a “Catch 22” situation, trying to avoid the “time triggered” malfunction of those errant diodes.

Below is an 4 minute exposure from behind a Lee Big Stopper on a 1Dx – click on both images to open at full resolution in a new window.

long exposure,slow shutter speed,ND filter,CMOS sensor,noise

Canon 1Dx
4 minutes @ f13
ISO 200 Lee 10stop

long exposure,slow shutter speed,ND filter,CMOS sensor,noise

The beastly Nikon D800E fairs a lot better under similar exposure parameters, but there are still a lot of repairs to be done:

long exposure,slow shutter speed,ND filter,CMOS sensor,noise

A 4 minute exposure on a D800, f11 at 200ISO

Most people use heavy ND filters for the same reason I do – smoothing out water.

long exposure,slow shutter speed,ND filter,CMOS sensor,noise

The texture of the water in the top shot clutters the image and adds nothing – so get rid of it! D4,ISO 50, 30secs f11 Lee Big Stopper

Then we change the camera orientation and get a commercial shot:

long exposure,slow shutter speed,ND filter,CMOS sensor,noise

Cemlyn Bay on the northwest coast of Anglesey, North Wales, Approximately 2.5 km to the east is Wylfa nuclear power station. Same exposure as above.

In this next shot all I’m interested in is the jetty, neither water surface texture or horizon land add anything – the land is easy to dump in PShop but the water would be impossible:

long exposure,slow shutter speed,ND filter,CMOS sensor,noise

I see the bottom image in my head when I look at the scene top left. Again, the 10 stop ND fixes the water, which adds precisely nothing to the image. D4 ISO 50, 60 secs, f14 B&W 10 stop

The mistake folk make is this, 30 seconds is usually enough time to get the effect on the water you want, and 90 to 120 seconds is truly the maximum you should ever really need.  Any longer and you’ll get at best no more effect, and at worst the effect will not look as visually appealing – that’s my opinion anyway.

This time requirement dovetails nicely with the “operating inside the design envelope” physics of the average 35mm format sensor.

So, as I said before, we could go out on a bit of a limb and say that our sensors are all “photon limited”; all diodes on the sensor must be struck by x number of photons.

And we can regard them as being exposure length limited; all diodes on the sensor must be struck by x photons in y seconds in order to avoid the pitfalls mentioned.

So next time you have the idea of obtaining something really daft, such as the 16 stop ND filter my friend ordered, try engaging your brain.  An unfiltered exposure that meters out at 1/30th sec will be 30 seconds behind a 10 stop ND filter, and a whopping 32 minutes behind a 16 stop ND filter.  Now at that sort of exposure time the sensor noise in the image will be astonishing in both presence and variety!

As I posted on my Book of Face page the other day, just for kicks I shot this last Wednesday night:

long exposure,slow shutter speed,ND filter,CMOS sensor,noise

Penmon Lighthouse in North Wales at twilight.
Sky is 90 secs, foreground is 4 minutes, D4, f16, ISO 50 B&W 10 stop ND filter

The image truly gives the wrong impression of reality – the wind was cold and gusting to 30mph, and the sea looked very lumpy and just plain ugly.

I spent at least 45 minutes just taking the bloody speckled colour read noise out of the 4 minute foreground exposure – I have to wonder if the image was truly worth the effort in processing.

When you take into account everything I’ve mentioned so far plus the following:

  • Long exposures are prone to ground vibration and the effects of wind on the tripod etc
  • Hanging around in places like the last shot above is plain dangerous, especially when it’s dark.

you must now see that keeping the exposures as short as possible is the sensible course of action, and that for doing this sort of work a 6 stop ND filter is a more sensible addition to your armoury than a 16 stop ND filter!

Just keep away from exposures above 2 minutes.

And before anyone asks, NO – you don’t shoot star trails in one frame over 4 hours unless you’re a complete numpty!  And for anyone who thinks you can cancel noise by shooting a black frame think on this – the black frame has to be shot immediately after the image, and has to be the same exposure duration as the main image.  That means a 4 hour single frame star trail plus black frame to go with it will take at least 8 hours – will your camera battery last that long?  If it dies before the black frame is finished then you lose BOTH frames……………

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