Flash Output Power

Flash output power raises a lot of questions when you are trying to decide how to spend your money.

A lot of people writing on the internet decry the versatility of portable speedlights and their use as studio-type lighting – something which is entirely wrong in my opinion; as there is nothing that can’t be done with them, as long as you have enough of them!

And you don’t have to take my word for it – just go and watch the worlds best exponent of the art, in my opinion anyway – Joe McNally. – then tell me if I’m wrong!

But with a top-of-the-line Nikon SB910 running at £340 and Canons new 600EXRT a cool £400 plus here in the UK, purchasing 10 to 15 of these puppies is a wallet-emptying proposition; though given the cash or sponsorship it’s the way I’d go all day long.

A lot of folk come to me with the same quandary – studio flash heads are a lot more cost-effective; notwithstanding their big limiting factor – lack of portability.

Leaving aside the other problems of many studio-style flash heads, namely lack of TTL and HSS/FP facility (though this can be walked-around on certain models with Pocket Wizards and the dark art of Hypersynch) they do give one big advantage – more photons for your buck.

But just how does one compare the flash output power of one unit/type with another – after all, this is what we want to know:

  • Can I get more light from flash A than I can from flash B
  • How many speedlights do I NOT have to buy if I get studio-style flash head C which costs 1.5x the price of one of my speedlights.

The problem is that manufacturers don’t make it easy to do direct comparisons of flash output power between brands and formats, and they tend to try and confuse the buyer with meaningless numbers and endless amounts of jargon.

Back in the days of manual-everything, we used to use flash in a very simple way using the units Guide Number.

The guide number is usually quoted as being at 100 ISO and at two values, one for metres and one for feet, and we use it with the following equation:

GUIDE No: = Distance x Aperture

So we might see a flash unit has a  guide number quoted as 40/131 at 100 ISO.  This means for example, that at 100 ISO and a flash to subject distance of 2.5 metres or 8.2 feet the correct aperture to use would be:

Guide No: divided by distance – in this case 40/2.5m or 131/8.2ft.

Either way the answer is 16, so we would set the shutter speed to the flash synch speed and the aperture to F16.

Simple!

Where things used to go a bit pear-shaped was when we introduced any form of output modifier such as a bounce board or diffuser because these spread and smooth the light and so reduce the number of photons falling on the subject by one or two stops.

But TTL flash metering soon put paid to all that grief.

Camera OEM Speedlights

Let’s compare a Nikon SB800 & SB910 – these have 100 ISO guide numbers of 38/125 & 34/112 respectively (published) – that’s right folks, the new one is weaker than the old one.

But by how much?

Well the old SB800 has a guide number that is 11.7% higher than the newer SB910, but what does this mean in terms of exposure value?

At a flash-to-subject distance of 3.4 metres, doing the maths says that our correct aperture would be 38/3.4 and 34/3.4 respectively. So the SB800 would put us at f11 (11.18 to be precise) while the SB910 would give us f10 – that’s an increase of over 1/3rd of a stop using the older unit.

When working with long lenses and wide apertures this extra 1/3rd of a stop gives me just that little bit more depth of field – and folk wonder why I don’t change mine!

Complications & Caveats

Nikon quote the two units above with guide numbers based on the head “zoom feature” being set to 35mm, which gives a fairly wide angle of lighting.  Someone said to me the other day that the new Canon 600EX was twice the power of the Nikon units I’ve already mentioned, simply because Canon quote the guide number for that device as a massive whopping 60!

The world is full of fools………..

Canon, in their infinite wisdom, quote that 60 value at a zoom head setting of 200mm.  The reality is that the guide number of this Canon unit varies between 26 with the zoom head at 20mm and 60 at 200mm – so in other words, give or take a bit, it’s pretty much in the same ball park as the Nikon units previously mentioned.

Canon speedlight naming policy tells you the units MAXIMUM guide number:

  • 600EX = 60 (metres)
  • 580EX = 58 (metres)
  • 550EX = 55 (metres)

The 550 specs also give you zoom length variations:

  • 105mm = 55 (metres)
  • 50mm = 42 (metres)
  • 17mm = 15 (metres)

Canon 600EX vs Nikon SB800 zoom lengths:

  • 105mm = 58 vs 56 (metres)
  • 50mm  = 42 vs 44 (metres)
  • 14mm = 15 vs 17 (metres)

Light leaves a flash unit in a cone of sorts, and the zoom heads on speedlight style units gather this cone of light so it basically matches the angle of view of the lens you are using and results in an efficient distribution of light across the image area – that’s the theory anyway.

Making the cone “tighter” forces the photons released by the flash into a more concentrated area, thus increasing the number falling on the subject and so increasing the overall exposure value.

So when we use guide numbers to compare various flash units we must ensure that we are comparing the units on a level playing field – in other words, the values we use are for the same “cone or reflector angle”.  And if the manufacturers use different reflector angles when assessing their flash guide numbers for promotion to the public, then you guys ‘n gals run the risk of being hood-winked into buying something that ain’t strictly what you thought it was when you ordered it.

So how do speed light style flash units stack up against studio type units?

Notwithstanding the lack of FP/HSS and any TTL metering problems, studio-type flash heads have guide numbers that are usually quoted as being “with standard reflector”.  This standard reflector is something which gathers those photons and shovels them out in a 50-55 degree spread; think “standard lens” on the image diagonal.

Current top end Nikon speed lights (and Canon) have guide numbers of sub 40 at 35mm reflector angles, and those equate to roughly 64 degrees diagonal coverage.  So if we were to “tighten them up” to 50 or 55 degrees we could, as a rough guide, round the guide numbers up to 42m or 44m.

Now we are on a more even playing field.

A Bowens Gemini 500R is quoted by Bowens as having a guide number of 85 with a standard reflector, so let’s be a bit cavalier with the numbers and say that it’s double the guide number of SB800/910 or 580EX etc.

So roughly how many speed lights is this puppy going to be equivalent to in terms of real flash output power ?

Hands up those who think two………….wrong!

This is where everything you thought you knew about exposure turns to shit in front of your very eyes (but not really!), and it’s called the Inverse Square Law.

Inverse Square Law

Now listen folks, this is as simple or as complicated as you care to make it!

When we capture a scene we capture a 2 dimensional plane filled with photons travelling towards us.

When we shine any light on an object we are actually throwing a flat sheet of light at it. This sheet is expanding outwards as it travels towards the subject because the photons in that sheet of light are all diverging.

So, let’s look at something tangible as an analogy – metric paper sizes!

How many sheets of A3 paper fit on a sheet of A2 paper?

That’s right, TWO – we’ve effectively doubled the surface area of the paper.

Now exposure works in stops – and making a 1 stop change in exposure effectively doubles or halves the exposure value depending on which way we’ve made the adjustment.

So moving from A3 to A2 is like making a 1 stop change in exposure; we’ve doubled the surface area of the paper.  BUT – we’ve not doubled the papers physical dimensions.

What paper size is twice the width AND twice the height of A3 – yep, that’s right, A1.

And how many sheets of A3 fit on a sheet of A1 – right again, 4.

So we have quadrupled the papers surface area – in exposure terms that would equate to 2 stops.

Now imagine a projector throwing an image onto a big screen and the screen to projector distance is 4 metres.  We go to the screen and measure the size of the projected image and it’s 1.5 metres by 2 metres.

How big will the image be if we move the projector to 8 metres from the screen?

Answer – 3 metres x 4 metres. (and the brightness of the image will have gone down by 2 stops).

And if we move the projector to 2 metres from the screen the image will be 0.75 metres x 1 metre. (and the brightness of the image will have increased by 2 stops!).

Inverse Square Law, Lights & Distances

Let’s say we have a theoretical flash with a metres guide number of 80.

If the subject is 10 metres from the light we need an aperture of f8 because 80/10 = 8.

If we now move the light to 5 metres from the subject our aperture decrease to 80/5 = f16

Halving the light-to-subject distance means we increase the overall intensity of the light (its effective flash output power) by 2 stops, so we have to reduce our overall exposure by two stops to compensate; otherwise we’ll just end up with 2 stops of over exposure.

And of course if we move the light away to 20 metres from the subject the inverse applies and we effectively reduce the flash output power by two stops and we’ll have to open the aperture up by two stops to avoid under exposure.

But what do we have to do in order to use f16 at 10 metres AND get correct exposure?

Use a flash with a guide number of 160 is what we’d need to do – it really is that simple.

Reality

So, how many guide number 45 speed lights would we need to equal one guide number 90 studio flash head in terms of effective flash output power?

Well it isn’t two – oh that we should be so lucky!

If we have two speed lights mounted together their cumulative guide number is equal to the square root of the sum of the squares of their individual guide numbers!

Sounds scary, but the answer is 63 or thereabouts.

But here’s the thing about photo-maths – it usually ends up as something really simple and this is no exception.

If you want to double the guide number you always need 4 identical units.

Do not forget what I’ve said above about published guide numbers – you have to ensure that the values were obtained using equal criteria, and manufacturers sometimes don’t always like to furnish you with the information you need in order to do easy comparisons.

Have they got something to hide – you may think that, but I couldn’t possibly comment!

What really does piss me off the meaningless crap they do furnish you with – watt-second, w/s, watt/sec or if you like Joules values.

The only thing these values do is inform you of the “potential energy” available at the capacitor; it’s no measure of how efficiently the flash tube converts that power into photons – and the photons is ALL we’re really interested in.

Other things such as tube temperature can have dramatic effects on both light output and the colour of that light.

Conclusion

This post has been a bit of a ramble but I’ve tried as best I can to give you a rough guide on how to compare one flash source with another.

Different photographers require different things – if all you want to do is shoot portraits and still life then shutter speeds above 1/250th synch are of little importance in general terms, so access to HSS/AutoFP via speed lights isn’t needed, and normal studio lights would be a far more economical proposition.

But on the other hand 8 speed lights in one bank, and two more banks of 4 speed lights each – all HSS/AutoFP compliant – crikey, the photographic possibilities are endless, and readily achievable – if your bank balance is endless too!

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Flash Photography

Flash Photography

 

Red Squirrel,Andy Astbury,Flash,flash photography,fill flash,photography techniques

Really Cute Red Squirrel

 

On Sunday myself and my buddy Mark Davies made a short foray up to the Lake District and our small Red Squirrel site.  The weather was horrible, sleet, sun. rain, cloudy, sunny then rain again – in other words just not conducive to a half-descent session on the D4.

The one Achilles Heal with this site is the fact that it’s hard to get a descent background for your shots – it’s in the middle of a small wooded valley and you just can’t get away from tree trunks in the background.

This is further complicated by the fact that the “Squidgers” have a propensity for keeping in the ‘not so sunny’ bits, so frequently you end up with a scenario where backgrounds are brighter than foregrounds – which just won’t DO!

So what’s needed is some way to switch the lighting balance around to give a brighter foreground/subject AND a darker background.

Now that sounds all very well BUT; how do we achieve it?

Reflectors perhaps?  They’d do the trick but have one big problem; they rely on AMBIENT light  – and in the conditions we were shooting in the other day the value of the ambient light was up and down like a Yo-Yo.

Wouldn’t it be cool if we could have a consistent level of subject/foreground illumination AND at the same time have some degree of control over the exposure of the background?

Well with flash we can do just that!

Let’s look at a shot without flash:

 

No FLASH

No FLASH, AMBIENT light only – 1/320th @ f7.1

 

I don’t suppose this shot is too bad because the background isn’t strongly lit by the sun (it’s gone behind a cloud again!) but the foreground and background are pretty much the same exposure-wise.  For me there is not enough tonal separation between the two areas of the image, and the lighting is a bit flat.

If we could knock a stop or so out of the background; under expose it, then the image would have more tonal separation between foreground and background, and would look a lot better, but of course if we’re just working with ambient light then our adjusted exposure would under expose the foreground as well, so we’d be no better off.

Now look at the next image – we’ve got a background that’s under exposed by around  -1.5Ev, but the subject and foreground are lit pretty much to the same degree as before, and we’ve got a little more shape and form to the squirrel itself – it’s not quite so flat-looking.

 

With FLASH

With FLASH added – 1/800th @ f7.1

 

The image also has the slight sense that it’s been shot in more sunny conditions – which I can promise you it wasn’t !

And both images are basically straight off the camera, just with my neutral camera profile applied to them on import.

 

The Set Up

The Setup - shocking iPhone 3 quality!

The Setup – shocking iPhone 3 quality!

 

The first secret to good looking flash photography OF ANY KIND is to get the damn flash OFF the camera.

If we were in a totally dark studio with the sexiest looking model on the planet we’d NOT be lighting her with one light from the camera position now would we?

So we use basic studio lighting layouts where ever we can.

There are two other things to consider too:

  •   It’s broad daylight, so our exposure will contain both FLASH and an element of AMBIENT light – so we are working along the premise of ADDING to what’s already there.
  •   If we put the flash closer to the subject (off camera) then the output energy has less distance to travel in order to do its job – so it doesn’t have to have as much power behind it as it would have if emanating from the camera position.

 

You can see in the horrible iPhone 3 shot I took of the setup that I’m using two flash guns with white Lambency diffusers on them; one on a stand to the left and slightly in front of the log where the squirrels will sit, and one placed on the set base (Mr. Davies old knackered Black & Decker Workmate!) slightly behind the log and about the same distance away from where I anticipate a squirrel will sit on the log as the left flash.

The thing to note here is that I’m using the SIDE output of these Lambency diffuser domes and NOT the front – that’s why they are pointed up at the sky. The side output of these diffusers is very soft – just what the flash photography doctor ordered in terms of ‘keeping it real’.

The left light is going to be my MAIN light, the right is my FILL light.

The sun, when & if it decides to pop its head out, will be behind me and to my left so I place my MAIN light in a position where it will ‘simulate’ said ball in the sky.

The FILL light basically exists to ‘counter balance’ the ‘directionality’ of the MAIN light, and to weaken any shadows thrown by the MAIN light.

Does this flash bother a subject? For the most part NOT SO YOU’D NOTICE!

Take a look at the shot below – the caption will be relevant shortly.

This SB800 has just fired in "front curtain synch" and the balance of the exposure is from the ambient light - the shutter is still open after the flash has died. Does the squirrel look bothered?

This SB800 has just fired in “front curtain synch” and the balance of the exposure is from the ambient light. Does the squirrel look bothered?

Settings & The Black Art!

Before we talk about anything else I need to address the shutter curtain synch question.

We have two curtain synch options, FRONT & REAR.

Front Curtain (as in the shot above) – this means that the flash will fire as the front curtain starts to move, and most likely, the flash will be finished long before the rear curtain closes. If your subject reacts to the flash then some element of subject movement might be present in the shot due to the ambient light part of the exposure.

Rear Curtain Synch – my recommended ‘modus operandi’ – the ‘ambient only’ part of the exposure gets done first, then the flash fires as the rear curtain begins to close the exposure. This way, if the subject reacts to the flash the exposure will be over before it has chance to – MOSTLY!

The framing I want, and the depth of field I want dictates my camera position and aperture – in this case f7 or f8 – actually f7.1 is what I went for.

 

I elect to go with 2000 iso on the D4.

So now my only variable is shutter speed.

Ambient light dictates that to be 1/320th on average, and I want to UNDER EXPOSE that background by at least a stop and a bit (technical terms indeed!) so I elect to use a shutter speed of 1/800th.

So that’s it – I’m done; seeing as the light from the flashes will be constant my foreground/subject will ALWAYS be exposed correctly. In rear curtain synch I’ll negate the risk of subject movement ‘ghosting’ in the image, and at 1/800th I’ll have a far better chance of eliminating motion blur caused by a squirrel chewing food or twitching its whiskers etc.

 

Triggering Off-Camera Flashes

 

We can fire off-camera flashes in a number of ways, but distance, wet ground, occasional rain and squirrels with a propensity for chewing everything they see means CORDS ain’t one of ’em!

With the Nikon system that I obviously use we could employ another flash on-camera in MASTER/COMMANDER mode, with the flash pulse deactivated; or a dedicated commander such as the SU800; or if your camera has one, the built-in flash if it has a commander mode in the menu.

The one problem with Nikon CLS triggering system, and Canons as far as I know, is the reliance upon infra-red as the communication band. This is prone to a degree of unreliability in what we might term ‘dodgy’ conditions outdoors.

I use a Pocket Wizard MiniTT1 atop the camera and a FlexTT5 under my main light. The beauty of this system is that the comms is RADIO – far more reliable outdoors than IR.

Because a. I’m poor and can’t afford another TT5, and b. the proximity of my MAIN and FILL light, I put the SB800 FILL light in SU mode so it gets triggered by the flash from the MAIN light.

What I wouldn’t give for a dozen Nikon SB901’s and 12 TT5s – I’d kill for them!

The MAIN light itself is in TTL FP mode.

The beauty of this setup is that the MAIN light ‘thinks’ the TT5 is a camera, and the camera ‘thinks’ the miniTTL is a flash gun, so I have direct communication between camera and flash of iso and aperture information.

Also, I can turn the flash output down by up to -3Ev using the flash exposure compensation button without it having an effect on the background ambient exposure.

Don’t forget, seeing as my exposure is always going to 1/800th @ f7.1 at 2000 iso the CAMERA is in MANUAL exposure mode. So as long as the two flashes output enough light to expose the subject correctly at those settings (which they always will until the batteries die!) I basically can’t go wrong.

When shooting like this I also have a major leaning towards shooting in single servo – one shot at a time with just one AF point active.

 

Flash Photography – Flash Duration or Burn Time

Now here’s what you need to get your head around. As you vary the output of a flash like the SB800 the DURATION of the flash or BURN TIME of the tube changes

Below are the quoted figures for the Nikon SB800, burn time/output:

1/1050 sec. at M1/1 (full) output
1/1100 sec. at M1/2 output
1/2700 sec. at M1/4 output
1/5900 sec. at M1/8 output
1/10900 sec. at M1/16 output
1/17800 sec. at M1/32 output
1/32300 sec. at M1/64 output
1/41600 sec. at M1/128 output

On top of that there’s something else we need to take into account – and this goes for Canon shooters too; though Canon terminology is different.

Shutter Speed & The FP Option

35mm format cameras all have a falling curtain shutter with two curtains, a front one, and a rear one.

As your press the shutter button the FRONT curtain starts to fall, then the rear curtain starts to chase after it, the two meet at the bottom of the shutter plane and the exposure is over.

The LONGER or slower the shutter speed the greater head-start the front curtain has!

At speeds of 1/250th and slower the front curtain has reached the end of its travel BEFORE the rear curtain wakes up and decides to move – in other words THE SENSOR is FULLY exposed.

The fastest shutter speed that results in a FULLY EXPOSED film plane/sensor is the basic camera-to-flash synch speed; X synch as it used to be called, and when I started learning about photography this was usually 1/60th; and on some really crap cameras it was 1/30th!

But with modern technology and light weight materials these curtains can now get moving a lot faster, so basic synch now runs at 1/250th for a full frame DSLR.

If you go into your flash camera menu you’ll find an AUTO FP setting for Nikon, Canon refer to this as HSS or High Speed Synch – which makes far more sense (Nikon please take note, Canon got something right so please replicate!).

There’s something of an argument as to whether FP stands for Focal Plane or Flash Pulse; and frankly both are applicable, but it means the same as Canon’s HSS or High Speed Synch.

At speeds above/faster than 1/250th the sensor/film plane is NOT fully exposed. The gap between the front and rear curtains forms a slot or ‘letter box’ that travels downwards across the face of the sensor, so the image is, if you like, ‘scanned’ onto the imaging plane.

Obviously this is going to cause on heck of an exposure problem if the flash output is ‘dumped’ as a single pulse.

So FP/HSS mode physically pulses or strobes the flash output to the point where it behaves like a continuous light source.

If the flash was to fire with a single pulse then the ‘letterbox slot’ would receive the flash exposure, but you’d end up with bands of under exposure at the bottom or top of the image depending on the curtain synch mode – front or rear.

In FP/HSS mode the power output of each individual pulse in the sequence will drop as the shutter speed shortens, so even though you might have 1:1 power selected on the back of the flash itself (which I usually do on the MAIN light, and 1/2 on the FILL light) the pulses of light will be of lower power, but their cumulative effect gives the desired result.

By reviewing the shot on the back of the camera we can compensate for changes in ambient in the entire scene (we might want to dilute the effect of the main light somewhat if the sun suddenly breaks out on the subject as well as the background) by raising the shutter speed a little – or we might want to lighten the shot globally by lowering the shutter speed if it suddenly goes very gloomy.

We might want to change the balance between ambient and flash; this again can be done from the camera with the flash exposure compensation controls; or if needs be, by physically getting up and moving the flash units are little nearer or further away from the subject.

All in all, using flash is really easy, and always has been.

Except nowadays manufacturers tend to put far more controls and modes on things then are really necessary; the upshot of which is to frighten the uninitiated and then confuse them even further with instruction manuals that appear to be written by someone under the influence of Class A drugs!

 

"Trouble Brewing.." Confrontation over the right to feed between two Red Squirrels.

“Trouble Brewing..” Confrontation over the right to feed between two Red Squirrels.

 

The whole idea of flash is that it should do its job but leave no obvious trace to the viewer.

But its benefits to you as the photographer are invaluable – higher shutter speeds, more depth of field and better isolation of the subject from its background are the three main ones that you need to be taking advantage of right now.

If you have the gear and don’t understand how to use it then why not book a tuition day with me – then perhaps I could afford some more TT5s!

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