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We're ready for our practical demonstration on how
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to determine a correct exposure.
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Before we do that, we have to discuss
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different camera modes because that'll, of course, affect
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our exposure.
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Now, you've probably bought your first camera, maybe
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you're actually an experienced professional, but the first
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time you picked up that camera, you actually
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noticed a few different settings.
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Now, of course, we have auto, program, shutter
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priority, aperture priority, and manual.
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Now, auto is quite seductive because it's usually
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green on the dial and basically the camera
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does all the thinking for you.
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My suggestion is don't do that because you
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probably would have noticed that the first time
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you use your camera on holiday, photographing your
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pets, family, whatever it may be, it's a
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little bit weird and the exposures are all
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out of the place.
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Perhaps it's blurry.
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There's all these things that can go wrong.
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The camera is only a tool.
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It can't do the thinking for you.
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It does a lot of the thinking for
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you, but you've got to actually use it
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properly.
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So now, program.
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Do we use program in a professional environment?
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My encouragement to you is do not use
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program because there's gonna be a lot of
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things that you'd need to change based upon
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the genre in which you're photographing.
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Now, that gives us three modes left.
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We have shutter priority, aperture priority, and manual.
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Well, shutter priority might work for people who
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do different kind of sports, for example.
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You might be photographing the tennis and you
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know that you have to be at a
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certain speed to photograph tennis or the football,
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or it could be car racing.
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Well, you know that it has to be
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at 2,000 speed, a fraction of a
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second, or 8,000th of a second.
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Well, that's fine, great.
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I'm telling you, if you're photographing people, though,
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then you actually arguably would only ever use
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two modes.
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And I'm saying to you, I would rather
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you only use one of them, and you
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probably know what mode that is.
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Well, aperture priority, for example.
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We understand what aperture priority is.
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We're prioritizing the aperture that we want, of
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course, which will determine how many things are
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in focus, and we call that depth of
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field.
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So if you want more things in focus,
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you've probably heard of f-stops, right?
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So you've got f-stop, like, say, 1
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.2, 1.8, 2.8, f4, 5.6,
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and so on.
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The confusing part about it is that if
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you go to f1.2 or 1.4,
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it's wide open, and you think, well, wait
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a second, is this more or less things
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in focus because of it?
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I want you to actually think about it
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this way.
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If it's f1.2, it's a small number.
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Yes, it's a big aperture.
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If it's a small number, it means less
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things are in focus.
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As it goes to 2.8, f4, 5
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.6, f8, there's gonna be more things in
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focus.
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So think of it like that.
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More things in focus, the higher the f
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number, the more things in focus, fantastic.
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So that's aperture priority.
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Now we prioritize the aperture, and then, of
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course, in that mode, we can prioritize the
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ISO that we want, but then the camera
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will choose the appropriate speed.
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But the problem is that, of course, the
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speed might not be the one that you
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need.
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It might be too slow, you might get
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blur, and there's all things that can go
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wrong.
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And yes, of course, as we talk about
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the golden triangle, or at least the triangle
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of exposure, we have ISO, we have shutter
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speed, and we have aperture.
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Yes, we can actually have any of these
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things on automatic, shutter priority, aperture priority.
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We can even have auto ISO.
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I strongly discourage you letting the camera doing
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the thinking for you, especially if you're photographing
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people, let alone in an environment that doesn't
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change.
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As in, if you're photographing me now, for
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example, that's quite predictable.
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Here's the exposure, fantastic.
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The minute you start to widen your angle
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of view, your exposure will change based upon
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the values within that frame.
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Now, we'll discuss this further a little bit
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in a moment.
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Now, if you photograph on manual, you're choosing
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everything, and arguably it's more difficult, no different
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than driving an automatic car and then driving
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a manual car.
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Yes, it's gonna be a little bit more
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difficult.
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You're gonna do more things, but you can
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take control more.
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Now, what we're doing right now is I'm
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gonna photograph a white piece of board.
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It's nothing exciting at this stage, but I
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wanna emulate a pale-skinned bride wearing a
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white dress sling and a white wool or
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a polar bear in a snowstorm.
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And let's see how aperture priority handles this
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environment.
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So right now, I am on aperture priority.
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I am at 3200 of a second, f2
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.8, 400 ISO.
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Now, it's a white board, and I've actually
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had to focus on a cut in the
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board because, of course, it's nondescript.
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It'll be very hard to focus.
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So right now, although I'm actually physically seeing
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a white board, in my camera, if you
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were to photograph something white, it's going to
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underexpose it.
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It's going to make it gray.
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You have to understand that the camera is
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not racist.
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It's actually gonna pick something in between.
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It doesn't care about black.
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It doesn't care about white.
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Whatever tones the camera sees, it's going to
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make it mid-gray.
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It has to have a standard.
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It's not gonna be polarizingly white or black.
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It's going to be mid-gray.
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So what happens is the camera is going
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to evaluate what's in the scene and then
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determine what it believes to be a correct
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exposure.
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Why aperture priority doesn't work, and we'll talk
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about metering modes in a moment, but at
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the moment, we're actually using matrix and evaluative
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metering.
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We're evaluating the entire frame, and now we
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are underexposing badly.
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Now, you'd think sort of almost the opposite.
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Now, if you sort of see something white,
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you think, oh my God, I'm photographing something
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white now.
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I should underexpose this.
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Well, the camera is already doing that for
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you.
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It's counterintuitive.
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You have to think about it.
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If something is light, bright, white, you have
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to overexpose, and I say that inverted commas
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because you're not overexposing.
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You're exposing correctly, but you have to understand
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what the camera is doing and thinking.
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So let's go back to this now.
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What we have to do now is I'm
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gonna switch the camera to manual and emulate
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the exact same settings.
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Now, yes, I can use compensation, exposure compensation.
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This is basically where I can leave it
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on aperture priority and compensate with the exposure,
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but that will get that value from the
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shutter speed.
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I would rather determine where I want that
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particular value to come out of.
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Does that make any sense?
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So in this case, I am going to
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emulate the exact same exposure.
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I'm gonna go 3,200 of a second,
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2.8, 400 ISO.
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So let me do that.
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3,200 and 2.8 and 400 ISO.
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Great, so we're seeing the exact same thing.
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Now, what did we say?
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If your subject matter is bright, you go
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bright, lean towards the plus, and if your
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subject is dark, you go dark, lean towards
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the minus.
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Now, what do I mean when I'm saying
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that?
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Well, if you look in your camera and
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your viewfinder, most cameras, of course, will have
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a exposure meter in the actual viewfinder.
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Now, here we have a plus, minus, and
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a zero.
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Zero represents where the camera thinks that good
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exposure is, plus represents overexposed, minus represents underexposed.
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So what I have to do now is
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this.
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I have to deliberately overexpose, as in expose
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correctly, because that's the exposure that I want,
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but overexpose what the camera is saying to
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make this white card look white.
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So now I have latitude and room to
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breathe in my shutter speed, and from experience,
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I believe we're gonna be about five to
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six clicks, and when I say clicks, I
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mean third-stop increments towards the plus sign.
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So in your exposure triangle, you have ISO,
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you have aperture, and you have shutter speed.
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You can use one, two, or three of
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these combinations to click towards the plus sign.
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So in this case, I am going to
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click once, two, three, four, five, six.
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So now I've determined that something white is
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going to be about two stops, as in
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there's six third-stop increments.
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A third, a third, a third is one
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stop, and then third, third, third is two
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stops.
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So now we've got two stops difference from
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the original.
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So if you shot aperture priority with a
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polar bear in a snowstorm, you would have
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underexposed all of those shots, and that's gonna
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be a problem, and the minute you start
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introducing different elements other than white, again, your
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exposure changes again.
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So all I know now is, and what
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you know, anything white, and if you cover
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up your camera and your meter, depending on
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whether you're spot metering or you're evaluative metering,
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matrix metering, which we'll discuss shortly, you need
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to overexpose, by what the camera is saying,
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by two stops.
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Okay, fantastic.
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So we've got that.
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Now what happens when we actually put, we
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switch this to black?
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Now we'll do that shortly, but what I
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wanna discuss with you is this.
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Once you determine a correct exposure, if you
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want more or less things in focus, you
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can't just move one thing, because right now
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I'm on manual, I'm at 800th of a
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second, F 2.8 400 ISO.
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Now I'm shooting with an 85 millimeter 1
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.8 lens, so if I want, now of
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course it doesn't matter because I've just got
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a white background here, but if I had
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subject matter in front of me, foreground, background,
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middle ground, and I wanted to choose, let's
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say an aperture of maybe F2, well you
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can see how now I've overexposed this by
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one stop, which means that I have to
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actually bring that value down, either with my
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shutter speed or my ISO or both.
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So, let's go back to where we were.
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I'm at 800th of a second, F 2
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.8 and 400 ISO.
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00:09:30,700 --> 00:09:32,500
We might say, well, wait a second, I
269
00:09:32,500 --> 00:09:35,060
can get more quality out of this photograph,
270
00:09:35,320 --> 00:09:37,500
which means that ISO affects quality.
271
00:09:38,020 --> 00:09:43,040
Let me now actually go to 200 ISO,
272
00:09:45,640 --> 00:09:47,800
and let's go three clicks down.
273
00:09:47,880 --> 00:09:49,780
So now I have 400th of a second
274
00:09:49,780 --> 00:09:51,460
at F 2.8 and 200 ISO.
275
00:09:52,380 --> 00:09:54,460
Both of those were correct exposures.
276
00:09:54,860 --> 00:09:57,920
This one, I get better quality, and I
277
00:09:57,920 --> 00:09:59,380
have a safe handheld speed.
278
00:09:59,880 --> 00:10:04,260
It really only changes really dramatically when you're
279
00:10:04,260 --> 00:10:06,100
looking at different F stops, as in how
280
00:10:06,100 --> 00:10:07,420
many things you want in focus.
281
00:10:07,720 --> 00:10:09,660
If you can get better quality, why wouldn't
282
00:10:09,660 --> 00:10:09,840
you?
283
00:10:10,480 --> 00:10:12,780
But certainly, depending on how many things you
284
00:10:12,780 --> 00:10:14,220
want in focus, you want to change that.
285
00:10:14,300 --> 00:10:16,360
So remember, once you determine the correct exposure,
286
00:10:16,540 --> 00:10:18,520
you change one more thing, you've got to
287
00:10:18,520 --> 00:10:22,680
change two or three things of that exposure
288
00:10:22,680 --> 00:10:23,240
triangle.
289
00:10:23,640 --> 00:10:26,820
So now that we've determined what will happen
290
00:10:26,820 --> 00:10:29,460
to a white subject matter, what will happen
291
00:10:29,460 --> 00:10:32,260
now when we look at black subject matter?
292
00:10:32,460 --> 00:10:32,980
Let's do it.
293
00:10:33,940 --> 00:10:35,840
So now we have black subject matter.
294
00:10:36,200 --> 00:10:37,860
It could be likens of maybe four African
295
00:10:37,860 --> 00:10:39,720
-American men wearing a black suit leaning on
296
00:10:39,720 --> 00:10:40,320
a black wall.
297
00:10:40,540 --> 00:10:44,020
If you were shooting aperture priority, then I
298
00:10:44,020 --> 00:10:45,380
think you'd know already what's going to happen.
299
00:10:45,560 --> 00:10:46,440
So if I'm going to look in the
300
00:10:46,440 --> 00:10:49,320
camera right now, I'm seeing a black piece
301
00:10:49,320 --> 00:10:52,120
of card and I'm shooting aperture priority.
302
00:10:52,260 --> 00:10:54,420
It's 125th of a second, 2.8, 400
303
00:10:54,420 --> 00:10:56,860
ISO, and it's a terrible exposure.
304
00:10:56,860 --> 00:10:58,700
What is black is now mid gray.
305
00:10:58,840 --> 00:10:59,360
It's terrible.
306
00:10:59,940 --> 00:11:04,980
You've just overexposed this shot ridiculously.
307
00:11:05,220 --> 00:11:08,860
Now, if we thought something white was actually,
308
00:11:09,040 --> 00:11:11,640
with two stops, we proved that we need
309
00:11:11,640 --> 00:11:14,140
to overexpose to get a correct exposure.
310
00:11:14,280 --> 00:11:14,840
What did we say?
311
00:11:14,920 --> 00:11:16,420
If something is bright, you go bright lean
312
00:11:16,420 --> 00:11:17,740
towards the plus sign.
313
00:11:18,260 --> 00:11:19,880
Now, if something is black, let's do the
314
00:11:19,880 --> 00:11:20,160
opposite.
315
00:11:20,340 --> 00:11:23,040
If something is black, let's go dark, let's
316
00:11:23,040 --> 00:11:25,880
go black lean towards the minus with one,
317
00:11:26,060 --> 00:11:27,820
two, or three of the things that affect
318
00:11:27,820 --> 00:11:30,300
our exposure, either with the ISO, the shutter
319
00:11:30,300 --> 00:11:31,520
speed or the aperture.
320
00:11:31,880 --> 00:11:33,060
So in this case, what I'm going to
321
00:11:33,060 --> 00:11:35,180
do now is I'm seeing something gray.
322
00:11:35,320 --> 00:11:37,680
I'm going to flick my mode, my camera
323
00:11:37,680 --> 00:11:40,660
mode to manual and I'm getting the exact
324
00:11:40,660 --> 00:11:41,380
same exposure.
325
00:11:41,640 --> 00:11:43,960
What is black is actually gray.
326
00:11:44,360 --> 00:11:46,400
So I'm going to move my shutter speed
327
00:11:46,400 --> 00:11:48,780
dial because I'm actually quite happy with 400
328
00:11:48,780 --> 00:11:51,100
ISO, quite happy with 2.8 in the
329
00:11:51,100 --> 00:11:52,180
context of this demonstration.
330
00:11:52,640 --> 00:11:56,140
And now I'm actually going to underexpose by
331
00:11:56,140 --> 00:11:59,520
about five clicks, as in five third stop
332
00:11:59,520 --> 00:12:01,740
increments, which is equal to one and two
333
00:12:01,740 --> 00:12:02,720
thirds of a stop.
334
00:12:03,080 --> 00:12:04,880
So let's count the clicks.
335
00:12:05,140 --> 00:12:08,840
We're going to go one, two, three, four,
336
00:12:09,360 --> 00:12:09,840
five.
337
00:12:09,920 --> 00:12:10,940
Let's have a look at that.
338
00:12:11,760 --> 00:12:13,640
I would say we can even go one
339
00:12:13,640 --> 00:12:14,780
more, which is the equivalent.
340
00:12:14,940 --> 00:12:17,460
So now I am seeing something black.
341
00:12:17,600 --> 00:12:19,100
So guess what we've just proven?
342
00:12:19,100 --> 00:12:23,320
We have proven that white and black accordingly
343
00:12:23,720 --> 00:12:27,340
will actually over and underexpose by two stops.
344
00:12:27,820 --> 00:12:30,240
Now that you know that, now you look
345
00:12:30,240 --> 00:12:31,400
at your subject matter in a bit of
346
00:12:31,400 --> 00:12:34,200
a different way and learn how each of
347
00:12:34,200 --> 00:12:36,900
those values will change based upon introducing new
348
00:12:36,900 --> 00:12:37,240
elements.
349
00:12:37,660 --> 00:12:39,740
For example, now we have something black.
350
00:12:40,060 --> 00:12:43,500
What happens if we added maybe a third
351
00:12:43,500 --> 00:12:45,960
of the frame with a white dress and
352
00:12:45,960 --> 00:12:47,080
maybe Caucasian skin?
353
00:12:47,320 --> 00:12:48,300
What will happen then?
354
00:12:48,300 --> 00:12:50,260
There's all these things we have to determine,
355
00:12:50,440 --> 00:12:53,280
but now that we've determined two stops will
356
00:12:53,280 --> 00:12:55,760
be under and overexposed respectively with black and
357
00:12:55,760 --> 00:12:58,800
white, now let's look at the nuances when
358
00:12:58,800 --> 00:13:01,020
we start to add some different subject matter
359
00:13:01,020 --> 00:13:01,540
in the frame.
360
00:13:02,340 --> 00:13:04,620
So we determined what we believe to be
361
00:13:04,620 --> 00:13:08,320
a correct exposure based upon a completely black
362
00:13:08,320 --> 00:13:08,820
scene.
363
00:13:09,460 --> 00:13:11,100
Now, yes, of course, if you start adding
364
00:13:11,100 --> 00:13:13,440
skin tones and white dresses and things like
365
00:13:13,440 --> 00:13:14,680
that, it may change.
366
00:13:15,260 --> 00:13:17,340
And yes, of course, too, if you're photographing
367
00:13:17,340 --> 00:13:18,900
with mirrorless, what you see is what you
368
00:13:18,900 --> 00:13:19,160
get.
369
00:13:19,400 --> 00:13:20,980
What we're trying to do now is determine
370
00:13:20,980 --> 00:13:22,860
what we believe to be a correct exposure
371
00:13:22,860 --> 00:13:24,480
and what's the quickest way of getting there
372
00:13:24,480 --> 00:13:26,440
and what's gonna be the most efficient way.
373
00:13:26,780 --> 00:13:28,940
Now, I didn't change my exposure whatsoever.
374
00:13:29,500 --> 00:13:31,520
Once I determined what I believed was black
375
00:13:32,000 --> 00:13:33,480
and I had a feeling it was a
376
00:13:33,480 --> 00:13:36,020
little bit light, but now I've actually introduced
377
00:13:36,020 --> 00:13:36,960
Sally, our mannequin.
378
00:13:37,360 --> 00:13:38,860
And if you look at her, you would
379
00:13:38,860 --> 00:13:40,320
say she's exposed correctly.
380
00:13:40,480 --> 00:13:43,080
We see detail in her skin tone per
381
00:13:43,080 --> 00:13:46,260
se, and we see detail and creases in
382
00:13:46,260 --> 00:13:46,620
the white.
383
00:13:46,620 --> 00:13:49,000
I still feel that maybe we're a touch
384
00:13:49,000 --> 00:13:49,420
over.
385
00:13:49,780 --> 00:13:51,480
So what I'm gonna do now is go
386
00:13:51,480 --> 00:13:53,560
one click down, and now you can start
387
00:13:53,560 --> 00:13:55,820
to see the shadow underneath her bust and
388
00:13:55,820 --> 00:13:56,540
a bit more detail.
389
00:13:56,980 --> 00:13:58,900
So we're about a third stop out.
390
00:13:59,080 --> 00:14:03,000
Of course, if I had skin tone, skin
391
00:14:03,000 --> 00:14:04,840
and white dress in my scene, it would
392
00:14:04,840 --> 00:14:06,300
have been more obvious, but I was about
393
00:14:06,300 --> 00:14:07,500
a third stop out.
394
00:14:07,880 --> 00:14:10,220
So now we're looking at that as well.
395
00:14:10,340 --> 00:14:11,000
We're looking good.
396
00:14:11,100 --> 00:14:11,820
So guess what?
397
00:14:12,120 --> 00:14:15,860
Now I can actually photograph my entire scene
398
00:14:16,260 --> 00:14:17,260
in this environment.
399
00:14:17,600 --> 00:14:20,000
When I start to introduce new elements in
400
00:14:20,000 --> 00:14:21,920
this shot, in other words, if I widen
401
00:14:21,920 --> 00:14:25,280
my angle of view, I have less white,
402
00:14:25,400 --> 00:14:26,700
I have more black, and so on and
403
00:14:26,700 --> 00:14:27,180
so forth.
404
00:14:27,500 --> 00:14:29,160
Now let me explain in more detail what
405
00:14:29,160 --> 00:14:29,620
that means.
406
00:14:30,120 --> 00:14:34,740
Right now, the camera originally was evaluating the
407
00:14:34,740 --> 00:14:35,860
actual entire scene.
408
00:14:36,280 --> 00:14:38,580
So with different camera systems, it's either called
409
00:14:38,580 --> 00:14:40,740
matrix metering or evaluative metering.
410
00:14:40,920 --> 00:14:42,560
We're evaluating the entire scene.
411
00:14:42,700 --> 00:14:44,580
If we look at our exposure meter now,
412
00:14:45,220 --> 00:14:45,980
look at it.
413
00:14:46,080 --> 00:14:48,220
We're only, by what the camera is saying,
414
00:14:48,300 --> 00:14:50,720
it's saying that we're only overexposing this shot
415
00:14:50,720 --> 00:14:51,720
by one click.
416
00:14:51,860 --> 00:14:52,820
Now, why is that?
417
00:14:53,180 --> 00:14:55,560
Whereas when we took her out, it was
418
00:14:55,560 --> 00:14:58,280
actually, it thought it was a correct exposure,
419
00:14:58,640 --> 00:14:59,600
but what did we say?
420
00:14:59,660 --> 00:15:02,060
If something is dark, you lean towards the
421
00:15:02,060 --> 00:15:04,320
dark and you underexpose.
422
00:15:04,740 --> 00:15:07,200
So we lean towards the minus, but now
423
00:15:07,200 --> 00:15:10,660
we're looking at what the camera thinks is
424
00:15:10,660 --> 00:15:14,200
actually a correct exposure, or about one third
425
00:15:14,200 --> 00:15:14,740
stop out.
426
00:15:14,900 --> 00:15:17,520
It's because we've introduced skin tone, we've introduced
427
00:15:17,520 --> 00:15:18,100
white.
428
00:15:18,580 --> 00:15:20,700
So you could confidently say that if you
429
00:15:20,700 --> 00:15:23,700
were photographing subject matter like this, and you
430
00:15:23,700 --> 00:15:25,400
had some black, you had some white, and
431
00:15:25,400 --> 00:15:27,000
you had some skin tone, it's close to
432
00:15:27,000 --> 00:15:27,420
mid gray.
433
00:15:28,740 --> 00:15:30,700
And that's why aperture priority in this case
434
00:15:30,700 --> 00:15:31,600
would work.
435
00:15:32,220 --> 00:15:34,740
But watch what happens now when we change
436
00:15:34,740 --> 00:15:36,140
to the different metering modes.
437
00:15:36,560 --> 00:15:37,440
So let's do this.
438
00:15:37,500 --> 00:15:38,880
We're gonna go into our camera settings.
439
00:15:39,940 --> 00:15:41,640
And right now, as you can see, we're
440
00:15:41,640 --> 00:15:43,320
on matrix metering, which is evaluative.
441
00:15:44,280 --> 00:15:45,360
Now there's center weighted.
442
00:15:46,460 --> 00:15:49,200
I discourage center weighted metering because basically it's
443
00:15:49,200 --> 00:15:52,340
gonna evaluate the entire scene, but then focus
444
00:15:52,340 --> 00:15:54,940
on what's in front of us in the
445
00:15:54,940 --> 00:15:56,480
middle of the frame, as in it's weighted,
446
00:15:56,600 --> 00:15:57,820
it's biased to the center.
447
00:15:58,200 --> 00:15:59,780
If it's biased to the center, if you
448
00:15:59,780 --> 00:16:01,120
add that white dress and add that skin
449
00:16:01,120 --> 00:16:03,060
tone, it's going to be brighter than mid
450
00:16:03,060 --> 00:16:03,260
gray.
451
00:16:03,380 --> 00:16:05,160
The camera's gonna make it mid gray, therefore
452
00:16:05,160 --> 00:16:06,180
underexpose this.
453
00:16:06,620 --> 00:16:07,900
So center weighted is not a good one
454
00:16:07,900 --> 00:16:08,220
at all.
455
00:16:08,220 --> 00:16:10,240
Now some people like the idea of spot
456
00:16:10,240 --> 00:16:12,180
metering, but this is what's gonna happen.
457
00:16:12,320 --> 00:16:16,120
If we spot meter, and let's go to
458
00:16:16,120 --> 00:16:18,620
aperture priority now, and let's see what happens.
459
00:16:21,920 --> 00:16:24,160
Okay, so you see what happens that if
460
00:16:24,160 --> 00:16:28,440
we go down to her chest, now what's
461
00:16:28,440 --> 00:16:28,720
happening?
462
00:16:28,860 --> 00:16:30,380
It's exactly what happened before.
463
00:16:30,600 --> 00:16:32,700
When we had the white piece of card,
464
00:16:33,340 --> 00:16:35,500
it was all white and the camera says,
465
00:16:35,620 --> 00:16:36,940
I don't like white, I wanna make it
466
00:16:36,940 --> 00:16:37,340
mid gray.
467
00:16:37,480 --> 00:16:39,220
So if you spot for a white dress
468
00:16:39,800 --> 00:16:41,700
and you just leave it at that, and
469
00:16:41,700 --> 00:16:43,740
you do an exposure lock, you're gonna underexpose.
470
00:16:44,700 --> 00:16:47,980
Now, if we know that shooting something white,
471
00:16:48,100 --> 00:16:50,660
we have to overexpose by about five to
472
00:16:50,660 --> 00:16:54,120
six clicks, almost two stops, then we know
473
00:16:54,120 --> 00:16:55,660
that we could spot for the dress.
474
00:16:56,560 --> 00:16:59,060
So now I'm gonna emulate this exact exposure
475
00:16:59,060 --> 00:17:02,760
with manual 2500 speed, 2.8 400.
476
00:17:09,230 --> 00:17:13,250
Okay, so this is exactly like what our
477
00:17:13,250 --> 00:17:14,030
spot meter did.
478
00:17:14,750 --> 00:17:16,170
And like I said, it's a problem.
479
00:17:16,270 --> 00:17:17,430
Let's see if our theory works.
480
00:17:17,910 --> 00:17:19,690
So what we need to do now is
481
00:17:19,690 --> 00:17:22,109
because we have some latitude in our speed,
482
00:17:22,369 --> 00:17:26,050
I'm gonna lean towards the plus sign, five
483
00:17:26,050 --> 00:17:26,670
to six clicks.
484
00:17:26,869 --> 00:17:27,470
Let's do it.
485
00:17:28,530 --> 00:17:32,110
One, two, three, four, five.
486
00:17:32,890 --> 00:17:33,790
I wanna stay there.
487
00:17:33,850 --> 00:17:35,070
So it's one and two thirds.
488
00:17:35,250 --> 00:17:36,350
So it's five clicks.
489
00:17:36,830 --> 00:17:37,610
And guess what?
490
00:17:37,790 --> 00:17:38,650
We've got a great exposure.
491
00:17:39,230 --> 00:17:40,990
It basically means that you could spot for
492
00:17:40,990 --> 00:17:43,250
a white dress, the highlight on the white
493
00:17:43,250 --> 00:17:45,230
dress, and then you know you're gonna be
494
00:17:45,230 --> 00:17:47,730
one and two thirds stops to the plus.
495
00:17:48,210 --> 00:17:48,630
Great.
496
00:17:49,010 --> 00:17:51,950
Now let's see what happens if we actually
497
00:17:51,950 --> 00:17:54,790
spot for the black in the environment.
498
00:17:59,340 --> 00:18:00,420
Look what just happened.
499
00:18:01,040 --> 00:18:02,760
The whole frame changed.
500
00:18:02,860 --> 00:18:04,480
You can see it's actually changing with everything
501
00:18:04,480 --> 00:18:05,000
that I'm doing.
502
00:18:06,500 --> 00:18:07,660
Guess what happened again?
503
00:18:08,280 --> 00:18:10,000
We see the camera sees black.
504
00:18:10,120 --> 00:18:11,980
It's actually gonna meter for that spot where
505
00:18:11,980 --> 00:18:14,360
my focus point is, and it sees something
506
00:18:14,360 --> 00:18:14,640
black.
507
00:18:14,740 --> 00:18:16,180
It's gonna make it be gray, which it
508
00:18:16,180 --> 00:18:16,640
has.
509
00:18:17,840 --> 00:18:19,920
And of course, all the dress, the skin
510
00:18:19,920 --> 00:18:21,320
tone blows out completely.
511
00:18:21,460 --> 00:18:21,960
That's terrible.
512
00:18:22,360 --> 00:18:23,200
So what do we wanna do?
513
00:18:23,480 --> 00:18:26,720
We are going to underexpose five clicks.
514
00:18:27,260 --> 00:18:28,460
Great, let's do that.
515
00:18:28,940 --> 00:18:30,920
We're exposing correctly, but what the camera is
516
00:18:30,920 --> 00:18:31,180
saying.
517
00:18:31,920 --> 00:18:32,760
So let's do this.
518
00:18:33,140 --> 00:18:34,980
Now, right now, let's emulate what we're doing
519
00:18:34,980 --> 00:18:35,700
in aperture priority.
520
00:18:35,800 --> 00:18:38,020
We're at 200, 2.8, 400.
521
00:18:43,840 --> 00:18:45,280
200, 2.8, 400.
522
00:18:45,500 --> 00:18:47,080
So what we're gonna do now is we
523
00:18:47,080 --> 00:18:49,540
are gonna move the shutter speed five clicks.
524
00:18:53,380 --> 00:18:54,380
And guess what?
525
00:18:54,560 --> 00:18:56,900
We arrived at the exact same destination.
526
00:19:00,160 --> 00:19:02,680
So let's now spot meter for the skin
527
00:19:02,680 --> 00:19:03,660
and let's see what happens.
528
00:19:04,080 --> 00:19:05,780
So right now, there's many places that I
529
00:19:05,780 --> 00:19:08,720
could choose, but she's a mannequin, obviously different
530
00:19:08,720 --> 00:19:10,820
properties than normal skin.
531
00:19:11,060 --> 00:19:12,520
But what I've done is I've chosen a
532
00:19:12,520 --> 00:19:14,340
highlight on her arm that's closest to the
533
00:19:14,340 --> 00:19:14,820
light source.
534
00:19:15,400 --> 00:19:18,140
So what we need to know from experience
535
00:19:18,140 --> 00:19:19,980
that I know that most of our skin
536
00:19:19,980 --> 00:19:22,400
tones are gonna be about two clicks, as
537
00:19:22,400 --> 00:19:25,980
in two thirds of a stop, brighter than
538
00:19:25,980 --> 00:19:26,480
mid gray.
539
00:19:27,080 --> 00:19:28,700
So what's gonna happen is the camera will
540
00:19:28,700 --> 00:19:30,500
see brighter than mid gray, go to mid
541
00:19:30,500 --> 00:19:32,720
gray as in underexposed, which is what you're
542
00:19:32,720 --> 00:19:35,420
seeing right now, which means usually you can
543
00:19:35,420 --> 00:19:38,360
actually overexpose by two thirds stops.
544
00:19:38,440 --> 00:19:41,080
Remember, we're not overexposing, we're exposing correctly, but
545
00:19:41,080 --> 00:19:42,900
only overexposing what the camera is saying.
546
00:19:43,260 --> 00:19:46,320
So I'm gonna emulate the exposure that the
547
00:19:46,320 --> 00:19:48,100
camera has given us on manual.
548
00:19:48,200 --> 00:19:50,320
So at the moment, it's aperture priority, 2000,
549
00:19:50,440 --> 00:19:51,580
2.8, 400 ISO.
550
00:19:52,120 --> 00:19:53,060
So let's do that.
551
00:19:54,280 --> 00:19:59,520
Let's go, 2000, 2.8, 400 ISO.
552
00:20:00,360 --> 00:20:02,820
And again, the camera thinks it's a good
553
00:20:02,820 --> 00:20:05,480
exposure because we've got the actual exposure meter
554
00:20:05,480 --> 00:20:07,660
right on zero, but we know we're actually
555
00:20:07,660 --> 00:20:09,680
looking at a bad exposure.
556
00:20:09,860 --> 00:20:11,300
So what I'm gonna do now using my
557
00:20:11,300 --> 00:20:13,700
shutter speed is gonna go a couple of
558
00:20:13,700 --> 00:20:14,140
clicks.
559
00:20:15,300 --> 00:20:19,200
In this case, I'm thinking three, and there
560
00:20:19,200 --> 00:20:20,480
we've got a good exposure.
561
00:20:20,760 --> 00:20:22,060
We're one stop different.
562
00:20:22,060 --> 00:20:25,080
So again, depending on different skin types, whether
563
00:20:25,080 --> 00:20:28,860
it's Caucasian skin, African-American, tan skin, it's
564
00:20:28,860 --> 00:20:30,020
gonna be different all the time.
565
00:20:30,360 --> 00:20:31,840
And the thing is, depending on where you
566
00:20:31,840 --> 00:20:34,340
put your spot meter, again, it'll change.
567
00:20:34,460 --> 00:20:36,680
We've just worked out how we can spot
568
00:20:36,680 --> 00:20:37,400
meter for a dress.
569
00:20:37,860 --> 00:20:39,800
We've learned how we can spot for a
570
00:20:39,800 --> 00:20:41,480
dark suit, let's say to emulate a dark
571
00:20:41,480 --> 00:20:41,740
suit.
572
00:20:41,940 --> 00:20:45,020
And now we're emulating arguably spot metering for
573
00:20:45,020 --> 00:20:47,360
the skin, but there is no standard per
574
00:20:47,360 --> 00:20:47,540
se.
575
00:20:47,780 --> 00:20:49,360
There is this white is white, black is
576
00:20:49,360 --> 00:20:51,160
black, but skin tones will vary.
577
00:20:51,680 --> 00:20:54,100
So again, just let's go to aperture priority.
578
00:20:54,200 --> 00:20:56,100
And once again, look at those differences there.
579
00:20:57,980 --> 00:21:03,810
And we go from white, skin tone, black.
580
00:21:04,390 --> 00:21:05,890
In other words, you can get to those
581
00:21:05,890 --> 00:21:08,150
destinations in any which way you want.
582
00:21:08,490 --> 00:21:10,810
If you spot meter for the eye, well,
583
00:21:10,850 --> 00:21:11,950
of course, now you've got a bit of
584
00:21:11,950 --> 00:21:12,670
dark in there.
585
00:21:12,810 --> 00:21:14,410
So you see how it's gone darker.
586
00:21:14,650 --> 00:21:17,870
If you actually expose for shadows, then that's
587
00:21:17,870 --> 00:21:19,310
gonna be a problem too, because now you're
588
00:21:19,310 --> 00:21:20,650
blowing everything out even more.
589
00:21:21,090 --> 00:21:22,910
So you just have to pick a system
590
00:21:22,910 --> 00:21:24,370
that you like and stick to it.
591
00:21:24,510 --> 00:21:27,130
As far as I'm concerned, I like to
592
00:21:27,130 --> 00:21:30,210
shoot on manual and I'm emulating what aperture
593
00:21:30,210 --> 00:21:31,050
priority does.
594
00:21:31,470 --> 00:21:32,270
So let me explain.
595
00:21:32,810 --> 00:21:35,030
So if I go to manual, independent of
596
00:21:35,030 --> 00:21:36,690
our conversation that we've had up to this
597
00:21:36,690 --> 00:21:39,090
point, if I go to manual and then
598
00:21:39,090 --> 00:21:41,730
I look at my screen here, let's ignore
599
00:21:41,730 --> 00:21:43,430
the fact that in mirrorless what you see
600
00:21:43,430 --> 00:21:44,110
is what you get.
601
00:21:44,390 --> 00:21:46,970
But if I'm shooting on manual, then I
602
00:21:46,970 --> 00:21:48,310
might start at this point.
603
00:21:49,170 --> 00:21:51,570
Okay, so let's say for example, if you're
604
00:21:51,570 --> 00:21:53,670
not shooting in mirrorless and you're looking at
605
00:21:53,670 --> 00:21:56,850
your subject matter and you are using aperture
606
00:21:56,850 --> 00:22:00,710
priority, let's in fact go to matrix metering.
607
00:22:01,070 --> 00:22:03,930
So we're back on matrix evaluative metering mode.
608
00:22:04,250 --> 00:22:05,930
And I wanna talk about now if we
609
00:22:05,930 --> 00:22:07,430
don't have any of the extremes.
610
00:22:07,950 --> 00:22:10,490
So in this case, we have Sally, she's
611
00:22:10,490 --> 00:22:12,630
wearing a white dress, we've got the black
612
00:22:12,630 --> 00:22:13,110
background.
613
00:22:13,510 --> 00:22:15,770
And at the moment I'm shooting aperture priority
614
00:22:15,770 --> 00:22:19,330
and on matrix mode, metering mode, it's a
615
00:22:19,330 --> 00:22:20,750
pretty decent exposure.
616
00:22:21,670 --> 00:22:23,610
Although of course, we've got to take everything
617
00:22:23,610 --> 00:22:24,090
into account.
618
00:22:24,210 --> 00:22:26,870
Now watch what happens when I have more
619
00:22:26,870 --> 00:22:28,250
negative space with black.
620
00:22:28,830 --> 00:22:29,990
Not gonna move anything here.
621
00:22:30,850 --> 00:22:32,710
Watch what happens to the exposure.
622
00:22:33,710 --> 00:22:35,570
See, now that the camera is seeing more
623
00:22:35,570 --> 00:22:37,310
black, it's freaking out and saying, well, I
624
00:22:37,310 --> 00:22:39,030
don't like black, I actually wanna go mid
625
00:22:39,030 --> 00:22:41,490
gray and it's making what was once black
626
00:22:41,490 --> 00:22:42,630
mid gray.
627
00:22:42,850 --> 00:22:44,850
And of course it's overexposing her skin tone
628
00:22:44,850 --> 00:22:46,470
and overexposing the white dress.
629
00:22:46,810 --> 00:22:47,770
That's a problem.
630
00:22:48,250 --> 00:22:50,170
So we have to know that the minute
631
00:22:50,170 --> 00:22:53,410
you actually introduce anything other than white and
632
00:22:53,410 --> 00:22:55,230
black, you have to compensate accordingly.
633
00:22:56,030 --> 00:22:58,670
So let's see now, let's emulate it.
634
00:22:58,850 --> 00:23:01,350
400 speed, 2.8, 400 ISO.
635
00:23:01,770 --> 00:23:04,350
I'm gonna flick to manual and do the
636
00:23:04,350 --> 00:23:05,510
exact same thing.
637
00:23:07,570 --> 00:23:10,230
400th of a second, 2.8, 400 ISO.
638
00:23:11,410 --> 00:23:15,170
And now what we'll do, let's lean towards
639
00:23:15,170 --> 00:23:15,990
the minus.
640
00:23:16,150 --> 00:23:16,830
What did we say?
641
00:23:16,930 --> 00:23:20,090
If something is dark, you go dark, lean
642
00:23:20,090 --> 00:23:20,850
towards the minus.
643
00:23:21,130 --> 00:23:23,190
In this case, we've got more dark than
644
00:23:23,190 --> 00:23:23,750
anything else.
645
00:23:23,970 --> 00:23:25,690
I like to emulate what I see in
646
00:23:25,690 --> 00:23:27,690
front of me like a paint palette, like
647
00:23:27,690 --> 00:23:28,710
putting it in a paint bucket.
648
00:23:28,870 --> 00:23:31,650
Right now we have, in fact, let's do
649
00:23:31,650 --> 00:23:32,050
this.
650
00:23:33,030 --> 00:23:35,350
I'm gonna go now to the picture control
651
00:23:35,350 --> 00:23:37,350
to monochrome.
652
00:23:37,510 --> 00:23:39,150
So we sort of void ourselves of any
653
00:23:39,150 --> 00:23:40,090
sort of color bias.
654
00:23:40,990 --> 00:23:42,010
Yes, there's not much color.
655
00:23:42,010 --> 00:23:43,450
The only color that they really have is
656
00:23:43,450 --> 00:23:45,810
her sort of red lips and then the
657
00:23:45,810 --> 00:23:46,250
skin tone.
658
00:23:46,330 --> 00:23:47,650
And of course, you've got the black background
659
00:23:47,650 --> 00:23:48,310
and the white dress.
660
00:23:48,650 --> 00:23:50,870
Now that I've made it black, picture what
661
00:23:50,870 --> 00:23:53,310
you're seeing in this particular viewfinder now as
662
00:23:53,310 --> 00:23:53,870
a paint bucket.
663
00:23:53,990 --> 00:23:55,390
That's all it is, it's a paint bucket.
664
00:23:56,250 --> 00:23:59,050
And we mix those tones in and what
665
00:23:59,050 --> 00:23:59,670
do we get?
666
00:23:59,810 --> 00:24:01,950
Well, we're actually gonna get quite dark.
667
00:24:02,030 --> 00:24:04,090
It's gonna be a dark gray because we
668
00:24:04,090 --> 00:24:05,310
only have a little bit of white, a
669
00:24:05,310 --> 00:24:07,090
little bit of skin tone and mostly black.
670
00:24:07,550 --> 00:24:09,790
If we get a dark gray, the camera's
671
00:24:09,790 --> 00:24:11,650
gonna make it a mid gray, make it
672
00:24:11,650 --> 00:24:13,710
light and overexpose as we're seeing now.
673
00:24:14,130 --> 00:24:16,090
So what we have to do is of
674
00:24:16,090 --> 00:24:19,710
our exposure triangle, use one, two or three
675
00:24:19,710 --> 00:24:22,410
of the things that affect exposure, aperture, ISO
676
00:24:22,410 --> 00:24:26,670
or shutter speed, and then bring ourselves underexposed
677
00:24:26,670 --> 00:24:27,770
by what the camera is saying.
678
00:24:27,830 --> 00:24:30,030
In this case, I am gonna use the
679
00:24:30,030 --> 00:24:30,550
shutter speed.
680
00:24:30,890 --> 00:24:32,250
So let me see how many clicks it
681
00:24:32,250 --> 00:24:32,570
takes.
682
00:24:35,830 --> 00:24:37,690
One, two, three.
683
00:24:38,890 --> 00:24:40,110
So there we have it.
684
00:24:40,110 --> 00:24:42,370
We've got detail in the whites, we've got
685
00:24:42,370 --> 00:24:43,810
detail in the skin tones.
686
00:24:44,330 --> 00:24:46,110
The blacks are looking pretty good.
687
00:24:46,210 --> 00:24:48,310
Maybe we go one more, maybe four.
688
00:24:48,430 --> 00:24:48,990
There we go.
689
00:24:50,450 --> 00:24:51,610
And it depends on the monitor that you're
690
00:24:51,610 --> 00:24:53,410
actually watching this tutorial on right now, but
691
00:24:53,410 --> 00:24:54,510
we're about four clicks.
692
00:24:54,650 --> 00:24:56,230
In other words, if you have subject matter
693
00:24:56,230 --> 00:25:00,230
that occupies about a bit less than third
694
00:25:00,230 --> 00:25:01,810
of a frame, not quite a quarter, but
695
00:25:01,810 --> 00:25:03,810
a third of the frame with mostly black,
696
00:25:03,890 --> 00:25:05,990
then you know, you're gonna be about three
697
00:25:05,990 --> 00:25:07,690
or four clicks to the under.
698
00:25:08,690 --> 00:25:11,010
So we've looked at a white subject matter,
699
00:25:11,130 --> 00:25:12,970
we've looked at dark subject matter, but what
700
00:25:12,970 --> 00:25:14,470
happens if you have something in between?
701
00:25:14,670 --> 00:25:16,790
And of course, we're not looking at black
702
00:25:16,790 --> 00:25:18,590
or white, we're looking at different colors in
703
00:25:18,590 --> 00:25:19,250
normal environment.
704
00:25:19,390 --> 00:25:22,090
You have skin tones, you have different color
705
00:25:22,090 --> 00:25:23,550
dresses and things like that.
706
00:25:23,670 --> 00:25:25,490
So right now, what I'm trying to do
707
00:25:25,490 --> 00:25:28,470
is emulate a scene that is quite typical.
708
00:25:28,730 --> 00:25:31,170
Now we have a brown part of the
709
00:25:31,170 --> 00:25:33,390
RV parking garage, we've got a gray background,
710
00:25:33,490 --> 00:25:34,330
that's a Muslim background.
711
00:25:34,750 --> 00:25:36,510
We've got the right white dress, we've got
712
00:25:36,510 --> 00:25:37,110
skin tone.
713
00:25:37,110 --> 00:25:39,450
We're back in normal color and we're actually
714
00:25:39,450 --> 00:25:42,350
back on aperture priority and we're on matrix
715
00:25:42,350 --> 00:25:44,370
metering mode or evaluative metering mode.
716
00:25:44,950 --> 00:25:46,630
So if I'm looking at this right now,
717
00:25:46,770 --> 00:25:50,570
I'm actually, if I'm shooting aperture priority, then
718
00:25:50,570 --> 00:25:52,970
it's, in other words, using the camera meter
719
00:25:52,970 --> 00:25:54,430
to give me what it believes to be
720
00:25:54,430 --> 00:25:57,090
a correct exposure, it's actually overexposing it.
721
00:25:57,510 --> 00:25:58,350
Well, why is that?
722
00:25:58,570 --> 00:26:01,150
Well, if you look at all those tones,
723
00:26:01,310 --> 00:26:02,850
we have to first convert them to black
724
00:26:02,850 --> 00:26:05,490
and white for me to explain what I'm
725
00:26:05,490 --> 00:26:06,070
talking about.
726
00:26:06,070 --> 00:26:09,510
We're no longer looking at, let's say a
727
00:26:09,510 --> 00:26:11,890
skin tone or a brown piece of wall
728
00:26:11,890 --> 00:26:12,770
or anything like that.
729
00:26:12,850 --> 00:26:14,350
Now we're just looking at shades of black
730
00:26:14,350 --> 00:26:14,770
to white.
731
00:26:15,330 --> 00:26:17,050
Now you would say that this is close
732
00:26:17,050 --> 00:26:19,270
to correct exposure because you do have whites,
733
00:26:19,390 --> 00:26:20,950
you do have dark grays and things like
734
00:26:20,950 --> 00:26:21,130
that.
735
00:26:21,170 --> 00:26:22,730
But if you were to mix all those
736
00:26:22,730 --> 00:26:24,950
tones in as we're doing right now, you
737
00:26:24,950 --> 00:26:27,290
would arguably say that that scene is darker
738
00:26:27,290 --> 00:26:28,050
than mid gray.
739
00:26:28,570 --> 00:26:32,270
Therefore, the camera is deliberately overexposing it, but
740
00:26:32,270 --> 00:26:34,570
it actually thinks it's a correct exposure because
741
00:26:34,570 --> 00:26:35,770
as we said, it has to have a
742
00:26:35,770 --> 00:26:36,090
standard.
743
00:26:36,550 --> 00:26:38,130
So what I'm gonna do now is I'm
744
00:26:38,130 --> 00:26:41,050
gonna emulate this exposure in manual mode.
745
00:26:41,090 --> 00:26:43,170
So 500th of a second, 2.8, 400,
746
00:26:47,830 --> 00:26:49,810
500th of a second, 2.8 at 400.
747
00:26:50,310 --> 00:26:52,890
And I believe it's a little bit bright.
748
00:26:53,130 --> 00:26:54,950
So I'm gonna get my shutter speed or
749
00:26:54,950 --> 00:26:55,570
my ISO.
750
00:26:55,810 --> 00:26:57,090
In this case, I might get my ISO
751
00:26:57,090 --> 00:26:57,770
down actually.
752
00:26:59,130 --> 00:27:02,010
And I believe that is a good exposure.
753
00:27:02,210 --> 00:27:04,850
We've got beautiful detail in the skin.
754
00:27:05,290 --> 00:27:09,110
We've got detail in the dress and that
755
00:27:09,110 --> 00:27:10,070
gives us a good exposure.
756
00:27:10,690 --> 00:27:13,310
So remember, you've got the polarizing white and
757
00:27:13,310 --> 00:27:15,350
black and we know that's about five clicks,
758
00:27:15,430 --> 00:27:18,210
almost two stops under and over respectively.
759
00:27:18,770 --> 00:27:21,210
And in this case, we're about two thirds
760
00:27:21,210 --> 00:27:23,330
of a stop out of the exposure by
761
00:27:23,330 --> 00:27:24,230
what the camera is saying.
762
00:27:24,670 --> 00:27:26,590
So remember what your job now is to
763
00:27:26,590 --> 00:27:29,090
do is to look at your subject matter,
764
00:27:29,230 --> 00:27:31,610
not in terms of color, but of tones
765
00:27:31,610 --> 00:27:32,510
of black to white.
766
00:27:32,910 --> 00:27:35,090
And if you're using your spot metering mode
767
00:27:35,090 --> 00:27:37,190
as we discussed and let's do that in
768
00:27:37,190 --> 00:27:39,330
fact, while I'm speaking about that right now,
769
00:27:39,450 --> 00:27:42,490
let's go to spot metering mode.
770
00:27:44,450 --> 00:27:47,110
And you'll see that as I move my
771
00:27:47,110 --> 00:27:51,390
spot in different places, let's go to aperture
772
00:27:51,390 --> 00:27:57,150
priority, you'll see how it'll affect the exposure.
773
00:27:59,530 --> 00:28:01,890
If you actually even grab your smart device
774
00:28:01,890 --> 00:28:04,410
out, your phone, you'll actually see that no
775
00:28:04,410 --> 00:28:06,130
matter where you are with your phone and
776
00:28:06,130 --> 00:28:07,790
you look at your subject matter, you can
777
00:28:07,790 --> 00:28:09,530
tap on that particular part of it and
778
00:28:09,530 --> 00:28:11,230
it would give you again, a mid gray
779
00:28:11,230 --> 00:28:11,970
sort of reading.
780
00:28:12,690 --> 00:28:14,610
You have to know that the camera can't
781
00:28:14,610 --> 00:28:16,070
think like a human so you have to
782
00:28:16,070 --> 00:28:19,690
over or underexpose accordingly or compensate accordingly to
783
00:28:19,690 --> 00:28:20,670
get your correct exposure.
784
00:28:21,190 --> 00:28:23,110
So when you're in an environment like this,
785
00:28:23,270 --> 00:28:26,010
if you don't have mirrorless, of course, mirrorless
786
00:28:26,010 --> 00:28:27,250
is easy because what you see is what
787
00:28:27,250 --> 00:28:27,510
you get.
788
00:28:27,570 --> 00:28:29,090
I can clearly see that's a bad exposure
789
00:28:29,610 --> 00:28:31,230
that you actually have to look at your
790
00:28:31,230 --> 00:28:33,650
scene and if you were to go on
791
00:28:33,650 --> 00:28:36,190
to manual and if you were to actually
792
00:28:36,190 --> 00:28:42,730
go to matrix metering again, okay, so let's
793
00:28:42,730 --> 00:28:45,290
say we're right there, we're focusing on the
794
00:28:45,290 --> 00:28:49,190
eye and we've already determined that that being
795
00:28:49,190 --> 00:28:49,910
a correct exposure.
796
00:28:50,310 --> 00:28:52,310
I'm saying is you have to diagnose that
797
00:28:52,310 --> 00:28:55,310
scene, put those tones in all involved and
798
00:28:55,310 --> 00:28:57,730
then compensate accordingly based upon what you're seeing.
799
00:28:58,210 --> 00:29:00,510
Once we know that, then you're always gonna
800
00:29:00,510 --> 00:29:02,130
be within a pocket of a third stop
801
00:29:02,130 --> 00:29:02,490
increment.
802
00:29:02,950 --> 00:29:04,570
And if you take a shot and have
803
00:29:04,570 --> 00:29:05,670
to look at the back of the camera,
804
00:29:06,390 --> 00:29:08,470
great, you're looking for detail in the highlights,
805
00:29:08,650 --> 00:29:10,410
detail on the skin tones, detail on the
806
00:29:10,410 --> 00:29:12,630
whites, I let that be my guide.
807
00:29:12,950 --> 00:29:18,470
I'm not looking for detailing shadows to determine
808
00:29:18,470 --> 00:29:20,390
my exposure because if I have a deep
809
00:29:20,390 --> 00:29:23,250
dark shadow and a strong piece of sunlight
810
00:29:23,250 --> 00:29:25,850
hitting that bride's face, for example, and I'm
811
00:29:25,850 --> 00:29:27,750
after detail in the shadow, of course, the
812
00:29:27,750 --> 00:29:29,550
actual skin tone is gonna be white, I'm
813
00:29:29,550 --> 00:29:30,710
gonna have no detail whatsoever.
814
00:29:31,160 --> 00:29:34,550
So I let the highlights on the skin,
815
00:29:34,670 --> 00:29:36,610
I let the highlight on the dress, if
816
00:29:36,610 --> 00:29:38,410
we're talking about weddings or white dress usually,
817
00:29:38,910 --> 00:29:41,150
that's gonna be my guide and the rest
818
00:29:41,150 --> 00:29:42,590
usually takes care of itself.
819
00:29:43,610 --> 00:29:45,070
Let's talk about white balance.
820
00:29:45,530 --> 00:29:47,550
Now, yes, if you're shooting in raw, you
821
00:29:47,550 --> 00:29:50,410
can actually fix up anything afterwards in raw
822
00:29:50,410 --> 00:29:51,490
conversion, no problem.
823
00:29:52,010 --> 00:29:53,550
And you might just say it's easy to
824
00:29:53,550 --> 00:29:55,590
put it on auto white balance and that's
825
00:29:55,590 --> 00:29:56,170
basically it.
826
00:29:56,210 --> 00:29:58,590
The problem is that when there is a
827
00:29:58,590 --> 00:30:01,150
problem, when you have got the wrong color
828
00:30:01,150 --> 00:30:03,850
temperature in a photograph, then you're gonna have
829
00:30:03,850 --> 00:30:06,550
to change almost every single shot because let's
830
00:30:06,550 --> 00:30:08,410
say for example, I'm photographing a scene like
831
00:30:08,410 --> 00:30:10,750
this and I'm cropping up close and then
832
00:30:10,750 --> 00:30:12,730
I'm shooting on auto white balance and then
833
00:30:12,730 --> 00:30:14,570
I widen my angle of view and start
834
00:30:14,570 --> 00:30:17,430
incorporating different elements into my frame, it will
835
00:30:17,430 --> 00:30:18,410
change the white balance.
836
00:30:18,990 --> 00:30:21,590
So I would prefer you to actually choose
837
00:30:21,590 --> 00:30:24,590
a specific Kelvin degree, whether it's actually choosing
838
00:30:24,590 --> 00:30:28,070
your color temperature specifically or arguably a preset
839
00:30:28,070 --> 00:30:28,890
will be a lot easier.
840
00:30:29,230 --> 00:30:30,390
So you know the presets, right?
841
00:30:30,470 --> 00:30:32,330
So let's go to them right now, go
842
00:30:32,330 --> 00:30:33,110
to the white balances.
843
00:30:33,370 --> 00:30:35,710
Of course, you've got auto, you've got direct
844
00:30:35,710 --> 00:30:36,230
sunlight.
845
00:30:36,390 --> 00:30:38,590
Now direct sunlight is 5,000 Kelvin.
846
00:30:39,190 --> 00:30:41,030
Cloudy, you've got 5,700.
847
00:30:41,810 --> 00:30:43,950
Shade, you've got 7,250.
848
00:30:45,170 --> 00:30:47,090
Incandescent, 2,950.
849
00:30:47,730 --> 00:30:50,190
And fluorescent is 4,000 Kelvin degrees.
850
00:30:50,790 --> 00:30:53,550
And then flash, you've got 6,150 Kelvin
851
00:30:53,550 --> 00:30:53,930
degrees.
852
00:30:54,490 --> 00:30:56,310
And of course, you can actually choose the
853
00:30:56,310 --> 00:30:58,790
exact temperature that you basically want if you
854
00:30:58,790 --> 00:31:01,530
wish, or you can actually pick a particular
855
00:31:01,530 --> 00:31:02,010
preset.
856
00:31:02,570 --> 00:31:05,310
Now my suggestion is pick a preset because
857
00:31:05,310 --> 00:31:06,810
it'll be consistent.
858
00:31:07,010 --> 00:31:09,270
Let's say for example, if in one particular
859
00:31:09,270 --> 00:31:11,710
scene, you screw up the temperature, then in
860
00:31:11,710 --> 00:31:14,370
raw conversion, you can globally grab all those
861
00:31:14,370 --> 00:31:16,770
shots and fix them rather than have to
862
00:31:16,770 --> 00:31:19,510
go through three images here, four images there,
863
00:31:19,670 --> 00:31:22,190
that wide shot, that closeup shot, everything will
864
00:31:22,190 --> 00:31:23,130
have a different white balance.
865
00:31:23,450 --> 00:31:24,470
So keep it consistent.
866
00:31:24,470 --> 00:31:27,150
So what do the white balances do for
867
00:31:27,150 --> 00:31:27,510
that matter?
868
00:31:28,230 --> 00:31:30,990
And why should we look at it a
869
00:31:30,990 --> 00:31:31,330
bit closer?
870
00:31:31,470 --> 00:31:32,530
So let's look at it right now.
871
00:31:32,910 --> 00:31:34,430
So right now we're looking at Sally.
872
00:31:34,490 --> 00:31:36,050
Let's just get a good exposure here.
873
00:31:36,150 --> 00:31:38,570
So we're looking at an exposure of around
874
00:31:38,570 --> 00:31:42,130
400th of a second, 4.5, 640 ISO.
875
00:31:42,630 --> 00:31:45,650
It's superfluous based upon the actual conversation we're
876
00:31:45,650 --> 00:31:47,210
having right now, and that is white balance.
877
00:31:47,330 --> 00:31:49,390
So right now, as you can see, it's
878
00:31:49,390 --> 00:31:50,790
on daylight white balance.
879
00:31:50,930 --> 00:31:53,550
We're basically saying this is the sun or
880
00:31:53,550 --> 00:31:54,250
daylight.
881
00:31:54,930 --> 00:31:59,250
Okay, so let's now, we're direct sunlight.
882
00:31:59,390 --> 00:32:00,330
It's not direct sunlight.
883
00:32:00,510 --> 00:32:02,710
We're actually in the shade of a garage,
884
00:32:02,990 --> 00:32:05,130
but we're choosing daylight because it actually looks
885
00:32:05,130 --> 00:32:07,130
quite realistic and it looks okay.
886
00:32:07,670 --> 00:32:09,590
Watch what happens now that we return the
887
00:32:09,590 --> 00:32:11,350
white balance to cloudy.
888
00:32:11,850 --> 00:32:13,770
So if you want cloudy, it will simply
889
00:32:13,770 --> 00:32:15,010
go warmer.
890
00:32:15,810 --> 00:32:18,410
And if you look at the difference, it's
891
00:32:18,410 --> 00:32:19,630
quite huge.
892
00:32:19,690 --> 00:32:20,910
In fact, what we'll do is this.
893
00:32:20,910 --> 00:32:24,230
I'll go back, I'll take a shot.
894
00:32:26,460 --> 00:32:31,520
Then I will go cloudy, take another shot.
895
00:32:31,580 --> 00:32:32,740
That looks quite pleasing to the eye.
896
00:32:34,690 --> 00:32:38,570
Let's go shade, even warmer still.
897
00:32:39,930 --> 00:32:41,530
Now let's look at the differences here.
898
00:32:42,590 --> 00:32:46,370
So we've got, see now that you compare
899
00:32:46,370 --> 00:32:49,170
them, now you realize which one's gonna be
900
00:32:49,170 --> 00:32:49,390
better.
901
00:32:49,650 --> 00:32:52,010
In this case, we've got daylight.
902
00:32:52,550 --> 00:32:56,570
We've got cloudy and we've got shade.
903
00:32:57,310 --> 00:32:59,710
So it really depends on your personal preference.
904
00:32:59,830 --> 00:33:01,990
Now you're gonna be careful because some people
905
00:33:01,990 --> 00:33:03,630
who already have darker skin who have gone
906
00:33:03,630 --> 00:33:05,690
tanning or anything like that, they're gonna almost
907
00:33:05,690 --> 00:33:06,990
look like oompa loompas if you go too
908
00:33:06,990 --> 00:33:08,850
far with your white balance.
909
00:33:09,410 --> 00:33:11,610
So now how do we think of white
910
00:33:11,610 --> 00:33:11,870
balance?
911
00:33:12,050 --> 00:33:13,950
What makes us understand it?
912
00:33:14,010 --> 00:33:15,210
Well, let's think about this for a moment.
913
00:33:15,930 --> 00:33:18,650
If we're shooting in direct sunlight, we're basically
914
00:33:18,650 --> 00:33:20,750
saying we're using a warm light source.
915
00:33:20,750 --> 00:33:23,150
So the sun is a warm light source.
916
00:33:23,270 --> 00:33:23,790
It's warm.
917
00:33:23,930 --> 00:33:26,730
So we're basically saying, okay, sun, you've already
918
00:33:26,730 --> 00:33:27,670
got a warm tone.
919
00:33:27,830 --> 00:33:30,410
Then I think that this will be, what
920
00:33:30,410 --> 00:33:31,910
I see with my own two eyes, this
921
00:33:31,910 --> 00:33:32,850
will look realistic.
922
00:33:33,570 --> 00:33:34,010
Great.
923
00:33:34,630 --> 00:33:37,550
If we're shooting with a cloudy white balance,
924
00:33:37,630 --> 00:33:39,890
let's say for example here, we're in actually
925
00:33:39,890 --> 00:33:41,930
an open shade, but let's say where the
926
00:33:41,930 --> 00:33:43,750
clouds go above the sun and now we're
927
00:33:43,750 --> 00:33:46,950
shooting cloudy, the clouds are filtering that light.
928
00:33:47,030 --> 00:33:48,310
It's no longer as warm.
929
00:33:48,630 --> 00:33:49,770
It's a little bit colder.
930
00:33:49,770 --> 00:33:51,990
So what we're saying to the camera by
931
00:33:51,990 --> 00:33:54,290
choosing the cloudy white balance, I wanna warm
932
00:33:54,290 --> 00:33:55,170
this up a little bit.
933
00:33:55,710 --> 00:33:57,830
In this case, we're in the shade of
934
00:33:57,830 --> 00:33:59,830
an RV parking here.
935
00:33:59,890 --> 00:34:00,690
So the shade of a building.
936
00:34:01,110 --> 00:34:03,850
We're basically saying it's actually a cold, cold
937
00:34:03,850 --> 00:34:04,630
color temperature.
938
00:34:04,830 --> 00:34:06,530
So we wanna warm things up a little
939
00:34:06,530 --> 00:34:06,750
bit.
940
00:34:06,990 --> 00:34:09,929
And therefore we get this particular skin tone.
941
00:34:10,050 --> 00:34:11,949
Now I actually think somewhere in between is
942
00:34:11,949 --> 00:34:12,949
probably about right.
943
00:34:14,409 --> 00:34:16,670
And you can see the difference between, like
944
00:34:16,670 --> 00:34:19,290
I said, right now we're seeing direct sunlight
945
00:34:19,290 --> 00:34:20,010
white balance.
946
00:34:20,190 --> 00:34:23,489
We're actually seeing the cloudy and then now
947
00:34:23,489 --> 00:34:24,449
we're seeing shade.
948
00:34:24,889 --> 00:34:26,850
And of course, as we go further up
949
00:34:26,850 --> 00:34:28,590
in the food chain, so to speak, you
950
00:34:28,590 --> 00:34:31,850
are going to get polarizing color temperatures.
951
00:34:31,969 --> 00:34:33,110
So let's do that for example.
952
00:34:33,530 --> 00:34:35,469
Let's deliberately choose incandescent.
953
00:34:35,570 --> 00:34:37,409
What we're saying to the camera, or to
954
00:34:37,409 --> 00:34:40,110
the camera, we're saying we are shooting with,
955
00:34:40,230 --> 00:34:43,690
let's say, could be a man-made light
956
00:34:43,690 --> 00:34:46,230
globe, tungsten light globe, or candlelight.
957
00:34:46,850 --> 00:34:48,449
And you are gonna see that this is
958
00:34:48,449 --> 00:34:49,350
gonna be blue.
959
00:34:50,090 --> 00:34:50,889
Do you see what happens?
960
00:34:51,030 --> 00:34:53,750
Is that we're basically saying that if our
961
00:34:53,750 --> 00:34:56,190
subject matter was illuminated with a very yellow,
962
00:34:56,410 --> 00:34:58,470
warm light source, this would correct it.
963
00:34:58,670 --> 00:35:01,090
But we're using this in this environment and
964
00:35:01,090 --> 00:35:02,350
she looks dead.
965
00:35:03,050 --> 00:35:06,470
Now, if I was photographing guys and I
966
00:35:06,470 --> 00:35:08,650
deliberately wanted to make a shot look cool
967
00:35:08,650 --> 00:35:10,470
in two senses of that word, cool as
968
00:35:10,470 --> 00:35:13,030
in it's got a cool vibe, or cool
969
00:35:13,030 --> 00:35:15,090
as in cold, then that's a masculine look
970
00:35:15,090 --> 00:35:15,850
and that could work.
971
00:35:16,330 --> 00:35:18,290
So be careful on where you're using this,
972
00:35:18,390 --> 00:35:21,010
but you would use incandescent in exactly what
973
00:35:21,010 --> 00:35:23,410
it implies, with an incandescent light, man-made
974
00:35:23,410 --> 00:35:26,950
tungsten light globes, and possibly even candlelight.
975
00:35:27,050 --> 00:35:29,130
Now, candlelight's gonna be warmer, but so you
976
00:35:29,130 --> 00:35:31,230
have to just determine what color temperature you
977
00:35:31,230 --> 00:35:32,070
prefer yourself.
978
00:35:32,610 --> 00:35:34,370
Now, here's the thing, and if you don't
979
00:35:34,370 --> 00:35:36,850
like these color temperatures, you can simply change
980
00:35:36,850 --> 00:35:37,030
them.
981
00:35:38,410 --> 00:35:41,490
Let's see what happens when we go auto.
982
00:35:44,420 --> 00:35:46,400
Now, auto has actually done a pretty good
983
00:35:46,400 --> 00:35:46,800
job here.
984
00:35:46,920 --> 00:35:48,540
Now, you might say, well, fantastic, Jerry, I'll
985
00:35:48,540 --> 00:35:49,260
use it all the time.
986
00:35:49,660 --> 00:35:51,740
But don't forget, the minute we start introducing
987
00:35:51,740 --> 00:35:54,220
new elements in this particular frame, it will
988
00:35:54,220 --> 00:35:55,100
not be consistent.
989
00:35:55,300 --> 00:35:56,940
So just remember, although it might give you
990
00:35:56,940 --> 00:35:59,380
a pretty good result in most situations, it
991
00:35:59,380 --> 00:36:00,100
won't be consistent.
992
00:36:00,860 --> 00:36:02,660
So play around with your color temperatures.
993
00:36:02,780 --> 00:36:03,980
My advice to you is to go to
994
00:36:03,980 --> 00:36:05,980
your favorite RAW conversion software.
995
00:36:06,100 --> 00:36:07,520
Let's say, for example, you use Lightroom.
996
00:36:08,120 --> 00:36:10,600
And as you look at the photograph that
997
00:36:10,600 --> 00:36:13,040
you've taken as shot, you will know the
998
00:36:13,040 --> 00:36:14,780
actual preset white balance that you chose.
999
00:36:15,140 --> 00:36:16,780
And slide them left and right, and you'll
1000
00:36:16,780 --> 00:36:18,700
begin to realize that maybe all this time
1001
00:36:18,700 --> 00:36:20,840
you've been shooting with direct sunlight, and you
1002
00:36:20,840 --> 00:36:22,300
prefer cloudy or vice versa.
1003
00:36:22,620 --> 00:36:23,680
So have fun with it.
1004
00:36:24,060 --> 00:36:25,320
Don't overcomplicate it.
1005
00:36:25,700 --> 00:36:27,940
But just know too, that if you wanna
1006
00:36:27,940 --> 00:36:30,580
get perfect color, you might do a custom
1007
00:36:30,580 --> 00:36:31,140
white balance.
1008
00:36:31,520 --> 00:36:35,180
You may even photograph a color picker in
1009
00:36:35,180 --> 00:36:36,360
your particular frame.
1010
00:36:36,680 --> 00:36:38,300
But I only do that when it comes
1011
00:36:38,300 --> 00:36:41,340
to maybe shooting fashion, where it's so critical
1012
00:36:41,340 --> 00:36:43,620
to get that color absolutely perfect of the
1013
00:36:43,620 --> 00:36:46,040
dress, more imperfect, more actually important than even
1014
00:36:46,040 --> 00:36:46,660
skin tone.
1015
00:36:46,880 --> 00:36:48,040
So you can do that as well.
1016
00:36:48,520 --> 00:36:51,080
So take that, run with it, have some
1017
00:36:51,080 --> 00:36:51,960
fun with your presets.
1018
00:36:52,220 --> 00:36:53,580
But my advice to you is make your
1019
00:36:53,580 --> 00:36:55,640
life easier, get it right in camera as
1020
00:36:55,640 --> 00:36:57,600
close as possible, and be consistent.
1021
00:36:58,520 --> 00:37:00,560
Arguably the most important element in the exposure
1022
00:37:00,560 --> 00:37:02,020
triangle is aperture.
1023
00:37:02,600 --> 00:37:04,820
How much light we're letting through the iris
1024
00:37:04,820 --> 00:37:07,180
of the lens, and how many things we
1025
00:37:07,180 --> 00:37:07,740
want in focus.
1026
00:37:07,740 --> 00:37:08,960
We call that depth of field.
1027
00:37:09,660 --> 00:37:11,700
So what we're gonna do now is actually
1028
00:37:11,700 --> 00:37:14,240
gonna look into the camera and notice what
1029
00:37:14,240 --> 00:37:16,820
an f-stop will actually do in terms
1030
00:37:16,820 --> 00:37:17,680
of it being wider.
1031
00:37:17,940 --> 00:37:20,720
What does 1.8 look like all the
1032
00:37:20,720 --> 00:37:22,080
way till say f22.
1033
00:37:22,680 --> 00:37:25,180
Every lens will have different compression of course,
1034
00:37:25,340 --> 00:37:27,820
and actually behave differently with the same f
1035
00:37:27,820 --> 00:37:28,080
-number.
1036
00:37:28,280 --> 00:37:31,420
For example, f4 with a longer focal length,
1037
00:37:31,560 --> 00:37:33,600
there'll be actually less depth of field.
1038
00:37:33,740 --> 00:37:36,320
Let's say than a wider angle lens with
1039
00:37:36,320 --> 00:37:38,820
the same f-number, say f4 for example
1040
00:37:38,820 --> 00:37:39,340
in this case.
1041
00:37:39,660 --> 00:37:41,000
So what I wanna do now is look
1042
00:37:41,000 --> 00:37:41,520
through the camera.
1043
00:37:41,960 --> 00:37:43,260
Of course, as we can see here, we've
1044
00:37:43,260 --> 00:37:45,300
just got this plant in front of us
1045
00:37:45,300 --> 00:37:45,960
with different leaves.
1046
00:37:46,420 --> 00:37:49,240
And I've actually set the camera, dare I
1047
00:37:49,240 --> 00:37:51,900
say it here to auto ISO, but it's
1048
00:37:51,900 --> 00:37:53,460
giving us a nice exposure.
1049
00:37:53,960 --> 00:37:56,480
So I've focused on a particular leaf there
1050
00:37:56,480 --> 00:37:57,800
as you can see right there.
1051
00:37:58,520 --> 00:38:00,540
And what I'm going to do is I
1052
00:38:00,540 --> 00:38:03,560
am going to move the aperture from 1
1053
00:38:03,560 --> 00:38:06,640
.8, and I want you to start looking
1054
00:38:06,640 --> 00:38:09,140
at how many more things we have in
1055
00:38:09,140 --> 00:38:11,220
focus, foreground and background.
1056
00:38:13,960 --> 00:38:15,840
You can sort of see how we're getting
1057
00:38:15,840 --> 00:38:17,600
that less milkiness in the background.
1058
00:38:18,100 --> 00:38:20,200
In this case, we don't really have a
1059
00:38:20,200 --> 00:38:20,800
bokeh.
1060
00:38:20,940 --> 00:38:21,760
And I know that a lot of people
1061
00:38:21,760 --> 00:38:22,660
love that word bokeh.
1062
00:38:23,060 --> 00:38:25,600
With this particular lens, I've got the range
1063
00:38:25,600 --> 00:38:28,980
from f16 all the way down to 1
1064
00:38:28,980 --> 00:38:33,040
.8. Now it's important to note that many
1065
00:38:33,040 --> 00:38:35,500
people think that focus starts from where you
1066
00:38:35,500 --> 00:38:37,060
focus from and it goes backwards.
1067
00:38:37,220 --> 00:38:40,200
In other words, depth of fields, you may
1068
00:38:40,200 --> 00:38:42,360
believe that starts from that point of focus
1069
00:38:42,360 --> 00:38:43,380
and working backwards.
1070
00:38:44,080 --> 00:38:46,820
So for example, if you're photographing, say me
1071
00:38:46,820 --> 00:38:49,340
at a very shallow depth of field, let's
1072
00:38:49,340 --> 00:38:51,020
say it may be at 1.8 or
1073
00:38:51,020 --> 00:38:53,560
f2, if you focus on my eye socket
1074
00:38:53,560 --> 00:38:54,920
where the glass of the eye meets the
1075
00:38:54,920 --> 00:38:57,160
eye socket, and you feel that the actual
1076
00:38:57,160 --> 00:38:59,860
focus is about this deep and it goes
1077
00:38:59,860 --> 00:39:01,920
backwards, then you might miss my eyelash.
1078
00:39:02,470 --> 00:39:04,200
Now, yes, that may happen depending on what
1079
00:39:04,200 --> 00:39:06,940
lens you use, but this information is extremely
1080
00:39:06,940 --> 00:39:10,260
important, especially when you're photographing groups of people.
1081
00:39:11,020 --> 00:39:13,100
Let's say for example, this particular lens looking
1082
00:39:13,100 --> 00:39:14,700
at me right now, you're looking at a
1083
00:39:14,700 --> 00:39:17,520
bird's eye view of three layers of people
1084
00:39:17,520 --> 00:39:19,040
in a family group shot, okay?
1085
00:39:19,140 --> 00:39:20,500
So bird's eye view, these are the top
1086
00:39:20,500 --> 00:39:20,920
of the heads.
1087
00:39:21,600 --> 00:39:25,040
If you actually photograph at f4, at the
1088
00:39:25,040 --> 00:39:27,980
tip of that person's nose or eyes, and
1089
00:39:27,980 --> 00:39:29,740
then your depth of field, let's say for
1090
00:39:29,740 --> 00:39:33,400
example, is like this, then what happens is
1091
00:39:33,400 --> 00:39:34,560
we're missing focus.
1092
00:39:35,180 --> 00:39:36,480
So what you have to do first of
1093
00:39:36,480 --> 00:39:39,380
all, understand that focus starts 1 3rd in
1094
00:39:39,380 --> 00:39:40,560
and 2 3rds back.
1095
00:39:40,760 --> 00:39:43,060
So if you are photographing three people, for
1096
00:39:43,060 --> 00:39:45,680
example, you will not actually focus on the
1097
00:39:45,680 --> 00:39:47,500
tip of that first person's eye or nose.
1098
00:39:47,800 --> 00:39:49,600
You will actually focus on the tip of
1099
00:39:49,600 --> 00:39:51,980
that person's nose or eyes on that second
1100
00:39:51,980 --> 00:39:52,340
level.
1101
00:39:52,620 --> 00:39:54,700
And now we have 1 3rd in and
1102
00:39:54,700 --> 00:39:55,540
2 3rds back.
1103
00:39:55,700 --> 00:39:57,760
And of course you have to determine what
1104
00:39:57,760 --> 00:40:00,200
f-stop is going to be needed for
1105
00:40:00,200 --> 00:40:02,900
your subject matter and appropriate to the lens
1106
00:40:02,900 --> 00:40:04,200
choice that you basically have.
1107
00:40:04,620 --> 00:40:06,340
So the example that I did just now,
1108
00:40:06,440 --> 00:40:09,020
it's very elementary, it's very fundamental, but what
1109
00:40:09,020 --> 00:40:10,820
we're just trying to ascertain here is the
1110
00:40:10,820 --> 00:40:12,420
fact that if you are shooting at, let's
1111
00:40:12,420 --> 00:40:14,500
say an f-stop number at f1.2,
1112
00:40:14,560 --> 00:40:16,880
1.4, 1.8, you are gonna have
1113
00:40:16,880 --> 00:40:17,920
less things in focus.
1114
00:40:18,400 --> 00:40:20,180
And then as you get deeper in focus,
1115
00:40:20,300 --> 00:40:21,440
you are gonna get more.
1116
00:40:21,600 --> 00:40:24,440
In other words, f16, f22 is where you
1117
00:40:24,440 --> 00:40:25,400
get more things in focus.
1118
00:40:25,400 --> 00:40:28,560
You simply have to choose the actual appropriate
1119
00:40:28,560 --> 00:40:31,420
f-number or the f-stop based upon
1120
00:40:31,420 --> 00:40:32,840
the subject matter that you're photographing.
1121
00:40:33,000 --> 00:40:35,440
So don't overthink it, but also don't play
1122
00:40:35,440 --> 00:40:35,940
with fire.
1123
00:40:36,140 --> 00:40:38,940
Never photograph family photographs at 1.2 or
1124
00:40:38,940 --> 00:40:40,780
f2 or anything like that.
1125
00:40:41,040 --> 00:40:42,260
The way I like to think about it,
1126
00:40:42,380 --> 00:40:44,060
depending on the lens choice that you have,
1127
00:40:44,320 --> 00:40:46,980
if you photograph two people, then that might
1128
00:40:46,980 --> 00:40:48,620
give you permission to photograph at 2.8
1129
00:40:49,140 --> 00:40:51,520
because you've got the two people right there,
1130
00:40:51,940 --> 00:40:53,560
their eyes are on the same sort of
1131
00:40:53,560 --> 00:40:55,820
plane of focus, and then you can arguably
1132
00:40:55,820 --> 00:40:56,660
get them in focus.
1133
00:40:56,880 --> 00:40:59,000
If you're photographing four people, you might wanna
1134
00:40:59,000 --> 00:41:02,560
shoot with f4, five people, 5.6, eight
1135
00:41:02,560 --> 00:41:04,360
people, f8, and so on.
1136
00:41:04,660 --> 00:41:06,000
Now, yes, that's not an absolute.
1137
00:41:06,280 --> 00:41:08,400
And of course, we said before that if
1138
00:41:08,400 --> 00:41:11,140
you're photographing with a wider angle lens, that
1139
00:41:11,140 --> 00:41:13,540
same f-stop like f8, for example, on
1140
00:41:13,540 --> 00:41:15,240
a wider angle lens, your depth of field
1141
00:41:15,240 --> 00:41:17,420
might be like this, but with a longer
1142
00:41:17,420 --> 00:41:21,120
focal length lens, your depth of field might
1143
00:41:21,120 --> 00:41:21,640
be like this.
1144
00:41:21,700 --> 00:41:24,100
So just make sure you understand your lenses,
1145
00:41:24,100 --> 00:41:25,960
the genre that you're photographing.
1146
00:41:26,460 --> 00:41:27,620
Don't overthink it, guys.
1147
00:41:27,800 --> 00:41:29,160
Aperture is actually really easy.
1148
00:41:29,360 --> 00:41:31,060
Just determine how many things you want in
1149
00:41:31,060 --> 00:41:33,920
focus, know the limitations of your lens based
1150
00:41:33,920 --> 00:41:35,900
upon the genre that you're photographing, and have
1151
00:41:35,900 --> 00:41:36,240
some fun.
80849
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