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Understanding
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flash power is absolutely crucial to
our understanding of studio lighting.
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So to help us do that, I've recruited
our model stiffany.
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I also have an aperture and shutter
speed chart.
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We have a camera tethered into the
computer so that we can see the
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results.
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And you'll also notice that I've put a
cstan at the back here, which you'll
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understand what that's for.
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Shortly,
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before we start, let's get some simple
clarification
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about the power
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of lamp heads.
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So we're going to start our first tests
with this particular lamp head.
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And this one is an 800
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jewel power.
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This one
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is a 400 jewel power.
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So it sounds like it's a lot lot less
than this one.
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Well, actually the difference is half,
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400 jewels is half the power of 800
jewels.
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And in lighting terms,
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half the amount of light
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is one stop less.
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So by now you should be familiar with
apertures and f stops if you're at that
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level of using studio lighting,
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and we're going to look at that
relationship
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between f stops
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and studio light power to clearly
understand it.
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But first of all, let's simply look at
this.
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So for example, if the correct exposure
was at f eleven.
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If we had
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the correct exposure at f eleven with
an 800 jewel lamp head at full power,
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then on a 400 jewel lamp head, we would
need one stop brighter, because
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f eight is allowing twice the amount of
light in.
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And a 400 jewel is half the amount of
power of the 800 jaw head.
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So
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the relationship between one stop
changes either a 200 jaw head of 400
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jaw head, 800 jaw head, 1600 jaw head,
is exactly the same as the relationship
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between one full f stop jumps.
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Now we know that we can change our f
stops and our apertures in smaller
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jumps.
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We can change them in one third
increments, if necessary.
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We can actually change the power on our
flush heads in 110th of an f stop
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increments, if we require.
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So let's start exploring
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the change in power on the lamp heads
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and see what it means when we go from
full power to minimum power, and why
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having a good range of power is
important.
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Now to make sure that our test is
consistent,
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I'm going to make sure that the
modeling lamp is off.
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You can see at the moment, the modeling
lamp is on.
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Now if we leave the modeling lamp on
that is quite a lot of extra light
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hitting our model.
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Now that extra light can actually
affect the exposure of our flashshot,
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because it's additional light to the
flash.
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So I'm going to turn the modeling light
off so that the exposures that we're
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reading, and the results that we're
seeing are purely the flash only.
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So
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I'm starting on power 10.
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And that is the maximum power that I
can get out of this light.
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If, for example, power ten was f sixteen
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required on the camera,
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then if I drop to power nine, I would
require f eleven.
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If I dropped to power eight, I would
require f eight.
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If I dropped a power seven, I would
require f 5.6.
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Because each drop from ten to nine to
eight to seven to six, on a studio
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light, is a one full f stop jump.
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So we'd have to adjust the apertures
accordingly.
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00:04:18,91 --> 00:04:23,463
But I don't know yet exactly what
aperture setting we need four power ten
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at this particular distance.
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Because also keep in mind that the
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power
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of a light
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is also related to the distance from
the subject.
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So as we move a light closer to our
subject, the power of the light will be
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stronger.
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If we move the light further away, the
power of the light will decrease.
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Now, other factors also affect the
power of the light, and that is when we
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put different modifiers on.
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00:04:51,858 --> 00:04:55,962
So if we put a soft box on the light,
or an umbrella, or we bounce the light
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off of a different surface, then a lot
of that power will be dispersed into
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different directions, and it will
reduce the power.
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00:05:03,703 --> 00:05:07,73
So for this test, I'm just using a
standard l forty reflector,
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and
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that's it.
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And we'll direct the light
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straight at our model, and we'll see
what exposure settings we require.
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So first of all,
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coming into my camera,
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framing up and focusing on my model,
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I'm using a shutter speed a 160th of a
second, because that's the
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sink speed that will work with this.
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The shutter speed doesn't have any real
bearing on the exposure for flash.
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But i'll explain a bit more about that
later.
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First of all, we're going to set our
aperture.
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So I'm going to set my aperture to
start with, to f 22
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in this case.
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So my starting aperture is f
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22.
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My lamp is on power ten, which is full
power,
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full power on an 800 head.
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If I had power ten on this head, which
is a 400 jewel,
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that would be equivalent
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to power nine on this head,
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because this light is one stop less
powerful than that light.
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So back to power ten.
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No modeling lamp.
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Let's take our first shot.
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We're using the trigger on top of the
camera to trigger the flash gun,
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taking our first picture.
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And you can
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hear that large outburst of light.
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So that picture is now going to come
into
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the computer.
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And we can see the first result there,
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which looks a little bit over exposed.
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So that's at f
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22,
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an aperture of f 22.
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And there's the result.
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So I'm going to close the aperture down
to f 32,
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to one stop.
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Less light able to get into the camera,
which will reduce that
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exposure.
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So let me do that quickly.
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So changing the camera now, I'm just
changing it to f 32.
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Taking that picture again.
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Same power on the studio.
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Lamp.
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Let's look at the result on screen.
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So there we go.
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We now have the correct exposure
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on
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We can see the skin tone seems well.
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Exposed.
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Is just a single light setup.
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Obviously, as we demonstrate more
lighting, examples will be showing you
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lots of ways to light a model.
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This is the most simple single light
setup.
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Now
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what's important to notice, here is the
level of detail on this cross bar in
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the background.
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So remember, we're at f 32,
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and we have the correct exposure,
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and our depth of field is quite large,
because we can see the model is sharp.
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And this object in the background,
which is actually about three
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meters behind the model, is also
becoming quite sharp in the picture.
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And this is why it's important to have
a large
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range of power in your flesh unit, so
that you can control depth of field.
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So we're now gradually going to change
the exposure
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of the flash and the apertures on the
camera,
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reducing depth of field at the same
time.
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But before I do that, I'm going to
leave the aperture at f 32,
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and I'm going to change the power of
the light just by 110th
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of an f stop.
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So I'm going to take it from power x to
power 9.9.
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So from ten
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to 9.9,
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take the shot.
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Let's take a look at the result.
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And there we go.
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We can see the difference here's at
power 9.9
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and there's at power 199,
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power, 199,
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power ten.
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So that's only 110th of an f stop.
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And that's why that difference looks
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so subtle, because it is very subtle.
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110th of an fstop is a very small
amount as you can see there.
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So let's carry on in full f stop.
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So at this time, we're going to go from
power ten, where we were here.
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I'm going to go to power nine.
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So power nine.
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Now, when a light goes down in power,
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you do need to allow the light the time
to reset its power.
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Some flash units require you to
actually dump the power manually out of
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it.
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But an advanced flash unit like this
one doesn't.
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It will rebuild balance itself.
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So we've now dropped down from power
ten,
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from the exposure on screen now, to
power nine, which is one f stop less.
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Let's take that shot,
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and let's take a look at the result.
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That was power ten.
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That's power nine.
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So you can see this is one f stop less
of light.
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That one was power 99.
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There's our power ten shot.
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Now there's power nine.
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So you can see a whole f stop of light.
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Now a whole f stop of light
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is actually a reduction, is half the
amount of light.
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Remember, an f stop is either half the
amount of light or double the amount of light.
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So in light terms, we add the correct
exposure at f 32.
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We've dropped the power to power nine.
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And now our picture is underexposed.
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00:10:46,12 --> 00:10:50,350
So we now need to open the aperture by
the equivalent amount by one f.
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Stop to f 22 to bring our exposure back
correct again.
199
00:10:56,656 --> 00:10:57,123
So
200
00:10:57,557 --> 00:10:59,993
changing my aperture in my camera
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to f 22,
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from f 32,
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leaving it a power nine.
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And we'll now see that the exposure
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on this one we'll now be correct.
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00:11:12,172 --> 00:11:13,540
So we can now see, f 22,
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that this exposure is correct for power
nine.
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00:11:18,745 --> 00:11:25,318
And if we go back, we can see that that
was the exposure at f 32 at power 10.
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And you can see that they are very
close.
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Now any discrepancy in power where
there's a slight little bit of
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00:11:32,892 --> 00:11:35,395
difference is not actually down to the
light.
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00:11:35,862 --> 00:11:39,466
It certainly won't be down to these
lights, because they are very, very
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00:11:39,799 --> 00:11:41,234
high quality professional lights.
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00:11:41,634 --> 00:11:44,804
The discrepancy here will be in the
aperture in the camera.
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00:11:46,740 --> 00:11:50,110
So we're now at f 22, and we have the
correct exposure.
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00:11:50,910 --> 00:11:53,913
But what happens if we change the light
more dramatically?
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If I go, say, four f stops
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brighter in aperture
219
00:11:59,519 --> 00:12:00,153
1234,
220
00:12:03,690 --> 00:12:05,592
maybe five, maybe six,
221
00:12:06,359 --> 00:12:07,360
let's go four.
222
00:12:07,794 --> 00:12:09,729
So we're going to go 1234
223
00:12:11,631 --> 00:12:13,933
f stops brighter on the aperture.
224
00:12:14,267 --> 00:12:16,803
That will require us to turn the power
of the light
225
00:12:16,970 --> 00:12:21,775
down four f stops, because we're
letting more light in with that aperture.
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00:12:22,108 --> 00:12:24,310
So I'm going to change from f 224,
227
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f stops brighter to f 5.6.
228
00:12:30,183 --> 00:12:31,518
So f 22,
229
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open the aperture up to f 5.6,
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take the shot.
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00:12:36,890 --> 00:12:38,24
And it will now be dramatically
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overexposed,
233
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because it's going to be four stops
over exposed, as you can see here,
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because we doubled the light, we
doubled the light, we doubled the
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00:12:48,501 --> 00:12:49,636
light, and we doubled it again.
236
00:12:49,703 --> 00:12:51,705
And there's the result, a massively
overexposed
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shot.
238
00:12:53,540 --> 00:12:57,444
So we have to turn the light down by
four f stops to match.
239
00:12:58,578 --> 00:13:00,146
So from power nine
240
00:13:00,580 --> 00:13:02,82
to power 8765
241
00:13:05,552 --> 00:13:06,820
that's a four stop reduction
242
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in power.
243
00:13:09,456 --> 00:13:13,293
We let the light rebalance itself take
that shot.
244
00:13:16,96 --> 00:13:19,199
And now we should have the correct
exposure
245
00:13:21,534 --> 00:13:22,235
and voila.
246
00:13:22,736 --> 00:13:26,573
So now we have the correct exposure
because we reduce the power of the light
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to match the aperture setting.
248
00:13:29,609 --> 00:13:30,710
And if we go back
249
00:13:31,211 --> 00:13:34,547
and we look, we can see that our
exposure is correct.
250
00:13:34,914 --> 00:13:38,251
But what we'll notice is the difference
in depth of field.
251
00:13:38,752 --> 00:13:43,156
And this is why it's very important to
have a large power range on your flash
252
00:13:43,390 --> 00:13:47,961
unit, because it gives you this Greater
creative control over depth of field.
253
00:13:48,495 --> 00:13:49,396
So here for example.
254
00:13:49,796 --> 00:13:51,231
Now we're shooting at f 5.6.
255
00:13:52,599 --> 00:13:54,868
Before we were shooting at f 32.
256
00:13:55,635 --> 00:13:56,636
Here is the result.
257
00:13:57,470 --> 00:13:59,372
Ah, I believe it was this one at f
258
00:13:59,506 --> 00:14:00,473
32.
259
00:14:01,241 --> 00:14:03,710
And now here is the result at f 5.6.
260
00:14:04,411 --> 00:14:09,382
So our model still looks sharp, but our
background, depth of field has changed dramatically.
261
00:14:10,917 --> 00:14:15,955
And with this particular flash unit, I
can even open the aperture more,
262
00:14:16,356 --> 00:14:19,192
because I'm only at power five.
263
00:14:19,559 --> 00:14:20,627
So I can open up
264
00:14:21,294 --> 00:14:24,464
two more stops, for example, from four
to three.
265
00:14:29,302 --> 00:14:31,471
And we'll try a test shot from 5.6.
266
00:14:32,672 --> 00:14:33,273
Now
267
00:14:33,773 --> 00:14:34,341
open up the
268
00:14:34,674 --> 00:14:35,375
aperture
269
00:14:36,509 --> 00:14:38,878
from four to 28.
270
00:14:44,351 --> 00:14:45,919
And let's have a look at the result.
271
00:14:50,23 --> 00:14:50,890
And there you go.
272
00:14:51,224 --> 00:14:55,628
So now we can see that the depth of
field has even more greatly reduced,
273
00:14:56,96 --> 00:14:58,898
lost focus on her a little bit, which
you can't be quite in focus.
274
00:14:59,132 --> 00:15:00,333
Let me just readjust,
275
00:15:07,140 --> 00:15:07,707
there we go.
276
00:15:07,774 --> 00:15:08,808
She's back in focus.
277
00:15:09,309 --> 00:15:12,345
So let's compare our shot at f 28
278
00:15:13,380 --> 00:15:14,881
at power three,
279
00:15:16,16 --> 00:15:17,283
compared to
280
00:15:17,851 --> 00:15:19,185
function 32
281
00:15:20,186 --> 00:15:21,54
at power ten.
282
00:15:22,756 --> 00:15:23,990
F 2.8,
283
00:15:26,259 --> 00:15:27,360
f 32,
284
00:15:28,661 --> 00:15:29,162
f 2.8
285
00:15:29,796 --> 00:15:31,31
is at power three,
286
00:15:32,265 --> 00:15:32,632
and f
287
00:15:34,234 --> 00:15:34,334
32
288
00:15:35,368 --> 00:15:36,636
is at power ten.
289
00:15:37,537 --> 00:15:40,674
So you can see that huge difference in
change of depth of field.
290
00:15:41,74 --> 00:15:41,307
And interestingly,
291
00:15:42,575 --> 00:15:45,311
I can still go down one more stop.
292
00:15:46,413 --> 00:15:46,579
But unfortunately,
293
00:15:47,614 --> 00:15:51,618
I can open my aperture any more than 28
on this particular lens.
294
00:15:52,185 --> 00:15:55,221
Because 28 is the maximum aperture of
that lens.
295
00:15:55,789 --> 00:16:00,360
But if I was using a different lens,
like one of my 12 lenses, I could open
296
00:16:00,427 --> 00:16:05,699
up another stop further to f two to
reduce depth of field even more, if
297
00:16:05,865 --> 00:16:06,32
required.
298
00:16:06,733 --> 00:16:11,304
So that's one of the reasons why it's
really important to have a great power
299
00:16:11,538 --> 00:16:16,643
range on your flash units, which this
particular flash does very well.
300
00:16:17,477 --> 00:16:22,182
So the next demonstration, and just to
prove the physics of it and the f
301
00:16:22,248 --> 00:16:29,456
stops, is to show you a 400 unit at
power ten, compared to an 800 unit,
302
00:16:29,856 --> 00:16:32,158
800 jewel unit at power x.
303
00:16:32,425 --> 00:16:36,262
So let's go back to f 32 at power ten.
304
00:16:36,429 --> 00:16:37,430
On this light,
305
00:16:46,106 --> 00:16:48,808
let's go back to f 32 on our camera.
306
00:16:53,947 --> 00:16:55,348
Let's take a look at the result.
307
00:16:56,349 --> 00:16:57,283
So we should have
308
00:16:57,617 --> 00:16:58,885
the same exposure.
309
00:16:59,52 --> 00:16:59,986
There we go.
310
00:17:00,253 --> 00:17:03,56
So we flip between the two again, and
you can see the difference
311
00:17:03,356 --> 00:17:04,324
clearly.
312
00:17:04,824 --> 00:17:06,593
So now we're f 32,
313
00:17:07,627 --> 00:17:10,663
we have the correct exposure, and we're
on power ten.
314
00:17:11,64 --> 00:17:13,133
I'm going to change the lamp head
315
00:17:13,700 --> 00:17:18,672
to a 400 jaw unit from this 800 jaw
unit, and we'll see what happens when
316
00:17:18,672 --> 00:17:20,6
we have that at power ten.
317
00:17:20,340 --> 00:17:22,976
If the physics is correct and the lamps
are correct.
318
00:17:23,476 --> 00:17:28,948
We should be required to open up a stop
to f 22 to retain the correct exposure.
319
00:17:31,718 --> 00:17:32,952
Let's turn this one off.
320
00:17:34,754 --> 00:17:38,358
Take it off of this lighting stand that
want to get it in exactly the same
321
00:17:38,425 --> 00:17:39,693
position with the new one.
322
00:17:40,260 --> 00:17:42,228
So let's lift that off of there,
323
00:17:42,729 --> 00:17:45,131
put that lap head on the floor.
324
00:17:45,932 --> 00:17:48,335
And let's take the 400 power lamp head,
325
00:17:49,536 --> 00:17:50,870
move that onto here.
326
00:17:51,638 --> 00:17:53,606
It has the same reflector on it.
327
00:17:54,174 --> 00:17:55,542
So everything should be equal.
328
00:17:55,608 --> 00:17:57,711
Or just need to make sure it is also
pointing directly
329
00:17:59,212 --> 00:17:59,679
our model,
330
00:18:02,349 --> 00:18:03,983
is pointing at our model.
331
00:18:04,351 --> 00:18:06,886
And I'm going to take this up to power
ten.
332
00:18:07,721 --> 00:18:10,724
Now the modeling light has come on, so
I'm going to turn the modeling light off,
333
00:18:11,691 --> 00:18:12,792
so everything is equal.
334
00:18:13,126 --> 00:18:13,593
So
335
00:18:14,494 --> 00:18:16,429
we have power ten on this lamp head.
336
00:18:16,663 --> 00:18:21,468
We had power ten on our last lump head,
but our last lamp head was 800 jewels.
337
00:18:21,868 --> 00:18:23,69
This is 400 jewels.
338
00:18:23,303 --> 00:18:27,374
So it should be one stop less powerful
than our last shot.
339
00:18:30,410 --> 00:18:31,678
Let's take that shot,
340
00:18:34,814 --> 00:18:35,715
and there we go.
341
00:18:36,16 --> 00:18:39,519
We can see the shot on the 400 jaw head
342
00:18:39,953 --> 00:18:44,324
is one stop less powerful than the shot
on the 800 jaw head.
343
00:18:44,657 --> 00:18:46,659
So the physics is exactly right.
344
00:18:46,893 --> 00:18:47,60
The apertures,
345
00:18:48,94 --> 00:18:51,998
the half in the amount of light
doubling them out light is absolutely correct.
346
00:18:52,332 --> 00:18:56,670
So to get the correct exposure on the
400 lamp head, I would now need to
347
00:18:56,670 --> 00:19:01,374
change my aperture from f 32 to f 22 to
get the same exposure.
348
00:19:02,409 --> 00:19:06,12
So whilst the number sounds a
significant difference from 800 to 400,
349
00:19:07,80 --> 00:19:10,550
it actually only relates to a one stop
change.
350
00:19:10,750 --> 00:19:11,384
So you can consider
351
00:19:12,819 --> 00:19:15,622
what type of lighting power you need by
calculating
352
00:19:17,157 --> 00:19:18,191
it in f stops.
353
00:19:18,591 --> 00:19:24,330
So going from an 800 jaw head to a 1600
jaw head, whilst that sounds like a
354
00:19:24,330 --> 00:19:28,101
great change, it's actually only a one
stop increase in power.
355
00:19:28,668 --> 00:19:31,805
However, keep in mind that one stop is
still quite significant.
356
00:19:32,272 --> 00:19:35,542
It's double the amount of light, or
it's half the amount of light.
357
00:19:36,9 --> 00:19:36,910
So to continue,
358
00:19:38,345 --> 00:19:43,149
I'm going to go back to my 800 jaw head
because there's something else I want
359
00:19:43,149 --> 00:19:44,351
to show you in relation to power.
360
00:19:44,984 --> 00:19:48,488
And that is, what do we do if we
361
00:19:50,590 --> 00:19:55,161
get the light power low enough for the
larger aperture that we want to use?
362
00:19:55,462 --> 00:19:59,632
So let me change back to the 800 power
head.
363
00:20:00,33 --> 00:20:04,971
And then I also want to show you a
comparison of the power of one of these heads,
364
00:20:05,638 --> 00:20:11,44
or the 800 head, especially compared to
the power of, say, a speed like flash gun.
365
00:20:19,319 --> 00:20:23,523
I'm going to change lens on my camera,
because, remember,
366
00:20:23,957 --> 00:20:25,291
I could only get
367
00:20:25,558 --> 00:20:26,426
to power three,
368
00:20:27,627 --> 00:20:28,928
f 28.
369
00:20:29,629 --> 00:20:33,299
Now I want to go to a lens that can go
much wider than that.
370
00:20:33,400 --> 00:20:37,303
So I'm going to switch to my 85
millimeter lens, which has a maximum
371
00:20:37,704 --> 00:20:39,372
aperture of f 1.2.
372
00:20:51,384 --> 00:20:51,551
Ok?
373
00:20:51,951 --> 00:20:56,156
So now we have a lens that can open to
a larger aperture.
374
00:20:57,57 --> 00:20:59,626
And remember, we were at f 2.8
375
00:21:00,260 --> 00:21:00,427
before.
376
00:21:00,760 --> 00:21:02,228
So I'm going to shoot
377
00:21:02,896 --> 00:21:03,396
the same
378
00:21:04,831 --> 00:21:06,99
exposure, f 2.8,
379
00:21:06,900 --> 00:21:10,70
and I'm going to change this lamp to
power three,
380
00:21:10,270 --> 00:21:11,471
which is where we were before
381
00:21:12,572 --> 00:21:14,40
when we were shooting f 2.8
382
00:21:14,574 --> 00:21:15,508
on the other lens.
383
00:21:15,709 --> 00:21:17,711
So now we've got a slightly wider angle
lens.
384
00:21:18,745 --> 00:21:19,212
We're at 2.8.
385
00:21:20,280 --> 00:21:21,614
We'll take this shot,
386
00:21:21,781 --> 00:21:25,285
and we should end up with exactly the
correct exposure.
387
00:21:31,624 --> 00:21:31,791
Ok?
388
00:21:32,25 --> 00:21:33,126
So there we have
389
00:21:34,27 --> 00:21:35,795
f 28 on this lens.
390
00:21:35,929 --> 00:21:37,630
You can see it's a wider angle lens.
391
00:21:37,697 --> 00:21:39,299
This an 85 millimeter lens.
392
00:21:39,399 --> 00:21:41,167
I was using a seventy to 200 before.
393
00:21:41,468 --> 00:21:43,403
And we can see the exposures pretty
good.
394
00:21:43,770 --> 00:21:48,274
It looks a little bit brighter than I
remember from the comparison on the
395
00:21:48,274 --> 00:21:48,675
other lens.
396
00:21:48,742 --> 00:21:51,678
But as I said, it's very unlikely that
the flash
397
00:21:51,945 --> 00:21:53,747
power is wrong.
398
00:21:54,14 --> 00:21:58,18
It is clearly the aperture number is
wrong, because we're using the same
399
00:21:58,518 --> 00:21:59,853
amount of flush
400
00:22:00,153 --> 00:22:00,787
power
401
00:22:00,987 --> 00:22:01,154
three.
402
00:22:01,621 --> 00:22:04,24
And we were using power three before.
403
00:22:04,758 --> 00:22:09,929
So there's a slight discrepancy here in
the actual camera aperture settings of
404
00:22:09,929 --> 00:22:10,363
f 2.8
405
00:22:10,897 --> 00:22:12,265
on one lens and f 2.8
406
00:22:12,832 --> 00:22:13,233
on the other.
407
00:22:13,533 --> 00:22:17,904
Now there shouldn't be, but this is
actually quite common in a lot of cameras.
408
00:22:18,71 --> 00:22:18,705
So
409
00:22:19,372 --> 00:22:22,509
anyway, we'll accept that as being the
correct exposure.
410
00:22:23,309 --> 00:22:28,281
So I can now drop that power from three
to the minimum power on this light,
411
00:22:28,415 --> 00:22:29,749
which is power two.
412
00:22:29,949 --> 00:22:31,851
So I'm going to go to power two.
413
00:22:34,521 --> 00:22:35,555
We go that's power, too.
414
00:22:35,689 --> 00:22:38,558
That's the lowest power I can set on
this light.
415
00:22:39,292 --> 00:22:41,928
Now I need to open the aperture
416
00:22:42,896 --> 00:22:43,997
on this camera
417
00:22:44,731 --> 00:22:46,66
by one stop.
418
00:22:46,599 --> 00:22:48,335
So we're going to f two.
419
00:22:49,769 --> 00:22:50,704
Take the picture.
420
00:22:52,672 --> 00:22:53,907
Take a look at the result.
421
00:22:55,75 --> 00:22:56,476
And we can see here
422
00:22:57,711 --> 00:22:58,244
we have
423
00:22:58,678 --> 00:23:00,914
the correct exposure, or this matching
exposure.
424
00:23:01,548 --> 00:23:03,516
See how the depth of field
425
00:23:04,984 --> 00:23:07,520
decreased again, even from 28
426
00:23:07,854 --> 00:23:09,289
to f ii.
427
00:23:10,357 --> 00:23:12,492
Some of the extra exposure that we're
seeing
428
00:23:13,560 --> 00:23:16,162
may be down to ambient light.
429
00:23:17,63 --> 00:23:23,536
And this is partly related to as that
aperture has become very, very large.
430
00:23:24,270 --> 00:23:27,874
It's now starting to pick up some of
the continuous light that we've got.
431
00:23:27,941 --> 00:23:28,441
Around us.
432
00:23:28,675 --> 00:23:32,445
So the lights that we're using to video
this sequence right now, or any
433
00:23:32,512 --> 00:23:37,217
daylight coming in through the window,
is actually starting to get captured as
434
00:23:37,550 --> 00:23:39,185
that aperture opens up.
435
00:23:39,853 --> 00:23:43,857
This is also how the shutter speed can
affect the amount of light.
436
00:23:44,90 --> 00:23:46,92
If we look at the shutter speed range,
437
00:23:46,493 --> 00:23:50,330
when we're talking about flush, we
don't really need to consider the
438
00:23:50,330 --> 00:23:51,197
shutter speed,
439
00:23:51,698 --> 00:23:53,233
because it's only the aperture.
440
00:23:55,468 --> 00:23:59,939
as we lower the shutter speed with
flush photography, then we let in
441
00:24:00,173 --> 00:24:02,575
daylight in addition to the flash.
442
00:24:03,143 --> 00:24:05,78
And that will build the exposure
brighter.
443
00:24:05,545 --> 00:24:08,314
But I'm going to cover that in more
detail later.
444
00:24:08,748 --> 00:24:11,51
So let's go back to our initial problem.
445
00:24:12,118 --> 00:24:17,57
And the problem is that I am now at the
minimum power on this light.
446
00:24:17,290 --> 00:24:18,191
I'm at power too.
447
00:24:18,758 --> 00:24:20,527
It doesn't go down to power one.
448
00:24:21,161 --> 00:24:24,631
If we were using this scorrow pack, for
example,
449
00:24:24,998 --> 00:24:28,902
I could not only go down to power too,
I could go down to power one.
450
00:24:29,235 --> 00:24:29,703
Power 0.98,
451
00:24:31,304 --> 00:24:32,272
I can go down to 0.1.
452
00:24:33,873 --> 00:24:37,143
But this is obviously a much more
expensive, much more professional
453
00:24:37,711 --> 00:24:37,877
system.
454
00:24:38,345 --> 00:24:41,648
It also has the ability to go much,
much higher in power.
455
00:24:41,948 --> 00:24:42,649
This is a 300200
456
00:24:44,918 --> 00:24:49,122
jewel unit compared to 800 jewels that
we have here.
457
00:24:49,389 --> 00:24:53,860
So that has the ability of going two
stops more powerful than the maximum
458
00:24:54,361 --> 00:24:55,829
power on this light.
459
00:24:56,329 --> 00:24:56,963
Anyway,
460
00:24:57,297 --> 00:24:58,598
how do we solve the problem?
461
00:24:58,998 --> 00:25:01,935
Now, if I want to go from f two
462
00:25:02,569 --> 00:25:04,871
down to f 1.4,
463
00:25:05,372 --> 00:25:06,339
let's watch what happens.
464
00:25:06,506 --> 00:25:07,140
If I go to 1.4,
465
00:25:08,274 --> 00:25:08,975
we know
466
00:25:09,542 --> 00:25:12,312
that the picture is going to end up
over exposed.
467
00:25:13,79 --> 00:25:14,714
So I go to 1.4,
468
00:25:15,148 --> 00:25:16,16
take the shot,
469
00:25:16,983 --> 00:25:18,84
and we'll see,
470
00:25:18,518 --> 00:25:19,185
the result
471
00:25:19,619 --> 00:25:20,787
is now a stop
472
00:25:21,54 --> 00:25:21,921
over exposed.
473
00:25:22,655 --> 00:25:24,624
And I can't do anything about it
474
00:25:25,58 --> 00:25:29,429
because I can't reduce the power of the
studio light any more.
475
00:25:29,863 --> 00:25:34,234
All I could do now is choose to move
the studio light further away
476
00:25:34,334 --> 00:25:35,301
to reduce the power.
477
00:25:35,702 --> 00:25:39,372
But there is one little trick that I
can apply, which i'll show you,
478
00:25:41,641 --> 00:25:42,876
and here's the trick.
479
00:25:43,543 --> 00:25:46,246
This is a neutral density filter.
480
00:25:46,579 --> 00:25:49,449
It's a filter that will cut out
481
00:25:50,16 --> 00:25:50,884
extra light.
482
00:25:51,317 --> 00:25:52,919
So in this case, this is a 0.9
483
00:25:53,386 --> 00:25:53,553
filter.
484
00:25:53,787 --> 00:25:56,156
That means it's three stops strength.
485
00:25:56,489 --> 00:25:59,25
It will cut out three stops of light.
486
00:25:59,626 --> 00:26:03,863
Now in this case, I don't actually want
to cut out three stops of light, only
487
00:26:03,930 --> 00:26:05,799
one to cut out about a stop of light.
488
00:26:06,99 --> 00:26:07,867
At the moment we are at f 14.
489
00:26:09,69 --> 00:26:12,5
I'm now going to cut out three stops of
light,
490
00:26:13,139 --> 00:26:14,207
which will be too much.
491
00:26:14,741 --> 00:26:16,309
We look at the result on screen,
492
00:26:19,946 --> 00:26:20,680
and there we go.
493
00:26:21,147 --> 00:26:23,350
This picture is now three stops
494
00:26:23,950 --> 00:26:25,852
underexposed from our previous picture,
495
00:26:27,53 --> 00:26:28,655
and we're at power
496
00:26:28,788 --> 00:26:29,289
too.
497
00:26:29,622 --> 00:26:34,994
But the beauty is that I can actually
now increase the power to compensate
498
00:26:35,695 --> 00:26:38,98
for the fact that the filter is too
dark.
499
00:26:38,732 --> 00:26:41,134
Filters obviously come in different
strengths,
500
00:26:41,534 --> 00:26:44,437
so you could have applied a less strong
filter.
501
00:26:45,138 --> 00:26:50,176
So looking at that result looks like, I
want to go up by about a stop in power.
502
00:26:50,677 --> 00:26:54,414
So I'm now going to take the light up
to power three.
503
00:26:57,50 --> 00:26:58,885
I'm going to take the shot again.
504
00:27:08,828 --> 00:27:11,531
Needs to go up a little bit more,
another stop.
505
00:27:12,32 --> 00:27:14,67
So we're up to power four now.
506
00:27:24,277 --> 00:27:24,978
And there we go.
507
00:27:25,211 --> 00:27:27,514
There's an exposure level that I'm
happy with.
508
00:27:27,881 --> 00:27:30,250
So I've managed to obtain
509
00:27:30,583 --> 00:27:31,151
f 1.4
510
00:27:32,752 --> 00:27:33,920
on my camera.
511
00:27:34,587 --> 00:27:36,156
And by using a filter,
512
00:27:36,356 --> 00:27:38,558
I've been able to increase the power
513
00:27:38,758 --> 00:27:41,594
to get it correct for 14.
514
00:27:42,28 --> 00:27:46,566
Previously we weren't able to obtain an
exposure less than 28,
515
00:27:47,233 --> 00:27:50,36
because the light would only go down to
power two.
516
00:27:50,503 --> 00:27:53,940
Now that is still a massive reduction
in light power.
517
00:27:54,507 --> 00:27:58,44
These particular lights are very good
for a large power range.
518
00:27:58,812 --> 00:28:01,881
But if I wanted to go lower than f 2.8,
519
00:28:02,415 --> 00:28:03,616
where I won't gone to 1.4
520
00:28:04,417 --> 00:28:07,87
by using a filter, I was able to
achieve it.
521
00:28:07,220 --> 00:28:10,357
In fact, I was able to achieve it so
easily, because this is a three stop
522
00:28:10,490 --> 00:28:14,561
filter, I had to actually turn the
power of the light back up again.
523
00:28:15,195 --> 00:28:15,829
Ok,
524
00:28:16,162 --> 00:28:16,262
finally,
525
00:28:17,697 --> 00:28:22,736
on flash power, we're now going to look
at the power of a monoblock studio
526
00:28:23,69 --> 00:28:27,374
lamp, such as this one, compared to an
on camera
527
00:28:27,474 --> 00:28:28,308
speed light.
528
00:28:32,679 --> 00:28:33,279
So on this
529
00:28:33,446 --> 00:28:33,913
stand
530
00:28:34,581 --> 00:28:35,515
all the time
531
00:28:36,182 --> 00:28:40,954
was a light meter, or more importantly,
a flash meter.
532
00:28:41,554 --> 00:28:42,889
Now flash meter
533
00:28:43,957 --> 00:28:45,558
does what it sounds like it would do.
534
00:28:45,625 --> 00:28:47,193
It measures the amount of flesh.
535
00:28:47,627 --> 00:28:50,63
So turning this flash meter on
536
00:28:50,830 --> 00:28:53,266
and just angle that down a little bit
so you can see it,
537
00:28:54,267 --> 00:28:56,469
you can see I've got some Numbers here,
538
00:28:57,137 --> 00:29:01,541
and I can set the iso, the shutter
speed, and then it's showing me an
539
00:29:01,641 --> 00:29:02,876
aperture value.
540
00:29:03,209 --> 00:29:07,781
So when I fire the flash, it will
measure what it thinks is the correct
541
00:29:08,14 --> 00:29:08,748
aperture value.
542
00:29:09,215 --> 00:29:14,821
Now we're going to come to using light
meters and why they might be a good
543
00:29:14,821 --> 00:29:19,559
idea, or why they might not be a good
idea in another section, but for the
544
00:29:19,559 --> 00:29:23,863
purpose of measuring the flash power
accurately right now, and comparing a
545
00:29:23,863 --> 00:29:25,865
monoblock head to a
546
00:29:27,233 --> 00:29:31,805
speed light, or maybe even comparing it
to the more powerful scorrow, pack this
547
00:29:31,871 --> 00:29:32,806
will be useful.
548
00:29:33,239 --> 00:29:34,240
So we'll just pop
549
00:29:34,741 --> 00:29:39,512
the flash meter there, which is where
the studio light was directed.
550
00:29:39,946 --> 00:29:41,915
And let's take a reading.
551
00:29:42,816 --> 00:29:45,285
And I'm going to aim that directly at
552
00:29:46,186 --> 00:29:46,820
the light meter.
553
00:29:46,986 --> 00:29:50,590
I'm going to turn the power on this up
to power ten, which is the maximum
554
00:29:50,990 --> 00:29:51,157
power.
555
00:29:51,791 --> 00:29:53,593
And I'm going to press the test button.
556
00:29:55,795 --> 00:29:57,564
Oh, I haven't activated this yet.
557
00:29:57,697 --> 00:29:58,398
Sorry, let's
558
00:29:58,832 --> 00:30:00,333
activate the light meter.
559
00:30:01,0 --> 00:30:02,736
Push that test button again.
560
00:30:04,838 --> 00:30:06,406
Now let's see what it says.
561
00:30:07,474 --> 00:30:08,475
It is saying
562
00:30:09,209 --> 00:30:09,776
f 32.
563
00:30:10,910 --> 00:30:12,178
Well, actually it says f 22.9.
564
00:30:13,380 --> 00:30:18,885
But if you look at the scale up here,
it says f 32, which is interesting, because
565
00:30:18,985 --> 00:30:21,321
our camera also required f 32
566
00:30:22,422 --> 00:30:24,24
to get the correct exposure.
567
00:30:24,657 --> 00:30:28,161
So this light meter is actually giving
us an accurate reading,
568
00:30:28,828 --> 00:30:32,165
very close reading to what we would
have needed to set in the camera.
569
00:30:32,665 --> 00:30:35,702
So by comparison, how would a speed
light?
570
00:30:35,869 --> 00:30:36,36
Ready?
571
00:30:36,336 --> 00:30:37,871
We've got f 32 or 229
572
00:30:38,972 --> 00:30:39,873
there on that.
573
00:30:39,873 --> 00:30:40,40
One.
574
00:30:40,173 --> 00:30:41,775
Let's see what we get with the speed
light.
575
00:30:44,277 --> 00:30:45,445
So here's a speed light.
576
00:30:45,945 --> 00:30:47,514
I've put it into
577
00:30:48,348 --> 00:30:49,282
manual mode,
578
00:30:49,849 --> 00:30:52,485
so I've got one to one that's full
power.
579
00:30:52,919 --> 00:30:56,256
You can see the zoom is at 28, which
means the spread of light will be quite
580
00:30:56,356 --> 00:30:56,523
wide.
581
00:30:56,990 --> 00:31:00,360
That wouldn't be really fair on this
because the spread of light, although
582
00:31:00,827 --> 00:31:03,163
wide on this, is a little bit more
directional.
583
00:31:03,530 --> 00:31:07,33
So I'm going to change the zoom to
seventy millimeter
584
00:31:07,634 --> 00:31:08,468
on here
585
00:31:09,536 --> 00:31:11,671
to give a more or less
586
00:31:12,505 --> 00:31:14,74
equivalent spread
587
00:31:14,407 --> 00:31:14,574
to
588
00:31:15,775 --> 00:31:16,476
the
589
00:31:17,477 --> 00:31:18,244
studio light,
590
00:31:18,812 --> 00:31:20,580
and then direct the lamp head.
591
00:31:20,680 --> 00:31:22,248
I'm going to turn this off,
592
00:31:23,216 --> 00:31:25,452
and I'm going to put this in the same
position.
593
00:31:25,952 --> 00:31:28,788
I'm just going to activate my light
meter.
594
00:31:29,956 --> 00:31:31,24
Press the test button,
595
00:31:34,761 --> 00:31:38,198
and we have a reading of f 11 and a
half,
596
00:31:39,532 --> 00:31:40,967
11 and a half
597
00:31:41,634 --> 00:31:42,736
compared to f 32.
598
00:31:43,136 --> 00:31:44,4
So we lost
599
00:31:44,337 --> 00:31:46,673
two and a half f stops of power.
600
00:31:47,374 --> 00:31:49,442
So this thing on full power,
601
00:31:49,876 --> 00:31:52,312
was two and a half f stops, less
602
00:31:52,812 --> 00:31:54,881
than our 800 jaw lamp head.
603
00:31:55,548 --> 00:31:58,885
The other reason that these lamp head,
these
604
00:31:59,719 --> 00:32:01,154
speed lights, have disadvantages,
605
00:32:02,188 --> 00:32:03,790
is, obviously, this is battery powered.
606
00:32:04,491 --> 00:32:09,629
It isn't as versatile with the amount
of adapters and umbrellas or soft boxes
607
00:32:10,96 --> 00:32:12,832
or accessories that we can add to our
light.
608
00:32:13,133 --> 00:32:18,104
And those are the most important
things, because we need to control the
609
00:32:18,104 --> 00:32:22,575
light, shape the light and change the
light to give the most
610
00:32:23,143 --> 00:32:26,79
aesthetically pleasing light on our
subjects.
611
00:32:26,279 --> 00:32:29,115
And those are things we'll be covering
later in this,
612
00:32:29,382 --> 00:32:29,749
of course,
47284
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