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These are the user uploaded subtitles that are being translated: 1 00:00:06,873 --> 00:00:07,374 Understanding 2 00:00:08,108 --> 00:00:13,747 flash power is absolutely crucial to our understanding of studio lighting. 3 00:00:14,414 --> 00:00:19,119 So to help us do that, I've recruited our model stiffany. 4 00:00:19,452 --> 00:00:23,356 I also have an aperture and shutter speed chart. 5 00:00:23,957 --> 00:00:28,194 We have a camera tethered into the computer so that we can see the 6 00:00:28,194 --> 00:00:28,361 results. 7 00:00:29,62 --> 00:00:33,800 And you'll also notice that I've put a cstan at the back here, which you'll 8 00:00:33,933 --> 00:00:35,235 understand what that's for. 9 00:00:35,368 --> 00:00:36,2 Shortly, 10 00:00:36,970 --> 00:00:40,573 before we start, let's get some simple clarification 11 00:00:41,708 --> 00:00:42,509 about the power 12 00:00:42,976 --> 00:00:43,877 of lamp heads. 13 00:00:44,678 --> 00:00:48,982 So we're going to start our first tests with this particular lamp head. 14 00:00:49,382 --> 00:00:50,984 And this one is an 800 15 00:00:52,185 --> 00:00:52,919 jewel power. 16 00:00:54,587 --> 00:00:55,188 This one 17 00:00:55,955 --> 00:00:58,224 is a 400 jewel power. 18 00:00:58,425 --> 00:01:01,928 So it sounds like it's a lot lot less than this one. 19 00:01:02,328 --> 00:01:04,330 Well, actually the difference is half, 20 00:01:05,398 --> 00:01:08,635 400 jewels is half the power of 800 jewels. 21 00:01:08,968 --> 00:01:10,570 And in lighting terms, 22 00:01:11,137 --> 00:01:12,639 half the amount of light 23 00:01:13,306 --> 00:01:14,874 is one stop less. 24 00:01:15,875 --> 00:01:21,781 So by now you should be familiar with apertures and f stops if you're at that 25 00:01:21,781 --> 00:01:23,683 level of using studio lighting, 26 00:01:24,117 --> 00:01:26,19 and we're going to look at that relationship 27 00:01:27,53 --> 00:01:28,154 between f stops 28 00:01:28,655 --> 00:01:31,858 and studio light power to clearly understand it. 29 00:01:32,359 --> 00:01:34,361 But first of all, let's simply look at this. 30 00:01:34,661 --> 00:01:39,366 So for example, if the correct exposure was at f eleven. 31 00:01:40,266 --> 00:01:40,967 If we had 32 00:01:41,701 --> 00:01:46,873 the correct exposure at f eleven with an 800 jewel lamp head at full power, 33 00:01:47,374 --> 00:01:53,279 then on a 400 jewel lamp head, we would need one stop brighter, because 34 00:01:53,713 --> 00:01:57,550 f eight is allowing twice the amount of light in. 35 00:01:57,717 --> 00:02:02,555 And a 400 jewel is half the amount of power of the 800 jaw head. 36 00:02:02,889 --> 00:02:03,356 So 37 00:02:03,857 --> 00:02:08,762 the relationship between one stop changes either a 200 jaw head of 400 38 00:02:09,229 --> 00:02:14,601 jaw head, 800 jaw head, 1600 jaw head, is exactly the same as the relationship 39 00:02:15,135 --> 00:02:18,71 between one full f stop jumps. 40 00:02:18,738 --> 00:02:22,442 Now we know that we can change our f stops and our apertures in smaller 41 00:02:22,575 --> 00:02:22,742 jumps. 42 00:02:22,976 --> 00:02:26,880 We can change them in one third increments, if necessary. 43 00:02:27,380 --> 00:02:33,153 We can actually change the power on our flush heads in 110th of an f stop 44 00:02:33,319 --> 00:02:35,188 increments, if we require. 45 00:02:36,22 --> 00:02:37,791 So let's start exploring 46 00:02:39,459 --> 00:02:42,228 the change in power on the lamp heads 47 00:02:43,63 --> 00:02:48,501 and see what it means when we go from full power to minimum power, and why 48 00:02:48,735 --> 00:02:51,504 having a good range of power is important. 49 00:02:53,73 --> 00:02:56,309 Now to make sure that our test is consistent, 50 00:02:56,676 --> 00:03:00,280 I'm going to make sure that the modeling lamp is off. 51 00:03:00,580 --> 00:03:03,149 You can see at the moment, the modeling lamp is on. 52 00:03:03,950 --> 00:03:08,988 Now if we leave the modeling lamp on that is quite a lot of extra light 53 00:03:09,389 --> 00:03:10,724 hitting our model. 54 00:03:11,291 --> 00:03:16,196 Now that extra light can actually affect the exposure of our flashshot, 55 00:03:16,896 --> 00:03:19,199 because it's additional light to the flash. 56 00:03:19,466 --> 00:03:23,870 So I'm going to turn the modeling light off so that the exposures that we're 57 00:03:24,37 --> 00:03:28,641 reading, and the results that we're seeing are purely the flash only. 58 00:03:35,215 --> 00:03:35,682 So 59 00:03:36,249 --> 00:03:38,718 I'm starting on power 10. 60 00:03:39,319 --> 00:03:43,990 And that is the maximum power that I can get out of this light. 61 00:03:45,58 --> 00:03:48,28 If, for example, power ten was f sixteen 62 00:03:49,62 --> 00:03:50,30 required on the camera, 63 00:03:51,64 --> 00:03:56,102 then if I drop to power nine, I would require f eleven. 64 00:03:56,736 --> 00:03:59,939 If I dropped to power eight, I would require f eight. 65 00:04:00,173 --> 00:04:03,877 If I dropped a power seven, I would require f 5.6. 66 00:04:05,78 --> 00:04:10,684 Because each drop from ten to nine to eight to seven to six, on a studio 67 00:04:10,984 --> 00:04:14,87 light, is a one full f stop jump. 68 00:04:14,921 --> 00:04:17,323 So we'd have to adjust the apertures accordingly. 69 00:04:18,91 --> 00:04:23,463 But I don't know yet exactly what aperture setting we need four power ten 70 00:04:24,30 --> 00:04:25,932 at this particular distance. 71 00:04:26,332 --> 00:04:28,635 Because also keep in mind that the 72 00:04:28,802 --> 00:04:29,135 power 73 00:04:29,369 --> 00:04:30,70 of a light 74 00:04:30,837 --> 00:04:34,341 is also related to the distance from the subject. 75 00:04:35,375 --> 00:04:40,180 So as we move a light closer to our subject, the power of the light will be 76 00:04:40,580 --> 00:04:40,747 stronger. 77 00:04:41,314 --> 00:04:45,285 If we move the light further away, the power of the light will decrease. 78 00:04:45,785 --> 00:04:50,23 Now, other factors also affect the power of the light, and that is when we 79 00:04:50,23 --> 00:04:51,691 put different modifiers on. 80 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 81 00:04:56,29 --> 00:05:00,200 off of a different surface, then a lot of that power will be dispersed into 82 00:05:00,266 --> 00:05:03,370 different directions, and it will reduce the power. 83 00:05:03,703 --> 00:05:07,73 So for this test, I'm just using a standard l forty reflector, 84 00:05:08,108 --> 00:05:08,308 and 85 00:05:08,742 --> 00:05:09,242 that's it. 86 00:05:09,542 --> 00:05:10,877 And we'll direct the light 87 00:05:11,144 --> 00:05:15,48 straight at our model, and we'll see what exposure settings we require. 88 00:05:16,649 --> 00:05:17,751 So first of all, 89 00:05:18,184 --> 00:05:19,519 coming into my camera, 90 00:05:20,353 --> 00:05:22,722 framing up and focusing on my model, 91 00:05:23,289 --> 00:05:27,193 I'm using a shutter speed a 160th of a second, because that's the 92 00:05:28,428 --> 00:05:29,963 sink speed that will work with this. 93 00:05:30,430 --> 00:05:35,635 The shutter speed doesn't have any real bearing on the exposure for flash. 94 00:05:35,869 --> 00:05:38,571 But i'll explain a bit more about that later. 95 00:05:39,239 --> 00:05:41,441 First of all, we're going to set our aperture. 96 00:05:42,175 --> 00:05:45,879 So I'm going to set my aperture to start with, to f 22 97 00:05:46,980 --> 00:05:47,647 in this case. 98 00:05:48,14 --> 00:05:50,383 So my starting aperture is f 99 00:05:50,717 --> 00:05:51,685 22. 100 00:05:52,185 --> 00:05:56,489 My lamp is on power ten, which is full power, 101 00:05:56,890 --> 00:05:59,359 full power on an 800 head. 102 00:06:00,26 --> 00:06:04,964 If I had power ten on this head, which is a 400 jewel, 103 00:06:05,699 --> 00:06:07,33 that would be equivalent 104 00:06:07,300 --> 00:06:10,236 to power nine on this head, 105 00:06:10,737 --> 00:06:15,675 because this light is one stop less powerful than that light. 106 00:06:16,176 --> 00:06:17,644 So back to power ten. 107 00:06:18,111 --> 00:06:18,978 No modeling lamp. 108 00:06:19,212 --> 00:06:20,513 Let's take our first shot. 109 00:06:21,81 --> 00:06:25,752 We're using the trigger on top of the camera to trigger the flash gun, 110 00:06:26,653 --> 00:06:28,154 taking our first picture. 111 00:06:30,23 --> 00:06:30,557 And you can 112 00:06:30,757 --> 00:06:32,759 hear that large outburst of light. 113 00:06:33,159 --> 00:06:35,462 So that picture is now going to come into 114 00:06:36,496 --> 00:06:36,830 the computer. 115 00:06:37,864 --> 00:06:39,532 And we can see the first result there, 116 00:06:40,734 --> 00:06:44,170 which looks a little bit over exposed. 117 00:06:44,738 --> 00:06:46,239 So that's at f 118 00:06:46,873 --> 00:06:47,907 22, 119 00:06:48,742 --> 00:06:50,877 an aperture of f 22. 120 00:06:51,378 --> 00:06:52,178 And there's the result. 121 00:06:52,912 --> 00:06:56,449 So I'm going to close the aperture down to f 32, 122 00:06:57,50 --> 00:06:58,184 to one stop. 123 00:06:59,219 --> 00:07:03,523 Less light able to get into the camera, which will reduce that 124 00:07:03,790 --> 00:07:03,957 exposure. 125 00:07:04,491 --> 00:07:05,925 So let me do that quickly. 126 00:07:07,627 --> 00:07:11,231 So changing the camera now, I'm just changing it to f 32. 127 00:07:12,32 --> 00:07:13,600 Taking that picture again. 128 00:07:14,200 --> 00:07:15,468 Same power on the studio. 129 00:07:15,769 --> 00:07:15,935 Lamp. 130 00:07:16,436 --> 00:07:18,71 Let's look at the result on screen. 131 00:07:18,571 --> 00:07:19,406 So there we go. 132 00:07:19,706 --> 00:07:22,709 We now have the correct exposure 133 00:07:22,876 --> 00:07:23,677 on 134 00:07:25,378 --> 00:07:27,247 We can see the skin tone seems well. 135 00:07:27,313 --> 00:07:27,480 Exposed. 136 00:07:27,714 --> 00:07:29,82 Is just a single light setup. 137 00:07:29,716 --> 00:07:33,319 Obviously, as we demonstrate more lighting, examples will be showing you 138 00:07:33,787 --> 00:07:35,321 lots of ways to light a model. 139 00:07:35,455 --> 00:07:38,91 This is the most simple single light setup. 140 00:07:38,725 --> 00:07:39,359 Now 141 00:07:39,859 --> 00:07:46,32 what's important to notice, here is the level of detail on this cross bar in 142 00:07:46,199 --> 00:07:47,200 the background. 143 00:07:47,534 --> 00:07:49,936 So remember, we're at f 32, 144 00:07:50,503 --> 00:07:52,639 and we have the correct exposure, 145 00:07:53,73 --> 00:07:57,477 and our depth of field is quite large, because we can see the model is sharp. 146 00:07:58,11 --> 00:08:02,248 And this object in the background, which is actually about three 147 00:08:03,550 --> 00:08:08,655 meters behind the model, is also becoming quite sharp in the picture. 148 00:08:09,55 --> 00:08:11,224 And this is why it's important to have a large 149 00:08:12,359 --> 00:08:18,665 range of power in your flesh unit, so that you can control depth of field. 150 00:08:19,232 --> 00:08:23,370 So we're now gradually going to change the exposure 151 00:08:23,870 --> 00:08:26,439 of the flash and the apertures on the camera, 152 00:08:27,474 --> 00:08:29,943 reducing depth of field at the same time. 153 00:08:30,677 --> 00:08:34,748 But before I do that, I'm going to leave the aperture at f 32, 154 00:08:35,782 --> 00:08:38,918 and I'm going to change the power of the light just by 110th 155 00:08:40,120 --> 00:08:40,754 of an f stop. 156 00:08:41,54 --> 00:08:44,791 So I'm going to take it from power x to power 9.9. 157 00:08:46,760 --> 00:08:47,827 So from ten 158 00:08:48,595 --> 00:08:49,829 to 9.9, 159 00:08:50,330 --> 00:08:51,364 take the shot. 160 00:08:51,798 --> 00:08:53,133 Let's take a look at the result. 161 00:08:54,434 --> 00:08:55,235 And there we go. 162 00:08:55,368 --> 00:08:58,872 We can see the difference here's at power 9.9 163 00:08:59,472 --> 00:09:00,807 and there's at power 199, 164 00:09:03,209 --> 00:09:04,10 power, 199, 165 00:09:06,12 --> 00:09:06,513 power ten. 166 00:09:06,680 --> 00:09:08,982 So that's only 110th of an f stop. 167 00:09:09,382 --> 00:09:11,685 And that's why that difference looks 168 00:09:11,951 --> 00:09:14,521 so subtle, because it is very subtle. 169 00:09:14,988 --> 00:09:19,192 110th of an fstop is a very small amount as you can see there. 170 00:09:19,793 --> 00:09:22,362 So let's carry on in full f stop. 171 00:09:22,595 --> 00:09:26,99 So at this time, we're going to go from power ten, where we were here. 172 00:09:26,499 --> 00:09:28,802 I'm going to go to power nine. 173 00:09:35,308 --> 00:09:36,476 So power nine. 174 00:09:37,143 --> 00:09:40,13 Now, when a light goes down in power, 175 00:09:40,680 --> 00:09:44,951 you do need to allow the light the time to reset its power. 176 00:09:45,452 --> 00:09:50,423 Some flash units require you to actually dump the power manually out of 177 00:09:50,423 --> 00:09:50,590 it. 178 00:09:50,590 --> 00:09:52,826 But an advanced flash unit like this one doesn't. 179 00:09:53,59 --> 00:09:54,828 It will rebuild balance itself. 180 00:09:55,395 --> 00:09:57,464 So we've now dropped down from power ten, 181 00:09:58,598 --> 00:10:03,3 from the exposure on screen now, to power nine, which is one f stop less. 182 00:10:03,136 --> 00:10:04,471 Let's take that shot, 183 00:10:05,872 --> 00:10:07,374 and let's take a look at the result. 184 00:10:10,276 --> 00:10:11,344 That was power ten. 185 00:10:12,579 --> 00:10:13,613 That's power nine. 186 00:10:14,14 --> 00:10:17,450 So you can see this is one f stop less of light. 187 00:10:17,851 --> 00:10:18,985 That one was power 99. 188 00:10:19,619 --> 00:10:20,820 There's our power ten shot. 189 00:10:21,221 --> 00:10:22,555 Now there's power nine. 190 00:10:22,989 --> 00:10:26,226 So you can see a whole f stop of light. 191 00:10:26,659 --> 00:10:28,328 Now a whole f stop of light 192 00:10:28,995 --> 00:10:32,432 is actually a reduction, is half the amount of light. 193 00:10:32,599 --> 00:10:36,469 Remember, an f stop is either half the amount of light or double the amount of light. 194 00:10:36,970 --> 00:10:40,40 So in light terms, we add the correct exposure at f 32. 195 00:10:41,141 --> 00:10:43,309 We've dropped the power to power nine. 196 00:10:43,610 --> 00:10:44,811 And now our picture is underexposed. 197 00:10:46,12 --> 00:10:50,350 So we now need to open the aperture by the equivalent amount by one f. 198 00:10:50,417 --> 00:10:54,721 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 201 00:11:00,260 --> 00:11:02,62 to f 22, 202 00:11:02,328 --> 00:11:03,63 from f 32, 203 00:11:04,330 --> 00:11:05,932 leaving it a power nine. 204 00:11:06,99 --> 00:11:08,635 And we'll now see that the exposure 205 00:11:09,636 --> 00:11:11,504 on this one we'll now be correct. 206 00:11:12,172 --> 00:11:13,540 So we can now see, f 22, 207 00:11:14,574 --> 00:11:18,244 that this exposure is correct for power nine. 208 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. 209 00:11:25,618 --> 00:11:28,655 And you can see that they are very close. 210 00:11:29,155 --> 00:11:32,892 Now any discrepancy in power where there's a slight little bit of 211 00:11:32,892 --> 00:11:35,395 difference is not actually down to the light. 212 00:11:35,862 --> 00:11:39,466 It certainly won't be down to these lights, because they are very, very 213 00:11:39,799 --> 00:11:41,234 high quality professional lights. 214 00:11:41,634 --> 00:11:44,804 The discrepancy here will be in the aperture in the camera. 215 00:11:46,740 --> 00:11:50,110 So we're now at f 22, and we have the correct exposure. 216 00:11:50,910 --> 00:11:53,913 But what happens if we change the light more dramatically? 217 00:11:54,180 --> 00:11:56,483 If I go, say, four f stops 218 00:11:56,916 --> 00:11:58,551 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. 226 00:12:22,108 --> 00:12:24,310 So I'm going to change from f 224, 227 00:12:24,811 --> 00:12:27,213 f stops brighter to f 5.6. 228 00:12:30,183 --> 00:12:31,518 So f 22, 229 00:12:32,752 --> 00:12:35,355 open the aperture up to f 5.6, 230 00:12:35,789 --> 00:12:36,656 take the shot. 231 00:12:36,890 --> 00:12:38,24 And it will now be dramatically 232 00:12:39,59 --> 00:12:39,993 overexposed, 233 00:12:41,227 --> 00:12:44,597 because it's going to be four stops over exposed, as you can see here, 234 00:12:45,65 --> 00:12:48,501 because we doubled the light, we doubled the light, we doubled the 235 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 237 00:12:52,839 --> 00:12:53,273 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 00:13:07,854 --> 00:13:08,788 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 247 00:13:26,673 --> 00:13:28,808 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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