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These are the user uploaded subtitles that are being translated: 1 00:00:00,066 --> 00:00:03,870 In this chapter, we're going to do a deep dive on color scopes. 2 00:00:03,937 --> 00:00:08,675 Color scopes are essential for colors actually are what you think they are, 3 00:00:08,875 --> 00:00:12,879 and not just how they look on your screen or how they might look to your eye. 4 00:00:13,013 --> 00:00:17,250 It's a way to technically measure where your colors actually are. 5 00:00:17,417 --> 00:00:19,252 And this is really important because kind of like 6 00:00:19,252 --> 00:00:22,622 we talked about in the environment lesson, your eyes can adjust 7 00:00:22,622 --> 00:00:25,892 to make an image look correct, even if the image isn't correct. 8 00:00:25,959 --> 00:00:29,362 If you've ever tried wearing like tinted sunglasses 9 00:00:29,362 --> 00:00:31,898 that maybe have a yellow kind of tinge to them, after a while, 10 00:00:31,898 --> 00:00:34,234 you kind of stop noticing that yellow tint. 11 00:00:34,234 --> 00:00:37,203 And then when you take your glasses off, everything looks kind of blue. 12 00:00:37,203 --> 00:00:39,739 That's because our eyes are always adjusting. 13 00:00:39,739 --> 00:00:43,910 So scopes are a really great way to see if something is actually white 14 00:00:43,910 --> 00:00:46,813 or if it is actually really dark or actually really light 15 00:00:46,813 --> 00:00:51,317 without having to rely on just your eyes or just your monitor. 16 00:00:51,418 --> 00:00:53,019 So here in resolve, in the lower 17 00:00:53,019 --> 00:00:56,856 left hand corner behind our keyframes, we have our scopes. 18 00:00:56,923 --> 00:00:59,926 And if we click this little expand button 19 00:01:00,026 --> 00:01:03,697 that will bring up by default four of our scopes. 20 00:01:03,763 --> 00:01:06,766 Now, this might look really complicated, 21 00:01:06,833 --> 00:01:09,736 but the basic concepts here are actually pretty easy. 22 00:01:09,736 --> 00:01:11,071 Let's take a look. 23 00:01:11,071 --> 00:01:14,674 By default, we have four different color scopes inside of resolve 24 00:01:14,741 --> 00:01:17,610 the parade, the waveform, 25 00:01:17,610 --> 00:01:20,480 the vector scope and the histogram. 26 00:01:20,480 --> 00:01:22,949 And like I said, these are all just different ways 27 00:01:22,949 --> 00:01:27,787 of viewing what the colors in our image actually are, 28 00:01:27,887 --> 00:01:31,358 the one that I like to start out with is the waveform, 29 00:01:31,458 --> 00:01:35,662 and at its default settings it can be a little bit hard to explain. 30 00:01:35,729 --> 00:01:38,298 So I'm going to switch a couple of settings here. 31 00:01:38,298 --> 00:01:41,935 Under this little settings thing, I'm going to turn off colorize 32 00:01:42,002 --> 00:01:44,704 and I'm going to go up here and click on Y. 33 00:01:44,771 --> 00:01:45,372 What this is going to 34 00:01:45,372 --> 00:01:48,375 do is kind of take away some of the fancy things 35 00:01:48,475 --> 00:01:51,644 and just give us our very basic waveform scope. 36 00:01:51,745 --> 00:01:54,748 You see, what this is, is actually a graph. 37 00:01:54,881 --> 00:01:59,819 We have the x axis going down here and the Y axis going up and down, 38 00:01:59,886 --> 00:02:02,922 and the waveform is primarily a graph 39 00:02:02,922 --> 00:02:06,559 to figure out how bright things are down here at zero. 40 00:02:06,559 --> 00:02:10,163 This is like perfect black and up here 41 00:02:10,163 --> 00:02:14,100 at 1023, that's like perfect white. 42 00:02:14,167 --> 00:02:17,303 And everything in between is somewhere between the very darkest 43 00:02:17,303 --> 00:02:20,707 it could be and the very latest it could be. 44 00:02:20,774 --> 00:02:24,277 So that is the y axis, how bright things are. 45 00:02:24,377 --> 00:02:26,813 And on the x axis, 46 00:02:26,813 --> 00:02:30,417 this is where things are on screen horizontally. 47 00:02:30,483 --> 00:02:33,253 So something that's on the right side of the screen is going to be 48 00:02:33,253 --> 00:02:35,422 on the right side of the graph, something that's in 49 00:02:35,422 --> 00:02:37,157 the middle of the screen is going to be in the middle, 50 00:02:37,157 --> 00:02:40,160 and something that's on the left side is going to be on the left, 51 00:02:40,160 --> 00:02:43,797 but it doesn't track whether it's at the top or the bottom of the screen. 52 00:02:43,863 --> 00:02:47,167 It only tracks left and right and brightness. 53 00:02:47,233 --> 00:02:47,567 So the 54 00:02:47,567 --> 00:02:50,904 waveform scope is really just a graph of the brightness 55 00:02:50,904 --> 00:02:54,908 on the y axis and the horizontal position on the x axis. 56 00:02:54,974 --> 00:02:56,142 And what it's sort of doing 57 00:02:56,142 --> 00:03:00,246 is drawing a line to kind of represent what's in your image. 58 00:03:00,313 --> 00:03:03,583 So if we were to do kind of a simple version of this ourselves, 59 00:03:03,683 --> 00:03:05,285 we can look at it this way. 60 00:03:05,285 --> 00:03:08,788 If we were to start on the left and kind of make a graph 61 00:03:08,855 --> 00:03:13,526 of how bright things are right here, these are really dark. 62 00:03:13,526 --> 00:03:14,894 So let's make a little dot here. 63 00:03:14,894 --> 00:03:16,763 So these are really dark. 64 00:03:16,763 --> 00:03:19,933 Then let's see in this little column, it's still pretty dark. 65 00:03:20,033 --> 00:03:22,869 In this column, it's still pretty dark in this column, 66 00:03:22,869 --> 00:03:24,337 it's starting to get a little bit brighter. 67 00:03:24,337 --> 00:03:26,106 So maybe we'll put this up here. 68 00:03:26,106 --> 00:03:28,775 Then it's getting a little brighter still. 69 00:03:28,842 --> 00:03:30,844 Then it's getting even brighter. 70 00:03:30,844 --> 00:03:33,546 Ooh, now it's a little bit darker. 71 00:03:33,546 --> 00:03:35,882 And now it's a little brighter than it was. 72 00:03:35,882 --> 00:03:37,650 This is about the same. 73 00:03:37,650 --> 00:03:39,019 This is maybe about the same. 74 00:03:39,019 --> 00:03:41,021 Ooh, look, this right here is really bright. 75 00:03:41,021 --> 00:03:43,690 So maybe that's up here. 76 00:03:43,690 --> 00:03:45,992 This is maybe not so much. 77 00:03:45,992 --> 00:03:47,694 Not so much. 78 00:03:47,694 --> 00:03:50,230 And then we're kind of back down to where we were 79 00:03:50,230 --> 00:03:54,567 a little bit darker, a little bit darker, really, really dark. 80 00:03:54,634 --> 00:03:55,735 Really dark. 81 00:03:55,735 --> 00:04:01,875 Okay, So now we have this kind of line 82 00:04:01,975 --> 00:04:04,244 that graphs 83 00:04:04,244 --> 00:04:08,648 how light or dark things are in the image as you go across. 84 00:04:08,715 --> 00:04:11,384 And this is basically what a wave form does. 85 00:04:11,384 --> 00:04:14,788 So if we were to get rid of that image, we can still have quite a bit of data 86 00:04:14,788 --> 00:04:16,056 about what our image is. 87 00:04:16,056 --> 00:04:16,623 It's something 88 00:04:16,623 --> 00:04:18,892 that's kind of dark on the left and dark on the right, 89 00:04:18,892 --> 00:04:21,327 and it has something that's pretty bright in the middle. 90 00:04:21,327 --> 00:04:23,863 So you can kind of tell how things relate to each other, 91 00:04:23,863 --> 00:04:26,866 but you can also tell how bright or dark they are. 92 00:04:26,900 --> 00:04:30,370 This part up here, it's really bright, but maybe it's not the very brightest 93 00:04:30,370 --> 00:04:32,539 it could be. That's why it's right here. 94 00:04:32,539 --> 00:04:34,407 This is maybe not the very darkest it could be. 95 00:04:34,407 --> 00:04:36,209 So it's not all the way at the bottom. 96 00:04:36,209 --> 00:04:38,912 So this is a great tool if you're trying to figure out 97 00:04:38,912 --> 00:04:41,715 how bright or dark something is on screen, 98 00:04:41,715 --> 00:04:45,585 you can have sort of an idea of where an element is on the scope 99 00:04:45,585 --> 00:04:48,588 by whether it's on the left or the right side of the scope 100 00:04:48,788 --> 00:04:53,526 and how bright it is by how far up or down it is on the Y axis. 101 00:04:53,593 --> 00:04:56,296 So here we have a shot of our actress 102 00:04:56,396 --> 00:04:58,498 and it's really dark on the left side. 103 00:04:58,498 --> 00:05:01,301 Then about a third of the way in, it's really bright. 104 00:05:01,301 --> 00:05:03,770 And then it kind of gets dark here. 105 00:05:03,770 --> 00:05:06,773 So we would expect our waveform to show something like that. 106 00:05:07,007 --> 00:05:10,010 Here we have it really dark on the left 107 00:05:10,010 --> 00:05:12,779 and then things get bright about a third of the way in 108 00:05:12,779 --> 00:05:15,482 and then they go back dark again on this side. 109 00:05:15,482 --> 00:05:17,951 And then we see we have this little spike right here. 110 00:05:17,951 --> 00:05:20,954 That's this tree that's a little bit brighter right here. 111 00:05:21,021 --> 00:05:24,657 This little spike right here is this tree. 112 00:05:24,724 --> 00:05:26,760 So it's pretty easy to find something 113 00:05:26,760 --> 00:05:30,930 on the waveform based on kind of your guess on how bright it is 114 00:05:31,197 --> 00:05:34,868 and then where it is from left to right on the screen. 115 00:05:34,934 --> 00:05:38,738 This little patch right here is this kind of lighter bush right here. 116 00:05:38,838 --> 00:05:41,608 So if this makes sense, you've actually 117 00:05:41,608 --> 00:05:44,878 already learned not only the waveform but the parade. 118 00:05:44,944 --> 00:05:46,813 The parade 119 00:05:46,913 --> 00:05:47,881 is just three 120 00:05:47,881 --> 00:05:50,884 wave forms right next to each other. 121 00:05:51,117 --> 00:05:53,219 But it's only looking at the red pixels, 122 00:05:53,219 --> 00:05:56,189 the green pixels, and the blue pixels. 123 00:05:56,389 --> 00:05:59,392 So this is the brightness of the red channel. 124 00:05:59,392 --> 00:06:01,294 This is the brightness of the green channel, 125 00:06:01,294 --> 00:06:04,297 and this is the brightness of the blue channel. 126 00:06:04,397 --> 00:06:07,000 So what do I mean by red, green and blue channels? 127 00:06:07,000 --> 00:06:09,235 Well, everything on a screen, 128 00:06:09,235 --> 00:06:13,306 every pixel is made out of a set of red, green and blue lights. 129 00:06:13,306 --> 00:06:16,810 So each pixel actually has three little colors. 130 00:06:16,910 --> 00:06:20,347 And depending on how bright each channel is, that determines 131 00:06:20,347 --> 00:06:23,683 what color this actually looks like when you zoom out. 132 00:06:23,783 --> 00:06:26,686 If we zoom out here, we see this kind of turns white, 133 00:06:26,686 --> 00:06:30,290 equal parts red, green and blue makes white light. 134 00:06:30,357 --> 00:06:30,957 And same thing. 135 00:06:30,957 --> 00:06:32,659 If you had equal parts red, green and blue, 136 00:06:32,659 --> 00:06:36,129 but it was only like half brightness that would make something like gray. 137 00:06:36,229 --> 00:06:41,034 If you wanted to make blue, you would have no red, no green and full blue. 138 00:06:41,101 --> 00:06:43,970 That's going to give you this pure kind of blue color. 139 00:06:43,970 --> 00:06:45,472 And so any color that you see on 140 00:06:45,472 --> 00:06:48,641 screen is really just a mixture of red, green and blue. 141 00:06:48,742 --> 00:06:51,644 So here we have each of these channels split out 142 00:06:51,644 --> 00:06:56,449 so that you can kind of tell not only how bright something is, 143 00:06:56,549 --> 00:07:00,587 not only where it is on the screen, but roughly 144 00:07:00,587 --> 00:07:05,859 what kind of color is being shown by comparing these three channels. 145 00:07:05,925 --> 00:07:07,627 If we look just at these channels, 146 00:07:07,627 --> 00:07:09,863 we can see this bright part right here is her face. 147 00:07:09,863 --> 00:07:13,400 I know that because this is just a squished waveform like this. 148 00:07:13,466 --> 00:07:15,135 So this is the right side of the screen. 149 00:07:15,135 --> 00:07:17,037 This is the left side of the screen. 150 00:07:17,037 --> 00:07:19,873 And about a third of the way in is her face. 151 00:07:19,873 --> 00:07:22,842 And it's really bright. Okay, Well, it's really high. 152 00:07:22,842 --> 00:07:26,079 And the red channel and the second highest channel is blue. 153 00:07:26,146 --> 00:07:29,649 And if you put red and blue together and there's not a whole lot of green, 154 00:07:29,749 --> 00:07:31,451 it turns out to be magenta. 155 00:07:31,451 --> 00:07:34,988 So I could look just by looking at this scope that there's 156 00:07:34,988 --> 00:07:39,059 a lot of magenta in the image because we have a big red channel, 157 00:07:39,259 --> 00:07:42,495 a medium sized blue channel and a little baby green channel. 158 00:07:42,595 --> 00:07:43,897 Let's try this another way. 159 00:07:43,897 --> 00:07:45,899 I'm going to bring up another random shot. 160 00:07:45,899 --> 00:07:49,402 And just looking at the scope, we can tell a few different things. 161 00:07:49,469 --> 00:07:52,739 One is there's nothing that's really, really bright 162 00:07:52,872 --> 00:07:56,076 because there's nothing up here kind of in the 7000 range. 163 00:07:56,076 --> 00:07:58,244 Everything's kind of middle range. 164 00:07:58,244 --> 00:08:00,180 So there's nothing that's a really bright. 165 00:08:00,180 --> 00:08:01,948 There are some things that are a little bit darker 166 00:08:01,948 --> 00:08:04,784 because we do have some kind of darker data here 167 00:08:04,784 --> 00:08:08,088 and everything from left to right is very similar brightness. 168 00:08:08,088 --> 00:08:11,558 There's a lot of kind of the same color tones here. 169 00:08:11,658 --> 00:08:14,961 But what's interesting is the red channel is kind 170 00:08:14,961 --> 00:08:18,798 of the same all the way through this right side. 171 00:08:18,798 --> 00:08:23,269 The red is pretty high, followed by the blue and the green just under that, 172 00:08:23,269 --> 00:08:27,140 which means that it's probably again, it's sort of a magenta, 173 00:08:27,207 --> 00:08:30,877 but there's a little bit more green, so it's not going to be quite as strong. 174 00:08:30,977 --> 00:08:36,082 We also have this big spike up here and the green and blue channels, 175 00:08:36,149 --> 00:08:39,419 which means that there's something that's, oh, I don't know 176 00:08:39,419 --> 00:08:43,690 about a third of the way through the shot that doesn't have much red in it. 177 00:08:43,790 --> 00:08:45,725 And if you have a lot of blue and a lot of green 178 00:08:45,725 --> 00:08:48,561 and not a whole lot of red, you get sort of a cyan. 179 00:08:48,561 --> 00:08:52,732 So we're going to be looking at an image that isn't very bright, 180 00:08:52,799 --> 00:08:55,769 but there is some kind of subject here 181 00:08:55,769 --> 00:08:59,139 that is sort of a mid brightness cyan. 182 00:08:59,239 --> 00:09:02,008 And to the right of them is going to be kind of a deeper 183 00:09:02,008 --> 00:09:04,978 magenta, sort of more purple tone. 184 00:09:05,078 --> 00:09:08,014 And we could tell all of that just by looking at the scopes. 185 00:09:08,014 --> 00:09:11,818 So if I move this over, I can see we have our little puppet here. 186 00:09:11,885 --> 00:09:15,722 And of course he is sort of a mid brightness cyan, this kind of bluish. 187 00:09:15,922 --> 00:09:18,291 And then here we have the purple background. 188 00:09:18,291 --> 00:09:21,327 So you can really tell a lot just by looking at the scopes. 189 00:09:21,327 --> 00:09:24,297 And the more you practice, the more you look at a shot, 190 00:09:24,531 --> 00:09:26,599 the more you can kind of really learn about it. 191 00:09:26,599 --> 00:09:28,068 We can also do this the other way. 192 00:09:28,068 --> 00:09:31,137 I'll move our scope off here 193 00:09:31,204 --> 00:09:33,039 and go to Shot 74 here. 194 00:09:33,039 --> 00:09:34,274 We have a very dark shot. 195 00:09:34,274 --> 00:09:36,843 This is actually the beginning of a shot. 196 00:09:36,843 --> 00:09:38,511 But let's just start at the beginning. 197 00:09:38,511 --> 00:09:42,882 We have a really dark shot, so our scope is going to be mostly at the bottom. 198 00:09:42,982 --> 00:09:46,019 And then right here where this kind of white part is, it's 199 00:09:46,019 --> 00:09:49,055 going to be up a little bit and then it's going to go back down. 200 00:09:49,055 --> 00:09:50,323 So we're going to have 201 00:09:50,323 --> 00:09:52,926 mostly at the bottom, there's going to be a little spike here, 202 00:09:52,926 --> 00:09:57,297 a little spike here, bigger spike here and dark here. 203 00:09:57,497 --> 00:10:01,901 This spike is going to be mostly in the green and blue channels. 204 00:10:02,002 --> 00:10:05,171 This one and this one, we're going have a little red spike here. 205 00:10:05,271 --> 00:10:08,742 This one is going to be mostly equal except for a little bit higher. 206 00:10:08,742 --> 00:10:12,545 And the red channel. So let's take a look. 207 00:10:12,612 --> 00:10:15,615 So here we have it's dark all the way through, 208 00:10:15,782 --> 00:10:19,919 and then we have our little spike here, which is mostly in the green and blue. 209 00:10:19,919 --> 00:10:20,820 That's right. 210 00:10:20,820 --> 00:10:24,624 This one's going to be mostly in the green and blue. Yep. 211 00:10:24,691 --> 00:10:27,327 And then we have this spike which is here, 212 00:10:27,327 --> 00:10:30,497 and it's just a little bit high in the red channel. 213 00:10:30,530 --> 00:10:33,033 Looks like there's a little more blue than initially saw there. 214 00:10:33,033 --> 00:10:34,801 That's why you have the scopes, because I would have kind of 215 00:10:34,801 --> 00:10:38,605 guess this is more red, but it actually is a little bit more purple than I thought. 216 00:10:38,672 --> 00:10:43,176 So you can really tell a lot about your image by looking at the scopes. 217 00:10:43,243 --> 00:10:45,912 So that's the wave form and the parade. 19325

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