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1 The Director of Photography – an overview

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Lighting ratios 109<br />

Figure 11.3 <strong>The</strong> r<strong>an</strong>ge <strong>of</strong><br />

lighting ratios that c<strong>an</strong> be<br />

shown on different systems<br />

Tape Tr<strong>an</strong>sfer Image Brightness<br />

Brightness Ratio 32:1<br />

Cinema Release Print<br />

Television Low Key Scene<br />

Television “Normal” Scene<br />

Television High Key Scene<br />

Print Density <strong>–</strong> Image brightness Ratio 128:1<br />

Lighting ratios when shooting for both cinema<br />

<strong>an</strong>d television<br />

<strong>The</strong> way films are funded these days, with <strong>of</strong>ten a signific<strong>an</strong>t amount <strong>of</strong><br />

the production’s capitalization coming up front from television rights<br />

<strong>an</strong>d video sell-throughs, it is import<strong>an</strong>t that the cinematographer<br />

knows when shooting a scene exactly how it will look when delivered<br />

on the two, quite different, media. <strong>The</strong> key to this is the lighting ratio.<br />

<strong>The</strong> first thing to realize is that the tonal r<strong>an</strong>ge <strong>of</strong> the television version<br />

is going to have to come from within the tonal r<strong>an</strong>ge <strong>of</strong> the cinema<br />

version.This is mainly because the television version will be, most<br />

<strong>of</strong>ten, telecined from the cinema print. This, in these circumst<strong>an</strong>ces, is<br />

not necessarily a disadv<strong>an</strong>tage. You have probably put considerable<br />

effort into grading the cinema copy <strong>an</strong>d, therefore, much <strong>of</strong> your grading<br />

for television, say the overall brightness <strong>an</strong>d colour, will have<br />

already been achieved.<br />

At the telecine grading <strong>of</strong> your cinema print you must remember<br />

that you don’t have to take your 32:1 television version from the middle<br />

<strong>of</strong> the 128:1 cinema version. For <strong>an</strong> absolutely normal daylight<br />

scene this may well be appropriate, but for a high-key or low-key scene<br />

or a night exterior scene or snowscape it would be inappropriate.<br />

Figure 11.3 shows the sensitometric curve for a typical cinema release<br />

print.<strong>The</strong> straight-line section has a box overlaid on it, representing the<br />

seven-stop exposure r<strong>an</strong>ge that would result in a first-class image on the<br />

cinema screen. Inside this box is <strong>an</strong>other, showing the centre section<br />

that would be used to make a normal tr<strong>an</strong>sfer from this print to a videotape.<br />

As is clear, the equivalent <strong>of</strong> one stop <strong>of</strong> information in the highlights<br />

together with <strong>an</strong>other stop <strong>of</strong> information in the shadows will not<br />

be tr<strong>an</strong>sferred <strong>an</strong>d will be totally lost to the television audience.<br />

By comparing the 128:1 tonal r<strong>an</strong>ge <strong>of</strong> the release print shown at the<br />

bottom <strong>of</strong> the print with the 32:1 tonal r<strong>an</strong>ge <strong>of</strong> the video tr<strong>an</strong>sfer<br />

shown at the side <strong>of</strong> Figure 11.3, you c<strong>an</strong> see a very graphic demonstration<br />

<strong>of</strong> how the r<strong>an</strong>ge is dramatically reduced.<br />

Just below the curve is a box showing how one might tr<strong>an</strong>sfer a lowkey,<br />

or night, scene to tape. In this kind <strong>of</strong> scene it is the shadows that<br />

contain most <strong>of</strong> the information the cinematographer wishes to show

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