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Outdoor Lighting and Crime - Amper

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2000). Regardless, there are often inexplicably large differences between countries in specific<br />

crime rates, eg homicide (Graycar 2001).<br />

The following sections present within-country comparisons of available lighting <strong>and</strong> crime<br />

growth data.<br />

2.3 GROWTH IN LIGHTING AND CRIME IN INDIVIDUAL<br />

COUNTRIES<br />

2.3.1 Australia<br />

Despite substantial effort, the writer did not find suitable records of energy use for outdoor<br />

lighting in Australia <strong>and</strong> the proportions of various lamp types installed. The same applies to<br />

records of illumination levels or total light output, so recourse has been had to astronomical<br />

observations.<br />

For the period 1880 to 2001, artificial skyglow values shown in Figure 1 (all of the figures are<br />

grouped at the end of this document) have been inferred from limiting unaided visual stellar<br />

magnitudes assembled by the writer from observations in recent decades from Melbourne<br />

suburbs plus a few more as far back as the mid-1950s (reported in Dudley 2000).<br />

Fluctuations must have taken place during social upheavals such as the Great Depression <strong>and</strong><br />

the two World Wars, especially WW2 because a blackout was enforced, 13 but they are not<br />

shown because of the absence of specific data for the years in question. The skyglow changes<br />

caused by population changes at those times were small in the USA (Garstang 2000), but<br />

social, economic <strong>and</strong> technological effects on skyglow could well be larger than the<br />

population effects. The sky reference area chosen for skyglow observations <strong>and</strong> calculations<br />

is at 45 degrees altitude, due south of an observing site about 11 km northeast of the<br />

Melbourne central business district. The zenith might have been a better reference position,<br />

but this is relatively unimportant for the present purpose.<br />

The pre-electric-lighting ordinate of the skyglow curve in Figure 1 is 0.27 mcd/m 2 , typical of<br />

the luminance of the natural clear moonless night sky. For the luminance of the Melbourne<br />

sky to start at that value <strong>and</strong> to be where it is now <strong>and</strong> where it has been in recent decades is<br />

most readily explained if the growth rate of the artificial component is taken as exponential.<br />

The observed increase is close to doubling in each decade. 14 To sufficient accuracy for the<br />

present purpose, the skyglow luminance S mcd/m 2 is given by<br />

S = 0.27 + 0.00189*2^((year-1880)/10).<br />

13 The writer recalls the household stress of this as a child.<br />

14 The writer’s original analysis of Melbourne skyglow observations was done in 1999<br />

because skyglow was interfering with measurements of astronomical performance of image<br />

intensifiers. At that time, the writer was unaware that prior results elsewhere showed<br />

exponential growth; yet another case of ‘reinventing the wheel’. Regardless, this finding does<br />

add a little more weight to the realisation that growth in light pollution represents a global<br />

problem in sustainability.<br />

10

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