Table 1. Pristine sites with natural sky background brightness can be identified by measuring the sky background (astronomical unit mag/arcsec² in the visual range corresponds to a negative logarithmic scale of sky luminance) at modern astronomical observatories. Older observatories were built at dark sites close to cities. Today, these peri-urban sites are characterized by bright skies. Some observatories in the southwest of the USA were able to preserve relatively dark skies because of lighting ordinances (low pressure sodium lamps, full cut-off luminaires) in the nearby cities, resulting in a decrease of sky brightness in Flagstaff, Arizona since 1982 (Lockwood et al. 1990). The increase of the sky background depends on different model assumptions for several observatories (Garstang 1989). Indirect values can be derived from the increase of power consumption and lamp efficiency for street lighting.
| |
| |
| |
Period |
Sky brightness (mag/arcsec²) |
Annual increase (%) |
Cause |
References |
| |
|
Pristine |
|
|
|
|
|
|
Mt. Graham, AZ, USA |
2000 – 2008 |
21.5 – 21.8 |
0 |
solar activity |
Pedani 2009 |
|
Hawaii, USA |
1986 – 1996 |
21.3 – 21.9 |
0 |
solar activity |
Krisciunas 1997 |
|
Cerro Tololo/Chile |
1992 – 2006 |
22.0 – 21.2 |
0 |
solar activity |
Krisciunas et al. 2007 |
|
Kitt Peak/Mt. Hopkins, AZ, USA |
1988 – 1999 |
Δ 0.1 –
0.2 |
1 – 2 |
ordinances |
Massey and Foltz
2000 |
|
|
|
|
|
|
|
|
Urban |
|
|
|
|
|
|
Flagstaff, AZ |
1974 – 1982 |
Δ 0.4 |
5 |
|
Lockwood et al.
1990 |
|
IAO, India |
2003 – 2007 |
21.3 – 21.1 |
5 |
|
Stalin et al. 2008 |
|
Mt. Wilson, USA |
1973 – 1999 |
19.8 – 18.8 |
3.6 |
city lights Los
Angeles |
Teare 2000 |
|
|
1900 – 2000 |
Δ 2.7 |
2.5 |
city lights Los
Angeles |
Garstang 2004 |
|
Mt. Hamilton, CA, USA |
1950 – 1975 |
21.9 – 20.6 |
5 |
city lights |
Walker 1973 |
|
Ekar, Asiago, Italy |
1960 – 1995 |
21.6 – 20.2 |
10 |
city lights |
Cinzano 2000 |
|
G. Haro, Mexico |
1994 – 1997 |
20.5 – 20.0 |
19 |
city lights |
Carrasco et al.
1998 |
|
NAO, Japan |
1958/1978/1989 |
20.5/19.5/17.6 |
5 – 17 |
city lights Tokyo |
Isobe and Kosai
1998 |
|
|
|
|
|
|
|
|
Worldwide |
|
|
|
|
|
|
Expert guess |
|
|
3 |
|
Narisada and Schreuder
2004 |
|
|
|
|
|
|
|
|
Indirect (energy consumption) |
|
UK Campaign to Protect Rural England (CPRE) |
1993 – 2000 |
|
4 |
DMSP data |
CPRE 2003 |
|
UK McNeill |
1984 – 1999 |
1.86x lmh |
4.2 |
street light |
McNeill 1999 |
|
UK Fouquet/Pearson |
1950 – 2000 |
5x lmh |
3.3 |
overall energy consumption for
light |
Fouquet and Pearson
2006 |
|
USA |
1967 – 1970 |
|
20 |
energy +
efficiency |
Riegel 1973 |
|
France |
1990 – 2000 |
|
3 |
energy |
ADEME 2007 |
|
Germany |
1950 – 1990 |
|
8 |
energy +
efficiency |
Hänel 2001 |
|
|
|
|
|
|
|
|
| |
Note: IAO India = Indian Astronomical Observatory, NAO Japan = National Astronomical Observatory of Japan
|