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. 2012 Dec;78(24):8849–8853. doi: 10.1128/AEM.02527-12

Table 2.

Environmental conditions used for Mars simulation experiments

Parameter Value
Avg pressure (kPa) ± SD 0.69 ± 0.01
Avg temp (°C) ± SD −10 ± 2
Avg relative humidity (%) ± SD 8 ± 2
UV-Vis-NIR radiationa fluence rate, kJ m−2 h−1 (total applied fluence)a
    Total UV (200–400 nm) 142.9 (1.14 MJ m−2)
    UV-C (200–280 nm) 14.4 kJ (115 kJ m−2)
    UV-B (280–320 nm) 24.8 kJ (199 kJ m−2)
    UV-A (320–400 nm) 103.7 kJ (829 kJ m−2)
    Vis (400–700 nm) 864.0 kJ (6.91 MJ m−2)
    NIR (700–1,100 nm) 882.0 kJ (7.05 MJ m−2)
    Total irradiance (200–1,100 nm) 1,888.9 (15.1 MJ m−2)
Time (h) 24b
% CO2 99.99
a

Details of the radiation dosimetry, fluence rates, and simulation of the UV-Vis-NIR radiation environment of the surface conditions on Mars have been described by Schuerger et al. (3840). Vis, visible; NIR, near IR.

b

With or without 8 h of irradiance.