Table 6.
Filter | Effective wavelength | Red | Green | Blue | |||
---|---|---|---|---|---|---|---|
±HWHM (nm) | β [10−3/C] | β [10−3/C] | β [10−3/C] | ||||
L0 | 530±90 | 0.202±0.0056 | 1.08±0.05 | 0.24±0.0058 | 0.18±0.06 | 0.273±0.006 | 0±0.1b |
L1 | 800±9 | 0.0665±0.0019 | 2.24±0.05 | 0.0443±0.0013 | 1.86±0.05 | 0.0425±0.0013 | 0±0.06b |
L2 | 754±10 | 0.0925±0.001 | 1.83±0.05 | 0.03±0.001 | 1.68±0.07 | 0.000719±0.001 | 0.00±0.05b |
L3 | 677±11 | 0.16±0.0007 | 1.76±0.05 | 0.0109±0.00068 | 0.18±0.05 | 0.00275±0.00067 | 0.00±0.05b |
L4 | 605±9 | 0.217±0.00049 | 0.75±0.05 | 0.0621±0.0005 | 2.57±0.05 | 0.00106±0.0005 | 0.00±0.05b |
L5 | 528±11 | 0.0111±0.00028 | 0.54±0.05 | 0.264±0.00028 | 0±0.05b | 0.1±0.00028 | 1.28±0.05 |
L6 | 442±12 | 0.0047±0.00013 | 0.00±0.05 | 0.0175±0.00014 | 0±0.05b | 0.256±0.00013 | −1±0.5 |
L7c | 590±88 | 1.97e-07±1.52e-08 | 0.85±0.10 | 1.44e-07±4.01e-08 | 0.89±0.50 | 1.31e-07±2.84e-08 | 0.85±0.50 |
R0 | 530±90 | 0.196±0.0056 | 1.08±0.05 | 0.226±0.0059 | 0.18±0.06 | 0.267±0.0059 | 0.0±0.1b |
R1 | 800±9 | 0.0668±0.0017 | 2.24±0.05 | 0.0437±0.0011 | 1.86±0.05 | 0.042±0.0011 | 0.00±0.06 |
R2 | 866±10 | 0.0364±0.0021 | 3.01±0.05 | 0.0352±0.00063 | 2.88±0.05 | 0.0352±0.00019 | 2.96±0.05 |
R3 | 910±12 | 0.0231±0.0031 | 3.56±0.05 | 0.0229±0.00016 | 3.51±0.05 | 0.0227±0.00025 | 3.53±0.05 |
R4 | 939±12 | 0.0155±0.0057 | 4.19±0.05 | 0.0156±0.0012 | 4.2±0.05 | 0.0155±0.00057 | 4.18±0.05 |
R5 | 978±10 | 0.00825±0.00015 | 5.56±0.05 | 0.00835±0.0053 | 5.45±0.05 | 0.00819±0.002 | 5.46±0.05 |
R6 | 1022±19 | 0.00429±0.00022 | 7.43±0.05 | 0.00439±0.00077 | 7.47±0.05 | 0.00432±0.0063 | 7.45±0.05 |
R7c | 880±10 | 2.57e-07±2.43e-08 | 3.40±0.50 | 2.57e-07±4.20e-08 | 3.20±0.50 | 2.50e-07±3.10e-08 | 3.30±0.50 |
aThe reported here are the peak response, which must be multiplied by the peak normalized to obtain
bThese β coefficients are set to zero because of large relative uncertainties
cTo derive solar filter radiometric coefficients, the vendor provided spectral profile were used