SDO HMI 2012-10-16 23:59:00 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 94.41 | 518.48 | 49.53 | 272.17 | 7.47 | 229.54 | -19.23 | 83.73 | 0.3305 | -1058.6 | -431.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.05 | 0.00 | 0.53 | 4.07 | 235.14 | -13.63 | 96.29 | 0.2375 | -929.0 | -752.9 | |
| 0.00 | 1.13 | 0.00 | 0.59 | 6.30 | 232.23 | -16.54 | 87.11 | 0.2846 | -821.0 | -670.9 | |
| 0.00 | 3.49 | 0.00 | 1.81 | 7.36 | 231.63 | -17.14 | 83.55 | 0.2955 | -116.0 | -67.7 | |
| 77.22 | 425.11 | 40.36 | 222.25 | 7.37 | 230.11 | -18.66 | 83.86 | 0.3206 | -1597.5 | -424.9 | |
| 0.00 | 1.48 | 0.00 | 0.79 | 14.95 | 228.49 | -20.28 | 63.56 | 0.3757 | -846.0 | -634.0 | |
| 0.00 | 1.83 | 0.00 | 0.98 | 15.42 | 228.01 | -20.76 | 62.89 | 0.3855 | -796.0 | -659.1 | |
| 6.72 | 12.65 | 3.54 | 6.67 | 5.08 | 228.54 | -20.23 | 90.82 | 0.3460 | -1051.4 | -813.1 | |
| 0.00 | 2.97 | 0.00 | 1.57 | 8.24 | 228.21 | -20.56 | 81.76 | 0.3527 | -618.0 | -530.3 | |
| 0.00 | 1.40 | 0.00 | 0.74 | 9.96 | 227.88 | -20.89 | 77.08 | 0.3619 | -827.0 | -583.1 | |
| 0.00 | 0.96 | 0.00 | 0.51 | 6.70 | 227.96 | -20.81 | 86.15 | 0.3552 | 591.0 | 380.1 | |
| 0.00 | 1.40 | 0.00 | 0.74 | 11.00 | 227.55 | -21.22 | 74.46 | 0.3704 | -750.0 | -544.9 | |
| 0.00 | 1.05 | 0.00 | 0.56 | 3.68 | 227.87 | -20.90 | 94.64 | 0.3587 | -742.0 | -500.7 | |
| 0.00 | 1.92 | 0.00 | 1.02 | 7.20 | 227.68 | -21.09 | 84.78 | 0.3600 | -821.0 | -617.5 | |
| 0.00 | 0.79 | 0.00 | 0.42 | 14.73 | 227.12 | -21.65 | 65.39 | 0.3942 | -768.0 | -610.0 | |
| 0.00 | 1.05 | 0.00 | 0.57 | 15.69 | 227.02 | -21.75 | 63.21 | 0.4014 | -524.0 | -418.2 | |
| 2.53 | 10.99 | 1.35 | 5.85 | 9.65 | 227.48 | -21.29 | 78.11 | 0.3674 | -881.6 | -702.7 | |
| 0.00 | 1.13 | 0.00 | 0.60 | 8.54 | 227.38 | -21.39 | 81.16 | 0.3665 | -572.0 | -386.5 | |
| 2.79 | 13.96 | 1.49 | 7.43 | 6.71 | 227.28 | -21.49 | 86.18 | 0.3662 | -994.6 | -865.4 | |
| 2.79 | 9.60 | 1.49 | 5.11 | 6.26 | 227.14 | -21.63 | 87.43 | 0.3683 | -1087.6 | -700.6 | |
| 0.00 | 1.92 | 0.00 | 1.02 | 7.15 | 227.00 | -21.77 | 85.01 | 0.3709 | -840.0 | -713.3 | |
| 1.05 | 1.48 | 0.56 | 0.79 | 6.10 | 226.95 | -21.82 | 87.85 | 0.3714 | -757.8 | -727.4 | |
| 0.00 | 1.13 | 0.00 | 0.61 | 8.34 | 226.84 | -21.93 | 81.84 | 0.3749 | 798.0 | 662.1 | |
| 0.00 | 1.05 | 0.00 | 0.56 | 4.28 | 226.99 | -21.78 | 92.77 | 0.3721 | -823.0 | -620.1 | |
| 0.00 | 1.13 | 0.00 | 0.61 | 6.84 | 226.82 | -21.95 | 85.85 | 0.3737 | -697.0 | -550.8 | |
| 0.00 | 0.79 | 0.00 | 0.42 | 6.18 | 226.79 | -21.98 | 87.62 | 0.3741 | -809.0 | -656.4 | |
| 0.00 | 1.05 | 0.00 | 0.56 | 9.10 | 226.41 | -22.36 | 79.96 | 0.3832 | 1098.0 | 970.8 | |
| 0.00 | 2.88 | 0.00 | 1.54 | 7.87 | 226.32 | -22.45 | 83.19 | 0.3827 | -632.0 | -450.6 | |
| 0.00 | 1.57 | 0.00 | 0.87 | 18.16 | 225.01 | -23.76 | 59.73 | 0.4452 | -873.0 | -591.8 | |
| 0.00 | 1.48 | 0.00 | 0.80 | 8.99 | 225.76 | -23.01 | 80.45 | 0.3933 | 946.0 | 743.5 | |
| 0.00 | 0.96 | 0.00 | 0.52 | 7.42 | 225.42 | -23.35 | 84.49 | 0.3965 | -790.0 | -700.6 | |
| 0.00 | 1.31 | 0.00 | 0.73 | 18.10 | 224.29 | -24.48 | 60.48 | 0.4545 | -785.0 | -551.9 | |
| 0.00 | 1.31 | 0.00 | 0.72 | 6.08 | 223.35 | -25.42 | 87.85 | 0.4290 | 857.0 | 642.7 | |
| 0.00 | 2.44 | 0.00 | 1.36 | 7.27 | 221.16 | -27.61 | 85.21 | 0.4633 | 842.0 | 665.6 | |
| 1.31 | 2.27 | 0.74 | 1.28 | 7.76 | 220.06 | -28.71 | 84.25 | 0.4803 | 690.4 | 697.3 | |
| 0.00 | 1.75 | 0.00 | 1.04 | 7.00 | 214.93 | -33.84 | 85.95 | 0.5562 | 581.0 | 388.7 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |