SDO HMI 2011-11-23 00:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 55.27 | 356.76 | 29.51 | 191.12 | 14.18 | 252.12 | -18.98 | 55.82 | 0.3825 | -548.9 | -427.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.20 | 0.00 | 0.64 | 18.24 | 257.36 | -13.74 | 38.70 | 0.3624 | -849.0 | -752.4 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 12.17 | 255.53 | -15.56 | 55.72 | 0.3188 | -788.0 | -687.9 | |
| 0.00 | 1.37 | 0.00 | 0.73 | 16.16 | 254.22 | -16.87 | 48.46 | 0.3741 | 780.0 | 651.7 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 16.86 | 253.28 | -17.81 | 48.52 | 0.3925 | -696.0 | -529.2 | |
| 35.65 | 277.40 | 18.99 | 147.84 | 13.87 | 252.87 | -18.22 | 55.56 | 0.3698 | -1386.8 | -508.3 | |
| 1.11 | 5.83 | 0.60 | 3.13 | 15.26 | 252.17 | -18.93 | 53.45 | 0.3912 | -784.6 | -728.6 | |
| 7.54 | -5.00 | 4.04 | -5.00 | 14.07 | 252.24 | -18.85 | 55.94 | 0.3800 | -913.8 | 999999 | |
| 1.97 | 2.83 | 1.06 | 1.52 | 14.80 | 252.18 | -18.92 | 54.42 | 0.3871 | -844.1 | -706.8 | |
| 7.03 | -5.00 | 3.76 | -5.00 | 13.68 | 252.18 | -18.92 | 56.92 | 0.3775 | -1065.8 | 999999 | |
| 1.97 | 2.57 | 1.06 | 1.39 | 15.71 | 251.80 | -19.29 | 52.99 | 0.4001 | 541.3 | 213.6 | |
| 0.00 | 2.06 | 0.00 | 1.10 | 12.56 | 251.76 | -19.34 | 60.08 | 0.3746 | -865.0 | -743.1 | |
| 0.00 | 16.03 | 0.00 | 8.65 | 15.22 | 251.46 | -19.64 | 54.48 | 0.4002 | -883.0 | -554.8 | |
| 0.00 | 1.29 | 0.00 | 0.69 | 12.77 | 251.61 | -19.48 | 59.76 | 0.3782 | -1027.0 | -854.5 | |
| 0.00 | 2.57 | 0.00 | 1.38 | 13.43 | 251.56 | -19.54 | 58.29 | 0.3841 | -477.0 | -287.1 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 12.67 | 251.49 | -19.61 | 60.12 | 0.3792 | -640.0 | -529.8 | |
| 0.00 | 6.77 | 0.00 | 3.64 | 13.73 | 251.21 | -19.89 | 58.04 | 0.3912 | -700.0 | -661.5 | |
| 0.00 | 1.37 | 0.00 | 0.74 | 14.09 | 250.98 | -20.12 | 57.52 | 0.3972 | -731.0 | -521.0 | |
| 0.00 | 1.97 | 0.00 | 1.07 | 14.51 | 250.75 | -20.35 | 56.88 | 0.4037 | -681.0 | -564.8 | |
| 0.00 | 1.37 | 0.00 | 0.74 | 14.36 | 250.73 | -20.37 | 57.23 | 0.4027 | -812.0 | -626.9 | |
| 0.00 | 5.66 | 0.00 | 3.07 | 14.78 | 250.62 | -20.48 | 56.45 | 0.4076 | -115.0 | -394.2 | |
| 0.00 | 3.51 | 0.00 | 1.91 | 13.89 | 249.79 | -21.31 | 59.32 | 0.4119 | 801.0 | 675.2 | |
| 0.00 | 1.71 | 0.00 | 0.93 | 14.41 | 249.58 | -21.52 | 58.46 | 0.4187 | 523.0 | 466.9 | |
| 0.00 | 0.86 | 0.00 | 0.48 | 17.88 | 249.11 | -21.99 | 52.14 | 0.4533 | -758.0 | -632.1 | |
| 0.00 | 1.03 | 0.00 | 0.57 | 15.91 | 247.95 | -23.15 | 57.17 | 0.4518 | 794.0 | 708.9 | |
| 0.00 | 1.71 | 0.00 | 0.95 | 15.48 | 247.97 | -23.13 | 57.99 | 0.4484 | 935.0 | 772.3 | |
| 0.00 | 1.63 | 0.00 | 0.90 | 15.82 | 247.93 | -23.17 | 57.37 | 0.4514 | 766.0 | 534.2 | |
| 0.00 | 0.77 | 0.00 | 0.43 | 15.66 | 247.91 | -23.19 | 57.69 | 0.4505 | 869.0 | 652.8 | |
| 0.00 | 1.03 | 0.00 | 0.57 | 16.82 | 247.70 | -23.40 | 55.69 | 0.4622 | 622.0 | 449.6 | |
| 0.00 | 1.46 | 0.00 | 0.82 | 16.64 | 245.82 | -25.28 | 57.88 | 0.4850 | 837.0 | 624.1 | |
| 0.00 | 1.11 | 0.00 | 0.64 | 17.65 | 245.22 | -25.87 | 56.63 | 0.5000 | 823.0 | 651.5 | |
| 0.00 | 2.06 | 0.00 | 1.17 | 17.43 | 245.12 | -25.98 | 57.10 | 0.4997 | 820.0 | 637.6 | |
| 0.00 | 1.54 | 0.00 | 0.88 | 16.93 | 244.54 | -26.56 | 58.51 | 0.5037 | 743.0 | 563.1 | |
| 0.00 | 1.11 | 0.00 | 0.65 | 18.78 | 244.17 | -26.93 | 55.65 | 0.5215 | 846.0 | 650.9 | |
| 0.00 | 0.86 | 0.00 | 0.50 | 19.73 | 243.82 | -27.28 | 54.38 | 0.5328 | 572.0 | 489.3 | |
| 0.00 | 1.03 | 0.00 | 0.60 | 18.73 | 242.84 | -28.26 | 56.88 | 0.5376 | 734.0 | 635.4 | |
| 0.00 | 1.63 | 0.00 | 0.96 | 18.37 | 242.01 | -29.09 | 58.13 | 0.5454 | 717.0 | 529.8 | |
| 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. | |