| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65.08 | 335.15 | 33.28 | 172.08 | 14.18 | 251.91 | -8.77 | 34.24 | 0.2614 | -707.0 | -370.6 | |
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back to the solar disc SDO HMI 2011-11-23 19:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.54 | 0.00 | 0.78 | 11.80 | 256.73 | -3.95 | 21.31 | 0.1864 | -901.0 | -703.7 | |
| 48.81 | 286.86 | 24.95 | 146.69 | 13.84 | 252.71 | -7.97 | 32.90 | 0.2489 | -1377.1 | -432.9 | |
| 0.00 | 5.74 | 0.00 | 2.96 | 15.41 | 252.16 | -8.52 | 31.31 | 0.2761 | -962.0 | -803.3 | |
| 16.27 | -2.00 | 8.33 | -2.00 | 13.78 | 252.07 | -8.61 | 35.09 | 0.2541 | -1109.5 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.57 | 15.29 | 251.76 | -8.92 | 32.72 | 0.2779 | -822.0 | -708.2 | |
| 0.00 | 1.71 | 0.00 | 0.87 | 12.57 | 251.74 | -8.94 | 39.14 | 0.2413 | -1086.0 | -781.5 | |
| 0.00 | 1.46 | 0.00 | 0.75 | 15.08 | 251.18 | -9.50 | 34.81 | 0.2804 | -878.0 | -694.8 | |
| 0.00 | 1.37 | 0.00 | 0.72 | 18.44 | 250.91 | -9.77 | 29.36 | 0.3296 | -867.0 | -657.1 | |
| 0.00 | 2.14 | 0.00 | 1.10 | 13.65 | 251.11 | -9.56 | 38.23 | 0.2620 | -854.0 | -728.0 | |
| 0.00 | 7.28 | 0.00 | 3.76 | 15.04 | 250.74 | -9.93 | 36.07 | 0.2842 | -743.0 | -700.4 | |
| 0.00 | 2.65 | 0.00 | 1.37 | 14.50 | 250.64 | -10.03 | 37.55 | 0.2779 | -1157.0 | -856.2 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 20.18 | 249.94 | -10.74 | 29.04 | 0.3618 | -883.0 | -746.8 | |
| 0.00 | 0.94 | 0.00 | 0.48 | 12.95 | 249.91 | -10.77 | 43.33 | 0.2665 | 849.0 | 635.3 | |
| 0.00 | 3.17 | 0.00 | 1.64 | 13.09 | 248.23 | -12.45 | 47.03 | 0.2882 | 1035.0 | 841.6 | |
| 0.00 | 0.77 | 0.00 | 0.41 | 16.98 | 247.65 | -13.03 | 39.49 | 0.3406 | 811.0 | 727.3 | |
| 0.00 | 1.20 | 0.00 | 0.64 | 17.42 | 245.34 | -15.33 | 43.12 | 0.3708 | 795.0 | 627.6 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 18.81 | 245.15 | -15.52 | 40.88 | 0.3888 | 826.0 | 743.7 | |
| 0.00 | 1.03 | 0.00 | 0.55 | 16.80 | 245.10 | -15.57 | 44.76 | 0.3666 | 732.0 | 548.9 | |
| 0.00 | 1.46 | 0.00 | 0.78 | 17.54 | 244.91 | -15.76 | 43.65 | 0.3769 | 768.0 | 635.4 | |
| 0.00 | 2.14 | 0.00 | 1.16 | 19.05 | 244.35 | -16.33 | 41.84 | 0.4002 | 616.0 | 573.6 | |
| 0.00 | 1.28 | 0.00 | 0.70 | 19.33 | 244.19 | -16.49 | 41.61 | 0.4050 | 737.0 | 610.9 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 17.84 | 243.95 | -16.73 | 44.72 | 0.3911 | 791.0 | 674.3 | |
| 0.00 | 0.69 | 0.00 | 0.37 | 19.10 | 243.16 | -17.51 | 43.67 | 0.4136 | 728.0 | 597.1 | |
| 0.00 | 0.86 | 0.00 | 0.47 | 18.16 | 242.28 | -18.40 | 46.72 | 0.4137 | 799.0 | 612.5 | |
| 0.00 | 4.02 | 0.00 | 2.20 | 19.31 | 242.05 | -18.63 | 44.99 | 0.4282 | 512.0 | 581.9 | |
| 0.00 | 1.28 | 0.00 | 0.70 | 18.84 | 241.81 | -18.87 | 46.17 | 0.4261 | 743.0 | 521.3 | |
| 0.00 | 1.63 | 0.00 | 0.89 | 19.02 | 241.42 | -19.25 | 46.40 | 0.4323 | 809.0 | 556.3 | |
| 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. | |