| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.57 | 129.48 | 20.06 | 67.26 | 20.04 | 97.60 | 10.79 | 324.23 | 0.3032 | -78.8 | -142.2 | |
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back to the solar disc SDO HMI 2011-10-13 09:59:02 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.14 | 0.00 | 0.59 | 20.09 | 99.05 | 12.25 | 320.95 | 0.3176 | -658.0 | -506.4 | |
| 9.54 | 66.66 | 4.96 | 34.63 | 19.39 | 98.61 | 11.80 | 320.44 | 0.3043 | -1125.0 | -603.9 | |
| 4.11 | 9.45 | 2.14 | 4.92 | 20.10 | 98.56 | 11.76 | 322.07 | 0.3127 | -896.1 | -677.5 | |
| 1.14 | -2.00 | 0.59 | -2.00 | 19.11 | 98.49 | 11.69 | 320.09 | 0.2996 | -1029.2 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.59 | 20.32 | 98.35 | 11.55 | 323.01 | 0.3134 | -678.0 | -492.5 | |
| 6.47 | -2.00 | 3.36 | -2.00 | 19.27 | 98.21 | 11.41 | 321.11 | 0.2987 | -1175.2 | 999999 | |
| 0.00 | 3.24 | 0.00 | 1.68 | 19.38 | 97.70 | 10.90 | 322.57 | 0.2947 | -290.0 | -344.6 | |
| 0.00 | 2.62 | 0.00 | 1.37 | 21.25 | 96.72 | 9.92 | 328.72 | 0.3107 | 848.0 | 565.7 | |
| 5.16 | 43.13 | 2.69 | 22.40 | 21.25 | 96.43 | 9.63 | 329.47 | 0.3082 | 863.4 | 767.8 | |
| 3.41 | -9.00 | 1.77 | -9.00 | 20.64 | 96.10 | 9.30 | 329.23 | 0.2968 | 932.3 | 999999 | |
| 7.17 | -9.00 | 3.73 | -9.00 | 21.10 | 96.03 | 9.23 | 330.24 | 0.3028 | 1125.6 | 999999 | |
| 1.57 | -9.00 | 0.82 | -9.00 | 21.11 | 95.80 | 9.00 | 330.85 | 0.3010 | 966.9 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.54 | 20.64 | 95.74 | 8.94 | 330.19 | 0.2939 | 884.0 | 712.0 | |
| 0.00 | 1.05 | 0.00 | 0.54 | 20.92 | 95.70 | 8.89 | 330.82 | 0.2975 | 929.0 | 777.7 | |
| 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. | |