| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.20 | 192.01 | 20.30 | 110.76 | 18.67 | 102.75 | 24.92 | 308.74 | 0.5137 | -299.6 | -246.6 | |
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back to the solar disc SDO HMI 2011-12-07 16:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.82 | 10.91 | 3.92 | 6.28 | 16.97 | 103.72 | 25.89 | 304.81 | 0.5108 | 838.5 | 480.2 | |
| 21.99 | 141.90 | 12.75 | 82.37 | 18.77 | 103.52 | 25.69 | 307.97 | 0.5228 | -1282.7 | -361.3 | |
| 1.53 | 2.73 | 0.87 | 1.55 | 17.52 | 101.96 | 24.13 | 307.55 | 0.4937 | 837.6 | 627.0 | |
| 0.00 | 1.28 | 0.00 | 0.73 | 19.02 | 102.01 | 24.18 | 309.95 | 0.5073 | -674.0 | -628.9 | |
| 0.00 | 1.19 | 0.00 | 0.68 | 17.55 | 101.52 | 23.69 | 308.08 | 0.4887 | 830.0 | 605.0 | |
| 4.86 | 17.81 | 2.76 | 10.12 | 18.27 | 101.42 | 23.59 | 309.39 | 0.4937 | -997.4 | -307.4 | |
| 0.00 | 0.85 | 0.00 | 0.49 | 19.33 | 101.20 | 23.37 | 311.36 | 0.5008 | 561.0 | 466.1 | |
| 0.00 | 1.79 | 0.00 | 1.02 | 19.39 | 101.04 | 23.21 | 311.64 | 0.4996 | 768.0 | 616.7 | |
| 0.00 | 1.62 | 0.00 | 0.91 | 17.86 | 100.18 | 22.35 | 310.15 | 0.4755 | 638.0 | 521.7 | |
| 0.00 | 2.47 | 0.00 | 1.37 | 16.35 | 99.39 | 21.56 | 308.45 | 0.4523 | 811.0 | 632.1 | |
| 0.00 | 1.11 | 0.00 | 0.62 | 18.49 | 99.56 | 21.73 | 311.95 | 0.4741 | 663.0 | 523.8 | |
| 0.00 | 1.79 | 0.00 | 0.99 | 19.11 | 97.17 | 19.35 | 316.16 | 0.4538 | 733.0 | 643.3 | |
| 0.00 | 1.28 | 0.00 | 0.72 | 22.01 | 96.01 | 18.18 | 322.22 | 0.4743 | 616.0 | 401.0 | |
| 0.00 | 1.62 | 0.00 | 0.91 | 21.66 | 95.87 | 18.04 | 321.95 | 0.4688 | 729.0 | 520.5 | |
| 0.00 | 1.28 | 0.00 | 0.71 | 22.87 | 92.62 | 14.79 | 328.72 | 0.4550 | 703.0 | 502.4 | |
| 0.00 | 1.02 | 0.00 | 0.55 | 19.96 | 88.74 | 10.92 | 332.35 | 0.3852 | -433.0 | -465.2 | |
| 0.00 | 1.36 | 0.00 | 0.74 | 22.30 | 88.34 | 10.51 | 335.94 | 0.4157 | -829.0 | -560.2 | |
| 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. | |