| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.82 | 166.71 | 18.71 | 95.15 | 18.52 | 103.24 | 23.75 | 309.62 | 0.4978 | -385.7 | -240.7 | |
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back to the solar disc SDO HMI 2011-12-07 13:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.03 | 8.27 | 2.85 | 4.69 | 17.07 | 103.58 | 24.10 | 306.79 | 0.4895 | 830.9 | 541.3 | |
| 23.36 | 131.95 | 13.37 | 75.59 | 18.77 | 103.53 | 24.04 | 309.70 | 0.5034 | -1280.2 | -365.9 | |
| 0.00 | 4.01 | 0.00 | 2.27 | 17.37 | 103.26 | 23.77 | 307.68 | 0.4881 | 657.0 | 468.3 | |
| 0.00 | 0.85 | 0.00 | 0.48 | 17.96 | 102.26 | 22.77 | 309.81 | 0.4813 | -454.0 | -339.1 | |
| 0.00 | 2.30 | 0.00 | 1.29 | 17.44 | 101.98 | 22.50 | 309.23 | 0.4733 | 935.0 | 790.2 | |
| 0.00 | 1.36 | 0.00 | 0.77 | 19.02 | 102.17 | 22.69 | 311.66 | 0.4901 | -707.0 | -519.2 | |
| 0.00 | 1.02 | 0.00 | 0.57 | 15.01 | 101.39 | 21.91 | 305.53 | 0.4448 | 821.0 | 632.6 | |
| 0.00 | 1.45 | 0.00 | 0.81 | 17.50 | 101.59 | 22.11 | 309.81 | 0.4692 | 808.0 | 700.1 | |
| 0.00 | 1.02 | 0.00 | 0.58 | 18.46 | 101.68 | 22.20 | 311.32 | 0.4792 | -835.0 | -625.4 | |
| 4.43 | 9.55 | 2.49 | 5.36 | 18.15 | 101.44 | 21.96 | 311.10 | 0.4735 | -845.6 | -102.2 | |
| 0.00 | 0.85 | 0.00 | 0.48 | 19.27 | 101.33 | 21.84 | 313.09 | 0.4829 | 686.0 | 459.3 | |
| 0.00 | 1.02 | 0.00 | 0.58 | 19.12 | 101.20 | 21.72 | 312.99 | 0.4800 | 749.0 | 581.8 | |
| 0.00 | 1.02 | 0.00 | 0.56 | 15.04 | 100.02 | 20.54 | 307.28 | 0.4276 | 767.0 | 556.3 | |
| 0.00 | 0.85 | 0.00 | 0.46 | 14.73 | 99.37 | 19.89 | 307.53 | 0.4166 | 773.0 | 580.7 | |
| 0.00 | 1.19 | 0.00 | 0.66 | 18.34 | 99.53 | 20.05 | 313.89 | 0.4534 | 810.0 | 680.6 | |
| 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. | |