| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.92 | 79.79 | 21.44 | 43.88 | 19.97 | 125.25 | -17.36 | 40.21 | 0.4356 | -51.4 | 64.5 | |
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back to the solar disc SDO HMI 2011-12-02 18:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.45 | 0.00 | 0.75 | 15.86 | 133.99 | -8.62 | 28.90 | 0.2997 | 832.0 | 691.2 | |
| 2.30 | 29.02 | 1.26 | 15.87 | 20.20 | 126.94 | -15.67 | 37.21 | 0.4210 | -1042.8 | -679.8 | |
| 7.85 | -2.00 | 4.29 | -2.00 | 20.30 | 126.70 | -15.91 | 37.47 | 0.4245 | -987.2 | 999999 | |
| 4.01 | -2.00 | 2.20 | -2.00 | 20.36 | 126.43 | -16.18 | 37.83 | 0.4278 | -895.4 | 999999 | |
| 2.30 | 5.29 | 1.27 | 2.91 | 20.74 | 126.00 | -16.62 | 37.97 | 0.4365 | -881.3 | -155.5 | |
| 8.11 | 8.71 | 4.47 | 4.80 | 20.80 | 125.59 | -17.02 | 38.52 | 0.4412 | -815.8 | -291.1 | |
| 0.00 | 1.11 | 0.00 | 0.61 | 20.99 | 125.27 | -17.34 | 38.74 | 0.4465 | -677.0 | -600.8 | |
| 0.34 | 0.85 | 0.19 | 0.47 | 19.36 | 125.39 | -17.22 | 41.12 | 0.4266 | 701.8 | 576.4 | |
| 0.00 | 1.02 | 0.00 | 0.56 | 19.26 | 125.01 | -17.60 | 41.88 | 0.4295 | 454.0 | 400.9 | |
| 0.00 | 1.02 | 0.00 | 0.57 | 20.13 | 123.88 | -18.73 | 42.17 | 0.4510 | 960.0 | 805.0 | |
| 0.00 | 0.85 | 0.00 | 0.47 | 20.29 | 123.76 | -18.85 | 42.09 | 0.4540 | 681.0 | 660.6 | |
| 1.37 | 2.05 | 0.76 | 1.13 | 19.60 | 123.78 | -18.83 | 43.17 | 0.4463 | 948.9 | 784.4 | |
| 0.00 | 1.62 | 0.00 | 0.90 | 19.85 | 123.69 | -18.93 | 42.91 | 0.4500 | 798.0 | 626.9 | |
| 1.28 | 2.65 | 0.71 | 1.47 | 20.48 | 123.41 | -19.21 | 42.31 | 0.4598 | 728.1 | 734.8 | |
| 1.71 | 2.39 | 0.95 | 1.33 | 19.94 | 123.34 | -19.27 | 43.25 | 0.4547 | 727.7 | 671.4 | |
| 7.94 | 19.37 | 4.39 | 10.71 | 19.19 | 123.37 | -19.25 | 44.44 | 0.4465 | 971.9 | 645.9 | |
| 1.71 | 2.39 | 0.95 | 1.33 | 19.66 | 123.21 | -19.40 | 43.89 | 0.4531 | 781.9 | 694.1 | |
| 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. | |