SDO HMI 2011-12-05 13:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.82 | 177.49 | 16.63 | 93.17 | 19.38 | 103.71 | -2.12 | 6.15 | 0.3293 | -803.6 | -394.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.62 | 0.00 | 0.84 | 17.61 | 108.36 | 2.52 | 351.94 | 0.3009 | -884.0 | -677.8 | |
| 0.00 | 5.37 | 0.00 | 2.92 | 24.50 | 104.78 | -1.06 | 2.35 | 0.4112 | -499.0 | -666.1 | |
| 0.77 | 155.57 | 0.40 | 81.40 | 19.01 | 104.26 | -1.58 | 4.65 | 0.3223 | -949.6 | -426.1 | |
| 31.05 | -3.00 | 16.23 | -3.00 | 18.95 | 103.85 | -1.98 | 5.86 | 0.3219 | -1310.7 | 999999 | |
| 0.00 | 0.77 | 0.00 | 0.42 | 26.23 | 102.33 | -3.51 | 7.17 | 0.4417 | -624.0 | -443.4 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 20.17 | 102.33 | -3.51 | 9.63 | 0.3453 | 911.0 | 799.4 | |
| 0.00 | 1.71 | 0.00 | 0.96 | 28.12 | 101.73 | -4.11 | 7.72 | 0.4720 | -701.0 | -602.8 | |
| 0.00 | 1.19 | 0.00 | 0.66 | 26.00 | 101.68 | -4.16 | 8.57 | 0.4395 | -907.0 | -823.9 | |
| 0.00 | 1.02 | 0.00 | 0.57 | 26.26 | 101.53 | -4.30 | 8.75 | 0.4439 | -787.0 | -686.1 | |
| 0.00 | 1.19 | 0.00 | 0.67 | 28.35 | 101.35 | -4.49 | 8.34 | 0.4764 | -861.0 | -741.5 | |
| 0.00 | 1.36 | 0.00 | 0.75 | 26.30 | 101.30 | -4.54 | 9.21 | 0.4450 | -824.0 | -731.1 | |
| 0.00 | 1.11 | 0.00 | 0.57 | 14.54 | 101.24 | -4.60 | 17.56 | 0.2582 | 793.0 | 597.8 | |
| 0.00 | 1.88 | 0.00 | 0.96 | 13.63 | 101.11 | -4.73 | 19.24 | 0.2443 | 786.0 | 625.2 | |
| 0.00 | 1.71 | 0.00 | 0.89 | 17.98 | 99.82 | -6.02 | 18.23 | 0.3203 | 786.0 | 714.2 | |
| 0.00 | 1.71 | 0.00 | 0.89 | 18.54 | 99.49 | -6.35 | 18.58 | 0.3307 | 798.0 | 637.7 | |
| 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. | |